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i
APPLICATION OF THE HLD AND NAC MODELS TO
THE FORMATION AND STABILITY OF EMULSIONS
By
Sumit Kumar Kiran
A thesis submitted in conformity with the requirements
for the degree of Doctor of Philosophy
Graduate Department of Chemical Engineering and Applied Chemistry
University of Toronto
© Copyright by Sumit Kumar Kiran (2013)
ii
APPLICATION OF THE HLD AND NAC MODELS TO THE
FORMATION AND STABILITY OF EMULSIONS
Sumit Kumar Kiran
Degree of Doctor of Philosophy
Graduate Department of Chemical Engineering and Applied Chemistry
University of Toronto
2013
ABSTRACT
This thesis explored how asphaltene and naphthenic amphiphile species influence the
formation (morphology and size) and stability of heavy crude oil (bitumen) emulsions. It was
experimentally shown that asphaltenes produce water-in-oil emulsions. Naphthenic amphiphiles
on the other hand flip the emulsion morphology to oil-in-water. It was further demonstrated that
the size and stability of these emulsions is influenced by physicochemical effects such as the
pH, solvent-bitumen-water ratios, solvent aromaticity, and temperature. In view of these
findings, the hydrophilic-lipophilic deviation (HLD) and net-average curvature (NAC) models
were looked at as potential means for predicting the formation and stability of emulsions. Owing
to the complexity of bitumen emulsions, however, the HLD and NAC models were instead
tested against well-defined sodium dihexyl sulfosuccinate-toluene-water emulsions. The
morphologies of these emulsions were predicted as a function of the formulation salinity
whereas corresponding droplet sizes were predicted as a function of the continuous phase
density and interfacial tension (γow). Emulsion stability trends were in turn predicted using a
collision-coalescence-separation assumption. From this assumption, emulsion stability was
iii
expressed as a function of the emulsion droplet collision frequency and activation energy. The
key parameters of the highly scrutinized activation energy term included the γow, interfacial
rigidity, and critical film thickness. In applying the same modeling approach to the stability of
other emulsions already published in the literature, it was found that the rigidity of adsorbed
multilayer/liquid crystal films cannot yet be fully accounted for. This shortcoming was the
reason for which only minimum stability times were reported for bitumen emulsions.
iv
ACKNOWLEDGEMENTS
I would first and foremost like to express my gratitude to my supervisor, Professor Edgar
J. Acosta, for his belief in me as a graduate student and as a leader of his laboratory. His
continuous guidance and support over the course of this work has allowed for me to publish in
several world renowned journals, present at various national and international conferences, and
collaborate with academic and industrial leaders in the field of colloid and formulation science.
He has further served as a close confidant and friend in helping me make tough personal and
professional decisions. I am also thankful to my committee members, Professors A.
Ramchandran, C.A. Mims, and C.M. Yip, for their constructive criticisms and insightful
suggestions to help improve the foundation of this work. Other university staff members that I
would like to recognize for their administrative and technical support include Dan Tomchyshyn,
Gorette Silva, Joan Chen, Julie Mendonca, Leticia Gutierrez, Paul Jowlabar, Pauline Martini,
and Phil Milczarek.
In addition to the above, I am also appreciative of the Natural Sciences and Engineering
Research Council of Canada (NSERC) and Syncrude Canada Ltd. for their financial support. I
would also like to thank the American Oil Chemists’ Society (AOCS) and the Society of
Cosmetic Chemists (SCC) for their generous student awards.
Finally, I would like dedicate this work to my parents, Ravi and Shashi Kiran, my elder
and wiser brother, Amit Kiran, and my best friend and wife, Roshni Patel. All of my
experienced achievements are a reflection of their infinite patience, unwavering love, and
continuous encouragement to never stop chasing my dreams.
v
TABLE OF CONTENTS
ABSTRACT ................................................................................................................................. ii
ACKNOWLEDGEMENTS ....................................................................................................... iv
TABLE OF CONTENTS ............................................................................................................ v
LIST OF FIGURES ................................................................................................................... xii
CHAPTER 1: THESIS OVERVIEW ........................................................................................ 1
1.1 OVERVIEW .................................................................................................................. 2
1.2 REFERENCES ............................................................................................................. 8
CHAPTER 2: STUDY OF SOLVENT-BITUMEN-WATER RAG LAYERS .................... 13
2.1 ABSTRACT ................................................................................................................ 14
2.2 INTRODUCTION ...................................................................................................... 14
2.3 MATERIALS AND METHODS ............................................................................... 16
2.3.1 Materials .............................................................................................................. 16
2.3.2 Formulation of Rag Layers .................................................................................. 16
2.3.3 Microscopy .......................................................................................................... 17
2.3.4 Material Balances ................................................................................................ 18
2.3.5 Asphaltene Losses ............................................................................................... 19
2.3.6 Interfacial Tension Measurements ....................................................................... 21
2.4 RESULTS .................................................................................................................... 22
2.4.1 Phase Separation of Solvent-Bitumen-Water Systems ........................................ 22
2.4.2 Development of Batch Emulsification-Separation Protocol................................ 24
2.4.3 Trends of Oil and Asphaltene Losses to the Rag Layer ...................................... 27
2.5 DISCUSSIONS ............................................................................................................ 30
2.5.1 Effect of Heptol 80/20 to Bitumen Dilution Ratio and Water Content on Rag
Layer Stability ..................................................................................................... 30
vi
2.5.2 Effect of Temperature and Solvent Aromaticity on Rag Layer Stability ............ 35
2.5.3 Surface Activity of Asphaltenes .......................................................................... 37
2.5.4 Correlation of Oil and Asphaltene Losses to the Rag Layer ............................... 41
2.6 CONCLUSIONS ......................................................................................................... 42
2.7 REFERENCES ........................................................................................................... 43
CHAPTER 3: IMPACT OF ASPHALTENES AND NAPHTHENIC AMPHIPHILES ON
THE PHASE BEHAVIOR OF SOLVENT-BITUMEN-WATER SYSTEMS .................... 49
3.1 ABSTRACT ................................................................................................................ 50
3.2 INTRODUCTION ...................................................................................................... 50
3.3 MATERIALS AND METHODS ............................................................................... 52
3.3.1 Materials .............................................................................................................. 52
3.3.2 Formulation Preparation ...................................................................................... 52
3.3.3 Microscopy and Material Balances ..................................................................... 53
3.3.4 Asphaltene Losses ............................................................................................... 53
3.3.5 Interfacial Tension Measurements ....................................................................... 54
3.3.6 Surface Pressure-Area Isotherms ......................................................................... 55
3.4 RESULTS .................................................................................................................... 56
3.4.1 Phase Behavior of Naphthenic Amphiphile Systems .......................................... 56
3.4.2 Transitions to the Rag Layer Morphology .......................................................... 59
3.4.3 Interfacial Tension Isotherms .............................................................................. 60
3.4.4 Impact of Naphthenic Acids on Asphaltene Film Properties .............................. 61
3.5 DISCUSSIONS ............................................................................................................ 63
3.5.1 Interfacial Co-Adsorption of Asphaltenes and Sodium Naphthenates ................ 63
3.5.2 Effect of Temperature and Solvent Aromaticity on Oil Recovery from Rag
Layers .................................................................................................................. 67
3.5.3 Effect of pH on Oil Recovery from Rag Layers .................................................. 68
3.6 CONCLUSIONS ......................................................................................................... 69
vii
3.7 REFERENCES ........................................................................................................... 70
CHAPTER 4: EVALUATING THE HYDROPHILIC-LIPOPHILIC NATURE OF
ASPHALTENIC OILS AND NAPHTHENIC AMPHIPHILES USING
MICROEMULSION MODELS ............................................................................................... 73
4.1 ABSTRACT ................................................................................................................ 74
4.2 INTRODUCTION ...................................................................................................... 74
4.3 MATERIALS AND METHODS ............................................................................... 80
4.3.1 Materials .............................................................................................................. 80
4.3.2 Asphaltene Precipitation ...................................................................................... 80
4.3.3 Formulation of Microemulsions with Test Oil and Toluene Mixtures ................ 81
4.3.4 Formulation of Microemulsions with Test Surfactant and SDHS Mixtures ....... 81
4.3.5 Interfacial Tension Measurements ....................................................................... 82
4.3.6 Asphaltene Partitioning at the Oil-Water Interface ............................................. 82
4.4 RESULTS .................................................................................................................... 82
4.4.1 Microemulsion Phase Behavior Scans................................................................. 82
4.4.2 Interfacial Tension of Test Oil and Toluene Mixtures ........................................ 83
4.4.3 EACN of Test Oils............................................................................................... 85
4.4.4 Interfacial Tension of Test Surfactant and SDHS Mixtures ................................ 88
4.4.5 Cc of Test Surfactants .......................................................................................... 90
4.5 DISCUSSIONS ............................................................................................................ 93
4.5.1 Analysis of the Hydrophilic-Lipophilic Nature of Asphaltenic Crude Oils ........ 93
4.5.2 Analysis of the Hydrophilic-Lipophilic Nature of Naphthenic Amphiphiles and
Asphaltene Aggregates ........................................................................................ 94
4.6 CONCLUSIONS ......................................................................................................... 95
4.7 REFERENCES ........................................................................................................... 95
CHAPTER 5: EXPERIMENTAL EVALUATION OF EMULSION STABILITY VIA
SURFACTANT-OIL-WATER PHASE BEHAVIOR SCANS ............................................ 100
5.1 ABSTRACT .............................................................................................................. 101
viii
5.2 INTRODUCTION .................................................................................................... 101
5.3 MATERIALS AND METHODS ............................................................................. 108
5.3.1 Materials ............................................................................................................ 108
5.3.2 Microemulsion Phase Behavior Scans and Emulsification ............................... 108
5.3.3 Interfacial Tension of Baseline Microemulsions ............................................... 109
5.3.4 Average Diameter of Baseline Emulsion Droplets ............................................ 110
5.3.5 Emulsion Phase Separation Profiles .................................................................. 110
5.4 RESULTS .................................................................................................................. 112
5.4.1 Interfacial Tension and Average Emulsion Droplet Diameter .......................... 112
5.4.2 Emulsion Phase Separation Profiles and Time Periods ..................................... 114
5.4.3 Effect of Temperature on Emulsion Phase Separation Time Periods ................ 117
5.5 DISCUSSIONS .......................................................................................................... 120
5.6 CONCLUSIONS ....................................................................................................... 127
5.7 REFERENCES ......................................................................................................... 128
CHAPTER 6: PREDICTING THE MORPHOLOGY AND VISCOSITY OF
MICROEMULSIONS USING THE NAC MODEL ............................................................ 133
6.1 ABSTRACT .............................................................................................................. 134
6.2 INTRODUCTION .................................................................................................... 134
6.3 DEVELOPMENT OF EXPRESSIONS FOR THE SHAPE-BASED NAC
MODEL AND MAXIMUM HYDRODYNAMIC RADIUS ................................. 140
6.4 MATERIALS AND METHODS ............................................................................. 142
6.4.1 Materials ............................................................................................................ 142
6.4.2 Microemulsion Phase Behavior Scans............................................................... 142
6.4.3 Oil-Water Solubilization .................................................................................... 142
6.4.4 Viscosity Measurements .................................................................................... 143
6.4.5 Dynamic Light Scattering .................................................................................. 143
6.4.6 Prediction of Oil and Water Solubilization with the NAC Model..................... 144
ix
6.4.7 Prediction of Small Angle Neutron Scattering Profiles ..................................... 146
6.5 RESULTS AND DISCUSSIONS ............................................................................. 147
6.5.1 Comparison of Spherical Viscosity Models and Experimental Measurements. 147
6.5.2 Comparison of Predicted and Experimental SANS Profiles for Type I and Type
II Microemulsions .............................................................................................. 150
6.5.3 Comparison of Maximum Predicted and Experimental Hydrodynamic Radii .. 152
6.5.4 Comparison of Non-Spherical Viscosity Models and Experimental
Measurements .................................................................................................... 153
6.6 CONCLUSIONS ....................................................................................................... 156
6.7 REFERENCES ......................................................................................................... 156
CHAPTER 7: MODELING THE SIZE AND STABILITY OF EMULSIONS AROUND
THE PHASE INVERSION POINT ....................................................................................... 164
7.1 ABSTRACT .............................................................................................................. 165
7.2 INTRODUCTION .................................................................................................... 166
7.3 DEVELOPMENT OF EMULSION STABILITY MODEL SOLUTION ........... 172
7.4 MATERIALS AND METHODOLOGIES ............................................................. 175
7.4.1 Materials ............................................................................................................ 175
7.4.2 NAC Modeling Methodology ............................................................................ 175
7.4.3 Density and Viscosity Measurements ................................................................ 178
7.5 RESULTS .................................................................................................................. 178
7.5.1 Experimental and Predicted SDHS-Toluene-Water Microemulsion Properties 178
7.5.2 Predicted Droplet Size of 0.1 M SDHS-Toluene-Water Emulsions ................. 180
7.5.3 Predicted Stability of 0.1 M SDHS-Toluene-Water Emulsions ........................ 181
7.5.4 Effect of Surfactant Concentration on the Predicted Stability of SDHS-Toluene-
Water Emulsions ................................................................................................ 184
7.5.5 Effect of Temperature on the Predicted Stability of SDHS-Toluene-Water
Emulsions .......................................................................................................... 185
7.6 DISCUSSIONS .......................................................................................................... 187
x
7.6.1 Prediction of the Droplet Size and Stability of SDHS-Toluene-Water Emulsions187
7.6.2 Prediction of the Emulsion Droplet Size of Lin et al......................................... 190
7.6.3 NAC Prediction of Initial Emulsion Droplet Size and Stability for the Systems of
Binks et al. with AOT and 0.65 cSt Silicone Oil ............................................... 192
7.6.4 NAC Prediction of Emulsion Stability for the Systems of Kabalnov et al. with
C12E5 and Octane ............................................................................................... 194
7.6.5 NAC Prediction of Emulsion Stability for the Systems of Salager et al. with
SDS, Pentanol, and Kerosene ............................................................................ 195
7.7 CONCLUSIONS ....................................................................................................... 196
7.8 REFERENCES ......................................................................................................... 197
CHAPTER 8: REVIEW OF THE FORMATION AND STABILITY OF BITUMEN
EMULSIONS ........................................................................................................................... 204
CHAPTER 9: CONCLUSIONS ............................................................................................. 213
CHAPTER 10: RECOMMENDATIONS.............................................................................. 218
10.1 RECOMMENDATIONS ......................................................................................... 219
10.2 REFERENCES ......................................................................................................... 221
APPENDIX 1: THE REVISED NET CURVATURE .......................................................... 223
APPENDIX 2: DISJOINING PRESSURE EQUATIONS ................................................... 227
xi
LIST OF TABLES
Table 2.1: Compositions (wt%) of tested heptol (H)-bitumen (B)-water (W) systems. ............. 17
Table 2.2: Material balance closure for systems prepared with 50 wt% water (W) at various
heptol 80/20 (H) to bitumen (B) dilution ratios and 25°C. .......................................................... 24
Table 3.1: Relative asphaltene and NA compositions in formulations tested. ........................... 62
Table 3.2: Measurements of ε for mixed asphaltene and NA films............................................ 62
Table 4.1: Calculated EACN of asphalt, bitumen, naphthalene, and deasphalted bitumen ....... 88
Table 4.2: Cc (* a
cC ) of NAs, NaNs, and asphaltene aggregates. ................................................ 91
Table 6.1: Reference viscosities () and refractive indices (n). ............................................... 144
Table 6.2: HLD and NAC modeling parameters for SDHS-toluene-water µEs. ...................... 145
Table 6.3: HLD and NAC modeling parameters for the non-ionic µEs of Leaver and Olsson28
.
................................................................................................................................................... 145
Table 7.1: Required HLD and NAC parameters for predicting the properties of the emulsions of
Kiran et al. (Chapter 5), Kabalnov et al., Salager et al., Binks et al., and Lin et al.16,18,19,20
. .... 177
xii
LIST OF FIGURES
Figure 1.1: Number of publications per year for emulsions across various industrial fields of
interest............................................................................................................................................ 2
Figure 1.2: Commercial hot water flotation process used in oil sands operations. ...................... 4
Figure 2.1: Calibration of asphaltene absorbance at a wavelength of 450 nm and as a function
of the bitumen to toluene ratio. .................................................................................................... 20
Figure 2.2: (i) Optical, (ii) cross-polarized, and (iii) fluorescent micrographs of samples of the
separated oil phase, aqueous phase, and rag layer for a system containing 68.2 wt% heptol
80/20, 6.8 wt% bitumen, and 25 wt% water at 25°C. .................................................................. 23
Figure 2.3: (a) Oil and (b) asphaltene losses to the rag layer as a function of the mixing time for
systems prepared with either 25 wt% or 75 wt% water and the balance oil with a heptol 80/20 to
bitumen dilution ratio of 3 at 25°C. ............................................................................................. 25
Figure 2.4: Oil losses to the rag layer as a function of the g force × time for systems prepared
with (a) 12.5 wt% heptol 80/20, 12.5 wt% bitumen, and 75 wt% water, (b) 20 wt% heptol 80/20,
5 wt% bitumen, and 75 wt% water, (c) 37.5 wt% heptol 80/20, 37.5 wt% bitumen, and 25 wt%
water, and (d) 60 wt% heptol 80/20, 15 wt% bitumen, and 25 wt% water. ................................ 26
Figure 2.5: Oil and asphaltene losses to the rag layer for systems prepared with (a and b) heptol
80/20 at 25°C, (c and d) heptol 80/20 at 80°C, and (e and f) heptol 50/50 at 25°C. ................... 27
Figure 2.6: Ternary phase diagrams for systems prepared with (a) heptol 80/20 at 25°C, (b)
heptol 80/20 at 80°C, and (c) heptol 50/50 at 25°C..................................................................... 29
Figure 2.7: (a) E
dd , (b) sample E
id distribution at 50 wt% water, and (c) normalized Aow of
heptol 80/20-diluted bitumen droplets at 25°C. ........................................................................... 33
Figure 2.8: Morphology of emulsions for systems prepared with (a) 10 wt% heptol 80/20, 15
wt% bitumen, and 75 wt% water, (b) 12.5 wt% heptol 80/20, 12.5 wt% bitumen, and 75 wt%
xiii
water, (c) 10 wt% heptol 50/50, 15 wt% bitumen, and 75 wt% water, and (d) 12.5 wt% heptol
50/50, 12.5 wt% bitumen, and 75 wt% water. ............................................................................. 37
Figure 2.9: The measured γow as a function of solvent-bitumen-water ratios for systems
prepared with (a) heptol 80/20 at 25°C, (b) heptol 80/20 at 80°C, and (c) heptol 50/50 at 25°C.
..................................................................................................................................................... 38
Figure 2.10: The measured γow (against water) of asphaltenes diluted in heptol 80/20 and heptol
50/50 at 25°C. .............................................................................................................................. 39
Figure 2.11: Correlations of oil and asphaltene losses to the rag layer for systems prepared with
heptol 80/20 at (a) 25°C and (b) 80°C. ........................................................................................ 41
Figure 3.1: Oil and asphaltene losses to the rag layer for 0 wt% (baseline) and 3 wt% NaN
systems prepared at pH 7.5 with (a and b) heptol 80/20 at 25°C, (c and d) heptol 80/20 at 80°C,
and (e and f) heptol 50/50 at 25°C. .............................................................................................. 57
Figure 3.2: Oil losses to the rag layer for 0 wt% (baseline) and 3 wt% NA systems as a function
of the heptol 80/20 to bitumen dilution ratio and water content. All systems are evaluated at pH
4 and 25°C. .................................................................................................................................. 58
Figure 3.3: Fluorescent micrographs of the effect of (a) NaNs (pH 7.5) and (b) NAs (pH 4) on
the morphology of heptol 80/20-bitumen-water rag layers. (c) Cross-polarized images of rag
layers containing NAs at pH 4. .................................................................................................... 59
Figure 3.4: Baseline γow isotherms as well as those for (a) NaN systems at pH 7.5 and (b) NA
systems at pH 4 as a function of the heptol 80/20 to bitumen dilution ratio. The temperature is
maintained at 25°C. ..................................................................................................................... 60
Figure 3.5: πp-Asp isotherms of asphaltene (A) and NA surfactant mixtures. ............................ 61
Figure 3.6: γow of bitumen diluted with heptol 80/20 versus the added NaN concentration to the
aqueous phase at pH 7.5 and 25°C. The included fluorescent micrographs show a transition in
the rag layer morphology from w/o to o/w at the CMC of NaNs (~1 wt%). ............................... 64
xiv
Figure 3.7: (a) Bilayer model proposed by Wu and Czarnecki for the interfacial co-adsorption
of asphaltenes and NaNs at the oil-water interface1. (b) Co-adsorption mechanisms proposed by
Varadaraj and Brons for asphaltenes and NAs at the oil-water interface include (i) mixed
monolayers and (ii) mixed aggregates3........................................................................................ 65
Figure 4.1: The phase behavior and corresponding γow of SDHS-oil (20 wt% naphthalene and
80 wt% toluene)-water µEs as a function of the salinity. ............................................................ 77
Figure 4.2: µE phase behavior transitions as a function of the salinity for a (a) 30 wt% bitumen
and 70 wt% toluene oil phase mixture and (b) 20 mol% NAs and 80 mol% SDHS surfactant
mixture. ........................................................................................................................................ 83
Figure 4.3: The measured γow as a function of the salinity for (a) bitumen and toluene, (b)
asphalt and toluene, (c) naphthalene and toluene, and (d) deasphalted bitumen and toluene oil
phase mixtures. ............................................................................................................................ 84
Figure 4.4: Experimented and modeled shifts of S* for µEs composed of hexadecane and
toluene oil phase mixtures and 0.1 M of a 35 mol% SDHS and 65 mol% AOT surfactant
mixture. ........................................................................................................................................ 87
Figure 4.5: The measured γow as a function of the salinity for (a) NAs and SDHS, (b) NaNs and
SDHS, and (c) asphaltenes and SDHS surfactant mixtures at a total concentration of 0.1 M. ... 89
Figure 4.6: Salinity shift of (a) NAs and SDHS and (b) NaNs and SDHS surfactant mixtures as
a function of the test surfactant mole fraction within the 0.1 M surfactant mixture. .................. 90
Figure 4.7: (a) Asphaltene partitioning and (b) the shift in S* for optimum µEs formulated with
an asphaltenes and SDHS surfactant mixture. ............................................................................. 92
Figure 5.1: A Type IType IIIType II phase behavior scan for 0.1 M SDHS-toluene-water
µEs at 25°C. ............................................................................................................................... 102
Figure 5.2: Emulsion aggregation, settling, film thinning, and coalescence processes. .......... 103
xv
Figure 5.3: (a) Evolution of the observable phase separation stages versus time in a test tube
for emulsions produced in Type II µEs. (b) Normalized displacement of the µE and excess
aqueous phase separation fronts versus time and the extrapolated ap, dp, and cp time periods. 104
Figure 5.4: In-house multipoint turbidimeter used to track the net displacement of µE and
excess phase separation fronts at a high time resolution. .......................................................... 111
Figure 5.5: Measured (a) interfacial tension (γow) and (b) emulsion droplet diameter ( E
dd )
profiles for baseline (0.1 M SDHS) emulsions at 25°C. ........................................................... 113
Figure 5.6: Example of sample time-lapse images and ΔsµE(t) and Δsw(t) profiles versus time
for a Type II baseline (0.1 M SDHS) emulsion at HLD=0.9 and 25°C. ................................... 114
Figure 5.7: Net rate of advance of the µE and excess phase separation fronts as a function of the
HLD for baseline (0.1 M SDHS) emulsions at 25°C. ............................................................... 116
Figure 5.8: Compiled ap, dp, cp, and ep (ap+dp+cp) time periods for emulsions at (a) 0.01 M, (b)
0.1 M, and (c) 0.3 M SDHS and 25°C. ...................................................................................... 117
Figure 5.9: Compiled ap, dp, cp, and ep (ap+dp+cp) time periods for baseline (0.1 M SDHS)
emulsions at (a) T=7°C, (b) T=15°C, (c) T=35°C, and (d) T=44°C. ........................................ 118
Figure 5.10: (a) Sample W* fittings for the aggregation, drainage, and coalescence of Type I
baseline (0.1 M SDHS) emulsion at HLD=-1 and (b) their values as a function of the HLD at
298 K. ........................................................................................................................................ 119
Figure 5.11: Dependence of the ap time period for baseline (0.1 M SDHS) emulsions at 25°C on
E
dd . The solid line represents the fit of tdiff from Equation 9 (R2=0.84).................................... 121
Figure 5.12: Comparison of the originally measured E
dd for baseline (0.1 M SDHS) emulsion
droplets at 25°C after mixing and the estimated E
appdd , required for settling (Equation 10) and
film thinning (Equation 11) as a function of the HLD. ............................................................. 123
Figure 5.13: General correlation between all of the fitted W* and the measured γow for baseline
(0.1 M SDHS) emulsions at 25°C. ............................................................................................ 125
xvi
Figure 6.1: Experimental and predicted (a) E
IoV , and E
IIwV , as well as (b) E
d
as a function of
the HLD for SDHS-toluene-water µEs. ..................................................................................... 147
Figure 6.2: Experimental and NAC modeled (for dilute liquid spheres (Equation 2) and
concentrated hard spheres (Equation 3)) ηµE of SDHS-toluene-water µEs as a function of the
HLD. .......................................................................................................................................... 148
Figure 6.3: Predicted (a) E
dr and E
dl as well as (b) total aspect ratio ( E
dl /2 E
dr ) as a function
of the HLD for SDHS-toluene-water µEs using the NAC model. ............................................ 149
Figure 6.4: Predicted SANS profiles of SDHS-toluene-water µEs formulated at (a) HLD=-0.9,
(b) HLD=-0.6, (c) HLD=-0.4, (d) HLD=0.3, (e) HLD=0.4, and (f) HLD=0.6 using the NAC
model. ........................................................................................................................................ 151
Figure 6.5: Experimental E
hr and predicted E
hr
max, for Type I and Type II SDHS-toluene-water
µEs as a function of the HLD. ................................................................................................... 152
Figure 6.6: Experimental and NAC modeled (for dilute rigid rods (Equation 6) and prolate
ellipsoids (Equation 8)) ηµE of SDHS-toluene-water µEs as a function of the HLD. ............... 154
Figure 6.7: Experimental and predicted E / E
c
ratio for the (a) C12E4-hexadecane-water and
(b) C12E5-cyclohexane and hexadecane-water µEs of Leaver and Olsson28
. ............................ 155
Figure 7.1: Overview of the simplified CCS demulsification mechanism used to model
emulsion stability. ...................................................................................................................... 170
Figure 7.2: Cross-section of coalescing emulsion droplets showing the formation of the
nucleating hole and its characteristic dimensions. ..................................................................... 171
Figure 7.3: General algorithm used to predict the size and stability of emulsions................... 172
Figure 7.4: Experimental and NAC modeled (a) γow, (b) ρµE, and (c) ηµE of SDHS-toluene-water
µEs. ............................................................................................................................................ 180
xvii
Figure 7.5: Predicted E
dr of 0.1 M SDHS-toluene-water emulsions at 298 K using the NAC
model. Experimental data are obtained from the work presented in Chapter 5. ....................... 181
Figure 7.6: Predicted (a) ut and (b) tH,crit of 0.1 M SDHS-toluene-water emulsions at 298 K
using the NAC model. ............................................................................................................... 182
Figure 7.7: Predicted Eac of 0.1 M SDHS-toluene-water emulsions at 298 K using the NAC
model. Experimental data are obtained from the work presented in Chapter 5. ....................... 183
Figure 7.8: Predicted stability (solid lines) of 0.1 M SDHS-toluene-water emulsions at room
temperature with E
d =0.5 (initial volume fraction) and 0.74 (closely packed hard spheres). All
experimental data is taken from Chapter 5. ............................................................................... 184
Figure 7.9: Predicted stability (solid lines) of (a) 0.01 M and (b) 0.3 M SDHS-toluene-water
emulsions at 298 K and E
d =0.5. Dashed line in (a) corresponds to predicted values using
tH,crit=0. All experimental data is taken from Chapter 5. ........................................................... 185
Figure 7.10: Predicted stability (solid lines) of 0.1 M SDHS-toluene-water emulsions at
E
d =0.5 and (a) 280 K, (b) 288 K, (c) 308 K, and (d) 317 K. All experimental data was taken
from Chapter 5. .......................................................................................................................... 186
Figure 7.11: Predicted emulsion droplet size (solid line) for the nonylphenol ethoxylate-mineral
oil-water systems at 294 K and as a function of the wt% of polyethylene oxide (PEO) in the
surfactant. See Table 7.1 for additional simulation conditions. The experimental data is taken
from Lin et al. ............................................................................................................................ 191
Figure 7.12: Predicted (a) interfacial tension and (b) emulsion stability (solid lines) for the
AOT-0.65 cSt silicone oil system. See Table 7.1 for additional simulation conditions. The
dashed line in (b) represents the predicted stability considering an additional contribution to
tH,crit of 15 nm. The experimental data is taken from Binks et al. .............................................. 193
Figure 7.13: Predicted emulsion stability (solid lines) for the system (a) C12E5–octane and (b)
SDS-pentanol-kerosene. See Table 7.1 for additional simulation conditions. The experimental
xviii
data for the systems in (a) and (b) is obtained from Kabalnov et al. and Salager et al.
respectively. ............................................................................................................................... 195
Figure 8.1: The HLD as a function of the heptol to bitumen dilution ratio for asphaltene-
stabilized rag layers prepared with heptol 80/20 and heptol 50/50 at 25°C………………...…206
Figure 8.2: The effect of 3 wt% sodium naphthenates (NaNs) on the HLD of bitumen emulsions
at an oil to water ratio of 1 to 1 and as a function of the heptol to bitumen dilution ratio…….207
Figure 8.3: The effect of 3 wt% naphthenic acids (NAs) on the HLD of bitumen emulsions as a
function of the heptol to bitumen dilution ratio………………………………………………..208
Figure 8.4: Experimental and predicted γow as a function of the HLD for o/w bitumen emulsions
stabilized by a mixture of asphaltenes and NaNs……………………….……………………..210
Figure 8.5: Experimental and predicted E
dd as a function of the HLD for o/w bitumen emulsion
droplets stabilized by a mixture of asphaltenes and NaNs…………………………………….211
Figure 8.6: Predicted stability of o/w bitumen emulsions stabilized by a mixture of asphaltenes
and NaNs as a function of the HLD……………………………………………………………212
xix
LIST OF SYMBOLS
α = 0.6 for turbulent flow and 1 for laminar
flow
= Shear rate
γow = Interfacial tension
δtail = Surfactant tail length
ɛ = Elasticity
ɛmix = Energy dissipation during mixing
ηµE = Viscosity of µE
E
c
= Viscosity of µE’s continuous phase
E
d
= Viscosity of µE’s dispersed phase
ηoil = Viscosity of oil phase
ηwater = Viscosity of aqueous phase
θ = Scattering angle
θc = Contact angle
κ = Bending modulus
= Saddle-splay modulus
~ = Dimensionless chemical potential
µE = Microemulsion
πp = Surface pressure
Δρ = Density difference
ρµE = Density of µE phase
E
c = Density of emulsion’s continuous
phase
E
d = Density of emulsified phase
ρoil = Density of oil phase
ρwater = Density of aqueous phase
σ = Surface tension in presence of surfactant
~ = Dimensionless excess free energy
σo = Surface tension of pure solvent
τ(t) = Measured turbidity
E
d
= Volume fraction of µE droplets
E
d
max, = Maximum E
d
E
wo
= Volume fraction of oil (water) in the
µE phase
E
d = Volume fraction of emulsion droplets
ϕ(A) = Co-surfactant effect on the HLD of
nonionic surfactants
ω = Rotational velocity
E
ella = Major axis of µE ellipsoids
ap = Aggregation time period
ai = Surface area per molecule of surfactant
species i
aT = Pre-factor of temperature effect on the
HLD of ionic surfactants
E
dA = Surface area of emulsion droplet
AH = Effective Hamaker constant
As = Interfacial area of surfactant
Asp = Area of spreading phase
Aow = Area of oil-water interface
ACN = Alkane carbon number
AOT = Sodium dioctyl sulfosuccinate
A(q) = Scattering amplitude
b = Pre-factor of salt effect on the HLD of
nonionic surfactants
∆b = Scattering length difference between
the µE’s continuous and dispersed phases
xx
E
ellb = Minor axis of µE ellipsoids
cµc = Critical µE concentration
cg = Concentration of µE rigid rods
cp = Coalescence time period
csi = Concentration of surfactant species i
C1 = Fitting constant (~0.5)
C2 = Fitting constant (~0.25)
Cc = Characteristic curvature of ionic
surfactant
Cc,mix = Characteristic curvature of ionic
surfactant mixture
Cn = Characteristic curvature of nonionic
surfactant
a
cC = Apparent characteristic curvature of
ionic surfactant
ref
cC = Characteristic curvature of reference
ionic surfactant
test
cC = Characteristic curvature of test ionic
surfactant
CSA,avg = Surface area-averaged curvature
CAC = Critical aggregation concentration
CCS = Collision-coalescence-separation
mechanism
CMC = Critical micelle concentration
CTC = Critical transition concentration
E
dd = Average emulsion droplet diameter
E
appdd , = Apparent average emulsion droplet
diameter
dH = Hole diameter
E
id = Emulsion droplet of diameter i
dp = Drainage time period
E
rodsd = Diameter of µE rigid rods
D = Diffusion coefficient
Dimp = Impeller diameter
ep = Equilibrium time period
E1 = Energy of hole formation
E2 = Energy of hole opening
Er = Interfacial rigidity
Eac = Activation energy of coalescence
EACN = Equivalent alkane carbon number
EACNmix = EACN of oil mixture
f = Pre-exponential factor
fc = Fitting constant for E1
fratio = Ratio of film radius to Rc
f(ϕ) = Entropic function of E
d
f(A) = Co-surfactant effect on the HLD of
ionic surfactants
F = Force exerted by Du Noüy ring
E
iF = Number frequency of E
id
g = Gravitational acceleration constant (9.81
m/s2)
ΔhµE(t) = Net displacement of µE phase
separation front
ΔhµE,tot = Total displacement of µE phase
separation front at equilibrium
Δho(t) = Net displacement of excess oil
phase separation front
Δho,tot = Total displacement of excess oil
phase separation front at equilibrium
Δhw(t) = Net displacement of excess
aqueous phase separation front
xxi
Δhw,tot = Total displacement of excess
aqueous phase separation front at
equilibrium
Ha = Average curvature
Hn = Net curvature
H’n = Revised net curvature = Hn/2
HLD = Hydrophilic-lipophilic deviation
HLDmix = HLD of an oil or surfactant
mixture
HLDref = HLD of reference oil or surfactant
HLDtest = HLD of test oil or surfactant
I(q) = Scattering intensity
k = Debye length at salinity S
k* = Debye length at optimal salinity S
*
kB = Boltzmann constant (1.38×10-23
J/K)
K = Pre-factor of Nc,o effect on the HLD of
ionic and nonionic surfactants
l = Characteristic diffusion length
E
dl = Length of µE’s cylindrical neck
E
rodsl = Length of µE rigid rods
L = Length scaling parameter
Lp = Laser path length
nE = Number concentration of emulsion
droplets
nEo = Initial number concentration of
emulsion droplets
ntoluene = Refractive index of toluene
nwater = Refractive index of water
N = Number density of µE rigid rods
Nc,o = General descriptor for ACN/EACN
ref
ocN , = General descriptor for the
ACN/EACN of a reference oil
test
ocN , = General descriptor for the
ACN/EACN of a test oil
Nimp = Impeller speed of mixing
NAs = Naphthenic acids
NAC = Net-average curvature
NaN(s) = Sodium naphthenates
o/w = Oil-in-water
p2 = Polydispersity
P~
= Dimensionless osmotic pressure
Pcons = Power consumption
Pe = Peclét number
q = Scattering vector
E
dr = Radius of µE’s hemispherical end cap
E
dr = Average emulsion droplet radius
E
hr = Hydrodynamic radius of µE droplets
E
hr
max, = Maximum E
hr
rH = Hole radius
E
wor = Sphere-equivalent radius of the oil
(aqueous) phase
rring = Probe ring radius
rwire = Probe wire radius
Rc = Radius of curvature
Re = Reynolds number
ΔsµE(t) = Normalized displacement of µE
phase separation front
Δso(t) = Normalized displacement of excess
oil phase separation front
xxii
Δsw(t) = Normalized displacement of excess
aqueous phase separation front
S = Aqueous phase salinity
S* = Optimal S (where HLD=0)
*
mixS = S* with reference to HLDmix
SDHS = Sodium dihexyl sulfosuccinate
SDS = Sodium dodecyl sulfate
td = Falling ball’s time of descent
tdiff = Characteristic diffusion time
tH = Film thickness
tH,crit = Critical film thickness at which hole
formation occurs
tp = Phase separation time of interest
T = Temperature
∆T = Temperature difference from 298 K
uosc = Oscillatory free energy contribution
to ut
ut = Free energy penalty of expelling µE
droplet layers during film thinning
uvdW = van der Waals free energy
contribution to ut
Uc = Rate of emulsion droplet coalescence
vrel = Relative mixing velocity
vs = Settling rate
VµE = Volume of µE phase
E
dV = Volume of emulsion droplet
VE = Volume of total emulsion
Vmax = Maximum V(t)
pulloV , = Volume of oil pulled through
interface
E
woV = Volume of oil (water) in the µE
phase
E
woV = Volume of emulsified oil (water)
V(t) = Voltage
w = Width of expanded oil droplet
w/o = Water-in-oil
W* = Apparent activation energy
We = Weber number
xi = Mol (volume) fraction of a given
surfactant (oil)
xref = Mol (volume) fraction of a reference
surfactant (oil)
xtest = Mol (volume) fraction of a test
surfactant (oil)
2
1.1 OVERVIEW
Emulsions are thermodynamically unfavorable mixtures of surfactant-encapsulated
droplets (>0.4 µm) of one medium (oil or water) dispersed throughout the other1. According to
the query conducted using SciVerse Scopus in Figure 1.1, the study of emulsions has
commanded a growing amount of attention across various applications. While a large part of
this growth has been experienced in developing new and innovative paint and coating, foodstuff,
and pharmaceutical products, it is projected that the role of emulsions as an undesirable process
intermediate in the oil sands sector will soon become a more prominent area of focus. The
reason for such is that billions of dollars are being spent to help expand the bitumen (i.e. heavy
crude oil) production capacity of oil sands operations in north-eastern Alberta (Canada)2,3,4
. In
view of this investment, it is expected that the bitumen output of 1,000,000 barrels/day will at
least triple over the next decade.
Paints and Coatings
Lubricants
0
300
600
900
1200
1500
1950 1955 1960 1965 1970 1975 1980 1985 1990 1995 2000 2005 2010 2015
Year
# P
ub
lic
ati
on
s
Foodstuffs
Cosmetics
Pharmaceuticals
Crude Oil
Pesticides
Cleaning
Figure 1.1: Number of publications per year for emulsions across various industrial fields of
interest.
3
An overview of the commercial hot water flotation process used in oil sands operations
is outlined in Figure 1.25. In this process, mined oil sands are first added along with hot water to
a rotating horizontal tumbler where their fragmentation and dispersion facilitates the liberation
of bitumen from quartz sand particles. To further help separate bitumen from water in
downstream process units, this mixed slurry is treated with sodium hydroxide (NaOH) and
steam so that it exits the tumbler at a conditioned pH (8), temperature (80°C), and degree of
aeration (30%). The resulting effluent next passes through a series of vibrating screens to
remove all oversized solid particles and undissociated oil sand lumps prior to being diluted with
excess hot water and pumped to a primary separation vessel. Within this vessel, the aerated
bitumen droplets rise to the top and are removed as a primary froth whereas most of the fine
solids collect at the bottom and are removed as a concentrated tailings solution. The middlings
region is on the other hand subjected to additional aeration steps to produce a secondary froth
that separates out from a secondary separation vessel at a similar composition as that of the
primary froth (60% bitumen, 30% water, and 10% fine solids). As a result of its large viscosity
(10,000 cP at 25°C) and similar density to that of water, the combined froth is diluted with a
solvent (naphtha) prior to passing through an energy-intensive mechanical separation cycle
where formed oil-in-water (o/w) and water-in-oil (w/o) emulsion droplets are broken and a final
and cleaner bitumen product ready for upgrading into synthetic crude oil is produced. The
formation and stability of these emulsions as “rag layers” is a major operational issue and
therefore serves as the main focus of this thesis.
