Carsten Timm: Theory of superconductivity
Carsten Timm: Theory of superconductivity
Carsten Timm: Theory of superconductivity
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5<br />
Electrodynamics <strong>of</strong> superconductors<br />
Superconductors are defined by electrodynamic properties—ideal conduction and magnetic-field repulsion. It is<br />
thus appropriate to ask how these materials can be described within the formal framework <strong>of</strong> electrodynamics.<br />
5.1 London theory<br />
In 1935, F. and H. London proposed a phenomenological theory for the electrodynamic properties <strong>of</strong> superconductors.<br />
It is based on a two-fluid picture: For unspecified reasons, the electrons from a normal fluid <strong>of</strong> concentration<br />
n n and a superfluid <strong>of</strong> concentration n s , where n n + n s = n = N/V . Such a picture seemed quite plausible based<br />
on Einstein’s theory <strong>of</strong> Bose-Einstein condensation, although nobody understood how the fermionic electrons<br />
could form a superfluid. The normal fluid is postulated to behave normally, i.e., to carry an ohmic current<br />
governed by the Drude law<br />
j n = σ n E (5.1)<br />
σ n = e2 n n τ<br />
m . (5.2)<br />
The superfluid is assumed to be insensitive to scattering. As noted in section 4.2, this leads to a free acceleration<br />
<strong>of</strong> the charges. With the supercurrent<br />
j s = −e n s v s (5.3)<br />
and Newton’s equation <strong>of</strong> motion<br />
d<br />
dt v s = F m = −eE m , (5.4)<br />
we obtain<br />
∂j s<br />
∂t = e2 n s<br />
E. (5.5)<br />
m<br />
This is the First London Equation. We are only interested in the stationary state, i.e., we assume n n and n s to be<br />
uniform in space, this is the most serious restriction <strong>of</strong> London theory, which will be overcome in Ginzburg-Landau<br />
theory.<br />
Note that the curl <strong>of</strong> the First London Equation is<br />
This can be integrated in time to give<br />
∂<br />
∂t ∇ × j s = e2 n s<br />
m ∇ × E = n s<br />
−e2 mc<br />
∂B<br />
∂t . (5.6)<br />
∇ × j s = − e2 n s<br />
B + C(r), (5.7)<br />
mc<br />
where the last term represents a constant <strong>of</strong> integration at each point r inside the superconductor. C(r) should<br />
be determined from the initial conditions. If we start from a superconducting body in zero applied magnetic<br />
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