Carsten Timm: Theory of superconductivity
Carsten Timm: Theory of superconductivity
Carsten Timm: Theory of superconductivity
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tant. The first one is<br />
(u k ′u k − v k ′v k ) 2 = 1 4<br />
{(<br />
1 +<br />
)<br />
ξ k ′<br />
ξ<br />
√<br />
(1 + √ k<br />
ξ<br />
2<br />
k ′ + ∆ 2 k ξ<br />
2 ′ k<br />
+ ∆ 2 k<br />
ξ k ′ ξ<br />
− 2√ √ k<br />
+<br />
ξ<br />
2<br />
k ′ + ∆ 2 k ξ<br />
2 ′ k<br />
+ ∆ 2 k<br />
= 1 (<br />
1 + ξ kξ k ′<br />
− ∆ )<br />
k∆ k ′<br />
2 E k E k ′ E k E k ′<br />
(<br />
1 −<br />
)<br />
)<br />
ξ k ′<br />
ξ<br />
√<br />
(1 − √ k<br />
ξ<br />
2<br />
k ′ + ∆ 2 k ξ<br />
2 ′ k<br />
+ ∆ 2 k<br />
)}<br />
(10.99)<br />
with E k = √ ξk 2 + ∆2 k<br />
. If the matrix elements B and the normal-state density <strong>of</strong> states are even functions <strong>of</strong> the<br />
normal-state energy relative to the Fermi energy, ξ k , the second term, which is odd in ξ k and ξ k ′, will drop out<br />
under the sum ∑ kk<br />
. Hence, this term is usually omitted, giving the coherence factor<br />
′<br />
F − (k, k ′ ) := 1 (<br />
1 − ∆ )<br />
k∆ k ′<br />
(10.100)<br />
2 E k E k ′<br />
relevant for quasiparticle scattering in ultrasound experiments.<br />
factor<br />
(<br />
σ 2 (u k ′v k + v k ′u k ) 2 = 1 + ∆ k∆ k ′<br />
E k E k ′<br />
}{{}<br />
= 1<br />
Analogously, we obtain the second coherence<br />
)<br />
=: F + (k, k ′ ) (10.101)<br />
for quasiparticle creation and annihilation.<br />
We can gain insight into the temperature dependence <strong>of</strong> ultrasound attenuation by making the rather crude<br />
approximation that the matrix element B is independent <strong>of</strong> k, k ′ and thus <strong>of</strong> energy. Furthermore, typical<br />
ultrasound frequencies Ω satisfy Ω ≪ ∆ 0 and Ω ≪ k B T . Then only scattering <strong>of</strong> quasiparticles by phonons<br />
but not their creation is important since the phonon energy is not sufficient for quasiparticle creation.<br />
The rate <strong>of</strong> ultrasound absorption (attenuation) can be written in a plausible form analogous to the current<br />
in the previous section:<br />
where now<br />
α s ∝<br />
∫ ∞<br />
−∞<br />
dω D s (|ω|) D s (|ω + Ω|) |B| 2 F − (ω, ω + Ω) [n F (ω) − n F (ω + Ω)] , (10.102)<br />
F − (ω, ω ′ ) = 1 2<br />
With the approximations introduced above we get<br />
α s ∝ D 2 n(E F ) |B| 2<br />
∫∞<br />
−∞<br />
( )<br />
1 − ∆2 0<br />
|ω| |ω ′ . (10.103)<br />
|<br />
dω D (<br />
s(|ω|) D s (|ω + Ω|) 1 ∆ 2 )<br />
0<br />
1 −<br />
[n F (ω) − n F (ω + Ω)] . (10.104)<br />
D n (E F ) D n (E F ) 2 |ω| |ω + Ω|<br />
The normal-state attentuation rate is found by letting ∆ 0 → 0:<br />
⇒<br />
α n ∝ D 2 n(E F ) |B| 2<br />
α s<br />
α n<br />
= 1 Ω<br />
∫ ∞<br />
−∞<br />
∫∞<br />
−∞<br />
dω n F (ω) − n F (ω + Ω)<br />
2<br />
dω D s(|ω|) D s (|ω + Ω|) |ω| |ω + Ω| − ∆ 2 0<br />
D n (E F ) D n (E F ) |ω| |ω + Ω|<br />
= 1 2 D2 n(E F ) |B| 2 Ω (10.105)<br />
[n F (ω) − n F (ω + Ω)] . (10.106)<br />
103