4
Mined Oil Sands
Tumbler
Vibrating Screens Solid
Rejects
Hot Water + NaOH
+ Steam
Excess
Hot Water
S
e
p
a
r
a
t
i
o
n
Tailings
MIddlingsAeration
S
e
p
a
r
a
t
i
o
n
Recycle
1 Froth
2 Froth
Mechanical
Separation Cycle
Upgrading
Figure 1.2: Commercial hot water flotation process used in oil sands operations.
The formation and stability of rag layers are governed by surfactant-like species found
naturally within bitumen. An example of one such component, which makes up close to 15% of
bitumen, is asphaltenes6. Asphaltenes may be classified as highly aromatic structures that
solubilize in aromatic hydrocarbons (e.g. benzene and toluene) and precipitate upon mixing with
paraffinic solvents (e.g. pentane and heptane)6,7
. The surface activity of asphaltenes varies
according to their solubility. As has been demonstrated by several previous researchers,
asphaltenes having undergone a monomer-to-aggregate transition under partially soluble
conditions show an enhanced affinity for the oil-water interface6,8,9
. The resulting adsorbed
asphaltene skins, which are characteristically lipophilic, promote the formation of w/o emulsion
droplets and act as a rigid energy barrier that they must overcome in order to coalesce10,11,12
.
Naphthenic amphiphiles, which make up no more than 4% of bitumen, are another class
of surfactants that notably impact rag layer properties13
. These species, which have a pKa of ~6,
may be categorized as either naphthenic acids (NAs) or naphthenate salts (e.g. sodium
5
naphthenates (NaNs)) depending on the pH of the system14
. Under acidic conditions, where the
pH is less than the pKa of naphthenic amphiphiles, NAs are the dominant surrogate. This term
encompasses all alkyl-substituted cycloaliphatic carboxylic acids (R-COOH) present within
bitumen15
. Like asphaltenes, NAs are oil-soluble and therefore promote the formation of w/o
emulsion droplets14,15
. Under alkaline conditions, where the pH is greater than the pKa of
naphthenic amphiphiles, NaNs are produced via the association of carboxylic acid anions
(COO-) in the oil phase with sodium cations (Na
+) dissolved in the aqueous phase
16. These
metallic soaps aid in emulsification by significantly reducing the oil-water interfacial tension17
.
Being water-soluble, they also induce a shift in the rag layer morphology from w/o to o/w18
. It
has been proposed that the principal mechanism by which naphthenic amphiphiles stabilize
emulsion droplets is by forming lamellar liquid crystals19,20
. These mesomorphic phases, which
are typically produced under concentrated surfactant regimes, spontaneously spread across the
oil-water interface and reduce its mobility and bending ability. Contributions of electrostatic
repulsion are also relevant for the case of NaNs21
.
A lot of work has evidently already gone into understanding the individual influence of
asphaltenes and naphthenic amphiphiles on rag layers. Despite these advancements, very few
efforts have been aimed at practically relating the observed findings to actual commercial hot
water flotation process variables. This highlighted gap is partially addressed in Chapter 2 by
studying the effects of solvent-bitumen-water ratios, solvent aromaticity, and temperature on
asphaltene-stabilized emulsions. A more complete picture emerges in Chapter 3 where the
added effect of naphthenic amphiphiles at different concentrations is tested. From this last set of
data, the theoretically proposed makeup of co-adsorbed asphaltene and naphthenic amphiphile
films is reviewed and new insights are offered.
6
An important lesson learned from Chapters 2 and 3 is that changes to the
physicochemical environment of formed w/o and o/w emulsions leads to changes in their
stability. In knowing so, the next logically posed question is how to predictively model this
relationship. The most widely used approach aimed at doing just so is the hydrophilic-lipophilic
balance (HLB) model22,23,24
. The general premise behind this model is that the experimental
emulsification behavior of a surfactant is related to the difference of its hydrophilic and
lipophilic group contributions. At HLB<10 (HLB>10), stable w/o (o/w) emulsion droplets are
formed. Closer to the balanced (or phase inversion) point (HLB=10), w/o and o/w emulsion
droplets phase separate almost instantaneously. The selection of a surfactant for a given
application is governed by the overall HLB requirement. A notable shortcoming of such is that
this parameter is based purely on the nature of the oil phase. Consequentially, the additional
effect of other physicochemical parameters is ignored.
The hydrophilic-lipophilic deviation (HLD) model has more recently been suggested as
a way of helping overcome the limitations of the HLB model25,26
. The HLD model was
originally devised to track the equilibrium phase behavior of microemulsions (µEs). By
scanning the salinity, oil phase/surfactant hydrophobicity, co-surfactant type/concentration,
and/or temperature to induce a HLD<0HLD=0HLD>0 transition, a shift from o/w µEs in
equilibrium with an excess oil phase (Type I)bicontinuous µEs in equilibrium with excess oil
and aqueous phases (Type III)w/o µEs in equilibrium with an excess aqueous phase (Type II)
is observed. It wasn’t realized until later that upon dispersing these excess phases as emulsion
droplets throughout their continuous µE phase that Type I and Type II stability maxima are
separated by a Type III stability minimum at the phase inversion point. To relate the formation
and stability of heavy crude oil emulsions (such as the above rag layers) using the HLD model,
7
the hydrophobicity of asphaltenic oils (bitumen, deasphalted bitumen, asphalt, and naphthalene)
as well as that of surface-active asphaltene aggregates and naphthenic amphiphiles is evaluated
in Chapter 4. A key finding is that bitumen and toluene share a similar hydrophobicity. This
finding is consistent with the fact that these oils are mutually soluble in one another. As a result
of this, toluene is instead used as the model oil phase of interest going forward because of its
simpler makeup and well-defined properties27,28
.
Despite the advanced usefulness of the HLD model compared to the HLB model in
predicting the stability of emulsions as a function of their formation, it can unfortunately only do
so qualitatively. A better grasp of how the HLD model relates to the kinetic processes common
to demulsification is required for a more quantitative prediction to be achieved. The objective of
Chapter 5 is to experimentally explore this relationship for anionic surfactant (sodium dihexyl
sulfosuccinate (SDHS))-toluene-water emulsions at different surfactant concentrations and
temperatures. In doing so, the total demulsification time is categorized into aggregation,
drainage (settling + film thinning), and coalescence time periods. The advantage of studying
these other emulsions is that it is suspected that the net-average curvature (NAC) model can be
employed to bridge together their HLD and corresponding experimental stability. This suspicion
is based on the fact that the NAC model has been used before to successfully predict numerous
other SDHS-based µE phase behavior properties29
.
The next chapters are thus aimed at predicting the stability of SDHS-toluene-water
emulsions with the aid of the NAC model. To do so, the NAC model is first used to predict the
shape of µE droplets in Chapter 6. These predicted µE droplet shapes are validated via Dr.
Edgar J. Acosta’s efforts to predict their small angle neutron scattering (SANS) profiles. From
these predicted µE droplet shapes, estimates of the continuous µE phase viscosity (ηµE) are
8
obtained. By being able to model ηµE on top of other continuous µE phase properties, emulsion
stability is finally predicted in Chapter 7 using an Arrhenius-like expression. The pre-
exponential part of this fundamental expression reflects the collision frequency of emulsion
droplets whereas the exponential part is indicative of their activation energy barrier. The
applicability of this modeling approach to the stability of other emulsions already published in
the literature is further presented.
In Chapter 8, the HLD and NAC models are both relayed back to the original formation
and stability of rag layers. The calculated HLD of these rag layers is compared against their
experimental morphology at different solvent-bitumen-water ratios, asphaltene to naphthenic
amphiphile ratios, solvent aromaticities, and temperatures. The NAC model is more specifically
applied to rag layers stabilized by a mixture of asphaltenes and NaNs. A discussion of the
experienced shortcomings and challenges that still lay ahead before a complete prediction of rag
layer stability can be obtained is provided towards the end of this chapter.
The conclusions chapter (Chapter 9) summarizes all of the major contributions that can
be drawn from this thesis. A final recommendations chapter (Chapter 10) is also included that
highlights proposed areas of related research that should be carried out to further substantiate
some of the above conclusions.
1.2 REFERENCES
1 Israelachvili, J. The Science and Applications of Emulsions-An Overview. Colloids Surf., A
1994, 91, 1-8.
9
2 Kasoff, M.J. East Meets West in the Canadian Oil Sands. Am. Rev. Can. Stud. 2007, 37, 177-
183.
3 Scales, M.; Werniuk, J. Oil Sands Changing the Face of Canada. Can. Min. J. 2008, 129, 16-
25.
4 Owen, N.A.; Inderwildi, O.R.; King, D.A. The Status of Conventional World Oil Reserves-
Hype or Cause for Concern? Energy Policy 2010, 38, 4743-4749.
5 Shaw, R.C.; Schramm, L.L.; Czarnecki, J. Suspensions in the Hot Water Flotation Process for
Canadian Oil Sands. Adv. Chem. Ser. 1996, 251, 639-675.
6 Yang, X.; Hamza, H.; Czarnecki, J. Investigation of Subfractions of Athabasca Asphaltenes
and Their Role in Emulsion Stability. Energy Fuels 2004, 18, 770-777.
7 Taylor, S.D.; Czarnecki, J.; Masliyah, J. Disjoining Pressure Isotherms of Water-in-Bitumen
Emulsion Films. J. Colloid Interface Sci. 2002, 252, 149-160.
8 Yarranton, H.W.; Hussein, H.; Masliyah, J. Water-in-Hydrocarbon Emulsions Stabilized by
Asphaltenes at Low Concentrations. J. Colloid Interface Sci. 2000, 228, 52-63.
9 Rondón, M.; Pereira, J.C.; Bouriat, P.; Graciaa, A.; Lachaise, J.; Salager, J.-L. Breaking of
Water-in-Crude Oil Emulsions. 2. Influence of Asphaltene Concentration and Diluent Nature on
Demulsifier Action. Energy Fuels 2008, 22, 702-707.
10
10 Sztukowski, D.M.; Jafari, M.; Alboudwarej, H.; Yarranton, H.W. Asphaltene Self-Association
and Water-in-Hydrocarbon Emulsions. J. Colloid Interface Sci. 2003, 265, 179-186.
11 Asekomhe, S.O.; Chiang, R.; Masliyah, J.H.; Elliott, J.A.W. Some Observations on the
Concentration Behavior of a Water-in-Oil Drop with Attached Solids. Ind. Eng. Chem. Res.
2005, 44, 1241-1249.
12 Jiang, T.; Hirasaki, G.; Miller, C.; Moran, K.; Fleury, M.; Diluted Bitumen Water-in-Oil
Emulsion Stability and Characterization by Nuclear Magnetic Resonance (NMR)
Measurements. Energy Fuels 2007, 21, 1325-1336.
13 Barrow, M.P.; Headley, J.V.; Peru, K.M.; Derrick, P.J. Data Visualization of the
Characterization of Naphthenic Acids within Petroleum Samples. Energy Fuels 2009, 23, 2592-
2599.
14 Havre, T.E.; Ese, M.-H.; Sjöblom, J.; Blokhus, A.M. Langmuir Films of Naphthenic Acids at
Different pH and Electrolyte Concentrations. Colloid Polym. Sci. 2002, 280, 647-652.
15 Havre, T.E.; Sjöblom, J. Emulsion Stabilization by Means of Combined Surfactant Multilayer
(D-Phase) and Asphaltene Particles. Colloids Surf., A 2003, 228, 131-142.
16 Brandal, Ø.; Sjöblom, J. Interfacial Behavior of Naphthenic Acids and Multivalent Cations in
Systems with Oil and Water. II: Formation and Stability of Metal Naphthenate Films at Oil-
Water Interfaces. J. Dispersion Sci. Technol. 2005, 26, 53-58.
11
17 Havre, T.E.; Sjöblom, J.; Vindstad, J.E. Oil/Water-Partitioning and Interfacial Behavior of
Naphthenic Acids. J. Dispersion Sci. Technol. 2003, 24, 789-801.
18 Acosta, E.J.; Yuan, J.S.; Bhakta, A.S. The Characteristic Curvature of Ionic Surfactants. J.
Surfactants Deterg. 2008, 11, 145-158.
19 Horváth-Szabó, G.; Czarnecki, J.; Masliyah, J.H. Sandwich Structures at Oil-Water Interfaces
under Alkaline Conditions. J. Colloid Interface Sci. 2002, 253, 427-434.
20 Häger, M.; Ese, M.-H.; Sjöblom, J. Emulsion Inversion in an Oil-Surfactant-Water System
Based on Model Naphthenic Acids under Alkaline Conditions. J. Dispersion Sci. Technol. 2005,
26, 673-682.
21 Arla, D.; Sinquin, A.; Palermo, T.; Hurteyent, C.; Graciaa, A.; Dicharry, C. Influence of pH
and Water Content on the Type and Stability of Acidic Crude Oil Emulsions. Energy Fuels
2007, 21, 1337-1342.
22 Griffin, W.C. Classification of Surface Active Agents by HLB. J. Soc. Cosmet. Chem. 1949,
1, 311-326.
23 Kruglyakov, P.M. Hydrophile-Lipophile Balance of Surfactants and Solid Particles-
Physicochemical Aspects and Applications, 1st ed.; Elsevier Science B.V.: Amsterdam, 2000.
24 Rosen, M.J. Surfactants and Interfacial Phenomena, 3
rd ed.; John Wiley & Sons, Inc.: New
Jersey, 2004.
12
25 Salager, J.L.; Antón, R.; Briceno, M.I.; Choplin, L.; Márquez, L.; Pizzino, A.; Rodriguez,
M.P. The Emergence of Formulation Engineering in Emulsion Making-Transferring Know-How
from Research Laboratory to Plant. Polym. Int. 2003, 52, 471-478.
26 Rondón, M.; Bouriat, P.; Lachaise, J.; Salager, J.-L. Breaking of Water-in-Crude Oil
Emulsions. 1. Physicochemical Phenomenology of Demulsifier Action. Energy Fuels 2006, 20,
1600-1604.
27 Scott, D.W.; Guthrie, G.B.; Messerly, J.F.; Todd, S.S.; Berg, W.T.; Hossenlopp, I.A.;
Mccullough, J.P. Toluene: Thermodynamic Properties, Molecular Vibrations, and Internal
Rotation. J. Phys. Chem. 1962, 66, 911-914.
28 Linde, B.B.J.; Skrodzka, E.B.; Lezhnev, N.B. Vibrational Relaxation in Several Derivatives
of Benzene. Int. J. Thermophys. 2012, 33, 664-679.
29 Acosta, E.; Szekeres, E.; Sabatini, D.A.; Harwell, J.H. Net-Average Curvature Model for
Solubilization and Supersolubilization in Surfactant Microemulsions. Langmuir 2003, 19, 186-
195.
13
CHAPTER 2:
STUDY OF SOLVENT-BITUMEN-WATER RAG LAYERS
This chapter is derived from the following published manuscript:
Kiran, S.K.; Acosta, E.J.; Moran, K. Study of Solvent-Bitumen-Water Rag Layers. Energy
Fuels 2009, 23, 3139-3149.
14
2.1 ABSTRACT
In this chapter, the stability of water-in-oil rag layers was evaluated as a function of
solvent-bitumen-water ratios, solvent aromaticity, and temperature using a combination of
microscopic imaging and spectroscopic techniques. With the aid of these techniques, it was
possible to obtain via material balances an estimate of the amount of oil, water, and asphaltenes
in the rag layer and excess phases. It was observed that when bitumen was diluted with a
paraffinic (or poor) solvent, such as heptol 80/20 (80 vol% heptane and 20 vol% toluene),
asphaltenes in solution tended to preferentially adsorb/segregate at the exposed oil-water
interface and stabilize rag layers. Diluting similar systems with a more aromatic solvent (heptol
50/50, 50 vol% heptane and 50 vol% toluene) reduced the surface activity of asphaltenes and
hence their ability to stabilize rag layers. It was further observed that an increase in temperature
minimized rag layer stability. This effect was explained by the lower viscosity of the oil, which
resulted in its improved drainage from the rag layer.
2.2 INTRODUCTION
A number of studies aimed at illustrating the role that asphaltenes play in stabilizing
water-in-oil (w/o) rag layers have already been published in the literature. Yan et al. showed that
the emulsifying capacity of deasphalted bitumen is minimal1. Yarranton et al. later showed that
asphaltene molecules at a low concentration (≤2 kg/m3) act as surfactant monomers capable of
stabilizing w/o emulsions2. Rondón et al. further demonstrated that a critical aggregation
concentration of asphaltenes exists (~1000 ppm in their system) where the oil-water interface is
saturated3. These researchers additionally hypothesized that the observed reduction in the rate of
demulsification in the presence of excess asphaltenes (beyond the critical aggregation
15
concentration) is due to the formation of micellar aggregates as well as a type of gel phase
adjacent to the interfacial layer. By deflating such asphaltene-stabilized emulsions using
micropipette techniques, Yeung et al. and Tsamantakis et al. proved that excess asphaltenes
adsorb at the oil-water interface as rigid multilayer skins4,5
. Additional results acquired by Yang
et al. showed that asphaltenes are most able to form rigid skins under partially soluble
conditions6. Wu finally revealed that the extent to which asphaltene skins form is enhanced at an
increased oil-water interfacial area (Aow)7. This was confirmed by Gelin et al. who analyzed the
effect of water concentration on the behavior of asphaltenes within reservoir hydrocarbon
fluids8. Obtained results indicate that the concentration of emulsified water significantly affects
the amount and physical properties of asphaltenes lost to the rag layer. While it is not typical for
asphaltenes to adsorb as liquid crystals, there is some evidence of their existence9,10,11
.
Despite these studies with model systems that point to the surface activity of asphaltenes
in stabilizing w/o rag layers, there is a lack of literature characterizing the effectiveness of heavy
crude oil processing variables on the stabilization potential of produced asphaltene skins. One of
the goals of this chapter is to introduce a batch emulsification-separation protocol and method of
analysis to study solvent-bitumen-water rag layers. The second goal of this chapter is to
subsequently study the effect that variables such as solvent-bitumen-water ratios, solvent
aromaticity, and temperature have on the surface activity of asphaltenes and the stability of
formed rag layers. These variables are evaluated by measuring the fraction of oil and asphaltene
losses to the rag layer and the interfacial tension (γow) of all the systems considered.
16
2.3 MATERIALS AND METHODS
2.3.1 Materials
All chemicals were used as supplied: anhydrous toluene (product #244511, 99.8%) was
purchased from Sigma-Aldrich Corp. (Oakville, ON, Canada), reagent grade heptane (product
#5400-1-10) was purchased from Caledon Laboratory Chemicals (Georgetown, ON, Canada),
and coker feed bitumen (16.3% saturates, 39.8% aromatics, 28.5% resins, and 14.7%
asphaltenes according to SARA analysis) was donated by Syncrude Canada Ltd. (Edmonton,
AB, Canada)12
. A salt water solution was prepared by dissolving 25 mmol/L NaCl, 15 mmol/L
NaHCO3, 2 mmol/L Na2SO4, 0.3 mmol/L CaCl2, and 0.3 mmol/L MgCl2 in deionized water to
simulate typical water compositions in oil field operations13
. The pH of this salt water solution
was ~7.5.
2.3.2 Formulation of Rag Layers
The oil phase was prepared by mixing heptol 80/20 (80 vol% heptane and 20 vol%
toluene) and bitumen together at various ratios in individual glass jars overnight using a wrist-
action shaker with a stroke length and frequency of 1.5 inches and 180 strokes/minute
respectively. These mixing parameters were used to ensure that a homogeneous oil phase was
obtained. The diluted bitumen solutions were next added to prescribed amounts of the aqueous
phase in 15 mL glass centrifuge tubes. These formulations were mixed (150 W VWR analog
vortex mixer) at 3200 rpm for 2 minutes and then centrifuged (IEC clinical centrifuge) at 500 g
for 1 minute at 25°C. The development of these emulsification and separation protocols will be
discussed later. The compositions of solvent-bitumen-water systems tested in this work are
presented in Table 2.1.
17
Table 2.1: Compositions (wt%) of tested heptol (H)-bitumen (B)-water (W) systems.
Heptol/Bitumen
Ratio 1/1.5 1/1 3/1 4/1 10/1
W H B H B H B H B H B
75 10 15 12.5 12.5 18.8 6.3 20 5 22.7 2.3
50 20 30 25 25 37.5 12.5 40 10 45.5 4.5
25 30 45 37.5 37.5 56.3 18.8 60 15 68.2 6.8
9.1 36.4 54.5 45.5 45.5 68.2 22.7 72.7 18.2 82.6 8.3
0 40 60 50 50 75 25 80 20 90.9 9.1
The same systems described in Table 2.1 were studied at 80°C by placing the test tubes
in a hot water bath prior to mixing and centrifuging. Another set of phase behavior studies was
also carried out using heptol 50/50 (50 vol% heptane and 50 vol% toluene) as the solvent.
2.3.3 Microscopy
The oil phase, aqueous phase, and rag layer produced in all the formulations after mixing
and centrifuging were sampled and analyzed according to slight variations in the procedure
developed by Varadaraj et al.14
. To sample the excess oil phase (top phase), a small volume of
oil was slowly extracted using a 5 mL pipet. When sampling the rag layer (middle phase) and
aqueous phase (bottom phase), a small positive pressure was applied during the insertion and
extraction of the pipet to ensure that no additional phases were sampled along with the phase of
interest. Three distinct sampling points were used for each of the phases to guarantee that the
sample was representative. All extracted samples were imaged using an Olympus C-7070 wide
zoom digital camera at 4× magnification mounted on top of an Olympus BX-51 microscope set
at 50× magnification. Three different microscope configurations were used: optical (transmitted)
light (to differentiate between solid and liquid phases), cross-polarized light (to detect liquid
crystals), and fluorescent light (to differentiate between oil (green) and aqueous (black) phases).
18
2.3.4 Material Balances
Because of the variable composition and density of the rag layer in all the systems
studied, material balances were performed by tracking the volume of each formulation
component in all the phases produced after mixing and centrifuging. The volume of each phase
produced was calculated by measuring the relative heights of the separated oil phase, aqueous
phase, and rag layer. The separated oil phase was considered a recoverable and useful product in
which only minor traces of water were dispersed throughout. This was confirmed by measuring
its water content using Karl Fischer titration (<0.2 vol% for all systems) and the microscopy
techniques in Section 2.3.3. The purity of the separated aqueous phase was confirmed using
only micrographs to track suspended or dissolved oil. To determine the volume of oil and water
within the rag layer, their volume fractions were first calculated by analyzing the captured
fluorescent micrographs using Scion Image Software15
:
1) A drop of the rag layer sample (20 µL) was deposited on top of a glass slide and then
carefully covered with a coverslip. This forced the rag layer sample to evenly spread and
form a thin film of 10 µm. This film thickness was determined by dividing the volume of
the deposited rag layer sample by the area of the glass slide-coverslip assembly.
2) The threshold used to transform a fluorescent micrograph into a binary map of clear (oil)
and dark (water) areas was adjusted such that the boundary between the oil and water areas
was located at the middle of their fuzzy interface. This fuzzy interface was caused by the
curvature of the walls of the squeezed water droplets. Non-squeezed water droplets with a
diameter <10 µm were not commonly observed.
19
3) The area of the rag layer image was calculated along with that of the oil and water phases
using measurement tools within the software package.
4) Knowing the area of both the oil and water phases (pixels2) as well as the area of the entire
image (pixels2), the fractional areas (and hence volume fractions) of oil and water within
the rag layer were calculated.
From these calculated volume fractions, the volumes of oil and water within the rag
layer were determined. The measured amount of oil and water in the excess phases and within
the rag layer in a given test tube agreed within ±1 vol% of the known volume of oil and water
initially added (this is the material balance closure). Experiments with larger deviations were
rejected and repeated. The standard deviation of oil losses to the rag layer in replicate systems
was ≤5 vol%. It needs to be clarified that the above material balance approach is only useful in
exploring oil-water phase separation trends. Its accuracy has yet to be compared against more
established methods (i.e. gravimetric techniques).
2.3.5 Asphaltene Losses
Yang et al. developed a UV-vis spectroscopic technique to analyze the concentration of
asphaltenes in heavy crude oils6. This technique was adapted here to quantify asphaltene losses
to the rag layer (as a fraction of their initial concentration in the oil phase). These losses include
interfacially adsorbed/segregated asphaltenes and precipitated aggregates. To this end, a
calibration curve of asphaltene absorbance (optical density) at a wavelength of 450 nm and as a
function of its concentration (expressed in terms of a bitumen dilution ratio) was generated to
establish a baseline asphaltene absorbance in the oil phase under soluble conditions. The optical
density of all the solutions was measured using an Ocean Optics spectrophotometer (model
20
#HR2000). Toluene was used as the solvent because it completely solubilizes asphaltenes. The
relationship between the optical density (absorbance) and concentration of asphaltenes is shown
in Figure 2.1.
y = 2.08x + 0.09 ( 0.03)R² = 0.99 0.09
0
0.5
1
1.5
2
2.5
3
3.5
0.0 0.5 1.0 1.5
Ab
so
rba
nc
e
Bitumen to Toluene Ratio (x103)
Figure 2.1: Calibration of asphaltene absorbance at a wavelength of 450 nm and as a function
of the bitumen to toluene ratio.
To determine the fraction of asphaltene losses from the separated oil phase of
experimental systems after mixing and centrifuging, a sample (which already includes heptol)
was further diluted with a known volume of toluene and its resulting optical density was
measured. The following difference between the baseline and experimental absorbances
represents the fraction of asphaltene losses to the rag layer:
100%
AbsorbanceBaseline
AbsorbancealExperimentAbsorbanceBaselineLossesAsphaltene (Eq. 1)
It is important to clarify that the fraction of asphaltene losses is not used in the material
balance of oil and it does not necessarily depend, at least from the material balance point of
view, on the fraction of oil losses to the rag layer. For example, one could have a significant
21
fraction of oil losses to the rag layer and yet no asphaltene losses if the concentration of
asphaltenes in the separated oil phase is the same as that of the original oil. The fraction of
asphaltene losses only reflects the change in the concentration of asphaltenes in the separated oil
phase with respect to the original oil.
2.3.6 Interfacial Tension Measurements
To measure the γow of the systems analyzed, a spinning drop tensiometer manufactured
by Temco Inc. (model #500) was used. In this technique, a borosilicate glass tube was first
completely filled with the separated aqueous phase that was recovered from the formulations
after mixing and centrifuging. A droplet (~5 µL) of the separated oil phase was then inserted
into the aqueous phase and the glass tube was spun at increasing rpm values until the oil droplet
expanded sufficiently such that its length was 4 times greater than its width. Once the oil droplet
expansion reached an equilibrium value at a given rpm, the γow was calculated as follows:
4
32wow
(Eq. 2)
In this equation, Δρ is the difference in density between the heavy (water) and light (oil)
phases, ω is the rotational velocity, and w is the width of the expanded oil droplet. Through the
use of a thermocouple and temperature controller, the operating temperature of the device was
easily adjusted.
22
2.4 RESULTS
2.4.1 Phase Separation of Solvent-Bitumen-Water Systems
The separated oil phase, aqueous phase, and rag layer of each of the mixed and
centrifuged formulations are analyzed using optical, cross-polarized, and fluorescence
microscopy. Micrographs taken for a system containing 68.2 wt% heptol 80/20, 6.8 wt%
bitumen, and 25 wt% water at 25°C are displayed in Figure 2.2. The images of Figure 2.2
illustrate that in these experiments, significant w/o emulsions occur throughout the rag layer
whereas the excess oil and aqueous phases contain insignificant traces of water and oil
respectively. As a result, the assumption of pure recoverable oil and aqueous phases when
performing material balances is reasonable. These results are consistent for all other
formulations analyzed. Although liquid crystals are sometimes observed in systems prepared at
25°C with heptol 80/20 and heptol 50/50 as the diluents, their relative concentration within the
rag layer (<1%) suggests that they play a minor role in promoting emulsion stability. No liquid
crystal formation occurred in the systems prepared at 80°C.
23
250 µm
RAG
LAYER
OIL
PHASE
AQUEOUS
PHASE
i) ii)
iii)
ii)
i)
iii)
i)
ii)
iii)
Figure 2.2: (i) Optical, (ii) cross-polarized, and (iii) fluorescent micrographs of samples of the
separated oil phase, aqueous phase, and rag layer for a system containing 68.2 wt% heptol
80/20, 6.8 wt% bitumen, and 25 wt% water at 25°C.
When the phase heights and micrographs are analyzed in greater detail, a material
balance closure is obtained in which the volumes of the separated oil and aqueous phases and
the volumes of oil and water within the rag layer are estimated. Table 2.2 displays calculated
values for each of these parameters for systems prepared with 50 wt% water at various heptol
80/20 to bitumen dilution ratios and 25°C. The columns labeled as % error refer to the
difference between the total volume of each component (oil or water) initially added and that
calculated using the material balance.
24
Table 2.2: Material balance closure for systems prepared with 50 wt% water (W) at various
heptol 80/20 (H) to bitumen (B) dilution ratios and 25°C.
Composition
(cm3) Phases
Phase
Height
(mm)
Phase
Volume
(cm3)
Rag Layer
Image
(Scion)
Water to
Oil Ratio
(vol/vol)
%
Asphaltene
Losses
%
Error
Oil
%
Error
Water W H B
5 2.8 3
Oil 34 4.9
5.6 8 0.1 -0.1 Rag 40 5.7
Water 1 0.1
5 3.4 2.5
Oil 35 5
5.5 10 -0.12 0.2 Rag 39.5 5.7
Water 1.5 0.2
5 5.2 1.2
Oil 37 5.2
2.6 13 -0.3 0.4 Rag 30 4.2
Water 14 2
5 5.5 1
Oil 37 5.2
3.2 17 -0.3 0.4 Rag 39 5.5
Water 6 0.8
5 6.3 0.5
Oil 36 5.1
2.7 27 0 0 Rag 41 5.9
Water 5 0.7
On the basis of these results, the material balance closure is satisfactory, which validates
the procedures used to analyze the systems produced with the batch emulsification-separation
protocol.
2.4.2 Development of Batch Emulsification-Separation Protocol
To determine the appropriate mixing conditions for solvent-bitumen-water systems that
reflect the rag layers produced in industry, various formulations are mixed at 3200 rpm from 20
seconds to 5 minutes. The samples are then centrifuged for 20 minutes at 1000 g and the fraction
of oil and asphaltene losses to the rag layer are determined according to the procedures
described above. The data is presented in Figures 2.3 (a) and (b).
25
(a)
Oil
Lo
sses
to R
ag
La
yer
(V
ol
%)
Asp
ha
lten
e L
oss
es t
o R
ag
La
yer
(%
)
Mixing Time (Minutes)
56.25 wt% Heptol 80/20-18.75 wt%
Bitumen-25 wt% Water
18.75 wt% Heptol 80/20-6.25 wt%
Bitumen-75 wt% Water
(b)
Figure 2.3: (a) Oil and (b) asphaltene losses to the rag layer as a function of the mixing time for
systems prepared with either 25 wt% or 75 wt% water and the balance oil with a heptol 80/20 to
bitumen dilution ratio of 3 at 25°C.
The trends observed in Figures 2.3 (a) and (b) suggest that mixing conditions have a
significant impact on rag layer stability and the fate of asphaltenes. Furthermore, the data shows
from the time required for oil and asphaltene losses to plateau for the different formulations that
a steady state condition is reached at ~2 minutes. This time is used as a standard mixing time
going forward.
To select the appropriate separation conditions for these rag layers, various formulations
are mixed for 2 minutes at 3200 rpm and then either left to settle on their own (1 g) for up to
5000 minutes or arbitrarily centrifuged at 35 g for up to 143 minutes. The fraction of oil losses
26
to the rag layer at different times is then determined from the measured phase volumes (heights).
In Figures 2.4 (a)-(d), the fraction of oil losses to the rag layer is presented for different
formulations as a function of the g force × time. According to common practice and recent
models, the separation of a given suspension is expected to be a function of the g force × time as
it is proportional to the settling velocity × time16
.
g Force x Time (g x Minutes)
Oil L
osses t
o R
ag
Layer
(Vo
l %
)
(a) (b)
(c) (d)
1 g, 5000 Minutes 35 g, 143 Minutes
Figure 2.4: Oil losses to the rag layer as a function of the g force × time for systems prepared
with (a) 12.5 wt% heptol 80/20, 12.5 wt% bitumen, and 75 wt% water, (b) 20 wt% heptol 80/20,
5 wt% bitumen, and 75 wt% water, (c) 37.5 wt% heptol 80/20, 37.5 wt% bitumen, and 25 wt%
water, and (d) 60 wt% heptol 80/20, 15 wt% bitumen, and 25 wt% water.
The data in Figures 2.4 (a)-(d) confirms that g force × time is indeed the governing
parameter that describes the phase separation efficiency of a given system. In this work, 500 g ×
27
min is selected as the condition to evaluate the separation of rag layers. This parameter is
consistent with that published in the literature17
.
2.4.3 Trends of Oil and Asphaltene Losses to the Rag Layer
Oil and asphaltene losses to the rag layer are evaluated as a function of the solvent-
bitumen-water ratios, solvent aromaticity, and temperature. A summary of the obtained results is
presented in Figures 2.5 (a)-(f).
(b)
(d)
(e) (f)
Oil
Lo
sses
to
Ra
g L
ay
er (
Vo
l%)
Asp
ha
lten
e L
oss
es t
o R
ag
La
yer
(%
)
Heptol 80/20 to Bitumen Dilution Ratio Heptol 80/20 to Bitumen Dilution Ratio
Heptol 50/50 to Bitumen Dilution Ratio Heptol 50/50 to Bitumen Dilution Ratio
(c)
(a)
75 wt% Water 50 wt% Water 25 wt% Water 9.1 wt% Water 0 wt% Water
Figure 2.5: Oil and asphaltene losses to the rag layer for systems prepared with (a and b) heptol
80/20 at 25°C, (c and d) heptol 80/20 at 80°C, and (e and f) heptol 50/50 at 25°C.
28
To facilitate the presentation of the data in Figures 2.5 (a)-(f) and to enhance the visual
clarity of the obtained trends, only the upper or lower half of the error bars is shown to prevent
overlapping of the results. For systems prepared with heptol 80/20 as the solvent, increasing the
bitumen dilution ratio or water content produces an increase in the fraction of oil and asphaltene
losses to the rag layer. At 80°C, however, the oil losses are approximately half of that observed
at 25°C, whereas the fraction of asphaltene losses is only slightly reduced. For systems prepared
with heptol 50/50 as the solvent at 25°C, increasing the bitumen dilution ratio reduces the
amount of oil and asphaltene losses to the rag layer and excellent phase separation is obtained
for most systems, with the exception of those prepared with high water content and low bitumen
dilution ratios. Although traces of insoluble asphaltene aggregates are physically observed in
formulations prepared with heptol 80/20 and heptol 50/50 in the presence of 0 wt% water, the
absolute error in the UV-vis method used to estimate asphaltene losses is close to 3%,
suggesting that precipitation is minimal in these systems. To estimate the onset of asphaltene
precipitation, the fraction of asphaltene losses from the oil is determined as a function of the
heptane concentration in heptol at a dilution ratio of 10 and in the absence of water. It is found
that the fraction of asphaltene losses from the oil phase increases from 5% to 52% (forming a
substantial amount of precipitate at the bottom of the vial) as the percentage of heptane in heptol
is increased from 80 vol% to 85 vol%. This observation confirms that heptol 80/20 can be
considered a “poor” solvent because its composition is very close to that of the onset of
asphaltene precipitation. On the other hand, heptol 50/50 is more aromatic than heptol 80/20 and
therefore a more suitable solvent to dissolve asphaltenes.
From a processing perspective, the ternary phase diagrams presented in Figures 2.6 (a)-
(c) display transitions in achievable oil recovery under a given set of operational conditions.
29
Gradient Scale
(Oil Losses to Rag Layer (Vol%)
wt% Bitumen
(a) (b)
wt% Bitumen
(c)
wt% Bitumen
Figure 2.6: Ternary phase diagrams for systems prepared with (a) heptol 80/20 at 25°C, (b)
heptol 80/20 at 80°C, and (c) heptol 50/50 at 25°C.
It should be noted that, although the trends of oil and asphaltene losses to the rag layer
using coker feed bitumen are relevant to the bitumen recovery process, one cannot forget the
fact that, in producing coker feed bitumen, the composition of bitumen may have changed to a
certain degree. It is important to keep this in mind when trying to extrapolate these results and
ensuing discussions to other bitumen sources or heavy crude oils.
30
2.5 DISCUSSIONS
2.5.1 Effect of Heptol 80/20 to Bitumen Dilution Ratio and Water Content on
Rag Layer Stability
As shown in Figures 2.5 (a)-(d), an increase in the heptol 80/20 to bitumen dilution ratio
results in increased oil and asphaltene losses to the rag layer. This effect can be explained on the
basis that heptol 80/20 is enriched in heptane to a point that it is almost at the asphaltene
precipitation threshold and it is therefore an environment not favorable for asphaltenes18,19
. It is
believed, according to Gawrys et al., that asphaltenes become less soluble in the oil phase at
dilution ratios up to 10 because their aggregate size continuously increases20
. The shift in the
equilibrium partitioning of asphaltenes within solvent-bitumen-water systems can be
represented using the following simple relation2:
(Eq. 3)
To interpret the data of Figures 2.5 (a)-(d) in light of Equation 3, it is necessary to
highlight that, in the absence of water, asphaltene losses, which are typically ≤5%, are only
associated with precipitation. However, in the presence of water, a significant fraction of
asphaltene losses are associated with the formation of asphaltene aggregates that segregate near
the oil-water interface. By promoting the formation of interfacially adsorbed asphaltene
aggregates at increased heptol 80/20 to bitumen dilution ratios, rigid asphaltene skins are
produced, which enhance emulsion stability and lead to an increased fraction of oil losses to the
rag layer. This explanation is consistent with the observations of Sztukowski et al. and Moran et
al. that, when the solubility of asphaltenes is reduced at increased bitumen dilution ratios in the
presence of water, emulsion stability is enhanced21,22
. These researchers suggested that
Interfacial
Asphaltenes
Soluble
Asphaltenes Precipitated
Asphaltenes
31
asphaltene aggregates adhere to the primary layer of adsorbed asphaltenes at the oil-water
interface, preventing bridging between adjacent droplets. There is little known about the
molecular interactions that lead to the formation of interfacial asphaltene aggregates. Tan et al.,
however, proposed that hydrogen bonding may induce their association at the oil-water
interface23
.
These findings suggest that it is important to quantify Aow and how it is produced. As
evidenced in Figures 2.3 (a) and (b), the method of emulsification (such as mixing time)
influences the fraction of oil and asphaltene losses to the rag layer. These observations are
consistent with previous reports24
. A simplistic way of understanding the process of
emulsification is through the use of the Weber (We) number. The We number relates the inertial
and interfacial forces of emulsion droplets as follows25,26
:
ow
rel
E
d
E
c vdWe
2
(Eq. 4)
In this equation, E
c is the density of the emulsion’s continuous oil phase, E
dd is the
average emulsion droplet diameter, and vrel is the relative mixing velocity of the continuous oil
phase and emulsified aqueous phase. As the We number of an emulsified water droplet
increases above its critical value (~1-2), it becomes unstable and breaks up into smaller droplets
until E
dd becomes small enough to offset any further shearing. According to Figures 2.3 (a) and
(b), the process of emulsion droplet break-up takes about 2 minutes, which is considerably lower
than the amount of time required for γow to reach equilibrium (~16-40 minutes depending on the
asphaltene concentration)27
. This difference in time scale can be explained by the formation of
asphaltene skins. It is important to clarify that in industrial practice the process of emulsification
can be quite different, depending upon the flow dynamics inherent to it.
