Page 401 - Electrical Properties of Materials
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The Landau–Ginzburg theory                         383

               will add to the total energy. It follows then that the appearance of alternating
               layers of normal and superconducting domains is energetically unfavour-
               able because it leads to a rapid variation of ψ, giving a large kinetic energy
               contribution to the total energy.
                 Equation (14.38) is not quite correct. It follows from classical
                            ∗
               electrodynamics that in the presence of a magnetic field the momentum  ∗  For a discussion, see The Feynman lec-
               is given by p – eA, where A is the magnetic vector potential. Hence, the  tures on Physics, vol. 3, pp. 21–5.
               correct formula for the kinetic energy is

                                       1               2                     2e is the charge on a superconduct-
                                 KE =    |–i ∇ψ –2eAψ| .             (14.39)
                                      2m                                     ing electron.

                 We may now write the Gibbs free energy in the form,

                                  1        2   1               2
                   G s (B)= G s (0) +  (B a – B) +  |–i ∇ψ –2eAψ| .  (14.40)
                                 2μ 0         2m

            5. The value of the Gibbs function at zero magnetic field should depend on
               the density of superconducting electrons, among other things. The simplest
               choice is a polynomial of the form,
                                                 2
                                                        4
                                G s (0) = G n (0) + a 1 |ψ| + a 2 |ψ| ,  (14.41)
               where the coefficients may be determined from empirical considerations. At
               a given temperature the density of superconducting electrons will be such
               as to minimize G s (0), that is,

                                        ∂G s (0)
                                              = 0,                   (14.42)
                                         ∂|ψ| 2

               leading to

                                             2
                                       2
                                    |ψ| ≡ |ψ 0 | =–  a 1  .          (14.43)
                                                  2a 2
                                        2
                 Substituting this value of |ψ| back into eqn (14.41) we get

                                                 a 2 1
                                     G s (0) = G n –  .              (14.44)
                                                4a 2
               Let us go back now to eqn (14.22) (rewritten for unit volume),


                                                    2
                                               1
                                    G s (0) = G n – μ 0 H .          (14.45)
                                               2    c
                 Comparing the last two equations, we get
                                                                             It is assumed that a 2 > 0 and
                                    H c =–a 1 /(2a 2 μ 0 ) 1/2 .     (14.46)  a 1 < 0.
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