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Dressel.Gruner.Electrodynamics of Solids.2003

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348

40

2

30

ε

constant

 

Dielectric

20

 

10

0

 

 

 

 

 

 

 

 

13 Semiconductors

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Energy

hω (eV)

 

 

 

 

 

 

 

 

1

2

3

 

 

4

 

 

5

6

Ge

 

 

 

 

 

 

 

 

 

 

 

 

 

Σ 4

 

 

 

Σ1

 

 

 

Experiment

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Χ 4

 

 

 

Χ1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Theory

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Λ3

 

 

Λ1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

L3' L3

Γ25' Γ15'

Γ25' Γ2'

L3' L1

1

2

3

4

5

Frequency ν (104 cm1)

Fig. 13.6. Calculated spectral structure of 2(ω) of germanium compared with experimental results obtained from transmission and reflection measurements (after [Phi63]). The peaks and shoulders identify the van Hove singularities; the transitions which are involved in the particular joint density of states Dcv(E) are also indicated. Important critical points in the band structure are marked according to Fig. 13.4.

1(ω) shows a zero-crossing at

ωp+ =

4π ne2

 

1/2

,

mb

the same expression which applies for metals (Eq. (12.1.8)), where interband transitions are accounted for by a high frequency dielectric constant . Just as for metals, plasma oscillations can also be examined by electron energy loss spectroscopy; both methods can be used to evaluate the loss function Im{−1/ ˆ(ω)}. This has been done for various semiconductors, and results are displayed in Fig. 13.7 for our example of germanium. The peak identifies the plasma frequency, and we observe an underdamped plasmon at energy of approximately 16 eV. The fundamental optical parameters of some semiconductors are collated in Table 13.1. For most band semiconductors, the bandgap is significantly smaller than the plasma frequency, leading also to a relatively large dielectric constant, which broadly

Loss function Im 1 / ε

 

 

 

 

 

 

13.1 Band semiconductors

 

 

 

349

 

 

 

 

 

 

 

 

 

 

Energy

hω (eV)

 

 

 

 

 

 

 

 

 

 

1.20

5

10

 

15

 

 

20

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

1.0

 

 

 

Ge

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

0.8

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

0.6

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

0.4

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

0.2

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Optical data

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Electron energy loss

 

 

0.00

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

5

10

 

15

 

 

20

25

Frequency ν (104 cm1)

Fig. 13.7. Electron energy loss spectra Im{1/ ˆ(ω)} of germanium as obtained from the optical data shown in Fig. 13.1 and from electron energy loss spectroscopy (after [Phi63, Pow60]). The data are normalized to the maximum of the measured loss.

Table 13.1. Optical gaps Eg = h¯ ωg, plasma frequencies ωp, and static dielectric constant 1= 0) of various semiconductors as obtained at low temperatures.

‘i’ indicates an indirect gap, ‘d’ a direct gap. After [Kit96, Mad96, Wea90].

Material

Gap

ωg/2π c

Eg

ωp/2π c

hωp

1= 0)

 

 

(cm

1

)

(eV)

(cm

1

)

¯

 

 

 

 

 

(eV)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Ge

i

5950

 

0.74

13.4

×

 

4

16.6

15.8

 

104

Si

i

9450

 

1.17

13.0

×

104

16.2

11.7

InSb

d

1850

4

0.24

9.7

×

104

12

17.9

GaAs

d

1.2

× 104

1.52

12.5

×

10

15.5

13.1

diamond

i

4.4

× 10

5.4

 

 

 

 

 

5.5

 

 

 

 

 

 

 

 

 

 

 

 

 

350

 

 

13 Semiconductors

correlates with the ratio

 

hωp/Eg

2 as derived in Eq. (6.3.5). The above equations

 

 

 

¯

 

apply at zero

temperature; at finite temperatures contributions to the optical prop-

 

 

 

