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Journal of Luminescence 104 (2003) 77–83
Observation of free-to-acceptor-type photoluminescence in
chlorine-doped Zn(Be)Se
Y. Gua,
*, Igor L. Kuskovskya
, G.F. Neumarka
, X. Zhoub
, O. Maksimovb
,
S.P. Guob
, M.C. Tamargob
a
Department of Applied Physics and Applied Mathematics, Columbia University, 500W 120th Street, New York, NY 10027, USA
b
Department of Chemistry, City College of CUNY, New York, NY 10036, USA
Received 25 June 2002; received in revised form 21 October 2002; accepted 15 November 2002
Abstract
We present photoluminescence (PL) studies of Cl-doped Zn1ÀxBexSe (x ¼ 0–0.029) alloys performed in wide ranges
of temperature (10–296 K) and of excitation intensities. We show that the high-temperature PL is characterized by a
free-to-acceptor-type transition, involving shallow state of the localized holes. We shall show that similar transitions are
also present in comparable undoped samples, but the PL intensity is substantially lower. Finally, we show that the
ionization energy of the relevant acceptor-like species increases with Be concentration, suggesting an effective mass type
defect.
r 2002 Elsevier Science B.V. All rights reserved.
PACS: 78.55.Àm; 78.55.Et
Keywords: ZnBeSe; n-Type; MBE; Free-to-acceptor photoluminescence; ZnSe
1. Introduction
ZnSe has been of great interest for fabricating
light emitting devices in the blue–green–yellow
spectral regions. These are of interest for various
devices; in particular, the use of green solid-state
lasers with plastic optical fibers is emerging as one
of the most important applications. However, such
devices still suffer from limited lifetime; one of the
reasons is the relative weakness of the ZnSe lattice
against defect formation. The use of the
Zn1ÀxBexSe ternary alloy system has been sug-
gested [1] for improving the lattice hardness and,
as a result, the device lifetime. Therefore, recently
many investigations were performed on this alloy
material (e.g. [2,3]).
For fabrication of such light emitting devices,
both n- and p-type ZnBeSe are required; however,
few studies are available on n-type ZnBeSe. In this
paper, we discuss photoluminescence (PL) results
for our n-type Zn1ÀxBexSe : Cl and, for compar-
ison, also PL from undoped Zn1ÀxBexSe and
ZnSe. We show that at low temperatures the
dominant PL is, as expected, due to neutral donor
bound excitons, but at high temperatures the
dominant PL is due to free-to-bound (FB)
*Corresponding author. Tel.: +1-212-854-1580; fax: +1-
212-854-8257.
E-mail address: yg99@columbia.edu (Y. Gu).
0022-2313/02/$ - see front matter r 2002 Elsevier Science B.V. All rights reserved.
doi:10.1016/S0022-2313(02)00666-X
radiative recombination, which, in our case, is
believed to be due to the recombination of free
electrons and holes localized at acceptors. It is
further important that the activation energy of
such acceptors is lower than that of standard
acceptors in these materials. We shall also discuss
the change of impurity activation energies as a
function of Be composition.
2. Experimental
All our samples (thickness of about 0.8–1:0 mm)
were grown by molecular beam epitaxy (MBE) on
(0 0 1) GaAs substrates. Most of the samples had
ZnBeSe buffer layers grown before the film
deposition. All the Cl-doped samples have free
electron concentration in the range from
1016
cmÀ3
to mid-1017
cmÀ3
as measured by Hall
effect at room temperature (RT). PL measure-
ments were performed at temperatures between 10
and 296 K; using a closed cycle refrigerator
system. Samples were excited by the 325 nm
emission from a He–Cd laser with 10 mW max-
imum power (the power intensity is estimated to be
28 W=cm2
). The PL was recorded with a 3
4 m
monochromator, a thermoelectrically cooled
GaAs photomultiplier tube, and a photon counter.
3. Results and discussion
Results of low-temperature ðT ¼ 10 KÞ PL
measurements for our Cl-doped Zn1ÀxBexSe sam-
ples with x between 0 and 2.9 are shown in Fig. 1.
The spectra are all dominated by a strong, fairly
sharp, peak in the band edge region. Specifically,
for the sample with x ¼ 0 (ZnSe:Cl), the peak is
at 2:797 eV with a full-width at half-maxima
(FWHM) of about 4:9 meV: This dominant PL
has been attributed to the recombination of
neutral donor (Cl) bound excitons (usually de-
noted as I2 line) (e.g. Ref. [4]). We believe that is
also the case for the present ZnBeSe:Cl since the
PL peak positions can be easily corrected with the
change of the band gap energy due to the addition
of Be.
Next we would like to discuss the line shape of
this dominant I2 line, which exhibits a long low-
energy tail. This type of asymmetric broadening
has been previously observed in ZnSe:Cl (e.g.
Ref. [5]) and was ascribed to the Stark effect due to
the interaction between charged impurities and
bound excitons [6]. From Fig. 1, however, it also is
obvious that such broadening increases with
increasing Be concentration; thus, we suggest that
in ZnBeSe:Cl, in addition to the Stark effect, the
alloy composition fluctuations (e.g. Ref. [7]) also
contribute to the broadening.
