Upload
independent
View
0
Download
0
Embed Size (px)
Citation preview
Band gap and trapping parameters of color tunable Yb3+/Er3+
codoped Y2O3 upconversion phosphor synthesized by combustionroute
S. Som • M. Chowdhury • S. K. Sharma
Received: 25 April 2013 / Accepted: 23 September 2013 / Published online: 10 October 2013
� Springer Science+Business Media New York 2013
Abstract This paper reports the structural, optical and
luminescence properties of Yb3?/Er3? codoped Y2O3
phosphor synthesized by combustion method. The prepared
phosphor was characterized by X-ray diffraction (XRD).
XRD studies confirm the body-centered cubic structure of
the phosphor. The optical properties such as diffuse
reflectance (DR), photoluminescence and thermolumines-
cence were studied. DR spectra were used to determine the
bandgap of the phosphor. Mechanism of upconversion by
two-photon and energy transfer processes are interpreted
and explained. The color coordinates were measured and
the color tunability was analyzed as a function of the
980 nm excitation source power. Different trapping
parameters associated with the glow peak were calculated
by various glow curve methods.
Introduction
Rare earth doped upconversion materials have been attrac-
ted intensive research attention from the past decade for
their excellent performance in the field of colorful display,
lighting source, optical communications, fluorescent labels,
biomedical imaging and upconversion lasers [1]. Recently,
a lot of research work is going on to achieve new upcon-
version materials with trivalent erbium ion (Er3?) due to
their potential applications in upconversion and near infra-
red lasers. In particular, color tunable lasers [2] have played
an important role in advancement of fundamental physics
and science. Among basic fields that employ tunable lasers
are astronomy, atomic physics, Bose–Einstein condensa-
tion, laser cooling and atomic/molecular spectroscopy. With
the advancements in nanomaterials synthesis, several com-
plementary methods have been developed to fine-tune the
upconversion emission in a broad range of color output
under single wavelength excitation (980 nm) [3]. These
methods mainly include three categories (i) lanthanide
dopant/codopant combination and their doping level
(ii) morphology and size control and (iii) input pump power.
The main interests of Er3? ion lay in its electronic energy
level scheme and long excited state lifetimes which allow for
many radiative transitions to occur and increased population
of electrons in meta-stable states by the absorption of pho-
tons in the near-infrared (NIR) region. It makes Er3? as a
suitable candidate to convert infrared light to visible effi-
ciently, which is called upconversion. Due to these unique
properties, Er3? doped materials are widely used in eye-safe
lasers, laser medical treatments and full color solid-state
displays [4, 5]. Since the absorption cross section of Er3? is
small [6] and concentration quenching happens to be at high
doping, Yb3? ion has been used as a very efficient sensitizer
[7] due to its large absorption cross section at 980 nm exci-
tation resulting an efficient energy transfer to Er3? ion. As a
result, the upconversion emission of Yb3?/Er3? codoped in
different host lattices (especially in yttrium oxide) has been
investigated extensively [8–10]. For efficient NIR to visible
frequency upconversion the host plays an important role.
Host matrices with less phonon energies are preferable for
this purpose as the energy loss due to non-radiative transi-
tions is reduced. Over the past years, yttrium oxide (Y2O3)
has been one of the best host materials owing to its good
chemical durability, thermal stability and broad optical
spectra. Its relatively low phonon cut-off energy reduces the
multiphonon relaxation process and leads to higher emission
efficiency [1]. It is one of the best host materials for Er3?
S. Som � M. Chowdhury � S. K. Sharma (&)
Department of Applied Physics, Indian School of Mines,
Dhanbad 826004, India
e-mail: [email protected]
123
J Mater Sci (2014) 49:858–867
DOI 10.1007/s10853-013-7769-8
because Er2O3 and Y2O3 have the same crystal structures
with very similar lattice constants, and Y3? and Er3? have
nearly the same ionic radii. Combustion synthesis is an
effective, low-cost method for production of Yb3?/Er3?
codoped Y2O3 upconversion phosphor. The extensive
research carried out in last 5 years emphasize the advantage
of materials development by combustion synthesis such as
energy saving and environmental protection [11]. Though,
combustion synthesis is easy method to prepare nanomate-
rials, a lot of attention is required especially in terms of
repeatability and the variation related to position of atoms/
ions in a sample.
