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SOUND DISPERSION FOR 3He (B) AND NEUTRAL SUPERFLUIDS WITH BCS PAIRING AT T = 0

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Submitted on 1 Jan 1978

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SOUND DISPERSION FOR 3He (B) AND NEUTRAL

SUPERFLUIDS WITH BCS PAIRING AT T = 0

J. Czerwonko

To cite this version:

(2)

JOURNAL DE PHYSIQUE Colloque C6, supplément au n" 8, Tome 39, août 1978, page C 6.9

SOUND DISPERSION FOR

3

He (B) AND NEUTRAL SUPERFLUIDS WITH BCS PAIRING AT T = 0

J. Czerwonko

Institute of Physios, Technical University of Wvooiaw, Wybrzeze Wyspianskiego 27, 50-370 Wroeiaw,

Poland.

Résumé.- Dans le cas d'un régime sans collisions et en considérant aussi le terme de l'ordre de kv(kv/2A)2, on a obtenu la dispersion du son pour He(B) et les liquides superfluides neutres avec le couplage BCS pour la température T = 0. On a montré que lorsque seul le couplage est important dans le canal particule-particule, le terme considéré contient les amplitudes spin-direct de Landau limitées à { , = 0 e t à £ = 1. Pour He (B) le terme correctif est négatif pour toutes les pressions. Pour les pressions supérieures à 20 bars le coefficient de ce terme correctif est de l'ordre de quelques milliers.

Abstract.- The dispersion of sound for He(B) and neutral superfluids with BCS pairing is obtained at T = 0 and in the collisionless regime, taking into account also the term of the order of kv(kv/2A)2. It is shown that spin-direct Landau amplitudes restricted to X, = 0 and 1 enter to this term, if only the pairing interaction is important in the particle-particle channel. For 3He (B) the correction term is negative at all pressures. The coefficient near this term is of the order of a few thousands for pressures greater than 20 bars.

The expression for correlation functions of normal Fermi liquids (NFL), in terms of matrix ele-ments of the appropriate resolvent operator, was per-formed by Luttinger and Noziere IM and by Leggett

111. These papers demonstrated that such an expres-sion is useful in some proofs or computations for NFL. We extended this program, 131, into superfluid Fermi liquids (SFL) with isotropic BCS pairing and with' BW pairing /4/. A starting point was Larkin-Migdal equations 15/ for BCS-SFL and our extension of these equations for BW-SFL /6/. The last case corresponds to 3He(B). We restricted ourselves to the consideration of only the pairing harmonic in the particle-particle channel of effective interac-tion and to the collisionless regime. Moreover, only spiniess vertices were considered by us but, on the other hand, our expressions, /3/, were valid also for T # 0.

According to 131, the poles of correlation functions describing spiniess longitudinal response of SFL, are given by B = 0 (BCS), BD - C2 = 0 (BW), (1) where B = <(t2-u2w2)g> - <(t+uw)gRAg(t+uw' )>, (2) C = <(l-w2)(t2-u2w2)g> - <(l-w2)(t+uw)gRAg(t+uw')> (3) D = <(l-w2)g(t2-u2w2-w2)> - <(l-w2)(t+uw)gRAg(t+w') (l-w'2)> (4)

Let us list the symbols appearing above. The bra-cket <...> denotes the average over spherical an-gles, t = u)/2A, u = kv/2A, where co, k are the

fre-quency and the wave vector of an external field, v is the quasiparticle velocity on the Fermi surface and A - the energy gap of SFL. The variable w = cos 9, with 8 being the azimuthal angle. The func-tion g passes, for T = 0, into the funcfunc-tion g(6), B2 = |t2 - u2 w2|, defined in /5,6/. For T 5* 0 g is the Maki-Ebisawa III function, which is not only 3 - dependent. For our present purposes it is suf-ficient to know that, for T = 0, g % 1 + 2(t2 - u2 w2)/3.

Among other symbols appearing in (2)-(4) A denotes spin-direct dimensionless Landau function, defined in a usual way, and determining appropriate Landau parameters. The symbol R is defined as the operator inverse to (1-AQ), where

Q = -j- g(l+?) + uw(l-g)/(t-uw), (5)

and P is the reflection operator of a unit vector connected with the integration over spherical an-gles. Note that the second terms of the formulae (2)-(A) should be treated as the matrix elements of the operator RA between the functions standing on both sides of RA. The multiplication of operators assumes there the average over intermediate sphe-rical angles.

