2. Appl. Phys. Lett., Vol. 79, No. 6, 6 August 2001 O. Maksimov and M. C. Tamargo 783
FIG. 3. Direct band gap at 298 K from reflectivity data ͑open circles͒ and
PL energy at 6 K ͑crosses͒ as a function of BeTe content ͑x͒ in Bex Zn1Ϫx Te.
The direct and indirect band gaps for BeTe are taken from Ref. 7. The
indirect band gap of ZnTe is taken from Ref. 9. The dashed line is a fit for
the ⌫→X transition and the solid line is a fit for the ⌫→⌫ transition of
FIG. 1. RT reflectivity spectra for several Bex Zn1Ϫx Te alloys of different
Bex Zn1Ϫx Te alloys as a function of composition.
compositions are shown.
a value of xу0.28. It should be noted that the intensity of the
dicate that the band gap continuously shifts to a higher en-
PL decreased sharply as the BeTe content became larger than
ergy as the Be concentration increases. The band gap energy
that value, and continued to decrease as the Be content in-
increases linearly with BeTe content at a rate of 18 meV for
creased.
a change of 1% in BeTe content.
Based on their optical properties, the samples can be
Figure 2 shows normalized PL spectra measured at 6 K
divided into two different groups. For Bex Zn1Ϫx Te with x
for the same group of samples. The PL spectra are dominated
Ͻ0.28, the PL emission energy increases with Be content. In
by narrow emission lines. In several spectra a second, usu-
this group of samples, the PL emission energy, which is mea-
ally weak peak is present at lower energy, about 50 meV
sured at 6 K, is about 90 meV above the RT band gap value
below the high-energy peak. It can be seen from the data in
obtained from the reflectivity measurements, consistent with
Fig. 2 that the energy of the dominant PL peak initially in-
the expected variation of the band gap with temperature.
creases with Be content and then becomes nearly constant at
Thus, the PL emission in this group of samples is assigned to
the ⌫→⌫ near bandedge emission. For the Bex Zn1Ϫx Te with
xу0.28, the PL emission energy is nearly constant while the
direct band gap value continues to increase linearly with
composition. Therefore, our results suggest that the
Bex Zn1Ϫx Te layers with xу0.28 are indirect band gap mate-
rials. This conclusion is also supported by the reduced PL
intensity observed for these samples.
In Fig. 3, we have plotted the direct band gaps obtained
from reflectivity measurements ͑open circles͒ and the PL
emission energies ͑crosses͒ as a function of Be content for a
larger set of samples that includes the six shown in Figs. 1
and 2. Using the RT band gap measured for ZnTe ͑2.263 eV͒
and the reported value for the direct band gap of BeTe ͑4.1
eV͒,7 the reflectivity data can be well fitted to the linear
equation:
E ⌫ g ͑ x ͒ ϭ2.263* ͑ 1Ϫx ͒ ϩ4.1* x for 0рxр1, ͑1͒
which describes the RT direct band gap dependence on com-
position for this alloy. The same equation corrected for the
temperature difference describes the behavior of 6 K PL data
for samples with xϽ0.28.
To analyze the PL data for xу0.28, we must consider
FIG. 2. Low-temperature ͑6 K͒ PL spectra for several Bex Zn1Ϫx Te alloys of the ⌫→X band gap energy for the binary end points. The
different compositions are shown. value for BeTe is well known to be at 2.8 eV.7 However, the
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3. 784 Appl. Phys. Lett., Vol. 79, No. 6, 6 August 2001 O. Maksimov and M. C. Tamargo
⌫→X transition energy for ZnTe is not known precisely. BeTe content at a rate of 18 meV for a change of 1% in BeTe
Recently, a value of 3.05 eV was reported,9 while a value of content for the entire compositional range. The dependence
3.45 eV was obtained using ab initio calculations.10 The val- of the indirect band gap on composition was also established
ues the same authors report for the X→X transition ͓5.45 eV and a good fit was obtained when a value of 3.05 eV was
͑Ref. 9͒ and 5.63 eV ͑Ref. 10͔͒ are comparable to the values used for the ZnTe ⌫→X transition. Our results indicate that
measured by other group ͓5.23 eV ͑Ref. 11͒ and 5.30 eV Be0.48Zn0.52Te, which is the composition that is lattice
͑Ref. 12͔͒. Assuming that the PL emission energies for the matched to InP, is an indirect semiconductor with a ⌫→X
samples with x above 0.28 correspond to the ⌫→X indirect indirect band gap of 2.77 eV, and a ⌫→⌫ direct band gap of
band gap transition, we have fitted the variation of the 3.14 eV. Therefore, it is well suited for use as a p-type con-
⌫→X indirect band gap with composition ͑x͒ to the equa- tact layer in LED structures emitting throughout the visible
tion: range.
