The inelastic electron – polar optical phonon scattering in

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The inelastic electron – polar optical phonon scattering in HgTe

MALYK O.P.

Semiconductor Electronics Department

“Lviv Polytechnic” National University

Bandera Street. 12, 79013, Lviv,

UKRAINE

Abstract: The model of inelastic electron scattering on polar optical phonons is proposed in which the scattering probability does not depend on macroscopic parameter – crystal permittivity. The reviewed model gives the good agreement between the theory and experiment in temperature range 77 - 300

К.

Key-Words: Electronic Transport , Inelastic Scattering , Mercury Telluride

1 Introduction

The electron-polar optical phonon scattering was considered in relaxation time approximation in [1]. In

[3, 4] this scattering mechanism was considered in view of inelastic character of scattering within the framework of a precise solution of the stationary

Boltzmann equation. There was exhibited that the crystal oscillations; b q ,

and b

 q ,

- operators of phonons annihilation and birth respectively of

-th branch with wave vector q ;

(

  i ( n

1

, n

2 n

2

, n

3 n

3

) a

0

2

1 , 2 ...

 j (

) ,

n

1 a

0

 n

3

) a

0

2

 k ( n

2

 n

1

) a

0

2

- lattice constant;

, i , j , k

-

usage of standard model of electron - polar optical phonon scattering reduces to a disagreement between

unitary vectors along crystal principal axis.

the theory and experiment in temperature range Т>

100 К. According to our opinion this model has following shortages: 1) the use of macroscopic parameter - permittivity- is not reasonable in

Under optical oscillations in a unit cell a polarization vector arises:

P

 e ( Q

1

V

0

Q

2

)

,

(2) microscopic processes; 2) the interaction potential of an electron with optical oscillations of a crystal lattice is long-range that contradicts the special relativity. The purpose of the present work is the build-up of such a model of scattering which at first would well match with experiment and secondly would not have the where V

0

 a

4

0

- the volume of the unit cell; e - elementary charge.

Using (1) and taking into account only the long wave ( q

0 ) oscillations one can obtain: above mentioned shortages.

2 The model of the electron – polar

4 e

P

 b q a

,

3

0 e

 q ,

 i qρ

2 M

 b q

,

 e

( q

 i qρ

)

1

2

( ξ

1

( q ,

)

 ξ

2

( q ,

) )

.

(3)

optical phonon scattering

Let's consider a displacement of j-th ( j =1, 2) atom in a unit cell of a crystal with zinc blende structure under the influence of optical oscillations [5]:

It must be noticed that the polarization vector is a function of discrete variables P

P ( n

1

, n

2

, n

3

) . To calculate the bound charge

 

div P let's make following replacement of a partial derivative of a

Q

  * j

(

1

G q ,

 q ,

) b q

,

2 M e

 i q

 q ) 

1

2

 j

( q ,

) b q ,

 e i q

 

(

, (1) where G – a number of unit cells in a crystal volume; M = M

Hg

+ M

Te

- the mass of the unit cell; q and

( q ) - wave vector and angular frequency of

-th branch of a crystal optical oscillations respectively (

 

4 , 5 , 6 ) ;

 j

- polarization vector of polarization vector on coordinates:

P x x

P x

( n

1

1 , n

2

, n

3

) x

P x

( n

1

P x

( n

1

, n

2

1 , n

3

)

P x

( n

1

, n

2

, n

3

, n

2

)

P x

( n

1

, n

2

, n

3

 x

1 )

 x

P x

( n

1

, n

2

, n

3

)

, n

3

)

, (4) where structure.

 x

 a

0

2

for a unit cell of the zinc blende

The similar relations can be written for partial derivatives

P y

 y

and

P z z with

 y

  z

 a

2

0

.

Then Poisson equation for a scalar potential bound up with crystal oscillations becomes:

 2   

0

8 i e a

0

3 

0

 q

2 G

( q ) 

 1 2

 

M

 b q

M

Hg e

Hg i qρ

M

M

Te

Te

 b q

 

 e

1 2

(

 i qρ q x

 q y

 q z

)

2

 q

, (5) where the relation q i a

0

2



1 ( i

 x , y , z ) is used and only optical longitudinal vibrations are taken into account,

0

- dielectric constant.