Although Yb3?/Er3? doped Y2O3 is one of the well-
known luminescent materials, there is a comparative lack
of information about the structural and defect properties in
these materials. The luminescence properties of the mate-
rials are markedly influenced by the structure and the
presence of intrinsic and extrinsic defects/traps [12]. To
know the information about the luminescence mechanism
in this well-known upconversion material, the knowledge
of defect/trap centers, their distribution in the band struc-
ture and different trapping parameters associated with the
defects/traps are very important. Diffuse reflectance (DR)
and thermoluminescence (TL) techniques play a vital role
in getting the information about the structure, bandgap,
distribution of defects/traps within the forbidden gap
present in a material and the associated trapping parame-
ters. Keeping this in view, DR and the TL characterization
of Yb3?/Er3? codoped Y2O3 phosphor synthesized by
combustion route along with the color tunable upconver-
sion studies were carried out first time. An attempt was
made to calculate the structural parameters, bandgap and
different trapping parameters associated with the defects/
traps.
Experimental
Yb/Er codoped Y2O3 phosphor was prepared by the well-
known combustion synthesis method using erbium oxide
(Er2O3), ytterbium oxide (Yb2O3), Y2O3, nitric acid
(HNO3) and urea (CO(NH2)2) as the starting raw mate-
rials. The stock solutions of Y(NO3)3, Er(NO3)3 and
Yb(NO3)3 were prepared by dissolving Y2O3, Er2O3 and
Yb2O3 in HNO3 and diluting with deionized water. The
stock solutions of Y(NO3)3, Er(NO3)3 and Yb(NO3)3 were
mixed according to the formula (Y0.98Er0.01Yb0.01)2O3. A
suitable amount of urea was added to the mixture of
corresponding nitrate solution keeping urea to metal
nitrate molar ratio as 2.5 [13]. The corresponding mixture
was then dissolved properly to achieve a uniform solution
and dried by heating at 80 �C using magnetic stirrer.
Finally, the solid residue was transferred to silica crucible
and heated at 600 �C in a furnace for an hour. The syn-
thesis reaction was [13]:
2� 2x� 2yð ÞY NO3ð Þ3þ2xEr NO3ð Þ3þ2yYb NO3ð Þ3þ 5 NH2ð Þ2CO ! Y1�x�yErxYby
� �2O3 þ 5CO2
þ 8N2 þ 10H2O x ¼ y ¼ 0:01ð Þ:
X-ray diffractogram of the prepared phosphor was
recorded in a wide range of Bragg angle 2h using a Bruker
D8 advanced X-ray diffraction (XRD) measuring
instrument with Cu target radiation (k = 0.154056 nm).
The DR spectra were recorded using Perkin-Elmer
Lambda 35, UV–Vis spectrophotometer in the
wavelength range 200–1100 nm. The photoluminescence
upconversion spectra of the phosphor were recorded by
exciting the phosphor samples with CW 980 nm diode
laser through a monochromator attached with a photo
multiplier tube. TL studies were carried out using Harshaw
TL analyzer at Inter University Accelerator Center
(IUAC), New Delhi.
Results and discussion
Structural analysis
XRD
XRD patterns of the Yb/Er codoped Y2O3 phosphor were
recorded to investigate the structure of the prepared com-
pound and compared with the JCPDS file No. 83-0927, as
shown in Fig. 1a. The sharp and single diffraction peaks of
the XRD pattern confirm the formation of single phase
compound, which is attributed to the high in situ temper-
ature generated during the combustion reaction. The XRD
peaks were identified and indexed according to the JCPDS
database [14]. The (hkl) values are labeled on the peaks.
This implies that the codoped phosphor is of body-centered
cubic structure with space group Ia-3 and point-group
symmetry m-3. The peak at 29.5� was observed as the
strongest peak corresponding to the plane (2 2 2) and no
peaks were observed due to dopant.
Structural parameters
The structural parameters such as Miller indices, lattice
constants, crystallite size, density, dislocation density, mi-
crostrain and inter-planar spacing were determined from
XRD data. The Miller indices (hkl) were calculated by an
analytical method described elsewhere [15]. The calculated
(hkl) values were matched with the JCPDS database. The
J Mater Sci (2014) 49:858–867 859
123
lattice constants were calculated using the following for-
mula [15]:
sin2 h ¼ k2
4a2ðh2 þ k2 þ l2Þ; ð1Þ
where the terms have their usual meanings.
