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ˇ
                                                                     ˇ
                                                       ˇ
                                                           ˇ
                        This implies a relationship between E 0 , D 0 , B 0 , and H 0 . Since V is arbitrary we see that
                                                                                          ˇ
                                                                                       ˇ
                                                                            ˇ
                                                                               ˇ
                        one possible relationship is simply to have one of each pair (E 0 , D 0 ) and (H 0 , B 0 ) equal to
                                                                                ˇ
                                                                     ˇ
                                                        ˇ
                                                                                              ˇ
                        zero. Then, by (4.163) and (4.164), E 0 = 0 implies B 0 = 0, and D 0 = 0 implies H 0 = 0.
                             ˇ
                                   ˇ
                        Thus E 1 = E 2 , etc., and the solution is unique throughout V . However, we cannot in
                        general rule out more complicated relationships. The number of possibilities depends on
                                                                        ˇ
                                                                                      ˇ
                                                                               ˇ
                                                                           ˇ
                        the additional constraints on the relationship between E 0 , D 0 , B 0 , and H 0 that we must
                        supply to describe the material supporting the field — i.e., the constitutive relationships.
                                                                c
                        For a simple medium described by ˜µ(ω) and ˜  (ω), equation (4.166) becomes

                                          ˇ
                                                              ˇ
                                            2  c                 2
                                                      c∗
                                                                          ∗
                                         |E 0 | [˜  ( ˇω) − ˜  ( ˇω)] +|H 0 | [ ˜µ( ˇω) − ˜µ ( ˇω)] dV = 0
                                       V
                        or

                                                              ˇ
                                                  ˇ
                                                                2
                                                    2 c

                                                 |E 0 | ˜  ( ˇω) +|H 0 | ˜µ ( ˇω) dV = 0.
                                               V

                        For a lossy medium, ˜  c    < 0 and ˜µ < 0 as shown in § 4.5.1. So both terms in the
                        integral must be negative. For the integral to be zero each term must vanish, requiring
                        ˇ
                             ˇ
                        E 0 = H 0 = 0, and uniqueness is guaranteed.
                          When establishing more complicated constitutive relations we must be careful to ensure
                        that they lead to a unique solution, and that the condition for uniqueness is understood.

                                                             = 0 implies that the tangential components of
                        In the case above, the assumption ˆ n×E 0
                                                         ˇ
                                                           S
                               ˇ
                        ˇ
                        E 1 and E 2 are identical over S — that is, we must give specific values of these quantities

                                                                                              = 0.
                        on S to ensure uniqueness. A similar statement holds for the condition ˆ n × H 0
                                                                                          ˇ
                                                                                             S
                          In summary, the conditions for the fields within a region V containing lossy isotropic
                        materials to be unique are as follows:
                          1. the sources within V must be specified;
                          2. the tangential component of the electric field must be specified over all or part of
                            the bounding surface S;
                          3. the tangential component of the magnetic field must be specified over the remainder
                            of S.
                        We may question the requirement of a lossy medium to demonstrate uniqueness of the
                        phasor fields. Does this mean that within a vacuum the specification of tangential fields
                        is insufficient? Experience shows that the fields in such a region are indeed properly
                        described by the surface fields, and it is just a case of the mathematical model being
                        slightly out of sync with the physics. As long as we recognize that the sinusoidal steady
                        state requires an initial transient period, we know that specification of the tangential
                        fields is sufficient. We must be careful, however, to understand the restrictions of the
                        mathematical model. Any attempt to describe the fields within a lossless cavity, for
                        instance, is fraught with difficulty if true time-harmonic fields are used to model the
                        actual physical fields. A helpful mathematical strategy is to think of free space as the
                        limit of a lossy medium as the loss recedes to zero. Of course this does not represent
                        the physical state of “empty” space. Although even interstellar space may have a few
                        particles for every cubic meter to interact with the electromagnetic field, the density of
                        these particles invalidates our initial macroscopic assumptions.
                          Another important concern is whether we can extend the uniqueness argument to all
                        of space. If we let S recede to infinity, must we continue to specify the fields over S,or
                        is it sufficient to merely specify the sources within S? Since the boundary fields provide
                        information to the internal region about sources that exist outside S, it is sensible to
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