Next: 3.3.2 Bandgap Offsets
Up: 3.3 Band-Structure
Previous: 3.3 Band-Structure
Subsections
3.3.1 Bandgap Energy
The bandgap (or forbidden energy zone) is one of the most important
semiconductor parameters. Various models define the temperature dependence of
the bandgap energy in semiconductors (e.g. [112]). For an alloy
, the temperature-dependent bandgaps of the constituents
(A and B) are calculated first. The bandgap and the energy offset are then
calculated depending on the material composition. This is important to assure
consistency between the values for alloy materials at and and the values
for the respective basic materials. For materials where the bandgap changes between
direct and indirect the multiple valley conduction bands are considered.
In MINIMOS-NT the model of Varshni [112] is used for basic materials. The
temperature dependence is calculated by (3.60), where
is the bandgap at 0 K.
|
|
|
(3.60) |
The parameter values are summarized in Table 3.8. Note, for these
materials always the lowest conduction band valley minimum is taken into
account. In addition, the resulting bandgaps at 300 K,
, are
included in Table 3.9.
Table 3.8:
Parameter values for modeling the bandgap energies
Material |
Minimum |
[eV] |
[eV/K] |
[K] |
Reported
[eV] |
References |
Si |
X |
1.1695 |
4.73
|
636 |
1.17 |
[90,86] |
Ge |
L |
0.7437 |
4.774
|
235 |
0.74 |
[86] |
GaAs |
G |
1.521 |
5.58
|
220 |
1.51-1.55 |
[113,114,115] |
AlAs |
X |
2.239 |
6.0
|
408 |
2.22-2.239 |
[94,90,108] |
InAs |
G |
0.420 |
2.5
|
75 |
0.414-0.43 |
[92,113] |
InP |
G |
1.421 |
3.63
|
162 |
1.42-1.432 |
[108,86,114] |
GaP |
X |
2.338 |
5.771
|
372 |
2.338-2.346 |
[108,86,90] |
|
Table 3.9:
Bandgap energies at room temperature compared to reported data
Material |
Minimum |
[eV] |
Reported
[eV] |
References |
Si |
X |
1.124 |
1.12-1.1242 |
[85,86,90] |
Ge |
L |
0.663 |
0.66-0.67 |
[90,85,86] |
GaAs |
G |
1.424 |
1.42-1.43 |
[116,95,104,85] |
AlAs |
X |
2.163 |
2.14-2.168 |
[94,116,104,90] |
InAs |
G |
0.360 |
0.354-0.37 |
[93,92,115,117] |
InP |
G |
1.350 |
1.34-1.351 |
[90,115,92] |
GaP |
X |
2.261 |
2.26-2.272 |
[85,92,90] |
|
For two additional models can be chosen which are based on
polynomial fits of second and third order. The first one after
Gaensslen [118,119]
was also used in MINIMOS 6. The second model is based on data from
Green [120].
|
|
|
(3.61) |
The parameter values for these models are summarized in Table 3.10.
Table 3.10:
Parameter values for modeling the bandgap energies
Model |
[eV] |
[eV] |
[eV] |
[eV] |
[eV] |
Gaensslen |
1.1785 |
-0.02708 |
-0.02745 |
0.0 |
1.124 |
Green |
1.17 |
0.00572 |
-0.06948 |
0.018 |
1.124 |
|
In Fig. 3.8 the results obtained with the three different models
for Si are compared to data from [120]. In Fig. 3.9 and Fig. 3.10 the
temperature dependence of the direct gap in GaAs and InP, respectively, are
compared to other models.
In the case of alloy materials the temperature-dependent bandgaps of the constituents,
and
, are calculated by (3.60).
However, for materials where the bandgap changes between direct and indirect
the multiple valley conduction bands are considered. For that purpose,
additional model parameters are needed for the higher energy valleys in the
respective III-V binary materials (Table 3.11). In addition, the
resulting bandgaps at 300 K,
, are included in Table 3.12.
Table 3.11:
Parameter values for modeling the bandgap energies
Material |
Minimum |
[eV] |
[eV/K] |
[K] |
Reported
[eV] |
References |
GaAs |
X |
1.981 |
4.6
|
204 |
1.9-1.91 |
[116,104] |
AlAs |
G |
2.891 |
8.78
|
332 |
2.907-3.02 |
[59,95,94,104] |
InAs |
X |
2.278 |
5.78
|
83 |
|
|
InP |
X |
2.32 |
7.66
|
327 |
2.32-2.38 |
[109,84,121] |
GaP |
G |
2.88 |
8.0
|
300 |
2.869-2.895 |
[91,84,122] |
|
Table 3.12:
Bandgap energies at room temperature compared to reported data
Material |
Minimum |
[eV] |
Reported
[eV] |
References |
GaAs |
X |
1.899 |
1.9-1.91 |
[116,104] |
AlAs |
G |
2.766 |
2.671-2.766 |
[93,59] |
InAs |
X |
2.142 |
1.37-2.14 |
[116,108,123] |
InP |
X |
2.21 |
2.21-2.30 |
[116,123,121] |
GaP |
G |
2.76 |
2.73-2.85 |
[84] |
|
The bandgap and the energy offset of an alloy
are calculated by
The bowing parameters
and
are summarized in
Table 3.13. Additional bowing parameters are given as a reference
for the case when a one-valley bandgap fit is used.