32
The value of Aow can be estimated as the product of the volume of the emulsified
aqueous phase ( E
wV ) and the average surface area ( E
dA ) to volume ( E
dV ) ratio of the spherical
water droplets as follows:
E
d
E
dE
wowV
AVA (Eq. 5)
The average E
dA to E
dV ratio of emulsified water droplets can be expressed in terms of
E
dd as follows2:
E
d
E
d
E
d
dV
A 6 (Eq. 6)
To calculate E
dd , the diameters of the squeezed cylindrical droplets obtained through
image analysis are first transformed into sphere-equivalent diameters. The calculated sphere-
equivalent water droplet diameters are then converted into E
dd as follows2:
2
3
E
ii
E
iiE
d
dF
dFd (Eq. 7)
In this equation, E
iF is the number frequency of water droplets of sphere-equivalent
diameter E
id . Equations 6 and 7 can be incorporated into Equation 5 to yield the following
alternative expression for Aow:
2
3
6
E
ii
E
ii
E
w
ow
dF
dF
VA (Eq. 8)
33
Figures 2.7 (a) and (b) present calculated estimates of E
dd as a function of the heptol
80/20 to bitumen dilution ratio and water content as well as a sample E
id distribution at 50 wt%
water. Figure 2.7 (c) presents estimates of Aow normalized by the volume of bitumen.
0
5
10
15
20
25
30
35
40
0 2 4 6 8 10
Sau
ter
Mean
Dia
mete
r (µ
m)
Heptol (80/20) to Bitumen Dilution Ratio
75 wt% SW
50 wt% SW
25 wt% SW
9.09 wt% SW
0
2
4
6H/B=1/1.5
H/B=1/1
H/B=3/1
H/B=4/1
H/B=10/1
FiE
diE (µm)
0
2000
4000
6000
8000
10000
12000
14000
16000
18000
0 2 4 6 8 10
Are
a/V
olu
me o
f B
itu
men
(1/c
m)
Heptol (80/20) to Bitumen Dilution Ratio
75 wt% SW
50 wt% SW
25 wt% SW
9.09 wt% SW
(a)
(b)
(c)
dd
E(µ
m)
No
rma
lize
d A
ow
(1/c
m)
Figure 2.7: (a) E
dd , (b) sample E
id distribution at 50 wt% water, and (c) normalized Aow of
heptol 80/20-diluted bitumen droplets at 25°C.
34
With respect to the calculated E
dd estimates in Figure 2.7 (a), larger droplet sizes are
obtained at increased heptol 80/20 to bitumen dilution ratios, which, as will be discussed later,
can be attributed to increased γow. With respect to the normalized Aow, Figure 2.7 (c) shows that
increasing the water content from 0 to 50 wt% increases Aow. For systems containing 25 wt%
and 75 wt% water, Aow are similar. These results suggest that Aow is proportional to the product
of the oil and water volume fractions in the test tube. Furthermore, one may also conclude by
analyzing the asphaltene losses presented in Figure 2.5 (b) in conjunction with the normalized
Aow results that the asphaltene surface coverage, calculated by assuming that the asphaltene
losses are due to adsorption only, for most heptol 80/20 systems at 25°C is 40-50 mg/m2. The
asphaltene surface coverage is ~1 order of magnitude larger for systems prepared with 9.1 wt%
water. This is likely due to the smaller Aow produced with these systems and the assumption that
all asphaltene losses correspond to adsorption. These observations support the hypothesis that
the formation of rag layers and their stability is highly dependent upon the amount of Aow
created during the different process operations. The average asphaltene surface coverage of 40-
50 mg/m2 is of the same order of magnitude but several folds larger than that obtained by
Gafonova and Yarranton using heptol 50/50 (~10 mg/m2)28
. For the heptol 50/50 systems
presented later, asphaltene surface coverage values of 6-12 mg/m2 are obtained at dilution ratios
≥3, corresponding to the range of asphaltene concentrations considered by Gafonova and
Yarranton.
The normalized Aow is also observed to increase with the heptol 80/20 to bitumen
dilution ratio. This suggests that diluting bitumen with such a poor solvent promotes the
segregation of asphaltenes near the oil-water interface, thus stabilizing more of the interface
35
created during mixing. This observation is consistent with the larger asphaltene losses at
increased heptol 80/20 to bitumen dilution ratios observed in Figure 2.5 (b).
2.5.2 Effect of Temperature and Solvent Aromaticity on Rag Layer Stability
According to Figures 2.5 (c) and (e), an improved separation of the oil phase can be
obtained by either increasing the temperature or the solvent aromaticity. With regards to an
increase in the temperature, it is important to note that this strategy reduces the fraction of oil
losses to the rag layer but does very little to the fraction of asphaltene losses. In this case, it
seems that increasing the temperature facilitates the drainage of oil from the rag layer, which
may be due to its reduction in viscosity and/or a weakening of the dipole-induced dipole or van
der Waals forces between the oil and asphaltene skins29,30,31
. This drainage effect at elevated
temperatures is believed to be furthermore assisted by the fact that the reduced viscosity of the
continuous oil phase and the reduced yield strength and elastic modulus of asphaltene skins
leads to more effective collisions of dispersed water droplets32
.
When Figures 2.5 (e) and (f) are compared to Figures 2.5 (a) and (b), one can appreciate
that the trends of oil and asphaltene losses to the rag layer with increasing bitumen dilution
ratios are opposite for heptol 80/20 and heptol 50/50. In the case of heptol 80/20, the large
fraction of heptane in the oil phase shifts the equilibrium of Equation 3 towards the formation of
interfacial asphaltene aggregates. These comments are consistent with the studies performed by
McLean et al. that show that asphaltenes stabilize w/o emulsions by collecting at the interface in
the form of aggregates33
. On the other hand, heptol 50/50 is an aromatic solvent, containing a
heptane concentration considerably lower than the threshold precipitation concentration of 80-
85 vol% of heptane. Thus, increasing the heptol 50/50 to bitumen dilution ratio reduces the
36
tendency of asphaltenes to segregate at the oil-water interface. This point will be discussed in
more detail in the next section.
A surprising element in Figures 2.5 (a) and (e) is that, at low bitumen dilution ratios
(≤1), heptol 50/50 significantly magnifies emulsion stability in comparison to heptol 80/20. A
likely explanation for this, according to the experimental proof Figures 2.8 (a)-(d), is that the
reduced droplet diameter in heptol 50/50 systems provides for an increased Aow that asphaltenes
can adsorb/segregate to. The Aow produced in heptol 80/20 and heptol 50/50 systems under such
processing conditions are 0.4 m2 and 1.5 m
2 respectively. Furthermore, the mechanical
properties of the adsorbed asphaltene skins and/or the kinetics of their formation (likely faster in
heptol 50/50 at low dilution ratios due to the enhanced diffusion of smaller aggregate sizes) may
be important factors to consider. Figures 2.8 (a)-(d) show that the water droplets in heptol 80/20
systems are separated but, for the case of heptol 50/50 systems, there is a network of smaller
droplets that are attached to each other.
37
Heptol 80/20 Systems
Heptol 50/50 Systems
a) b)
c) d)
250 µm
Figure 2.8: Morphology of emulsions for systems prepared with (a) 10 wt% heptol 80/20, 15
wt% bitumen, and 75 wt% water, (b) 12.5 wt% heptol 80/20, 12.5 wt% bitumen, and 75 wt%
water, (c) 10 wt% heptol 50/50, 15 wt% bitumen, and 75 wt% water, and (d) 12.5 wt% heptol
50/50, 12.5 wt% bitumen, and 75 wt% water.
2.5.3 Surface Activity of Asphaltenes
The γow of the separated oil and aqueous phases for the formulations in Figures 2.5 (a)-
(f) are measured to substantiate previously established phase behavior results and gain a better
understanding of the surface activity of asphaltenes and their role in promoting emulsion
stability. This data is presented in Figures 2.9 (a)-(c) as a function of the solvent-bitumen-water
ratios.
38
(b)
(c)
Heptol (50/50) to Bitumen Dilution Ratio
Heptol (80/20) to Bitumen Dilution Ratio
γo
w(m
N/m
)
(a)
(b)
(c)
75 wt% Water 50 wt% Water 25 wt% Water 9.1 wt% Water
Figure 2.9: The measured γow as a function of solvent-bitumen-water ratios for systems
prepared with (a) heptol 80/20 at 25°C, (b) heptol 80/20 at 80°C, and (c) heptol 50/50 at 25°C.
According to this data, the γow of all the systems increases with increasing heptol to
bitumen dilution ratios and water content. For the case of the heptol 80/20 systems in Figures
2.9 (a) and (b), the increased γow can be linked to the increased asphaltene losses from the
separated oil phase at an increased bitumen dilution ratio and water content. In the case of
39
heptol 50/50 systems, the increased γow can be explained on the basis of a dilution effect. When
the bitumen dilution ratio is increased, the concentration of asphaltenes in the recovered oil
phase falls below their critical transition concentration and their surface activity is compromised
(see discussion of Figure 2.10). The increased γow with the heptol to bitumen dilution ratios can,
according to the critical We number, be linked to the increase in E
dd .
To evaluate the surface activity of asphaltenes in heptol 80/20 and heptol 50/50,
asphaltenes are first extracted from bitumen (after a 13 to 1 dilution with heptane) and then
redissolved in each solvent at different concentrations. The measured γow as a function of the
asphaltene concentration is presented in Figure 2.10.
8
13
18
23
28
33
0.001 0.01 0.1 1 10
Asphaltene Concentration (%)
γow
(mN
/m)
Heptol 80/20
Heptol 50/50
Critical Aggregation Concentration
(CAC) for asphaltene monomers in
heptol 80/20
Critical Transition Concentration
(CTC) for asphaltene aggregates
in heptol 80/20
Figure 2.10: The measured γow (against water) of asphaltenes diluted in heptol 80/20 and heptol
50/50 at 25°C.
The difference between the initial and final (equilibrium) asphaltene concentrations are
estimated using known values of asphaltene surface coverage. At low asphaltene concentrations
(~1×10-3
%), one expects monolayer coverage (~1 mg/m2). Because a 5 µL droplet of
40
asphaltenes in heptol is introduced into the tensiometer, this represents an equivalent loss of
asphaltenes of ~2×10-4
% (or a 20% difference in concentration). At high asphaltene
concentrations (~6%), the asphaltene surface coverage is, at most, 50 mg/m2. This would
produce an equivalent loss of asphaltenes of ~1×10-2
% (or a 0.2% difference in concentration).
Therefore, the trends observed in Figure 2.10 should approach the trends observed if the
equilibrium concentrations were used instead of the initial concentrations. As the concentration
of asphaltenes in heptol 80/20 increases up to ~250 ppm, the γow decreases to a value near 17
mN/m. This transition is typically referred to as the critical aggregation concentration (or CAC)
where asphaltene aggregates begin to form. The values of γow leading up to the CAC and near
the CAC are consistent with those reported in most of the studies involving asphaltenes and
bitumen.
As the asphaltene concentration is increased beyond the CAC for heptol 80/20 systems,
γow remains nearly constant until the asphaltene concentration approaches 1%. At this point,
which will be referred to as the critical transition concentration (CTC), there is a second
transition in γow. The γow values leading up to the CTC and after the CTC are not as common as
those associated with the CAC. They have, however, been observed for select systems
containing asphaltenes with acidic or highly polar moieties34,35
. One cannot disregard the
possibility that these highly polar species are residual process aids in the bitumen. It is unlikely,
however, that they would have precipitated along with asphaltenes in the hexane dilution step.
This kind of transition associated with the CTC has been observed before in microemulsions
where it is commonly referred to as the critical microemulsion concentration (cµc)36
. The cµc
marks the formation of net-zero curvature films of surfactants adsorbed at oil-water interfaces. It
is possible, therefore, that the CTC marks the change in morphology of the asphaltene
41
aggregates segregated near the oil-water interface. Considering Figure 2.10, Figures 2.5 (b) and
(f), and that bitumen contains ~15% asphaltenes, one can infer that, for system above the CTC
(dilution ratios lower than 10 for heptol 80/20 and lower than 3 for heptol 50/50), asphaltenes
tend to segregate near the oil-water interface (the left side of Equation 3). This also reinforces
the fact that asphaltenes in heptol 50/50 are less surface-active than asphaltenes dissolved in a
“poor” solvent such as heptol 80/20.
2.5.4 Correlation of Oil and Asphaltene Losses to the Rag Layer
The general correlations of oil and asphaltene losses to the rag layer for systems
prepared with heptol 80/20 at 25°C and 80°C are presented in Figure 2.11.
(b)
(a)
Oil
Lo
sses
to
Ra
g L
ay
er (
Vo
l%)
Asphaltene Losses to Rag Layer (%)
Figure 2.11: Correlations of oil and asphaltene losses to the rag layer for systems prepared with
heptol 80/20 at (a) 25°C and (b) 80°C.
42
This data reinforces the hypothesis that asphaltene losses to the rag layer help stabilize
emulsions because a reduced concentration of asphaltenes is observed in the recovered oil phase
at increased oil losses to the rag layer. While one could argue that there is a linear correlation
between these variables, there is also substantial scatter in the data. This scatter is partially
explained by variations in the physical characteristics of monomeric asphaltenes37
. The resulting
packing constraints of asphaltenes affect their aggregation behavior at different dilution ratios
and ability to adsorb at the oil-water interface. As a result, the mechanical properties of
asphaltene skins produced differ, which results in different extents of rag layer formation and
stabilization. The real value of Figure 2.11 is to highlight the importance of the formulation
conditions because they affect the fraction of asphaltene losses that, in turn, influence the
fraction of oil losses to the rag layer. To find a numerical relation, the equilibrium between the
dissolved and interfacial asphaltenes needs to be better understood as well as the morphology
and mechanical properties of the asphaltene skins produced under different formulation
conditions.
2.6 CONCLUSIONS
In this work, a methodology involving phase volume measurements, optical, cross-
polarized, and fluorescence microscopy, and UV-vis spectroscopy was introduced to evaluate
the stability of solvent-bitumen-water rag layers and its relation to the surface activity of
asphaltenes. It was confirmed that the phase separation of these systems was severely impacted
by the formation of asphaltene aggregates that segregated near the oil-water interface. A major
finding in this study was that the water content in the formulation played a critical role on the
observed phase behavior because it impacted the amount of interfacial area produced that
asphaltenes could potentially segregate to. The tendency of asphaltenes to segregate or adsorb at
43
the oil-water interface depended upon the nature of the solvent used to dilute the bitumen. When
using a poor solvent, such as heptol 80/20, whose high heptane concentration is close to that of
the onset of asphaltene precipitation, an increase in the dilution ratio created a less suitable
environment for asphaltenes. This induced the segregation of asphaltenes at the oil-water
interface. Using a more aromatic solvent, such as heptol 50/50, reduced the tendency of
asphaltenes to segregate near the oil-water interface as the dilution ratio increased. In all cases,
the segregation of asphaltenes at the oil-water interface, as reflected by the asphaltene losses,
was correlated with increased oil losses to the rag layer. Another interesting finding was that the
increase in temperature did not seem to affect the segregation of asphaltenes. It did, however,
facilitate the drainage (and hence recovery) of the continuous oil phase from the rag layer.
Finally, the interfacial tension studies of precipitated and redissolved asphaltenes suggested that
asphaltenes may undergo different transitions with an increase in their concentration. The nature
of such transitions is a topic that should be further investigated.
2.7 REFERENCES
1 Yan, Z.; Elliott, J.A.W.; Masliyah, J. Roles of Various Bitumen Components in the Stability of
Water-in-Diluted Bitumen Emulsions. J. Colloid Interface Sci. 1999, 220, 329-337.
2 Yarranton, H.W.; Hussein, H.; Masliyah, J. Water-in-Hydrocarbon Emulsions Stabilized by
Asphaltenes at Low Concentrations. J. Colloid Interface Sci. 2000, 228, 52-63.
44
3 Rondón, M.; Pereira, J.C.; Bouriat, P.; Graciaa, A.; Lachaise, J.; Salager, J.-L. Breaking of
Water-in-Crude Oil Emulsions. 2. Influence of Asphaltene Concentration and Diluent Nature on
Demulsifier Action. Energy Fuels 2008, 22, 702-707.
4 Yeung, A.; Dabros, T.; Masliyah, J.; Czarnecki, J. Micropipette: A New Technique in
Emulsion Research. Colloids Surf., A 2000, 174, 169-181.
5 Tsamantakis, C.; Masliyah, J.; Yeung, A.; Gentzis, T. Investigation of the Interfacial
Properties of Water-in-Diluted Bitumen Emulsions using Micropipette Techniques. J. Colloid
Interface Sci. 2005, 284, 176-183.
6 Yang, X.; Hamza, H.; Czarnecki, J. Investigation of Subfractions of Athabasca Asphaltenes
and Their Role in Emulsion Stability. Energy Fuels 2004, 18, 770-777.
7 Wu, X. Investigating the Stability Mechanism of Water-in-Diluted Bitumen Emulsions
through Isolation and Characterization of the Stabilizing Materials at the Interface. Energy Fuels
2003, 17, 179-190.
8 Gelin, F.; Grutters, M.; Cornelisse, P.; Taylor, S. Asphaltene Precipitation from Live Oil
Containing Emulsified Water. Proceedings of the 5th
International Conference on Petroleum
Phase Behaviour and Fouling, Banff, Alberta, Canada, 2004.
9 Horváth-Szabó, G.; Czarnecki, J.; Masliyah, J. H. Sandwich Structures at Oil-Water Interfaces
under Alkaline Conditions. J. Colloid Interface Sci. 2002, 253, 427-434.
45
10 Yang, X.; Czarnecki, J. The Effect of Naphtha to Bitumen Ratio on Properties of Water in
Diluted Bitumen Emulsions. Colloids Surf., A 2002, 211, 213-222.
11 Häger, M.; Ese, M.-H.; Sjöblom, J. Emulsion Inversion in an Oil-Surfactant-Water System
Based on Model Naphthenic Acids under Alkaline Conditions. J. Dispersion Sci. Technol. 2005,
26, 673-682.
12 Akbarzadeh, K.; Alboudwarej, H.; Svrcek, W.Y.; Yarranton, H.W. A Generalized Regular
Solution Model for Asphaltene Precipitation from n-Alkane Diluted Heavy Oils and Bitumens.
Fluid Phase Equilib. 2005, 232, 159-170.
13 Allen, E.W. Process Water Treatment in Canada’s Oil Sands Industry: I. Target Pollutants and
Treatment Objectives. Journal of Environmental Engineering and Science 2008, 7, 123-138.
14 Varadaraj, R.; Brons, C. Molecular Origins of Crude Oil Interfacial Activity Part 3:
Characterization of the Complex Fluid Rag Layers Formed at Crude Oil-Water Interfaces.
Energy Fuels 2007, 21, 1617-1621.
15 Scion Corporation. Scion Imaging Software. Last Updated: December, 2007.
16 Leung, W. Separation of Dispersed Suspension in Rotating Test Tube. Sep. Purif. Technol.
2004, 38, 99-119.
46
17 Klasson, K.T.; Taylor, P.A.; Walker Jr., J.F.; Jones, S.A.; Cummins, R.L.; Richardson, S.A.
Investigation of a Centrifugal Separator for In-Well Oil Water Separation. Pet. Sci. Technol.
2004, 22, 1143-1159.
18 Spiecker, P.M.; Gawrys, K.L.; Trail, C.B.; Kilpatrick, P.K. Effects of Petroleum Resins on
Asphaltene Aggregation and Water-in-Oil Emulsion Formation. Colloids Surf., A 2003, 220, 9-
27.
19 Barré, L.; Simon, S.; Palermo, T. Solution Properties of Asphaltenes. Langmuir 2008, 24,
3709-3717.
20 Gawrys, K.L.; Spiecker, P.M.; Kilpatrick, P.K. The Role of Asphaltene Solubility and
Chemistry on Asphaltene Aggregation. ACS Div. Pet Chem. Preprints 2002, 47, 332-335.
21 Sztukowski, D.M.; Yarranton, H.W. Characterization and Interfacial Behavior of Oil Sands
Solids Implicated in Emulsion Stability. J. Dispersion Sci. Technol. 2004, 25, 299-310.
22 Moran, K.; Czarnecki, J. Competitive Adsorption of Sodium Naphthenates and Naturally
Occurring Species at Water-in-Crude Oil Emulsion Droplet Surfaces. Colloids Surf., A 2007,
292, 87-98.
23 Tan, X.; Fenniri, H.; Gray, M.R. Investigation of the Effects of Water on Aggregation of
Model Asphaltenes in Organic Solution. Proceedings of the 9th
Annual International Conference
on Petroleum Phase Behaviour and Fouling, Victoria, British Columbia, Canada, 2008.
47
24 Johansen, E.J.; Skjärvö, I.M.; Lund, T.; Sjöblom, J.; Söderlund, H.; Boström, G. Water-in-
Crude Oil Emulsions from the Norwegian Continental Shelf Part I. Formation, Characterization,
and Stability Correlations. Colloids Surf. 1988, 34, 353-370.
25 Walstra, P. Principles of Emulsion Formation. Chem. Eng. Sci. 1993, 48, 333-349.
26 Kocherginsky, N.M.; Tan, C.L.; Lu, W.F. Demulsification of Water-in-Oil Emulsions via
Filtration through a Hydrophilic Polymer Membrane. J. Membr. Sci. 2003, 220, 117-128.
27 Jeribi, M.; Almir-Assad, B.; Langevin, D.; Hénaut, I.; Argillier, J.F. Adsorption Kinetics of
Asphaltenes at Liquid Interfaces. J. Colloid Interface Sci. 2002, 256, 268-272.
28 Gafonova, O.; Yarranton, H. The Stabilization of Water-in-Hydrocarbon Emulsions by
Asphaltenes and Resins. J. Colloid Interface Sci. 2001, 241, 469-478.
29 Rosen, M.J. Surfactants and Interfacial Phenomena, 3
rd ed.; John Wiley & Sons, Inc.: New
Jersey, 2004.
30 Liu, J.; Zhang, L.; Xu, Z.; Masliyah, J. Colloidal Interactions between Asphaltene Surfaces in
Aqueous Solutions. Langmuir 2006, 22, 1485-1492.
31 Nour, A.H.; Suliman, A.; Hadow, M.M. Stabilization Mechanisms of Water-in-Crude Oil
Emulsions. J. App. Sci. 2008, 8, 1571-1575.
32 Rodríguez-Abreu, C.; Lazzari, M. Emulsions with Structured Continuous Phases. Curr. Opin.
Colloid Interface Sci. 2008, 13, 198-205.
48
33 McLean, J.D.; Kilpatrick, P.K. Effects of Asphaltene Solvency on Stability of Water-in-Crude
Oil Emulsions. J. Colloid Interface Sci. 1997, 189, 242-253.
34 Norgård, E.L.; Sjöblom, J. Model Compounds for Asphaltenes and C80 Isoprenoid Tetraacids.
Part I: Synthesis and Interfacial Activities. J. Dispersion Sci. Technol. 2008, 29, 1114-1122.
35 Acevedo, S.; Escobar, G.; Ranaudo, M.A.; Khazen, J.; Borges, B.; Pereira, J.C.; Méndez, B.
Isolation and Characterization of Low and High Molecular Weight Acidic Compounds from
Cerro Negro Extraheavy Crude Oil. Role of These Acids in the Interfacial Properties of the
Crude Oil Emulsions. Energy Fuels 1999, 13, 333-335.
36 Acosta, E.J.; Harwell, J.H.; Sabatini, D.A. Self-Assembly in Linker-Modified
Microemulsions. J. Colloid Interface Sci. 2004, 274, 652-664.
37 Victorov, A.I.; Smirnova, N.A. Thermodynamic Model of Petroleum Fluids Containing
Polydisperse Asphaltene Aggregates. Ind. Eng. Chem. Res. 1998, 37, 3242-3251.
49
CHAPTER 3:
IMPACT OF ASPHALTENES AND NAPHTHENIC
AMPHIPHILES ON THE PHASE BEHAVIOR OF SOLVENT-
BITUMEN-WATER SYSTEMS
This chapter is derived from the following published manuscript:
Kiran, S.K.; Ng, S.; Acosta, E.J. Impact of Asphaltenes and Naphthenic Amphiphiles on the
Phase Behavior of Solvent-Bitumen-Water Systems. Energy Fuels 2011, 25, 2223-2231.
50
3.1 ABSTRACT
The impact of asphaltene partitioning on oil-water phase separation was previously
evaluated as a function of solvent-bitumen-water ratios, solvent aromaticity, and temperature in
Chapter 2. In this chapter, the added effect of naphthenic amphiphiles at concentrations of 3
wt% and 10 wt% was assessed. The observed phase behavior of the resulting rag layers was
discussed in view of interfacial co-adsorption mechanisms proposed in the literature. A major
finding was that, under alkaline process conditions, a shift in the rag layer morphology from
water-in-oil (w/o) to oil-in-water (o/w) at increased sodium naphthenate (NaN) concentrations
limited oil-water phase separation as a result of an increase in the surface area to volume ratio of
emulsion droplets and interfacial asphaltene partitioning. Contrary to NaN-free systems, it was
also observed that both temperature and solvent aromaticity had a minimal effect on the phase
behavior of NaN systems. Furthermore, naphthenic acids (NAs) were capable of promoting the
separation of w/o rag layers under acidic formulation conditions.
3.2 INTRODUCTION
A detailed overview of the recent advances in understanding the individual role of
asphaltenes and naphthenic amphiphiles on the formation and stability of water-in-oil (w/o) and
oil-in-water (o/w) rag layers has been provided in Chapters 1 and 2. Their synergistic behavior,
however, still remains relatively unexplored. Insight into this matter for mixtures of asphaltenes
and sodium naphthenates (NaNs) was offered by Wu and Czarnecki using a thermodynamic
modeling approach1. These researchers proposed a bilayer structure to describe the competitive
adsorption of asphaltenes and NaNs at the oil-water interface. In this hypothesized structure,
NaNs occupy the primary adsorbed layer and therefore act to sufficiently reduce the interfacial
51
tension (γow) and promote an o/w rag layer morphology. The makeup of the secondary, or
“floating”, layer is predominantly asphaltenes. Because of the minimal interaction of this layer
with the oil-water interface, it mainly serves to enhance rag layer stability. Elements of this
interfacial model were justified experimentally in a follow-up study by Moran and Czarnecki2.
By comparing the γow isotherms of an aqueous solution of NaNs with a highly diluted bitumen
sample and synthetic solvent (heptol), they observed that NaNs completely displace asphaltenes
from direct oil-water interfacial adsorption at a concentration of 0.1 wt%. Furthermore, using
droplet interaction experiments, these researchers showed that emulsion droplets prepared using
diluted bitumen, instead of heptol, exhibit a more rigid interface because they are able to
withstand coalescence over prolonged contact periods. The nature of asphaltene and naphthenic
acid (NA) films is less well-defined. Upon analyzing their molecular adsorption characteristics,
Varadaraj and Brons concluded that these components likely adsorb at the oil-water interface as
either mixed aggregates or mixed monolayers3. The impact of the resulting surfactant mixture
on the stability of w/o emulsion droplets was assessed indirectly by Poteau et al. via coalescence
studies involving the addition of maltenes (containing NAs) to diluted asphaltene solutions4.
These authors observed that asphaltene and maltene mixtures considerably enhance emulsion
stability. In contrast to these indirect observations, Gao et al. suggested that NAs soften the oil-
water interface and promote emulsion coalescence5.
The aim of this chapter is to address how naphthenic amphiphiles impact the phase
behavior of solvent-bitumen-water rag layers under formulation conditions that are compatible
with bitumen extraction processes. It is hypothesized that the stability of these rag layers is
influenced by the presence of naphthenic amphiphiles when using formulation conditions that
promote their adsorption at the oil-water interface and that the nature of this influence may vary
52
depending on the interaction of the naphthenic amphiphiles with asphaltenes. To evaluate this
influence, oil-water phase separation, asphaltene partitioning, and rag layer properties will be
characterized as a function of the solvent-bitumen-water ratios, solvent aromaticity, pH, and
temperature at different naphthenic amphiphile concentrations. The resulting phase behaviors
will also be discussed in light of interfacial co-adsorption mechanisms currently available in the
literature.
3.3 MATERIALS AND METHODS
3.3.1 Materials
All materials were used as received: anhydrous toluene (product #244511, 99.8%) and
NAs (product #70340, technical-grade extract) were purchased from Sigma-Aldrich Corp.
(Oakville, ON, Canada), reagent grade heptane (product #5400-1-10) and hexane (product
#5500-1-10) were obtained from Caledon Laboratory Chemicals (Georgetown, ON, Canada),
NaNs (90%) were supplied by Eastman Kodak, HCl (6 N, product #CABDH3204-1) and NaOH
(10 N, product #CABDH3247-1) were acquired from VWR (Mississauga, ON, Canada), and
coker feed bitumen (16.3% saturates, 39.8% aromatics, 28.5% resins, and 14.7% asphaltenes
according to SARA analysis) was donated by Syncrude Canada Ltd. (Edmonton, AB, Canada)6.
A similar salt water solution as that prepared in Chapter 2 was used here.
3.3.2 Formulation Preparation
Homogeneous oil phases were prepared by mixing heptol 80/20 (80 vol% heptane and
20 vol% toluene) and heptol 50/50 (50 vol% heptane and 50 vol% toluene) together with
bitumen at the same mass ratios of 1 to 1.5, 1 to 1, 3 to 1, 4 to 1, and 10 to 1 and using the same
53
wrist-action shaking parameters described in Chapter 2. These oil phases were then added to
aqueous solutions consisting of 3 wt% and 10 wt% NaNs at mass ratios of 1 to 10, 1 to 3, 1 to 1,
and 3 to 1 in 15 mL flat-bottom glass centrifuge tubes. Using the previously established batch
emulsification-separation protocol, these formulations were mixed (150 W VWR analog vortex
mixer) at 3200 rpm for 2 minutes and then centrifuged (IEC clinical centrifuge) at 500 g for 1
minute at 25°C. The effect of temperature on oil-water phase separation was evaluated by
placing the above formulations in a hot water bath at 80°C prior to mixing and centrifuging. To
modify the formulation pH, 6 N HCl and 10 N NaOH were added dropwise to the aqueous
phase until the respective titration endpoints of pH 4 and pH 10 were detected using an Oakton
Benchtop pH/ion 510 meter. As a result of the precipitation of NaNs upon HCl addition, NAs
were instead pre-dissolved within the oil phase at concentrations of 3 wt% and 10 wt%.
3.3.3 Microscopy and Material Balances
Optical, cross-polarized, and fluorescent micrographs of the separated oil phase, aqueous
phase, and rag layer of all the formulations in Section 3.3.2 were taken according to the
procedure outlined in Chapter 2. Material balances were also similarly performed with the aid of
these micrographs.
3.3.4 Asphaltene Losses
The UV-vis spectroscopic methodology developed to track asphaltene losses to the rag
layer in Chapter 2 was employed here.
54
3.3.5 Interfacial Tension Measurements
The γow of NaN formulations, where γow<1 mN/m, was measured according to the
procedure for the spinning drop tensiometer manufactured by Temco Inc. (model #500) in
Chapter 2. The only difference in this application was that freshly prepared solutions of NaNs
and diluted bitumen were respectively used as the heavy (aqueous) and light (oil) phases
because of the poor phase separation results. A KSV Sigma 700 tensiometer equipped with a
platinum Du Noüy ring probe was alternatively used to measure the larger γow values (20-26
mN/m) of pH 4 systems. In this technique, the Du Noüy ring was initially immersed within 5
mL of a given oil phase that resided on top of 10 mL of acidified salt water. As the Du Noüy
ring was lowered through the oil-water interface, the resulting force exerted on it (F) was
calculated using the following relationship7:
pullogVF , (Eq. 1)
Here, Δρ is the difference in density between the heavy (water) and light (oil) phases, g
is the gravitational acceleration constant (9.81 m/s2), and Vo,pull is the volume of oil pulled
through the interface. The γow was subsequently determined as follows:
wire
ring
pullo
ring
ring
owr
r
V
rf
r
F,
4 ,
3
(Eq. 2)
Tabulated values of
wire
ring
pullo
ring
r
r
V
rf ,
,
3
, which is a dimensionless quantity that may be
expressed exclusively as a function of the probe’s ring (rring=9.545 mm) and wire (rwire=0.185
mm) radii as well as Vo,pull, are available throughout the literature8,9,10
. The Du Noüy ring was
rinsed with toluene, ethanol, and deionized water prior to reuse. Due to the large volumes of the
55
separated aqueous and oil phases required for this methodology, the effect of water to oil ratios
on γow could not be assessed in situ.
3.3.6 Surface Pressure-Area Isotherms
The effect of NAs on the collapse pressure and elasticity (ε) of asphaltene skins was
tested using a KSV Minitrough operated on a vibration-free table. Initially, asphaltenes were
precipitated from bitumen via hexane dilution at ratios greater than 40 to 1. Recovered
asphaltenes were next rinsed with additional quantities of hexane in order to minimize maltene
contamination11
. Surfactant mixtures of 100% asphaltenes, 75% asphaltenes and 25% NAs, 50%
asphaltenes and 50% NAs, 25% asphaltenes and 75% NAs, and 100% NAs were subsequently
diluted with toluene to a concentration of 0.1%. A volume of 45 µL of each of these mixed
surfactant solutions was then spread onto a subphase composed of pure deionized water with a
surface tension comparable to that of the salt water solution (~71 mN/m). After waiting 10
minutes to allow for solvent evaporation, the area of the spreading phase (Asp) was compressed
symmetrically at a constant rate of 8 mm/minute from 256 cm2 to 23 cm
2 using a pair of
interlinked surface barriers. The change in surface pressure (πp) during compression was
measured using a Wilhelmy plate as follows12
:
op (Eq. 3)
In this equation, σo and σ represent the respective surface tensions in the absence and
presence of surface-active molecules. The collapse pressure of mixed asphaltene and NA films
was interpreted from the resulting πp-Asp isotherms as the maximum attainable πp. Furthermore,
their ε, which is a measure of their resistance against compression, was calculated as follows13
:
56
sp
p
Aln
(Eq. 4)
Each compression test was followed by a cleaning cycle in which all of the
instrumentation was thoroughly rinsed with ethanol and deionized water. The cleanliness of the
subphase was verified by ensuring that πp<0.3 mN/m prior to depositing the spreading phase. In
addition, it was verified by spreading toluene alone onto pure deionized water that the solvent
had a negligible impact on πp. Although the πp-Asp isotherms generated in this study were not a
true reflection of those attainable at the oil-water interface, they provided an accurate depiction
of the trends in changes of the surfactant film stability for controlled asphaltene and NA
mixtures. This point was illustrated in an earlier study by Zhang et al. where similarities in the
trends of πp and interfacial pressure isotherms for asphaltene and demulsifier mixtures were
observed12
.
3.4 RESULTS
3.4.1 Phase Behavior of Naphthenic Amphiphile Systems
The phase behavior results presented in Figures 3.1 (a)-(f) for solvent-bitumen-water
systems composed of 3 wt% NaNs at pH 7.5 are overlaid on top of those for the baseline
systems at 0 wt% NaNs and 9.1 wt% and 50 wt% water taken from Chapter 2.
57
0
10
20
30
40
0 2 4 6 8 10
Asp
halt
en
es L
osses t
o R
ag
Layer
(%)
Heptol 80/20 to Bitumen Dilution Ratio
0
20
40
60
80
100
0 2 4 6 8 10
Oil
Lo
sses t
o R
ag
Layer
(Vo
l %
)
0
20
40
60
80
100
0 2 4 6 8 10
75 wt% Water (3 wt% NaNs) 50 wt% Water (3 wt% NaNs) 25 wt% Water (3 wt% NaNs)
9.1 wt% Water (3 wt% NaNs) 50 wt% Water (Baseline) 9.1 wt% Water (Baseline)
0
10
20
30
40
0 2 4 6 8 10
Heptol 50/50 to Bitumen Dilution Ratio
0
10
20
30
40
0 2 4 6 8 10
0
20
40
60
80
100
0 2 4 6 8 10
(a) (b)
(d)
(f)
(c)
(e)
Figure 3.1: Oil and asphaltene losses to the rag layer for 0 wt% (baseline) and 3 wt% NaN
systems prepared at pH 7.5 with (a and b) heptol 80/20 at 25°C, (c and d) heptol 80/20 at 80°C,
and (e and f) heptol 50/50 at 25°C.
For systems prepared with heptol 80/20 at 25°C (Figures 3.1 (a)), oil losses to the rag
layer are worsened at increased water contents. At a water content of 75 wt%, the entire oil
phase is emulsified within the rag layer. For systems containing ≤50 wt% water, reducing the
solvent to bitumen dilution ratio significantly increases the oil losses to the rag layer. Despite
58
observing similar trends in oil-water phase separation at 80°C (Figure 3.1 (c)) and when using
heptol 50/50 as the solvent (Figure 3.1 (e)), complete emulsification of the oil phase within the
rag layer is observed at a water content ≥50 wt%. As illustrated in Figure 3.2, acidifying
solvent-bitumen-water systems to pH 4 significantly improves oil recovery.
0
10
20
30
40
0 2 4 6 8 10
Oil
Lo
ss
es
to
Ra
g L
aye
r (V
ol %
)
Heptol 80/20 to Bitumen Dilution Ratio
75 wt% Water (3 wt% NAs)
50 wt% Water (3 wt% NAs)
25 wt% Water (3 wt% NAs)
9.1 wt% Water (3 wt% NAs)
50 wt% Water (Baseline)
9.1 wt% Water (Baseline)
Figure 3.2: Oil losses to the rag layer for 0 wt% (baseline) and 3 wt% NA systems as a function
of the heptol 80/20 to bitumen dilution ratio and water content. All systems are evaluated at pH
4 and 25°C.
With regards to the partitioning behavior of asphaltenes, Figures 3.1 (b) and (d) show
that an increase in the heptol 80/20 to bitumen dilution ratio promotes an increase in the
asphaltene losses to the rag layer. Whereas asphaltene losses are independent of temperature,
they are notably lower for heptol 50/50 systems (Figure 3.1 (f)) and decrease with increased
solvent to bitumen dilution ratios. In all cases, the presence of 3 wt% NaNs induces an increase
in asphaltene losses relative to the baseline formulations. Asphaltene losses are not evaluated for
systems at pH 4. Here, the presence of NAs changed the visible absorbance spectrum of diluted
59
bitumen. A similar shift observed by Östlund et al. in the near-IR spectrum of bitumen and NA
mixtures supports the idea of asphaltene and NA interactions14
.
3.4.2 Transitions to the Rag Layer Morphology
Changes to the rag layer morphology of solvent-bitumen-water systems produced upon
increasing the naphthenic amphiphile concentration from 0 wt% to 10 wt% are illustrated in
Figures 3.3 (a)-(c).
3 wt% NaNs 10 wt% NaNs
0 wt% NAs
(a)
Multiple Emulsions
0 wt% NaNs
250 µm
3 wt% NAs 10 wt% NAs(b)
10 wt% NAs3 wt% NAs0 wt% NAs(c)
Figure 3.3: Fluorescent micrographs of the effect of (a) NaNs (pH 7.5) and (b) NAs (pH 4) on
the morphology of heptol 80/20-bitumen-water rag layers. (c) Cross-polarized images of rag
layers containing NAs at pH 4.
