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leaves the expressions (5.17) and (5.18) unchanged. This is called a gauge transformation,
                        and the choice of a certain   alters the specification of ∇· A e . Thus we may begin with
                        the Coulomb gauge as our baseline, and allowany alteration of A e according to (5.20)
                                                               2
                        as long as we augment ∇· A e by ∇· ∇  =∇  .
                          Once ∇· A e is specified, the relationship between the potentials and the current J
                        can be found by substitution of (5.17) and (5.18) into Ampere’s law. At this point
                        we assume media that are linear, homogeneous, isotropic, and described by the time-
                                                                  i
                        invariant parameters µ,  , and σ. Writing J = J + σE we have
                                                                          2
                                     1                i    ∂A e          ∂ A e   ∂
                                       ∇× (∇× A e ) = J − σ    − σ∇φ e −      −    ∇φ e .      (5.22)
                                     µ                      ∂t            ∂t  2  ∂t
                        Taking the divergence of both sides of (5.22) we get
                                                ∂                   ∂ 2         ∂
                                           i
                                   0 =∇ · J − σ   ∇· A − σ∇· ∇φ e −    ∇· A e −    ∇· ∇φ e .   (5.23)
                                                ∂t                  ∂t 2        ∂t
                        Then, by substitution from the continuity equation and use of (5.19) along with ∇·∇φ e =
                         2
                        ∇ φ e we obtain
                                                   ∂    i   2  	       2
                                                     ρ +  ∇ φ e =−σ∇ φ e .
                                                  ∂t
                        For a lossless medium this reduces to
                                                          2
                                                                  i
                                                        ∇ φ e =−ρ /                            (5.24)
                        and we have
                                                                i
                                                              ρ (r , t)

                                                   φ e (r, t) =      dV .                      (5.25)
                                                             V 4π R
                          We can obtain an equation for A e by expanding the left-hand side of (5.22) to get
                                                                           2       ∂
                                                   i
                                           2
                              ∇ (∇· A e ) −∇ A e = µJ − σµ  ∂A e  − σµ∇φ e − µ   ∂ A e  − µ   ∇φ e ,  (5.26)
                                                         ∂t               ∂t  2    ∂t
                        hence
                                                2                                ∂
                                       2
                                                          i
                                      ∇ A e − µ   ∂ A e  =−µJ + σµ  ∂A e  + σµ∇φ e + µ   ∇φ e
                                                ∂t 2             ∂t              ∂t
                        under the Coulomb gauge. For lossless media this becomes
                                                         2
                                                2       ∂ A e     i     ∂
                                              ∇ A e − µ     =−µJ + µ      ∇φ e .               (5.27)
                                                        ∂t 2            ∂t
                          Observe that the left-hand side of (5.27) is solenoidal (since the Laplacian term came
                        from the curl-curl, and ∇· A e = 0), while the right-hand side contains a general vector
                             i
                        field J and a lamellar term. We might expect the ∇φ e term to cancel the lamellar
                                  i
                        portion of J , and this does happen [91]. By (5.12) and the continuity equation we can
                        write the lamellar component of the current as
                                                ∇ · J (r , t)   ∂      ρ (r , t)     ∂
                                                    i                   i
                                  i


                                 J (r, t) =−∇             dV =    ∇           dV =     ∇φ e .
                                  l
                                              V    4π R         ∂t   V  4π R         ∂t
                        Thus (5.27) becomes
                                                              2
                                                             ∂ A e
                                                                        i
                                                     2
                                                   ∇ A e − µ      =−µJ .                       (5.28)
                                                                        s
                                                             ∂t 2
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