Furthermore, in addition to the dominant PL,
we can also observe some other lines, two on the
high-energy side of the dominant line for the
ZnSe:Cl sample. Specifically, from the inset of
Fig. 2(a), one can see that they are at about
2.800 and 2:803 eV; we attribute these to the
light and heavy holes free exciton transitions,
respectively [8].
Additionally, there is a peak,1
of relatively low
intensity, at the low-energy side of the dominant
peak in all the samples, which is plotted
in Figs. 2(a) and (b) for ZnSe:Cl and
Zn0:973Be0:027Se : Cl; respectively. This small peak
T=10K
2.797eV
Zn0.971
Be0.029
Se:Cl
ZnSe:Cl
Zn0.990
Be0.010
Se:Cl
Zn0.973
Be0.027
Se:Cl
Norm.Intensity(arb.unit)
Photon Energy(eV)
2.75 2.80 2.85 2.90 2.95
Fig. 1. PL spectra of Cl-doped Zn1ÀxBexSe with x ¼ 0 to 2.9%.
1
It can be noted that in the ZnBeSe sample, where this peak
is of relatively higher intensity than in the ZnSe sample, there is
a second, smaller, peak which is presumably a phonon replica,
being about 32 meV lower in energy.
Y. Gu et al. / Journal of Luminescence 104 (2003) 77–8378
shifts weakly to the red with decreasing excitation
intensity, indicative of a donor–acceptor-pair
(DAP)-like behavior. We note that for ZnSe:Cl,
the peak position is at 2:742 eV at high excitation
intensity, and it coincides with the DAP emission
observed earlier by Sakakibara et al. [5]. In view of
this, we believe that a DAP transition is indeed the
most plausible explanation. Using [9],
hu ¼ EG À ðED þ EAÞ þ e2
=eR; ð1Þ
where hu is the emitted photon energy, EG is the
band gap energy, e2
=eR represents the Coloumb
energy between charged donors and acceptors (e is
the electronic charge, e is the dielectric constant of
the material, and R is the average distance between
a donor and an acceptor), and ED ðEAÞ is the
donor (acceptor) activation energy, and assuming
Cl as the donor (ED ¼ 27 meV [10]), we can
calculate, for any e2
=eR; the activation energy
ðEAÞ of the acceptor. Assuming that there is no
preferential paring see e.g. Ref. [34], and assuming
a Coloumb energy of 1075 meV;2
the result is EA
of 6375 meV:
We next consider evolution of the PL spectra
with temperature. We use the PL spectra from the
Zn0:99Be0:01Se : Cl as an example (Fig. 3). It is
clear that as the temperature increases, the
dominant peak becomes broader and, at first,
more symmetric until at TE180 K it becomes
asymmetric again, with a tail on the high-energy
side of the spectrum. At room temperatures
ðTX294 KÞ; the peak still maintains a relatively
high intensity with a FWHM of about 54 meV: We
plotted the integrated PL intensity of the dominant
peak as a function of excitation intensity at
different temperatures in Fig. 4; one can clearly
observe a single slope close to unity at T ¼ 10 K;
which is expected for a single excitonic transition
[13], while at an intermediate temperature
2.70 2.75 2.80 2.85
2.70 2.75 2.80 2.85 2.90
T=10K
Zn0.973
Be0.027
Se:Cl
(b)
2.756eV
2.850eV
2.788eV
⋅ 20
Norm.Intensity(arb.units)
Photon Energy (eV)
T=10K
ZnSe:Cl
(a)
2.742eV
2.797eV
⋅ 50
2.79 2.80 2.81
2.800eV
2.803eV
Fig. 2. PL spectra of ZnSe:Cl (a) and Zn0:973Be0:027Se:Cl (b) at
T ¼ 10 K: In the inset of (a), the spectrum is magnified to show
the fine structure.
2.5 2.6 2.7 2.8 2.9 3.0
Zn0.99
Be0.01
Se:Cl
T=80K
T=15K
T=150K
T=250K
T=297K
2.715eV
2.826eV
Norm.Intensity(arb.unit)
Photon Energy (eV)
Fig. 3. Temperature evolution of PL spectra of
Zn0:99Be0:01Se:Cl.
2
It is well known that the Coulomb shift depends on impurity
concentration, impurity Bohr radii, and excitation intensity.
However, as shown for instance by G. F. Neumark et al. [11],
the primary dependence is on the Bohr radius of the shallower
impurity ðaDÞ and on the excitation intensity; thus, at low-
intensity, the shift is proportional to N
1=3
maj (Eq. (9)) and to aD at
high intensity (Eq. (10)). We estimate from our laser power
ð10 mWÞ and from the optical losses in our systems that we are
in the low-intensity region. We also estimate a Bohr radius of
about 30 (A for Cl, from scaled effective mass theory (as
presented for instance in Ref. [12]). This leads to our estimated
shift of 1075 meV:
Y. Gu et al. / Journal of Luminescence 104 (2003) 77–83 79
ðTB100 KÞ; there are two distinct slopes, indicat-
ing two types of transitions [14]. Therefore, we
suggest that, in addition to the I2 line, there is
another transition beginning to emerge at some
intermediate temperature, which then becomes
dominant at T > 180 K: It is also interesting that
the peak energy of the observed PL closely follows
the band gap with the temperature, so that we
cannot resolve these two transitions; moreover, the
broadening of the PL spectra as the temperature
increases also contributes to our difficulties in
resolving these two peaks. Finally, at RT the plot
shows a single slope again, indicating only one
dominant transition. (Note that due to the power
limit of our laser, we could only measure the PL at
RT with excitation intensity varying over less than
three orders of magnitude.) This peak shows no
energy shift with changes in excitation intensity,
which excludes a donor–acceptor pair origin. We
note that since the energy of the exciton bound to
Cl in ZnSe is relatively small ðB4 meVÞ [11], the
Cl-bound excitonic transition would not be
expected to survive at such high temperatures.