For all NaN systems at pH ≥7.5, an increase in the surfactant concentration results in a
transition of the rag layer from w/o to o/w. This transition is accompanied by a major decrease
in the droplet size from 0 wt% to 3 wt% NaNs, whereas such changes are less dramatic from 3
60
wt% to 10 wt% NaNs. At pH 4, where NAs are dominant, a w/o rag layer is continuously
observed despite an increase in the surfactant concentration. Traces of multiple emulsions also
become evident. Of special interest for systems prepared at pH 4 is the increased observance of
liquid crystals at larger NA concentrations. These phases, which appear as bright spots in Figure
3.3 (c), do not form continuous films adsorbed at the oil-water interface as has been suggested
by other researchers15
. Instead, they appear as aggregates dispersed throughout the oil phase.
Differences in the resulting liquid crystal structures may be attributed to variations in the
emulsification protocol.
3.4.3 Interfacial Tension Isotherms
Baseline γow isotherms as well as those obtained for naphthenic amphiphile systems are
presented in Figures 3.4 (a) and (b).
0
10
20
30
40
0 2 4 6 8 10
γo
w(m
N/m
)
Heptol 80/20 to Bitumen Dilution Ratio
3 wt% NaN/NA 10 wt% NaN/NA 50 wt% Water (Baseline)
9.1 wt% Water (Baseline) pH 4 (Baseline)
0
10
20
30
40
0 2 4 6 8 10
(a) (b)
Figure 3.4: Baseline γow isotherms as well as those for (a) NaN systems at pH 7.5 and (b) NA
systems at pH 4 as a function of the heptol 80/20 to bitumen dilution ratio. The temperature is
maintained at 25°C.
61
At increased heptol 80/20 to bitumen dilution ratios, it is observed that NaNs
significantly reduce γow from 5-10 mN/m to 0.5-0.9 mN/m. Introducing NAs into similar
formulations at pH 4 results in an increase in γow from ~20-22 mN/m to ~23-26 mN/m. In both
of the above scenarios, increasing the naphthenic amphiphile concentration from 3 wt% to 10
wt% results in negligible changes to γow. Furthermore, varying the formulation temperature and
solvent aromaticity has little influence on all of the above isotherms. Equilibrium γow values are
obtained almost instantaneously in all of the above systems (on the order of seconds). This
finding is in agreement with that of Moran and Czarnecki who suggested that all dynamic
behavior is lost at such large asphaltene and naphthenic amphiphile concentrations because of
their relatively fast adsorption kinetics and high interfacial packing2.
3.4.4 Impact of Naphthenic Acids on Asphaltene Film Properties
The effect of NAs on the collapse pressure and ε of asphaltene skins may be interpreted
from the πp-Asp isotherms illustrated in Figure 3.5.
0
15
30
45
60
75
0 1 2 3 4 5 6
100% A
75% A-25% NAs
25% A-75% NAs
100% NAs
ln (Asp (cm2))
πp
(mN
/m)
50% A-50% NAs
Figure 3.5: πp-Asp isotherms of asphaltene (A) and NA surfactant mixtures.
62
According to these results, pure asphaltenes produce more stable films than pure NAs.
This is indicated by their larger collapse pressure. Mixtures of these components show an
intermediate behavior where the film stability is reduced at increased NA concentrations. As
shown in Table 3.1, such mixtures are a good representation of the spread in the relative bulk
phase asphaltene and NA compositions tested.
Table 3.1: Relative asphaltene and NA compositions in formulations tested.
Heptol 80/20 to Bitumen 3 wt% NAs 10 wt% NAs
% Asphaltenes % NAs % Asphaltenes % NAs
1 to 1.5 78 22 52 48
1 to 1 75 25 47 53
3 to 1 60 40 31 69
4 to 1 55 45 26 74
10 to 1 35 65 14 86
Values of ε for produced asphaltene and NA films are calculated at πp values ranging
from 0 mN/m to 10 mN/m as it is the common linear regime amongst all generated πp-Asp
isotherms. The results presented in Table 3.2 suggest that all such films are prone to
deformation. It is interesting to note that the ε of mixed asphaltene and NA films in the NA-rich
domain is lower than that of pure NAs.
Table 3.2: Measurements of ε for mixed asphaltene and NA films.
System ε (mN/m)
100% Asphaltenes 73
75% Asphaltenes and 25% NAs 34
50% Asphaltenes and 50% NAs 16
25% Asphaltenes and 75% NAs 16
100% NAs 23
The πp-Asp isotherms for NaN systems are also conducted by first spreading 45 µL of a
0.1% asphaltene solution onto deionized water. A concentrated NaN solution is then infused
within the subphase such that its final concentrations tested are 0.1%, 1%, and 3%. The resulting
63
measured collapse pressures are 25 mN/m, 9 mN/m, and 6 mN/m respectively. Although this
data illustrates the ability of NaNs to significantly weaken asphaltene films, it cannot be
extrapolated to phase behavior studies because a liquid-liquid trough is required to permit for
the formation of a secondary asphaltene layer on top of the primary adsorbed NaN layer. Gao et
al. successfully implemented the above recommendation for interfacial films composed of
asphaltenes and NaNs in a 1 to 1 volume ratio5. The resulting πp-Asp isotherm of the bilayer
structure showed an intermediate behavior compared to pure asphaltenes and pure NaNs with a
collapse pressure >30 mN/m.
3.5 DISCUSSIONS
3.5.1 Interfacial Co-Adsorption of Asphaltenes and Sodium Naphthenates
In a comparison of the asphaltene-controlled (baseline) and NaN-controlled phase
behavior results in Figures 3.1 (a)-(f), trends depicting increased oil losses to the rag layer at
increased water to oil ratios are maintained in addition to the partitioning behavior of
asphaltenes. Of special interest, however, is the increased magnitude of oil losses observed in
NaN systems. To understand this behavior, the effect of NaN concentration on emulsification
must first be evaluated. The first step in establishing this link is to discuss the relationship
between the γow and average emulsion droplet diameter ( E
dd )16
:
ow
E
dd (Eq. 5)
In this equation, α is 1 for laminar flow and 0.6 for turbulent flow. According to this
relationship, any reduction in γow produces a reduction in the drop size. The change in E
dd also
changes the surface area ( E
dA ) to volume ( E
dV ) ratio of emulsion droplets as follows:
64
E
d
E
d
E
d
dV
A 6 (Eq. 6)
From the above equations, it is apparent that γow is inversely related to the E
dA to E
dV
ratio of a given emulsion droplet. Figure 3.6 illustrates measured changes in γow for a given
diluted bitumen oil phase as a function of the added NaN concentration to the aqueous phase.
0
1
2
3
4
5
6
7
0 1 2 3NaN Concentration (wt%)
y1 = -6.20x1 + 7.38
y2 = -0.32x2 + 1.68
CMCNaN
γo
w(m
N/m
)
Figure 3.6: γow of bitumen diluted with heptol 80/20 versus the added NaN concentration to the
aqueous phase at pH 7.5 and 25°C. The included fluorescent micrographs show a transition in
the rag layer morphology from w/o to o/w at the CMC of NaNs (~1 wt%).
According to this data, γow decreases linearly up to a NaN concentration of 1 wt%
(Δγow/ΔNaN~-6.2 (mN/m)/wt% NaNs). By holding all parameters constant in Equation 5 other
than γow, Equation 6 reveals a potential increase in the E
dA to E
dV ratio of emulsion droplets by a
factor of 3 upon increasing the NaN concentration from 0 wt% to 1 wt%. Emulsion stabilization
is facilitated at such large oil-water interfacial areas (Aow) as the potential for asphaltene
adsorption is enhanced. Figure 3.1 (b) shows the increase in asphaltene losses to the rag layer.
65
At NaN concentrations >1 wt%, changes to the E
dA to E
dV ratio of emulsion droplets are less
pronounced (Δγow/ΔNaN~-0.3 (mN/m)/wt% NaNs). Furthermore, it is here where the dominant
morphology of the emulsion switches from w/o to o/w. This transition coincides with the fact
that the critical micelle concentration (CMC) of NaNs is 1 wt%. A similar CMC value was
previously reported by Moran and Czarnecki2. Beyond this concentration, the spontaneous
increase in the total number of dispersed droplets further increases the overall Aow and
asphaltene losses to the rag layer. Under interfacial saturation conditions, which occurs at NaN
concentrations >1 wt%, the bilayer model proposed by Wu and Czarnecki is believed to
uphold1. Here, asphaltene skins must adsorb as a secondary layer at the oil-water interface
because NaNs predominantly occupy the primary adsorbed layer. A modified schematic of this
model is provided in Figure 3. 7 (a).
(a)
WaterNaNs
Asphaltenes Oil
i) Mixed Monolayer ii) Mixed Aggregate
NAsAsphaltenes
Oil
Water
Mixed
aggregate
(b)
Figure 3.7: (a) Bilayer model proposed by Wu and Czarnecki for the interfacial co-adsorption
of asphaltenes and NaNs at the oil-water interface1. (b) Co-adsorption mechanisms proposed by
Varadaraj and Brons for asphaltenes and NAs at the oil-water interface include (i) mixed
monolayers and (ii) mixed aggregates3.
66
Of the mechanisms available for increasing Aow, an increase in the E
dA to E
dV ratio of
emulsion droplets is the primary factor leading to larger oil losses to the rag layer. This is
supported by the data in Figure 3.1 (a) for systems prepared with 0 wt% and 3 wt% NaNs.
Contributions from spontaneous emulsification are less significant because changes in oil losses
to the rag layer for systems prepared with 3 wt% and 10 wt% NaNs are marginal. It should be
noted that Δγow/ΔNaN in Figure 3.6 below the CMC of NaNs is impacted significantly by
formulation conditions. This is concluded from Figure 3.4 (a) for systems prepared with 0 wt%
NaNs where γow is observed to vary according to changes in the heptol 80/20 to bitumen dilution
ratio and water content as a result of modifications to the asphaltene partitioning within the rag
layer. Also depicted in Figure 3.4 (a) is that the impact of the above variables on γow at NaN
concentrations >1 wt% is less prominent.
The decrease in oil losses to the rag layer at the large bitumen dilution ratios described in
Figure 3.1 (a) for 3 wt% NaN systems at low water contents opposes the theoretical principles
relating asphaltene losses to emulsion stability for the NaN-free systems in Chapter 2. In the
presence of NaNs, however, the ratio of asphaltenes to NaNs decreases with an increase in the
dilution ratio, thus producing thinner, or “softer”, asphaltene skins. Emulsion coalescence
studies conducted by Gao et al. support this conclusion5. These researchers showed that a
critical asphaltene to NaN ratio exists below which asphaltene skins can no longer mask the
softening effect of NaNs and emulsion destabilization is promoted.
67
3.5.2 Effect of Temperature and Solvent Aromaticity on Oil Recovery from Rag
Layers
A more realistic depiction of the phase behavior of crude oil formulations that is in line
with actual processing conditions is to evaluate oil recovery from rag layers at 80°C. As was
previously outlined for baseline systems, increasing the temperature from 25°C to 80°C helps to
reduce oil losses to the rag layer from a maximum of 30 vol% to 10 vol% despite having a
negligible influence on the asphaltene partitioning characteristics. This effect is a direct
consequence of the rag layer being composed of water droplets dispersed throughout a
continuous oil phase. The reduced viscosity of the continuous oil phase at elevated temperatures
facilitates its drainage and hence overall recovery. For 3 wt% (and 10 wt%) NaN systems,
increasing the temperature from 25°C to 80°C is of negligible benefit to oil-water phase
separation because the γow isotherm presented in Figure 3.4 (a) remains unchanged. This
observation is supported by Acosta et al. who found that the temperature has little influence on
the interfacial activity of ionic surfactants17
. As a result, the hydrophilic nature of NaNs
continues to induce a transition in the rag layer morphology from w/o to o/w and therefore the
drainage of the aqueous phase is instead facilitated. It should be emphasized for NaN
formulations that asphaltene losses to the rag layer remain independent of the temperature.
The effect of solvent aromaticity on rag layer stability is tested by decreasing heptol’s
heptane to toluene ratio from 80/20 to 50/50. To understand the effect of such a change on the
observed phase behavior of baseline systems, the concept of critical transition concentration
(CTC) in Chapter 2 should be reviewed. In short, the CTC refers to the solvent to bitumen
dilution ratio below which the surface activity of asphaltene aggregates may be associated with
an increased tendency to stabilize rag layers. From γow measurements, the CTC of heptol 80/20
68
and heptol 50/50 systems is observed to correspond respectively to solvent to bitumen dilution
ratios of 10 and 2-3. In the presence of 3 wt% (and 10 wt%) NaNs, the effect of solvent
aromaticity becomes less relevant. As illustrated in Figures 3.1 (a) and (e) for the solvents
heptol 80/20 and heptol 50/50, respectively, oil losses to the rag layer are quite similar. This is a
result of emulsification being governed by NaNs, which are water-soluble molecules whose
surface activity is independent of the solvent type. It is surprising that, despite the reduced
surface activity of asphaltenes in heptol 50/50 systems (Figure 3.1 (f)), sufficient surface
coverage is still achieved to promote emulsion stability. The interfacial co-adsorption model
proposed by Wu and Czarnecki is a useful tool to understand this phenomenon1. These authors
speculated that the secondary adsorbed asphaltene layer is predominantly anchored into place
via polar point contacts with the oil-water interface instead of cross-linking with the primary
adsorbed NaN layer. Therefore, the smaller-sized asphaltene aggregates adsorb more efficiently
at the secondary layer of the interface. Such efficient adsorption promotes larger oil losses to the
rag layer for systems prepared with an aqueous phase content of 50 wt%.
3.5.3 Effect of pH on Oil Recovery from Rag Layers
As previously reported in Chapter 1, the pKa of naphthenic amphiphiles is ~6.
Increasing the pH of solvent-bitumen-water formulations containing 3 wt% NaNs from pH 7.5
to pH 10 is therefore expected to have no substantial impact on the observed phase behavior
because the ionized surfactant already exists in its dissociated state. Although the results at pH
10 are not presented, this hypothesis can indeed be experimentally validated using the
procedures outlined in Section 3.3.
69
As illustrated in Figure 3.2, reducing the pH of baseline solvent-bitumen-water
formulations results in improved oil-water phase separation. This behavior is unexpected
because asphaltenes should show an increased surface activity under such conditions as a result
of the protonation of their basic function groups, such as amines18
. Because of similarities in the
γow isotherms (Figure 3.4 (b)) and oil losses to the rag layer (Figure 3.2) for 0 wt% and 3 wt%
NA systems at pH 4, it is suspected that a considerable fraction of endogenous NAs remain in
the coker feed bitumen that, at low pH, are less active at the oil-water interface, promoting
higher γow and improved oil-water phase separation. This theory may also explain why lower γow
values are observed for solvent-bitumen-water systems under neutral conditions compared to
other values published in the literature2,5
. Although it cannot be confirmed from the air-liquid
πp-Asp isotherms presented in Figure 3.5, it is likely that NAs help to destabilize emulsion
droplets by weakening the asphaltene films adsorbed at the oil-water interface. The
experimental observations recently published by Gao et al. hint at a similar softening effect5.
Conflicting results obtained by Poteau et al. are likely a result of constituents other than NAs
present within the maltene solution added to the oil phase4. The possible mechanisms
highlighted by Varadaraj and Brons to describe the co-adsorption of asphaltenes and NAs at the
oil-water interface are provided in Figure 3.7 (b).
3.6 CONCLUSIONS
The results and ensuing discussions revealed that, consistent with the initial hypothesis,
the presence of naphthenic amphiphiles influenced the separation of solvent-bitumen-water rag
layers in formulations that promoted the adsorption of these species. Formulations with high
water content and low interfacial tensions (γow) produced smaller droplet sizes and increased oil-
water interfacial areas during emulsification, which magnified the effect of naphthenic
70
amphiphiles. For sodium naphthenates (NaNs), stable oil-in-water rag layers were produced in
formulations with high asphaltene and NaN contents (i.e. high bitumen and water contents). The
increased asphaltene losses in the presence of NaNs suggested that NaNs improved the
segregation of asphaltenes at the oil-water interface. Although indirect evidence suggested that
NaNs produced softer films, this apparent softening effect did not compensate for the decreased
γow and droplet size. In acidic environments, undissociated naphthenic acids (NAs) led to higher
γow that facilitated the separation of water-in-oil rag layers. Once again, indirect evidence at the
air-liquid interface suggested that NAs softened asphaltene films. This observation was
consistent with the improved separation obtained in NA-containing systems at pH 4 compared
with baseline systems at pH 7.5. Interfacial co-adsorption mechanisms proposed in the literature
were compatible with the results highlighted above. Although results obtained under acidic
conditions showed improved oil recovery, further studies are required to assess how NAs
modify the properties of asphaltene films adsorbed at the oil-water interface.
3.7 REFERENCES
1 Wu, X.A.; Czarnecki, J. Modeling of Diluted Bitumen-Water Interfacial Compositions using a
Thermodynamic Approach. Energy Fuels 2005, 19, 1353-1359.
2 Moran, K.; Czarnecki, J. Competitive Adsorption of Sodium Naphthenates and Naturally
Occurring Species at Water-in-Crude Oil Emulsion Droplet Surfaces. Colloids Surf., A 2007,
292, 87-98.
71
3 Varadaraj, R.; Brons, C. Molecular Origins of Heavy Crude Oil Interfacial Activity. Part 2:
Fundamental Interfacial Properties of Model Naphthenic Acids and Naphthenic Acids Separated
from Heavy Crude Oils. Energy Fuels 2007, 21, 199-204.
4 Poteau, S.; Argillier, J.-F.; Langevin, D.; Pincet, F.; Perez, E. Influence of pH on Stability and
Dynamic Properties of Asphaltenes and Other Amphiphilic Molecules at the Oil-Water
Interface. Energy Fuels 2005, 19, 1337-1341.
5 Gao, S.; Moran, K.; Xu, Z.; Masliyah, J. Role of Naphthenic Acids in Stabilizing Water-in-
Diluted Model Oil Emulsions. J. Phys. Chem. B 2010, 114, 7710-7718.
6 Akbarzadeh, K.; Alboudwarej, H.; Svrcek, W.Y.; Yarranton, H.W. A Generalized Regular
Solution Model for Asphaltene Precipitation from n-Alkane Diluted Heavy Oils and Bitumens.
Fluid Phase Equilib. 2005, 232, 159-170.
7 Huh, C.; Mason, S.G. A Rigorous Theory of Ring Tensiometry. Colloid Polym Sci. 1975, 253,
566-580.
8 Harkins, W.D.; Jordan, H.F. A Method for the Determination of Surface and Interfacial
Tension from the Maximum Pull on a Ring. J. Am. Chem. Soc. 1930, 52, 1751-1772.
9 Zuidema, H.H.; Waters, G.W. Ring Method for the Determination of Interfacial Tension. Ind.
Eng. Chem. 1941, 13, 312-313.
72
10 Fox, H.W.; Chrisman Jr., C.H. The Ring Method of Measuring Surface Tension for Liquids
of High Density and Low Surface Tension. J. Phys. Chem. 1952, 56, 284-287.
11 Yang, X.; Hamza, H.; Czarnecki, J. Investigation of Subfractions of Athabasca Asphaltenes
and Their Role in Emulsion Stability. Energy Fuels 2004, 18, 770-777.
12 Zhang, L.Y.; Xu, Z.; Masliyah, J.H. Langmuir and Langmuir-Blodgett Films of Mixed
Asphaltene and a Demulsifier. Langmuir 2003, 19, 9730-9741.
13 Saad, S.M.I.; Policova, Z.; Acosta, E.J.; Hair, M.L.; Neumann, A.W. Mixed DPPC/DPPG
Monolayers at Very High Compression. Langmuir 2009, 25, 10907-10912.
14 Östlund, J.-A.; Nydén, M.; Auflem, I.-H.; Sjöblom, J. Interactions between Asphaltenes and
Naphthenic Acids. Energy Fuels 2003, 17, 113-119.
15 Horváth-Szabó, G.; Czarnecki, J.; Masliyah, J.H. Sandwich Structures at Oil-Water Interfaces
under Alkaline Conditions. J. Colloid Interface Sci. 2002, 253, 427-434.
16 Walstra, P. Principles of Emulsion Formation. Chem. Eng. Sci. 1993, 48, 333-349.
17 Acosta, E.J.; Yuan, J.S.; Bhakta, A.S. The Characteristic Curvature of Ionic Surfactants. J.
Surfactants Deterg. 2008, 11, 145-158.
18 Aguilera, B.M.; Delgado, J.G.; Cárdenas, A.L. Water-in-Oil Emulsions Stabilized by
Asphaltenes Obtained from Venezuelan Crude Oils. J. Dispersion Sci. Technol. 2010, 31, 359-
363.
73
CHAPTER 4:
EVALUATING THE HYDROPHILIC-LIPOPHILIC NATURE
OF ASPHALTENIC OILS AND NAPHTHENIC AMPHIPHILES
USING MICROEMULSION MODELS
This chapter is derived from the following published manuscript:
Kiran, S.K.; Acosta, E.J; Moran, K. Evaluating the Hydrophilic-Lipophilic Nature of
Asphaltenic Oils and Naphthenic Amphiphiles Using Microemulsion Models. J. Colloid
Interface Sci. 2009, 336, 304-313.
74
4.1 ABSTRACT
In this chapter, microemulsion (µE) phase behavior models were applied to quantify the
hydrophilic-lipophilic nature of asphaltenic oils (bitumen, deasphalted bitumen, asphalt, and
naphthalene) and surface-active asphaltene aggregates and naphthenic amphiphiles. For the test
oils, the equivalent alkane carbon number (EACN) was determined by evaluating the salinity
shifts of µEs formulated with a reference surfactant (sodium dihexyl sulfosuccinate (SDHS))
and a reference oil (toluene) at different volume fractions. Similarly, the characteristic curvature
(Cc) of test surfactants was determined by evaluating their salinity shifts in mixtures with SDHS
at different molar fractions. As a part of the oil phase, asphaltenes and asphaltene-like species
were highly hydrophilic. This led to low EACN values despite their large molecular weight. As
a surfactant, asphaltenes were hydrophobic species that led to the formation of water-in-oil
emulsions. Naphthenic amphiphiles, particularly sodium naphthenates, were on the other hand
highly hydrophilic compounds that led to the formation of oil-in-water emulsions. These
hydrophilic-lipophilic characterization parameters, and the methods used to determine them,
could potentially be used in the future to understand the phase behavior of complex oil-water
systems (such as rag layers).
4.2 INTRODUCTION
A common methodology for determining the hydrophilic-lipophilic nature of different
oils and surfactants is to analyze the impact of these compounds on the observed microemulsion
(µE) phase behavior. The advantage of using the µE phase behavior as a “hydrophilic-lipophilic
scale” stems from the fact that these are systems in thermodynamic equilibrium. Therefore, any
parameter obtained from these studies reflects the balance of surfactant, oil, and water
75
interactions1. As was described in Chapter 1, the three basic µE types are: oil-in-water (o/w)
µEs in equilibrium with an excess oil phase (Type I), bicontinuous µEs in equilibrium with
excess oil and aqueous phases (Type III), and water-in-oil (w/o) µEs in equilibrium with an
excess aqueous phase (Type II). For µEs formulated with an ionic surfactant, an increase in the
electrolyte concentration leads to a Type IType IIIType II µE phase behavior transition. In
other words, increasing the salinity favors the partitioning of the surfactant into the oil phase.
Along this transition, the interfacial tension (γow) of the system changes significantly, reaching
an ultralow value at Type III conditions where the net curvature of the surfactant at the oil-water
interface is 0 (see Figure 4.1)2. This specific Type III condition is referred to as the “optimum”
point where one also typically finds equal volumes of solubilized oil and water3,4,5
. The
electrolyte concentration needed to obtain a net 0 curvature is the optimal salinity (S*).
From the above discussion, one can extrapolate that a larger salt concentration is
required to produce a Type IType IIIType II µE phase behavior transition in systems
formulated with a more hydrophobic oil as it is more difficult for the surfactant to partition into
such an oil. Similarly, a larger salt concentration is required to produce a Type IType
IIIType II µE phase behavior transition in systems formulated with a more hydrophilic
surfactant as it is highly soluble in water and resists leaving the aqueous phase. In this chapter,
the plan is to use these principles to evaluate the hydrophilic-lipophilic nature of asphaltenic oils
(bitumen, deasphalted bitumen, asphalt, and naphthalene) and surface-active asphaltene
aggregates, naphthenic acids (NAs), and sodium naphthenates (NaNs).
Unfortunately, these oils and surfactants do not form µEs on their own. As a result, µE
formation is facilitated by mixing each test oil and surfactant with a reference phase. The
reference oil and anionic surfactant used in this study is toluene and sodium dihexyl
76
sulfosuccinate (SDHS) respectively. By determining the shift in S* as a function of the fraction
of the test oil or surfactant in the mixture, the relative hydrophobicity of the test oils and
surfactants will be determined.
The hydrophilic-lipophilic deviation (HLD) model is used in this study to quantify the
relative impact of the hydrophilic-lipophilic nature of the above specified test oils and
surfactants on the µE phase behavior. The HLD equation developed by Salager et al. for µEs
containing an ionic surfactant, or mixture of ionic surfactants, is as follows1,2,6,7,8
:
cToc CTaAfKNSHLD ,ln (Eq. 1)
In this equation, the natural logarithm ln(S) describes the effect of the aqueous phase salt
concentration (S, in g/100 mL) on the suppression of the ionic surfactant’s electrical double
layer. The next term KNc,o reflects the ability of the surfactant to induce a dipole-dipole
interaction with the oil phase. An average K value of 0.17 is typically applied to most
surfactant-oil combinations. On the other hand, Nc,o is an explicit measure of the oil phase
hydrophobicity. For basic alkanes, Nc,o is simply equal to the number of oil molecule carbon
atoms and is thus commonly referred to as the alkane carbon number (ACN). For more complex
oils, Nc,o, which needs to be solved for experimentally, is instead referred to as the equivalent
alkane carbon number (EACN). The additional function f(A) varies with the co-surfactant type
and concentration. In the event where no co-surfactant is added, f(A) is set to 0. Furthermore,
the term ΔT is the difference in temperature from 298 K. An associated pre-factor value of
aT=0.01 K-1
is commonly reported in the literature. The final characteristic curvature term, Cc, is
indicative of the hydrophilic-lipophilic nature of the surfactant of surfactant mixture.
77
The effect of varying a specific parameter (e.g. salinity) while keeping all others
constant in Equation 1 is explored with respect to the phase behavior of SDHS-oil (20 wt%
naphthalene and 80 wt% toluene)-water µEs in Figure 4.1.
γo
w (
mN
/m)
NaCl (g/100 mL)
Figure 4.1: The phase behavior and corresponding γow of SDHS-oil (20 wt% naphthalene and
80 wt% toluene)-water µEs as a function of the salinity.
According to this figure, a HLD<0HLD=0HLD>0 shift corresponds to a Type
IType IIIType II µE phase behavior transition. The point of optimum formulation is at
HLD=0.
Limited data is currently available on the use of the HLD equation to characterize crude
oil components as most efforts have been focused on characterizing contaminants, oils used in
cosmetic and pharmaceutical formulations, and vegetable oils7,9,10,11
. Rondón et al. made the
first attempt to relate the HLD concept to the phase behavior of crude oil formulations by
adjusting the concentration of added demulsifier such that an ultralow γow is observed at
HLD=012
. They, however, fell short of obtaining both the EACN of the oil and the “apparent”
78
characteristic curvature ( a
cC ) of asphaltenes. In addition, these researchers did not consider the
role of naphthenic amphiphiles in their system. It should be clarified that the qualifier
“apparent” is used to reflect the fact that asphaltenes are better classified as a solubility class
rather than a pure component or well-defined mixture.
One of the most complete sets of data used to determine the EACN of a wide range of
oils was produced by Baran Jr. et al.13
. These researchers used the phase behavior of µEs
produced with SDHS at 25°C, without alcohols or other co-surfactants, to obtain the value of S*
for oils with different ACNs ranging from 6 to 10. The following linear correlation was
established to relate these parameters:
92.017.0ln * ACNS (Eq. 2)
From the measured value of S* for non-alkane test oils, these researchers were able to
employ this equation to solve for their EACN (e.g. the EACN of toluene is 1). By comparing
Equation 2 with Equation 1 for optimum formulations (HLD=0) under similar processing
conditions as those used by Baran Jr. et al. (f(A)=0 and ΔT=0), one may conclude that the Cc of
SDHS=-0.92. It should be noted that large EACN values represent hydrophobic oils whereas
negative Cc (or a
cC ) values represent hydrophilic surfactants.
Baran Jr. et al. also confirmed that the EACN of oil mixture (EACNmix) follows a linear
mixing rule13
:
iimix EACNxEACN (Eq. 3)
79
In this equation, xi and EACNi represent the fraction and EACN of component i
respectively. This equation will be made use of later to estimate the EACN of the test oils in
mixtures with toluene.
Recently, Acosta et al. determined the Cc of various surfactants, including that of NaNs
obtained from Eastman Kodak8. The solved for Cc is -2.4 (highly hydrophilic). This finding is
consistent with the fact that NaNs are water-soluble and therefore tend to produce o/w
emulsions as in Chapter 3.
In the same work of Acosta et al., the Cc of ionic surfactant mixtures (Cc,mix) was shown
to follow a linear mixing rule as well8:
icimixc CxC ,, (Eq. 4)
In this chapter, S* is determined for µEs formulated with mixtures of asphaltenes, NAs,
and NaNs with SDHS at 25°C (ΔT=0) and in the absence of other co-surfactants (f(A)=0). To
obtain Cc,mix, Equation 1 is used with the aforementioned conditions.
The significances of the EACN obtained for asphaltenic oils, the a
cC obtained for
asphaltenes, and the Cc obtained for naphthenic amphiphiles are discussed in light of the EACN
and Cc of other oils and surfactants. It is also later presented in Chapter 8 how these parameters
can be used to interpret the formation and stability of rag layers. The solved for EACN and Cc
values presented in this chapter will vary according to the source of the oils, except for
naphthalene, and surfactants analyzed due to their complexity and ill-defined makeup.
80
4.3 MATERIALS AND METHODS
4.3.1 Materials
The following chemicals were used as purchased from Sigma-Aldrich Corp. (Oakville,
ON, Canada): anhydrous toluene (product #244511, 99.8%), anhydrous hexadecane (product
#296317, ≥99%), anhydrous hexane (product #296090, 95%), naphthalene (product #147141,
99%), NAs (product #70340, technical-grade extract), SDHS (product #86146, ~80% in water),
and NaCl (product #S9625, ≥99.5%). The purchased NAs are a technical grade extract from
crude oil (no defined origin) with an acid number of 230 g/equivalent, which is used here as its
molecular weight14,15
. Recent studies have shown that naphthenic amphiphiles obtained from
Alberta’s oil sands have a similar composition to those found in this sample and are enriched in
C12-C16 fatty acid equivalents with 3-6 double bond equivalents16
. The calculated Cc values of
naphthenic amphiphiles presented later are reflective of the wide distribution of such surfactants
found naturally within Canadian crude oil reserves. NaOH (product #LC24270-5, 0.1 N) was
purchased from Caledon Laboratory Chemicals (Georgetown, ON, Canada), black asphalt
(Dominion Sure Seal Ltd.) was purchased from a local retailer (Toronto, ON, Canada), and
coker feed bitumen (16.3% saturates, 39.8% aromatics, 28.5% resins, and 14.7% asphaltenes
according to SARA analysis) was provided by Syncrude Canada Ltd. (Edmonton, AB,
Canada)17
. Tap water was deionized using an APS Ultra mixed bed resin to a conductivity <3
µs/cm.
4.3.2 Asphaltene Precipitation
The same procedure as that used to precipitate asphaltenes in Chapter 3 was also
employed here.
81
4.3.3 Formulation of Microemulsions with Test Oil and Toluene Mixtures
Each of the test oils was mixed with toluene using a wrist-action shaker until a
homogeneous oil phase was obtained. The concentration of all the test oils (other than
naphthalene in toluene) ranged from 10 to 50 wt%. The concentration of naphthalene was
limited to just 30 wt% due to its lower solubility18
. 5 mL aliquots of these oil mixtures were
mixed together with 5 mL aqueous phase solutions composed of 0.1 M SDHS and 1-10 g
NaCl/100 mL in 15 mL flat bottom glass centrifuge tubes. These mixtures were allowed to
equilibrate for 1 week.
4.3.4 Formulation of Microemulsions with Test Surfactant and SDHS Mixtures
A similar formulation procedure as that described in Section 4.3.3 was used here. The
major differences were that pure toluene was used as the oil phase and the surfactant was a 0.1
M mixture of the test surfactant and SDHS. In addition, the volumes of the added aqueous and
oil phases were 5 mL and 2 mL respectively. The purpose of only using 2 mL of toluene instead
of 5 mL here was to reduce its consumption. For such systems at a relatively low surfactant
concentration, it is not expected that a 2.5 to 1 water to oil volume ratio will affect the µE phase
behavior19
. This was indeed confirmed by repeating the µE phase behavior of only select
systems using a 1 to 1 water to oil volume ratio. Asphaltenes and NAs, being oil soluble, were
diluted with toluene prior to being added to the formulations. The final compositions of the test
surfactant analyzed in the surfactant mixtures were 10 mol%, 30 mol%, 50 mol%, and 70 mol%.
In the case of asphaltene-SDHS mixtures, the surfactant mixture compositions were
calculated by assuming an average molecular weight of 600 g/mol for asphaltenes. This
assumption is based on the observation of Pomerantz et al. who analyzed the molecular weight
82
distribution of asphaltenes in similar bitumen via two-step laser mass spectroscopy20
. To
produce NaNs, NAs were neutralized with the appropriate amount of NaOH. A salinity scan was
performed on each surfactant mixture to determine S*.
4.3.5 Interfacial Tension Measurements
The optimum formulation along each of the performed salinity scans for the various test
oil and test surfactant mixtures was pinpointed by detecting the minimum γow according to the
spinning drop tensiometer procedure outlined in Chapter 2. For Type III µEs, γow was measured
between the excess oil and aqueous phases.
4.3.6 Asphaltene Partitioning at the Oil-Water Interface
As has been described before (and will be reinforced later), asphaltenes can be treated as
both an oil phase component and surfactant. To determine the fraction of asphaltenes that adsorb
at the oil-water interface, the concentration of asphaltenes in the bulk oil phase before and after
producing µEs was assessed using the same UV-vis spectroscopic technique developed in
Chapter 2. It was also confirmed using this technique that the asphaltenes content of the
prepared deasphalted bitumen in Section 4.3.2 was <10% of the original asphaltenes content.
4.4 RESULTS
4.4.1 Microemulsion Phase Behavior Scans
A Type IType IIIType II µE phase behavior transition is observed in all of the
salinity scans. In addition to the example of these transitions already presented in Figure 4.1,
other examples for formulations composed of a bitumen and toluene mixture as the oil phase
83
and a NAs and SDHS mixture as the surfactant are presented in Figures 4.2 (a) and (b). In the
case of Figure 4.2 (a), a bicontinuous middle phase µE is obtained at 3 g NaCl/100 mL. Due to
the high SDHS concentration in that phase, however, and the fact that bitumen and SDHS have
relatively high densities, it sinks to the bottom of the vial. To accurately determine S* for these
systems and others, the γow is measured as a function of the salinity, using smaller salt
increments of 0.2 g NaCl/100 mL in the vicinity of the Type III µEs.
(b) (a)
Figure 4.2: µE phase behavior transitions as a function of the salinity for a (a) 30 wt% bitumen
and 70 wt% toluene oil phase mixture and (b) 20 mol% NAs and 80 mol% SDHS surfactant
mixture.
4.4.2 Interfacial Tension of Test Oil and Toluene Mixtures
The γow measurements of the test oil and toluene mixtures are presented as a function of
the salinity in Figures 4.3 (a)-(d).
84
(a) (b)
(c) (d)
NaCl (g/100 mL)
γo
w (
mN
/m)
Figure 4.3: The measured γow as a function of the salinity for (a) bitumen and toluene, (b)
asphalt and toluene, (c) naphthalene and toluene, and (d) deasphalted bitumen and toluene oil
phase mixtures.
According to this γow data, S* increases from ~3 g/100 mL to 3.5 g/100 mL as the
bitumen fraction in the oil phase is increased from 10 wt% to 50 wt%. However, for all the
fractions of asphalt and naphthalene dissolved in toluene, S* remains constant at 3 g/100 mL.
This is an indication that bitumen is more hydrophobic than both asphalt and naphthalene,
which have a similar polarity to that of toluene. For deasphalted bitumen, the increase in S*
reflects that the non-asphaltenic part of bitumen is more hydrophobic than whole bitumen and
its asphaltene-like components. This result is consistent with the fact that toluene is a suitable
solvent for asphaltenes whereas hexane and heptane are suitable solvents for maltenes. For
85
bitumen, asphalt, and deasphalted bitumen, the minimum γow increases with the test oil
composition. This observation is consistent with the fact that increasing the molar volume of the
solubilized oil reduces its solubilization capacity, likely due to the fact that it is more difficult to
disrupt the interaction amongst oil molecules21
. A reduction of the solubilization capacity is
directly linked to an increase in the minimum γow as expressed by the Chun Huh relationship
and the concept of interfacial rigidity19
.
4.4.3 EACN of Test Oils
To determine the average EACN of asphalt, bitumen, naphthalene, and deasphalted
bitumen, the EACNmix of each oil mixture is first calculated using the estimated S* from the γow
data presented in Figures 4.3 (a)-(d) as well as Equation 2. Knowing EACNmix and that the
EACN of toluene is 1, the EACN of each test oil can be calculated using Equation 3. However,
there is a question to be resolved before carrying out that calculation. That question is if the
composition xi in Equation 3 should be on the basis of moles, weight, or volume. While Baran
Jr. et al. assumed that the composition was based on the mole fraction, it is important to keep in
mind that the HLD equation is semi-empirical, and that there are therefore no fundamental bases
to argue one cause or the other. In fact, because the molecular weight of the different
compounds analyzed by Baran et al. is approximately the same, mole and weight fractions are
similar. The situation is different for mixtures of toluene with large asphaltenic crude oils,
making it imperative to determine if molar, weight, or volume fractions are more appropriate.
This issue is elucidated by determining, experimentally, the shifts in S* of hexadecane and
toluene mixtures and comparing these values to the salinity shifts calculated from the HLD
equation.
86
To obtain the equation for the salinity shift in the presence of electrolyte, the concept of
ideal mixing is applied to the HLD for a mixture of oils. Considering this mixture at optimal
conditions:
testtestrefrefmix HLDxHLDxHLD 0 (Eq. 5)
In this equation, the subscripts “ref” and “test” refer to the reference and test oils
respectively. Furthermore, considering Equation 1 at f(A)=0 and ΔT=0:
c
test
ocmixtestc
ref
ocmixref CKNSxCKNSx ,
*
,
* lnln0 (Eq. 6)
Knowing that *
refx + *
testx =1, one obtains:
c
test
octest
ref
ocrefmix CKNxKNxS ,,
*ln0 (Eq. 7)
For the reference oil alone, the following is true:
c
ref
ocref CKNS ,
*ln0 (Eq. 8)
Subtracting Equation 8 from Equation 7 yields the desired expression for the salinity
shift:
ref
oc
test
octest
ref
mix NNKxS
S,,*
*
ln
(Eq. 9)
To determine whether testx should be expressed on a molar, weight, or volume basis,
Equation 9 is applied to µEs produced in systems composed of hexadecane and toluene mixtures
as the oil phase and SDHS and sodium dioctyl sulfosuccinate (AOT) mixtures as the surfactant.
The results of this test are presented in Figure 4.4.
87
xhexadecane
Figure 4.4: Experimented and modeled shifts of S* for µEs composed of hexadecane and
toluene oil phase mixtures and 0.1 M of a 35 mol% SDHS and 65 mol% AOT surfactant
mixture.
