Carsten Timm: Theory of superconductivity
Carsten Timm: Theory of superconductivity
Carsten Timm: Theory of superconductivity
You also want an ePaper? Increase the reach of your titles
YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.
6<br />
Ginzburg-Landau theory<br />
Within London and Pippard theory, the superfluid density n s is treated as given. There is no way to understand<br />
the dependence <strong>of</strong> n s on, for example, temperature or applied magnetic field within these theories. Moreover, n s<br />
has been assumed to be constant in time and uniform and in space—an assumption that is expected to fail close<br />
to the surface <strong>of</strong> a superconductor.<br />
These deficiencies are cured by the Ginzburg-Landau theory put forward in 1950. Like Ginzburg and Landau<br />
we ignore complications due to the nonlocal electromagnetic response. Ginzburg-Landau theory is developed as<br />
a generalization <strong>of</strong> London theory, not <strong>of</strong> Pippard theory. The starting point is the much more general and very<br />
powerful Landau theory <strong>of</strong> phase transitions, which we will review first.<br />
6.1 Landau theory <strong>of</strong> phase transitions<br />
Landau introduced the concept <strong>of</strong> the order parameter to describe phase transitions. In this context, an order<br />
parameter is a thermodynamic variable that is zero on one side <strong>of</strong> the transition and non-zero on the other. In<br />
ferromagnets, the magnetization M is the order parameter. The theory neglects fluctuations, which means that<br />
the order parameter is assumed to be constant in time and space. Landau theory is thus a mean-field theory. Now<br />
the appropriate thermodynamic potential can be written as a function <strong>of</strong> the order parameter, which we call ∆,<br />
and certain other thermodynamic quantities such as pressure or volume, magnetic field, etc. We will always call<br />
the potential the free energy F , but whether it really is a free energy, a free enthalpy, or something else depends<br />
on which quantities are given (pressure vs. volume etc.). Hence, we write<br />
F = F (∆, T ), (6.1)<br />
where T is the temperature, and further variables have been suppressed. The equilibrium state at temperature<br />
T is the one that minimizes the free energy. Generally, we do not know F (∆, T ) explicitly. Landau’s idea was to<br />
expand F in terms <strong>of</strong> ∆, including only those terms that are allowed by the symmetry <strong>of</strong> the system and keeping<br />
the minimum number <strong>of</strong> the simplest terms required to get non-trivial results.<br />
For example, in an isotropic ferromagnet, the order parameter is the three-component vector M. The free<br />
energy must be invariant under rotations <strong>of</strong> M because <strong>of</strong> isotropy. Furthermore, since we want to minimize F<br />
as a function <strong>of</strong> M, F should be differentiable in M. Then the leading terms, apart from a trivial constant, are<br />
F ∼ = α M · M + β 2 (M · M)2 + O ( (M · M) 3) . (6.2)<br />
Denoting the coefficients by α and β/2 is just convention. α and β are functions <strong>of</strong> temperature (and pressure<br />
etc.).<br />
What is the corresponding expansion for a superconductor or superfluid? Lacking a microscopic theory,<br />
Ginzburg and Landau assumed based on the analogy with Bose-Einstein condensation that the superfluid part is<br />
described by a single one-particle wave function Ψ s (r). They imposed the plausible normalization<br />
∫<br />
d 3 r |Ψ s (r)| 2 = N s = n s V ; (6.3)<br />
30