 

erties coming from thermally excited electrons and holes have to be included. The number of these excitations increases exponentially with increasing temperature, and is small even at room temperature in most typical (undoped) semiconductors. If the relaxation time associated with these excitations is long, absorption due to these excitations – often called the free-electron absorption – occurs well below the gap frequency, and, as a rule, a simple Drude model accounts for the optical properties [Ext90]. In Fig. 13.8 the optical conductivity σ1(ω) and σ2(ω) of silicon is displayed for two different doping levels: for an acceptor concentration of 1.1 × 1015 cm3 leading to a resistivity of 9.0 cm, and a donor concentration of 4.2 × 1014 cm3 which gives ρdc = 8.1 cm. The frequency dependence measured by time domain spectroscopy at room temperature can be well described for both cases by a simple Drude model with somewhat different scattering rates: 1/(2π τ c) = 40 cm1 and 20 cm1, respectively.

The onset of the absorption is different for a highly anisotropic band structure. Of course, strictly one-dimensional materials are difficult to make, but in several so-called linear chain compounds (the name indicates the atomic or molecular arrangements in the crystal) the band structure is anisotropic enough such that it can be regarded as nearly or quasi-one-dimensional. Near to the gap, the optical conductivity of such materials can be described by the one-dimensional form of semiconductors we have discussed in Chapter 6. Expression (6.3.16) assumes that the transition matrix element between the valence and conduction states is independent of frequency; thus the functional dependence of σ1 on ω is determined solely by the joint density of states. In general this is not the case, as can be seen from the following simple arguments. The periodic potential leads to a strong modification of the electronic wavefunctions only for states close to the gap; for wavevectors away from the gap (and therefore for transition energies significantly different from the gap energy Eg) such perturbation is less significant, and the electron states are close to the original states which correspond to a single band. As transitions between states labeled by different k values in a single band are not possible (note that optical transitions correspond to q = 0), the transition probability is presumed to be strongly reduced as the energy of such transitions is increased from the gap energy Eg. Thus the conductivity is expected to display a stronger frequency dependence than that given by Eq. (6.3.16). All this can be made quantitative by considering the transitions in one dimension [Lee74]. One finds that

σ1(ω) =

π N e2Eg2

1

,

(13.1.9)

2h¯ 2m

 

ω3 1 (Eg/h¯ ω)2 1/2

σ1 (1 cm1)

σ 2 (1 cm1)

 

13.1 Band semiconductors

 

351

 

Frequency f (THz)

 

0

0.5

1.0

1.5

2.0

0.12

 

 

 

Si

 

 

 

 

0.08

0.04

(a)

0.0

(b)

0.06

0.04

0.02

0.00

20

40

60

 

Frequency ν (cm1)

 

Fig. 13.8. Frequency dependence of the (a) real and (b) imaginary parts of the optical conductivity of silicon weakly doped by holes (1.1 × 1015 cm3, open circles) or electrons (4.2 × 1014 cm3, solid circles). The experiments were performed at T = 300 K in the time domain; the full lines correspond to σ1(ω) and σ2(ω) as obtained by the Drude model with the parameters given in the text (after [Ext90]).

an expression which has a leading ω3 frequency dependence for frequencies well exceeding Eg/h¯ ; near to the gap the familiar square root frequency dependence is recovered. There is no effective mass µ here, as in the perturbation treatment of

352

13 Semiconductors

 

 

 

 

 

Energy hω (eV)

 

104

 

 

 

 

1

 

(a)

 

 

 

 

 

 

 

 

 

)

 

 

 

 

 

 

 

1

 

 

(NbSe4)3I

 

 

cm

 

 

 

 

103

 

 

 

 

 

1

 

 

 

 

 

(

 

 

 

3

 

 

 

1

 

 

)

 

 

 

σ

 

 

 

 

 

 

 

 

1

 

 

 

 

Conductivity

 

 

cm

2

 

 

 

 

 

1

 

 

 

10

2

 

 