The modeled shift in S* (solid line) for all fractions of hexadecane presented in Figure
4.4 are established using test
ocN , (hexadecane)=167. The data points presented as circles,
diamonds, and triangles in this figure are obtained by plotting the experimental salinity shift
versus the composition of hexadecane on a molar, weight, and volume basis respectively.
According to the data obtained, the volume fraction is the most accurate descriptor of the
composition terms in the EACN mixing rule. This finding is in agreement with that of Puerto et
al. who suggested that representing the oil phase composition on a molar basis reveals
nonlinearities in the phase behavior of surfactant-oil-water formulations22
. Until the
fundamental bases of the EACN mixing rule are elucidated, the significance of this finding may
not be fully appreciated. From a practical point of view, this finding provides a significant
advantage towards the elucidation of the EACN values of oils of unknown structure or complex
composition, such as bitumen and asphalt.
88
Equation 9 is subsequently applied (using testx as a volume fraction) to mixtures of the
test oils and toluene. Table 4.1 summarizes the parameters for these formulations and the
calculated EACN values for the oil mixtures and test oils.
Table 4.1: Calculated EACN of asphalt, bitumen, naphthalene, and deasphalted bitumen
Test Oil xtest ln( *
mixS ) EACNmix EACNtest
Asphalt
0.1 1.1 1.1
1.3 0.3 1.1 1.1
0.5 1.1 1.1
Bitumen
0.1 1.1 1.1
2.5 0.3 1.1 1.1
0.5 1.3 2.0
Naphthalene
0.1 1.1 1.1
1.3 0.2 1.1 1.1
0.3 1.1 1.1
Deasphalted
Bitumen
0.1 3.3 1.5
6.2 0.3 3.9 2.6
0.5 4.6 3.6
4.4.4 Interfacial Tension of Test Surfactant and SDHS Mixtures
The measured γow of µEs formulated for the test surfactant and SDHS mixtures
described in Section 4.3.4 are presented in Figures 4.5 (a)-(c) as a function of the salinity.
89
NaCl (g/100 mL)
(c) γ
ow (
mN
/m)
NaCl (g/100 mL) NaCl (g/100 mL)
γo
w (
mN
/m)
(a)
NaCl (g/100 mL)
(b)
γo
w (
mN
/m)
Figure 4.5: The measured γow as a function of the salinity for (a) NAs and SDHS, (b) NaNs and
SDHS, and (c) asphaltenes and SDHS surfactant mixtures at a total concentration of 0.1 M.
The data in Figure 4.5 suggests that NAs are more lipophilic than SDHS since an
increase in the surfactant mixture concentration of NAs produced a decrease in S*. On the other
hand, NaNs are more hydrophilic than SDHS since an increase in their concentration in the
surfactant mixture produced an increase in S*. By comparing Figures 4.5 (a) and (b), it is
evident that the displacement in S* for the case of NAs and SDHS mixtures is not substantial.
With regards to asphaltenes (Figure 4.5 (c)), a slight decrease in S* is observed as its
concentration within the surfactant mixture is increased from 10 mol% to 70 mol%. This
suggests that asphaltenes are lipophilic relative to both SDHS and NaNs. To compare the
hydrophilic-lipophilic nature of asphaltenes relative to NAs, however, the partitioning behavior
90
of asphaltenes at the oil-water interface must be accounted for. This data will be presented in
Section 4.4.5.
4.4.5 Cc of Test Surfactants
Acosta et al. previously developed Equation 10 below to determine the Cc of anionic
surfactants and fatty acids based on the shift of S* as a function of the surfactant composition
8:
test
c
ref
c
ref
mix CCS
S
test*
*
xln (Eq. 10)
The salinity shift of NAs and SDHS and NaNs and SDHS surfactant mixtures is
presented in Figures 4.6 (a) and (b) as a function of the test surfactant mole fraction within the
0.1 M surfactant mixture.
(a) (b)
xNA xNaN
Figure 4.6: Salinity shift of (a) NAs and SDHS and (b) NaNs and SDHS surfactant mixtures as
a function of the test surfactant mole fraction within the 0.1 M surfactant mixture.
91
The values of the salinity shifts in Figures 4.6 (a) and (b) are analyzed using the linear
regression tool within Microsoft Excel (2003). The linear regression analysis produced with this
tool yields the value of the slope and the 95% confidence interval for this value. These values
are presented in Table 4.2. The slope values can be introduced into Equation 10 to calculate the
Cc of NAs and NaNs. The results from these calculations are also presented in Table 4.2.
Table 4.2: Cc (* a
cC ) of NAs, NaNs, and asphaltene aggregates.
Test Surfactant Ln[ *
mixS / *
refS ]/X2 test
cC
NAs -0.31±0.05 -0.61±0.05
NaNs 1.7±0.1 -2.6±0.1
Asphaltene Aggregates* -2.0±0.2
* 1.1±0.2
*
Evaluating the a
cC of asphaltene aggregates requires an understanding of the partitioning
of asphaltenes between the bulk oil phase and the oil-water interface. Figure 4.7 (a) presents the
molar fraction of asphaltenes (in mixtures with SDHS) at the interface versus the equilibrium
volume fraction of asphaltenes (in mixture with toluene) in the excess bulk phase. According to
this figure, only when the volume fraction of asphaltenes in toluene is larger than 0.03 do the
asphaltenes adsorb significantly at the oil-water interface. A plateau fraction of asphaltenes at
the oil-water interface is reached at ~0.12. At asphaltene volume fractions in the oil phase larger
than 0.05, these asphaltenes tend to precipitate out of solution. While asphaltenes in toluene
alone are completely soluble, the observed precipitation is consistent with earlier observations
by Yarranton et al. that the presence of oil-water interfaces induces the precipitation of
asphaltenes23
.
92
(a) (b)
Figure 4.7: (a) Asphaltene partitioning and (b) the shift in S* for optimum µEs formulated with
an asphaltenes and SDHS surfactant mixture.
In previous work involving the characterization of the Cc of polar organic molecules,
like lipophilic linkers, partitioning has been identified as a source of error8. In order to account
for these effects, the shift in S* is plotted in Figure 4.7 (b) as a function of the calculated molar
fraction of asphaltenes in mixtures with SDHS at the interface. Using the same mathematical
approach as used for the characterization of the Cc of NAs and NaNs, the a
cC of asphaltene
aggregates may be determined. Unlike the case for NAs and NaNs, a single regression line
cannot be used to fit the data presented here. To overcome this issue, the data is separated into a
non surface-active asphaltenes cluster and a surface-active asphaltenes cluster at the transition
point indicated in the above discussion (~0.1). In doing so, separate regression lines can be fit to
each of the clusters. Considering that the concept of Cc applies to surface-active species, the
slope of the regression line for surface-active asphaltenes and Equation 10 were used to
calculate the a
cC of surface-active asphaltene aggregates as presented in Table 4.2.
93
4.5 DISCUSSIONS
4.5.1 Analysis of the Hydrophilic-Lipophilic Nature of Asphaltenic Crude Oils
The calculated EACN of the asphaltenic oils listed in Table 4.1 confirm that, indeed,
these oils have a similar hydrophilic-lipophilic nature as that of toluene. It is counter intuitive to
think that such heavy crude oil fractions are less hydrophobic than light crude oils, which are
typically simulated (in µE phase behavior studies) with oils such as octane (EACN=8)24
. Such
counterintuitive behavior has been reported before, but this is the first time that it has been
quantified through the EACN value25
.
Another interesting observation is that the EACN of bitumen is slightly larger than that
of asphalt. This could be explained by the fact that bitumen contains less asphaltenes (~15%)
than asphalt (~45%)26
. The impact of asphaltenes on the polarity of these crude oils may be
elucidated from the EACN of the deasphalted (maltene-like) fraction of bitumen. The EACN of
this deasphalted bitumen fraction is between that of hexane and heptane. Considering that
asphaltenes only represent ~15% of bitumen but reduces the EACN of bitumen to a value of
approximately 2 suggests that the polar nature of asphaltenes dominates the hydrophilic-
lipophilic nature of bitumen. Furthermore, the relatively low EACN of asphaltenic oils also
suggests that they should have amphiphilic properties. For example, it has been shown that
benzene is a polar molecule (EACN=0) that is also surface-active and tends to segregate near
the oil-water interface27
.
The simple method of mixing a test oil and reference oil to determine the EACN of the
test oil is successful in principle. The fact that volume fractions, instead of mole fractions, are
more in line with the HLD model allows the use of this method for oils of unknown structure
94
and composition. This simple test and reference oil phase mixture method is simpler than other
available methods to determine the EACN of a wide range of oils7.
4.5.2 Analysis of the Hydrophilic-Lipophilic Nature of Naphthenic Amphiphiles
and Asphaltene Aggregates
To put the Cc of NAs and NaNs presented in Table 4.2 into context, it is important to
recall that Acosta et al. determined that the Cc value of NaNs obtained from Eastman Kodak is
-2.4±0.28. While the NaNs source studied here is different (obtained by neutralizing NAs
purchased from Sigma-Aldrich Canada, Inc.), the obtained Cc is similar. In the case of NAs, the
calculated Cc is in between that of oleic acid (Cc=0) and SDHS (Cc=-0.92). In other words, NAs
are more hydrophilic than oleic acid. Another interesting point of comparison is that sodium
oleate, the salt of oleic acid, has a Cc of -1.78. In this case, the neutralization of the fatty acid
produced a decrease in Cc of 1.7. In the case of NAs, the neutralization to NaNs produced a
similar decrease in Cc of 2.
With regards to the a
cC of asphaltene aggregates, it should be re-emphasized that the
molecular weight of asphaltenes is a probability distribution with a peak intensity at 600 g/mol.
Assuming that the molecular weight distribution of asphaltenes varies from 500 g/mol to 1000
g/mol according to the analysis performed by Pomerantz et al., the a
cC limits of the asphaltene
aggregates may range from 0.8 to 2.320
. In comparison to both NAs and NaNs, it may be
concluded that asphaltene aggregates are much more lipophilic. In general terms, the upper a
cC
limit of asphaltene aggregates is comparable to that of AOT (Cc=2.55), which is one of the most
lipophilic surfactants identified thus far8.
95
4.6 CONCLUSIONS
Using the HLD model for ionic surfactants as well as several basic mixing rules, it was
shown that bitumen had an equivalent alkane carbon number (EACN) of 2.5, a value slightly
larger than that of asphalt (EACN=1.3) and naphthalene (EACN=1.3). These low EACN values
reflect the polar nature of polyunsaturated aromatic compounds present in these oils. The polar
nature of asphaltenes was additionally justified by the fact that the EACN of deasphalted
bitumen was ~6.2. It was furthermore demonstrated that asphaltenes were surface-active under
certain conditions and that they were significantly more lipophilic than both naphthenic acids
(NAs, Cc=-0.61) and sodium naphthenates (NaNs, Cc=-2.6).
4.7 REFERENCES
1 Salager, J.-L.; Antón, R.E.; Sabatini, D.A.; Harwell, J.H.; Acosta, E.J.; Tolosa, L.I. Enhancing
Solubilization in Microemulsions-State of the Art and Current Trends. J. Surfactants Deterg.
2005, 8, 3-21.
2 Acosta, E.J. The HLD-NAC Equation of State for Microemulsions Formulated with Nonionic
Alcohol Ethoxylate and Alkylphenol Ethoxylate Surfactants. Colloids Surf., A 2008, 320, 193-
204.
3 Healy, R.N.; Reed, R.L. Physicochemical Aspects of Microemulsion Flooding. Soc. Pet. Eng.
AIME J. 1974, 14, 491-501.
96
4 Healy, R.N.; Reed, R.L.; Stenmark, D.G. Multiphase Microemulsion Systems. Soc. Pet. Eng.
AIME J. 1976, 16, 147-160.
5 Antón, R.E.; Salager, J.-L. Effect of the Electrolyte Anion on the Salinity Contribution to
Optimum Formulation of Anionic Surfactant Microemulsions. J. Colloid Interface Sci. 1990,
140, 75-81.
6 Salager, J.-L.; Morgan, R.; Schechter, R.S.; Wade, W.H.; Vasquez, E. Optimum Formulation
of Surfactant/Water/Oil Systems for Minimum Interfacial Tension or Phase Behavior. Soc. Pet.
Eng. AIME J. 1979, 19, 107-115.
7 Nardello, V.; Chailloux, N.; Poprawski, J.; Salager, J.-L.; Aubry, J.-M. HLD Concept as a
Tool for the Characterization of Cosmetic Hydrocarbon Oils. Polym. Int. 2003, 52, 602-609.
8 Acosta, E.J.; Yuan, J.S.; Bhakta, A.S. The Characteristic Curvature of Ionic Surfactants. J.
Surfactants Deterg. 2008, 11, 145-158.
9 Van Hecke, E.; Catté, M.; Poprawski, J.; Aubry, J.-M.; Salager, J.-L. A Novel Criterion for
Studying the Phase Equilibria of Nonionic Surfactant-Triglyceride Oil-Water Systems. Polym.
Int. 2003, 52, 559-562.
10 Tongcumpou, C.; Acosta, E.J.; Scamehorn, J.F.; Sabatini, D.A.; Yanumet, N.; Chavadej, S.
Enhanced Triolein Removal using Microemulsions Formulated with Mixed Surfactants. J.
Surfactants Deterg. 2006, 9, 181-189.
97
11 Thakur, R.K.; Villette, C.; Aubry, J.-M.; Delaplace, G. Formulation-Composition Map of a
Lecithin-Based Emulsion. Colloids Surf., A 2007, 310, 55-61.
12 Rondón, M.; Bouriat, P.; Lachaise, J.; Salager, J.-L. Breaking of Water-in-Crude Oil
Emulsions. 1. Physicochemical Phenomenology of Demulsifier Action. Energy Fuels 2006, 20,
1600-1604.
13 Baran Jr., J.R.; Pope, G.A.; Wade, W.H.; Weerasooriya, V.; Yapa, A. Microemulsion
Formation with Mixed Chlorinated Hydrocarbon Liquids. J. Colloid Interface Sci. 1994, 168,
67-72.
14 Smith, D.F.; Schaub, T.M.; Kim, S.; Rodgers, R.P.; Rahimi, P.; Teclemariam, A.; Marshall,
A.G. Characterization of Acidic Species in Athabasca Bitumen and Bitumen Heavy Vacuum
Gas Oil by Negative-Ion ESI FT-ICR MS with and without Acid-Ion Exchange Resin
Prefractionation. Energy Fuels 2008, 22, 2372-2378.
15 Frank, R.A.; Kavanagh, R.; Kent Burnison, B.; Arsenault, G.; Headley, J.V.; Peru, K.M.; Van
Der Kraak, G.; Solomon, K.R. Toxicity Assessment of Collected Fractions from an Extracted
Naphthenic Acid Mixture. Chemosphere 2008, 72, 1309-1314.
16 Headley, J.V.; Peru, K.M.; Armstrong, S.A.; Han, X.; Martin, J.W.; Mapolelo, M.M.; Smith,
D.F.; Rogers, R.P.; Marshall, A.G. Aquatic Plant-Derived Changes in Oil Sands Naphthenic
Acid Signatures Determined by Low-, High-, and Ultrahigh-Resolution Mass Spectrometry.
Rapid Commun. Mass Spectrom. 2009, 23, 515-522.
98
17 Akbarzadeh, K.; Alboudwarej, H.; Svrcek, W.Y.; Yarranton, H.W. A Generalized Regular
Solution Model for Asphaltene Precipitation from n-Alkane Diluted Heavy Oils and Bitumens.
Fluid Phase Equilib. 2005, 232, 159-170.
18 Heric, E.L.; Posey, C.D. Interaction in Nonelectrolyte Solutions. II. Solubility of Naphthalene
at 25°C in some Mixed Solvents Containing Toluene, Ethylbenzene. J. Chem. Eng. Data 1964,
9, 161-165.
19 Acosta, E.; Szekeres, E.; Sabatini, D.A.; Harwell, J.H. Net-Average Curvature Model for
Solubilization and Supersolubilization in Surfactant Microemulsions. Langmuir 2003, 19, 186-
195.
20 Pomerantz, A.E.; Hammond, M.R.; Morrow, A.L.; Mullins, O.C.; Zare, R.N. Two-Step Laser
Mass Spectrometry of Asphaltenes. J. Am. Chem. Soc. 2008, 130, 7216-7217.
21 Acosta, E.J.; Nguyen, T.; Witthayapanyanon, A.; Harwell, J.H.; Sabatini, D.A. Linker-Based
Bio-Compatible Microemulsions. Environ. Sci. Technol. 2005, 39, 1275-1282.
22 Puerto, M.C.; Reed, R.L. Three-Parameter Representation of Surfactant/Oil/Brine Interaction.
Soc. Pet. Eng. J. 1983, 23, 669-682.
23 Yarranton, H.W.; Hussein, H.; Masliyah, J.H. Water-in-Hydrocarbon Emulsions Stabilized by
Asphaltenes at Low Concentrations. J. Colloid Interface Sci. 2000, 228, 52-63.
99
24 Bourrel, M. and Schechter, R., 1988. Microemulsions and Related Systems: Formulation,
Solvency, and Physical Properties. New York: Marcel Dekker, Inc.
25 Acevedo, S.; Borges, B.; Quintero, F.; Piscitelly, V.; Gutierrez, L.B. Asphaltenes and Other
Natural Surfactants from Cerro Negro Crude Oil. Stepwise Adsorption at the Water/Toluene
Interface: Film Formation and Hydrophobic Effects. Energy Fuels 2005, 19, 1948-1953.
26 Shakirullah, M.; Ahmad, I.; Arsala Khan, M.; Ali Shah, A.; Ishaq, M.; Habib-ur-Rehman.
Conversion of Asphalt into Distillate Products. Energy Convers. Manage. 2008, 49, 107-112.
27 Szekeres, E.; Acosta, E.; Sabatini, D.A.; Harwell, J.H. A Two-State Model for Selective
Solubilization of Benzene-Limonene Mixtures in Sodium Dihexyl Sulfosuccinate
Microemulsions. Langmuir 2004, 20, 6560-6569.
100
CHAPTER 5:
EXPERIMENTAL EVALUATION OF EMULSION STABILITY
VIA SURFACTANT-OIL-WATER PHASE BEHAVIOR SCANS
This chapter is derived from the following submitted manuscript:
Kiran, S.K.; Acosta, E.J. Experimental Evaluation of Emulsion Stability Via Surfactant-Oil-
Water Phase Behavior Scans. J. Surfactants Deterg. (ID: JSD-13-0018).
101
5.1 ABSTRACT
The stability of anionic surfactant (sodium dihexyl sulfosuccinate (SDHS))-oil (toluene)-
water emulsions was characterized in this chapter in terms of aggregation (ap), drainage (dp), and
coalescence (cp) time periods. These time periods, determined by tracking the normalized
displacement of a set of phase separation fronts, were evaluated as a function of the quantified
proximity to the phase inversion point using the hydrophilic-lipophilic deviation (HLD)
framework. The secondary effects of surfactant concentration and temperature on emulsion
stability were also evaluated. It was determined that at a low surfactant concentration (0.01 M
SDHS), the cp time period was most dominant for oil droplets in water-continuous formulations
(HLD<0) and water droplets in oil-continuous formulations (HLD>0). At larger surfactant
concentrations, the ap time period was most dominant at HLD<0 whereas all of the time periods
were comparable at HLD>0. In addition, the apparent drainage and coalescence activation
energies were shown to be strongly influenced by the interfacial tension, whose minimum
coincides with that of the overall emulsion stability at the phase inversion point (HLD=0).
5.2 INTRODUCTION
It was previously described in Chapters 1 and 4 that microemulsion (µE) phase behavior
scans can be used to evaluate formulation conditions that produce an inversion in the surfactant
partitioning between the aqueous and oil phases. Under net formulation conditions that favor an
overall hydrophilic (hydrophobic) environment, the surfactant preferentially partitions into the
aqueous (oil) phase as oil (water)-swollen micelles (or Type I (Type II) µEs) in equilibrium with
an excess oil (aqueous) phase. At balanced formulation conditions, where phase inversion takes
place, oil and water co-solubilize into a bicontinuous (or Type III) µE phase that co-exists with
102
excess oil and aqueous phases. A Type IType IIIType II phase behavior scan for sodium
dihexyl sulfosuccinate (SDHS)-toluene-water µEs is illustrated in Figure 5.1. The ability to
evaluate various equilibrium properties including solubilization capacities, interfacial tensions
(γow), densities (ρµE), and, as will be described in the next chapter, viscosities (ηµE) from such a
simple phase behavior scan is useful in applications ranging from surfactant enhanced oil
recovery to the design of cosmetic and pharmaceutical drug delivery systems1,2
.
NaCl
(g/100 mL): 10752.41.50.8 432.3
0HLD: -1.4 -0.7 -0.3 -0.2 0.3 0.5 0.9 1.2
Type I Type III Type II
Figure 5.1: A Type IType IIIType II phase behavior scan for 0.1 M SDHS-toluene-water
µEs at 25°C.
Phase behavior scans also produce information that is relevant to the dynamics of
emulsification3,4,5,6,7,8,9,10,11
. Under the same formulation conditions as for Type I (Type II) µEs,
emulsions take the form of the excess oil (aqueous) phase dispersed throughout the oil-in-water
(o/w) (water-in-oil (w/o)) µE phase itself. Under Type III conditions, both the excess oil and
aqueous phases are dispersed throughout the bicontinuous µE phase. The corresponding
connection to the stability of these emulsions is less well understood. The aim of this work is to
103
provide a new insight into this connection by evaluating the kinetics of the different separation
processes that take place as a function of the surfactant concentration and temperature.
Salager et al. and Binks et al. proposed different separation processes that influence the
kinetics of demulsification around the phase inversion point7,9,10
. By identifying and tracking the
normalized displacement of the µE and excess phase separation fronts versus time, these authors
argued that the aggregation of emulsion droplets into flocs leads to a faster rate of settling. The
subsequent onset of film thinning into the resulting Plateau borders of a highly concentrated
emulsion layer further accelerates the onset of coalescence. A schematic overview of each of
these processes is illustrated in Figure 5.2.
Aggregation
Film Thinning
Coalescence
Settling
Figure 5.2: Emulsion aggregation, settling, film thinning, and coalescence processes.
104
While the studies of Salager et al. and Binks et al. showed that the µE and excess phases
separate the fastest at the phase inversion point, they failed to provide a detailed description of
its kinetics. The first objective of this chapter is to assess how aggregation, settling, film
thinning, and coalescence contribute to the total separation time. This will be conducted as a
function of the proximity to the phase inversion point. Figure 5.3 (a) illustrates how the
observable phase separation stages evolve over time in a test tube for emulsified water droplets
(black) dispersed throughout a continuous Type II µE phase (gray). Figure 5.3 (b) presents the
normalized displacement of the phase separation fronts versus time and the extrapolated time
periods.
μE Phase Aqueous Phase
Δhw(t)=Δhw,tot
ΔhμE(t)=ΔhμE,totΔhμE(t)ΔhμE(t)
Δhw(t)Δhw(t)
ΔhμE(t)
Time
ap dp
No
rmalized
Dis
pla
cem
en
t
Timecp
(a)
(b)
Figure 5.3: (a) Evolution of the observable phase separation stages versus time in a test tube for
emulsions produced in Type II µEs. (b) Normalized displacement of the µE and excess aqueous
phase separation fronts versus time and the extrapolated ap, dp, and cp time periods.
105
No observable changes to the emulsion can be visually detected over the initial induction
(or aggregation) time period (ap) until a µE phase separation front develops. The period of time
between the onset of the µE phase separation front and the appearance of an aqueous phase
separation front is referred to as the drainage time period (dp). Over this time period, the
drainage of the continuous µE phase essentially leads to the production of a more concentrated
emulsion layer. The final period of time between the onset of the aqueous phase separation front
and its complete separation is referred to as the coalescence time period (cp). The onset of the
final cp time period is realized once a critical packing is reached and represents the rejection of
the excess phase from the emulsion. It is important to clarify that the intent of selecting the
names for these phase separation time periods as such is to reflect the rate-limiting process that
is expected to dominate demulsification. In reality, however, a multitude of these processes may
be acting together at any point in time.
The second objective of this chapter is to develop an understanding of how the µE phase
behavior properties influence the duration of the emulsion phase separation time periods. The
initial ap time period likely depends on the original emulsion droplet size. The original emulsion
droplet size is in turn a function of the mixing energy input and γow12
. Lower γow should
theoretically lead to the formation of smaller emulsion droplets that settle slowly but that are
much more mobile as a result of Brownian motion13,14
. This increase in mobility should lead to
an increase in the collision frequency of emulsion droplets and a therefore greater probability of
their aggregation. It is very possible that the emulsion droplets that make up this aggregated
state undergo an internal coalescence process that does not result in any separation of the excess
phase. The next dp time period is more complex in nature as it likely involves the settling of
aggregated flocs of growing emulsion droplets as well as film thinning. The final cp time period
106
is likely associated with coalescence processes resulting from the breakage of oil-water-oil
and/or water-oil-water interfaces. The rupture of these interfaces may be explained by the hole
nucleation theory. This theory predicts that the activation energy of coalescence is directly
proportional to γow15,16,17
.
Another objective of this chapter is to explore the influence of the surfactant
concentration on the emulsion phase separation time periods. According to the literature, an
increase in the surfactant concentration may lead to several possible outcomes. For one, the
initial ap time period may be lengthened due to an increase in the electrostatic and steric
repulsions caused by the additional µE droplets in the continuous phase medium that separates
the approaching emulsion droplets18
. On the other hand, it is also possible for the ap time period
to decrease via attractive depletion interactions at low volume fractions of µE droplets17,18,19,20
.
The ap time period should also decrease in the event of µE-mediated Ostwald ripening10,21,22
.
With regards to the subsequent dp time period, an increase in its timescale can be expected
because of the hindered settling of emulsion droplets throughout a continuous µE phase of
increased ηµE6,10
. This effect may become even more pronounced if the number of metastable
µE layers that need to be expelled during film thinning increases23,24
. For the final cp time
period, the added amount of adsorbed surfactant should lead to an increase in its timescale due
to a better ability to withstand any sort of film rupturing11
. Additionally, depletion-repulsion
mechanics (i.e. the osmotic pressure cost of excluding µE droplets from the inter-droplet
continuous phase medium) may even further prolong the cp time period25,26
.
The last objective of this work is to study the effect of temperature (T) on the emulsion
phase separation time periods. By treating aggregation, drainage, and coalescence as a series of
chemical reactions that conform to Arrhenius’s law, an increase in T should foreseeably lead to
107
a decrease in their time periods across the µE phase behavior spectrum. The apparent activation
energy (W*) for a given one of aggregation, drainage, and coalescence can be calculated using
the following expression of Kabalnov et al.16,27
:
Tk
Wft
B
p
*exp (Eq. 1)
Here, tp is the emulsion phase separation time period of interest, f is a proportionality
constant that is assumed to be independent of T, and kB is the Boltzmann constant. Kabalnov et
al. applied Equation 1 to determine W* for only the coalescence of Type III emulsions. Other
efforts by Acosta et al. and Witthayapanyanon et al., which are equally as constrained as those
of Kabalnov et al., looked to instead fit W* according to changes in the emulsion coalescence
rate as a function of the interfacial rigidity of the system28,29
.
In this chapter, the ap, dp, and cp time periods will be studied for SDHS-toluene-water
emulsions. As will be shown in greater detail later, the total stability of these emulsions falls in
the range of just seconds to a few hours. These are much more reasonable timeframes for
performing high throughput analysis compared to days as has been published for sodium dioctyl
sulfosuccinate (AOT) stabilized emulsions9,10
. The proximity to the phase inversion point will
be quantified for SDHS-toluene-water emulsions using the following hydrophilic-lipophilic
deviation (HLD) expression for ionic surfactants that was described in detail in Chapter 4:
coc CTAfNSHLD 01.017.0ln , (Eq. 2)
In short, S is the electrolyte concentration (in g/100 mL), Nc,o is the equivalent alkane
carbon number (EACN) of the oil phase (EACN=1 for toluene), f(A) is a function of the co-
surfactant type and concentration, ΔT is the difference in temperature from 25°C, and Cc is the
108
characteristic curvature of the surfactant (Cc=-0.92 for SDHS). A HLD<0HLD=0HLD>0
scan reflects a Type IType IIIType II µE phase behavior transition.
5.3 MATERIALS AND METHODS
5.3.1 Materials
NaCl (product #S9625, ≥99.5%) and SDHS (product #86146, ~80% in water) were
purchased from Sigma-Aldrich Corp. (Oakville, ON, Canada). Reagent grade acetone (product
#1200-1-10) and toluene (product #9200-1-10) were purchased from Caledon Laboratory
Chemicals (Georgetown, ON, Canada). All of these materials were stored at 25°C and used as
received. Tap water was deionized using an APS Ultra mixed bed resin to a conductivity <3
µs/cm.
A multipoint turbidimeter was constructed in-house using laser modules (product
#VLM-650-03-LPA), linear photodiodes (product #OPT101P), and digital potentiometers
(product #AD5206BN10) acquired from Digi-Key (Thief River Falls, MN, USA). Almost all
other electrical components (solderless breadboards, insulated wires, hex inverters (product
#74LS04), and an Arduino Diecimilia microcontroller) were obtained from Creatron Inc.
(Toronto, ON, Canada). To expand the number of input/output ports on the Arduino Diecimilia
microcontroller, a third party multiplexer (mux) shield was purchased from Mayhew
Laboratories (Greenville, SC, USA).
5.3.2 Microemulsion Phase Behavior Scans and Emulsification
The baseline µE phase behavior scan, shown in Figure 5.1, was conducted in 15 mL flat-
bottom glass test tubes at 25°C by adding 5.5 mL of toluene to 5.5 mL of an aqueous phase
109
solution composed of 0.8-10 g/100 mL NaCl and 0.1 M SDHS. After having mixed these phases
together for 1 minute at 3200 rpm using a 150 W VWR analog vortex mixer, they were allowed
to equilibrate. The resulting sphere-equivalent µE droplet sizes, as calculated using the net-
average curvature (NAC) model in the next chapters, were on the order of ~1-30 nm.
Emulsification was induced by re-agitating these pre-equilibrated µEs. It is safe to assume from
the similar viscosities of toluene and water that emulsion droplet breakup occurred
instantaneously under the applied mixing conditions12
. It can further be concluded from the
interplay of hydrodynamic and thermodynamic effects that the resulting emulsion droplets
immediately took on the expected morphology as predicted by the HLD model30
.
Additional µE phase behavior scans were conducted at 0.01 M and 0.3 M SDHS. To
account for SDHS’s contribution to the total electrolyte concentration (S in Equation 2), 15% of
its sodium counterion was assumed to dissociate. This assumption is consistent with previous
observations for SDHS phase behavior scans31,32
. Only select baseline (0.1 M SDHS) µEs at
HLD=0, ±0.4, ±0.7, and ±1.1 were formulated at T=7°C, 15°C, 35°C, and 44°C. At 7°C and
15°C, all emulsification and phase separation experiments were carried out in a refrigerated
incubator (Fisher Scientific International Inc.). At 35°C and 44°C, all emulsification and phase
separation experiments were carried out in an oven (Cenco Instruments Corp.).
5.3.3 Interfacial Tension of Baseline Microemulsions
The γow between the heavy and light phases of equilibrium baseline (0.1 M SDHS) µEs
at 25°C was measured using the spinning drop tensiometer technique described in Chapters 2.
110
5.3.4 Average Diameter of Baseline Emulsion Droplets
Optical micrographs of a 10 µL emulsified baseline (0.1 M SDHS) sample at 25°C were
taken using an Olympus wide zoom digital camera at 4× magnification mounted on top of an
Olympus BX-51 microscope set at 100× magnification within 1 minute after the test tube was
shaken. From the number frequency (Fi) of observed emulsion droplets of measured diameter
E
id in a population size of 30, the average emulsion droplet diameter ( E
dd ) was calculated as per
Chapter 2:
2
3
E
ii
E
iiE
d
dF
dFd (Eq. 3)
5.3.5 Emulsion Phase Separation Profiles
Emulsion phase separation profiles were assessed by evaluating the normalized
displacement of the µE (ΔsµE(t)), excess oil (Δso(t)), and/or excess aqueous (Δsw(t)) phase
separation fronts versus time as follows:
totE
E
Eh
thts
,
(Eq. 4)
toto
o
oh
thts
,
(Eq. 5)
totw
ww
h
thts
,
(Eq. 6)
In these equations, ΔhµE(t), Δho(t), and Δhw(t) are the tracked net displacement of the
moving µE, excess oil, and excess aqueous phase separation fronts whereas ΔhµE,tot, Δho,tot, and
111
Δhw,tot are their respective total required displacement for equilibrium to be reached. The net and
total required displacements of the relevant phase separation fronts for a Type II emulsion are
described in Figure 5.3 (a). The primary method of tracking the net displacement of moving
phase separation fronts was by taking time-lapse images every 15 seconds. The gradient in the
gray level for each series of images pertaining to a given emulsion was analyzed using
MATLAB’s image processing toolbox in order to help identify the location of the moving phase
separation fronts.
The net displacement of moving phase separation fronts was additionally tracked using
high frequency turbidity (τ(t)) measurements with the array of laser-photodiode pairs (switched
on/off for 0.5 seconds/cycle in a preset order) shown in Figure 5.4.
0.8 cm
2.2 cm
3.7 cm
5.1 cm
6.5 cm
1.5 cm
3 cm
4.5 cm
6 cm
Figure 5.4: In-house multipoint turbidimeter used to track the net displacement of µE and
excess phase separation fronts at a high time resolution.
The τ(t) was calculated using this multipoint turbidimeter at the different heights as
follows28,29
:
112
tV
V
Lt
p
maxln1
(Eq. 7)
In this equation, Lp is the laser path length, V(t) is the voltage of the photodiode obtained
at a given time during the measurement, and Vmax is the maximum attainable voltage of the
photodiode in a transparent sample. In this case, the passage of a moving phase separation front
through a given set of laser-photodiode pairs was identified by a sharp decay in τ(t) to 0. The
data taken from the time-lapse images and multipoint τ(t) measurements were both used (for
validation purposes) to plot the normalized displacement of the moving µE and excess phase
separation fronts versus time as in Figure 5.3 (b). These graphs were then used to determine the
resulting ap, dp, and cp time periods.
5.4 RESULTS
5.4.1 Interfacial Tension and Average Emulsion Droplet Diameter
The baseline (0.1 M SDHS) γow profile at 25°C is presented in Figure 5.5 (a) as a
function of the HLD. The measured data, which follows the same trend as that observed for the
other µEs in Chapter 4, shows that an ultralow minimum is attained at HLD=0.
113
0.01
0.1
1
-1.5 -1 -0.5 0 0.5 1 1.5
γo
w(m
N/m
)
(a)
Type I Type III Type II
(μm)
HLD
(b)
0.1
1
10
-1.5 -1 -0.5 0 0.5 1 1.5
Type I Type III Type II
Figure 5.5: Measured (a) interfacial tension (γow) and (b) emulsion droplet diameter ( E
dd )
profiles for baseline (0.1 M SDHS) emulsions at 25°C.
The baseline (0.1 M SDHS) E
dd profile at 25°C in Figure 5.5 (b) is also presented as a
function of the HLD. It can be extrapolated from the data that E
dd tends to a minimum at
HLD=0. This trend is directly related to the changes in γow as a function of the HLD. The
relationship between E
dd and γow can be expressed based on the balance of hydrodynamic and
interfacial forces as discussed in Chapter 3 as follows:
ow
E
dd (Eq. 8)
It should be noted here that the reported E
dd are of the same order of magnitude as the
calculated number average droplet diameter. Furthermore, E
dd are not reported for emulsions in
the vicinity of the Type III region as their E
id could not accurately be measured.
dd
E (
µm
)
114
5.4.2 Emulsion Phase Separation Profiles and Time Periods
In Figure 5.6, ΔsµE(t) and Δsw(t) profiles versus time for a Type II baseline (0.1 M
SDHS) emulsion at HLD=0.9 and 25°C are presented along with sample time-lapse images that
show the real progression of the phase separation fronts.
0
0.2
0.4
0.6
0.8
1
0 1750 3500 5250 7000
y1 = 0.0008x1 - 1.46R² = 0.95
0
0.2
0.4
0.6
0.8
1
0 1750 3500 5250 7000
y2 = 0.0008x2 - 2.13R² = 0.96
0
0.2
0.4
0.6
0.8
1
0 1750 3500 5250 7000
0
0.2
0.4
0.6
0.8
1
ep
0
0.2
0.4
0.6
0.
8
1
0 1750 3500 5250 7000
cpdpap
Time (Seconds)Time
Images - ΔsμE(t)
Images - Δsw(t)
τ(t) - ΔsμE(t)
τ(t) - Δsw(t)
Linear Approximation - ΔsμE(t)
Linear Approximation - Δsw(t)
ΔsμE(t) (or Δs
w(t
))
Figure 5.6: Example of sample time-lapse images and ΔsµE(t) and Δsw(t) profiles versus time
for a Type II baseline (0.1 M SDHS) emulsion at HLD=0.9 and 25°C.
The ap time period is represented by the initial lag time before which the µE phase
separation front begins to advance. To calculate the duration of the ap time period, the advance
of the µE phase separation front is fitted to a linear equation that assumes a constant advance
rate. The intercept of this linear equation at ΔsµE(t)=0 corresponds to the ap time period. A
similar method is used to calculate the dp time period. What is different in this case, however, is
that the ap time period is subtracted from the intercept of this second linear equation at Δsw(t)=0.
The final cp time period is calculated by subtracting the ap and dp time periods from the time at
115
which the second linear equation intercepts Δsw(t)=1. An interesting feature of these phase
separation profiles, which is clearly illustrated in the accompanying time-lapse images, is that
the advance of the µE phase separation front does not leave behind a “clean” µE phase. Instead,
a small volume fraction of isolated emulsion droplets settles very slowly before eventually
coalescing. The impact of this phenomenon on the total time required to reach equilibrium (ep)
is ignored. The exact same approach applies to Type I emulsions (but for Δso(t) instead of
Δsw(t)). For Type III emulsions, where oil and water droplets co-exist, the dp time period is
allowed to span the time interval between the onset of ΔsµE(t) and the more stable emulsion
type. The cp time period is thereafter allowed to proceed until equilibrium is reached. At the
phase inversion point (i.e. HLD=0), no ap and dp time periods are observed as the coalescence of
oil and water emulsion droplets occurs instantaneously. The maximum calculated error between
the times estimated using the time-lapse images and multipoint turbidimeter is, on average,
15%.
Figure 5.7 presents the net rate of advance of the µE and excess phase separation fronts
as a function of the HLD for baseline (0.1 M SDHS) emulsions at 25°C. Overall, the net rate of
advance of both fronts tend to be similar and increase upon approaching the phase inversion
point at HLD=0. It should be noted that the net rate of advance of the µE and excess phase
separation fronts were not originally expected to be so similar. The fact that they are however so
similar may suggest some strong commonalities with respect to their rate-controlling separation
processes. Near the phase inversion point, the µE phase separation front advances faster than the
excess phase separation front. The net rate of advance of the phase separation fronts for Type III
emulsions are not included because these emulsions separate almost instantaneously.
116
0
0.1
0.2
0.3
-1.5 -1 -0.5 0 0.5 1 1.5
HLD
Net
Rate
of
Ad
van
ce (
mm
/s)
μE Phase Separation Front Excess Phase Separation Front
Type I Type III Type II
Figure 5.7: Net rate of advance of the µE and excess phase separation fronts as a function of the
HLD for baseline (0.1 M SDHS) emulsions at 25°C.
In Figures 5.8 (a)-(c), a compilation of the ap, dp, cp, and ep (ap+dp+cp) time periods is
presented as a function of the HLD at 0.01 M, 0.1 M, and 0.3 M SDHS and 25°C. In general, all
of these time periods tend to decrease upon approaching HLD=0. For emulsions at 0.01 M
SDHS, the overall stability is dominated by the cp time period whereas the ap time period
represents the smallest contribution. For emulsions at 0.1 M and 0.3 M SDHS, the ep time
periods, which are substantially larger than those obtained at 0.01 M SDHS, appear close.