For estimating the crystallite size (D), Scherrer formula
[15] was used:
D ¼ 0:9kb cos h
; ð2Þ
where k is the wavelength of the X-ray radiation, b is the
full-width at half-maximum (FWHM) and h is the angle of
diffraction. The estimated crystallite size of Yb3?/Er3?
codoped Y2O3 was found to be in the range of 10–20 nm.
In the present case, broad XRD peaks were obtained.
Broadening of XRD lines was associated with small
crystallite size of coherently diffracting crystallites or
strains present within the sample or both. Small crystallites
had relatively few lattice planes that contribute to the
broadening of the diffraction lines. Broadening of the peak
might also occur due to microstraining of the crystal
structure arising from defects like dislocation and twinning
etc. These defects were considered to be associated with
the chemically synthesized materials because they grew
spontaneously during chemical reaction. As a result, the
chemical ligands got almost negligible time to be
associated with an energetically favorable site. In some
cases this might be arising due to insufficient energy that
was needed for an atom to move a proper site in forming
Fig. 1 a XRD. b Hall–Williamson plot. c TEM image for the Yb3?/Er3? codoped phosphor (Color figure online)
860 J Mater Sci (2014) 49:858–867
123
the crystallite. The strain and the crystallite size were also
calculated from the FWHMs of the diffraction peaks. The
FWHMs (b) can be expressed as a linear combination of
the contributions from the strain (e) and crystallite size (D)
through the Hall and Williamson relation [15]
b cos hk¼ 1
Dþ e sin h
k: ð3Þ
Figure 1b shows the plot of bcosh/k versus sinh/k for the
codoped Y2O3, which is almost a straight line. The
reciprocal of intercept on the bcosh/k axis gave the
average crystallite size as 18 nm. It is in good agreement
with that calculated by Scherrer formula. The slope of this
equation e implies the microstrain (e) present in the samples.
The density (Dx), dislocation density (d) and microstrain (e)were calculated using the following relations [14, 15]:
Dx ¼16M
Na3; ð4Þ
d ¼ 1
D2; ð5Þ
e ¼ b cos h4
; ð6Þ
where M is the molecular mass and N is Avogadro’s
number. The inter-planar spacing was calculated using the
following formula [15]:
d ¼ affiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffih2 þ k2 þ l2p : ð7Þ
All these calculated structural parameters are summarized
in Table 1.
TEM studies
Figure 1c depicts the TEM micrograph for the Yb/Er
codoped Y2O3 phosphor. The corresponding selected area
electron diffraction (SAED) pattern and frequency plot of
the size distribution are shown as the inset of Fig. 1c. The
phosphor shows agglomerated particles with particle size
*17 nm. The SAED pattern of the phosphor exhibits the
diffraction spots indicating a high degree of crystallinity.
The frequency plot of the size distribution was obtained by
measuring the size of a large number of particles in the
phosphor. Size distribution of the particles was found to
obey a log normal nature [16]
PðdÞ ¼ 1
drffiffiffiffiffiffi2pp exp
� ln2ðd=dÞ2r2
� �ð8Þ
Here d and r are related to the average size and the size
distribution of the particles. By fitting the frequency plot
using the above equation (solid blue line in Fig. 1c), the
average particle size of the codoped phosphor was esti-
mated 17 nm with a wide size distribution of 0.20.
Optical properties
DR
The DR spectra of the codoped Y2O3 powder phosphor were
measured against a white reference standard Spectralon. In
DR spectra, a sharp band at 209 nm was observed for the
prepared sample, as shown in Fig. 2. This corresponds to the
fact that light having this particular wavelength was absor-
bed. The band at 209 nm was due to the bandgap of the
codoped Y2O3 phosphor. Other weak bands beyond 300 nm
were also observed in the prepared sample. These bands were
due to meta-stable energy states formed between the valence
band and the conduction band by the Er3? ions.