Furthermore, a transition due to an exciton bound
to some accidental center deeper than Cl also
seems unlikely based on the line shape and
FWHM of the spectra.
Having excluded bound excitonic PL, we further
exclude free excitonic recombination since free
excitons are usually observed only in high-purity
semiconductors at relatively low temperatures (see
e.g. Ref. [15]); moreover, the energy separation
between the peak position and the band gap is
somewhat large—38 meV for ZnSe:Cl (using the
band gap value from Ref. [16])—compared to
20 meV; which is the typical free exciton binding
energy in ZnSe [17], and at high temperatures is
expected to be even lower due to screening effects.
Thus, we suggest, based on the line shape (see
Fig. 3) and the discussion above, that this high-
temperature transition is FB, where it is generally
assumed that the line shape is given by [18]
IðhnÞ pðhnÞ2
ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi
g½ðhn À EGðTÞ þ EIÞ=EIŠ
p
½1 þ gðhn À EGðTÞ þ EIÞ=EIŠ4
 exp hn À EGðTÞ þ EI
kBT
 
; ð2Þ
where I is the PL intensity, hn is the emitted
photon energy, g is defined as mc=mv for the free-
to-acceptor (FA) transition, and as mv=mc for the
free-to-donor (FD) transition (here mc and mv are
the electron and hole effective masses, respec-
tively), kB is the Boltzmann constant, and EGðTÞ
and EI are the band gap energy as a function of the
temperature and the impurity activation energy,
respectively.
Before using this line shape function to fit our
experimental data, first we should point out that T
is, strictly, the electron temperature rather than the
lattice temperature. However, we use the lattice
temperature values for T since it approaches the
lattice temperature at high temperatures [19].
Moreover, from Fig. 5, one can infer that the
slope of the high-energy tail of all our spectra at
T  180 K matches the corresponding value of
kBT almost exactly if T is taken as the lattice
temperature. Secondly, for fitting to ZnBeSe:Cl,
the appropriate EG is required. This, so far, has
not been well established, especially at low Be
concentrations ðo4%Þ; despite several reports, e.g.
10
-4
10
-3
10
-2
10
-1
10
0
Slope=1.13T=296K
Excitation Intensity (arb. units)
Slope=1.28
Slope=1.06T=100K
Slope=0.93
Integratedintensity(arb.unit)
T=9K
Fig. 4. Integrated PL intensity as a function laser excitation
intensity for Zn0:99Be0:01Se:Cl at T ¼ 9 K; 100 K and 296 K:
Y. Gu et al. / Journal of Luminescence 104 (2003) 77–8380
Refs. [20–23]. In Ref. [22] the direct band gap
values were obtained at RT via absorption, but
with only four data points. In other literature the
excitonic band gap values were obtained (We note
that in Ref. [21] the data are referred to as the
direct band gap; however, by extrapolating the
curve, one obtains 2:80 eV for ZnSe, which clearly
suggests that, in fact, the excitonic band gap was
obtained). Since Refs. [22,23] pertain to bulk
crystals, for our purpose we shall use values from
Refs. [20,21] corrected for the binding energy of
the ZnSe free exciton ðB20 meVÞ: We note that
only Kuskovsky et al. [20] have given more than
two data points in the range of Be concentrations
below 5%. For the temperature dependence of the
band gap, we assumed the relation for ZnBeSe to
follow that of pure ZnSe, which is given by Passler
et al. [16], since the Be compositions in our
samples are relatively low.
The resultant fit, with the parameter values
given in Table 1, is shown in Fig. 6. We note that
the experimental data is fitted very well by this
simple line shape function on the high-energy side.
However, for the low-energy tail, the fitting is
unsatisfactory. Eagles [18] observed this discre-
pancy at low temperatures in GaAs and attributed
it to the formation of a continuum of energy levels
due to impurity interactions [18]. At high tem-
peratures, other broadening mechanisms, includ-
ing phonon broadening, might set in and cause or
contribute to the deviation of the experimental
curves from the theory. Such broadening mechan-
isms can, for instance, be accounted for by
convolution with Gaussian functions due to lattice
vibrations and impurity distribution (see e.g.
Ref. [24]); however, it would dramatically increase
Table 1
Fitting parameters for samples with various Be compositions
Be (%) EI
a
(meV) EI
b
(meV) g
0 48 48 0.20
1 52 40 0.10
2.5 70 52 0.17
2.7 71 51 0.13
2.9 70 51 0.10
a
Using band gap values given by Kuskovsky et al. [20].
b
Using band gap values given by Chauvet et al. [21].
