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Boris V. Vasiliev Supercondustivity Superfluidity

Boris V. Vasiliev
Supercondustivity Superfluidity

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Chapter 4 Basic Milestones in the Study of Superconductivity<br />

Therefore, the increment of free energy is<br />

δF = δU − T δS − SδT. (4.24)<br />

According to the first law of thermodynamics, the increment of the density of thermal<br />

energy δQ is the sum of the work made by a sample on external bodies δR, and the<br />

increment of its internal energy δU:<br />

δQ = δR + δF (4.25)<br />

as a reversible process heat increment of δQ = T δS, then<br />

δF = −δR − SδT (4.26)<br />

thus the entropy<br />

( ) ∂F<br />

S = − . (4.27)<br />

∂T<br />

R<br />

In accordance with this equation,<br />

superconducting states (4.22) can be written as:<br />

S s − S n = H c<br />

4π<br />

the difference of entropy in normal and<br />

( ∂Hc<br />

∂T<br />

)<br />

. (4.28)<br />

R<br />

Since critical field at any temperature decreases with rising temperature:<br />

( ) ∂Hc<br />

< 0, (4.29)<br />

∂T<br />

then we can conclude (from equation (4.28)), that the superconducting state is more<br />

ordered and therefore its entropy is lower. Besides this, since at T = 0, the derivative of<br />

the critical field is also zero, then the entropy of the normal and superconducting state, at<br />

this point, are equal. Any abrupt changes of the first derivatives of the thermodynamic<br />

potential must also be absent, i.e., this transition is a transition of the order-disorder in<br />

electron system.<br />

Since, by definition, the specific heat C = T ( )<br />

∂S<br />

∂T , then the difference of specific heats<br />

of superconducting and normal states:<br />

[<br />

C s − C n = T (∂Hc ) ]<br />

2<br />

∂ 2 H c<br />

+ H c<br />

4π ∂T ∂T 2 . (4.30)<br />

Science Publishing Group 37

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