To solve the equation (5) let’s substitute the unit cell by an orb of effective radius R

  a

0

the magnitude which lays within the limits from half of smaller diagonal up to half of greater diagonal of a unit cell ( 0.5

< γ < 3 2 ). Magnitude γ =0.628 is picked so to adjust the theory with experiment.

Spherically symmetric solution of a Poisson equation looks like:

 

2

0

( R

2  r

3

) , ( 0

 r

R ) . (6)

Then the interaction energy of an electron with polar optical oscillations of a lattice is determined from expression:

U

  e

 

4 i e a

0

3 

2

0

( R

2  r

3

)

 q

2 G

( q ) 

 1 2

 

 b

M q

M e

Hg

Hg

 i qρ

M

M

Te

Te

 b q

 

 e

1 2

(

 i qρ q x

 q y

 q z

)

2

 q

.

(7)

Let's mark that the potential (7) is short-range as it takes into account interaction of an electron only with one unit cell. To calculate the transition probability connected with electron – phonon interaction let’s write the wave function of the system “electron + phonons” in a form:

 

1 exp( i kr )

( x

1

, x

1

...

x n

) , (8)

V where V - crystal volume;

( x

1

, x

1

...

x n

) - wave function of the system of independent harmonic oscillators.

Then the transition matrix element from interaction energy looks like:

N

 q

, k

| U | N q

, k

  a

0

4 i e

3 

0

2

V

 exp( i s r ) ( R

2  r

3

) d r

 q

2 G

  

(

( q )

 1 x

1

, x

1

...

x n

2

)

 

 b q

 dx

1 dx

2

...

dx n

, s

M

M

Hg e k

Hg i qρ

M

M

Te

 b

Te

 q

 

 e

1 2

 i qρ

( q x

(

 x

1 q

, y q x

1

 q z

...

x n k

.

(9)

)

2

)

The integration over the electron coordinates is carried out in the limits of unit cell and gives:

I ( s )

  exp( i s r ) ( R

2  r

) d r

3

( 8 sin Rs

8 Rs cos Rs

8 3 R

3 s

3 cos Rs )

(10) s

5

The calculation shows that the electron wave vector ( and s together with it) varies within the limits from 0 up to 10 9 м -1 at energy changing from 0 up to 10 к

В

Т ( к

В

– Boltzmann constant) at the temperature range 4.2 – 300 К .

I ( s ) / I ( 0 )

1,0

0,5

0,0

10

7

10

8 s

10

9

10

10

10

11

Fig. 1. The dependence of the function I ( s ) from s

| k

 k

| .

I ( 0 )

As introduced at fig. 1 the dependence of the value

I ( s ) I ( 0 ) from s it is seen that at the indicated limits of varying of wave vector the following relation is well fulfilled:

I ( s )

I ( 0 )

16 15

R

5 

16 15

 a

0

5  5

The integration over the harmonic oscillators coordinates gives the factors N q

and N q

1

( N q

– the number of phonons with a frequency

( q )

 

0 at q

0 ) for phonon annihilation and birth operators respectively. To

calculate the sum over the vector q let’s do the following simplifications –1) taking into consideration quasi continuous character of varying of wave vector let’s pass from summation to integration over q ; 2) let's pass from an integration on a cube with a crossbar

2

 a

0

to an integration on an orb with effective radius

 a

0

:

 q

...

(

V

2

2

 

 

0 0 0 a

0

...

q

2

)

3

 a

0

 a

0

   a

0 a

0 a

0

...

dq x a

0 dq y dq z

 sin

 dq d

 d

.

(11)

Then we obtain for the sum the following expression:

 q

...

F (

)

 

8 cos

Q

8

Q sin

Q

 4

4

 2

Q

2 cos

Q

8



N q

N q

 absorption ;

1

 radiation.