Fig. 2 DR spectra of Yb3?/Er3? codoped phosphor (inset Bandgap
calculation)
Table 1 Structural parameters of Yb3?/Er3? codoped phosphor
Lattice constants a (A) Crystallite size D (nm) Density (Dx)
(gm/cm-3)
Dislocation density (d)
(91015 m-2)
Microstrain e (910-3)
JCPDS Calculated Debye–Scherrer Hall–Williamson’s Calculated Hall–Williamson’s
10.60 10.61 10–20 18 5.02177 3.09 2.22 5.13
J Mater Sci (2014) 49:858–867 861
123
Bandgap
The K–M theory [17] was used to calculate the bandgap of
the codoped Y2O3 phosphor using a DR spectrum. In a DR
spectrum, the ratio of the light scattered from a thick layer
of sample and an ideal non-absorbing reference sample is
measured as a function of the wavelength k, R? = Rsample/
Rreference [17]. The relation between the DR of the sample
(R?), absorption coefficient (K) and scattering coefficient
(S) is given by the K–M function
F R1ð Þ ¼ 1� R1ð Þ2
2R1¼ K
S: ð9Þ
The bandgap Eg and the linear absorption coefficient a of a
material are related through the well-known Tauc relation:
ahm ¼ C1 hm� Eg
� �n=2; ð10Þ
where m is the photon energy and C1 is a proportionality
constant. When the material scatters in perfectly diffuse
manner (or when it is illuminated at 60� incidence), the
K–M absorption coefficient K becomes equal to 2a(K = 2a). Considering the scattering coefficient S as
constant with respect to wavelength, and using Eqs. (8)
and (9), the following expression can be written as:
F R1ð Þhm ¼ C2ðhm� EgÞn: ð11Þ
The value of n is 1 for direct allowed transitions, 2 for
non-metallic materials, 3 for direct forbidden transitions,
4 for indirect allowed transition and 6 for indirect for-
bidden transition. Now, among the plot of [F(R?)hm]2,
[F(R?)hm], [F(R?)hm]2/3, [F(R?)hm]1/2, [F(R?)hm]1/3 as a
function of photon energy hm, the best fitting was
obtained with n = 1 in Eq. (10), i.e., [F(R?)hm]2 as a
function of hm indicating that the band transitions
occurred are direct in nature, as suggested by Tauc et al.
[18].
From the plot of [F(R?)hm]2 versus hm, the value of Eg is
obtained by extrapolating the linear fitted regions to
[F(R?)hm]2 = 0. The inset curve of Fig. 2 exhibits non-
linear and linear portions. The nonlinear portion corre-
sponds to a residual absorption involving impurity states
and the linear portion characterizes the fundamental
absorption. The bandgap calculated from the DR spectra
using the K–M function F(R?) was found to be 5.8 eV for
the prepared sample.
Upconversion spectra
Figure 3a shows upconversion emission spectra of Y2O3:
Yb3?, Er3? phosphor excited by a laser diode CW,
980 nm. It can be seen that there are three typical emission
bands around green and red region [19]. Each band is
composed of numerous narrow emission peaks. The sharp
peaks in the green region of 520–541 and 545–565 nm are
assigned to the transitions 2H11/2 ? 4I15/2 and 4S3/2 ? 4I15/2
of Er3? ions, respectively, while the peaks in the red
region of 650–685 nm correspond to the 4F9/2 ? 4I15/2
transition.
Upconversion mechanism
To understand the upconversion mechanism, the emission
intensity (I) of the band was recorded as a function of laser
pump power (P). Intensity of the upconversion bands fol-
lows the relation Iemission / Pn where n denotes the number
of incident photons involved in the emission of an up-
converted photon [19]. Inset of Fig. 3a shows the power
dependence for different bands. Slope of the straight line of
the log–log plot of I versus P gives the value of n. The
slope (n) was found as 1.94 for the red transition and
1.95 for the green transition. This clearly indicates the
involvement of two photons in upconversion process.
The excited states for upconversion can be populated by
several well-known mechanisms: (1) excited-state absorp-
tion (ESA), (2) energy transfer (ET) and (3) photon ava-
lanche (PA). PA was ruled out as a possible mechanism for
upconversion because no inflection point was observed in the
power dependence study [19]. Since Yb3? ions have much
larger absorption cross section compared to Er3? ions at
980 nm, the ET process dominates. Figure 3b shows the
energy level diagram of Er3? and Yb3? ions as well as the
probable upconversion mechanisms accounting for the green
and red emissions under 980 nm excitation. A 980 nm
photon excites an Yb3? ion from the ground state 2F7/2 to the
excited state 2F5/2, which may transfer the energy to a nearby
Er3? ion, promoting the Er3? ion from 4I15/2 to the 4I11/2 state,
and if the latter is already populated, the Er3? ion may transit
from the 4I11/2 to the 4F7/2 states. Subsequent nonradiative
relaxations could populate the 2H11/2 and 4S3/2 states that are
the emitting levels for the green luminescence.