 

 

 

 

 

 

 

 

 

 

 

 

3

1

 

 

 

 

 

 

 

 

 

 

(10

 

 

 

 

 

 

 

 

 

 

 

1

 

 

 

~ω4.25

 

 

σ

0

5

10

 

 

 

 

0

15

 

101

 

 

ν (10

3 cm1)

 

 

 

 

 

 

104

 

 

103

 

 

 

 

 

 

 

 

Frequency ν (cm1)

Energy hω (eV)

 

 

 

 

100

 

 

 

 

101

 

10

4

 

)

1.5

 

 

 

 

 

 

 

 

1

 

 

 

 

 

 

)

 

 

 

 

 

 

 

 

 

1

 

 

 

cm

1.0

 

 

 

 

 

cm

 

 

 

1

 

 

 

 

 

 

1

 

 

 

4

0.5

 

 

 

 

 

103

KCP

(10

 

 

 

 

 

 

 

 

 

 

 

1

 

 

 

 

 

 

(

 

 

 

σ

 

 

 

 

 

 

1

 

 

 

 

0.0

 

 

 

 

 

σ

 

 

 

 

 

 

 

 

 

 

 

 

 

0

1

2

3

4

5

Conductivity

 

 

 

 

 

ν (103 cm1)

 

102

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

101

(b)

 

 

 

~ω3

 

 

 

 

 

 

 

 

 

 

 

 

104

 

 

 

 

105

 

 

103

 

 

 

 

 

 

 

 

 

 

Frequency ν (cm1)

 

 

 

Fig. 13.9. Frequency dependence of the conductivity in highly anisotropic semiconductors K2[Pt(CN)4]Br0.3·3H2O (KCP) at 40 K and (NbSe4)3I at room temperature (data taken from [Bru75, Ves00]). The lines correspond to a power law behavior with exponents as indicated. The insets show the same data on linear scales.

13.1 Band semiconductors

353

the periodic potential the valence and conduction bands have the same curvature and the same mass. Both can be expressed in terms of the gap energy Eg.

A strongly frequency dependent optical conductivity has indeed been found in several one-dimensional or nearly one-dimensional semiconductors, such as K2[Pt(CN)4]Br0.3·3H2O (better known by the abbreviation KCP) [Bru75] and (NbSe4)3I [Ves00]. The conductivity of these much studied compounds is displayed in Fig. 13.9. The full line plotted in Fig. 13.9a is the expected ω3 frequency dependence; for (NbSe4)3I, however, we find a stronger dependence, presumably due to the narrow band, with the bandwidth comparable to the optical frequencies where the measurements were made.

Electron–electron interactions may modify this picture. Such interactions lead, in strictly one dimension, to an electron gas which is distinctively different from a Fermi liquid. In not strictly but only nearly one dimension such interactions lead to a gap, and the features predicted by theory [Gia97] are expected to be observed only at high energies. These features include a power law dependence of the conductivity, with the exponents on ω different from 3 (see above). Experiments on highly anisotropic materials, such as (TMTSF)2PF6 [Sch98], have been interpreted as evidence for such novel, so-called Luttinger liquids.

A strict singularity at the single-particle gap, of course, cannot be expected for real materials; deviations from one dimensionality, impurities, and the frequency dependence of the transition matrix element involved, all tend to broaden the optical transition. In materials where the band structure is strongly anisotropic, another effect is also of importance. For a highly anisotropic system where the bands do not depend on the wavevector k, but with decreasing anisotropy, the parallel sheets of the band edges become warped, and the gap assumes a momentum dependence. Consequently the gap – defined as the minimum energy separation between both bands – becomes indirect. This can be seen most clearly by contrasting the thermal and optical gaps in materials of varying degrees of band anisotropy with the thermal measurements (i.e. dc resistivity) resulting in smaller gaps as expected and the difference increasing with decreasing anisotropy [Mih97].