2.6 2.7 2.8 2.9 3.0
T=296K
(b)
Zn0.971
Be0.029
Se:Cl
Norm.Intensity(arb.units)
Photon Energy (eV)
2.6 2.7 2.8 2.9
T=296K
(a)
ZnSe:Cl
Fig. 6. Fitting of experimental PL spectra (solid line) at T ¼
296 K with the function (circle) given by Eq. (2): (a) ZnSe:Cl;
(b) Zn0:971Be0:029Se:Cl.
2.6 2.7 2.8 2.9 3.0
Norm.Intensity(arb.units)
Photon energy (eV)
T=297K
Slope=63.8eV
-1
1/kT=64.5eV
-1
T=250K
Slope=38.4eV
-1
1/kT=39.1eV
-1
T=200K
Slope=47.3eV
-1
1/kT=46.4eV
-1
T=180K
Slope=63.4eV
-1
1/kT=58.0eV
-1
Fig. 5. PL of one typical sample (circles) at various tempera-
tures with solid line representing the corresponding 1=kT values
(shown in the figure). The intensity in the figure is plotted in
natural log scale.
Y. Gu et al. / Journal of Luminescence 104 (2003) 77–83 81
the complexities of the fitting procedure and is not
expected to change the impurity ionization en-
ergies, which are important for our further
analysis. For a FB transition, it then remains to
be established whether it is FD or FA. In a prior
observation of this transition, in ZnSe, it was
suggested that it was FD, with holes recombining
with Cl donors located in the tail of a presumed
impurity band [25]. However, this explanation
seems unlikely for a number of reasons. First, we
also observed such PL in our undoped samples
(with much lower intensity) and samples with low
Cl concentration ðB1016
cmÀ3
Þ; where no such
impurity band is expected. Secondly, we note that
the impurity activation energy obtained from our
fitting for ZnSe:Cl (see Table 1), is 48 meV;
appreciably higher than the Cl activation energy
in ZnSe (B27 meV [11]). Moreover, one would
expect the actual Cl donor activation energy at RT
to be even lower than 27 meV due to the screening
(for effects of screening on impurity ionization
energies, see e.g. Refs. [26,27] and references
therein); indeed, formal application of screening
theory to Cl gives zero activation energy for our
samples with free electron concentrations
B5 Â 1017
cmÀ3
;3
where this type of PL is still
observed, which clearly excludes Cl as the parti-
cipating donor for this PL. We further note that
the fit shown in Fig. 6 was obtained with g values
of about 0.1–0.2. Since such values are appropriate
for acceptors ðmc=mvB0:19 for ZnSe assuming
that mc ¼ 0:15m0 and mv ¼ 0:78m0 [29]), and since
we observed that the fit was very sensitive to the g
value, we attribute this transition to a free electron
to acceptor recombination. This then leaves the
puzzle that the activation energy (48 meV for
ZnSe:Cl) is lower than that ð 100 meVÞ of
‘‘standard’’ acceptors in ZnSe ðLi; Na; NÞ; how-
ever, lower-than-standard values have already
been previously reported (e.g. 56 meV for an
unknown acceptor in undoped ZnSe [30], and
85 meV for P acceptors in p-type ZnSe [31]). We
note again that the acceptor activation energy
obtained by ascribing the 2:742 eV ZnSe:Cl peak
to a DAP peak (at 10 K) is 6375 meV; which is
relatively close to the 48 meV obtained at RT from
the FB fitting. The difference between these two
energies ðB15 meVÞ can be accounted for by
screening.4
Additionally, for ZnBeSe:Cl this en-
ergy difference is also in the range of 15B17 meV;
if one uses band gap values consistently. There-
fore, we believe that the FA transition is the most
likely mechanism for this PL. The observation of
the same PL in undoped samples but with much
lower intensities (more than two orders of
magnitude) can be explained as follows: first, the
free electron concentration in the Cl-doped (n-
type) sample is much higher than that in the
undoped sample, and as a result, the recombina-
tion involving free electrons and acceptor-type
centers would be much more significant. Secondly,
the concentration of this acceptor-type species
might increase as Cl is introduced into Zn(Be)Se,
which can also contribute to higher PL intensity in
Cl-doped samples.
The origin of this acceptor-type species still remains
unclear at this point. However, since the PL is also
present in undoped samples, it may well be a native-
type defect, although the possibility of a pervasive
cantaminant cannot be excluded at this time.
By fitting the FA spectra, we also obtained the
acceptor activation energy as a function of Be
concentration (see Table 1); the trend is that the
activation energy generally increases with Be
composition. This can be qualitatively explained
as follows. It is well known that the dielectric
constant decreases with increasing band gap (see
e.g. Ref. [33] for a good qualitative discussion as
well as a simple theoretical approach). Further-
more, according to the standard effective-mass
theory (see e.g. Ref. [15]), the effective mass
generally increases as the band gap increases.
Therefore, for an effective-mass-type impurity, its
activation energy would increase with the band
gap (i.e. with increasing Be), both because of a
decrease in the dielectric constant and an increase
in effective mass.
3
We calculated the Cl activation energy to approach zero for
samples with ½nŠB5 Â 1017
cmÀ3
; using the theory developed by
J.B. Krieger [28] and G.F. Neumark [26].
