Page 353 - Determinants and Their Applications in Mathematical Physics
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338   Appendix
                                       c

                              ∇ζ = −    ∇ζ + ,
                                +      2
                                      ζ
                                       +
                                       c          2
                              2            2             2
                             ∇ ζ = −      ∇ ζ + −   (∇ζ + )  .
                                +      2
                                      ζ +        ζ +
          Hence,
                                          c 2
             1          2       2    2         1          2          2
                +
                          +
                                  +
             2 (ζ + ζ )∇ ζ − (∇ ζ ) = −   3    2 (ζ + + ζ − )∇ ζ + − (∇ζ + )
                    −
                                          +
                                         ζ ζ −
                                     =0.


          This identity remains valid when ζ and ζ are interchanged, which proves
                                       +
                                              −
          the validity of transformation γ. It follows from the particular case in which
          c = 1 and d = 0 that if the pair P(φ, ψ) is a solution of (A.12.4) and (A.12.5)
          and
                                           φ
                                   φ =         ,

                                         2
                                        φ + ψ 2
                                            ψ

                                   ψ = −        ,
                                           2
                                         φ + ψ 2



          then the pair P (φ ,ψ ) is also a solution of (A.12.4) and (A.12.5). This
          relation is applied in Section 6.10.2 on the intermediate solution of the
          Einstein equations.
          Transformation ε
          Combining transformation γ and δ with a = d = 1 and c = −2b, it is found
          that if ζ + and ζ − are solutions of (A.12.1) and
                                         ζ − − b

                                    ζ =        ,
                                     +
                                         ζ − + b
                                         b + ζ +
                                    ζ =        ,

                                     −
                                         b − ζ +
          then ζ    and ζ     are also solutions of (A.12.1). This transformation is ap-
               +      −
          plied in Section 6.10.4 on physically significant solutions of the Einstein
          equations.
            The following formulas are well known and will be applied later. (ρ, z)
          are cylindrical polar coordinates:

                                       ∂V ∂V
                                ∇V =      ,     ,                  (A.12.6)
                                        ∂ρ ∂z
                                      1 ∂
                              ∇· F =      (ρF ρ )+  ∂F z  ,        (A.12.7)
                                      ρ ∂ρ        ∂z
                                       2
                                                     2
                                      ∂ V   1 ∂V    ∂ V
                                2
                               ∇ V =      +       +     ,          (A.12.8)
                                      ∂ρ 2  ρ ∂ρ    ∂z 2
                           ∇· (V F)= V ∇· F + F ·  V,              (A.12.9)
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