Page 98 - Electromagnetics Handbook
P. 98

hence
                                                                           ∂D
                                           w em =−∇ · (E × H) + H · (∇× E) −   · E
                                                                            ∂t
                        by (B.44). Substituting for ∇× E from (2.1) we have


                                                                   ∂D       ∂B
                                            w em =−∇ · (E × H) − E ·   + H ·    .
                                                                    ∂t      ∂t
                        This is not quite of the form (2.285) since a single term representing the time rate of
                        change of energy density is not present. However, for a linear isotropic medium in which
                        
 and µ do not depend on time (i.e., a nondispersive medium) we have

                                            ∂D       ∂E    1 ∂          1 ∂
                                         E ·   = 
E ·    =  
  (E · E) =   (D · E),           (2.295)
                                            ∂t        ∂t   2 ∂t         2 ∂t
                                            ∂B        ∂H    1  ∂          1 ∂
                                         H ·   = µH ·    =   µ   (H · H) =   (H · B).         (2.296)
                                            ∂t        ∂t    2 ∂t          2 ∂t
                        Using this we obtain
                                                       ∂
                                              ∇· S em +  W em =−f em · v =−J · E              (2.297)
                                                       ∂t
                        where
                                                          1
                                                    W em =  (D · E + B · H)
                                                          2
                        and

                                                        S em = E × H.                         (2.298)

                        Equation (2.297) is the point form of the energy conservation theorem, also called Poynt-
                        ing’s theorem after J.H. Poynting who first proposed it. The quantity S em given in
                        (2.298) is known as the Poynting vector. Integrating (2.297) over a volume and using the
                        divergence theorem, we obtain the large-scale form

                                                      1 ∂

                                     −   J · E dV =      (D · E + B · H) dV +  (E × H) · dS.  (2.299)
                                        V           V 2 ∂t                  S
                        This also holds for a nondispersive, linear, bianisotropic medium with a symmetric con-
                        stitutive matrix [101, 185].
                          We see that the electromagnetic energy conservation theorem (2.297) is identical in
                        form to the mechanical energy conservation theorem (2.285). Thus, if the system is com-
                        posed of just the kinetic and electromagnetic subsystems, the mechanical force exactly
                        balances the Lorentz force, and (2.297) and (2.285) add to give

                                                             ∂
                                               ∇· (S em + S k ) +  (W em + W k ) = 0,         (2.300)
                                                             ∂t
                        showing that energy is conserved for the entire system.
                          As in the mechanical system, we identify W em as the volume electromagnetic energy
                        density in V , and S em as the density of electromagnetic energy flowing across the bound-
                        ary of V . This interpretation is somewhat controversial, as discussed below.




                        © 2001 by CRC Press LLC
   93   94   95   96   97   98   99   100   101   102   103