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Flame acceleration and DDT of hydrogeneoxygen gaseousmixtures in channels with no-slip walls
M.F. Ivanov a, A.D. Kiverin a, M.A. Liberman b,c,*a Joint Institute for High Temperatures, Russian Academy of Science, Moscow, Russiab Skobeltsyn Institute of Nuclear Physics, Moscow State University, 119991 Moscow, RussiacDepartment of Physics and Astronomy, Uppsala University, Box 516, 751 21 Uppsala, Sweden
a r t i c l e i n f o
Article history:
Received 23 January 2011
Received in revised form
18 March 2011
Accepted 22 March 2011
Available online 23 April 2011
Keywords:
Hydrogen
Flame acceleration
Shock wave
DDT
Detonation
a b s t r a c t
Hydrogeneoxygen flame acceleration and transition from deflagration to detonation (DDT)
in channels with no-slip walls were studied theoretically and using high resolution
simulations of 2D reactive NaviereStokes equations, including the effects of viscosity,
thermal conduction, molecular diffusion, real equation of state and a detailed chemical
reaction mechanism. It is shown that in “wide” channels (D> 1 mm) there are three
distinctive stages of the combustion wave propagation: the initial short stage of expo-
nential acceleration; the second stage of slower flame acceleration; the third stage of the
actual transition to detonation. In a thin channel (D< 1 mm) the flame exponential
acceleration is not bounded till the transition to detonation. While velocity of the steady
detonation waves formed in wider channels (10, 5, 3, 2 mm) is close to the Chap-
maneJouguet velocity, the oscillating detonation waves with velocities slightly below the
CJ velocity are formed in thinner channels (D< 1.0 mm). We analyse applicability of the
gradient mechanism of detonation ignition for a detailed chemical reaction model to be
a mechanism of the deflagration-to-detonation transition. The results of high resolution
simulations are fully consistent with experimental observations of flame acceleration and
DDT in hydrogeneoxygen gaseous mixtures.
Copyright ª 2011, Hydrogen Energy Publications, LLC. Published by Elsevier Ltd. All rights
reserved.
1. Introduction
Flame propagation and the deflagration-to-detonation tran-
sition (DDT) in channels have been intensively studied both
experimentally and numerically over the past decades. These
studies are inspired by their importance for industrial safety
concerns [1e3] and because their potential application for
micro-scale propulsion and power devices [4,5]. The classical
formulation of the problem in question and an experimental
set-up is an initially laminar flame, which is ignited near the
closed end of the tube and then propagates to an open end.
The flame accelerates, produces weak shocks, may become
turbulent, and eventually DDT occurs, which appears as
a sudden explosion in the vicinity of the flame front [6e14].
From the earlier studies [6,8,12,13] it was thought that the
crucial aspect for DDT is a high intensity of turbulence in the
flow ahead of the flame. A common belief was that the fast
flame acceleration and the DDT are possible only for strongly
turbulent flames. The first explanation of the flame accelera-
tion in tubes with no-slip walls before the DDT goes back to
the work by Shchelkin [13] who argued that due to the wall
friction and the thermal expansion of the burning matter the
flame front becomes curved and therefore accelerates. The
accelerating flame acts like a piston pushing compression
* Corresponding author. Department of Physics and Astronomy, Uppsala University, Box 516, 751 21 Uppsala, Sweden. Tel.: þ46 18329277.E-mail addresses: [email protected], [email protected] (M.A. Liberman).
Avai lab le at www.sc iencedi rect .com
journa l homepage : www.e lsev ie r . com/ loca te /he
i n t e rn a t i o n a l j o u r n a l o f h y d r o g e n en e r g y 3 6 ( 2 0 1 1 ) 7 7 1 4e7 7 2 7
0360-3199/$ e see front matter Copyright ª 2011, Hydrogen Energy Publications, LLC. Published by Elsevier Ltd. All rights reserved.doi:10.1016/j.ijhydene.2011.03.134
Author's personal copy
waves into the fuel mixture, which may steepen into the
shock waves. The flame acceleration in tubes with no-slip
walls has been widely accepted as an important factor that
influences the DDT [6e16].
DDT is a stochastic process meaning that there is some
uncertainty regarding time and location of the transition.
Exactly how DDT occurs may vary depending on particular
experimental conditions [6e14]. Since the work by Shchelkin
[13] it is known that the presence of obstacles along the
channel walls increases the flame acceleration and shortens
drastically the run-up distance. The experiments demon-
strated that a flame accelerates more rapidly toward the open
end if it passes through an array of turbulence-generating
baffles. This presumably was the reason why the first
attempts to explain DDT were associated with turbulent
flames and were based on assumption that DDT might occur
only in the case of turbulent flames [6,13]. Channels with
rough walls or obstacles are often used to study DDT since in
this case the run-up distance is more or less controlled [17,18].
All the same DDT occurs in channels with relatively smooth
walls [17,19] and in thin capillary tubes [20].
Over the years significant efforts have been devoted to
understand the nature of the flame acceleration and mecha-
nism of the transition from deflagration to detonation.
Although the qualitative picture of the DDT is more or less
clear, however a quantitative theory and the physical mech-
anism of DDT are still poorly understood and require better
theoretical and physical interpretation. Without a doubt the
difficulties are the turbulent burning by itself and the need to
use a detailed chemical model. The conclusions about
possible mechanism of the DDT that have been drawn from
the previous studies were based on a simplified model in
which the reaction proceeds via a single-step exothermic
reaction with Arrhenius kinetics which cannot reproduce the
main properties of the combustion such as the induction time
in chain-branching kinetics and detonation initiation. It is
therefore important to investigate the qualitative and quan-
titative differences of the processes between chain-branching
kinetics and the predictions from one-step models.
The objective of the present work is to examine effect of
the channel width on the flame dynamics and DDT in
hydrogeneoxygenmixtures in channels of different widths. It
is shown that the flame acceleration in channels with no-slip
walls is entirely determined by the features of the flow formed
ahead of the flame. It is shown that the flame dynamics prior
the transition to detonation is considerably different for the
width of the channel less than the critical one in accordance
with the experiments [20]. The results of high resolution
simulations and theoretical analysis are found to be consis-
tent with the experimental studies of the DDT in ethyl-
eneeoxygen [20] and hydrogeneoxygen [21] highly reactive
gaseous mixtures. When DDT occurred, the detonations that
developed always arose from the exponentially growing
pressure pulse, which then triggers the transition to detona-
tion according to themechanism of DDT recently proposed by
Liberman et al. [22,23]. Finally in Section 6 we discuss
a possibility of the DDT to originate due to the Zeldovich
gradient mechanism with the emphasis on comparing the
results using a detailed chemical model with previous studies
that used a one-step chemical model.