4
It has been observed by Bowers et al. [32] that in p-type
ZnSe:N the donor activation energy also decreased; the change
is as high as 22% (from 31 to 24 meV) when T increases from
77 K to RT.
Y. Gu et al. / Journal of Luminescence 104 (2003) 77–8382
4. Conclusions
We have performed a PL study of Cl-doped
Zn(Be)Se. The low-temperature PL is, as expected,
dominated by the Cl-bound excitonic transitions.
As the temperature increases, the PL begins to be
dominated by FB transitions. By analyzing the PL
spectra at various temperatures, we conclude that
the species involved in this transition is of
acceptor-type. Interestingly, we also observed the
same type of PL in undoped samples. We also
found that the activation energy of this species
increases with Be concentration, which can be
accounted for by the decrease of the dielectric
constant and of the increase in effective mass with
increasing Be. However, the origin of this accep-
tor-type species is still unclear at this point and
needs further study.
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Observation of free-to-acceptor-type photoluminescence in chlorine-doped Zn(Be)Se

  • 1. Journal of Luminescence 104 (2003) 77–83 Observation of free-to-acceptor-type photoluminescence in chlorine-doped Zn(Be)Se Y. Gua, *, Igor L. Kuskovskya , G.F. Neumarka , X. Zhoub , O. Maksimovb , S.P. Guob , M.C. Tamargob a Department of Applied Physics and Applied Mathematics, Columbia University, 500W 120th Street, New York, NY 10027, USA b Department of Chemistry, City College of CUNY, New York, NY 10036, USA Received 25 June 2002; received in revised form 21 October 2002; accepted 15 November 2002 Abstract We present photoluminescence (PL) studies of Cl-doped Zn1ÀxBexSe (x ¼ 0–0.029) alloys performed in wide ranges of temperature (10–296 K) and of excitation intensities. We show that the high-temperature PL is characterized by a free-to-acceptor-type transition, involving shallow state of the localized holes. We shall show that similar transitions are also present in comparable undoped samples, but the PL intensity is substantially lower. Finally, we show that the ionization energy of the relevant acceptor-like species increases with Be concentration, suggesting an effective mass type defect. r 2002 Elsevier Science B.V. All rights reserved. PACS: 78.55.Àm; 78.55.Et Keywords: ZnBeSe; n-Type; MBE; Free-to-acceptor photoluminescence; ZnSe 1. Introduction ZnSe has been of great interest for fabricating light emitting devices in the blue–green–yellow spectral regions. These are of interest for various devices; in particular, the use of green solid-state lasers with plastic optical fibers is emerging as one of the most important applications. However, such devices still suffer from limited lifetime; one of the reasons is the relative weakness of the ZnSe lattice against defect formation. The use of the Zn1ÀxBexSe ternary alloy system has been sug- gested [1] for improving the lattice hardness and, as a result, the device lifetime. Therefore, recently many investigations were performed on this alloy material (e.g. [2,3]). For fabrication of such light emitting devices, both n- and p-type ZnBeSe are required; however, few studies are available on n-type ZnBeSe. In this paper, we discuss photoluminescence (PL) results for our n-type Zn1ÀxBexSe : Cl and, for compar- ison, also PL from undoped Zn1ÀxBexSe and ZnSe. We show that at low temperatures the dominant PL is, as expected, due to neutral donor bound excitons, but at high temperatures the dominant PL is due to free-to-bound (FB) *Corresponding author. Tel.: +1-212-854-1580; fax: +1- 212-854-8257. E-mail address: yg99@columbia.edu (Y. Gu). 0022-2313/02/$ - see front matter r 2002 Elsevier Science B.V. All rights reserved. doi:10.1016/S0022-2313(02)00666-X
  • 2. radiative recombination, which, in our case, is believed to be due to the recombination of free electrons and holes localized at acceptors. It is further important that the activation energy of such acceptors is lower than that of standard acceptors in these materials. We shall also discuss the change of impurity activation energies as a function of Be composition. 2. Experimental All our samples (thickness of about 0.8–1:0 mm) were grown by molecular beam epitaxy (MBE) on (0 0 1) GaAs substrates. Most of the samples had ZnBeSe buffer layers grown before the film deposition. All the Cl-doped samples have free electron concentration in the range from 1016 cmÀ3 to mid-1017 cmÀ3 as measured by Hall effect at room temperature (RT). PL measure- ments were performed at temperatures between 10 and 296 K; using a closed cycle refrigerator system. Samples were excited by the 325 nm emission from a He–Cd laser with 10 mW max- imum power (the power intensity is estimated to be 28 W=cm2 ). The PL was recorded with a 3 4 m monochromator, a thermoelectrically cooled GaAs photomultiplier tube, and a photon counter. 