Q

  a

0

.

(12)

As introduced at fig. 2 the dependence of the value

F (

) / F ( 0 ) from

it is seen that the function

F (

) can be approximated by the expression:

F ( 0 )

 

Q

4 



N q

N q

1

(12a)

F (

) / F ( 0 )

1,0

0,5

0,0

10

-11

1x10

-10

1x10

-9

1x10

-8

Fig. 2. The dependence of the function

F (

) / F ( 0 ) from

.

After the calculations we can obtain the expression for electron transition probability connected with phonon absorption and radiation:

W ( k , k

)

64

225

0

2

7 a

0

10

4 e

G

4

0

M

M

Hg

Hg

M

M

Te

Te

N q

(

     

0

)

( N q

 where

- electron energy.

1 )

(

     

0

)

, (13)

10

7

10

6

10

5

2

1

10

4

T , K

100

Fig. 3. The temperature dependence of electron mobility in HgTe : solid line –mixed scattering mechanism; 1 –intraband scattering; 2 –interband scattering. Experiment – [2].

On the base of this for intra- and interband electron transitions the values K n m

  a b

figuring in a method of a precise solution of the stationary

Boltzmann equation can be obtained [3,4] :

K n m

 

1 1

 

2

2 V

 

3

64

675

0

6

2 e a

4

0

2

0

 k

10

B

T

M

M

Hg

Hg

M

M

Te

Te

N

 k (

 q f

0

 

(

0

)

1

)

( f

0

N

( q

1

)

0

(

)

 k

2

(

0

)

 f

0

(

0

)

)

1

 f

0

(

  

0

)

 k

2

(

  

0

)

 k (

 

 

0

) k

4



(

)

 k (

 

)

 n

 m d

;

K n m

 

1 2

 

2

2 V

 

3

32

675

0

6 e

4 

2 a

0

2  10

0 k

B

T

M

M

Hg

Hg

M

M

Te

Te 

(

2 m h h

 

 2

  g

3

2 where



( N q

1 ) f

0

(

)

1

 f

0

(

 

0

)

 

0

)

1

2 k

4

(

)

 k (

 

)



- Kronecker delta ; n

 m f

0

( d

,

) - Fermi –

Dirac function;

( x ) - step function.

The calculation of the temperature dependence of electron mobility was made for acceptor concentration

N

A

= 3 x 10 15 сm -3 thus it is possible to neglect the contribution of heavy holes ( about 1%). At calculations the same scattering mechanisms as in

[3,4] were taken into consideration. As it seen from

Fig. 3 the theoretical curve well coincides with experimental data at the temperature range T >100 K.

It testifies that the model, offered by us, adequately describes the electron-polar optical phonon scattering process as against model introduced in [1]. From figure it is also seen that the basic scattering mechanism in the interval T > 100 K is intraband scattering on polar optical phonons. The contribution of the interband scattering is negligible and can be neglected.

3 Conclusion

The model of inelastic electron-polar optical phonon scattering in HgTe is designed which in the framework of a precise solution of the stationary

Boltzmann equation well coincides with experiment at the temperature range T > 100 K.

References:

[1] W. Szymanska, T. Dietl, Electron scattering and transport phenomena in small-gap zinc-blende semiconductors, J. Phys. Chem. Solids, Vol. 39,

1978, pp. 1025-1040.

[2] J. Dubowski, T. Dietl, W. Szymanska, Electron scattering in Cd x

Hg

1-x

Te, J. Phys. Chem. Solids,

Vol. 42, 1981, pp. 351-362.

[3] O.P.Malyk, Nonelastic electron scattering in mercury telluride. Ukr. Phys. Zhurn., Vol.47,

2002, pp. 842-845.

[4] O.P. Malyk, Nonelastic charge carrier scattering in mercury telluride, Accepted to publication in

Journal of Alloys and Compounds.

[5] V.L. Bonch-Bruevich, S.G. Kalashnikov, Physics of Semiconductors, Nauka, Moscow, 1977 (in

Russian).

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