2. Formulation of the problem
The high resolution simulations modeled a flame ignited near
the closed end and then propagating to the open end of the
two-dimensional channel. The computations solved the two-
dimensional, time-dependent, reactive NaviereStokes equa-
tions for compressible flow including the effects of viscosity,
thermal conduction, molecular diffusion, the real equation of
state and detailed chemical kinetics for the reactive species
H2, O2, H, O, OH, H2O, H2O2, and HO2 with subsequent chain
branching and energy release in the form
vr
vtþ vðruÞ
vxþ vðrvÞ
vz¼ 0; (1)
vYi
vtþu
vYi
vxþv
vYi
vz¼1r
�v
vx
�rDi
vYi
vx
�þ v
vz
�rDi
vYi
vz
��þ�vYi
vt
�ch
; (2)
r
�vuvt
þ uvuvx
þ vvuvz
�¼ �vP
vxþ vsxx
vxþ vsxz
vz; (3)
r
�vvvt
þ uvvvx
þ vvvvz
�¼ �vP
vzþ vsxz
vxþ vszz
vz; (4)
r
�vEvt
þ uvEvx
þ vvEvz
�¼ �
�vðPuÞvx
þ vðPvÞvz
�þ v
vxðsxxuþ sxzvÞ
þ v
vzðszxuþ szzvÞ þ v
vx
�kðTÞvT
vx
�þ v
vz
�kðTÞvT
vz
�þXk
hk
mk
�v
vx
�rDkðTÞvYk
vx
�þ v
vz
�rDkðTÞvYk
vz
��; ð5Þ
P ¼ RBTn ¼ X
i
RB
miYi
!rT ¼ rT
Xi
RiYi; (6)
e ¼ cvTþXk
hkrk
r¼ cvTþ
Xk
hkYk; (7)
sxx ¼ 2mvuvx
� 23m
�vuvx
þ vvvz
�; (8)
szz ¼ 2mvvvz
� 23m
�vuvx
þ vvvz
�; (9)
szx ¼ sxz ¼ m
�vv
vxþ vu
vz
�: (10)
Here P, r, u, v e are pressure, mass density, x and z compo-
nents of the velocity, Yi¼ ri/r e the mass fractions of the
species, E¼ eþ (u2þ v2)/2 e the total energy density, e e the
inner energy density, RB e is the universal gas constant, mi e
the molar mass of i-species, Ri¼ RB/mi, n e the molar density,
sij e the viscous stress tensor, cv ¼Pi
cviYi e is the constant
volume specific heat, cvie the constant volume specific heat of
i-species, hi e the enthalpy of formation of i-species, k(T ) and
m(T ) are the coefficients of thermal conductivity and viscosity,
Di(T ) e is the diffusion coefficients of i-species, ðvYi=vtÞch e is
the variation of i-species concentration (mass fraction) in
chemical reactions.
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The real equations of state for the fresh mixture and
combustion products were taken with the temperature
dependenceof thespecificheats andenthalpies of eachspecies
borrowed from the JANAF tables and interpolated by the fifth-
order polynomials [24]. The transport coefficients were calcu-
lated from the first principles using the gas kinetic theory
[25,26]. The viscosity coefficients for the gaseous mixture are
m ¼ 12
"Xi
aimi þ X
i
ai
mi
!�1#; (11)
where ai ¼ ni=n is the molar fraction, mi ¼ ð5=16Þx� ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffip bmikT
q=
�pS2
i~Uð2;2Þi
��is the viscosity coefficient of i-species,
~Uð2;2Þ
e is the collision integral which is calculated using
the Lennard-Jones potential [26], bmi is the molecule mass
of the i-th species of the mixture, Si is the effective molecule
size. The thermal conductivity coefficient of the mixture is
k ¼ 12
"Xi
aiki þ X
i
ai
ki
!�1#: (12)
Coefficient of the heat conduction of i-th species ki¼ micpi/Pr
can be expressed via the viscosity mi and the Prandtl number,
which is taken Pr¼ 0.75.
The binary coefficients of diffusion are
Dij ¼ 38
ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi2pkT bmi
bmj=� bmi þ bmj
�qp$r$S2
ij~Uð1;1Þ
T�ij
;
where Sij¼ 0.5(SiþSj), Tij*¼ kT/eij*, e�ij ¼ffiffiffiffiffiffiffiffie�i e
�j
q; e* are the
constants in the expression of the Lennard-Jones potential,
and ~Uð1;1Þij is the collision integral similar to ~U
ð2;2Þ[25,26].
The diffusion coefficient of i-th species is
Di ¼ ð1� YiÞ=Xisj
ai=Dij: (13)
Variation of the concentrations Yi due to chemical reactions
is defined by system of chemical kinetics
dYi
dt¼ FiðY1;Y2;.YN;TÞ; i ¼ 1;2;.N: (14)
The right hand parts of (14) contain the rates of chemical
reactions, which depend on temperature according to the
Arrhenius law in a standard form [25]. The elementary reac-
tions of the Arrhenius type together with pre-exponential
constants and activation energies used in the simulations
are presented in Table 1.
3. Code validation: resolution andconvergence tests
The convergence of the solutions and the proper resolution to
capture details of DDT is of paramount importance, especially
when a detailed chemical mechanism is used. Thorough
convergence and resolution tests were carried out to verify
that the observed phenomena and the mechanism of DDT
remain unchanged with increasing resolution, especially
during late stages of the flame acceleration when the flame
thicknessmay decrease due to pressure rise in the flow ahead.
3.1. The numerical method and the code validation
TheNaviereStokes equations (1)e(10)were integrated using the
second-order numerical scheme based on splitting of the
Eulerian and Lagrangian stages, also known as the coarse
particlemethod (CPM) [27]. High stability of themethod is due to
dividing one time-step calculation into three stages. On the first
stage, the change of hydrodynamic characteristics on the fixed
Eulerian space grid is calculated using the explicit scheme
without regardingofmass,momentumandenergytransfer.The
hydrodynamic variables are transferred through the cell
boundaries on the second stage using the values of hydrody-
namic characteristics from the first stage. The third stage
consists of final calculation of the values of all parameters for
every cell and for thewholesystem. Itwasshown [28] that ahigh
numerical stability of the method is achieved if the hydrody-
namic variables are transferred across the grid boundary with
the velocity, which is an average value of the velocities in
neighboring grids. The overall modified solver is then the
second-orderaccurate,providinghighaccuracyof thesolutions.
The modified CPM and optimal approximation scheme were
thoroughly tested and successfully used for simulation engine
combustion knock occurrence in SI engine [28,29].
The convergence and resolution tests are shown in Figs. 1
and 2. Fig. 1 shows the convergence tests and accuracy of
calculations for different mesh resolutions for the one-
dimensional steady-state laminar flame. The meshes were
taken to resolve the structure of the flame front with 6, 8, 16,
32 and 64 computational cells, corresponding to the compu-
tational cell sizes: of 0.1, 0.05, 0.02, 0.01, 0.005 mm, respec-
tively. Fig. 1 shows that accuracy of the solution is quite
satisfactory already for 8 computational cells per flamewidth.
