Page 274 - Electromagnetics
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By (4.228) we know that α is even in ω and β is odd in ω. Since the derivative of an

                        odd function is an even function, we also know that β is even in ω. We can therefore
                        write (4.235) as
                                                    1     ∞  1         − jβ(ω 0 ) ˆ k·r − jβ (ω 0 )(ω−ω 0 ) ˆ k·r
                                             −α(ω 0 ) ˆ k·r
                                                             ˜

                               ˆ eE(r, t) = ˆ eE 0 e         F(ω − ω 0 )e     e            +
                                                   2π  −∞ 2

                                         ˜

                                                         e
                                      + F(ω + ω 0 )e jβ(ω 0 ) ˆ k·r − jβ (ω 0 )(ω+ω 0 ) ˆ k·r  e  jωt  dω.
                        Multiplying and dividing by e  jω 0 t  and rearranging, we have
                                                        1     ∞  1
                                                                  ˜
                                                                           jφ j(ω−ω 0 )[t−τ]
                                    ˆ eE(r, t) = ˆ eE 0 e −α(ω 0 ) ˆ k·r  F(ω − ω 0 )e e  +
                                                        2π  −∞ 2
                                              ˜
                                                          e
                                           + F(ω + ω 0 )e − jφ j(ω+ω 0 )[t−τ]     dω
                        where
                                                                            ˆ
                                                           ˆ
                                            φ = ω 0 t − β(ω 0 )k · r,  τ = β (ω 0 )k · r.

                        Setting u = ω − ω 0 in the first term and u = ω + ω 0 in the second term we have
                                                                 1     ∞    ju(t−τ)
                                                                        ˜
                                                     −α(ω 0 ) ˆ k·r
                                        ˆ eE(r, t) = ˆ eE 0 e  cos φ   F(u)e      du.
                                                                2π
                                                                    −∞
                        Finally, the time-shifting theorem (A.3) gives us the time-domain wave field
                                                            ˆ
                                                                              ˆ



                              ˆ eE(r, t) = ˆ eE 0 e −α(ω 0 ) ˆ k·r  cos ω 0 t − k · r/v p (ω 0 )     f t − k · r/v g (ω 0 )    (4.236)
                        where
                                                  v g (ω) = dω/dβ = [dβ/dω] −1                (4.237)
                        is called the group velocity and
                                                         v p (ω) = ω/β
                        is called the phase velocity.
                          To interpret (4.236), we note that at any given time t the field is constant over the
                        surface described by
                                                           ˆ
                                                          k · r = C                           (4.238)
                        where  C  is some constant. This surface isa plane, as shown in Figure 4.10, with its
                                    ˆ
                        normal along k. It is easy to verify that any point r on this plane satisfies (4.238). Let
                                                                                               ˆ
                              ˆ
                        r 0 = r 0 k describe the point on the plane with position vector in the direction of k, and
                        let d be a displacement vector from this point to any other point on the plane. Then
                                                                          ˆ
                                                                   ˆ ˆ
                                               ˆ
                                                     ˆ
                                              k · r = k · (r 0 + d) = r 0 (k · k) + k · d.
                            ˆ
                        But k · d = 0,so
                                                          ˆ
                                                          k · r = r 0 ,                       (4.239)
                        which is a fixed distance, so (238) holds.
                          Let us identify the plane over which the envelope f takes on a certain value, and follow
                        its motion as time progresses. The value of r 0 associated with this plane must increase
                        with increasing time in such a way that the argument of f remains constant:
                                                      t − r 0 /v g (ω 0 ) = C.


                        © 2001 by CRC Press LLC
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