Page 131 - Fiber Optic Communications Fund
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112                                                               Fiber Optic Communications


            Since u ∝ N , the time rate of change of photon density is
                      ph
                                               dN ph         N ph
                                                    = GN −      ,                             (3.78)
                                                        ph
                                                dt           
                                                              ph
            where
                                                         1
                                                     =                                      (3.79)
                                                    ph
                                                        
                                                          cav
            is the photon lifetime. In the absence of gain (G = 0), Eq. (3.78) can be solved to yield
                                            N (t)= N (0) exp (−t∕ ).                        (3.80)
                                             ph
                                                    ph
                                                                ph
                                  −1
            At t = t , N (t)= N (0)e . Thus, the photon density reduces by e over a time t . In Eq. (3.78), G repre-
                   ph  ph     ph                                              ph
            sents the net gain coefficient due to stimulated emission and absorption and, therefore, the first term on the
            right-hand side of Eq. (3.78) can be identified as
                                               R stim  + R abs  = GN ,                        (3.81)
                                                              ph
            or
                                              BuN − BuN = GN .                                (3.82)
                                                               ph
                                                  2
                                                         1
            Since u = N ℏ, from Eq. (3.82) we find
                      ph
                                               G = B(N − N )ℏ.                              (3.83)
                                                       2   1
              In Eq. (3.78), the second term represents the loss, rate due to scattering, mirror loss, and other possible loss
            mechanisms,
                                                         N ph
                                                  R   =−     .                                (3.84)
                                                   loss
                                                          
                                                           ph
            Eq. (3.78) does not include the photon gain rate due to spontaneous emission. Using Eqs. (3.81), (3.84), and
            (3.4) in Eq. (3.74), we find
                                            dN                 N
                                               ph                ph
                                                 = GN + AN −      .                           (3.85)
                                                      ph
                                                            2
                                             dt                  ph
            Note that when N > N , population inversion is achieved, G > 0 (see Eq. (3.83)) and amplification of photons
                          2
                               1
            takes place. In other words, the energy of the atomic system is transferred to the electromagnetic wave. When
            N < N , the electromagnetic wave is attenuated and the energy of the wave is transferred to the atomic system.
                  1
              2
              Using Eq. (3.82), Eqs. (3.72) and (3.73) can be rewritten as
                                            dN 2                N 2
                                                = R pump  − GN −  ,                           (3.86)
                                                            ph
                                             dt                  21
                                                dN           N
                                                  1  = GN +   2  ,                            (3.87)
                                                dt      ph  
                                                             21
            where
                                                         1
                                                   21  =                                    (3.88)
                                                        A + C
            is the lifetime associated with spontaneous emission and non-radiative decay from the excited state to the
            ground state. Eqs. (3.86) and (3.87) can be simplified further under the assumption that the population density
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