Even with six cells per the flame width, the flame velocity,
density and temperature differ less than 2% from the
Table 1 e Reactions and reactions rates.
Reactions Af (cm3/mol s) Eaf (kcal/mol) Ab (cm3/mol s) Eab (kcal/mol)
(R1) H2þO2¼ 2OH 2.52� 1012 39.0 1.16� 1013 21.0
(R2) OHþH2¼H2OþH 2.25� 1013 5.24 9.90� 1013 20.3
(R3) HþO2¼OHþO 1.55� 1014 16.7 1.16� 1013 0.705
(R4) H2þO¼OHþH 2.46� 1013 9.84 1.07� 1013 7.90
(R5) 2HþM¼H2þM 3.60� 1015 0.0 1.46� 1016 104.0
(R6) HþO2þM¼HO2þM 3.60� 1015 0.0 3.01� 1015 47.8
(R7) 2HO2¼H2O2þO2 1.0� 1013 0.0 1.30� 1014 40.0
(R8) 2OHþM¼H2O2þM 1.11� 1016 1.92 7.40� 1018 47.0
(R9) HþH2O2¼H2þHO2 1.17� 1014 11.8 1.55� 1014 28.5
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converged solution. With resolution of 16 computational cells
per flame width the difference between computed values and
the converged solution is negligible.
Fig. 2 shows the one-dimensional steady-state laminar
flame structure computed using four different numerical
resolutions. Themesheswere taken to resolve structure of the
flame front for temperature and concentration of species
YH2 ; YH; YOH with 6, 8, 16 and 32 computational cells per width
of the flame. The results obtained using more than 8 compu-
tational cells agree very well with the converged solution,
whereas there are some small differences between the
converged solution and the solution using 6 cells to resolve the
flame structure. Similar resolution and convergence tests
were also performed for higher initial pressures to ensure that
the resolution is adequate to capture details of DDT during
late stages.We concluded that a resolution from 8 to 12 cells is
adequate to capture details of the flame acceleration and the
mechanism of DDT.
Table 2 shows the parameters of the shocks calculated
using the RankineeHugoniot adiabatic, the experimental
parameters of hydrogeneoxygen detonation [30] and hydro-
geneoxygen flame and the corresponding parameters
computed using the code. The agreement between the theo-
retical, experimental and computed values is very good. The
slight difference of some theoretical and computed values is
because the theoretical calculations used an ideal equation of
state, while the computations used a real equation of state.
3.2. Chemical reaction scheme: sensitivity analysis
The chemical reactions are the set of ordinary differential
equations (14) for concentrations Yi of eight species H2O, H2, H,
O2, O, OH, HO2, H2O2 per computational cell. Stiff systemof the
differential equations of chemical kinetics was solved using
the Gear method [31]. Third body efficiencies for the recombi-
nation reactions were considered in way similar to paper [32].
Themass diffusivity of themixturewasmodeled using kinetic
theorywithdefault values for the Lennard-Jones characteristic
length and energy parameters for the individual species. The
viscosity and the specific heat of the mixture have been eval-
uated using mass weighted mixing laws. For the individual
species in the mixture these properties have been taken from
JANAF Tables with their temperature dependence approxi-
mated by the fifth-order polynomials.
It was found that the flame structure and the thermody-
namic characteristics of the flame and detonation are only
slightly dependent if any when different detailed chemical
schemes are used in hydrodynamic calculations. Fig. 3 shows
the induction times calculated using different chemical
kinetics schemes for H2eO2 mixture, where curves 1e6 are
calculated for the reaction schemes [33e38] and curve 7 is for
the one-step Arrhenius kinetics, respectively. It is seen that
the various detailed reaction schemes give rather similar
values of the induction times. There is some deviation in the
induction times in the temperature range 850e950 K for the
schemes [35e37] which is not significant. At the same time
there is a significant difference between the induction time
obtained from the single-step Arrhenius model and from the
detailed chemical reaction schemes. The induction time for
a single-step Arrhenius model is several orders of magnitude
0 20 40 60
0.98
1
Lf /�x
ρ b/ ρ
,b0
ρb/ρb0Tb /Tb0Uf /Uf0
Uf/U
f0T b
/ T,
b0
Fig. 1 e Convergence test for the one-dimensional steady-
state laminar flame structure. Comparisons are shown for
density, velocity and temperature normalized to their
ambient values.
T,K
0
500
1000
1500
2000
2500
3000
- 32- 16- 8- 6
Y H2
0.1
0.2
0.3
0.4
0.5
0.6
0.7
Y H
-0.05
0
0.05
0.1
0.15
0.2
0.25
x, mm
Y OH
-0.5 0 0.5
0
0.02
0.04
0.06
0.08
0.1
Fig. 2 e Resolution test for the one-dimensional steady-
state laminar flame structure. Comparisons are shown for
temperature and concentration of species YH2 ; YH; YOH
computed with 6, 8, 16 and 32 computational cells per
width of the flame.
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shorter than the induction time for the detailed chemical
models in the most important temperature range T< 1000 K.
A one-step Arrhenius model cannot reproduce the chain-
branching kinetics because in order to have a correct induc-
tion time for a one-step chemicalmodel, the activation energy
must be extremely high, but then the thickness of the reaction
zone in the flame becomes extremely thin.
Computations showed that the velocity, thickness and
adiabatic temperature of a laminar flame obtained for
different detailed chemical reaction schemes [33e38] are close
to each other with accuracy better than 10%. The flame
structure and parameters of the flame in Table 2 were repro-
duced with high accuracy using the reactive NaviereStokes
code based on the third order upwind-biased finite volume
method [39], which has been traditionally used for the spatial
discretization of theNaviereStokes equations for DNS andhas
proved to be robust for modeling complex hydrodynamic
flows [40] and combustion problems [41].
4. Effect of the channel width on the flameacceleration
Simulations of the flame propagating in channels with no-slip
walls filled with the stoichiometric H2eO2 mixture at initial
temperature and pressure T0¼ 298 K and P0¼ 1 atm were per-
formedfor thechannelsofwidthsD from10mmto0.5 mmwith
the minimum computational cell size: D¼ 0.02 mm. A laminar
planar flame was initiated near the left closed end of two-
dimensional channel and propagated to the right open end.
Fig. 4 shows the computed velocityetime dependence of
the combustion wave during the flame acceleration and the
transition to detonation in channels of widths: 0.5, 1, 3, and
5 mm. For the channels of width D> 1.0 mm, the veloc-
ityetime dependence plots demonstrate the same feature of
three distinctive stages of the flame acceleration: a short stage
of the exponential increase of the flame velocity; the second
stagewhen the acceleration rate decreases comparedwith the
first stage; the sharp increase of the flame velocity and actual
transition to detonation. On the contrary, scenario of the
flame acceleration is different for thinner channels,D< 1 mm.