Table 3.13:
Parameter values for the bandgap of alloy materials
Material |
[eV] |
[eV] |
[eV] |
Reported |
References |
SiGe |
|
|
-0.4 |
-0.4 |
[124] |
AlGaAs |
0.0 |
-0.143 |
0.7 |
0, -0.143 |
[93,125] |
InGaAs |
|
|
-0.475 |
-0.4, -0.475, -0.555 |
[108,90,71] |
InAlAs |
-0.3 |
-0.713 |
1.2 |
-0.689,-0.24 |
[108,90] |
InAsP |
|
|
-0.32 |
-0.101, -0.32 |
[108,90] |
GaAsP |
-0.21 |
-0.21 |
0.5 |
-0.176,-0.23 |
[108,126] |
InGaP |
-0.67 |
-0.17 |
0.6 |
-0.786,-0.6,-0.18 |
[108,90,109] |
|
For example, such a one-valley bandgap fit is used in the case of the
technologically important strained SiGe grown on Si (see
Fig. 3.11). In certain cases for the bandgap can become smaller than the
one of pure Ge [127] depending on the strain. In the unstrained case,
however, an -to- gap transition is observed at about .
The material composition dependence of the , , and -band
gaps in AlGaAs at 300 K is shown in Fig. 3.12. A
direct-to-indirect gap transition is observed at about . The one-valley
bandgap fit which is included for comparison gives a good agreement only for
. In Fig. 3.13 the temperature dependence of the bandgap in
AlGaAs with Al content as a parameter is shown. In Fig. 3.14
the material composition dependence of the , , and -band
gaps in InGaAs at 300 K is shown. As can be seen this material has
a direct bandgap for the entire composition range. Therefore, only the energy
of the valley is taken into account. However, in the case of strain
the bandgap can significantly differ [128]. For example, a good fit to
the strained bandgap values of InGaAs grown on GaAs can be achieved
by changing the
of InAs from 0.42 eV to 0.58 eV. In Fig. 3.15 the
temperature dependence of the bandgap in InGaAs with In content as
a parameter is shown. In the case of InAlAs there is
direct-to-indirect gap transition at about and the use of one valley
fit is nearly impossible. It gives comparatively accurate values for the
lattice matched case of and above (see Fig. 3.16).
InAsP has a direct gap for the complete material composition range
so only the valley energy is calculated. The bowing parameter value
suggested in [108] is used. GaAsP has a direct-to-indirect
gap transition at about . As can be seen in Fig. 3.17 a one valley
model can be successfully used for this material. In Fig. 3.18 the
material composition dependence of the , , and -bandgaps
in GaInP at 300 K is shown. The direct-to-indirect gap transition
is at about . Only at the technologically important value of ,
when GaInP lattice matches the one of GaAs the one-valley model
gives a good fit for the bandgap. The temperature dependence of the bandgap in
GaInP with Ga content as a parameter is shown in Fig. 3.19.
Figure 3.8:
Comparison of different models for the
temperature dependence of the bandgap in Si
|
Figure 3.9:
Comparison of different models for the
temperature dependence of the bandgap in GaAs
|
Figure 3.10:
Comparison of different models for the
temperature dependence of the bandgap in InP
|
Figure 3.11:
Material composition dependence of the
, , and -bandgaps in SiGe at 300 K
|
Figure 3.12:
Material composition dependence of the
, , and -bandgaps in AlGaAs at 300 K
|
Figure 3.13:
Temperature dependence of the bandgap
in AlGaAs with Al content as a parameter
|
Figure 3.14:
Material composition dependence of the
, , and -bandgaps in InGaAs at 300 K
|
Figure 3.15:
Temperature dependence of the bandgap
in InGaAs with In content as a parameter
|
Figure 3.16:
Material composition dependence of the
, , and -bandgaps in InAlAs at 300 K
|
Figure 3.17:
Material composition dependence of the
, , and -bandgaps in GaAsP at 300 K
|
Figure 3.18:
Material composition dependence of the
, , and -bandgaps in GaInP at 300 K
|
Figure 3.19:
Temperature dependence of the bandgap
in GaInP with Ga content as a parameter
|
Next: 3.3.2 Bandgap Offsets
Up: 3.3 Band-Structure
Previous: 3.3 Band-Structure
Vassil Palankovski
2001-02-28