However, the ap time period for Type I emulsions at 0.1 M SDHS, which is the major
contributor to their overall stability, is noticeably larger than those obtained at 0.3 M SDHS.
117
epcpdpap
1
10
100
1000
10000
100000
-1.5 -1 -0.5 0 0.5 1 1.5
Tim
e (
Seco
nd
s)
Type I Type III Type II(a)
1
10
100
1000
10000
100000
-1.5 -1 -0.5 0 0.5 1 1.5
Tim
e (
Seco
nd
s)
(b)
1
10
100
1000
10000
100000
-1.5 -1 -0.5 0 0.5 1 1.5
Tim
e (
Seco
nd
s)
(c)
HLD
Figure 5.8: Compiled ap, dp, cp, and ep (ap+dp+cp) time periods for emulsions at (a) 0.01 M, (b)
0.1 M, and (c) 0.3 M SDHS and 25°C.
5.4.3 Effect of Temperature on Emulsion Phase Separation Time Periods
The effect of T on the ap, dp, cp, and ep time periods is illustrated in Figures 5.9 (a)-(d) as
a function of the HLD for baseline (0.1 M SDHS) emulsions. All of these phase separation time
118
periods tend to decrease with an increase in T, but this decrease is more noticeable for
emulsions that are far from HLD=0. One point that deserves closer inspection is to compare the
effect of T on the ap time periods at HLD=-0.4 and HLD=0.4. At HLD=-0.4, the increase in T
produces a substantial decrease in the ap time period. At HLD=0.4, however, the ap time period
does not change very much with T and remains quite low. This finding suggests that, at least for
the ap time period, the morphology of the emulsion plays a role (particularly close to HLD=0).
1
10
100
1000
10000
100000
-1.5 -1 -0.5 0 0.5 1 1.5
1
10
100
1000
10000
100000
-1.5 -1 -0.5 0 0.5 1 1.5
1
10
100
1000
10000
100000
-1.5 -1 -0.5 0 0.5 1 1.5
(a) (b)
(c) (d)
Tim
e (
Se
co
nd
s)
Tim
e (
Se
co
nd
s)
Type I Type III Type II
epcpdpap
1
10
100
1000
10000
100000
-1.5 -1 -0.5 0 0.5 1 1.5
HLD HLD
Type I Type III Type II
Figure 5.9: Compiled ap, dp, cp, and ep (ap+dp+cp) time periods for baseline (0.1 M SDHS)
emulsions at (a) T=7°C, (b) T=15°C, (c) T=35°C, and (d) T=44°C.
119
In Figure 5.10 (a), an example of the Arrhenius-like relationship proposed by Kabalnov
et al. (Equation 1) to describe the emulsion phase separation time periods is shown versus 1/T
for baseline (0.1 M SDHS) emulsions at HLD=0.4.
DrainageAggregation Coalescence
(a) y = 1E-10e9141x
R² = 0.98
y = 3E-06e5648x
R² = 0.55
y = 2E-05e5391x
R² = 0.94
1
10
100
1000
10000
100000
0.003 0.0032 0.0034 0.0036 0.0038 0.004
Tim
e (
Se
co
nd
s)
1/T (1/K)
(b)
0
10
20
30
40
50
-1.5 -1 -0.5 0 0.5 1 1.5
HLD
W*(k
BT
)
Type I Type III Type II
Figure 5.10: (a) Sample W* fittings for the aggregation, drainage, and coalescence of Type I
baseline (0.1 M SDHS) emulsion at HLD=-1 and (b) their values as a function of the HLD at
298 K.
120
The exponential factors taken from these regressions are in turn used to calculate W* for
aggregation, drainage, and coalescence as presented in Figure 5.10 (b) in equivalent kBT units at
298 K and as a function of the HLD. From this figure, it appears that W* for all these time
periods tends to decrease, and reach a minimum, towards HLD=0. Although these W* are
consistent with previous observations regarding the stability of Type III emulsions close to
HLD=0, they are not in complete agreement with the modeled predictions of Kabalnov et al. for
Type I and Type II emulsions16,27
. These researchers suggested that W* is constant for Type I
and Type II emulsions. Another interesting feature in Figure 5.10 (b) is that W* for the
aggregation of Type I emulsions is considerably greater than that for their drainage and
coalescence. This finding is consistent with the previous observation in Figure 5.8 (b) that the ap
time period generally seems to control the separation of Type I emulsions. It is important to
keep in mind that although these values produce reasonable estimates for W* around the phase
inversion point, they do not reflect any changes in the pre-exponential factor f of Equation 1.
5.5 DISCUSSIONS
It was previously mentioned that the ap time period likely involves the aggregation of
emulsion droplets. To evaluate this possibility, one can assume that the Brownian motion of
emulsion droplets is what leads to the collisions responsible for this overall process. An estimate
for the experimental ap time period can thus be obtained from the characteristic diffusion time
(tdiff). To calculate tdiff, the characteristic diffusion length ( diffDtl 2 ) is taken together with
the Einstein-Stokes relation for the diffusivity of an emulsion droplet after mixing
(E
dE
B
d
TkD
3 ) and is in turn set proportional to E
dd as follows:
121
Tk
dt
B
E
dE
diff4
33
(Eq. 9)
The assumption of l being proportional to E
dd is believed to be valid as E
dE
d
dl 3
3
4
2
1
in
both dilute and concentrated emulsions (where E
d is the emulsion droplet volume fraction). In
Figure 5.11, the ap time period and tdiff are presented as a function of the experimental E
dd for
baseline (0.1 M SDHS) emulsions at 25°C (data taken from Figure 5.5 (b)).
y = 72.3x2.5
1
10
100
1000
10000
100000
0 2 4 6 8
d32 (μm)
ap
or
t dif
f(S
ec
on
ds
)
Figure 5.11: Dependence of the ap time period for baseline (0.1 M SDHS) emulsions at 25°C on
E
dd . The solid line represents the fit of tdiff from Equation 9 (R2=0.84).
Despite having neglected hydrodynamic interactions, the power correlation in Figure
5.11 presents a fitted exponent of 2.5. This fitted exponent is fairly close to the predicted value
ddE (µm)
122
of 3 in Equation 9. The dispersion in the data is pronounced at larger values of E
dd . For Type I
emulsions, the power correlation underpredicts the experimental ap time period by 2 orders of
magnitude. This observation suggests that the aggregation of Type I emulsions is perhaps
hindered at low electrolyte concentrations by repulsive electrostatic forces. Furthermore, it is
likely that these emulsion droplets must collide numerous times before they can form large
enough aggregates for settling and film thinning to continue the separation process. For Type II
emulsions, the power correlation only slightly overpredicts the experimental ap time period.
The additional likelihood of such growth in the emulsion droplet aggregate size over the
ap time period can be evaluated by calculating the apparent average emulsion droplet diameter
( E
appdd , ) at the onset of settling. This can be done with the aid of Stokes’ law as follows10,33
:
E
E
appdE
E
d
s
dgv
18
2
, (Eq. 10)
In this equation, vs is the settling rate, E
d is the density of the emulsified phase, and g is
the gravitational acceleration constant (9.81 m/s2). By taking the vs of baseline (0.1 M SDHS)
emulsion droplets at 25°C as the net rate of advance of the µE phase separation front (Figure
5.7), ηµE as 1 cP, and Δρ ( E
d -ρµE) as 65 kg/m3, E
appdd , is calculated as presented in Figure 5.12.
The Reynolds number associated with E
appdd , is on the order of 10-3
, which is consistent with the
use of Stokes’ law. One limitation of Stokes’ law is that it does not consider hindered settling. If
one were to consider this phenomenon by introducing the appropriate empirical correction factor
(e.g. (1- E
d )4.5
), even larger E
appdd , than those presented in Figure 5.12 would need to be
produced34
. The data of Figure 5.12 proves that the emulsion droplets formed upon mixing do
123
not settle on their own and that the aggregation of pre-coalesced emulsion droplets that takes
place over the ap time period is in fact a necessary prerequisite. These conclusions are consistent
with the observations of others35,36
.
1
10
100
1000
10000
100000
-1.5 -1 -0.5 0 0.5 1 1.5
HLD
Emulsion Droplet Diameter (μm)
Initial (Measured) Settling (Equation 10) Film Thinning (Equation 11)
Type I Type III Type II
Figure 5.12: Comparison of the originally measured E
dd for baseline (0.1 M SDHS) emulsion
droplets at 25°C after mixing and the estimated E
appdd , required for settling (Equation 10) and
film thinning (Equation 11) as a function of the HLD.
Any further growth in E
appdd , due to gravitationally-induced collisions occurring over the
dp time period can be calculated by considering the process of film thinning as follows37,38
:
223
3
13
4
ratioratioEc
HowH
ffR
t
dt
dt
(Eq. 11)
124
In this expression, which was derived by taking Reynolds’ equation together with the
Laplace pressure at the Plateau border (neglecting DLVO forces), -dtH/dt is the rate of film
thinning, tH is the film thickness, Rc (estimated as E
appdd , /2) is the radius of curvature at the
Plateau border, and fratio is the ratio between the radius of the circumference of contact between
emulsion droplets (or the radius of the film) and Rc. By considering a dodecahedron foam-like
structure, fratio=0.6. To estimate tH, a simple ratio of the volume of the continuous µE phase to
the total area of the originally formed emulsion droplets is calculated. An initial estimated range
for tH of 0.2-0.9 µm is calculated as a function of the HLD for baseline (0.1 M SDHS)
emulsions at 25°C. At these separation distances, the magnitude of the DLVO forces acting to
squeeze toluene and water emulsion droplets together is only 0.1%-1% of the total Laplace
pressure38
. An estimate for -dtH/dt is further calculated by taking a ratio between the flow rate of
the liberated µE phase (determined from Figure 5.7 as the net rate of advance of the µE phase
separation front) and the area of the originally formed emulsion droplets. Using Equation 11 and
all of the values listed above, Rc can be calculated as a function of the HLD. These values are
presented in Figure 5.12 as E
appdd , =2Rc. From this, the calculated E
appdd , appear substantially
larger than the values calculated based on vs in Equation 10 and are close to 2 orders of
magnitude larger than the originally measured E
dd in Figure 5.5 (b). According to Figure 5.12, a
foam-like structure should be formed at HLD=0.9 with a characteristic cell size of ~1 mm. As
can be observed from the series of pictures in Figure 5.6, such structures do become apparent in
the latter stages of film thinning.
To evaluate the hole nucleation theory of coalescence, W* for baseline (0.1 M SDHS)
emulsions at 25°C (or 298 K) in Figure 5.10 (b) are plotted as a function of γow in Figure 5.13.
125
0
10
20
30
40
50
0 0.2 0.4 0.6 0.8 1
W*(k
BT
)
γow (mN/m)
DrainageAggregation Coalescence
HLD=-0.4
HLD=-0.7
Figure 5.13: General correlation between all of the fitted W* and the measured γow for baseline
(0.1 M SDHS) emulsions at 25°C.
The data in Figure 5.13 suggests that the apparent activation energy, W*, for drainage
and coalescence increases linearly with increasing γow as predicted by the hole nucleation
theory. This suggests that coalescence plays an important role in controlling these phase
separation time periods. If coalescence is the rate limiting process for the dp and cp time periods,
this would be consistent with the fact that the rate of advance of the µE and excess phase
separation fronts is almost the same. On the other hand, W* for aggregation deviates from the
linear trend predicted by the hole nucleation theory for Type I emulsions at intermediate
HLDs<0. This deviation is not surprising as the ap time period seems to be more or less
controlled by the previously described Brownian collisions. The larger W* for aggregation at
HLD<0 suggests that electrostatic forces strongly oppose the formation of flocs.
126
The emulsion phase separation studies carried out at 0.01 M SDHS and 25°C provide
some insight into the effect of the surfactant concentration. One of those effects is that reducing
the surfactant concentration from 0.1 M to 0.01 M SDHS reduces the ap time period by more
than 1 order of magnitude at the HLD extremes. It is unlikely that the presence of surfactant
would modify the frequency of emulsion droplet collisions as ηµE is almost the same. Also, γow
at these surfactant concentrations should be the same since they both lie above the critical µE
concentration (cµc) of 8 mM for SDHS-toluene-water µEs32
. Therefore, according to Equation
8, E
dd at both surfactant concentrations should be the same. The difference in the final emulsion
stability results is likely associated with the probability of these Brownian collisions leading to
the formation of flocs. At a higher surfactant concentration, more µE droplets are present in the
film that separates emulsion droplets. In squeezing out this inter-droplet film to allow for
coalescence to take place, depletion-repulsion interactions result from the increase in the
osmotic pressure associated with the overlap of structured µE droplet zones25
. The magnitude of
these interactions is presented in Chapter 7.
In comparing the emulsion phase separation time periods at 0.1 M and 0.3 M SDHS and
25°C (Figure 5.8), the ap and ep time periods appear to slightly decrease with an increase in the
surfactant concentration for Type I emulsions. This suggests that Ostwald ripening may play a
role in helping for these emulsion droplets to grow and more quickly assemble into an aggregate
size at which subsequent drainage can occur. It is expected that the prolonged dp time period
observed at an increased surfactant concentration for these same emulsions is a result of the
increased number of metastable µE layers that need to be expelled during film thinning. The
contributions of an increased ηµE leading to a decreased vs should be minimal.
127
5.6 CONCLUSIONS
The objective of this chapter was to study and describe how the stability of emulsions
prepared with an anionic surfactant (sodium dihexyl sulfosuccinate, SDHS), oil (toluene), and
water change around the phase inversion point of corresponding microemulsions (µEs). To do
so, emulsion phase separation profiles were described in terms of aggregation (ap), drainage
(settling + film thinning) (dp), and coalescence (cp) time periods. These phase separation time
periods were assessed as a function of the hydrophilic-lipophilic deviation (HLD). Here, the
phase inversion point lies at HLD=0. At a low surfactant concentration (0.01 M SDHS), the cp
time period dominated for oil (HLD<0) and water (HLD>0) emulsion droplets. At larger
surfactant concentrations, the ap time period dominated at HLD<0 whereas all of the time
periods were more comparable at HLD>0. The ap time period seemed to be controlled by the
frequency of Brownian collisions that effectively led to the formation of aggregated flocs of
larger emulsion droplets. The frequency of these underlying Brownian collisions was hindered
by the presence of µE droplets in the emulsion’s continuous phase. The dp and cp time periods
seemed to be controlled to a greater extent by the coalescence of neighboring emulsion droplets.
The apparent activation energies (W*) associated with these latter phase separation time periods
was proportional to the oil-water interfacial tension, suggesting that they can be explained by
the hole nucleation theory for emulsion coalescence.
This work illustrates the amount of information that can be obtained from relatively
simple phase separation studies, as well as the risks of oversimplifying the interpretation of the
data by just using a single equation (e.g. settling velocity). Having differentiated the stability
analysis of emulsions according to their different phase separation time periods and associated
W* further opens the possibility for a more detailed modeling of these processes.
128
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133
CHAPTER 6:
PREDICTING THE MORPHOLOGY AND VISCOSITY OF
MICROEMULSIONS USING THE NAC MODEL
This chapter is derived from the following published manuscript:
Kiran, S.K.; Acosta, E.J. Predicting the Morphology and Viscosity of Microemulsions using the
HLD-NAC Model. Ind. Eng. Chem. Res. 2010, 49, 3424-3432.
134
6.1 ABSTRACT
This chapter focused on extending the net-average curvature (NAC) model to help
predict the shape and viscosity (ηµE) of anionic surfactant (sodium dihexyl sulfosuccinate
(SDHS))-oil (toluene)-water microemulsions (µEs) from readily available formulation
parameters. To do so, a new shape-based NAC model was introduced which related the net and
average curvatures to the length and radius of µE droplets possessing a hypothesized cylindrical
core with hemispherical end caps. Knowing the shape of these µE droplets, theoretical scattering
profiles and maximum hydrodynamic radii were predicted. Furthermore, considering the
predicted volume fraction of the dispersed µE droplets alongside their shape allowed for the
accurate prediction of ηµE. It was found that treating the µE phase as a dilute suspension of rigid
rods yielded predicted ηµE close to experimental values near the bicontinuous phase transition
limits. These correlations were further extended to published experimental ηµE data of non-ionic
surfactant systems. The predicted µE morphology and ηµE may be useful in the design of
formulations for nanoparticle synthesis, enhanced oil recovery, and various environmental
remediation technologies.
6.2 INTRODUCTION
As has been highlighted in earlier chapters, there are three basic microemulsion (µE)
types: oil-in-water (o/w) µEs in equilibrium with an excess oil phase (Type I), bicontinuous µEs
in equilibrium with excess oil and aqueous phases (Type III), and water-in-oil (w/o) µEs in
equilibrium with an excess aqueous phase (Type II). Various researchers have experimentally
demonstrated that the length to radius ratio of µE droplets varies significantly according to
formulation conditions1,2,3,4,5
. The resulting changes in µE droplet shape and size, which arise
135
from underlying changes to the surfactant packing at the interface, have a profound effect on the
manufacturing of nanoparticles, latexes, and other nanostructured fluids6,7
. Another important
property of µEs is their viscosity (ηµE). As was previously noted by Trickett et al., ηµE ranges
from a fluid-like state to a solid-like gel8. Examples of instances where ηµE is an important
parameter to consider, and control, include in soil remediation, oil recovery, alternative fuels,
and hydraulic fluids9,10
.
The size of µE droplets has been estimated by Eastoe and others from the ratio of the
dispersed phase to the mass of the surfactant11,12,13
. Furthermore, Acosta et al. have predicted the
size of µE droplets using the inverse of their sphere-equivalent radius of curvature as calculated
from the net-average curvature (NAC) model14,15
. While there are a number of theoretical
equations dedicated to explaining the shape and changes in shape of µE droplets, thus far there
are no theoretical or empirical equations that can predict the shape of µE droplets from
formulation conditions (e.g. type of surfactant and oil, electrolyte concentration, and
temperature) 16,17,18,19,20,21,22,23,24,25,26
. The first objective of this chapter is to extend the NAC
model to predict the shape of Type I and Type II µE droplets. The predicted shape will be used
to generate theoretical small angle neutron scattering (SANS) profiles that will be compared to
experimental scattering profiles. Furthermore, the predicted shape will also be used to estimate
the maximum hydrodynamic radius of µE droplets. The second objective of this chapter is to
use the predicted volume fraction ( E
d
) and shape of µE droplets to estimate ηµE.
Numerous correlations have been established by several researchers to help predict ηµE.
Einstein first developed the following model for the dilute dispersion of hard spheres within a
liquid medium9:
136
E
d
E
cE
5.21 (Eq. 1)
In this equation, E
c
is the viscosity of the µE’s continuous phase. An extension of this
model was later proposed by Taylor et al. for the dilute suspension of liquid spheres within a
reference continuous phase9,27
:
E
d
E
c
E
d
E
cE
d
E
cE
5.21 (Eq. 2)
In Equation 2, E
d
represents the viscosity of the µE’s dispersed phase. For the hard-
sphere scenario where E
d
>> E
c
, Taylor’s model simplifies to that of Einstein. To describe ηµE
under more concentrated regimes ( E
d
>0.02), Saito et al. derived the following expression by
considering the hydrodynamic interactions between non-correlated spheres9,28
:
E
d
E
dE
cE
1
5.11 (Eq. 3)
A shortcoming of Equation 3 is that it does a poor job of replicating experimental ηµE
peaks at the maximum packing condition of dispersed droplets. This was corrected for in the
Dougherty-Krieger relationship as follows9,29,30
:
Ed
E
d
E
dE
cE
max,5.2
max,
1
(Eq. 4)
In Equation 4, E
d
max, reflects the maximum volume fraction of rigid dispersed spheres,
which ranges from 0.6 to 0.7 according to the shear rate31
. In addition to Equations 1-4, Thomas
137
et al. established an empirical expression for predicting the ηµE of concentrated µEs by
expanding Einstein’s model to higher orders of E
d
9,32:
E
d
E
d
E
d
E
cE
6.16exp00273.005.105.21
2 (Eq. 5)
A key assumption in the derivation of Equations 1-5 is that the shape of the dispersed µE
droplets is spherical. As was previously described, however, cylindrical and elliptical µE
droplets are also common. Doi and Edwards treated the case for a dilute and semi-dilute
concentration of rigid rods by taking into account their rotary diffusion in Equations 6 and 7
respectively9,33
:
E
E
rods
E
rodsgE
c
E
rods
E
cE
d
lclN
2
2
3 411 , where
31
E
rodslN
(Eq. 6)
E
rods
E
rodsE
rodsE
E
rodsgE
cE
d
ld
lc
ln5
96
632
63
, where 23
11
E
rods
E
rods
E
rods ldN
l (Eq. 7)
In these equations, N is the number density of rigid µE rods, E
rodsl and E
rodsd are their
respective length and diameter, cg is their concentration in mass per unit volume, and E is the
density of the µE phase. Similar correlations have yet to be developed for liquid rods.
Additional models for µEs consisting of prolate and oblate ellipsoids as the dispersed phase are
as in Equations 8 and 9 respectively9,34
:
138
15
14
5.12
ln155.02
ln5
1
22
E
ell
E
ell
E
ell
E
ell
E
ell
E
ell
E
ell
E
ell
E
d
E
cE
b
a
b
a
b
a
b
a
(Eq. 8)
E
ell
E
ell
E
ell
E
ell
E
d
E
cE
b
a
b
a
arctan
15
16
1 (Eq. 9)
Equations 8 and 9 are applicable when the ratio of the ellipsoid’s major axis ( E
ella ) to
minor axis ( E
ellb ) is greater than 10.
The E
d
and shape of the dispersed µE droplets predicted by the NAC model will be
incorporated into Equations 1-9 to predict the ηµE of Type I and Type II anionic surfactant
(sodium dihexyl sulfosuccinate (SDHS))-oil (toluene)-water µEs. The predicted ηµE will be
compared to experimental results obtained for similar µEs.
The NAC model allows for the prediction of µE properties (e.g. solubilization capacity,
phase volumes, phase transitions, and interfacial tensions) as a function of thermodynamic
formulation parameters (e.g. electrolyte concentration, temperature, and oil and surfactant
hydrophobicity)14,15
. A key element of this model is the calculation of the hydrophilic-lipophilic
deviation (HLD). As was previously described in earlier chapters, the HLD for ionic surfactants
can be expressed as follows:
coc CTAfNSHLD 01.017.0ln , (Eq. 10)
139
In this equation, S is the electrolyte concentration, Nc,o is the equivalent alkane carbon
number, f(A) is a function of the co-surfactant type and concentration, ΔT is the temperature
deviation from 25°C, and Cc is the characteristic curvature of the ionic surfactant. The HLD
equation for non-ionic surfactants differs ever so slightly15,35
:
noc CTANSbHLD 06.017.0 , (Eq. 11)
In this equation, b(S) accounts for the “salting” out of the non-ionic surfactant. Published
values of b include 0.1 for CaCl2 and 0.13 for NaCl. Also, ϕ(A) represents the effect of alcohol
(co-surfactant) and Cn is the characteristic curvature of the non-ionic surfactant. For both
Equations 10 and 11, a HLD<0HLD=0HLD>0 scan reflects a Type IType IIIType II
µE phase behavior transition.
To obtain the desired physical properties of µEs, the HLD is included within the NAC
model as a scaling parameter for the net curvature (Hn) of the surfactant film at the oil-water
interface14,15
:
L
HLD
rrH
E
w
E
o
n
11 (Eq. 12)
In Equation 12, E
or and E
wr are the sphere-equivalent radii of hypothetically co-existing
oil and water µE droplets whereas L is a length scaling parameter that is proportional to the
extended length of the surfactant tail (~1.2 times). Hn is 0 for bicontinuous (Type III) µEs
containing similar amounts of oil and water ( E
or = E
wr ), >0 for Type I µEs ( E
or << E
wr ), and <0
for Type II µEs ( E
or >> E
wr ). The average curvature term (Ha) in the NAC model is used to
describe the size of the µE’s oil and water domains14,15
:
140
111
2
1
E
w
E
o
arr
H (Eq. 13)
The inequality on the right-hand size of Equation 13 suggests that the size of µE droplets
is limited by their characteristic length (), a concept that was previously introduced by De
Gennes et al.36
. These authors demonstrated that this parameter, which represents the distance at
which an oil or water molecule can be separated from a surfactant membrane and still interact
with it, is calculated as follows14,15,36
:
s
E
E
w
E
o
A
V
6
(Eq. 14)
Here, E
o
and E
w
are the respective oil and water volume fractions within the µE phase
of volume EV . At HLD=0, is a maximum and serves as a benchmark for the transition to a
bicontinuous µE.
6.3 DEVELOPMENT OF EXPRESSIONS FOR THE SHAPE-BASED
NAC MODEL AND MAXIMUM HYDRODYNAMIC RADIUS
To predict the shape of Type I and Type II µE droplets, it is assumed that these droplets
have a cylindrical neck region of length E
dl with hemispherical end caps of radius E
dr . In this
way, a smooth transition from spheres ( E
dl =0) to rods ( E
dl >> E
dr ) can be obtained. The total
integrated curvature of these droplets at the oil-water interface is equivalent to the surface area-
averaged curvature (CSA,avg) whereby the curvature of the cylindrical neck region is 1/2 E
dr and
the curvature of the hemispherical end caps is 1/ E
dr :
141
AreaSurfaceTotal
HemisphereofAreaSurfacer
CylinderofAreaSurfacer
C
E
d
E
d
avgSA
12
2
1
, (Eq. 15)
As demonstrated in Appendix 1, a new revised net curvature term ( '
nH ) is a reasonable
approximation of the sphere-equivalent curvature of these droplets. Incorporating this parameter
within Equation 15 yields the following expression in terms of E
dr and E
dl :
E
d
E
d
E
d
E
d
E
d
E
d
n
nrlr
l
rl
HH
42
1
2
2
2
'
(Eq. 16)
Using neutron scattering data, it has been shown that Ha represents the sphere-equivalent
surface area to volume ratio of µE droplets37
. Ha can therefore be related to E
dr and E
dl as
follows:
243
42
E
d
E
d
E
d
E
d
E
da
rrl
rlH
(Eq. 17)
Obtaining Hn (and thus '
nH ) and Ha from the original NAC model, the shape of the µE
droplets can be determined by simultaneously solving Equations 16 and 17 for E
dr and E
dl .
Furthermore, these solved values of E
dr and E
dl , as well as the surfactant tail length (δtail), can
be used to estimate the maximum hydrodynamic radius of rigid µE droplets ( E
hr
max, ) as follows:
tail
E
dE
d
E
h
lrr
2max, (Eq. 18)
The actual hydrodynamic radius ( E
hr ) is only equal to the calculated
E
hr
max, for rigid and
fully extended µE droplets. Droplets demonstrating an experimental E
hr smaller than
E
hr
max, (as
142
determined via light scattering) are flexible. Such types of light scattering experiments have
been performed in the past to assess the flexibility of sodium dodecyl sulfate (SDS) micelles38
.
6.4 MATERIALS AND METHODS
6.4.1 Materials
The following materials were used as purchased from Sigma-Aldrich Corp. (Oakville,
ON, Canada): anhydrous toluene (product #244511, 99.8%), SDHS (product #86146, ~80% in
water), and NaCl (product #S9625, ≥99.5%). Acetonitrile (product #1401-7-10, HPLC grade)
was obtained from Caledon Laboratory Chemicals (Georgetown, ON, Canada) and deionized
water (conductivity <3 µs/cm) was prepared in the laboratory using an anion exchange resin.
6.4.2 Microemulsion Phase Behavior Scans
A series of SDHS-toluene-water µE phase behavior scans at a SDHS concentration of
0.1 M and 1-10 g/100 mL NaCl in the aqueous phase was prepared according to the procedure
outlined in Chapter 5.
6.4.3 Oil-Water Solubilization
Solubilization of toluene in water was measured experimentally using a Dionex 3000
ionic chromatographic system equipped with a C18 column. The mobile phase, which consisted
of water and acetonitrile in a 55 to 45 volume ratio, was pumped through the column at a flow
rate of 1 mL/min. An AD25 absorbance detector was used to detect toluene at a wavelength of
220 nm. Water solubilization in the oil phase was measured using a Kam Control Inc. Karl
Fischer moisture analyzer.
143
6.4.4 Viscosity Measurements
A Gilmont Instruments falling ball viscometer (model #GV-2200) was used in order to
target ηµE measurements <10 cp. The vertical glass tube apparatus was first filled with ~4.5 mL
of the µE sample of interest. Once filled, a glass ball of diameter 0.6 cm was released within the
tube and its time of descent (td, in minutes) between two sets of red reference markings was
measured using a stopwatch. A glass ball was used here as opposed to a heavier stainless steel
ball in order to reduce the shear rate ( ) and minimize the possible risk of shear-thinning
behavior reported by Bennett et al.39
. The maximum applied was limited to 0.1 seconds-1
. For
each sample, triplicate measurements were performed. The ηµE was subsequently calculated in
units of centipoise (cP) by taking into consideration the density of the glass ball (2.53 g/mL), the
density of the µE phase (ρµE, in g/mL), and the viscometer constant (3.3):
EdE t 53.23.3 (Eq. 19)
6.4.5 Dynamic Light Scattering
Dynamic light scattering (DLS) measurements were performed at 25°C using a
Brookhaven Instruments Corp. 90Plus Particle Size Analyzer. This instrument is equipped with
a 15 mW solid state laser (wavelength of 635 nm) and a detector positioned at a scattering angle
of 90° with respect to the incident light beam. To operate, standard glass cuvettes were filled
with the µE samples 15 minutes prior to being inserted within the sample chamber for
analysis40
. Droplet sizes were measured on the basis of decay times of fluctuating intensity
readings. Reference viscosities and refractive indices are provided in Table 6.1.
144
Table 6.1: Reference viscosities () and refractive indices (n).
Parameter Value
water (25°C) 0.89 cP41
toluene (25°C) 0.56 cP42
nwater (25°C) 1.3343
ntoluene (25°C) 1.4944
6.4.6 Prediction of Oil and Water Solubilization with the NAC Model
To calculate Hn for Type I (Type II) µEs, a fictitious sphere-equivalent radius of the
continuous aqueous (oil) phase ( E
IIIowr
, ) was first calculated as follows14,15
:
s
E
IIIowE
IIIowA
Vr
,
,
3 (Eq. 20)
si
E
wsis aVcA 231002.6 (Eq. 21)
In Equations 20 and 21, E
IIIowV , represents the continuous volume of water (oil) within
the Type I (Type II) µE phase, As is the total surfactant interfacial area, and csi and ai represent
the concentration and surface area per molecule of surfactant or co-surfactant species i pre-
dissolved within the aqueous phase. Here, the critical micelle concentration (cmc) of non-
adsorbed surfactant is neglected since the total surfactant concentration is more than 1 order of
magnitude larger14,15
. By establishing E
IIIowV , and csi as experimental constants and using
literature values for ai, E
IIIowr
, was calculated as per Equations 20 and 21. Knowing this
parameter as well as L, and having calculated the HLD using either Equation 10 or 11, the
sphere-equivalent radius of the dispersed oil (E
Ior
, ) and water (E
IIwr
, ) droplets for Type I and
Type II µEs were respectively estimated through the use of Equation 12. The volumes of oil
(E
IoV , ) and water (
E
IIwV , ) solubilized within the µE phase were respectively solved for by subbing
145
E
Ior, and E
IIwr
, back into Equation 20. For Type III µEs, Ha=1/ and Equations 12 and 13 were
solved simultaneously for E
IIIor, and E
IIIwr, . Oil and water solubilization for SDHS-toluene-water
µEs across a Type IType IIIType II phase behavior scan was determined from the list of
HLD and NAC modeling parameters in Table 6.2.
Table 6.2: HLD and NAC modeling parameters for SDHS-toluene-water µEs.
Parameter Value
S (g/100 mL) 1-10 g/100 mL
Nc,o 1
f(A) 0
∆T 0
Cc -0.92
L (Å) 10 Å14,37
E
IIIowV , (mL) 5 mL
csi 0.1 mol/L
ai 100 Å2/molecule
14
(HLD≈0) 68 Å37
This same approach was used to calculate E
Ior
, and E
IoV , for Type I µEs of the non-ionic
surfactant (C12E4)-oil (hexadecane)-water and non-ionic surfactant (C12E5)-oil (cyclohexane and
hexadecane in a 1 to 1 weight ratio)-water systems studied by Leaver and Olsson28
. The list of
HLD and NAC modeling parameters for these µEs is summarized in Table 6.3.
Table 6.3: HLD and NAC modeling parameters for the non-ionic µEs of Leaver and Olsson28
.
Parameter C12E4-Hexadecane-Water C12E5-Cyclohexane and Hexadecane-Water
S (g/100 mL) 0 0
Nc,o 1615,45
9
ϕ(A) 0 0
∆T (-8) to (+2) (-5) to (+3)
Cn 1.815
0.815,46
L (Å) 2515
2515
E
IwV , (mL) 73 83
csi (M) 0.4 0.2
ai (Å2/molecule) 54
15 60
15
146
From the above calculations for the different µEs of interest, E
dr and E
dl were
calculated. These values were then used to predict ηµE.
6.4.7 Prediction of Small Angle Neutron Scattering Profiles
The small angle neutron scattering (SANS) profiles of cylindrical droplets with
hemispherical end caps were predicted by incorporating the NAC model within the theoretical
profile developed by Cusack et al.47,48
:
2/
0
2 sin
dqAqI E
d (Eq. 22)
In this equation, I(q) is the scattering intensity, q is the scattering vector, θ is the
scattering angle, and A(q) represents the scattering amplitude defined by:
1
0
3
3
312)(sin4
)cos()sin(cos4
sin
sin2sindttfXr
qr
qrqrqrXr
qr
qrJ
X
Xlr
b
qA E
dE
d
E
d
E
d
E
dE
dE
d
E
dE
d
E
d
(Eq. 23)
In Equation 23, X=sin(q( E
dl /2)cosθ), f(t)=(1-t
2)sin(q E
dr tcosθ)[J1(q
E
dr sinθ(1-
t2)0.5
)]/(q E
dr sinθ(1-t
2)0.5
), and Δb is the difference in the scattering length density between the
µE’s dispersed and continuous phases.
For both the Type I and Type II SDHS-toluene-water µEs, scattering profiles were
generated by predicting E
dr and E
dl using Equations 16 and 17. The predicted profiles were
then compared to experimental scattering profiles obtained from Acosta et al. for similar
systems37
. For Type I scattering profiles, which were obtained using deuterated toluene
solubilized in the micelles, Δb=4.8×10-6
Ǻ-2
. For Type II µEs, deuterated water was solubilized
in the reverse micelles and Δb=5.4×10-6
Ǻ-2
.
147
6.5 RESULTS AND DISCUSSIONS
6.5.1 Comparison of Spherical Viscosity Models and Experimental
Measurements
As was previously described, predicting ηµE for µEs composed of spherical droplets
requires the knowledge of E
d
. Figures 6.1 (a) and (b) present the experimental and predicted
E
IoV , and E
IIwV , as well as E
d
as a function of the HLD. This data suggests that the experimental
and predicted data are in good agreement. Similar agreements have been reported in the past for
other ionic and non-ionic surfactant µEs2,14,15
.
0
0.5
1
1.5
-1.5 -1 -0.5 0 0.5 1 1.5
HLD
(b)(a)
0
0.2
0.4
0.6
0.8
1
-1.5 -1 -0.5 0 0.5 1 1.5
0
0.5
1
1.5
-1.5 -1 -0.5 0 0.5 1 1.5
Y-Values
Column1
Column3(mL
)
HLD
(b)(a)
0
0.2
0.4
0.6
0.8
1
-1.5 -1 -0.5 0 0.5 1 1.5
Y-Values
Column1
Column3NAC Model
NAC Model
E
d
E
d
(Oil)
(Water)
0
0.5
1
1.5
-1.5 -1 -0.5 0 0.5 1 1.5
Y-Values
Column1
Column3(mL
)
HLD
(b)(a)
0
0.2
0.4
0.6
0.8
1
-1.5 -1 -0.5 0 0.5 1 1.5
Y-Values
Column1
Column3NAC Model
NAC Model
E
d
E
d
(Oil)
(Water)
0
0.5
1
1.5
-1.5 -1 -0.5 0 0.5 1 1.5
Y-Values
Column1
Column3(mL
)
HLD
(b)(a)
0
0.2
0.4
0.6
0.8
1
-1.5 -1 -0.5 0 0.5 1 1.5
Y-Values
Column1
Column3NAC Model
NAC Model
E
d
E
d
(Oil)
(Water)
0
0.5
1
1.5
-1.5 -1 -0.5 0 0.5 1 1.5
Y-Values
Column1
Column3(mL
)
HLD
(b)(a)
0
0.2
0.4
0.6
0.8
1
-1.5 -1 -0.5 0 0.5 1 1.5
Y-Values
Column1
Column3NAC Model
NAC Model
E
d
E
d
(Oil)
(Water)
Figure 6.1: Experimental and predicted (a) E
IoV , and E
IIwV , as well as (b) E
d
as a function of the
HLD for SDHS-toluene-water µEs.
The ηµE can be calculated by substituting the predicted E
d
, in addition to the volume
fraction of surfactant, as well as E
c
(from Table 6.1) into Equations 1-5. Figure 6.2 presents
148
the measured E
c
along with the values predicted using Equations 2 (for dilute liquid spheres)
and 3 (for concentrated hard spheres). The values predicted using Equations 1, 4, and 5 all fall in
between the calculated ηµE using Equations 2 and 3. When compared to the experimental data, it
is apparent that away from the Type I-Type III and Type II-Type III transitions (HLD<-0.5 and
HLD>0.5 respectively) is where the predicted ηµE assuming spherical droplets is most
reasonable. The predicted ηµE are however substantially lower than the measured values in the
transition regions. The inaccuracy of these spherical droplet models near the transition regions
has been reported before9. It has been proposed that the ηµE models for spherical droplets fail as
they severely underestimate the interaction amongst rod-like µE droplets.
1
2
ηµ
E (
cP)
5
0.5
-1.5 -1 -0.5 0 0.5 1 1.5
Experimental
Dilute liquid
spheres (Eq. 2)
Concentrated hard
spheres (Eq. 3)
Figure 6.2: Experimental and NAC modeled (for dilute liquid spheres (Equation 2) and
concentrated hard spheres (Equation 3)) ηµE of SDHS-toluene-water µEs as a function of the
HLD.
The new shape-based NAC model can potentially resolve this issue since the predicted
E
dr and E
dl of the µE droplets can be used to calculate the ηµE of non-spherical droplets. The
149
E
dr and E
dl as well as the total aspect ratio ( E
dl /2 E
dr ) of SDHS-toluene-water µE droplets as
predicted by the NAC model are displayed in Figures 6.3 (a) and (b) as a function of the HLD.
Consistent with the trends predicted by conceptual models, and previous experimental
observations, E
dl of the µE droplets increases upon transitioning into the bicontinuous
region19,26
. Such elongated structures demonstrate enhanced interactions via overlapping which
results in quasi-stable clusters of droplets49,50
. Predictions of ηµE for bicontinuous µEs will be
omitted here as their complex interconnected structural network is not yet well understood and
falls outside the scope of this chapter.
(Å)
Asp
ect
Ra
tio
HLD
(b)(a)
Rd
Ld
(NAC Model)
(NAC Model)
0
3
6
9
12
15
-1.5 -1 -0.5 0 0.5 1 1.5
Figure 6.3: Predicted (a) E
dr and E
dl as well as (b) aspect ratio ( E
dl / E
dr ) as a function of the
HLD for SDHS-toluene-water µEs using the NAC model.