13.1.2 Forbidden and indirect transitions

Forbidden transitions, as a rule, have low transition probabilities and therefore are difficult to observe experimentally. A possible example is presented in Fig. 13.2 for PbS, where the characteristic ωg)3/2 dependence of the absorption is seen, together with the ωg)1/2 dependence close to the bandgap; this latter gives evidence for direct allowed interband transitions as discussed above.

Less controversial is the observation of indirect transitions; the reason for this is that – in addition to the different frequency dependence – these transitions are

354

13 Semiconductors

α1/2 (cm1/2)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Energy

hω (eV)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

100.60

 

 

 

 

0.65

 

 

 

0.70

 

 

 

0.75

 

 

 

0.80

 

 

 

0.85

Ge

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

8

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

K

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

6

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

291

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

249

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

195

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

4

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

90

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

2

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

.

 

 

 

 

 

 

 

 

 

 

 

 

 

2

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

4

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

0

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

5.0

 

 

5.2

 

 

5.4

5.6

5.8

6.0

 

 

6.2

6.4

 

 

6.6

6.8

 

 

 

 

 

 

 

 

 

Frequency ν (103 cm1)

Fig. 13.10. Absorption spectra of germanium in the vicinity of the indirect bandgap at various temperatures as indicated (after [Mac55, Yu96]). The two onsets of absorption identify the two indirect processes; for both the absorption coefficient α(ω) is proportional to the square of the frequency. The temperature dependence – analyzed in terms of the one-phonon model – provides evidence for the indirect transition.

also strongly temperature dependent. Since the two possible processes discussed in Section 6.4.1 involve different phonon states, two different frequencies where the onset of the absorption occurs are expected. This is nicely demonstrated in Fig. 13.10, in which the data on germanium are taken at different temperatures. The functional dependence of the absorption (h¯ ω Eg)2 is also in accordance with that calculated for indirect transitions in Eq. (6.4.4). In addition to the two absorption processes we have discussed earlier, the low temperature gap, determined by the onset of absorption at 20 K, can be estimated to approximately 0.74 eV.

13.1.3 Excitons

In addition to the transitions involving single-particle states, optical absorption associated with the creation of excitons is observed in various semiconductors. Let us first estimate the energies and spatial extension of excitons, following our discussion in Section 6.5. For a typical semiconductor the static dielectric constant

13.1 Band semiconductors

355

Transmission

 

 

 

 

 

 

Energy

hω (eV)

 

 

 

2.12

2.13

2.14

2.15

2.16

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

CuO

 

 

 

 

 

j=3 j=4 j=5

 

 

 

 

 

 

 

 

101

 

 

 

 

 

j=2

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

10

0

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

1.72

1.73

1.74

1.71

Frequency ν (104 cm1)

Fig. 13.11. Optical transmission through a 0.1 mm slab of cuprous oxide (CuO) in the frequency region below the single-particle gap measured at T = 77 K (after [Bau61]). Note the inverted transmission scale; the peaks correspond to absorption of electrodynamic radiation by the transitions to the various excitation states j.

10) 10. If we assume that both mc and mv are 1/3 of the free-electron mass, µ1 = mv 1 + mc 1 is approximately 6/m, and we arrive at a binding energy

– the energy required to break up the exciton – of approximately

E1exc = Eg

e4µ

 

15 meV ;

2h2

 

2

 

¯

1

 

while the spatial extension rexc corresponding to the j = 1 state is about 20 A,˚ significantly larger than the typical lattice constant. The binding energy Eexcj decreases

significantly for semiconductors with smaller gaps. As 1 1 + h¯ ωp/Eg 2, it follows from Eq. (6.3.6) that the exciton energy Eexcj depends on the fourth power of the single-particle gap Eg. Well defined and unambiguously resolved exciton lines can hence be observed only in wide bandgap semiconductors, and in Fig. 13.11 the absorption spectrum of CuO is displayed as an example. The quantum numbers j = 2, 3, . . . are arrived at on fitting the observed energies to the Rydberg series, Eq. (6.5.1).