3. Results and discussion Results of low-temperature ðT ¼ 10 KÞ PL measurements for our Cl-doped Zn1ÀxBexSe sam- ples with x between 0 and 2.9 are shown in Fig. 1. The spectra are all dominated by a strong, fairly sharp, peak in the band edge region. Specifically, for the sample with x ¼ 0 (ZnSe:Cl), the peak is at 2:797 eV with a full-width at half-maxima (FWHM) of about 4:9 meV: This dominant PL has been attributed to the recombination of neutral donor (Cl) bound excitons (usually de- noted as I2 line) (e.g. Ref. [4]). We believe that is also the case for the present ZnBeSe:Cl since the PL peak positions can be easily corrected with the change of the band gap energy due to the addition of Be. Next we would like to discuss the line shape of this dominant I2 line, which exhibits a long low- energy tail. This type of asymmetric broadening has been previously observed in ZnSe:Cl (e.g. Ref. [5]) and was ascribed to the Stark effect due to the interaction between charged impurities and bound excitons [6]. From Fig. 1, however, it also is obvious that such broadening increases with increasing Be concentration; thus, we suggest that in ZnBeSe:Cl, in addition to the Stark effect, the alloy composition fluctuations (e.g. Ref. [7]) also contribute to the broadening. Furthermore, in addition to the dominant PL, we can also observe some other lines, two on the high-energy side of the dominant line for the ZnSe:Cl sample. Specifically, from the inset of Fig. 2(a), one can see that they are at about 2.800 and 2:803 eV; we attribute these to the light and heavy holes free exciton transitions, respectively [8]. Additionally, there is a peak,1 of relatively low intensity, at the low-energy side of the dominant peak in all the samples, which is plotted in Figs. 2(a) and (b) for ZnSe:Cl and Zn0:973Be0:027Se : Cl; respectively. This small peak T=10K 2.797eV Zn0.971 Be0.029 Se:Cl ZnSe:Cl Zn0.990 Be0.010 Se:Cl Zn0.973 Be0.027 Se:Cl Norm.Intensity(arb.unit) Photon Energy(eV) 2.75 2.80 2.85 2.90 2.95 Fig. 1. PL spectra of Cl-doped Zn1ÀxBexSe with x ¼ 0 to 2.9%. 1 It can be noted that in the ZnBeSe sample, where this peak is of relatively higher intensity than in the ZnSe sample, there is a second, smaller, peak which is presumably a phonon replica, being about 32 meV lower in energy. Y. Gu et al. / Journal of Luminescence 104 (2003) 77–8378
  • 3. shifts weakly to the red with decreasing excitation intensity, indicative of a donor–acceptor-pair (DAP)-like behavior. We note that for ZnSe:Cl, the peak position is at 2:742 eV at high excitation intensity, and it coincides with the DAP emission observed earlier by Sakakibara et al. [5]. In view of this, we believe that a DAP transition is indeed the most plausible explanation. Using [9], hu ¼ EG À ðED þ EAÞ þ e2 =eR; ð1Þ where hu is the emitted photon energy, EG is the band gap energy, e2 =eR represents the Coloumb energy between charged donors and acceptors (e is the electronic charge, e is the dielectric constant of the material, and R is the average distance between a donor and an acceptor), and ED ðEAÞ is the donor (acceptor) activation energy, and assuming Cl as the donor (ED ¼ 27 meV [10]), we can calculate, for any e2 =eR; the activation energy ðEAÞ of the acceptor. Assuming that there is no preferential paring see e.g. Ref. [34], and assuming a Coloumb energy of 1075 meV;2 the result is EA of 6375 meV: We next consider evolution of the PL spectra with temperature. We use the PL spectra from the Zn0:99Be0:01Se : Cl as an example (Fig. 3). It is clear that as the temperature increases, the dominant peak becomes broader and, at first, more symmetric until at TE180 K it becomes asymmetric again, with a tail on the high-energy side of the spectrum. At room temperatures ðTX294 KÞ; the peak still maintains a relatively high intensity with a FWHM of about 54 meV: We plotted the integrated PL intensity of the dominant peak as a function of excitation intensity at different temperatures in Fig. 4; one can clearly observe a single slope close to unity at T ¼ 10 K; which is expected for a single excitonic transition [13], while at an intermediate temperature 2.70 2.75 2.80 2.85 2.70 2.75 2.80 2.85 2.90 T=10K Zn0.973 Be0.027 Se:Cl (b) 2.756eV 2.850eV 2.788eV ⋅ 20 Norm.Intensity(arb.units) Photon Energy (eV) T=10K ZnSe:Cl (a) 2.742eV 2.797eV ⋅ 50 2.79 2.80 2.81 2.800eV 2.803eV Fig. 2. PL spectra of ZnSe:Cl (a) and Zn0:973Be0:027Se:Cl (b) at T ¼ 10 K: In the inset of (a), the spectrum is magnified to show the fine structure. 2.5 2.6 2.7 2.8 2.9 3.0 Zn0.99 Be0.01 Se:Cl T=80K T=15K T=150K T=250K T=297K 2.715eV 2.826eV Norm.Intensity(arb.unit) Photon Energy (eV) Fig. 3. Temperature evolution of PL spectra of Zn0:99Be0:01Se:Cl. 2 It is well known that the Coulomb shift depends on impurity concentration, impurity Bohr radii, and excitation intensity. However, as shown for instance by G. F. Neumark et al. [11], the primary dependence is on the Bohr radius of the shallower impurity ðaDÞ and on the excitation intensity; thus, at low- intensity, the shift is proportional to N 1=3 maj (Eq. (9)) and to aD at high intensity (Eq. (10)). We estimate from our laser power ð10 mWÞ and from the optical losses in our systems that we are in the low-intensity region. We also estimate a Bohr radius of about 30 (A for Cl, from scaled effective mass theory (as presented for instance in Ref. [12]). This leads to our estimated shift of 1075 meV: Y. Gu et al. / Journal of Luminescence 104 (2003) 77–83 79
