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76                                                                Fiber Optic Communications


            2.7.4   Dispersion Slope
            The dispersion parameter depends on the wavelength. For a single-channel low-bit-rate optical communica-
            tion system, the spectral width Δf (and therefore the wavelength spread |Δ|) is quite small and the dispersion
            parameter D() can be considered as a constant over a small Δ. However, for a high-bit-rate wide-band
            communication system, the dependence of D on the wavelength can not be ignored. For example, the spectral
            width of an optical non-return-to-zero (NRZ) signal at B = 160 Gb/s is roughly (see Chapter 4)

                                               Δf ≃ 2B = 320 GHz.                            (2.206)

            Since c = f,
                                                   Δ    Δf
                                                      =−    .                                (2.207)
                                                        f
            At the carrier wavelength  = 1550 nm, Δ =−2.56 nm. The change in dispersion over such a large wave-
                                  c
            length spread around 1550 nm can not be ignored. It is useful to define the dispersion slope as
                                                        dD
                                                    S =   .                                  (2.208)
                                                        d
            Using Eq. (2.204), the dispersion slope for a standard SMF can be calculated as
                                                     [      4  ]
                                                   S 0    3 0
                                               S =     1 +     .                             (2.209)
                                                    4       4

            If the dispersion parameter D and the dispersion slope S at the carrier wavelength  are known, the disper-
                                                         c
                                                                                c
                                    c
            sion parameter in the vicinity of the carrier wavelength can be obtained by the linear approximation [29]
                                              D()= D + S ( −  ).                       (2.210)
                                                     c   c     0
                                                                     2
            In Eq. (2.102), we have retained the Taylor expansion terms up to  Ω ∕2. Under this approximation,  or
                                                                                               2
                                                                   2
            D is constant over the spectral width of the signal. To include the impact of the dispersion slope, we need to
            include a higher-order term in the Taylor expansion of Eq. (2.102),
                                                                    3
                                                           2
                                        (Ω) =  +  Ω+  Ω ∕2 +  Ω ∕6,                (2.211)
                                                   1
                                                         2
                                                                 3
                                               0
            where
                                                  3 |
                                                             2
                                                 d  |    d |
                                             =    |    =    |    .                         (2.212)
                                             3
                                                   3
                                                              |
                                                d |      d |= 0
                                                    |= 0
            Substituting Eq. (2.211) in Eq. (2.98), we obtain
                                                        ∞
                                        [  (        )]
                                                          ̃
                              F(t, z)= exp −i  t −  z  ∫  B(Ω)H (Ω, z) exp (−iΩt) dΩ,    (2.213)
                                                  0
                                                                f
                                              0
                                                       −∞
            where the fiber transfer function is modified as
                                              [                2         3  ]
                                  H (Ω, z)= exp −z + i Ωz + i Ω z∕2 + i Ω z∕6 .      (2.214)
                                                      1
                                   f
                                                             2
                                                                      3
            The field envelope at the output is given by Eq. (2.113) as before,
                                                     ]
                                                                       ]
                                      s (t)=  −1  [ ̃ s (Ω) =  −1  [ H (Ω, z)̃s (Ω) .      (2.215)
                                                              f
                                       o
                                                                    i
                                                  o
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