150
6.5.2 Comparison of Predicted and Experimental SANS Profiles for Type I and
Type II Microemulsions
The predicted values of E
dr and E
dl in Figure 6.3 are used to generate theoretical SANS
profiles for Type I and Type II µE droplets assuming a polydispersity value of 0.3 for E
dr ,
consistent with the average polydispersity obtained in DLS experiments. At a low electrolyte
concentration (1.2 g/100 mL NaCl where HLD=-0.9), Figure 6.4 (a) shows that the predicted
scattering curves have a transitional feature (related to E
dr ) at high q values (~0.15Å
-1), but that
transitional feature is observed at lower q values (~0.07Å-1
) in the experimental profile. From
this observation, one infers that the µE droplets are more spherical than cylindrical at low
electrolyte concentrations and that the NAC model underestimates their size. This
underestimation of the size of µE droplets at such a low electrolyte has been observed before37
.
Such deviation has been explained by the fact that the simple NAC model discussed here only
accounts for solubilization in the core of the micelles and not in their palisade layer. Aromatic
oils like toluene also solubilize in the palisade layer of the micelles, a phenomenon that has been
reproduced using a modified form of the NAC model51
.
151
0.01
0.1
1
10
100
0.01 0.1 1
0.01
0.1
1
10
100
0.01 0.1 1
0.01
0.1
1
10
100
0.01 0.1 1
0.01
0.1
1
10
100
0.01 0.1 1
0.01
0.1
1
10
100
0.01 0.1 1
0.01
0.1
1
10
100
0.01 0.1 1
q, Å-1
I(q
), c
m-1
(c)
q, Å-1
I(q
), c
m-1
I(q
), c
m-1
(b)
(a) (d)
(e)
(f)
1.2 g NaCl/100 ml
1.7 g NaCl/100 ml
2.0 g NaCl/100 ml
3.8 g NaCl/100 ml
4.3 g NaCl/100 ml
5.5 g NaCl/100 ml
Figure 6.4: Predicted SANS profiles of SDHS-toluene-water µEs formulated at (a) HLD=-0.9,
(b) HLD=-0.6, (c) HLD=-0.4, (d) HLD=0.3, (e) HLD=0.4, and (f) HLD=0.6 using the NAC
model.
As the electrolyte concentration increases, solubilization in the micelle core increases
and the scattering profiles predicted by the NAC model match more closely the experimental
scattering profiles, as shown in Figures 6.4 (b)-(c). For Type II µEs (Figures 6.4 (d)-(f)), the
predicted scattering profiles also produce a reasonable match with the experimental trends. The
good agreement between the predicted and experimental profiles supports the assumption and
approximations made in the new shape-based NAC model.
152
6.5.3 Comparison of Maximum Predicted and Experimental Hydrodynamic Radii
Values of E
hr
max, predicted via Equation 18 as well as experimentally measured E
hr using
DLS are plotted in Figure 6.5 as a function of the HLD. Although the predicted and
experimental trends are similar for Type I µEs, E
hr
max, consistently appears slightly larger than
the measured values. This indicates that the dispersed droplets are flexible as they do not fully
reach the maximum extended length. For Type II µEs, however, the predicted E
hr
max, more
closely traces the experimental data, suggesting that these cylinder-like droplets are able to
better maintain their shape as they randomly move throughout the continuous oil phase.
1
-1.5 -1 -0.5 0 0.5 1 1.5
(n
m)
Type I (Experimental)
Type II (Experimental)
NAC Model
Figure 6.5: Experimental E
hr and predicted
E
hr
max, for Type I and Type II SDHS-toluene-water
µEs as a function of the HLD.
153
6.5.4 Comparison of Non-Spherical Viscosity Models and Experimental
Measurements
The ηµE of elongated µE droplets can be calculated by incorporating the predicted E
d
in
Figure 6.1, the volume fraction of the surfactant, and the predicted E
dr and E
dl in Figure 6.3
into Equations 6-9. Figure 6.6 presents the same experimentally measured ηµE previously
presented in Figure 6.2 along with the predicted ηµE using Equations 6 (for dilute rigid rods) and
8 (for prolate ellipsoids). The values of ηµE predicted using Equation 7 (for semi-dilute rigid
rods) are substantially lower than the measured ηµE values for µEs away from the transition
regions and higher than the measured ηµE values near the transition regions. Equation 9 (for
oblate ellipsoids) produces ηµE values that are similar to those predicted for prolate ellipsoids. In
comparing Figures 6.2 and 6.6, it is shown that modeling the ηµE of SDHS-toluene-water µEs as
non-spherical droplets yields a closer approximation to the experimental data near the Type I-
Type III and Type II-Type III transition regions. Away from these transition regions, the
spherical models work best. Of the non-spherical models, that for dilute rigid rods is the most
accurate. This observation is believed to be a result of the fact that the condition N<1/ 3E
dl is
satisfied across all HLD values.
154
1
2
1.5 1 0.5 0 -0.5 -1 -1.5
5
ηµ
E (
cP
)
Experimental
Dilute rigid rods (Eq. 6)
Prolate ellipsoids (Eq. 8)
Figure 6.6: Experimental and NAC modeled (for dilute rigid rods (Equation 6) and prolate
ellipsoids (Equation 8)) ηµE of SDHS-toluene-water µEs as a function of the HLD.
The NAC model is also applied to the non-ionic µEs of Leaver and Olsson28
. For the
C12E4-hexadecane-water µEs, the NAC model predicts that the oil-swollen micelles take on the
shape of rods at 16°C and that these rods continuously lengthen with temperature. Figure 6.7 (a)
presents the resulting experimental viscosities for these µEs (plotted as a ratio of E / E
c
)
along with the predicted values obtained by applying the NAC model to dilute hard spheres
(Equation 1) and dilute rigid rods (Equation 6). Similar to the case for Type I SDHS-toluene-
water µEs, the dilute hard-sphere model greatly underestimates the experimental E / E
c
ratio
of these non-ionic µEs over 17-21°C where the maximum increase in E
d
is only 0.05. The
dilute rigid rods model produces a closer match with the experimental values. Using the semi-
dilute rigid rods model produces an overestimation of the E / E
c
ratio. An interesting feature
of Figure 6.7 (a) is the presence of an experimental E / E
c
maximum at 23°C. This maximum
coincides with the transition predicted by the NAC model where the rod structure is no longer
155
stable, yielding alternative morphologies with lower curvatures at higher temperatures. The
same trends are observed for the C12E5-cyclohexane and hexadecane-water µEs in Figure 6.7
(b). However, the predicted trend in the E / E
c
ratio for dilute rigid rods is shifted by about
3°C from the experimental data. This shift could be related to the value of Cn used in Table 6.3.
Using a value of Cn of 0.9 instead of 0.8 would produce a predicted ηµE curve for dilute rigid
rods that overlaps with the experimental data. This is a reasonable deviation considering that the
standard deviation in the estimated values of Cc and Cn range between ±0.1 and ±0.515,46
.
0
10
20
30
40
50
60
17 18 19 20 21 22 23 24 25 26 27
r
Temperature ( C)
Data of Leaver and Olsson
Dilute rigid spheres, Eq. 1
Dilute rigid rods, Eq. 6
0
5
10
15
20
25
30
20 21 22 23 24 25 26 27 28
r
Temperature ( C)
(a)
(b)
1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
T(°C)
T(°C)
Figure 6.7: Experimental and predicted E / E
c
ratio for the (a) C12E4-hexadecane-water and
(b) C12E5-cyclohexane and hexadecane-water µEs of Leaver and Olsson28
.
156
While there are a number of gaps to still be filled to accurately predict ηµE (e.g.
bicontinuous and concentrated µEs), incorporating shape considerations can be used to estimate
the significant changes in ηµE that occur over a relatively narrow range of formulation
conditions near the phase transition regions.
6.6 CONCLUSIONS
The new shape-based NAC model effectively estimated the shape of microemulsion
(µE) droplets assuming that they possess a cylindrical core with hemispherical end caps. This
proposed structure was confirmed via neutron scattering profiles as well as DLS measurements
of hydrodynamic radii. Introducing the predicted µE droplet shape and volume fraction into pre-
existing viscosity (ηµE) models allowed for the ηµE of µEs to be estimated. For toluene-water
µEs produced with 0.1 M SDHS, it was determined that the model of Doi and Edwards for a
dilute concentration of rigid rods produced a reasonable prediction of ηµE for oil-in-water (or
Type I) and water-in-oil (or Type II) µEs, especially near the bicontinuous (or Type III)
transition limits. Similar trends were observed in an attempt to model the experimental ηµE data
of non-ionic µEs taken from the literature. The capability of predicting µE morphologies and
ηµE from formulation conditions may potentially be useful in applications including nanoparticle
synthesis, transdermal drug delivery, environmental remediation, and enhanced oil recovery.
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165
7.1 ABSTRACT
In this chapter, the size and stability of emulsions around the phase inversion point was
estimated with the aid of the hydrophilic-lipophilic deviation (HLD) and net-average curvature
(NAC) models. The HLD and NAC models were used to predict the interfacial tensions,
densities, and viscosities of microemulsions (µEs) prepared with an anionic surfactant (sodium
dihexyl sulfosuccinate (SDHS)), toluene, and aqueous phase solutions of sodium chloride.
These predicted properties were introduced into known models that estimated the average
emulsion droplet size as a function of the mixing conditions. The predicted oil droplet sizes
compared well with those determined via optical microscopy. A simplified model of emulsion
stability, which was previously proposed in the literature, was used here to estimate the stability
of the emulsions formed after mixing. This emulsification model combined the assumption of
emulsion droplet diffusion-collision with an activation energy term for coalescence. This
activation energy term was calculated using the hole nucleation theory and by assuming that the
critical spacing between 2 approaching emulsion droplets was equal to the sphere-equivalent
diameter of their corresponding µE droplets. With the aid of the HLD and NAC models, the
stability of SDHS-toluene-water emulsions was reasonably predicted at surfactant
concentrations of 0.01 M, 0.1 M, and 0.3 M SDHS and temperatures ranging from 7°C to 44°C.
The largest deviations were observed at temperature and HLD extremes where the activation
energies might be dominated by factors that were not accounted for in the hole nucleation
theory. The HLD and NAC models were also used to predict literature data on the size and
stability of emulsions produced with other surfactants and oils. Overall, the applied models were
capable of producing reasonable estimates except for in situations that involved charge-
166
stabilized emulsion droplets and/or emulsion droplets stabilized by highly rigid surfactant
phases (e.g. liquid crystals).
7.2 INTRODUCTION
Large changes to the size and stability of emulsions dispersed throughout a
microemulsion (µE) continuum have been observed in Chapter 5 to occur around the
bicontinuous (or Type III) phase inversion point where oil-in-water (o/w, or Type I) µEs invert
into water-in-oil (w/o, or Type II) µEs. At this point, the interfacial tension (γow) reaches an
ultralow value, facilitating the production of submicron emulsions with a minimum energy
input. Furthermore, the stability of emulsions also reaches a minimum at this point. To make use
of these trends in the design of emulsification and phase separation processes, it is important to
be able to quantify the proximity to the phase inversion point. The most effective way of doing
so has been shown to be through the use of the following hydrophilic-lipophilic deviation
(HLD) models for ionic (Equation 1) and non-ionic (Equation 2) surfactants1,2,3,4,5,6
:
coc CTAfNSHLD 01.017.0ln , (Eq. 1)
noc CTANSHLD 06.017.013.0 , (Eq. 2)
In these equations, S is the NaCl concentration (in g/100 mL), Nc,o, for non-alkane oils,
is the equivalent alkane carbon number (EACN), f(A) and ϕ(A) are functions of the co-
surfactant type and concentration, ΔT is the difference in temperature from 25°C, and Cc and Cn
are the respective characteristic curvatures of ionic and non-ionic surfactants. Scanning
Equations 1 and 2 from HLD<0HLD=0HLD>0 reflects a Type IType IIIType II µE
phase behavior transition.
167
While the HLD model can be used to quantify the general approach of emulsions to the
phase inversion point (HLD=0), it fails to reveal how specific physical properties related to their
size and stability change. These properties, and more, can be estimated through the use of the
net-average curvature (NAC) model that was introduced for µEs in Chapter 6. The key
equations of the NAC model are as follows7,8
:
E
w
E
o
nrrL
HLDH
11 (Eq. 3)
E
w
E
o
arr
H
11
2
1 (Eq. 4)
In these equations, Hn and Ha are the respective net and average curvatures of the
surfactant at the oil-water interface, L is a scaling constant this is proportional to the extended
length of the surfactant tail (~1.2 times), and E
or and E
wr are the respective sphere-equivalent
radii of hypothetically co-existing oil and water µE droplets. Based on convention, a shift in
Equation 3 from Hn>0Hn=0Hn<0 corresponds to a HLD<0HLD=0HLD>0 transition.
By solving Equations 3 and 4, some of the continuous µE phase properties that can in turn be
predicted include solubilization capacities, phase transition and volumes, densities (ρµE), γow,
actual droplet shapes, and viscosities (ηµE).
The average emulsion droplet radius ( E
dr ) depends on the physical properties of the
system being considered and its mixing conditions. For turbulent mixing conditions in stirred
tanks (Re>10,000), E
dr can either be estimated via the energy dissipation per unit volume (εmix)
in Equation 5 or the impeller speed (Nimp) and diameter (Dimp) in Equation 69,10
:
168
5/15/2
5/3
1
Emix
owE
d
Cr
(Eq. 5)
5/35/45/6
5/3
2
Eimpimp
owE
dDN
Cr
(Eq. 6)
In these equations, C1 is a fitting constant that is close to 0.5 and C2 is 0.25 according to
the Hinze-Kolmogorov model. Given the power consumption (Pcons) and the total volume of the
emulsion (VE) in the mixer, ε can be estimated as Pcons/VE. Alternatively, Nimp and Dimp can be
used together instead of εmix.
The NAC model may also be used to predict the stability of emulsions around the µE
phase inversion point. That being said, the process of demulsification is quite complex and
system-dependent, involving a number of different stages, each one with its own governing
equation. For the anionic surfactant (sodium dihexyl sulfosuccinate (SDHS))-toluene-water
emulsions in Chapter 5, each one of these demulsification stages was experimentally
characterized by a time period. In the first aggregation time period (ap), it was proposed that
small emulsion droplets collide with neighboring emulsion droplets via Brownian motion to
form larger flocs. The ap time period is followed by a drainage time period (dp) where all flocs
settle into a more concentrated emulsion layer and undergo film thinning. The individual
emulsion droplets continue to grow via an internal coalescence process over this time period. In
the final coalescence time period (cp), all of the concentrated emulsion droplets gradually begin
to phase separate into a free excess phase. Based on similar phase separation profiles at different
SDHS concentrations, it was also determined that Ostwald ripening only pertains to emulsions
formulated at high surfactant concentrations, away from the phase separation point (HLD<-1
and HLD>1).
169
The simplest of the available demulsification models is that of Davies and Rideal for the
rate of emulsion droplet coalescence (Uc)11,12,13
:
Tk
EaTnkU
B
c
E
EBc exp
3
4 2
(Eq. 7)
The pre-exponential part of this model, which accounts for the average number of
Brownian collisions, is based on von Smoluchowski’s theory of colloid flocculation (truncated
to the formation of doublets) and Einstein’s definition of the diffusion of spheres. The undefined
terms in the pre-exponential part of this model include the number concentration of
monodisperse emulsion droplets (nE), the Boltzmann constant (kB, 1.38×10-23
J/K), and the
absolute temperature (T). The additional exponential activation energy term (Eac) further
describes the probability of an emulsion droplet collision leading to coalescence.
The schematic in Figure 7.1 shows a simplified overview of the collision-coalescence-
separation (CCS) mechanism used to implement Equation 7. According to this mechanism, as 2
emulsion droplets collide and coalesce, they are quickly released into the excess free phase and
the continuous µE phase then drains relatively quickly to help re-establish the initial number
concentration of emulsion droplets (nEo). In this simplified mechanism, both nE (=nEo) and the
average emulsion droplet size (as described by E
dr ) are considered as steady state constants.
This simplification is questionable as experimental observations for SDHS-toluene-water
emulsions in Chapter 5 suggest that although E
dr does not seem to change substantially over the
ap time period, it does increase in size over the latter dp and cp time periods. The CCS
mechanism is nevertheless still able to reproduce the fact that Uc is experimentally observed to
remain constant and that the ap time period is approximately proportional to ( E
dr )3.
170
Collision
Aggregation
CoalescenceSeparated phase
Continuous phase
Figure 7.1: Overview of the simplified CCS demulsification mechanism used to model
emulsion stability.
Finally, the total emulsion stability time period (ep) can be estimated using the following
expression:
c
Eo
pU
ne (Eq. 8)
To model Uc, the Eac term in Equation 7 will be estimated using the hole nucleation
theory for emulsion droplets14,15,16,17
. According to this theory, neighboring emulsion droplets
adjoin, as illustrated in Figure 7.2, by forming a hole across a film of thickness tH and diameter
(radius) dH (rH). Whether this formed hole evolves into a coalescence event depends on the size
of the hole. Small holes tend to contract and close, but large holes continue to grow and lead to
coalescence. Neglecting electrostatic or solvation effects, the hole nucleation theory accounts
for the interfacial rigidity (Er) of the surfactant self-assembly and γow.
171
dH=2rH
tH
rdE
Figure 7.2: Cross-section of coalescing emulsion droplets showing the formation of the
nucleating hole and its characteristic dimensions.
Figure 7.3 presents a summary of the strategies outlined above that will be used in this
chapter to predict the size and stability of Type I and Type II emulsions around the phase
inversion point. This modeling approach will primarily be applied to the SDHS-toluene-water
emulsions characterized at surfactant concentrations of 0.01 M, 0.1 M, and 0.3 M SDHS and
T=280 K, 288 K, 298 K, 308 K, and 317 K in Chapter 5. This same modeling approach will also
be used to predict the size and stability of the emulsions studied by Kabalnov et al., Salager et
al., Binks et al., and Lin et al.16,18,19,20
. The discussion section concentrates on highlighting the
advantages and limitations of the proposed modeling approach.
172
Formulation conditions(surfactant, oil, temperature,
electrolyte concentration, volume fraction)
Mixing conditions
Calculation of HLD
Calculation of SOW properties (HLD-NAC)
Calculation of emulsion initial drop size
Calculation of emulsion stability
Figure 7.3: General algorithm used to predict the size and stability of emulsions.
7.3 DEVELOPMENT OF EMULSION STABILITY MODEL SOLUTION
To model emulsion stability according to Equations 7 and 8, nEo is first solved for by
dividing the volume fraction of the emulsified phase ( E
d ) by the volume of an emulsion droplet
of radius E
dr (calculated using either Equation 5 or 6) as follows:
3
3
4 E
d
E
d
Eo
r
n
(Eq. 9)
The oil to water volume ratio for all of the emulsions modeled in this work is 1 (except
for those of Lin et al.). For this reason, E
d is set equal to 0.5. The sensitivity of Equations 7 and
173
8 to this assumption is tested by considering a range of E
d values up to, and including, the hard
sphere packing limit (=0.74). Increasing E
d any further would result in the transformation of
emulsion droplets into foam-like polyhedrons that no longer collide in a Brownian fashion17
.
For the SDHS-toluene-water emulsions in Chapter 5, εmix is estimated as 14 W/mL based
on a Pcons of 150 W and a VE of 11 mL. A similar value of εmix is assumed for the emulsions of
Kabalnov et al., Salager et al., and Binks et al. as these authors did not provide enough
information to solve for it16,18,19
.
To solve for Eac, the necessary energies of first forming the hole described in Figure 7.2
(E1) and then fully opening it (E2) are considered. Acosta et al. produced an empirical estimate
for E1 of Type III emulsions at HLD=0 (where γow~0)12
:
rc EfE 1 (Eq. 10)
In this equation, fc is a fitting constant. The fitted value of fc ~4 used by Acosta et al. is
employed here. The additional E2 contribution was modeled by de Vries as follows14
:
owHtE 2
2 73.0 (Eq. 11)
Several researchers have proposed different expressions for predicting the critical value
of tH (tH,crit). One such set of expressions derived by de Vries looked to calculate tH,crit according
to the geometrical packing constraints of bubbles21
. Another set of expressions derived by
Klaseboer et al. and Yaminsky et al. looked to calculate tH,crit by balancing the hydrodynamic
pressure at the center of a thinning film with the capillary pressure of fast approaching
bubbles22,23
. However, both sets of expressions do not take into account any of the interaction
energies at play. A more detailed analysis of how tH,crit is influenced by the inclusion of DLVO
174
interactions was issued by Vrij et al. and Chesters for thinning films at low surfactant
concentrations24,25
. Both of these research groups represented tH,crit as the film thickness below
which the attractive component of the DLVO interactions drives the immediate flocculation and
coalescence of emulsion droplets. The emulsions considered in this chapter are however at a
relatively high surfactant concentration where coalescence, and not film thinning, is more rate
limiting. For these emulsions, the thin film remains stable even after tH,crit is reached due to a
disjoining pressure effect. Ivanov et al. and others have demonstrated that the osmotic pressure
contribution to this disjoining pressure effect is most dominant and is closely associated with
expelling µE droplet layers during the film thinning process26,27
. The free energy penalty (ut) of
expelling the last layer of µE droplets, which can be modeled as per the equations of Basheva et
al. in Appendix 2, is the greatest28
. It is therefore proposed that tH,crit can be estimated as
follows:
Lrt E
dcritH 2, (Eq. 12)
In thereby summing E1 and E2 together, the following expression for Eac is obtained:
ow
E
drcc LrEfEa 292.2 (Eq. 13)
An alternative expression for Eac was developed by Kabalnov et al. using the hole
nucleation theory and Helfrich’s model that considers surfactant bending energies15.16,17
. Despite
the several similarities with Kabalnov et al., the simplified Equation 13 uses variables that are
easily predicted by the NAC model and its parameter database.
175
7.4 MATERIALS AND METHODOLOGIES
7.4.1 Materials
The following chemicals were purchased from Sigma-Aldrich Corp. (Oakville, ON,
Canada): NaCl (product #S9625, ≥99.5%) and SDHS (product #86146, ~80% in water).
Furthermore, reagent grade toluene (product #9200-1-30) was obtained from Caledon
Laboratory Chemicals (Georgetown, ON, Canada). Tap water was deionized to a conductivity
<3 µS/cm in the laboratory using an APS Ultra mixed bed resin.
7.4.2 NAC Modeling Methodology
The first step in applying the NAC model was to solve for Hn as a function of the change
in the HLD of ionic (Equation 14) and nonionic (Equation 15) surfactants at salinities S and S*:
L
S
S
L
HLDHn
*
ln
(Eq. 14)
L
SSb
L
HLDHn
* (Eq. 15)
In these equations, S is treated as a scanning parameter and S* is the optimal (or
reference) salinity at HLD=0 where emulsion stability is a minimum. It should be noted that this
alternative approach to solving for Hn (rather than that described in Chapter 6) was used here as
published values of S* for all of the emulsions under consideration were more easily obtained
from the literature instead of all the individual HLD parameters listed in Equations 1 and 2.
Aside from the above calculated Hn, the sphere-equivalent radius of the µE’s Type I (Type II)
continuous ( E
IIIowr
, ) and dispersed ( E
IIIwor
, ) phases, their respective volumes E
IIIowV , and
176
E
IIIwoV , , their respective droplet volume fractions
E
IIIow
, and E
IIIwo
, , and Ha were calculated
using the exact same procedure outlined in Chapter 6. With the aid of E
IIIwor
, as a basis of
calculation, Er was fitted to the measured isotherm γow as follows7,8
:
2,4 E
IIIwo
row
r
E
(Eq. 16)
By also taking E
IIIowV , and
E
IIIwoV , (or
E
IIIow
, and E
IIIwo
, ) together, ρµE was solved
for via the following expression:
E
IIIwo
E
IIIow
E
IIIwo
E
IIIwo
E
IIIow
E
IIIow
EVV
VV
,,
,,,,
(Eq. 17)
In this equation, E
IIIow
, and E
IIIwo
, are the respective densities of the µE’s Type I
(Type II) continuous and dispersed phases. The real length ( E
dl ) and radius ( E
dr ) of the µE
droplets was calculated as per Chapter 6:
E
reald
E
reald
E
reald
E
reald
E
reald
E
reald
nrlr
l
rlH
,,,
,
,, 42
12
2
4 (Eq. 18)
2,,,
,,
43
42
E
reald
E
reald
E
reald
E
reald
E
reald
a
rrl
rlH
(Eq. 19)
The impact of a change in the µE droplet shape from spheres (where E
dl =0) to rods
(where E
dl >> E
dr ) on ηµE was also estimated by assuming that the model for dilute rigid rods is
valid as per Chapter 6:
177
2
2
1E
dE
E
dgE
cE
r
lc
(Eq. 20)
In this equation, E
c
is the viscosity of the µE’s continuous phase and cg is the mass
concentration of µE droplet rods. The required HLD and NAC modeling parameters for
predicting the properties of the different emulsions of interest are listed in Table 7.1.
Table 7.1: Required HLD and NAC parameters for predicting the properties of the emulsions of
Kiran et al. (Chapter 5), Kabalnov et al., Salager et al., Binks et al., and Lin et al.16,18,19,20
.
Parameter Kiran et al. Kabalnov et al. Salager et al. Binks et al. Lin et al.
Surfactant SDHS
Alcohol
Ethoxylate
(C12E5)
Sodium
Dodecyl
Sulfate (SDS)
Aerosol OT
(AOT)
Nonylphenol
Co-surfactant N/A N/A Pentanol N/A N/A
Oil Toluene Octane Kerosene 0.65 cS
PDMS Mineral oil
S (g/100 mL) 1-10 1-20 1-10 0.1-6 0
S* (g/100 mL) 3 9 3.3 0.7 --
T (K) 298 293 298* 298 294
L (Ǻ) 106 25
8 20
7 11
6 18
8
ρoil (g/mL) 0.8729
0.730
0.8731
0.7632
0.84
ρwater (g/mL) f(S)33
ηoil (cP) 0.5629,34,35
0.5130,35
1.3531
0.49 2536
ηwater (cP) 0.8937
Voil (mL) 5.5 1 5.5* 5 20 g
Vwater (mL) 5.5 1 5.5* 5 75 g
csi (M) 0.01, 0.1,
and 0.3 0.08
SDS = 0.009
Pentanol =
0.6
0.04
5 g
ai
(Ǻ2/molecule)
1006 60
8
SDS = 607
Pentanol =
307
100
--
In this table, all of the fields marked by an asterisk “*” are unknown experimental
constants whose values are not available in the literature and that were therefore assumed to be
178
equal to those specified in Chapter 5. Furthermore, ρwater was extrapolated as a function of the
salinity from the referenced website.
7.4.3 Density and Viscosity Measurements
The validity of Equations 17 and 20 were tested for Type I and Type II SDHS-toluene-
water µEs. These µEs were prepared by allowing the mixed components in Table 1 to
equilibrate for 1 week. An estimate for ρµE was obtained by weighing out a 1 mL µE sample
using a Denver Instruments analytical scale (model #TP-214). For ηµE, a Gilmont Instruments
falling ball viscometer (model #GV-2200) was used. A detailed operating procedure for this
technique is provided in Chapter 6.
7.5 RESULTS
7.5.1 Experimental and Predicted SDHS-Toluene-Water Microemulsion
Properties
The experimental and NAC modeled µE properties required for the prediction of the size
and stability of SDHS-toluene-water emulsions are presented in Figures 7.4 (a)-(c). The γow at
0.01 M, 0.1 M, and 0.3 M SDHS can be represented by the single experimental isotherm taken
from Chapter 5 and replotted in Figure 7.4 (a). A fitted Er=1.5 kBT yields an accurate prediction
of γow at all of the tested surfactant concentrations.
The experimental and predicted ρµE in Figure 7.4 (b) are also in good agreement. Here,
Type I and Type II ρµE at a given SDHS concentration are shown to remain approximately
constant. A decrease (increase) in the Type I (Type II) ρµE is however observed with an increase
in the SDHS concentration.
179
In the final plot of ηµE in Figure 7.4 (c), the experimental and predicted values at both
0.01 M and 0.1 M SDHS are very close. At 0.01 M SDHS, ηµE across the Type I and Type II
regions is essentially equal to E
c
. At 0.1 M SDHS, ηµE peaks appear near the Type I-Type III
and Type II-Type III phase behavior limits. This system is an exact reproduction of the previous
modeling efforts in Chapter 6. Unlike at 0.01 M and 0.1 M SDHS, Equation 20 greatly over-
predicts ηµE at 0.3 M SDHS near the Type I-Type III and Type II-Type III phase behavior
limits. The dilute rigid rods model is likely inaccurate at this surfactant concentration and some
level of interaction amongst the rods must lead to the lower ηµE values. One thought by the likes
of Quemada et al. is that the interaction between µE droplets may lead to the early onset of
bicontinuous structures before an actual transition into the Type III region is physically
observed38
. The results in Figure 7.4 (c) suggest that the predicted ηµE should be limited to
values less than 5 cP, consistent with the experimental observations in Chapter 6.
180
0.8
0.9
1
1.1
1.2
-1.5 -1 -0.5 0 0.5 1 1.5
0.01
0.1
1
-1.5 -1 -0.5 0 0.5 1 1.5
0.3
3
30
-1.5 -1 -0.5 0 0.5 1 1.5
HLD
γo
w(m
N/m
)ρμE
(g/m
L)
ημE
(cP
)
(a)
(b)
(c)
Type I Type III Type II
Experimental (Kiran et al.) NAC (0.01 M SDHS) NAC (0.1 M SDHS) NAC (0.3 M SDHS)
Experimental (0.01 M SDHS) Experimental (0.1 M SDHS) Experimental (0.3 M SDHS)
NAC (0.01 M SDHS) NAC (0.1 M SDHS) NAC (0.3 M SDHS)
Figure 7.4: Experimental and NAC modeled (a) γow, (b) ρµE, and (c) ηµE of SDHS-toluene-water
µEs.
7.5.2 Predicted Droplet Size of 0.1 M SDHS-Toluene-Water Emulsions
Figure 7.5 presents the predicted E
dr , calculated using Equation 5, as a function of HLD.
The fitted value of C1 is 0.4 for Type I emulsions (HLD<0) and 0.6 for Type II emulsions
181
(HLD>0). The need for two different fitting constants might be due to the different fluid
properties of the continuous phase (water and toluene respectively). Overall, the experimental
values reported in Chapter 5 are closely reproduced, except for the E
dr of Type I emulsions
close to the Type III transition that are slightly underpredicted. These fitted C values are
employed in all the other emulsion modeling efforts, except for the systems of Lin et al.20
. r d
E(μm)
0.1
1
10
-1.5 -1 -0.5 0 0.5 1 1.5
Type I Type III Type II
Experimental (Kiran et al.)
NAC
HLD
Figure 7.5: Predicted E
dr of 0.1 M SDHS-toluene-water emulsions at 298 K using the NAC
model. Experimental data are obtained from the work presented in Chapter 5.
7.5.3 Predicted Stability of 0.1 M SDHS-Toluene-Water Emulsions
A theoretical demonstration of the prediction of ut from the equations listed in Appendix
2 is presented in Figure 7.6 (a) as a function of the number of µE droplet layers (tH/2 E
dr ) at
HLD=±0.5. These predictions were made by varying the µE droplet volume fraction ( E
d
) from
0.1 to 0.2 and setting the second term in the expression for π1 as P~
. A maximum in ut is clearly
observed in this figure upon expelling the last layer of droplets. The increase in ut at increased
182
E
d
is also consistent with the previous results of Basheva et al.28
. To estimate tH,crit, the NAC
modeled E
dr is incorporated into Equation 12. Figure 7.6 (b) presents the estimated values of
tH,crit as a function of the HLD. As illustrated in this figure, the value of tH,crit increases from 3 to
11 nm upon approaching the Type I-Type III and Type II-Type III phase boundaries. The
reason for this increase in tH,crit is that E
dr also increases as the formulation approaches the
phase boundaries. While close, the predicted tH,crit values are smaller than the 10-20 nm range
measured by Nikolov et al. for the anionic surfactant SDS using a reflected light interferometric
technique39
. Nevertheless, they are still greater than the minimum range for black films (1.3-2.5
nm) reported by Sonneville-Aubrun et al.40
.
-60
-40
-20
0
20
40
60
0 1 2 3 4 5
0
3
6
9
12
15
-1.5 -1 -0.5 0 0.5 1 1.5
t H,c
rit(n
m)
Type I Type III Type II
HLD
ut(k
BT
)
(a) (b)
# µE Droplet Layers
1.0,5.0 E
dHLD
2.0,5.0 E
dHLD
15.0,5.0 E
dHLD
1.0,5.0 E
dHLD
2.0,5.0 E
dHLD
15.0,5.0 E
dHLD
Figure 7.6: Predicted (a) ut and (b) tH,crit of 0.1 M SDHS-toluene-water emulsions at 298 K
using the NAC model.
The predicted Eac are presented in Figure 7.7 as a function of the HLD, along with the
apparent activation energies determined experimentally in Chapter 5. The predicted Eac values
are close to the apparent values at -0.5<HLD<0.5. At the HLD extremes, however, where γow
183
effects are more prominent, the predicted Eac are significantly smaller than the apparent values.
It is possible that the apparent activation energies may contain systematic errors because they
were obtained by assuming that the pre-exponential factor does not vary with changes in
temperature.
1
10
100
-1.5 -1 -0.5 0 0.5 1 1.5
Ea
c(k
BT
)
Type I Type III Type II
Experimental (Kiran et al.)
NAC
HLD
Figure 7.7: Predicted Eac of 0.1 M SDHS-toluene-water emulsions at 298 K using the NAC
model. Experimental data are obtained from the work presented in Chapter 5.
Figure 7.8 presents the estimated stability for 0.1 M SDHS-toluene-water emulsions at
room temperature and as a function of the HLD. Within the range of E
d from 0.5 to 0.74, the
predicted emulsion stabilities compare well with the measured ep time periods in Chapter 5. The
largest deviations occur near the Type I-Type III phase boundary where the stability is under-
predicted by one order of magnitude. However, the predicted values at the Type I-III phase
boundary are consistent with the experimental ap time periods. A smaller over-prediction of the
ep time period occurs at HLD>1.
184
epcpdpap
NAC ( =0.5) NAC ( =0.74)
1
10
100
1000
10000
100000
-1.5 -1 -0.5 0 0.5 1 1.5
Type I Type III Type II
Tim
e (
Se
co
nd
s)
HLD
E
dE
d
Figure 7.8: Predicted stability (solid lines) of 0.1 M SDHS-toluene-water emulsions at room
temperature with E
d =0.5 (initial volume fraction) and 0.74 (closely packed hard spheres). All
experimental data is taken from Chapter 5.
7.5.4 Effect of Surfactant Concentration on the Predicted Stability of SDHS-
Toluene-Water Emulsions
Figure 7.9 presents the experimental and NAC modeled (solid lines) stability of
emulsions prepared with (a) 0.01 M and (b) 0.3 M SDHS. At 0.01 M SDHS, the model over-
predicts, by at least 1 order of magnitude, the stability of emulsions at HLD<-1 and HLD>1.
Conversely, the stability is still underpredicted near the Type I-Type III and Type II-Type III
phase boundaries. At 0.3 M SDHS, relatively accurate stability predictions are obtained for all
the emulsions. It is important to reiterate that the predicted ηµE at 0.3M SDHS is limited to no
more than 5 cP to be consistent with experimental results. Larger predicted ηµE would have
produced local stability peaks near the μE phase boundaries. Although these stability peaks are
185
not experimentally observed for these particular emulsions, they have been observed in the past
for others41
.
epcpdpap NAC
1
10
100
1000
10000
100000
-1.5 -1 -0.5 0 0.5 1 1.5
Tim
e (
Se
co
nd
s)
Type I Type III Type II
(a)
1
10
100
1000
10000
100000
-1.5 -1 -0.5 0 0.5 1 1.5
Tim
e (
Se
co
nd
s)
(b)
HLD
Figure 7.9: Predicted stability (solid lines) of (a) 0.01 M and (b) 0.3 M SDHS-toluene-water
emulsions at 298 K and E
d =0.5. Dashed line in (a) corresponds to predicted values using
tH,crit=0. All experimental data is taken from Chapter 5.
7.5.5 Effect of Temperature on the Predicted Stability of SDHS-Toluene-Water
Emulsions
Figure 7.10 presents the stability of 0.1 M SDHS emulsions at (a) 280 K, (b) 288 K, (c)
308 K, and (d) 317 K. It should be noted here that the effect of temperature on the HLD was
taken into account at the time of calculating the properties of the μEs. Overall, within the range
186
of temperatures considered in Figure 7.10, the stability of these emulsions is reasonably
predicted except at the phase boundaries where it is consistently underpredicted. One also
observes that the stability at HLD=-1.1 and 317 K is overpredicted by a factor of 2.
These observations suggest that the predicted activation energies of Figure 7.7 are, for
the most part, adequate and that the deviations from the experimental values observed at
extreme HLDs might be explained by the method used to estimate those experimental values.
epcpdpap NAC
1
10
100
1000
10000
100000
-1.5 -1 -0.5 0 0.5 1 1.5
1
10
100
1000
10000
100000
-1.5 -1 -0.5 0 0.5 1 1.5
(a) (b)
(c) (d)
Tim
e (
Seco
nd
s)
Tim
e (
Seco
nd
s)
Type I Type III Type II
HLD HLD
Type I Type III Type II
1
10
100
1000
10000
100000
-1.5 -1 -0.5 0 0.5 1 1.5
1
10
100
1000
10000
100000
-1.5 -1 -0.5 0 0.5 1 1.5
Figure 7.10: Predicted stability (solid lines) of 0.1 M SDHS-toluene-water emulsions at
E
d =0.5 and (a) 280 K, (b) 288 K, (c) 308 K, and (d) 317 K. All experimental data was taken
from Chapter 5.
187
7.6 DISCUSSIONS
7.6.1 Prediction of the Droplet Size and Stability of SDHS-Toluene-Water
Emulsions
The match between the predicted E
dr using the NAC model and the experimental data is
not surprising considering that the NAC modeled µE properties in Figures 7.4 (a)-(c) fitted the
experimental values reasonably well. However, it is important to note that the droplet sizes near
the Type I-Type III boundary are underpredicted. This seems to be connected with the under-
prediction of γow in that region (Figure 7.4 (a)). This deviation in γow may be due to a small
underestimation of the value of S*. The deviation in E
dr near the Type I-Type III phase
boundary might also explain the underprediction of emulsion stabilities at the Type I-Type III
phase boundary for nearly all the SDHS systems. According to the CCS mechanism (Figure 7.1
and Equations 7 and 8), the stability of the emulsion is proportional to the inverse of the initial
drop concentration (epnEo-1
), which in turn means that emulsion stability is proportional to the
cube of the initial emulsion droplet size (ep ( E
dr )3). Therefore an underprediction in E
dr would
produce an even more severe underprediction of emulsion stability.
The surprising element in this work is that the implementation of the simple kinetic
model of Davies together with the simple, and physically inaccurate, CCS mechanism is able to
predict reasonably well (within 1 order of magnitude) the stability of SDHS-toluene-water
emulsions. This might be explained by the fact that the selection of the model and the CCS
mechanism is guided by the features of the separation profiles: constant and nearly identical
coalescence and drainage rates, a relatively long ap time period where almost no changes in the
emulsion are observed, and that the aggregation time scaled to ( E
dr )2.5
. It is unlikely that any
188
other single equation can represent the exact physics of the complex multistep demulsification
process. However, the reason that the kinetic model is successful for the SDHS-toluene-water
emulsions is because it captures the main features of the stages of aggregation and coalescence
that seem to be the rate limiting steps. It is unlikely that this kinetic model and CCS
approximation would work for emulsions where the drainage rate controls the overall
separation.
All the droplets considered in this work are relatively small for creaming or
sedimentation to contribute to droplet collisions. However, for emulsions produced with more
positive or negative HLDs, the larger γow would produce larger droplets that should lead to an
increase in creaming and sedimentation and an acceleration of the overall separation of the
emulsion. Another important clarification is that for the SDHS-toluene-water emulsions
evaluated in this work, Ostwald ripening is not an important factor. Ostwald ripening can
accelerate the overall separation process, particularly for systems with more positive or negative
HLDs that experience larger γow.
