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into Ampere’s and Faraday’s laws. It is most convenient to analyze the relationships
                        using superposition of the cases for which J m = 0 and J = 0.
                          With J m = 0 Faraday’s lawis
                                                                 ∂B
                                                        ∇× E =−     .                          (5.16)
                                                                  ∂t
                        Since ∇× E is solenoidal, B must be solenoidal and thus ∇φ B = 0. This implies
                        that φ B = 0, which is equivalent to the auxiliary Maxwell equation ∇· B = 0.Now,
                        substitution of (5.14) and (5.15) into (5.16) gives
                                                                    ∂
                                             ∇× [∇× A E +∇φ E ] =−    [∇× A B ] .
                                                                    ∂t
                        Using ∇× (∇φ E ) = 0 and combining the terms we get

                                                                 ∂A B
                                                  ∇× ∇× A E +         = 0,
                                                                  ∂t
                        hence

                                                               ∂A B
                                                    ∇× A E =−      +∇ξ.
                                                                ∂t
                        Substitution into (5.14) gives

                                                        ∂A B
                                                  E =−       + [∇φ E +∇ξ] .
                                                         ∂t
                        Combining the two gradient functions together, we see that we can write both E and B
                        in terms of two potentials:

                                                            ∂A e
                                                      E =−      −∇φ e ,                        (5.17)
                                                             ∂t
                                                      B =∇ × A e ,                             (5.18)
                        where the negative sign on the gradient term is introduced by convention.


                        Gauge transformations and the Coulomb gauge.     We pay a price for the simplicity
                        of using only two potentials to represent E and B. While ∇× A e is definitely solenoidal,
                        A e itself may not be: because of this (5.17) may not be a decomposition into solenoidal
                        and lamellar components. However, a corollary of the Helmholtz theorem states that a
                        vector field is uniquely specified only when both its curl and divergence are specified. Here
                        there is an ambiguity in the representation of E and B; we may remove this ambiguity
                        and define A e uniquely by requiring that

                                                         ∇· A e = 0.                           (5.19)
                        Then A e is solenoidal and the decomposition (5.17) is solenoidal–lamellar. This require-
                        ment on A e is called the Coulomb gauge.
                          The ambiguity implied by the non-uniqueness of ∇· A e can also be expressed by the
                        observation that a transformation of the type

                                                       A e → A e +∇ ,                          (5.20)
                                                                 ∂
                                                       φ e → φ e −  ,                          (5.21)
                                                                  ∂t



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