The difference in dynamics of the flame acceleration in
a narrow and in awide channels is clearly seen in Figs. 5 and 6,
which show zoomed images of the velocityetime depen-
dences during the initial stages of the flame acceleration in
the channels of width D¼ 2, 3, 5, 10 mm in Fig. 5 and in the
channels of widths D¼ 0.5, 0.8, 1.0 mm plotted in Fig. 6. For
a wider channel, the initial stage which is approximated by
the exponential increase of the velocity shown by the dashed
lines in Fig. 5, turns into the stage of a slower velocity increase,
which can be described by a polynomial function
ULffaþ btn1 þ ctn2 þ/ with the exponents ni< 1. On the
contrary, in a thinner channel, D< 1 mm, the exponential
increase of the flame velocity (the dashed lines in Fig. 6) is not
bounded in time and an initially subsonic deflagration wave
may accelerate exponentially till the actual transition to
detonation.
Table 2 e Shock, detonation and flame parameters forhydrogeneoxygen.
Shock parameters Computed Theory
Pressure, bar 7.06 7.11
Density, kg/m3 1.67 1.60
Gas velocity, m/s 947.45 943.25
Mach number 2.5 2.5
Detonation parameters Computed Experiment
Initial temperature, K 300 298
D, m/s 2722 2713
Pressure ratio, p2/p0 17.3 17.3
T2, K 3463 3278
Mach number 5.05 5.05
Overdriven detonation Computed Experiment
Preheating, K 600 600
Pressure ratio, p2/p0 7.7 7.74
T2, K 3187.0 3187.6
Deflagration Computed Experiment
Flame thickness 0.32 0.26
Adiabatic temperature 3050 3100
Expansion factor 8.2 8.4
Fig. 3 e Induction times for H2eO2 mixture calculated using
different chemical kinetic schemes: curves 1e6 for the
detailed chemical kinetic schemes; curve 7 is for the one-
step Arrhenius kinetics.
t, ms
UfL
,m/s
0 0.5 10
1000
2000
3000
4000
CJ-detonation0.5
1.0 3.0 5.0
Fig. 4 e Computed H2eO2 flame velocityetime
dependences in channels of widths: 0.5, 1, 3, 5 mm.
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A propagating flame initiated near the closed end of the
channel controls the flow forming ahead of it, which results in
the flame acceleration compatible with the physical boundary
conditions. It is therefore important to examine the acceler-
ation mechanisms for a propagating flame depending on the
physical conditions such as, thickness of the boundary layer
and the velocity distribution in the flow ahead of the flame.
The feature of the flame acceleration depends on the width of
a channel with no-slip walls and influences the physical
mechanism of the transition to detonation. When the flame is
initiated near the closed end, the expansion of the high
temperature burned gas induces an outward flow of the
unburned mixture with the velocity u¼ (Q� 1)Uf ahead of the
flame front while the flame propagates with the velocity
UfL¼QUf in the laboratory reference of frame [42], where Uf is
the normal velocity of laminar flame, Q¼ ru/rbz 10 is the
density ratio of the unburned ru and burned rb gases,
respectively. Because of the wall friction the flow velocity
vanishes at the channel walls and the flow field ahead of the
flame is not uniform. Every part of the flame front moves with
respect to the unreacted mixture with normal velocity Uf and
simultaneously it is drifted with the local velocity of the flow
ahead of the flame. Thus, the flame shape is defined by the
relative motion of different parts of the flame front. As the
flame front advances into a nonuniform velocity field, the
flame surfacewill be stretched taking the shape of the velocity
profile in the flow ahead, and the flame surface will increase.
The stretched flame consumes fresh fuel over a larger surface
areawhich results in an increase in the rate of heat release per
unit projected flame area. The increase in the rate of heat
release due to the flame stretching gives rise to a higher
volumetric burning rate, and a higher effective burning
velocity based on the average heat release rate per frontal area
of the stretched flame sheet. A higher burning velocity results
in an enhancement of the flow velocity ahead of the flame,
which in turn gives rise to a larger gradient field and enhanced
flame stretching, and so on. In this way a positive feedback
coupling is established between the upstream flow and the
burning velocity as the flame is stretched in the velocity field
ahead of the flame front.
For a wide channel the flow ahead of the flame is nearly
uniform in the bulk, with the flow velocity dropping to zero at
the channel walls within a thin boundary layer of thickness:
dl�D. The flame sheet “repeats” the shape of the upstream
flow velocity profile remaining almost flat in the bulk with the
edges of the flame skirt stretched backward within the
boundary layer. Within the model of a thin flame the increase
of the burning rate (combustion wave velocity) is proportional
to the relative increase of the flame surface (length in 2D case)
which grows linearly in timewith accuracy dl/D� 1 andwhich
in turn gives rise to a larger gradient of the velocity field ahead.
Therefore the combustion wave velocity increases exponen-
tially in time, which can be presented as
UfL ¼ QUf$exp�aUft=D
�; (15)
where a is a numerical factor of the order of unity.
Expression (15) for the combustion wave velocity is similar
to the exponential increase of a finger flame velocity obtained
in [43], but the expression (15) arises due to the specific
structure of the upstream flow with a thin boundary layer
with accuracy dl/D� 1.
The accelerating flame acts as a piston producing
compression waves in the unreacted gas. The time and the
coordinate where the compression wave steepens into a shock
wave are determined by the condition that the velocity u(x,t) in
theRiemannsolution for a compressionwavebecomesamulti-
valued function [44]. From this condition, one can obtain the
distance between the flame (x¼Xf) and the coordinate (x¼Xsh)
where shock is formed (Xsh�Xf)w 5D. Then the thickness of
the boundary layer can be estimated as dlwðXsh � XfÞ=ffiffiffiffiffiffiRe
p,
whereRe¼ (Q� 1)UfD/nxQUfD/n is the Reynolds number in the
upstream flow, and n is the kinematic viscosity coefficient.
For a wide channel the condition dl/D� 1 is satisfied since
Re[ 1. In these cases the Poiseuille flow ahead of the flame is
not established until the actual transition to detonation. The
width of a channel for which the Poiseuille flow is formed
before the DDT occurs can be estimated from the condition
that thickness of the boundary layer dlw5D=ffiffiffiffiffiffiRe
pwill become
of the order of the channel width D, which gives Rew 25. For
numerical estimates it is convenient to express the Reynolds
number in terms of the flame thickness Lf and the normal
velocity of a laminar flame [42] taking into account LfUfx n
[40], so that RewQD/Lf.
t, ms
UfL
,m/s
0 0.2 0.4 0.6 0.8 10
200
400
600
23
510
Fig. 5 e Enlargement of the flame velocityetime
dependence for the channels: D[ 2, 3, 5 and 10 mm.