One of the consequences of the kinetic model and CCS mechanism is that most of the
changes in emulsion stability around the phase inversion point might be explained by the
changes in E
dr rather than the changes in activation energies as initially proposed by Kabalnov
et al.15,16
. As indicated in Figure 7.7, the changes in Eac around the phase inversion point are
relatively small due to the fact that tH,crit grows as the HLD approaches 0 while γow reduces.
These activation energies produce reasonable predictions of emulsion stability at different
temperatures. The experimentally-determined apparent activation energies used the assumption
of Kabalnov et al. that the pre-exponential factor is constant (i.e. does not change with
temperature) which might have produced an over-estimation of some of the values of activation
189
energies, particularly for large (negative or positive) values of HLD. Another aspect that
deserves some consideration is the estimation of tH,crit as 2( E
dr +L). Overall, this assumption
seems to be consistent as the predicted activation energies help reproduce the experimental
emulsion stabilities at different temperatures. However, it is important to remember that this
estimation of tH,crit is justified by the osmotic pressure associated with removing this last layer of
μE drops. Therefore, surfactant concentration (i.e. the concentration of μE drops) must play a
role on the value of this thickness. In particular, for the case of the 0.01 M SDHS system, the
surfactant concentration is just above the critical μE concentration for this system, therefore the
osmotic pressure contribution is very low for this system and the emulsion drops can approach
each other with negligible resistance. To obtain a better prediction of emulsion stability at 0.01
M SDHS, one could assume that the E2 term can be neglected by setting tH,crit=0. The dashed
line in Figure 7.9 (a) shows the prediction of the emulsion stabilities with no E2 contribution,
which clearly produces a better approximation to the experimental values. Two elements that
were not considered in the estimation of the activation energy were solvation effects and
electrostatic repulsion. Hydration can be important for systems of ethoxylated nonionic
surfactants, particularly at low temperatures, and electrostatic repulsion is likely to be important
for ionic surfactant systems prepared with little or no added electrolyte.
To the best of our knowledge, all previous efforts in studying the changes in emulsion
stability around the phase inversion point have been limited to the qualitative description of
these changes from proposed mechanisms. No quantitative predictions have been produced. The
NAC model used in combination with the kinetic model of Davies and the CCS mechanism has
been able to quantitatively predict the order of magnitude of these stabilities for the first time.
Despite this advancement, there are several modeling limitations that still need to be addressed.
190
The most notable of these limitations is the case where settling becomes more rate-limiting.
Such a scenario is likely to occur when either the gravitational field is << 1 g or ∆ρ approaches
0. Under these types of conditions, the validity of the CCS mechanism breaks down as one can
no longer assume that growing emulsion droplets immediately phase separate. This furthermore
introduces polydispersity effects which cannot be ignored (especially when dealing with
Ostwald ripening). The proposed model conversely breaks down at the other extreme where
either the gravitational field is >> 1 g or ∆ρ is very large. Under these alternative conditions, the
separation of dispersed droplets no longer depends on their Brownian collisions, but instead on
the rate of collisions induced by creaming/sedimentation. Another limitation of the proposed
emulsion stability model is that it ignores solvation and electrostatic repulsion effects. Under
conditions where these effects are prominent, an increase in tH,crit and hence emulsion stability is
expected. One last limitation is that the stability model does not account for rigid structures (i.e.
liquid crystals) at the interface. These types of structures enhance emulsion stability via an
increase in Er.
The idea of using the proposed modeling framework to evaluate the formation and
stability of other emulsions already in the literature is considered in the next sections.
7.6.2 Prediction of the Emulsion Droplet Size of Lin et al.
Lin et al. reported the average emulsion drop diameters produced with 65 wt% water, 5
wt% nonylphenol ethoxylates with different degrees of ethoxylation, and 30 wt% mineral oils.
The emulsions were prepared by mixing 100g of the emulsion at 150 rpm and an impeller with 6
cm diameter. The HLD of nonylphenol ethoxylate - mineral oil systems was evaluated using
Equation 2, with an EACN of 13 for mineral oil, and characteristic curvatures (Cn) for
191
nonylphenol ethoxylates estimated as 7-#ethylene oxide groups, in the absence of salt (S=0) and
at 21°C (ΔT=-4°C)8,42
. The γow of these nonylphenol-mineral oil systems were predicted using
Er=4kBT8. Figure 7.11 presents the drop diameter calculated using Equation 6 and the
properties of the nonylphenol-mineral oil system predicted with the NAC model. One of the
points that Lin et al. made in their contribution was that the optimal emulsification conditions
could be predicted by the determining, experimentally, the maximum solubilization capacity of
their system. Not knowingly, these authors were getting at the point that the optimal
emulsification (lowest drop size) is obtained at HLD=0. The data in Figure 7.11 accurately
predicts (without experiments) that the optimal emulsification occurs in nonylphenols where the
ethylene oxide groups represent 50% of the mass of the surfactant. The minimum drop size of
the emulsion was also predicted. The predicted range of optimal emulsification is relatively
narrow compared to the range of optimal emulsification proposed by Lin et al.
0
25
50
75
100
30 40 50 60 70
Dro
p d
iam
ete
r, u
m
wt% PEO in the surfactant
NAC predicted drop size
Trend proposed by
Lin et al.
Figure 7.11: Predicted emulsion droplet size (solid line) for the nonylphenol ethoxylate-mineral
oil-water systems at 294 K and as a function of the wt% of polyethylene oxide (PEO) in the
192
surfactant. See Table 7.1 for additional simulation conditions. The experimental data is taken
from Lin et al.
7.6.3 NAC Prediction of Initial Emulsion Droplet Size and Stability for the
Systems of Binks et al. with AOT and 0.65 cSt Silicone Oil
The prediction of the HLD and solubilization for the AOT-silicone system has been
reported by Castellino et al.43
. Figure 7.12 (a) presents the predicted γow using Er=1 kBT and its
comparison to the experimental values of Binks et al. The predicted γow match the experimental
values reasonably well. It is important to mention that Binks et al. do not describe the power
input for the mixer. They do, however, present some average drop sizes. The drop sizes
predicted by using the NAC model together with Equation 5 and εmix=14 W/mL range from 0.5
to 5 μm across a HLD range of -0.3 to -2. Binks et al. measured drop size ranges from 1 to 4 μm
across the same range of HLD values. The predicted emulsion stabilities (ep) are presented as
the solid lines in Figure 7.12 (b). In accordance with the ep definitions of Binks et al., the
predicted Type I results are multiplied by a factor of 0.05 and the predicted Type II results are
multiplied by a factor of 0.5. It is observed that the predicted ep is smaller than those obtained
experimentally, particularly at the Type I and Type II extremes. Solvation effects, electrostatic
repulsion, formation of rigid interfaces (e.g. liquid crystals), and/or film drainage issues could
be responsible for these inconsistencies. One crude method to test for solvation/electrostatic
effects is to simply add an additional term to the estimated tH,crit. The estimated tH,crit as per
Equation 12 ranges from 3 to 15 nm as the HLD is reduced from 2 to 0.2. Adding an additional
thickness of 15 nm to all the estimated values of tH,crit produced emulsion stabilities represented
by the dashed lines in Figures 7.12 (b), which represent more closely the experimental trends.
This additional thickness is consistent with measurements of disjoining pressures determined in
193
a liquid surface force apparatus using the system of AOT-water-dodecane (similar EACN to
0.65 cSt silicone oil), in the presence of very low surfactant concentrations and electrolyte
concentrations similar to those used in the Type I μE systems44
. In that work, the authors
determined that the emulsions films could only be compressed until about 10 to 20 nm of
separation. In the presence of higher surfactant concentrations, this separation could grow as
large as 60 nm.
0.001
0.01
0.1
1
10
-2 -1.5 -1 -0.5 0 0.5 1 1.5 2
NACExperimental (Binks et al.)
γo
w(m
N/m
)
Type I Type III Type II
HLD
Tim
e (
Se
co
nd
s)
0.001
0.1
10
1000
100000
10000000
-2 -1.5 -1 -0.5 0 0.5 1 1.5 2
(b)
(a)
Figure 7.12: Predicted (a) interfacial tension and (b) emulsion stability (solid lines) for the
AOT-0.65 cSt silicone oil system. See Table 7.1 for additional simulation conditions. The
dashed line in (b) represents the predicted stability considering an additional contribution to
tH,crit of 15 nm. The experimental data is taken from Binks et al.
194
7.6.4 NAC Prediction of Emulsion Stability for the Systems of Kabalnov et al.
with C12E5 and Octane
The NAC parameters and prediction of the interfacial tension for the C12E5 system has
been presented in a previous work. Unfortunately, in the work of Kabalnov et al., the method of
mixing is simply described as vigorous hand shaking (~5 times) and that other methods of
mixing did not introduce substantial changes. To this end, the “vigorous” hand mixing is simply
simulated as εmix=14W/mL. The work of Kabalnov does not present data on the initial drop size
that could be used to compare/validate the predicted values. Figure 7.13 (a) presents the NAC
predicted and experimental stabilities for C12E5-octane systems. It is important to clarify that
Kabalnov et al. did not follow the data for more than one month and that upward pointing
arrows (as presented by the authors) indicate that the stability of those systems is larger than the
time reported. It is also worth noting that these predicted stabilities are multiplied by a factor of
0.5, consistent with the definition of stability used by Kabalnov et al. Despite all the
extrapolations required to predict the stability of the emulsions of Kabalnov, the stabilities near
the phase transitions are of the same order of magnitude as the experimental values. The rest of
the data, considering that it was not tracked for more than one month, is also consistent with the
predictions of the model.
195
Tim
e (
Se
co
nd
s)
Tim
e (
Se
co
nd
s)
1.E+00
1.E+02
1.E+04
1.E+06
1.E+08
1.E+10
-1.5 -1 -0.5 0 0.5 1 1.5
(a)
Type I
Experimental (Kabalnov et al.)
NAC
HLD
(b)
1
10
100
1000
10000
100000
1000000
-1.5 -1 -0.5 0 0.5 1 1.5
Experimental (Salager et al.)
NAC
Type III Type II
Type I Type III Type II
Er = 2.5 kBT
Er = 1.8 kBT
Er = 1.0 kBT
Figure 7.13: Predicted emulsion stability (solid lines) for the system (a) C12E5–octane and (b)
SDS-pentanol-kerosene. See Table 7.1 for additional simulation conditions. The experimental
data for the systems in (a) and (b) is obtained from Kabalnov et al. and Salager et al.
respectively.
7.6.5 NAC Prediction of Emulsion Stability for the Systems of Salager et al. with
SDS, Pentanol, and Kerosene
For the SDS-pentanol-kerosene system there is no information to validate the prediction
of γow and E
dr . For this reason, Er values of 1 kBT, 1.8 kBT, and 2.5 kBT were used in predicting
the emulsion stabilities as shown in Figure 7.13 (b). The predicted emulsion stabilities (solid
196
lines) for o/w systems (negative HLDs), using Er=2.5 kBT, produces reasonable predictions
whereas the stability of w/o systems is reproduced using Er=1.8 kBT. Although the γow of most
SOW systems can be predicted using a single value of Er, one study reported a case where the
interfacial rigidities of o/w and w/o systems were different45
. It is possible that the partition of
pentanol into the oil-continuous and water-continuous environments is responsible for the
different Er obtained in both scenarios. One feature of the proposed modeling framework that is
illustrated in Figure 7.13 (b) is that even relatively small changes in Er can produce substantial
changes in emulsion stability. This also explains why liquid crystal systems (Er~10 kBT)
produce highly stable emulsions.
7.7 CONCLUSIONS
In this work, the formation and stability of SDHS-toluene-water emulsions around the
phase inversion point was reasonably reproduced using HLD and NAC predicted properties of
the surfactant-oil-water (SOW) system and mixing and demulsification modeling parameters. A
simple collision-coalescence-separation (CCS) mechanism was used to implement the
demulsification model of Davies. This CCS mechanism incorporates the main features of the
drop aggregation and coalescence that were identified as the rate-controlling steps in Chapter 5.
The activation energy of the kinetic model of demulsification was evaluated using the hole
nucleation theory and an assumption that the critical film thickness was defined by the cross
sectional dimension of the μE drops that need to be removed from the film. Overall, the model
was able to predict the size of the emulsion drops and the order of magnitude of the stability of
the SDHS-toluene-water systems around the phase inversion point (HLD from -1.5 to +1.5) for
systems prepared at temperatures ranging from 7 to 44°C and SDHS concentration of 0.01 M to
0.3 M. When this methodology was extrapolated to explain other literature data, the predictions
197
were consistent with the data. The model can be used to produce benchmark estimates that need
to be further discussed in light of the relative importance of other phenomena including
creaming/sedimentation, Ostwald ripening, film drainage, surfactant solvation and electrostatic
interactions, and the potential formation of rigid interfaces, including liquid crystals.
7.8 REFERENCES
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Solubilization and Supersolubilization in Surfactant Microemulsions. Langmuir 2003, 19, 186-
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8 Acosta, E.J. The HLD-NAC Equation of State for Microemulsions Formulated with Nonionic
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205
The overall goal of this thesis was to study the formation and stability of emulsions both
experimentally and with the aid of the hydrophilic-lipophilic deviation (HLD) and net-average
curvature (NAC) models. The formation and stability of bitumen emulsions (i.e. rag layers) was
of particular interest due to its relevance in the processing of oil sands. In Chapters 2 and 3, the
ability of asphaltenes and naphthenic amphiphiles to stabilize rag layers was experimentally
assessed as a function of solvent-bitumen-water ratios, solvent aromaticity, and temperature. In
Chapter 4, the hydrophilic-lipophilic natures of bitumen as well as that of endogenous surface-
active asphaltenes and naphthenic amphiphiles were quantified. Using toluene as a model oil
phase for bitumen in Chapters 5-7, a new approach for modeling emulsion stability as a function
of the equilibrium phase behavior of related microemulsions (µEs) was developed. The aim of
this review chapter is to revisit the formation and stability of bitumen emulsions and provide
new insight into how they themselves can be predicted.
In considering the formation of bitumen emulsions, the following HLD model is used to
predict the preferential oil-water partitioning behavior of the surfactant (or surfactant mixture):
coc CTAfNSHLD 01.017.0ln , (Eq. 1)
The salinity (S) of the aqueous phase used to formulate these emulsions can be expressed
in terms of an equivalent NaCl concentration of 0.3 g/100 mL. Additionally, the hydrophobicity
of bitumen (Nc,o), expressed in terms of its equivalent alkane carbon number (EACN), is 2.5 and
that of the solvents used to dilute bitumen, heptol 80/20 (80 vol% heptane and 20 vol% toluene)
and heptol 50/50 (50 vol% heptane and 50 vol% toluene), are 5.8 and 4 respectively. For the
case when asphaltenes, with a maximum hydrophobicity (or characteristic curvature (Cc)) of 2.3,
are used as the sole surfactant in the absence of any co-surfactant (f(A)=0) at 25°C (ΔT=0), the
HLD can be expressed as in Figures 8.1 as function of the heptol to bitumen dilution ratio. Here,
206
the range of heptol 80/20 (heptol 50/50) to bitumen dilution ratios from 1/1.5 to 10/1 represents
a corresponding range in the EACN of the mixed oils from 3.6 to 5.4 (3 to 3.8). The fact that a
calculated HLD>0 is observed across all these heptol to bitumen dilution ratios is consistent
with the experimental observance of water-in-oil (w/o) bitumen emulsions in Chapter 2. It
should be noted that the maximum Cc of 2.3 used here is for high molecular weight asphaltenes
(~1000 g/mol). By using a minimum Cc of 0.8 for low molecular weight asphaltenes (~500
g/mol), a range of HLD<0 values is instead observed.
0
0.2
0.4
0.6
0.8
1
0 2 4 6 8 10
Heptol 80/20
Heptol 50/50
Heptol to Bitumen Dilution Ratio (w/w)
HL
D
Figure 8.1: The HLD as a function of the heptol to bitumen dilution ratio for asphaltene-
stabilized rag layers prepared with heptol 80/20 and heptol 50/50 at 25°C.
The effect of 3 wt% sodium naphthenates (NaNs) on the HLD of the above bitumen
emulsions is plotted in Figure 8.2 at an oil to water ratio of 1 to 1 and as a function of the heptol
to bitumen dilution ratio.
207
-5
-4
-3
-2
-1
0
0 2 4 6 8 10
Heptol 80/20
Heptol 50/50
Heptol to Bitumen Dilution Ratio (w/w)
HL
D
Figure 8.2: The effect of 3 wt% sodium naphthenates (NaNs) on the HLD of bitumen emulsions
at an oil to water ratio of 1 to 1 and as a function of the heptol to bitumen dilution ratio.
It is assumed in Figure 8.2 that bitumen is composed of 15% asphaltenes and that all
these asphaltenes are high molecular weight aggregates that are surface-active. The observed
HLD<0 values across the heptol 80/20 and heptol 50/50 to bitumen dilution ratios are in
agreement with the experimentally observed o/w emulsions reported in Chapter 3. While an
increase in the oil to water ratio up until 10 to 1 is observed to drive a more positive HLD as a
result of the increase in the ratio of asphaltenes to NaNs, HLD<0 values are still observed. A 10
wt% NaN concentration would produce ever more negative HLDs.
A similar procedure can be used to evaluate the effect of introducing 3 wt% naphthenic
acids (NAs) on the HLD of bitumen emulsions. The estimated HLD values are presented in
Figure 8.3 as a function of the heptol to bitumen dilution ratio.
208
-5
-4
-3
-2
-1
0
0 2 4 6 8 10
Heptol 80/20
Heptol 50/50
Heptol to Bitumen Dilution Ratio (w/w)
HL
D
Figure 8.3: The effect of 3 wt% naphthenic acids (NAs) on the HLD of bitumen emulsions as a
function of the heptol to bitumen dilution ratio.
The results depicted in Figure 8.3 show that HLD<0 values are predicted at the heptol
80/20 and heptol 50/50 to bitumen dilution ratios considered. These HLD<0 values are to a
certain degree logical in that some signs of o/w emulsions are observed within the bitumen
emulsions evaluated in Chapter 3. For the most part, however, dominant w/o morphologies are
observed. A potential reason for which the formation of o/w bitumen emulsions is predicted
instead of w/o emulsions is because no special attention is given to the effect of NA partitioning
on the actual HLD calculation itself. Also, according to Figure 3.5 (surface pressure isotherm
for mixtures of asphaltenes and NAs) in Chapter 3, even a mixture containing 3 parts (per
weight) of asphaltenes to 1 part of NAs still shows the same surface pressure isotherm of pure
asphaltenes. Considering that bitumen contains 15% asphaltenes, it would take more than 5 wt%
NAs to start replacing some of the asphaltenes from the interface. This would suggest that the 3
209
wt% NAs added to the system has a limited influence on changing the Cc of the surfactant
mixture.
In addition to being able to predict the formation of the above rag layers, the use of the
HLD framework can also be employed to qualitatively interpret their relative stabilities. For
example, asphaltenes alone produce w/o rag layers that are only ~0 to 0.4 units above the
optimum point of minimum emulsion stability (HLD=0). On the other hand, mixtures of
asphaltenes and NaNs produce o/w rag layers that are ~1.5 to 4 units below HLD=0. What this
should signify, at least according to Chapters 5 and 7, is that o/w rag layers stabilized by
mixtures of asphaltenes and NaNs are much more stable than w/o rag layers stabilized by
asphaltenes alone. This hypothesis can indeed be confirmed from the experimental rag layer
stability results presented in Chapters 2 and 3. It can further be concluded from this theory that
mixtures of asphaltenes and NAs should consistently produce rag layers with an HLD~0
(instead of ~-1 to -2 as in Figure 8.3) as they are highly unstable.
The last aspect to be considered in this chapter is how the NAC model can be introduced
to quantitatively predict the stability of o/w bitumen emulsions stabilized by asphaltene and
NaN mixtures. This modeling approach is considered valid for these emulsions as their
measured interfacial tension (γow) values in Chapter 3 are comparable to those for the different
SDHS-based µEs in Chapters 4 and 5. The experimental and predicted γow of these o/w
emulsions as a function of their HLD are presented in Figure 8.4.
210
Figure 8.4: Experimental and predicted γow as a function of the HLD for o/w bitumen emulsions
stabilized by a mixture of asphaltenes and NaNs.
To obtain this figure, it is assumed from the competitive adsorption results presented in
Chapter 3 that NaNs populate the primary adsorbed surfactant layer at the oil-water interface.
Furthermore, the interfacial rigidity (Er) of NaNs is 1 kBT (typical for ionic surfactant systems)
by fitting the extended tail length (L) as 20 Ǻ (assuming that the molecule has the equivalent of
12 carbon groups in length) and taking an area per molecule (asi) of 50 Ǻ2. The predicted
estimates of γow presented in Figure 8.4 are quite reasonable when one considers the complexity
of the system being modeled.
From the predicted γow values in Figure 8.4, predictions of the average o/w bitumen
emulsion droplet diameter ( E
dd ) are obtained as a function of the HLD in Figure 8.5. To
calculate E
dd , Equation 5 of Chapter 7 is used with a known energy dissipation rate ε=14W/mL
and a fitted proportionality constant C1=2. The fact that the value of C1 required to reproduce
211
this data is 4 times larger than that used for toluene emulsions may be due in part to the larger
viscosity ratio between the dispersed and continuous phases. This would also explain why the
emulsion droplet sizes are underpredicted at HLDs closer to 0 (lower heptol to bitumen dilution
ratios) even when using a value of C1=2.
0
3
6
9
12
15
-5 -4 -3 -2 -1 0
Experimental
Predicted
HLD
dd
E(µ
m)
Figure 8.5: Experimental and predicted E
dd as a function of the HLD for o/w bitumen emulsion
droplets stabilized by a mixture of asphaltenes and NaNs.
By taking γow and E
dd together, as well as the calculated activation energies of
coalescence (Eac) from modeled film thicknesses of 7 nm to 9 nm, predictions of o/w bitumen
emulsion stability as a function of the HLD are obtained as in Figure 8.6.
212
1.E+00
1.E+02
1.E+04
1.E+06
1.E+08
1.E+10
-5 -4 -3 -2 -1 0
HLD
Tim
e (S
econ
ds)
Figure 8.6: Predicted stability of o/w bitumen emulsions stabilized by a mixture of asphaltenes
and NaNs as a function of the HLD.
The predicted stability trend depicted in Figure 8.6 closely follows those of the other
emulsions studied in Chapter 7. Unfortunately, however, these predictions cannot be compared
against the experimental rag layer stabilities presented in Chapter 3 as they were subjected to
centrifugal separation. As such, their separation cannot be simply described as per Brownian
collisions in this work. They instead require a careful consideration of hydrodynamic
interactions. It should also be noted here that the predicted emulsion stability times are
minimum values that do not consider the added rigidity imparted by the adsorption of asphaltene
skins.
214
This thesis explored the stability of bitumen emulsions from an experimental and
modeling perspective. In Chapter 2, it was shown via microscopic and spectroscopic techniques
that the phase separation of water-in-oil (w/o) bitumen emulsion droplets was impacted by the
extent to which asphaltenes adsorbed at the interface. By increasing the water fraction, the
amount of interfacial area produced that asphaltenes could potentially adsorb to also increased.
The likelihood of asphaltenes actually adsorbing depended on their aggregation state. For
instance, monomeric asphaltenes, which were formed by diluting bitumen with an aromatic
solvent, were not very surface-active and therefore tended to remain solubilized within the oil
phase. On the other hand, asphaltene aggregates, which were formed by diluting bitumen with a
more aliphatic solvent, were much more surface-active and therefore tended to readily adsorb at
the interface. While an increase in the formulation temperature did not seem to have an effect on
asphaltene adsorption, phase separation was nevertheless assisted by the enhanced drainage of
the continuous oil phase.
In Chapter 3, the added effect of naphthenic amphiphiles (naphthenic acids (NAs) and
sodium naphthenates (NaNs)) on the stability of the above emulsions was assessed. It was
revealed that under acidic conditions at pH 4, the inclusion of NAs (pre-solubilized in the oil
phase) significantly weakened the stability of governing w/o emulsions. Potential mechanisms
responsible for this behavior included the formation of mixed monolayers and mixed
aggregates. Under more basic conditions (pH 7.5 and 10), NaNs were observed to reverse the
emulsion morphology to oil-in-water (o/w) as a result of displacing asphaltenes from direct
contact with the interface. By also significantly reducing the interfacial tension (γow) of these
systems, the potential for asphaltenes to adsorb as a secondary layer at the interface was
enhanced. This proved to further worsen emulsion stability.
215
Chapter 4 assessed the hydrophilic-lipophilic nature of asphaltenic oils (bitumen,
deasphalted bitumen, asphalt, and naphthalene) as well as surface-active asphaltenes and
naphthenic amphiphiles. The obtained results showed that bitumen and toluene share a similar
hydrophobicity, which explains why they are soluble in one another. It was also demonstrated
that the asphaltene fraction of bitumen was primarily responsible for this similar hydrophobicity
as deasphalted bitumen had a hydrophobicity closer to that of hexane. With regards to the
studied surfactants, asphaltenes and NaNs were shown to be characteristically hydrophobic and
hydrophilic respectively. This supported the formed w/o and o/w emulsion droplet morphologies
of these surfactants in Chapters 2 and 3. Additionally, NAs were shown to have an intermediate
hydrophobicity. This could explain why o/w and w/o emulsion droplets were formed for
asphaltene and NA mixtures.
The stability of anionic surfactant (SDHS)-toluene (used to model the hydrophobicity of
bitumen)-water emulsions, expressed in terms of their aggregation, drainage, and coalescence
time periods, was assessed in Chapter 5 as a function of their proximity to the phase inversion
point. This proximity to the phase inversion point was quantified according to the hydrophilic-
lipophilic deviation (HLD) of related microemulsions (µEs). A notable result from this work
was that emulsion stability tended towards a minimum upon approaching the phase inversion
point (where HLD=0). Furthermore, coalescence appeared to be the rate-limiting
demulsification process for o/w (HLD<0) and w/o (HLD>0) emulsion droplets at a low SDHS
concentration (0.01 M). At larger SDHS concentrations (>0.1 M), aggregation became most
dominant. By also measuring emulsion stability at temperatures ranging from 7°C-44°C, it was
found that the “apparent” activation energies associated with drainage and coalescence were
correlated with γow and tended towards a minimum at HLD=0.
216
In Chapter 6, efforts were made to model the shape of µE droplets and their resulting
viscosity (ηµE) as a function of the HLD using a revised form of the net-average curvature
(NAC) model. To model the shape of µE droplets, it was assumed that they possess a cylindrical
core of length E
realdl, and hemispherical end caps of radius E
realdr, . According to this assumed
morphology, a smooth transition from spheres (where E
realdl, =0) to rods (where E
realdl, >> E
realdr, )
was observed upon approaching HLD=0. These µE droplet shape parameters were in turn used
by Dr. Edgar J. Acosta to predict small angle neutron scattering (SANS) profiles. Knowing how
the shape of µE droplets vary over the HLD spectrum, it was concluded that treating µE droplets
as a dilute mixture of rigid rods allowed for the accurate prediction of experimental ηµE peaks in
the nearby vicinity of HLD=0.
In Chapter 7, the NAC model was used to predict the experimental formation and
stability of the SDHS-toluene-water emulsions studied in Chapter 5 at HLD<0 and HLD>0. In
modeling the formation of these emulsions, their predicted average droplet size under turbulent
mixing conditions was matched to microscopic measurements. To model their stability, it was
assumed that the dispersed droplets collide via Brownian motion. The frequency of these
collisions was a function of the number concentration of emulsion droplets (which was taken as
a constant according to the simplified collision-coalescence-separation assumption) and ηµE.
The probability of a given collision leading to coalescence was controlled by an exponential
activation energy term. This activation energy term was modeled using the hole nucleation
theory. The key parameters of this theory include γow, the interfacial rigidity (Er), and the critical
film thickness (tH,crit) at which the formed hole fully opens rather than closes. While it has
already been demonstrated how to model γow and Er in the literature, a new approach was
introduced here for predicting tH,crit. The obtained modeling results fairly reproduced the
217
experimental emulsion stability trends. The model was also able to reproduce the stability
trends, and in some cases the absolute stability values, of other emulsions already in the
literature. Instances did however occur where modeling adjustments were made to account for
phenomena such as the added rigidity imparted by liquid crystals and surfactant multilayers.
In Chapter 8, the formation and stability of bitumen emulsions was finally revisited
using the HLD and NAC frameworks. The experimental formation of these emulsions with pure
asphaltenes and asphaltene and NaN surfactant mixtures was accurately reproduced using the
HLD model. To be able to accurately reproduce the formation of similar emulsions with
asphaltene and NA surfactant mixtures, partitioning effects need to be considered. The relative
stability of these emulsions was also accurately compared from HLD considerations alone. The
NAC model was able to further predict the γow and the emulsion droplet size for asphaltene and
NaN mixtures. Minimum stability times were also reported that did not take into account the
added effect of secondary asphaltene layers adsorbed on top of a primary adsorbed NaN layer.
219
10.1 RECOMMENDATIONS
Going forward, it is recommended that several studies be carried out to further the
conclusions drawn from this thesis. One such study involves experimentally assessing the effect
of fine clay solids (e.g. kaolinite and illite) on the stability of bitumen emulsions. These fine
clay solids are best described by the likes of Yan et al. and Jiang et al. as having a
heterogeneous surface charge distribution (and hence wettability)1,2
. It is therefore expected that
their molecular interactions with asphaltenes and naphthenic amphiphiles will vary significantly
as a function of solvent-bitumen-water ratios, solvent aromaticity, temperature, and pH.
Another study worthwhile pursuing is how the wettability of solid particles varies
according to the hydrophilic-lipophilic deviation (HLD) model. The wettability of solid particles
in a mixture of different liquids can be described as per the contact angle (θc). At θc<90º, solid
particles are hydrophilic and water-wet. At θc>90º, solid particles are conversely hydrophobic
and oil-wet. It is hypothesized that θc will vary according to HLD modifications as the
molecular interactions between the solid particles and different liquids and between the different
liquids themselves will also be impacted. These changes in molecular interactions can generally
be expressed via interfacial tensions according to Young’s equation. By better understanding
how to fine-tune the stability of solid stabilized emulsions, emulsification and/or demulsification
processes can more accurately be designed.
In next looking at the developed emulsion stability model, there are several parameters
that still require experimental validation. The most significant of these parameters is the
interfacial rigidity of the surfactant self-assembly (Er). A proposed method of indirectly
evaluating Er is by measuring the polydispersity (p2) of related microemulsion (µE) droplets. An
220
approach of this sort was formerly taken by Gradzielski et al. who alternatively related p2 to the
surfactant film’s bending (κ) and saddle-splay ( ) moduli as follows3:
Tfk
Tkp
B
B
228
2
(1)
The other parameters in this equation include the Boltzmann constant (kB), temperature
(T), and f( ), which is an entropic function of the µE droplet volume fraction. Exactly how Er is
related to κ and is not yet understood. Another possible approach for measuring Er is via the
surfactant film elasticity (ε). The reason for such is because both parameters are proportional to
the interfacial tension and available interfacial area.
An additional modeling parameter requiring experimental investigation is the critical
film thickness (tH,crit) at the onset of coalescence. This parameter is currently being
approximated as the thickness of the final layer of expelled µE droplets between approaching
emulsion droplets. It is suggested that a cryo-based imaging technique be applied to frozen
samples to validate the calculated range of tH,crit values from 3-11 nm. An example of such an
imaging technique, with a spot size resolution of 1-20 nm, is scanning electron microscopy
(SEM). SEM has been applied by Binks et al. to the nanoscale study of several emulsion types
in the past4,5
. Other possibilities include time of flight-secondary ion mass spectroscopy (ToF-
SIMS) and x-ray photoelectron spectroscopy (XPS). While the lateral resolution of these latter
imaging techniques is on the order of microns, they are able to profile a sample at a depth
resolution of 1-5 nm6,7
.
The final recommendation is to extend the emulsion stability model. The existing model
is only valid under conditions where emulsion droplet growth takes place over the entire
221
demulsification process. Under alternative conditions where aggregation, settling, film thinning,
and coalescence are less well connected, it is expected that a new set of governing
demulsification equations will apply. How to additionally incorporate complications arising
from multilayer adsorption (i.e. liquid crystals) and/or a change in the separation driving force
(i.e. centrifugation) is of even further interest. Understanding this would permit for a more
accurate prediction of the stability of bitumen emulsions.
10.2 REFERENCES
1 Yan, Z.; Elliott, J.A.W.; Masliyah, J.H. Roles of Various Bitumen Components in the Stability
of Water-in-Diluted Bitumen Emulsions. J. Colloid Interface Sci. 1999, 220, 329-337.
2 Jiang, T.; Hirasaki, G.J.; Miller, C.A.; Ng, S. Effects of Clay Wettability and Process Variables
on Separation of Diluted Bitumen Emulsions. Energy Fuels 2011, 25, 545-554.
3 Gradzielski, M.; Langevin, D.; Farago, B. Experimental Investigation of the Structure of
Nonionic Microemulsions and Their Relation to the Bending Elasticity of the Amphiphilic Film.
Phys. Rev. E: Stat. Phys., Plasmas, Fluids, Relat. Interdiscip. Top. 1996, 53, 3900-3919.
4 Binks, B.P.; Rodrigues, J.A. Enhanced Stabilization of Emulsions Due to Surfactant-Induced
Nanoparticle Flocculation. Langmuir 2007, 23, 7436-7439.
5 Binks, B.P.; Rodrigues, J.A. Double Inversion of Emulsions by Using Nanoparticles and a Di-
Chain Surfactant. Angew. Chem., Int. Ed. 2007, 46, 5389-5392,
222
6 Sodhi, R.N.S. Time-of-Flight Secondary Ion Mass Spectroscopy (ToF-SIMS): Versatility in
Chemical and Imaging Surface Analysis. Analyst 2004, 129, 483-487.
7 Cumpson, P.J. Angle-Resolved XPS and AES: Depth-Resolution Limits and a General
Comparison of Properties of Depth-Profile Reconstruction Methods. J. Electron Spectrosc.
Relat. Phenom. 1995, 73, 25-52.
223
APPENDIX 1:
THE REVISED NET CURVATURE
This chapter is derived from the following published manuscript:
Kiran, S.K.; Acosta, E.J. Predicting the Morphology and Viscosity of Microemulsions using the
HLD-NAC Model. Ind. Eng. Chem. Res. 2010, 49, 3424-3432.
224
The original definition of the net curvature (Hn) was introduced in the NAC model to
reflect the changes in the curvature of the interface with formulation conditions. Its relation to
the actual curvature of the interface was however never established1. In order to re-examine Hn,
it is useful to consider the expression for the radius of curvature (Rc) that Hwan et al. developed
for ionic microemulsions (µEs) based on changes in the electrical double layer surrounding the
head groups of ionic surfactants as a function of the electrolyte concentration2:
1
1
11
1
1
*
*
S
S
k
k
R
tail
c
(Eq. 1)
In this equation, k and k* are the inverse of the Debye length at a given electrolyte
concentration (S) and at the optimal formulation S* (where HLD=0), respectively, and δtail is the
surfactant tail length. In order to compare Hn and Rc, a normalized form of Hn is developed
based on the HLD equation, as a function of S/S*:
S
SHL n*
ln
11 (Eq. 2)
Using values of S/S* ranging from 1×10
-5 to 0.9, the normalized radius of curvature of
Hwan et al. (Rc/δtail) and the normalized net curvature (1/(L×Hn)) were calculated and are
presented in Figure 1.
225
0
5
10
15
20
0 2 4 6 8 10
Rc/δ
tail
1/(L×Hn)
Rc/δtail =2/(L Hn)
Figure 1: Comparison between the normalized radius of curvature predicted by Huang et al.
(Rc/δtail)2 and the normalized net curvature predicted as 1/(L×Hn).
According to these results, there is certainly a close correlation between the 2 normalized
curvatures which supports the idea that, as determined experimentally, the scaling factor L is
proportional to the surfactant tail length δtail. Furthermore, the comparison confirms that the
term “ln(S)” in the HLD equation reflects the effect of the electrolyte on the double layer
thickness. Finally, the solid line in Figure 1 is obtained by using the simple approximation
Rc/δtail=2/(L×Hn). Considering that L~δtail, then a revised net curvature term (H’n) can be
proposed:
c
E
w
E
o
nn
RL
HLD
rr
HH
1
2
11
2
1
2'
(Eq. 3)
According to this equation, H’n provides a better estimation of the curvature (1/Rc) of the
oil-water interface than Hn. However, it is important to keep in mind that the approximation
Rc/δtail=2/(L×Hn) is not accurate at low S/S* values. The value of Rc/δtail calculated using this
226
approximation is 20% larger than the value calculated using equation 1 when S/S*=0.4. As S/S*
tends to 1, this error approaches 0.
1 Acosta, E.; Szekeres, E.; Sabatini, D.A.; Harwell, J.H. Net-Average Curvature Model for
Solubilization and Supersolubilization in Surfactant Microemulsions. Langmuir 2003, 19, 186-
195.
2 Hwan, R.-N.; Miller, C.A.; Fort Jr., T. Determination of Microemulsion Phase Continuity and
Drop Size by Ultracentrifugation. J. Colloid Interface Sci. 1979, 68, 221-234.
228
The free energy penalty (ut) of expelling microemulsion (µE) droplet layers during the
film thinning process was modeled by Basheva et al. as follows1:
E
d
H
vdWE
d
H
oscE
d
E
d
E
d
H
tr
tu
r
tu
r
r
r
tu
2222 (Eq. 1)
In this equation, E
dr is the µE droplet radius, E
dr is the emulsion droplet radius, tH is the
emulsion droplet film thickness, and uosc and uvdW are the oscillatory and attractive van der
Waals contributions respectively. Expressions for uosc and uvdW are as follows:
1
221~4
~
21
21
20
E
d
H
oscE
d
H
E
d
H
E
d
H
oscr
tu
r
tP
r
t
r
tu
(Eq. 2)
Ed
H
Ed
Ho
r
t
r
tq
E
d
Ho
oE
d
Ho
o
oo
E
d
Hosc
w
r
t
r
tq
q
w
r
tu
21
12
1122
0 expexp2
sin2
cos12
(Eq. 3)
E
d
H
E
d
B
HHvdW
r
t
r
LTk
Atu
22
212
(Eq. 4)
In these equations, the dimensionless osmotic pressure ( P~
) is equal to
3
32
1
16
E
d
E
d
E
d
E
d
E
d
, the dimensionless excess free energy (~ ) is equal to
3
2
12
19
E
d
E
d
E
d
, w0 is equal to 265315.883439.057909.0 E
d
E
d
, ωo is equal to
3229751.830671.810586.745160.4 E
d
E
d
E
d
, qo is equal to
3259647.3037944.3764378.1978366.4 E
d
E
d
E
d
, 1 is equal to E
d
10336.240095.0 ,
229
w1 is equal to q
ow expcos~2 10 , δ is equal to 1
1
w
, π1 is equal to
oq
o
B
E
d
E
d
Tk
rp
expcos8exp6
20
3~
, the dimensionless chemical potential ( ~ ) is
equal to
32
1
398
E
d
E
d
E
d
E
d
, π0 is equal to 267381.7610572.306281.4 E
d
E
d
, 2 is
equal to 23027.23948.039687.0 E
d
E
d
, E
d
is the µE droplet volume fraction, and AH
is the effective Hamaker constant. The parameter p in the expression for π1 was left undefined
by the authors.
1 Basheva, E.S.; Kralchevsky, P.A.; Danov, K.D.; Ananthapadmanabhan, P.; Lips, A. The
Colloid Structural Forces as a Tool for Particle Characterization and Control of Dispersion
Stability. Phys. Chem. Chem. Phys. 2007, 9, 5183-5198.