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244   So l i d - S t at e   La s e r s                     Thin-Disc Lasers    245


                             lϑ
                      and HR(, ) (highly reflective). The AR face is on the top and the HR
                      face is at the bottom.
                         The AR face is typically the interface between the crystalline laser
                      medium and air (or vacuum); it is antireflective for normal incidence
                      at the laser and pump wavelengths. Thus it is reasonable to assume
                      that the AR face is nonreflective for angles smaller than the critical
                      angle of total reflection  ϑ = arcsin (1/ n), with n the index of refraction
                                           tr
                      of the active medium, and that it is ideally reflecting for larger angles.
                      In addition, we can assume  HR(, )lϑ ≠ 0  for all ϑ due to technical
                      limitations of the coating design.
                         In spherical coordinates, Eq. (10.22) transforms to:

                                                  s
                                               b   max
                                (,
                                                                   ϑ
                            dΦ fϑ)sin    ϑϑf    l  ∫  N s fϑ(, ,) g s f(, ,, )ds    (10.23)
                                          d d
                                    =
                                                              l
                                                πτ
                               l
                                                       2
                                               4
                                                   0
                         Taking into account the multiple reflections at the faces of the cyl-
                      inder,  s   can be expressed by:
                            max
                                            R −  2  sin f  2  −ρ  ρ  cos f
                                      s max  =    sin ϑ                   (10.24)
                           lϑ
                      if  AR(, ) HR( ,) ≠ 0 .
                                   lϑ
                         To account for losses at the AR and HR faces, the gain coefficient
                      can be modified to:
                                                lϑ
                                                        lϑ))
                                  γ  lϑ  =  γ  l  +  ln(AR ( ,)HR (,  cos ϑ     (10.25)
                                    ,
                                                  2
                                                   h
                      if  AR(, )lϑ  HR( ,) ≠ 0 .
                                   lϑ
                      10.5.11  Time Resolved Numerical Model
                      Based on these considerations, it is possible to develop a numerical
                      model  of  the  interaction  of  amplified  spontaneous  emission  and
                                                                              34
                      excitation, a more detailed description can be found in literature .
                      For this, we discretize the problem in ρ, ϑ, f , and  l . Neglecting the
                      variation of excitation and gain in axial direction and assuming rota-
                                                                  %
                      tional  symmetry,  only  the  radial  variation  of  Nr ()  and  % γ ()r
                                                                            l
                                                                   2
                      remains.
                         The temporal development of the excitation can easily be calcu-
                      lated by integrating the differential Eq. (10.19) with implicit methods.
                      For each time step, the source Q and the photon flux densities dΦ (ˆ s)
                                                                             l
                      are calculated based on the distribution of excitation from the previous
                      time step. Because the typical time constant of the excitation is in the
                      order of the spontaneous lifetime (several hundreds of microseconds),
                      this is adequate for time steps of a few microseconds.
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