It is easy to see that for u,t « 1 B,C = = 0(u2,t2) whereas D = 0(1). Hence, remembering also (1), one finds that the main terms of the dis-persion of sound coincide for BCS and BW SFL s. In order to calculate the next terms one has to calcu-late B with the accuracy up to fourth order terms

(3)

and C,D

-

up to the second order terms. Let us ex-

pand R and g

(6)

in (2)-(4)

with respect to t

and u

with the above accuracy. Then, of simple applica-

tion of recurrence properties and the addition the-

orem for spherical functions show us that Landau

parameters fork

=

0 and

1

enter to such B and C

whereas to D

-

for R

<

3

;

D

%

-

2/15 if one ne-

glects second order terms. Finding zeros of the

function B one can express

w

as a function of k

as follows

w

=

kv(XY/3)'I2

{I-

(Y-I)(x-I)~

+

$

XY

1,

(6)

9X

'

[

1

where X

-

1

+

Ao, Y

Z 1 +

Al/3,

with A,

-

Landau

parameters for

9, =

0 and

1.

The variables X,Y have

to be positive in virtue of stability conditions of

FL 181. The formula (6) gives the sound dispersion

curve for BCS SFL.

For BW SFL the equation (1)

is more complica-

ted

;

it contains also A2,A3 via D. Taking into

account that

B =

t2/x-u2y/3

+

H.O.T. we find that

B

=

0(u4) on the dispersion curve. Hence, if we are

looking for zeros of BD-c2, we can neglect second

order terms in D. Hence, taking into account that

C

%

2t2/3x-2u2y/15 passes on the dispersion curve

into 4u2/45, and the formula (6) we find.

' 1 2

w

=

kv(XYI3)

{I-

+

-5.

XY

1.

(7)

9X

I

In such a way the sound dispersion curve was obtai-

ned for BW SFL, .i.e. 3~e(~).

It is easy to see that, according to 191, the

correction term in (7) is negative for 3 ~ e ( ~ )

for

all pressures.

The correction terms in the curly bracket (7)

divided by -u2 are listed in table

I,

for

p

from

zero to

34.36

bars. Parameters A g and Al are taken

from

/ 9 / ;

is is assumed that their accuracy is

f

0.005, which allow us to estimate the error of

the correction term. Direct multiplication of our

errors allow to pass to more realistic case. It is

easy to estimate that for

w %

10' Hz the correction

term should be remarkable at p

>

20 bars. For so

high frequencies the regime should be rather colli-

sionless.

This work was performed during my short stay

at the University of Sussex. I

am greatly indebted

to Professors D.F. Brewer and A.J. Leggett for

their kind hospitality.

TABLE

I

p = 0 ; 33.6410.1

p

=

12

;

559.17' 0.9

p

=

3

;

88.07 f

0.2

p

=

15

;

845.71

'

1.3

p

=

6

;

190.53 kO.4

p

=

18

;

1212.21

+

1.7

p

=

9

;

344.62

f

0.6

p

=

21

;

1645.44

f

2.2

p

=

24 ;2162.73

+

2.8

p

=

33

;

4576.75

+

5

p

=

27 ;2826.74

2

3.4

p =34.36 5105.36

f

5.5

p

=

30 ;3617.81

2

4.1

References

/I/ Luttinger, J.M. andNoziSres, P., Phys. Rev.

127

(1962) 1431.

/2/ Leggett, A.J., Ann. Phys.

46

(1968) 76.

/3/ Czerwonko, J., in preparation.

141 Balian, R. and Werthamer, N.R., Phys. Rev.

131

(1963) 1553.

/5/ Larkin, A.I. and Migdal, A.B., Zh.Eksp. Teor.

Fiz.

5

(1963) 1703.

/6/ Czerwonko, J., Acta Phys. Polon.

32

(1967) 335.

171 Maki, K. and Ebisawa, H., J.Low Temp. Phys.

15

(1974) 213.

/8/ Pomeranchuk, I.Ya., Zh. Eksp.Teor..Fiz.

2

(1958) 524.

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