4I15/2 ? 4I11/24I11/2 ? 4F7/24F7/2 ? 2H11/2/4S3/22H11/2/4S3/2 ? 4I15/2
The 4I11/2 states of Er3? ions could be depopulated by an
alternative relaxation route to 4I13/2 states, which may be
further excited to the red emitting levels 4F9/2, and the
corresponding transition to the ground state 4I15/2 produces
red emission.
4I15/2 ? 4I11/24I11/2 ? 4I13/24I13/2 ? 4F9/24F9/2 ? 4I15/2
862 J Mater Sci (2014) 49:858–867
123
Another way is also possible for red emission. The 4I11/2
states of Er3?ions could be depopulated 4F7/2 states, which
may be further excited to levels 4F7/2. Subsequent nonra-
diative relaxations could populate the red emitting levels4F9/2 which further emit red light.
4I15/2 ? 4I11/24I11/2 ? 4F7/24F7/2 ? 2H11/2/4S3/22H11/2/4S3/2 ? 4F9/24F9/2 ? 4I15/2
Photometric characterization
To measure the color of the visible emission, color coor-
dinates (x, y) were calculated by the spectrophotometric
method using the spectral energy distribution of the chro-
maticity diagram [20]. In addition, using the color coor-
dinates calculated above, the correlated color temperatures
(CCTs) of the mixed upconversion fluorescence corre-
sponding to different excitation powers were given by the
McCamy empirical formula [21]
CCT ¼ �473n3 þ 3601n2 � 6861nþ 5514:31; ð12Þ
where n = (x - xe)/(y - ye) is the inverse slop line, and the
CCT epicenter is xe = 0.3320 and ye = 0.1858 [17]. The
CIE (Commission Internationale de l’Eclairage) parameters
such as color coordinate, color correlated temperature
(CCT) and luminescence efficacy of radiation (LER) were
calculated to know the photometric characteristics of the
prepared phosphor. The CIE parameters under different
excitation powers are given in Table 2 and the color
Fig. 3 Upconversion spectra of Yb3?/Er3? codoped phosphor
J Mater Sci (2014) 49:858–867 863
123
coordinates are marked in Fig. 3c. A wide range of color
from red to yellow was achieved on varying the laser power.
The power dependence of both x and y coordinates is
plotted in Fig. 3d. The x and y CIE coordinates can be
fitted with a cubic function of the form x, f(x) = A ?
Bx ? Cx2 ? Dx3. The power dependence shows that the
x-coordinate decreases and the y-coordinate increases with
power [17]. The color tuning range of the phosphor is
shown in Fig. 3d where it can be seen that the emission
color can simply be tuned from 575 to 594 nm by
changing the excitation power from 537 to 1410 mW.
With the increase in pump power, the intensity of red and
green colors is greatly enhanced (Fig. 3a). However, the
integrated intensity ratio of red to green color decreases
significantly from 28.3 to 13.5 (Fig. 4). Figure 4 indi-
cates the increment of green color intensity at the cost
of decrement of red color intensity and so the tunability
of color is achieved from red to green with pump
power [2].
TL
To characterize the trap levels, the codoped Y2O3 phosphor
was irradiated with different c-doses and the TL glow
curves of the irradiated phosphor were recorded at different
heating rates. Thus, the effects of c-dose and heating rate
on the TL glow curves along with the determination of
trapping parameters were studied in detail.
Effect of c-dose TL glow curve of Y2O3:Yb3?, Er3?
phosphor was recorded after the c-ray irradiation with
different c-doses ranging from 1 to 5 kGy to check the
dose dependence effect on the peak position. The TL glow
curve of different c-doses for the codoped phosphor at a
constant heating rate of 5 �C s-1 is shown in Fig. 5. The
glow curve of the prepared phosphor exhibits single broad
glow peak around 320 �C for different c-doses. The shape
of the glow peak did not alter significantly with an increase
in c-ray dose. The only effect observed is the shifting of
glow peak towards lower temperature region along with an
increase in intensity of glow peak with dose.
The variation in the intensity of glow peak with irradiation
dose is shown as an inset in Fig. 5. The peak height increases
linearly with the increase of irradiation dose. The intensity of
the glow peak also increases with increasing c-doses sug-
gesting that an increasing number of traps responsible for
these glow peak were getting filled with an increase of irra-
diation dose and these traps release the charge carriers on
thermal stimulation to finally recombine with their coun-
terparts, thus giving rise to different glow peaks [22].