E X g ͑ x ͒ ϭ3.05* ͑ 1Ϫx ͒ ϩ2.8* xϪ0.5* x * ͑ 1Ϫx ͒ The authors would like to acknowledge support from the
for 0рxр1, ͑2͒ National Science Foundation through Grant Nos. DMR-
9805760 and DGE-9972892. The work was performed under
where 0.5 eV is a bowing parameter. A good correlation of the auspices of the New York State Center for Advanced
Eq. ͑2͒, with our data was obtained, while attempts to fit to Technology on Ultrafast Photonics and the Center for Analy-
an equation that uses 3.45 eV as the ZnTe ⌫→X indirect sis of Structures and Interfaces.
band gap was not successful. This supports our interpretation
of the data and indicates that the ⌫→X band gap transition
for ZnTe is about 3.05 eV. 1
M. C. Tamargo, W. Lin, S. P. Guo, Y. Guo, Y. Luo, and Y. C. Chen, J.
Comparison of the reflectivity and PL data shows that Cryst. Growth 214, 1058 ͑2000͒.
the direct-to-indirect crossover occurs at xϷ0.28. This result 2
W. Faschinger and J. Nurnberger, Appl. Phys. Lett. 77, 187 ͑2000͒.
¨
3
implies that Be0.48Zn0.52Te, which is the alloy composition W. Shinozaki, I. Nomura, H. Shimbo, H. Hattori, T. Sano, S. B. Che, A.
that is lattice matched to InP, is an indirect semiconductor Kikuchi, K. Shimomura, and K. Kishino, Jpn. J. Appl. Phys., Part 1 38,
2598 ͑1999͒.
with a ⌫→X indirect band gap of 2.77 eV and a ⌫→⌫ direct 4
W. Lin, B. X. Yang, S. P. Guo, A. Elmoumni, F. Fernandez, and M. C.
band gap of 3.14 eV. A previous report5 predicted that the Tamargo, Appl. Phys. Lett. 75, 2608 ͑1999͒.
5
direct-to-indirect crossover for Bex Zn1Ϫx Te alloy would oc- S. B. Che, I. Nomura, W. Shinozaki, A. Kikuchi, K. Shimomura, and K.
cur at a much higher Be content (xϾ0.7). This prediction Kishino, J. Cryst. Growth 214, 321 ͑2000͒.
6
M. W. Cho, S. K. Hong, J. H. Chang, S. Saeki, M. Nakajima, and T. Yao,
was based on the assumption that the ⌫→X ZnTe band gap J. Cryst. Growth 214Õ215, 487 ͑2000͒.
is at 5.97 eV. Our data gives a clear evidence of the position 7
A. Waag, F. Fischer, H. J. Lugauer, Th. Litz, J. Laubender, U. Lunz, U.
of the direct-to-indirect crossover and indicates that 5.97 eV Zehnder, W. Ossau, T. Gerhardt, M. Moller, and G. Landwehr, J. Appl.
Phys. 80, 792 ͑1996͒.
is not the correct value for the ⌫→X transition for ZnTe. 8
M. W. Cho, J. H. Chang, S. Saeki, and S. Q. Wang, and T. Yao, J. Vac. Sci.
In summary, epitaxial layers of Bex Zn1Ϫx Te were grown Technol. B 18, 457 ͑2000͒.
by MBE on InP substrates and their band structure and opti- 9
G. D. Lee, M. H. Lee, and J. Ihm, Phys. Rev. B 52, 1459 ͑1995͒; and
cal properties were investigated. It was shown that references therein.
10
O. Zakharov, A. Rubio, X. Blase, M. L. Cohen, and S. G. Louie, Phys.
Bex Zn1Ϫx Te has a direct band gap for low BeTe concentra- Rev. B 50, 10780 ͑1994͒.
tions and becomes indirect, exhibiting a ⌫→X character, for 11
K. Sato and S. Adachi, J. Appl. Phys. 73, 926 ͑1993͒.
xу0.28. The ⌫→⌫ direct band gap increases linearly with 12
K. Suzuki and S. Adachi, J. Appl. Phys. 82, 1320 ͑1997͒.
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