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Submitted on 1 Jan 1978
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OSCILLATIONS OF THE RELAXATION TIME IN
STRONG MAGNETIC FIELDS
P. Středa, L. Smrćka
To cite this version:
JOURNAL DE PHYSIQUE Colloque C6, suppliment au no 8, Tome 39, aolit 1978, page C6-1110
O S C I L L A T ! O N S O F THE R E L A X A T I O N T I M E I N STRONG MAGNETIC F I E L D S
P. StFeda and L. SmrEka
I n s t i t u t e of Solid State Physics, CzechosZovak Acad. Sci., 162 53 Prague, CzechosZoualcia
R6sumb.- Les oscillations quantiques de la magn6toconductivit6 et de la force magn6to6lectrique sont calculbes dans un modSle de bande de conduction parabolique. L'on montre que la contribution principale 1 ces effets est due aux ascillations du temps de relaxation.
Abstract.- Quantum oscillations of the longitudinal magnetoconductivity and magnetothermopower were calculated for a simple model of solid with parabolic electron band. It is shown that the main con- tribution originates in oscillations of the relaxation time.
INTRODUCTION.- A strong magnetic field applied to the system of electrons causes the quantization of the electron energy spectrum. The quantum effects be- come particularly important at low temperatures and manifest themselves e.g. in the oscillatory behaviour of the magnetic susceptibility and transport coeffi- cients as functions of the magnetic field H. The theory predicts that both the density of electron states p(EF) and the electron mean lifetime =(EF) at the Fermi energy EF will oscillate while changing magnetic field /1,2/. The density of states give the main contribution to the oscillations of susceptibi- lity. In this communication we shall demonstrate
that, at least for a simple model, the oscillations of the longitudinal magnetoconductivity are mainly due to the oscillations in the relaxation time. This effect will even be more pronounced in the longitu-
dinal magnetothennopower S which is related to the longitudinal conductivity all by the Mott formula
written in the well known form
where the effective number of carriers NI, is given /2,4/ by relation
Here G denotes the resolvent
a I ~fi~k:
G~ = [E~
-
E~-
Z(E~)]-'
; E~ = HU(~ + +-
2m(4) where E is the eigenenergy of electron state a, a
a
substitutes for (n,kx,kz). The effective number N
I I
becomes close to the number of electrons only inthelow field limit w~ << 1 and if the Landau-Peierls criterion EF >> l? is well satisfied 141. Let us af- so note that for the short-range scattering poten- tial of impurities the relaxation time appearing in (2) is just equal to the mean lifetime.
(l) RESULTS AND DISCUSSION.- In order to analyse semi- quantitatively the behaviour of conductivity, it is If the scattering of electrons is elastic, and Hw useful to separate all quantities of interest into >> kT holds 131 (L is the Lorenz number, w = eH/mc the smooth and oscillatory parts using the Poisson is the cyclotron frequency). summation formula
+oJ +m +a
THE MODEL AND BASIC FORMULAE
.-
Let the electron stru-1
f (n) =+l
£(X)+
2I
[
f(x)cos(2~x)dx. (5) cture is given by a parabolic dispersion law, and n=o.b
n=16the randomly distributed impurities are described by Then we can write
YI
= No + NosCS T = 'lo+ 'losc
6-fynction-like potentials. The scattering of elec- and the longitudinii conductivity reads trons calculated self-consistently leads to the dam-
Nose
=osc )
,
ping of-singularities in the density of states and l/' = 0' +
-
No ) ( l +-
=o
yields the oscillatory self-energy of electrons C, where smooth n o = e 2 ~ o ~ o / m is multiplied by two oscil- which is related to the mean lifetime r.by expres- lating factors proportional to the relative magni- sion T = %/2r,
r
= -Id. The longitudinal conducti- t u d e ~ of oscillations in N and inx.vity was calculated via the Kubo formula and can be Since ~ ~ ~is approximately equal to the ~ /
11
' l ~p6sc/~o (posc/po is the relative magnitude of osci- llations in the density of states p(E F ) =
-
;
ImC G ) equations (33 and (5) yield the expression
CL a
Condition EF >> implies T ~ ~>>Nosc/~O ~ / T ~and so the oscillations in the relaxation time dominate in the oscillations of conductivity.
This conclusion is confirmed by the numeri- cal results presented in figure 1 which were obtai- ned for the model with parameters corresponding to the case of a strongly doped semiconductor with electron density 10"
Fig.1 : The relative oscillation amplitudes of T ~ ~ (full line) and Nosc/No (broken line) as ~ / T ~ functions of inverse magnetic field.
Though the quantity EF/lfiw ranges only from 2 to 7
and the condition EF >>
h
is only approximately valid, the% those of
relative changes of N I , do not exceed 10 'Cosc/~o '
The relative magnitude of oscillations of the longitudinal magnetoconductivity itself is shown on figure 2, together a' the derivative with
/l'
respect to the EF, which forms the main contribu- tion to the thermopower (1). The very large oscil- lations, which even change the sign of a;,, can be understood on the basis of intimate relation bet- ween the derivatives of a with respect to EF and
l/
with respect to 1 /H.
Fig. 2 : The relative oscillation amplitudes of uosc/~o (broken line) and U
'
/U: (full line) asOSC
functions of inverse magnetlc field.
References
/l/ Tanaka, S. and Morita, T., Progr. Theor. Phys. 47 (1972) 378.
121 Gerhardts, R. and Hajdu, J.Z., Physik 245 (1971) 126.
131 SmrEka, L. and ~t;eda, P., J. Phys. C 10 (1977) 2153.