Effect of heating rate Figure 6 shows the TL glow curves
of the prepared Y2O3 phosphor recorded at different heat-
ing rates (3, 5 and 7 �C s-1) for the c-dose of 5 kGy. The
shift in peak temperature of the glow peak was observed
around 20 �C with heating rates and the peak shifts towards
higher temperature.
Table 2 CIE parameters of Yb3?/Er3? codoped phosphor
Power (mW) Emission color (nm) x y CCT LER
537 594 0.5917 0.4001 3199 75
618 592 0.5777 0.4145 2629 81
694 589 0.5697 0.4218 2099 84
860 585 0.5429 0.4482 1810 95
1030 580 0.5066 0.4815 1758 113
1410 575 0.4716 0.5113 1710 133
Fig. 4 Plot of pump power versus red to green ratio Fig. 5 TL glow curves of Yb3?/Er3? codoped phosphor
864 J Mater Sci (2014) 49:858–867
123
Trapping parameters
The trap levels formed after c-irradiation were character-
ized by trapping parameters such as order of kinetics, trap
depth and frequency factor [22]. TL glow curves were used
to calculate these trapping parameters. The mechanism of
recombination of detrapped charge carriers with their
counterparts is known as the order of kinetics. The loss of
dosimetry information stored in the materials after irradi-
ation is strongly dependent on the position of trapping
levels within the band gap which is known as trap depth or
activation energy (E). The frequency factor (s) represents
the product of the number of times an electron hits the wall
and the wall reflection coefficient, treating the trap as a
potential well [22]. A reliable dosimetry study of an up-
conversion phosphor is based on its trapping parameters. In
the present paper, the trapping parameters associated with
the trap levels of upconversion phosphor were calculated
by different methods.
Computerized glow curve deconvolution (CGCD)
The recorded glow curves of the prepared phosphor
exposed to 5 kGy c-irradiation dose at different heating
rates 3, 5 and 7 �C s-1 seem to be composite in nature as
they exhibit a broad peak. So, CGCD method was used to
deconvolute and calculate the trapping parameters. Here in
the present case, the glow curves of maximum c-dose
irradiated phosphors were deconvoluted by CGCD method
using TLanal computer program [23]. This computer pro-
gram is based on Halperin and Braner equations which
describe the flow of the charges between the various energy
levels during a trap emptying by thermal heating. Chung
et al. [23] derived the equation given below for TL inten-
sity by applying some physical assumptions to Halperin
and Braner equations. Assuming the free carrier concen-
tration in the conduction band (nc) to be very small com-
pared to trapped carrier concentration (n) and also the rate
of change of nc to be much smaller than the rate of change
of n, the TL intensity can be expressed as:
IðtÞ ¼ �adn
dt¼ a
n2p
nþ RðN � nÞ ; ð13Þ
where R is the ratio of the retrap and recombination coef-
ficient, N is the concentration of the available electron traps
of depth E below the conduction band and a is a scaling
factor of the detecting system. Here, p = s exp (-E/kT) is
defined as the probability per unit time of the release of an
electron from the trap and s is the frequency factor for the
escape from the traps to the conduction band. In the case of
the linear temperature rise, the above equation is called the
general one trap (GOT) equation. Although this method is
based on the GOT model, there is no restriction in the
temperature profile; this program can be used in the case
where the temperature changes linearly as well as arbi-
trarily. The software works for the deconvolution of the TL
glow curves having mixed order, first-order, second-order
and general order kinetics. It was shown that this method/
software is efficient and fast in generating TL glow peaks
and can be adopted into a numerical curve fitting [23].
The trapping parameters of trap levels were then
determined for each deconvoluted peak by this program.
The theoretically generated glow curves were fitted with
the experimental glow curves and the quality of fitting was
checked by calculating the figure of merit (FOM) for each
fitting defined by
FOM ¼P
TLExp � TLThePTLThe
ð14Þ
Fig. 6 TL glow curves at different heating rates
Fig. 7 Deconvolution of TL glow curves
J Mater Sci (2014) 49:858–867 865
123
Here TLExp and TLThe represent the TL intensity of
experimental and theoretical glow curves, respectively.
