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4.5.2   Energy stored in a dispersive material
                          In the previous section we were able to isolate the dissipative effects for a dispersive
                        material under special circumstances. It is not generally possible, however, to isolate
                        a term describing the stored energy. The Kronig–Kramers relations imply that if the
                        constitutive parameters of a material are frequency-dependent, they must have both real
                        and imaginary parts; such a material, if isotropic, must be lossy. So dispersive materials
                        are generally lossy and must have both dissipative and energy-storage characteristics.
                        However, many materials have frequency ranges called transparency ranges over which


                        ˜    c    and ˜µ are small compared to ˜  and ˜µ . If we restrict our interest to these ranges,
                                                       c
                        we may approximate the material as lossless and compute a stored energy. An important
                        special case involves a monochromatic field oscillating at a frequency within this range.
                          To study the energy stored by a monochromatic field in a dispersive material we
                        must consider the transient period during which energy accumulates in the fields. The
                        assumption of a purely sinusoidal field variation would not include the effects described
                        by the temporal constitutive relations (2.29)–(2.31), which show that as the field builds
                        the energy must be added with a time lag. Instead we shall assume fields with the
                        temporal variation
                                                         3
                                                        
                   E
                                            E(r, t) = f (t)  ˆ i i |E i (r)| cos[ω 0 t + ξ (r)]  (4.51)
                                                                            i
                                                        i=1
                        where f (t) is an appropriate function describing the build-up of the sinusoidal field. To
                        compute the stored energy of a sinusoidal wave we must parameterize f (t) so that we
                        may drive it to unity as a limiting case of the parameter. A simple choice is

                                                                       π   ω 2
                                                        2 2
                                                      −α t
                                                              ˜
                                               f (t) = e   ↔ F(ω) =      e − 4α 2  .           (4.52)
                                                                      α 2
                        Note that since f (t) approaches unity as α → 0, we have the generalized Fourier trans-
                        form relation
                                                          ˜
                                                      lim F(ω) = 2πδ(ω).                       (4.53)
                                                      α→0
                          Substituting (4.51) into the Fourier transform formula (4.1) we find that
                                          3
                                                                      3
                                       1  
          E             1  
           E
                              ˜             ˆ       jξ (r) ˜            ˆ      − jξ (r) ˜
                              E(r,ω) =      i i |E i (r)|e  i  F(ω − ω 0 ) +  i i |E i (r)|e  i  F(ω + ω 0 ).
                                       2                           2
                                         i=1                         i=1
                        We can simplify this by defining
                                                           3
                                                                      E
                                                    ˇ     
  ˆ       jξ (r)
                                                   E(r) =    i i |E i (r)|e  i                 (4.54)
                                                          i=1
                        as the phasor vector field to obtain
                                          ˜       1    ˇ  ˜         ˇ ∗  ˜
                                         E(r,ω) =    E(r)F(ω − ω 0 ) + E (r)F(ω + ω 0 ) .      (4.55)
                                                  2
                        We shall discuss the phasor concept in detail in § 4.7.
                                                                                    ˜
                          The field  E(r, t) is shown in Figure 4.2 as a function of t, while  E(r, ω) is shown in
                        Figure 4.2 as a function of ω. As α becomes small the spectrum of E(r, t) concentrates
                        around ω =±ω 0 . We assume the material is transparent for all values α of interest so




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