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Boris V. Vasiliev Supercondustivity Superfluidity

Boris V. Vasiliev
Supercondustivity Superfluidity

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Superconductivity and Superfluidity<br />

where a and b are model parameters. Using the principle of minimum free energy of the<br />

system in a steady state, we can find the relation between these parameters:<br />

d(∆W )<br />

dn s<br />

= −a + b · n s = 0. (4.13)<br />

Whence<br />

b = a n s<br />

(4.14)<br />

and the energy gain in the transition to an ordered state:<br />

∆W = − a 2 n s. (4.15)<br />

The reverse transition from the superconducting state to a normal state occurs at the<br />

critical magnetic field strength, H c . This is required to create the density of the magnetic<br />

energy H2 c<br />

8π<br />

. According to the above description, this equation is therefore obtained:<br />

H 2 c<br />

8π = a 2 n s. (4.16)<br />

In order to express the parameter a of GL-theory in terms of physical characteristics of<br />

a sample, the density of “superconducting” carriers generally charge from the London’s<br />

equation (4.8). 2<br />

The important step in the Ginzburg-Landau theory is the changeover of the<br />

concentration of superconducting carriers, n s , to the order parameter Ψ<br />

|Ψ(x)| 2 = n s . (4.17)<br />

At this the standard Schrodinger equation (in case of one dimension) takes the form:<br />

−<br />

<br />

2m [∇Ψ(x)]2 − aΨ 2 (x) + b 2 Ψ4 (x) = E. (4.18)<br />

Again using the condition of minimum energy<br />

dE<br />

dΨ = 0 (4.19)<br />

2 It should be noted that due to the fact that the London equation does not correctly describes the ratio of the<br />

penetration depth with a density of carriers, one should used the revised equation (9.13) in order to find the<br />

a.<br />

34 Science Publishing Group

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