The summation extends over all the available experimental
data points. Quality of fitting and choice of appropriate
number of peaks were refined by repeating the process of
fitting to get the minimum FOM with minimum number of
possible peaks. The fits were considered adequate when the
FOM values were observed below 5 %, with most actually
being below 2 %. In the present studies, FOM was found
around 1 % which confirms a very good agreement
between theoretically generated and experimentally recor-
ded glow curves [23]. The fitted TL glow curves for ion
irradiated phosphors are shown in Fig. 7.
The order of kinetics for each deconvoluted peaks was
found as second order (b = 2). Other trapping parameters
namely trap depth (E) and frequency factor (s) for c-irra-
diated phosphor are summarized in Table 3.
Glow curve shape methods
The various methods based on the shape of the glow curve
were used to verify the above calculated trapping param-
eters of the deconvoluted peaks.
Order of kinetics (b)
According to Chen method, the following shape parameters
were calculated to get the order of kinetics [24]:
Total half intensity width (x = T2 - T1)
High temperature half width (d = T2 - Tm) and
Low temperature half width (s = Tm - T1).
Here Tm is the peak temperature, T1 and T2 are the tem-
peratures on either side of Tm corresponding to half peak
intensity. Chen introduced a symmetry factor (lg) to differ-
entiate between first- and second-order TL glow peaks:
lg = d/x = (T2 - Tm)/(T2 - T1)
lg = 0.42 for first-order kinetics
lg = 0.52 for second-order kinetics
In the present case, the value of lg for the deconvoluted
glow peaks for c-irradiated Y2O3: Yb3?/Er3? phosphors
was found to be around 0.52 indicates the existence of
second-order kinetics. Trapping parameters calculation was
done for both the deconvoluted peaks only.
Trap depth (E)
General formulae [24] for calculating trap depth (E) by
various glow curve shape methods are given by:
Ec ¼ ccðkT2
m
cÞ � bcð2kTmÞ Chenð Þ ð15Þ
Ec ¼ cckTmT1
cGrossweinerð Þ ð16Þ
Ec ¼ cckT2
m
cLuschikð Þ; ð17Þ
where c is s, d or x. Thus, trap depth was calculated by
averaging the Es, Ed and Ex values. The constants cc and bc for
the three methods for second-order kinetics are given in [24].
Frequency factor (s)
Frequency factor (s) [24] was calculated by Chen and
Winer equation after getting the trap depth (E) and order of
kinetics (b):
Table 3 Trapping parameters by CGCD method
b Peak 1 Peak 2 FOM
(%)E (eV) s (s-1) E (eV) s (s-1)
3 1.05 6.08 9 108 1.18 1.19 9 109 1.08
5 1.07 8.16 9 108 1.21 1.85 9 109 1.05
7 1.09 8.92 9 108 1.31 9.06 9 109 1.02
Table 4 Trapping parameters
by glow curve shape methodsMethods b Peak 1 Peak 2
E (eV) s (s-1) E (eV) s (s-1)
Chen 3 1.02 2.97 9 108 1.14 5.30 9 108
Grossweiner 1.03 3.71 9 108 1.13 4.31 9 108
Luschik 1.03 3.71 9 108 1.15 6.51 9 108
Chen 5 1.02 2.84 9 108 1.17 9.18 9 108
Grossweiner 1.02 2.84 9 108 1.15 6.14 9 108
Luschik 1.04 4.40 9 108 1.18 1.12 9 109
Chen 7 1.05 4.09 9 108 1.28 5.19 9 109
Grossweiner 1.05 4.09 9 108 1.26 3.52 9 109
Luschik 1.07 6.27 9 108 1.28 5.19 9 109
866 J Mater Sci (2014) 49:858–867
123
bE
kT2m
¼ s 1þ ðb� 1Þ 2KTm
E
� �exp
�E
kTm
� �: ð18Þ
The values of trap depth and frequency factor are sum-
marized in Table 4.
The composite TL glow curve of Yb/Er codoped Y2O3
phosphor in the c-dose range 1–5 kGy can be best described
as a superposition of two glow peaks which indicates two
different sets of traps were being activated having their own
trapping parameters. All the deconvoluted peaks were found
to obey second-order kinetics indicating the occurrence of
retrapping phenomena. The calculation of trapping param-
eters by various glow curve methods shows a close agree-
ment. TL glow peak shift towards higher temperature sides
with the increase in heating rate which is in good agreement
of Garlick–Gibson equation for second-order kinetics [24].
