Lattice mobility in n-germanium at low temperatures

Lattice mobility in n-germanium at low temperatures

PHYSICS Volume 26A, number 2 LATTICE MOBILITY IN LETTERS n-GERMANIUM 16 December 1967 AT LOW TEMPERATURES K. BAUMANN, P. KOCEVAR and M. KRI...

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PHYSICS

Volume 26A, number 2

LATTICE

MOBILITY

IN

LETTERS

n-GERMANIUM

16 December 1967

AT

LOW

TEMPERATURES

K. BAUMANN, P. KOCEVAR and M. KRIECHBAUM Institut fir theoretische Physik der Universittit Graz, Graz, Austria Received 8 November 1967

The lattice mobility /.l~ of hot electrons is calculated for a sample of n-germanium at 4.0°K. Assuming 5 X lo14 donors per cm3 and a cross-dimension of 0.1 cm, we find /.&L0~ Ti0e9, Te being the electron temperature. _ Conwell [l] has given a theory of the disturbance of the acoustic phonon ‘distribution caused by hot electrons in a many-valley semiconductor at low temperatures. The phonon generation rate is calculated using the electron-phonon scattering matrix elements of Herring and Vogt [2]. For the decrease of the phonon number only boundary scattering is taken into account. Thus the phonon relaxation time is given by L/U,, where L is the smallest cross-dimension of the sample, and u, are the sound velocities. The phonon distribution derived by Conwell may be combined with the expression for the electron relaxation time tensor as given in [2]. In this way we have calculated numerically the electron mobility in n-Ge for six selected electron temperatures between 30°K and 150’K. The other parameters are chosen in accordance with an experiment performed by Seeger [3]. Especially, the sample temperature has been taken as 4.2oK, the carrier concentration as 5 x 1014/cm3 , and L = 0.117 cm. The other constants are the same as in [l]. The electric field vector is assumed to point into the [loo] direction. The field strength belonging to each electron temperature is found from energy balance. Our results are shown in fig. 1. It can be seen that the mobility ,u versus electron temperature T, and field strength E has practically a pure power behaviour , viz.

p cc .,Oag,

and

~1cc E-o.75 .

ELr$TRIC

FIEL,;

(V/cm)

1

EL&&

TEMPE~~URE

loK

)

Fig. 1. The circles represent the points for which the computation was done.

simple parabolic conduction band. Thus we see that the use of spheroidal energy valleys is essential for obtaining the correct field dependence of the mobility. We are grateful to K.Seeger for much valuable advice. Thanks are also due to the Mathematisches Institut der Technischen Hochschule Wien for making available their computer.

(1)

It should be mentioned

tive reasoning

derives

@ 0~ Teoe5,

that Conwell by qualitadifferent power laws, viz.

and

/.~a E-Oa5 .

References

(1’)

The reason for this discrepancy lies in the fact that the dependence of ip (defined in formula (31) of ref. 1 on Te is not negligible. The results (l’), have already been found by Paranjape [4] using a 62

1. 2. 3. 4.

E. M. Conwell, Phys. Rev. 135 (1964) A814. C.Herring and E.Vogt, Phys. Rev. 101 (1956) 944. K.Seeger, Z. Phys. 182 (1965) 510. V.V.Paranjape, Proc. Phys. Sot. (London) 80 (1962) 971.