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POYNTING's THEOREM                                                      117

            Table 1.5 can help to check that every term in (3.7) has the same unit dimension W m . The
                                                                                  3
                                                                                ⁄
            assumption that the dielectric and  magnetic constants are time-independent  is not  entirely
            correct because of the polarization and magnetization effects in materials discussed in Chapter
            2. However, all such transient effects usually require some attention but short living and thus
            can be neglected in most cases.

            The integral form of energy conservation law in the space-time domain. Eventually, the total
            power balance can be calculated by integrating both sides in (3.7) over the stationary volume
            V bounded by a closed surface A

                                 2
                                                         ⁄
            − ∫    ∘  = ∫   +    ∫ ( ∘  +  ∘ ) 2  + ∫  ∘ ( x ) [W] (3.8)
                                     
            Applying the divergent theorem (A.60) from Appendix to the last integral on the right-hand
            side, we get


                                      2
                − ∫    ∘  = ∫   +    ∫ ( ∘  +  ∘ ) 2  + ∯  x  ∘     (3.9)
                                                              ⁄
                                           
            The equity (3.9) expressing electromagnetic energy conservation law was introduced in 1884
            by  English physicist  John Henry  Poynting and  is  known as  the  integral  form  of  Poynting’s
            theorem. If so, the expression (3.7) can be treated as the differential form of Poynting’s theorem
            or the continuity equation for power density.


            Another probably more explicit physically and not so formal way to Poynting’s theorem is to
            define the energy  of  EM  fields  straight from  Lorentz’s  force  equation  instead  of  formal
            manipulation  of  (3.2).  Indeed,  we  know  that  the  tiny  portion  of  mechanical work  or  energy
            d   required to move a charge particle Δ  at the distance  in E- and H-fields is equal (see
                                       
            (1.11)) to d   =      ∘  and  = , where  is the time of movement. Then d    =
            Δ ( +  x ) ∘  = (Δ) ∘  =      ∘ .  The  2 nd  M ax well’s e quat ion  says
              
            that  x  − ⁄ =  . Therefore,   ⁄ = ( x  − ⁄) ∘ . The vector identity
                               
                                                     st
             ∘ ( x ) = ( x ) ∘  − ( x ) ∘  and the 1  Maxwell’s equation directly leads to (3.7)
            giving us the identical balance of power.
            Each term in (3.9) needs some explanation to get its physical meaning.

            3.1.2  Power Delivered by Excitation Currents

            From the discussion in Section 1.7 of Chapter 1, we know that the integral on the left-hand side of
            (3.9) describes the power given to the electromagnetic field by sources


                                         () = − ∫    ∘   [W]       (3.10)
                                                    
                                                 
                            
            Here the product     ∘  < 0 and    > 0 due to the fact that the current charges donating
            their energy to the fields slow down as they move against the electric force.
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