Page 436 - Electromagnetics
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We now state Love’s equivalence principle [39]. Consider the fields within a homoge-
                                                                 c
                        neous, source-free region V with parameters (˜  , ˜µ) bounded by a surface S. We know
                        how to compute the fields using the Franz formula and the surface fields. Now consider
                        a second problem in which the same surface S exists in an unbounded medium with
                        identical parameters. If the surface carries the equivalent sources (6.41) then the electro-
                        magnetic fields within V calculated using the Hertzian potentials (6.39) and (6.40) are
                        identical to those of the first problem, while the fields calculated outside V are zero. We
                        see that this must be true since the Franz formulas and the field/potential formulas are
                        identical, and the Franz formula (since it was derived from the Stratton–Chu formula)
                        gives the null field outside V . The two problems are equivalent in the sense that they
                        produce identical fields within V .
                          The fields produced by the equivalent sources obey the appropriate boundary condi-
                        tions across S. From (2.194) and (2.195) we have the boundary conditions
                                                                   ˜
                                                              ˜
                                                         ˜
                                                    ˆ n × (H 1 − H 2 ) = J s ,
                                                                     ˜
                                                              ˜
                                                         ˜
                                                     ˆ n × (E 1 − E 2 ) =−J ms .
                                                     ˜
                                                                                      ˜
                                                                                  ˜
                                                  ˜
                        Here ˆ n points inward to V , (E 1 , H 1 ) are the fields within V , and (E 2 , H 2 ) are the fields
                        within the excluded region. If the fields produced by the equivalent sources within the
                        excluded region are zero, then the fields must obey
                                                           ˜
                                                                ˜ eq
                                                       ˆ n × H 1 = J ,
                                                                 s
                                                                  ˜ eq
                                                           ˜
                                                        ˆ n × E 1 =−J ,
                                                                  ms
                                                          eq
                                                       eq
                                                         ˜
                                                      ˜
                        which is true by the definition of (J s , J sm ).
                          Note that we can extend the equivalence principle to the case where the media are
                        different internal to V than external to V . See Chen [29].
                          With the equivalent sources identified we may compute the electromagnetic field in
                        V using standard techniques. Specifically, we may use the Hertzian potentials as shown
                        above or, since the Hertzian potentials are a simple remapping of the vector potentials,
                        we may use (5.60) and (5.61) to write
                                                                        1
                                            ˜
                                                                 2 ˜
                                                           ˜
                                                                              ˜

                                                   ω
                                           E =− j     ∇(∇· A e ) + k A e −  ∇× A h ,
                                                  k 2                   ˜   c
                                                                        1
                                            ˜
                                                           ˜
                                                                              ˜
                                                                 2 ˜

                                                   ω
                                           H =− j     ∇(∇· A h ) + k A h +  ∇× A e ,
                                                  k 2                   ˜ µ
                        where

                                         ˜               ˜ eq
                                        A e (r,ω) =  ˜ µ(ω)J (r ,ω)G(r|r ; ω) dS               (6.42)
                                                         s
                                                   S

                                                             ˜




                                                =   ˜ µ(ω)[ˆ n × H(r ,ω)]G(r|r ; ω) dS ,       (6.43)
                                                   S

                                        ˜            c   ˜ eq
                                        A h (r,ω) =  ˜   (ω)J (r ,ω)G(r|r ; ω) dS              (6.44)
                                                          ms
                                                   S

                                                               ˜
                                                     c




                                                =   ˜   (ω)[−ˆ n × E(r ,ω)]G(r|r ; ω) dS .     (6.45)
                                                   S
                        At points where the source is zero we can write the fields in the alternative form
                                                      ω              1
                                                                           ˜
                                               ˜
                                                                ˜
                                               E =− j   ∇× ∇× A e −   ∇× A h ,                 (6.46)
                                                      k 2            ˜   c
                                                      ω              1
                                                                ˜
                                               ˜
                                                                           ˜
                                              H =− j    ∇× ∇× A h +   ∇× A.                    (6.47)
                                                      k 2            ˜ µ
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