Dashed lines are approximations by the solution (15).
t, ms
UfL
,m/s
0 0.05 0.1 0.15 0.2 0.25 0.30
200
400
600
800
1000
1200
0.5
0.8
1.0
Fig. 6 e Enlargement of the flame velocityetime
dependence for thin channels D[ 0.5, 0.8 and 1.0 mm.
Dashed lines are exponential approximations.
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Taking for H2eO2 flame at P0¼ 1 bar: Lf¼ 0.32 mm,
Ufx 10 m/s, Qx 8, and we find out that the Poiseuille flow is
formed in the channel of width less than Dw 25Lf/Qx 1 mm
long before DDT. The qualitative difference of the flow fields
developing ahead of the flame in a “wide” channel and in
a thin channel is illustrated by Fig. 7, computed for the
channel of width D¼ 5 mm and Fig. 8 computed for the
channel D¼ 0.5 mm. The figures show the velocity contours
and the corresponding longitudinal velocity profiles (right
part) in the cross section AA of the channels.
For a flame propagating in a thin channel the parabolic
velocity profile corresponding to Poiseuille flow can be
established ahead of the flame long before the transition to
detonation occurs. In this case the combustion wave velocity
also increases exponentially similar to Eq. (15) with slightly
different value of a due to a positive feedback coupling
between the flame and the upstream flow. However, contrary
to the wide channels, in a thin channel the exponential
velocity increase is not bounded in time until the transition to
detonation. Fig. 9 shows computed values of a for the veloc-
ityetime dependence (15) for channels of widths from 0.5 mm
to 10 mm. For an ideal case, when small perturbations were
not imposed, the flame shape is symmetrical developing well
familiar tulip shape [45,46]. The corresponding values of a are
shown by the solid line with squares. For more realistic case,
when small perturbations (less then 1% of the flame velocity)
were imposed from the beginning, the shape of the flame
shown in Fig. 10 became asymmetrical, and the corresponding
values of a are shown by the solid line with the triangles. The
linewith circles is for the thin channelsD< 1 mm. It should be
stressed that in a thin capillary channels only a single-mode
(non-tulip) flame develops.
As the flame front is stretched along the walls in a wide
channel, a narrow fold is formed within the boundary layer
between the flame skirt and the wall. As the fold becomes
deeper, the angle at the fold’s tip becomes smaller, and parts
of the flame front near the fold’s tip approaches the wall. A
simple geometric consideration [47] shows that after the time
about t2wðLf=UfÞffiffiffiffiffiffiffiffiffiffiffiffiffiffiD=QLf
pthe edges of the flame skirt near the
walls will be shortened reducing the surface of the flame front
area and thus decreasing the rate of the flame acceleration.
Since this time interval is short, during the first stage the
flame acceleration is nearly constant with accuracy of the first
order terms of series expansion in Lf/D� 1. Therefore during
the next stage, t� t2, the flame velocityetime dependence can
be approximated as
UfLxQUf
1þ b
�t=sf
�n�; where 0 < n < 1: (16)
For a piston moving with the velocityetime dependence (16)
the function u(x,t) in the Riemann solution for a simple trav-
elling wave is multi-valued everywhere for any values
0< n< 1. This means that formally the compression wave
produced by the flame steepens into the shock directly on the
surface of the flame. Specific value of 0< n< 1 in expression
(16) does not matter since we are interested only in the loca-
tion where the compression wave steepens and the shock is
formed.
In contrast to a stationary flame, the flow with the accel-
erating flame is not isobaric. In the latter case pressure is
growing at about the same rate as the flame velocity. From the
time when the compression waves steepen into the shock
close to the flame front, the unreacted mixture of higher
density enters the flame front and produces a narrowpressure
pulse on the scale of the order of the flamewidth. The increase
of pressure enhances reaction rate and the heat release in the
reaction zone creating a positive feedback coupling between
the pressure pulse and the heat released in the reaction. As
a result the peak of the pressure pulse will grow exponentially
increasing the reaction rate. In a thin channel the combustion
wave velocity increases exponentially, so that the compres-
sion waves steepen into the shock at the distance about
several widths of the channel. Because of small width of the
channel, the distance to the shock is comparable to the flame
thickness. Therefore, the pressure pulse in a thin channel
increases exponentially from the beginning of the flame
acceleration. This difference in the dynamics of flame
x, mm410 420 430
5mm
A
z, mm
u, m
/ s
0 1 2 3 4 50
200
400
600
A-A
Fig. 7 e Flow field ahead of the flame front in “wide”
channel, D[ 5 mm at t[ 1 ms (left), and corresponding
velocity profile along the channel in the cross AA (right).
x, mm7 8 9 10 11
A
z, mm
u, m
/s
0 0.1 0.2 0.3 0.40
50
100
150
200
A-A0.5mm
Fig. 8 e Flow field ahead of the flame front in capillary
channel D[ 0.5 mm, at t[ 0.1 ms (left), and corresponding
velocity profile along the channel in the cross AA (right).
D,mm
α
0 2 4 6 8 10
1
1.5
2
2.5
3
3.5
Fig. 9 e Numerical factor a in the expression (15) for the
combustion wave velocity in channels D[ 0.5, 0.8, 1.0, 2, 3,
5, 10 mm. Solid lines with squares are computed for tulip
flames, solid lines with triangles are computed for
asymmetric flames, circles are for single-mode flames in
capillary channels.
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acceleration in a wide and in a thin channel is clearly seen in
the experimentally measured velocityetime dependence [20].
In simulations of H2eO2 flames there are three distinctive
stages of the flame acceleration for wide channels, D> 1 mm,
while for D< 1 mm there is only one stage of exponential
acceleration, which ends up with the transition to detonation.
For the experimental studies of ethyleneeoxygen combustion
in capillary tubes [20] the critical diameter of the tube when
the flame dynamics is changed can be estimated about
0.35e0.4 mm, taking into account that for the ethylene/
oxygen flame at atmospheric pressure, Lf¼ 0.075 mm,
Uf¼ 5.5 m/s, Q¼ 14 compared to Lf¼ 0.32 mm, Ufx 10 m/s,
Qx 8 for the flame in hydrogeneoxygen.