TL glow curves are always related to the defects present in
the phosphors. The two e- traps existing at 1.05 and 1.2 eV
are shown in Fig. 8 as confirmed from TL studies. The
occurrence of detrapping/retrapping phenomena during the
release of the electron is also shown in this figure. The released
electrons recombine with holes at the luminescence center
giving rise to TL. Though in some papers it is reported that the
increase in defect level concentration causes an increase in the
upconversion intensity [2], but in the present work, the up-
conversion intensity is completely related on the position of
energy levels associated with Er3? and Yb3? ions which exist
far below compared to the defect levels created by c-irradia-
tion. And hence the defect levels created by c-irradiation do
not affect the upconversion properties of this phosphor.
Conclusion
• XRD/TEM studies and quantitative calculation of
structural parameters confirm the structure of Yb/Er
codoped Y2O3 phosphor as cubic with crystallite size
10–20 nm.
• The wide bandgap (5.8 eV) of the phosphor calculated
from DR studies indicates that this phosphor can be
used as the promising candidate for applications in
different optoelectronic devices.
• The prepared phosphor offers power dependent color
tuning properties indicating its applications in color
tunable laser.
• Simple glow peak, good linearity in TL dose–response,
excellent TL sensitivity under studied c-dose range
make this upconversion phosphor suitable for radiation
dosimetry.
Acknowledgements The authors are thankful to University Grants
Commission, New Delhi, Government of India for funding this work
under Special Assistance Program No. F.530/1/DRS/2009 (SAP-I).
The authors are also thankful to Dr. S. P. Lochab, IUAC, New Delhi
for TL measurements.
References
1. Tan C, Liu Y, Han Y, Li W (2011) J Lumin 131:1198
2. Lu Q, Hou Y, Tang A, Wu H, Teng F (2013) Appl Phys Lett
102:233103
3. Pires AM, Heer S, Gudel HU (2006) J Fluoresc 16:461
4. Patra A, Saha S, Alencar MARC, Rakov N, Maciel GS (2005)
Chem Phys Lett 407:477
5. Boyer JC, Vetrone F, Capobianco JA, Speghini A, Zambelli M,
Bettinelli M (2004) J Lumin 106:263
6. Cantelar E, Sanz-Garcia JA, Cusso FJ (1999) Cryst Growth 205:196
7. Zhang J, Wang SW, Rong TJ, Chen LD (2004) J Am Ceram Soc
87:1072
8. Liu M, Wang SW, Zhang J, An LQ, Chen LD (2007) Opt Mater
29:1352
9. Vetrone F, Boyer JC, Capobianco JA, Speghini A, Bettinelli M
(2003) J Phys Chem B 107:1107
10. Liu K, Pun EYB (2009) J Alloys Compd 470:340
11. Singanahally TA, Alexander SM (2008) Curr Opin Solid State
Mater Sci 12:44
12. Singh V, Rai VK, Rak IL, Watanabe S, Rao TKG, Chubaci JFD,
Badie L, Pelle F, Ivanova S (2009) J Phys D 42:065104
13. Vu N, Anh TK, Yi G, Strek W (2007) J Lumin 122–123:776
14. Som S, Sharma SK (2012) J Phys D 45:415102
15. Cullity BD (1978) Elements of X-ray diffraction, 2nd edn.
Addison Wesley, Reading
16. Mitrikas G, Trapalis CC, Kordas G (2001) J Non-Cryst Solids
286:41
17. Morales AE, Mora ES, Pal U (2007) Rev Mex Fis 53:18
18. Tauc J, Menth A (1972) J Non-Cryst Solids 8:569
19. Guo H, Dong N, Yin M, Zhang W, Lou L, Xia S (2004) J Phys
Chem B 108:19205
20. Jayasimhadri M, Moorthy LR, Kojima K, Yamamoto K, Wada N,
Wada N (2006) J Phys D 39:635
21. McCamy CS (1992) Color Res Appl 17:142
22. Choubey A, Sharma SK, Lochab SP, Kanjilal D (2011) J Phys
Chem Solids 72:136
23. Chung KS, Choe HS, Lee JI, Kim JL (2007) Radiat Meas 42:731
24. Furetta C (2003) Handbook of thermoluminescence, 2nd edn.
World Scientific, Singapore
Fig. 8 Representation of defect levels in energy diagram
J Mater Sci (2014) 49:858–867 867
123