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136                                                                Chapter 3

        3.2   UNIQUENESS THEOREM FOR INTERIOR
        ELECTROMAGNETICS PROBLEMS


        3.2.1   Necessary of Uniqueness Theorem

        Ultimately, Maxwell’s equations describe  in  the  sense of  macroscopic electrodynamics all
        possible varieties of electromagnetic fields that can be generated by the probably enormous
        diversity of  sources  surrounded by  an  infinite  mixture of  physical  objects with multiple
        combinations  of dielectric and  magnetic parameters.  If  so, how from this  endless  maze of
        solutions we could choose one and only one solution to our actual problem. Poynting’s theorem
        and following from it the Uniqueness Theorem dictates how any real EM problem should be
        adequately  conveyed  to  provide one and only one solution.  Apparently, such  additional
        conditions should state as long as we care to get the experimentally verified solutions. There
        are two slightly different formulations of uniqueness theorem, one for solutions in the time
        domain, and another one in the frequency domain. To begin with, we will draw up each of them
        for the finite and  time-invariant  volume     enclosed by the regular surface     (interior
                                            1
                                                                           1
        electromagnetics problems). Then we will study the case of the asymptotic limits for the fields
        at infinity or simply A at “infinity” (radiation problems).
        3.2.2   Uniqueness Theorem in Space-Time Domain

        Maxwell’s equations have a unique solution { (, ),  (, )} at each point of   and at any
                                                      
                                              
                                                                          1
        moment of time t > 0 if
        1.  The field sources and their distributions are given at each point of   and at any moment
                                                                   1
            of time  ≥ 0,
        2.  The following initial conditions at  = 0 { ( = 0, ),  ( = 0, )} are given at each
                                                
                                                           
            point of   and there are no fields at any moment of time  < 0. In other words, the field
                    1
            configuration in the future (t > 0) can be predicted as long as the volume V is isolated and
            does not receive any energy from outside before the moment of time  = 0,
        3.  The  following  mixed  boundary conditions  are  fulfilled  at each point of    and at any
                                                                         1
                                                                              ′
            moment of time  ≥ 0: the projection  (, )|  ′  tangential to the some part   of  
                                              ∈ 1             1    1
                                                                      ′′
            is given and the projection  (, )|  ′′ tangential to the rest part   of    is given
                                    
                                           ∈ 1                1     1
            while  =  ∪  . Note that these boundary conditions can be rewritten in the vector
                       ′
                           ′′
                       1
                           1
                  1
            form as
                                                               ′
                                                       ′
                                                           ′
                                (, )|  ′ =  (, ) x  ,     ∈ 
                                    ∈ 1    1  �                (3.54)
                                                       ′′
                                                            ′′
                                (, )| ∈ 1 ′′ =  (, ) x  ,     ∈  ′′
                                                                1
                                               
                                
        Here n is the outward normal to surface  . These boundary conditions includes two specific
                                          1
        and more simple variants when  = 0 and  = 0 meaning that the electrical or magnetic
                                    ′′
                                              ′
                                    1
                                              1
        tangential component is given, respectively, on the whole surface  .
                                                              1
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