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Carsten Timm: Theory of superconductivity

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As above, we keep only terms up to second order in the fluctuations (Gaussian approximation), i.e., terms<br />

proportional to δψ 2 , δψ ϕ, or ϕ 2 . We get<br />

∫ [<br />

F [δψ, ϕ] ∼ ✭<br />

= d 3 r ✭✭✭✭✭✭✭<br />

2αψ 0 δψ + 2βψ0δψ 3 + αδψ 2 + 3βψ0δψ 3 2 + 1 ( ) ∗ <br />

2m ∗ i ∇δψ · <br />

i ∇δψ<br />

(<br />

+ 1 ( ) )<br />

]<br />

∗ <br />

2m<br />

✭✭✭✭✭✭✭✭✭✭✭✭✭✭✭✭✭✭<br />

∗ i ∇δψ · ψ 0 ∇ϕ + (ψ 0 ∇ϕ) ∗ · <br />

i ∇δψ + 1<br />

2m ∗ (ψ 0∇ϕ) ∗ · ψ 0 ∇ϕ (+ const). (6.40)<br />

Note that the first-order terms cancel since we are expanding about a minimum. Furthermore, up to second order<br />

there are no terms mixing amplitude fluctuations δψ and phase fluctuations ϕ. We can simplify the expression:<br />

[<br />

−2αδψ 2 + 1<br />

2m ∗ ( <br />

i ∇δψ ) ∗<br />

· <br />

i ∇δψ −<br />

∫<br />

F [δψ, ϕ] ∼ = d 3 r<br />

= ∑ [(<br />

−2α + 2 k 2 )<br />

}{{} 2m ∗ δψkδψ ∗ k − α β<br />

k > 0<br />

2 k 2<br />

2m ∗<br />

} {{ }<br />

> 0<br />

]<br />

2 α<br />

2m ∗ β (∇ϕ)∗ ∇ϕ<br />

ϕ ∗ kϕ k<br />

], (6.41)<br />

in analogy to the case T > T c . We see that amplitude fluctuations are gapped (massive) with an energy gap<br />

−2α = α ′ (T c − T ). They are not degenerate. Phase fluctuations on the other hand are ungapped (massless) with<br />

quadratic dispersion<br />

ϵ ϕ k = −α 2 k 2<br />

β 2m ∗ . (6.42)<br />

The appearance <strong>of</strong> ungapped so-called Goldstone modes is characteristic for systems with spontaneously broken<br />

continuous symmetries. We state without derivation that the heat capacity diverges like C ∼ √ T c − T for<br />

T → Tc − , analogous to the case T > T c .<br />

6.3 Ginzburg-Landau theory for superconductors<br />

To describe superconductors, we have to take the charge q <strong>of</strong> the particles forming the condensate into account.<br />

We allow for the possibility that q is not the electron charge −e. Then there are two additional terms in the<br />

Landau functional:<br />

• The canonical momentum has to be replaced by the kinetic momentum:<br />

where A is the vector potential.<br />

• The energy density <strong>of</strong> the magnetic field, B 2 /8π, has to be included.<br />

<br />

i ∇ → i ∇ − q A, (6.43)<br />

c<br />

Thus we obtain the functional<br />

∫<br />

F [ψ, A] ∼ =<br />

[<br />

d 3 r α |ψ| 2 + β 2 |ψ|4 + 1 ∣( ∣∣∣ <br />

2m ∗ i ∇ − q )<br />

c A ψ<br />

∣<br />

2<br />

+ B2<br />

8π<br />

]<br />

. (6.44)<br />

Minimizing this free-energy functional with respect to ψ, we obtain, in analogy to the previous section,<br />

1<br />

2m ∗ ( <br />

i ∇ − q c A ) 2<br />

ψ + α ψ + β |ψ| 2 ψ = 0. (6.45)<br />

37

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