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Carsten Timm: Theory of superconductivity

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which is valid within the film and away from vortex cores so that |ψ| 2 ∼ = −α/β. However, the current is confined<br />

to the thin film. We can write<br />

j(r) = K(x, y) δ(z) (7.94)<br />

with a surface current density K. Thus<br />

K(x, y) =<br />

∫ ∞<br />

−∞<br />

∫<br />

dz j(r) =<br />

If the thickness is d and A is approximately constant across the thickness, we have<br />

and finally<br />

⇒<br />

film<br />

K(x, y) = − c<br />

4π<br />

j(r) = − c<br />

4π<br />

(<br />

dz −<br />

c )<br />

4πλ 2 A(r). (7.95)<br />

d<br />

A(x, y, 0)<br />

λ2 (7.96)<br />

d<br />

A(r) δ(z)<br />

λ2 (7.97)<br />

∇ 2 A = d A δ(z). (7.98)<br />

λ2 This result exhibits the new length scale that controls the spatial variation <strong>of</strong> A and thus <strong>of</strong> the current j,<br />

λ ⊥ := λ2<br />

d , (7.99)<br />

which is large, λ ⊥ ≫ λ, for a thin film. We see that in thin films, λ ⊥ assumes the role <strong>of</strong> the penetration depth<br />

λ. Since λ ⊥ is large for thin films, one could say that thin films are always effectively <strong>of</strong> type II.<br />

We here do not discuss the full derivation <strong>of</strong> Pearl but only consider the “far field” for large r ≫ λ ⊥ and show<br />

that it does not lead to a diverging free energy for a single vortex. We assume that most <strong>of</strong> the magnetic flux <strong>of</strong><br />

Φ 0 penetrates the film for ϱ = √ x 2 + y 2 λ ⊥ . Then the magnetic field above (and below) the film looks like a<br />

monopole field for r ≫ λ ⊥ .<br />

z<br />

B<br />

This field is easy to obtain from symmetry:<br />

∫<br />

da · B = Φ 0 ⇒ 2πr 2 B = Φ 0 (7.100)<br />

By symmetry,<br />

half space<br />

for z>0<br />

⇒ B(r) = Φ 0<br />

2πr 2 and B(r) = Φ 0 ˆr for z > 0. (7.101)<br />

2πr2 B(r) = sgn z Φ 0 ˆr. (7.102)<br />

2πr2 65

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