5. Formation of the pressure pulse and DDT
The computed overall picture of the flow, the flame develop-
ment and the transition to detonation in the channel of width
D¼ 5 mmare shown in Fig. 10 representing the time sequence
of the density gradient fields. The physical times in millisec-
onds shown for each frame in Fig. 10 are not evenly spaced but
clustered to reveal the most important details of the flame
acceleration and the transition to detonation. As it was said, in
a wider channels, D> 1 mm, if the perturbations were not
imposed the flame is developing symmetrically in a tulip
shape. The shape of the flame depends on the imposed initial
small perturbations, but the overall dynamics of the flame
acceleration is not affected by the initial small perturbations
(less than 1% of the flame velocity). Well known [19,47] sto-
chasticity of the DDT process better corresponds to the model
when small perturbations are imposed on the flame from the
beginning, so that they tend to destroy the tulip shapemaking
the flame front asymmetrical, as it is shown in Fig. 10.
Fig. 10 shows different stages of the flame acceleration and
the transition to detonation. Some frames in Fig. 10 show only
part of the computational domain adjacent to the reaction
front at selected times. The flame propagates with themoving
flow and quickly becomes convoluted and stretched along the
channel walls. The increasing flame surface area results in the
faster energy release, thus increasing the flame speed and
accelerating the flow ahead. The earliest frame at 0.15 ms
shows the perturbed flame in the left end of the computa-
tional domain and the compression waves produced by the
accelerating flame which steepen into the shocks on the right
side. As time passes, after 0.4 ms, the flame acceleration slows
down and compression waves start steepening into the
shocks in the immediate proximity ahead of the flame. During
the next stage, from 0.4 ms till 1.21 ms, the shock waves are
formed close to the flame front. They are coalesced, merged,
amplified and create a layer of compressed and heated
unreacted gas e the preheat zone [47]. During this stage the
flame consumes the unreacted mixture of considerably larger
density. As a result, a pressure pulse forms at the tip of the
flame, it strengthens and grows exponentially in time. From
1.21 ms to 1.211 ms the pressure pulse steepens into a strong
shock which is coupled with the reaction zone forming over-
driven detonation. The last frame in Fig. 10 shows the reto-
nation wave, and the overdriven detonation with
a characteristic cellular structure.
Fig. 11 presents variations of the pressure and temperature
profiles at sequential times from 0.2 ms till 1.2 ms with the
time interval 0.1 ms. The pressure pulse sits on the flame tip
which is fast accelerating. At the beginning the flame accel-
eration is a 2D effect closely related to the 2D shape of the
flame in the presence of a boundary layer. Further fast
Fig. 11 e Temperature (dashed lines) and pressure (solid
lines) profiles corresponding to leading point in the flame
front represent the flame structure and the pressure peak
formation; D[ 5 mm, time instants are from t0[ 0.2 ms,
Dt[ 0.1 ms, tf[ 1.2 ms.
Shock
0 10 20 30 40 50
x, mm30 640 650 660 6706 680
Flame Oblique shock
Detonation
0.065ms
340 350 360 370330 380
Retonation
Flame
0.2ms
0.4ms
1.2065ms
1.21ms
1.21187ms
1.2183125ms
(p ), bar /m0 4E+6 8E+6
2 2Δ
Fig. 10 e Pressure gradient at a sequential times showing
the overall flow development during transition to
detonation in channel D[ 5 mm for P0[ 1 bar. The
computational times are shown on the left of each frame.
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acceleration of the flame tip is due to coupling with the
pressure pulse. Eventually, the pressure pulse becomes strong
enough to affect reactions. The pressure pulse and the flame
appear coupled because a positive feedback between the
pressure, the reaction rate and the heat release in the reaction
zone. The pressure at which the coupling begins is around
3 atm and since this time pressure starts to grow exponen-
tially. An ignition arisingwithin the body of the pressure pulse
is synchronic with its growth, which is manifested by the
exponential in time growth of the pressure peak after 0.5 ms
shown by the dashed line in Fig. 12. Figs. 11 and 12 need to be
considered in unison to obtain a clear picture of the pressure
peak evolution, with the time and length-scales of each stage
described on the figures. It should be stressed that tempera-
ture ahead of the flame front does not exceed 600 K till
the moment of the actual transition to detonation, so that the
rates of chemical reactions are negligibly small ahead of the
flame. Thus, a temperature gradient ahead of the flame if any
cannot produce a detonation through the Zeldovich gradient
mechanism involving gradients of reactivity.
From the beginning the amplitude of the pressure pulse is
not enough for steepening effects to be important. Because of
a positive feedback between the pressure rise and the
enhanced reaction, the propagating pressure pulse grows
exponentially and simultaneously drags the reactions with it.
By the time 1.21 ms the amplitude of the pressure peak
becomes large enough, it steepens into a strong shock and
after this moment the transition to detonation occurs in less
than 1 ms. It should be noted that the pressure peak reaches
14 bar at 1.2 ms and it increases above 20 bar at 1.21 ms when
the transition to detonation starts. Such amplitude of the
pressure peak is comparable to a pressure jump across the
shock with the Mach number Mshz 5, which is close to
the strength of the leading shock in a detonation wave.
The last stage of the actual transition to detonation is
shown in Fig. 13, which presents variations of the pressure
temperature and concentration YH of H-radicals profiles at
sequential times, from t¼ 1.2101875 ms till 1.2113125 ms with
the time interval 0.25 ms for the same conditions as in Fig. 10.
The transition to detonation is clearly seen from the
steepening of the temperature profile and the increased
temperature of the products corresponding to a detonation.
One can see that the distribution of H-radicals is different for
a deflagration and after the transition to a detonation. In the
deflagration H-radicals appears within the front of the
combustion wave, while structure of the detonation wave
consists of the well pronounced shock wave with the jump in
temperature and pressure following by the reaction.
In a thin channel the overall picture of the flame velocity
evolution before the DDT differs from that in a wide channel,
but themechanism of DDT is similar to that in a wide channel
except of some details of the detonationwavewhich is formed
after the transition. Fig. 14 shows density gradient evolution at
a sequential times for the hydrogeneoxygen flame develop-
ment and the transition to detonation in channel D¼ 0.5 mm,
P0¼ 1 bar. The compression waves generated by the acceler-
ating flame steepen into the shocks at the distance compa-
rable to the width of the flame and a pocket of compressed
unreactedmixture is formed close ahead of the flame from the
very beginning. As a result, the flame consumes a fresh
mixture of higher density, and the pressure peak starts to
t, ms
p,ba
r
0 0.5 1
10
20
Fig. 12 e Peak pressure history in the channel D[ 5 mm.
Dashed line is exponential approximation on the 2nd stage
of the flame acceleration.
x, mm
T,K
p,ba
r
652 654 656
1000
2000
3000
4000
0
0.02
0.04
0.06
0.08
0.1
0.12
0
20
40
60
80pTYH
H
Fig. 13 e Pressure, temperature and H-radical
concentration distributions in the flame tip during the
actual transition to detonation in the channel D[ 5 mm
from 1.2101875 ms till 1.2113125 ms, Dt[ 0.25 ms.