  • 4. ðTB100 KÞ; there are two distinct slopes, indicat- ing two types of transitions [14]. Therefore, we suggest that, in addition to the I2 line, there is another transition beginning to emerge at some intermediate temperature, which then becomes dominant at T > 180 K: It is also interesting that the peak energy of the observed PL closely follows the band gap with the temperature, so that we cannot resolve these two transitions; moreover, the broadening of the PL spectra as the temperature increases also contributes to our difficulties in resolving these two peaks. Finally, at RT the plot shows a single slope again, indicating only one dominant transition. (Note that due to the power limit of our laser, we could only measure the PL at RT with excitation intensity varying over less than three orders of magnitude.) This peak shows no energy shift with changes in excitation intensity, which excludes a donor–acceptor pair origin. We note that since the energy of the exciton bound to Cl in ZnSe is relatively small ðB4 meVÞ [11], the Cl-bound excitonic transition would not be expected to survive at such high temperatures. Furthermore, a transition due to an exciton bound to some accidental center deeper than Cl also seems unlikely based on the line shape and FWHM of the spectra. Having excluded bound excitonic PL, we further exclude free excitonic recombination since free excitons are usually observed only in high-purity semiconductors at relatively low temperatures (see e.g. Ref. [15]); moreover, the energy separation between the peak position and the band gap is somewhat large—38 meV for ZnSe:Cl (using the band gap value from Ref. [16])—compared to 20 meV; which is the typical free exciton binding energy in ZnSe [17], and at high temperatures is expected to be even lower due to screening effects. Thus, we suggest, based on the line shape (see Fig. 3) and the discussion above, that this high- temperature transition is FB, where it is generally assumed that the line shape is given by [18] IðhnÞ pðhnÞ2 ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi g½ðhn À EGðTÞ þ EIÞ=EIŠ p ½1 þ gðhn À EGðTÞ þ EIÞ=EIŠ4  exp À hn À EGðTÞ þ EI kBT ; ð2Þ where I is the PL intensity, hn is the emitted photon energy, g is defined as mc=mv for the free- to-acceptor (FA) transition, and as mv=mc for the free-to-donor (FD) transition (here mc and mv are the electron and hole effective masses, respec- tively), kB is the Boltzmann constant, and EGðTÞ and EI are the band gap energy as a function of the temperature and the impurity activation energy, respectively. Before using this line shape function to fit our experimental data, first we should point out that T is, strictly, the electron temperature rather than the lattice temperature. However, we use the lattice temperature values for T since it approaches the lattice temperature at high temperatures [19]. Moreover, from Fig. 5, one can infer that the slope of the high-energy tail of all our spectra at T 180 K matches the corresponding value of kBT almost exactly if T is taken as the lattice temperature. Secondly, for fitting to ZnBeSe:Cl, the appropriate EG is required. This, so far, has not been well established, especially at low Be concentrations ðo4%Þ; despite several reports, e.g. 10 -4 10 -3 10 -2 10 -1 10 0 Slope=1.13T=296K Excitation Intensity (arb. units) Slope=1.28 Slope=1.06T=100K Slope=0.93 Integratedintensity(arb.unit) T=9K Fig. 4. Integrated PL intensity as a function laser excitation intensity for Zn0:99Be0:01Se:Cl at T ¼ 9 K; 100 K and 296 K: Y. Gu et al. / Journal of Luminescence 104 (2003) 77–8380
  • 5. Refs. [20–23]. In Ref. [22] the direct band gap values were obtained at RT via absorption, but with only four data points. In other literature the excitonic band gap values were obtained (We note that in Ref. [21] the data are referred to as the direct band gap; however, by extrapolating the curve, one obtains 2:80 eV for ZnSe, which clearly suggests that, in fact, the excitonic band gap was obtained). Since Refs. [22,23] pertain to bulk crystals, for our purpose we shall use values from Refs. [20,21] corrected for the binding energy of the ZnSe free exciton ðB20 meVÞ: We note that only Kuskovsky et al. [20] have given more than two data points in the range of Be concentrations below 5%. For the temperature dependence of the band gap, we assumed the relation for ZnBeSe to follow that of pure ZnSe, which is given by Passler et al. [16], since the Be compositions in our samples are relatively low. The resultant fit, with the parameter values given in Table 1, is shown in Fig. 6. We note that the experimental data is fitted very well by this simple line shape function on the high-energy side. However, for the low-energy tail, the fitting is unsatisfactory. Eagles [18] observed this discre- pancy at low temperatures in GaAs and attributed it to the formation of a continuum of energy levels due to impurity interactions [18]. At high tem- peratures, other broadening mechanisms, includ- ing phonon broadening, might set in and cause or contribute to the deviation of the experimental curves from the theory. Such broadening mechan- isms can, for instance, be accounted for by convolution with Gaussian functions due to lattice vibrations and impurity distribution (see e.g. Ref. [24]); however, it would dramatically increase Table 1 Fitting parameters for samples with various Be compositions Be (%) EI a (meV) EI b (meV) g 0 48 48 0.20 1 52 40 0.10 2.5 70 52 0.17 2.7 71 51 0.13 2.9 70 51 0.10 a Using band gap values given by Kuskovsky et al. [20]. b Using band gap values given by Chauvet et al. [21]. 2.6 2.7 2.8 2.9 3.0 T=296K (b) Zn0.971 Be0.029 Se:Cl Norm.Intensity(arb.units) Photon Energy (eV) 2.6 2.7 2.8 2.9 T=296K (a) ZnSe:Cl Fig. 6. Fitting of experimental PL spectra (solid line) at T ¼ 296 K with the function (circle) given by Eq. (2): (a) ZnSe:Cl; (b) Zn0:971Be0:029Se:Cl. 2.6 2.7 2.8 2.9 3.0 Norm.Intensity(arb.units) Photon energy (eV) T=297K Slope=63.8eV -1 1/kT=64.5eV -1 T=250K Slope=38.4eV -1 1/kT=39.1eV -1 T=200K Slope=47.3eV -1 1/kT=46.4eV -1 T=180K Slope=63.4eV -1 1/kT=58.0eV -1 Fig. 5. PL of one typical sample (circles) at various tempera- tures with solid line representing the corresponding 1=kT values (shown in the figure). The intensity in the figure is plotted in natural log scale. Y. Gu et al. / Journal of Luminescence 104 (2003) 77–83 81
