Page 549 - Fiber Optic Communications Fund
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530                                                               Fiber Optic Communications


            Next we consider the photon net gain rate due to absorption and spontaneous/stimulated emission. In this
            analysis, we ignore the loss of photons due to scattering and other possible mechanisms. From Eqs. (3.74)
            and (3.81), we have
                                          dN
                                            ph
                                               = R stim  + R abs  + R spont
                                           dt
                                               = ℏBN (N − N )+ AN .                        (A.20)
                                                         2
                                                      ph
                                                                    2
                                                             1
                                                    3
            Let n  be the number of photons in the volume L ,
                 ph
                                                           3
                                                  n ph  = N L .                              (A.21)
                                                         ph
            Using Eqs. (A.21) and (A.19), Eq. (A.20) may be rewritten as
                                         dn
                                           ph
                                             = ℏBn (N − N )+ ℏBN .                       (A.22)
                                                        2
                                                                     2
                                                    ph
                                                            1
                                          dt
            Using  = dz∕dt and simplifying Eq. (A.22), we obtain
                                                 dn ph       ℏBdz
                                                           =       .                         (A.23)
                                            (N − N )n + N       
                                              2   1  ph   2
            Eq. (A.23) can be rewritten as
                                             dn
                                               ph     ℏB(N − N )dz
                                                           2
                                                                1
                                                   =               ,                         (A.24)
                                           n + n            
                                            ph   sp
            where
                                                         N 2
                                                  n =                                        (A.25)
                                                   sp
                                                       N − N
                                                        2   1
            is known as the spontaneous emission factor or population-inversion factor. For an amplifier, N > N and,
                                                                                              1
                                                                                         2
            therefore, n ≥ 1. Integrating Eq. (A.24) from 0 to L, we find
                      sp
                                       ln [n (L)+ n ]− ln [n (0)+ n ]= gL,                   (A.26)
                                                                 sp
                                                  sp
                                           ph
                                                          ph
                                                   ℏB(N − N )
                                                              1
                                                         2
                                                g =                                          (A.27)
                                                         
            or
                                      n (L)= n (0) exp(gL)+ n [exp (gL)− 1].                 (A.28)
                                       ph     ph            sp
            Since G = exp (gL), Eq. (A.28) can be written as
                                           n (L)= n (0)G + n (G − 1).                        (A.29)
                                                            sp
                                            ph
                                                   ph
            Eq. (A.29) is of fundamental significance. The first and second terms on the right hand side represent the
            photon gain due to stimulated emission and spontaneous emission, respectively.
              Next, let us consider the average noise power due to spontaneous emission. A photon of energy ℏ is
                                                                                                0
            assumed to occupy a length L or equivalently time L∕[1, 2]. The noise power of a photon is
                                                        ℏ 0
                                                   P  =     .                                (A.30)
                                                     0
                                                        L∕
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