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as desired.
                          To solve for   in V we shall make some seemingly unmotivated substitutions into this
                        identity. First note that by (3.52)and (3.53)we can write
                                                       2
                                                    ∇ G(r|r ) =−δ(r − r).                      (3.54)



                        We now set φ(r ) =  (r ) and ψ(r ) = G(r|r ) to obtain


                                                     2                2
                                            [ (r )∇ G(r|r ) − G(r|r )∇  (r )] dV =
                                           V
                                                      ∂G(r|r )       ∂ (r )




                                            −     (r )       − G(r|r )       dS ,              (3.55)
                                               S        ∂n             ∂n
                        hence




                                                  ρ(r )               ∂G(r|r )        ∂ (r )







                               (r )δ(r − r) − G(r|r )   dV =      (r )        − G(r|r )      dS .
                           V                        	          S        ∂n             ∂n
                        By the sifting property of the Dirac delta
                                              ρ(r )              ∂G(r|r )        ∂ (r )






                               (r) =    G(r|r )    dV +      (r )        − G(r|r )      dS +
                                      V        	         S B       ∂n             ∂n
                                        N
                                       
           ∂G(r|r )        ∂ (r )



                                     +         (r )        − G(r|r )      dS .                 (3.56)
                                                     ∂n             ∂n
                                       n=1  S n
                        With this we may compute the potential anywhere within V in terms of the charge
                        density within V and the values of the potential and its normal derivative over S.We
                        must simply determine G(r|r ) first.

                          Let us take a moment to specialize (3.56)to the case of unbounded space. Provided
                        that the sources are of finite extent, as S B →∞ we shall find that


                                                         N
                                             ρ(r )      
          ∂G(r|r )        ∂ (r )






                               (r) =   G(r|r )    dV +          (r )       − G(r|r )       dS .
                                               	                      ∂n             ∂n
                                      V                 n=1  S n
                        A useful derivative identity.  Many differential operations on the displacement vector
                        R = r − r occur in the study of electromagnetics. The identities

                                                                                  ˆ
                                                                                  R
                                                                          1
                                                               1
                                                     ˆ

                                        ∇ R =−∇ R = R,     ∇      =−∇         =−    ,          (3.57)
                                                               R          R       R 2
                        for example, follow from direct differentiation of the rectangular coordinate representa-
                        tion



                                              R = ˆ x(x − x ) + ˆ y(y − y ) + ˆ z(z − z ).
                        The identity

                                                        1
                                                     2
                                                   ∇       =−4πδ(r − r ),                      (3.58)
                                                        R
                        crucial to potential theory, is more difficult to establish. We shall prove the equivalent
                        version

                                                       2  1
                                                   ∇        =−4πδ(r − r)
                                                        R
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