  • 6. the complexities of the fitting procedure and is not expected to change the impurity ionization en- ergies, which are important for our further analysis. For a FB transition, it then remains to be established whether it is FD or FA. In a prior observation of this transition, in ZnSe, it was suggested that it was FD, with holes recombining with Cl donors located in the tail of a presumed impurity band [25]. However, this explanation seems unlikely for a number of reasons. First, we also observed such PL in our undoped samples (with much lower intensity) and samples with low Cl concentration ðB1016 cmÀ3 Þ; where no such impurity band is expected. Secondly, we note that the impurity activation energy obtained from our fitting for ZnSe:Cl (see Table 1), is 48 meV; appreciably higher than the Cl activation energy in ZnSe (B27 meV [11]). Moreover, one would expect the actual Cl donor activation energy at RT to be even lower than 27 meV due to the screening (for effects of screening on impurity ionization energies, see e.g. Refs. [26,27] and references therein); indeed, formal application of screening theory to Cl gives zero activation energy for our samples with free electron concentrations B5 Â 1017 cmÀ3 ;3 where this type of PL is still observed, which clearly excludes Cl as the parti- cipating donor for this PL. We further note that the fit shown in Fig. 6 was obtained with g values of about 0.1–0.2. Since such values are appropriate for acceptors ðmc=mvB0:19 for ZnSe assuming that mc ¼ 0:15m0 and mv ¼ 0:78m0 [29]), and since we observed that the fit was very sensitive to the g value, we attribute this transition to a free electron to acceptor recombination. This then leaves the puzzle that the activation energy (48 meV for ZnSe:Cl) is lower than that ð 100 meVÞ of ‘‘standard’’ acceptors in ZnSe ðLi; Na; NÞ; how- ever, lower-than-standard values have already been previously reported (e.g. 56 meV for an unknown acceptor in undoped ZnSe [30], and 85 meV for P acceptors in p-type ZnSe [31]). We note again that the acceptor activation energy obtained by ascribing the 2:742 eV ZnSe:Cl peak to a DAP peak (at 10 K) is 6375 meV; which is relatively close to the 48 meV obtained at RT from the FB fitting. The difference between these two energies ðB15 meVÞ can be accounted for by screening.4 Additionally, for ZnBeSe:Cl this en- ergy difference is also in the range of 15B17 meV; if one uses band gap values consistently. There- fore, we believe that the FA transition is the most likely mechanism for this PL. The observation of the same PL in undoped samples but with much lower intensities (more than two orders of magnitude) can be explained as follows: first, the free electron concentration in the Cl-doped (n- type) sample is much higher than that in the undoped sample, and as a result, the recombina- tion involving free electrons and acceptor-type centers would be much more significant. Secondly, the concentration of this acceptor-type species might increase as Cl is introduced into Zn(Be)Se, which can also contribute to higher PL intensity in Cl-doped samples. The origin of this acceptor-type species still remains unclear at this point. However, since the PL is also present in undoped samples, it may well be a native- type defect, although the possibility of a pervasive cantaminant cannot be excluded at this time. By fitting the FA spectra, we also obtained the acceptor activation energy as a function of Be concentration (see Table 1); the trend is that the activation energy generally increases with Be composition. This can be qualitatively explained as follows. It is well known that the dielectric constant decreases with increasing band gap (see e.g. Ref. [33] for a good qualitative discussion as well as a simple theoretical approach). Further- more, according to the standard effective-mass theory (see e.g. Ref. [15]), the effective mass generally increases as the band gap increases. Therefore, for an effective-mass-type impurity, its activation energy would increase with the band gap (i.e. with increasing Be), both because of a decrease in the dielectric constant and an increase in effective mass. 3 We calculated the Cl activation energy to approach zero for samples with ½nŠB5 Â 1017 cmÀ3 ; using the theory developed by J.B. Krieger [28] and G.F. Neumark [26]. 4 It has been observed by Bowers et al. [32] that in p-type ZnSe:N the donor activation energy also decreased; the change is as high as 22% (from 31 to 24 meV) when T increases from 77 K to RT. Y. Gu et al. / Journal of Luminescence 104 (2003) 77–8382
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