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Appendix B                                                                         535


           where n is the linear refractive index of the fiber. For a single-mode fiber we have
                                                    2 2
                                             2
                                        2
                                              n (r,)  2
                                          +     +           =  (),                  (B.17)
                                       x 2  y 2   c 2
           where () is the propagation constant. Substituting Eqs. (B.16) and (B.17) in Eq. (B.13), we obtain
                                                 2
                    ̃q(z, Ω)  2     2       3  (3)  3          ∗
                2i       +[ ()−  ]̃q =−  { (x, y)[̃q(z, Ω) ⊗̃q (z, −Ω) ⊗̃q(z, Ω)]}.  (B.18)
                   0                  0           2
                      z                       4c
           To remove the dependence of transverse field distributions, we multiply Eq. (B.18) by (x, y) and integrate
           from −∞ to ∞ in the x–y plane to obtain
                                         2
                                  2
                                                   2
                           ̃q  [ ()−  ]̃q  3  (3)    ∗
                                         0
                           i  +             =−         [̃q(z, Ω) ⊗̃q (z, −Ω) ⊗̃q(z, Ω)],    (B.19)
                            z     2 0       8c A 
                                                  2
                                                    eff 0
           where                                 ∞   ∞
                                                ∫  ∫    (x, y)dxdy
                                                        2
                                          A  =  −∞ −∞            .                          (B.20)
                                           eff   ∞   ∞
                                                ∫  ∫    (x, y)dxdy
                                                        4
                                                −∞ −∞
           The second term on the left-hand side of Eq. (B.19) can be approximated as
                                2
                                       2
                              [ ()−  ]̃q  [()+  ][()−  ]̃q
                                       0            0        0
                                          =                      ≅[()−  ]̃q.          (B.21)
                                                                          0
                                   2               2
                                     0                 0
           The above approximation is valid if the difference between () and  is quite small. If the spectral width
                                                                   0
           of the optical signal is comparable with or larger than  , the above approximation could be incorrect. When
                                                       0
           the spectral width Δ≪ , we can approximate () as a Taylor series around  and retain the first three
                                0                                            0
           terms,
                                                      2     2    3     3
                               ()=  +  ( −  )+  ( −  ) +  ( −  ) ,      (B.22)
                                       0   1     0           0           0
                                                     2            6
           where                                     n
                                                    d  |
                                                =     |                                   (B.23)
                                                n      n |
                                                    d |= 0
           is known as the nth-order dispersion coefficient (see Chapter 2). Substituting Eqs. (B.21) and (B.22) in
           Eq. (B.19), we obtain
                      (                  )              2  (3)
                  ̃q        2  2   3  3   3( +Ω)            ∗
                                                   0
                 i  +  Ω+    Ω +    Ω    ̃ q =−           [̃q(z, Ω) ⊗̃q (z, −Ω) ⊗̃q(z, Ω)].  (B.24)
                         1
                                                    2
                  z         2      6            8c A 
                                                      eff 0
            If we include the fiber losses by treating the refractive index n as complex with its imaginary part being
           frequency independent, Eq. (B.24) is modified as
                   (                  )                   2  (3)
               ̃q         2  2   3  3  ̃q  3( +Ω)           ∗
                                                     0
              i   +  Ω+    Ω +    Ω   ̃ q =−i  −             [̃q(z, Ω) ⊗̃q (z, −Ω) ⊗̃q(z, Ω)],  (B.25)
                      1
                                                       2
               z         2      6           2      8c A 
                                                         eff 0
           where  is the fiber loss coefficient related to the imaginary part of the refractive index through Eq. (10.37). We
                                                                      2
                                                                          2
           have assumed  to be independent of frequency. Since Ω ≪ , ( +Ω) ≃  + 2 Ω. Now, performing
                                                             0  0         0     0
           the inverse Fourier transform, we obtain
                           (          )     2                3           2
                             q   q      q      2   i  q  i2 (|q| q)  i
                                                           3
                          i     +  1  −  2  + i|q| q =   −            +   q,          (B.26)
                             z    t     t 2         6 t 3   0  t  2
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