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Boris V. Vasiliev Supercondustivity Superfluidity

Boris V. Vasiliev
Supercondustivity Superfluidity

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Superconductivity and Superfluidity<br />

Unfortunately, no direct experiments of the effect of isotopic substitution on the<br />

electronic properties (such as the electronic specific heat and the Fermi energy), exist for<br />

metals substantial for our consideration.<br />

Let us consider what should be expected in such measurements. A convenient choice<br />

for the superconductor is mercury, as it has many isotopes and their isotope effect has<br />

been carefully measured back in the 50s of the last century as aforementioned.<br />

The linear dependence of the critical temperature of a superconductor on its Fermi<br />

energy (Eq.(6.20)) and also the existence of the isotope effect suggests the dependence of<br />

the ion density in the crystal lattice from the mass of the isotope. Let us consider what<br />

should be expected in such measurements.<br />

Even then, it was found that the isotope effect is described by Eq.(10.4) in only a few<br />

superconductors. In others, it displays different values, and therefore in a general case it<br />

can be described by introducing of the parameter a:<br />

Mi a T c = Const. (10.5)<br />

At taking into account Eq.(6.20), we can write<br />

T c ∼ E F ∼ n 2/3<br />

e (10.6)<br />

The parameter l which characterizes the ion lattice obtains an increment ∆l with an<br />

isotope substitution:<br />

where M i and ∆M i are the mass of isotope and its increment.<br />

∆l<br />

l<br />

= − a 2 · ∆M i<br />

M i<br />

, (10.7)<br />

It is generally accepted that in an accordance with the terms of the phonon mechanism,<br />

the parameter a ≈ 1 2<br />

for mercury. However, the analysis of experimental data [35]-[<strong>36</strong>]<br />

(see Figure 4.3) shows that this parameter is actually closer to 1/3. Accordingly, one can<br />

expect that the ratio of the mercury parameters is close to:<br />

)<br />

(<br />

( ∆l<br />

l<br />

∆M i<br />

M i<br />

) ≈ − 1 6 . (10.8)<br />

106 Science Publishing Group

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