0.0 4.0E+5
Δρ , kg /m2 2 7
54 55
42 43
50 51 52
t=0.1650ms
t=0.1705ms
t=0.1720ms
Fig. 14 e Density gradient at a sequential times showing
the overall hydrogeneoxygen flame development and the
transition to detonation in channel D[ 0.5 mm,
P0[ 1 atm.
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grow exponentially almost from the very beginning. Fig. 15
shows a sequence of the temperature (dashed lines) and
pressure (solid lines) profiles calculated for the flame in the
channel D¼ 0.5 mm from t0¼ 73.75 ms till tf¼ 168.75 ms with
the time interval Dt¼ 5 ms. It shows the exponential increase
of the pressure peak at the flame front until themomentwhen
the transition to detonation starts. The overall picture of the
transition is similar to what takes place in a wide channel, but
there are features associated with specific of a narrow
channel. In a narrow channel there are no shocks, which
runaway and compress the unburnedmixture far ahead of the
flame. Therefore in a narrow channel the ChapmaneJouguet
detonation is formed almost bypassing the stage of an over-
driven detonation and the overdriven detonation is much less
pronounced compared to the case of wide channels. The
characteristic detonation cell size in H2eO2 at the initial
pressure 1 atm is 2.5 mm, which is larger than the channel
width. Therefore in a thin channel a steady detonation wave
cannot be properly formed. This are presumably manifested
by the pressure and density profiles oscillations seen as the
density spikes in Fig. 16, where the density in the detonation
wave are plotted for the channel D¼ 0.5 mm, and in Fig. 17
which show time history of pressure for the same condi-
tions. The average detonation pressure is close to that for the
CJ steady detonation but the average detonation speed is
slightly less than the ChapmaneJouguet velocity and the
retonationwave ismuch less pronounced. It can be because of
the width of the channel is about 5 times less than the deto-
nation cell size and detonation is below the propagation limit.
It is possible also that this effect may be enhanced by the
hydrodynamic resistance in the narrow channels. At present
there is no enough experimental data to make a certain
judgment and the propagation of detonation in thin channels
requires more detailed study. In the present study we are
interested only in the process of the flame acceleration and
the transition from a slow combustion to a detonation regime.
Details of the propagation of a detonation wave in a thin
channel will be considered in a separate work.
6. About possible mechanism of DDT in gas-phase combustion
The question that drove this work was a particular combus-
tion problem: What are the origin and the physical mecha-
nism underlying the deflagration-to-detonation transition in
gaseous combustible mixtures? Uncontrolled DDT has enor-
mous destructive potential and the study of DDT is an
important topic associated with hydrogen and explosion
safety. There were significant prior works made in an attempt
to identify the mechanism of DDT. It was argued that the
accelerating flame creates conditions in nearby unreacted
material that lead to ignition centers in unreacted material
called “hot spots.” If local conditions in unreacted material
allow a spontaneous wave to form then this wave evolves into
a shock that is synchronized with the reaction and became
strong enough to become a detonation through the Zeldovich
gradient mechanism involving gradients of reactivity [48].
Thus the conclusion was that the mechanism of DDT is the
Zeldovich gradient mechanism. It should be emphasized that
all the previous studies of DDT used a simplified reaction
model in which the reaction proceeds via a one-step
exothermic reaction with Arrhenius kinetics. However,
Fig. 15 e Evolution of temperature (dashed lines) and
pressure (solid lines) profiles on the flame tip; D[ 0.5 mm,
time instants are from t0[ 0.07375 ms, Dt[ 0.005 ms,
tf[ 0.16875 ms.
Fig. 16 e Density profiles for the detonation evolution in
channel D[ 0.5 mm; t0[ 175 ms, tf[ 370 ms with Dt[ 5 ms.
t, ms
p,ba
r
0 0.1 0.2 0.3 0.4
10
20
30
40
50
Δt=4.625 sμ
Fig. 17 e Pressure evolution in channel D[ 0.5 mm. Period
of pressure oscillations at the detonation front is 4.625 ms.
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a one-step reaction model cannot reproduce correctly the
main properties of the combustion such as the induction time
in chain-branching kinetics and detonation initiation.
The gradient mechanism of detonation initiation proposed
by Zeldovich has been widely studied also using a simplified
chemical model of a single-step exothermic reaction with
Arrhenius kinetics (see [49] for a recent review and numerical
study of the problem). Questions then arise such as: Is the
temperature gradient can develop in unreactedmaterial ahead
of the flame that can give rise to a detonation? Is the tempera-
ture gradient inhot spots canproduce adetonation through the
Zeldovich gradientmechanism? To answer these questionswe
consider the evolution from a linear temperature gradient to
a detonation using high resolution numerical simulations for
combustible materials whose chemistry is governed by
a detailed chemical kinetics model. We employ a model which
has been widely studied representing an initial linear temper-
ature gradient in the fuel. Emphasis is on comparing the results
with that used a one-step chemical model.
The burning chemistry in fuels such as hydrogeneoxygen,
hydrogeneair and the like is governed by kinetics with chain
initiation and branching reactions corresponding to Arrhenius
kinetics with small if any energy release (typically it is slightly
endothermic), and followed by the exothermic chain termi-
nation reactions. Both these stages have well-defined times of
induction zones followed by the stage of exothermic reactions
of chain recombination or termination reactions. The main
difference between the real chain-branching reactions and
a one-step chemical model is that in a single-step Arrhenius
model the induction time is several orders of magnitude
shorter than the real induction time in the important
temperature range, T< 1200 K. In order to have a well-defined
induction zone for one-step chemistry, the activation energy
should be taken very high, but then the reaction zone becomes
exponentially thin. Another difference is that in a single-step
Arrhenius model reaction is exothermic for all temperatures,
while the chain-branching reactions are slightly endothermic
during induction stage. Therefore considerably different
results are obtained using chain-branching chemistry models
than that found for one-step chemistry. For a detonation to be
ignited the temperature gradient must be much shallower to
create a balance between the acoustic and reaction times at
some point in the evolution.
Because of limited space, we shall discuss here mainly
the case of H2eO2, more detailed studies for another fuels
will be published elsewhere. The governing equations are
the one-dimensional version of time-dependent, reactive
NaviereStokes equations (1)e(10). We consider uniform initial
conditionsapart froma linear temperaturegradient. The initial
conditions at t¼ 0, prior to ignition are constant pressure and
zero velocity of the unburned mixture. The temperature at
x¼ 0 is taken maximum and it decreases in the positive
x-direction: T¼ T0(1� ax). The temperature non-uniformity is
large enough for a detonation to ignite or fail inside the
gradient area, so we are not concerned by the conditions
outside it. The boundary condition at x¼ 0 is a reflective
boundary condition so that this boundary is a solid, reflecting
wall. Example of the detonation initiation by the steepest
temperature gradient in H2eO2 mixture at initial pressure
P0¼ 1 atmandT0¼ 1500 K calculatedusing a detailed chemical
kinetics scheme is shown in Fig. 18. The deceleration of the
spontaneous wave and its coupling with the pressure wave
Fig. 18 e Formation of detonation in the temperature
gradient for a detailed chemical model: pressure (solid
lines) and temperature (dashed lines) profiles evolution;
Dt[ 2 ms.
