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276                                                               Fiber Optic Communications


            If a light wave of energy E crosses the area A over the time interval Δt, the optical intensity is
                                  p
                                                        E p
                                                    =     .                                 (6.163)
                                                    p
                                                        AΔt
            Since the energy E = n ℏ , where  is the frequency of the pump wave, we find
                           p    p  p        p
                                                          p
                                                    =    .                                 (6.164)
                                                    p
                                                        ℏ p
            Using Eqs. (6.161) and (6.164) in Eq. (6.160), we find

                                                 R abs  =  N  ,                          (6.165)
                                                        13 1 p
            where
                                                       ℏ B
                                                         p 13
                                                   13  =                                   (6.166)
                                                          
            is known as the absorption cross-section associated with the transition from level 1 to level 3. The physical
            meaning of   is as follows. The optical power absorbed by an erbium ion is proportional to the optical
                       13
            intensity  of the light wave incident,
                     p
                                                   P   = k ,                                (6.167)
                                                    abs    p
            where k is a constant of proportionality that depends on the medium. Since P abs ∕ℏ is the number of photons
                                                                              p
            absorbed per unit time by an erbium ion (photon absorption rate) and  ∕ℏ is the photon flux density
                                                                        p
                                                                            p
            (Eq. (6.164)), dividing Eq. (6.167) by ℏ , we find
                                             p
                                                   P
                                                    abs
                                                       = k .                               (6.168)
                                                           p
                                                   ℏ p
            If there are N erbium ions per unit volume in the ground state, the total absorption rate is
                       1
                                                  R abs  = kN  ,                           (6.169)
                                                          1 p
            which is the same as Eq. (6.165) if k =  . Thus, the absorption cross-section can be imagined as an effective
                                            13
            area that “captures” a fraction of the incident photons [1]. Similarly, the stimulated emission rate from level
            3tolevel 1isgiven by
                                                R   =− N  ,                              (6.170)
                                                 stim    31 3 p
            where  = B ℏ ∕ is the cross-section associated with the transition from j to k and  is the energy
                   jk
                        jk
                            jk
                                                                                      jk
            difference between the levels j and k. Since the transition from level 3 to level 2 is mostly non-radiative,
            absorption and stimulated emission between level 3 and level 2 can be ignored. Using Eqs. (6.165) and (6.170)
            in Eq. (6.159), we find
                                          dN 3                    N 3
                                              =( N −  N ) −   .                        (6.171)
                                                         31 3
                                                               p
                                                  13 1
                                           dt                      32
            In the case of the two-level atomic system discussed in Chapter 3, Section 3.2, we found that B 12  = B , which
                                                                                           21
            implies that the emission and absorption cross-section are equal. However, in general, they could be different
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