356

13 Semiconductors

α (104 cm1)

 

 

 

Energy hω (eV)

 

 

 

1.2 1.42

1.44

1.46

1.48

1.50

1.52

1.54

1.56

GaAs

 

 

 

 

 

 

1.1

 

 

 

 

 

 

 

1.0

0.9

0.8

 

 

 

 

 

 

 

 

186 K

21 K

 

0.7

294 K

 

 

 

 

90 K

 

 

 

 

 

 

 

0.6

 

 

 

 

 

0.5

 

 

 

 

 

1.14

1.16

1.18

1.20

1.22

1.24

Frequency ν (104 cm1)

Fig. 13.12. Exciton absorption in gallium arsenide (GaAs) at different temperatures. The full line is a fit to theory [Ell57] (after [Stu62]).

For small semiconductor gaps, the binding energies are also small, and individual transitions from the top of the valence band to the various exciton energy levels (corresponding to different j values) cannot be resolved. The levels, by definition, form a continuum near to the single-particle gap as j → ∞; this continuum then leads to a broad absorption and thus modifies the characteristic onset near Eg. The intensity of this absorption is straightforward to estimate, using results available for the hydrogen atom. Combining the expressions available for the absorption associated with the various Rydberg states with the density of states as j → ∞, we obtain [Yu96]

 

(ω)

32π 2e2|pcv|2µ2

,

(13.1.10)

3m3Eg2

2

 

 

 

where |pcv| is the transition matrix element of exciting one state for j → ∞. The above expression – valid at the band edge – corresponds to a frequency

13.2 Effects of interactions and disorder

357

independent absorption at Eg, in contrast to the absorption process which goes to zero for singe-particle transitions as the bandgap is approached from above. Calculations can be performed for transitions with energies near to the gap, and in general one finds a broad peak at Eg due to excitonic absorption which merges with the single-particle absorption as the energy increases [Ell57]. This has been seen in a number of small bandgap semiconductors, and the frequency dependence of the absorption coefficient of GaAs measured at different temperatures is displayed in Fig. 13.12 as an example. The full lines are fits according to an expression derived for the energy dependence of the process [Stu62]; note also the strong temperature dependence and the thermal smearing of the excitonic absorption peak

– both natural consequences of the small energy scales involved.

13.2 Effects of interactions and disorder

Optical transitions discussed previously occur for pure and crystalline semiconductors where the nature of transition and its dependence on the underlying band structure depends essentially on the existence of well defined k states. Now we turn to situations where this strict periodicity is broken, either by the introduction of impurities or by the preparation conditions which prevent the lattice forming. In the former case we talk about impure semiconductors; and in the latter case about amorphous semiconductors.

13.2.1 Optical response of impurity states of semiconductors

Impurity states have been extensively studied by a wide range of optical methods, mainly because of the enormous role these electronic states play in the semiconductor industry. Extrinsic conduction associated with such impurity states is a standard issue for solid state physics, and transport effects which depend on the impurity concentration are also well studied. For small concentrations these impurity states are localized to the underlying lattice, but an insulator–metal transition occurs at zero temperature [Cas89] as the impurity concentration increases.

While there are numerous examples for these impurity effects phenomena, they have been studied in detail for phosphorus doped silicon Si:P. From transport and various spectroscopic studies it is found, for example, that the ionization energy, i.e. the energy needed to promote an electron from the j = 1 level of the donor phosphorus to the conduction band, is 44 meV; via the description (6.5.3) in terms of Bohr’s model this corresponds to the spatial extension of the impurity states of approximately 25 A,˚ significantly larger than the lattice periodicity. It is also known that due to valley–orbital interaction the various s and p impurity levels are slightly split; this splitting is about one order of magnitude smaller than the ionization energy. Localized impurity states can be described by the Rydberg