Fig. 19 e Formation of detonation in the temperature
gradient for one-step chemical model: pressure (solid lines)
and temperature (dashed lines) profiles evolution,
Dt[ 1 ms.
T, K
L,cm
500 1000 1500 2000 2500 30000
2
4
6
8
10
12
14
16
18
20
9 reactionsone-step
Fig. 20 e The length of the steepest temperature gradient
for initiating a detonation in H2eO2 at P0[ 1 atm.
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takes place along the gradient region where exothermal time
scale becomes higher than the induction one. For a steeper
gradient this coupling fails in the region where the induction
stage is shorter than the exothermal time scale and the
resulting will be a deflagration instead of detonation. The
evolutionof spontaneouswave calculated for the conditions in
Fig. 18 but using a one-step reactionmodel is shown in Fig. 19.
For a one-step reaction there is a heat release at the induction
stagewhichswitchesongasdynamics fromtheverybeginning
along the whole gradient, and if the gradient is sufficiently
shallowthesupersonic spontaneouswave followedby thermal
wave decelerates, couples with the pressure wave and trans-
forms into detonation. In the detailed chemical model if the
temperature gradient is sufficiently shallow so that the reac-
tion initially propagates supersonically, there are no gas
dynamic perturbations at the induction stage since the initi-
ating reactions proceed without heat release and the wave of
exothermal reaction follows the spontaneous wave path with
the delay determined by the time scale of termination reac-
tions. The result is that even when the thermal runaway point
propagates supersonically (it does so through an evolving
induction region) the thermal runaway path differs consider-
ably from the spontaneous wave path. It is seen from Figs. 18
and 19 that the length of the steepest temperature gradient
which can ignite a detonation is considerably longer compared
to the length predicted from a one-step model. The lengths of
the steepest temperature gradients, which can ignite a deto-
nation, depending on the maximum temperature at x¼ 0 for
a detailed chemicalmodel and for a one-stepmodel are shown
inFig. 20. It is seen that for temperature atx¼ 0 less than1200 K
the length of the steepest temperature gradient is at least one
or two orders of magnitude longer than that predicted from
a one-step model. In the case of lower initial pressures, or for
slower reacting mixtures, such as hydrogeneair, this differ-
ence ismuchgreater. For example, forH2eO2 at initial pressure
0.1 atm, this length already becomes several meters.
Compared to highly reactive mixtures (e.g. H2eO2, C2H4eO2)
the real ignition time forH2eair andmethaneeair differsmuch
stronger from that calculated from a one-step model. Accord-
ingly, the steepest temperature gradient which can ignite
a detonation in H2eair and methaneeair mixtures is many
orders of magnitude shallower compared to that predicted
from a one-step model. Thus, we come to the important
conclusion that thegradientof temperaturewhicharises inhot
spots and the like is very unlikely to be the DDT origin or
mechanism of the deflagration-to-detonation transition. For
example, in hydrogeneoxygen at initial pressure 0.1 atm the
temperature gradient which can ignite a detonation would
have to be several meters long, which exceeds the size of the
experimental facility.
7. Conclusions
The major conclusion of this work is that the flame acceler-
ation in tubes with no-slip walls is an important factor in
creating the right conditions for DDT to occur. Effects of the
channel width on reaction propagation and the dynamics of
reaction wave propagating in the channels of different widths
from 0.5 mm to 10 mmhave been systematically investigated.
The critical widths of the channel about 1.0 mm for hydro-
geneoxygenmixture and 0.35 mm for ethyleneeoxygen at the
atmospheric initial pressure have been obtained. It is shown
that dynamics of the hydrogeneoxygen flame before DDT is
different in wide (D> 1.0 mm) and in narrow (D< 1.0 mm)
channels and it is defined by the upstreamflowfield generated
by the accelerating flame.
Insight into how DDT occurs and what is the mechanism of
DDT was obtained by analyzing a series of high resolution
multidimensional numerical simulations with a detailed
chemical reaction model. DDT was simulated from first princi-
ples resolving the scales ranging from the size of the system to
the scales much smaller than the flame thickness. It is shown
that the shock formed close to the flame front is the primary
factor for generating exponentially growing pressure peak
whichstarts-upmechanismofDDT.Thisexponentially growing
pressure pulse then triggers the transition to DDT without the
temperature gradient involving the Zel’dovichmechanism. The
mechanism of DDT appears to be similar in both thin and wide
channels though the flame dynamics is different.
One-dimensional analysis of the detonation initiation by
a temperature gradient using a detailed chemical model
shows that in the DDT events a detonation cannot develop
through the Zeldovich’s gradient mechanism. The minimal
length of the temperature gradient capable to initiate deto-
nation obtained for a detailed chemical reaction model is
several orders of magnitude larger than that predicted from
a one-step Arrhenius model. The widely spread conclusion
drawn from previous studies, which used a single-step
chemical model, was that the detonations always arose
from hot spots in unreacted material formed ahead of accel-
erating flame and that the temperature gradient in these hot
spots is themechanism of the transition to detonation. On the
contrary, the temperature gradient cannot be a mechanism of
the deflagration-to-detonation transition simply because the
actual length of the temperature gradient which can initiate
detonation in real fuels is by orders of magnitude larger than
the size of hot spots and even size of the experimental facility.
The calculations of the present work are 2D and some
features can be expected in a 3D case, for example the tran-
sition could be faster. Another important factor that needs
careful investigation is related to turbulence. It is not very
important in the case of highly reactivemixture, but it is likely
that for slow reactive mixtures (e.g. methaneeair) DDT can be
influenced by turbulence.
Acknowledgments
This workwas supported by the Russian Agency of Innovation
(Award number No 02.740.11.5108) “Study of fundamental
processes of laminar and turbulent combustion”, and sup-
ported by the Russian Foundation of the High education. The
authors are grateful to T. Elperin, S. Frolov, M. Kuznetsov,
V. Lvov, A. Rakhimov, T. Rakhimova, N. Smirnov and
N. Zaretsky for fruitful discussions. The authors wish to thank
Nikolay Popov and Alexander Chukalovskii for insightful
discussions of different chemical schemes.M.L. is grateful to I.
Koshatskii for considerable help and useful discussions.
i n t e r n a t i o n a l j o u r n a l o f h y d r o g e n en e r g y 3 6 ( 2 0 1 1 ) 7 7 1 4e7 7 2 7 7725
Author's personal copy
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