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446   Fi b er   L a s er s            Intr oduction to Optical Fiber Lasers    447


                         Ultraviolet photosensitivity in the germanium-doped core of an
                      optical  fiber  originates  from  germanium  oxygen-deficient  centers
                      with well-defined absorption of around 240 nm, accessible by KrF
                      excimer lasers, frequency-doubled argon ion lasers, or frequency-
                      quadrupled Nd:YAG lasers. In addition to the depletion of the ger-
                      manium oxygen-deficient centers upon UV exposure, there is also
                      evidence of stress relaxation and sometimes compaction. All these
                      effects are believed to contribute to the observed refractive index
                      change. It was eventually found that hydrogen loading in a high-
                      pressure cell near room temperature prior to UV exposure leads to
                      a significant improvement of photosensitivity.  This discovery has
                                                              57
                      enabled  FBG  writing  in  some  germanium-free  glasses.  Large
                      amounts of hydroxyls are found in the glass after UV exposure, and
                      the significant composition modification is believed, in this case, to
                      play  a  role  in  the  refractive  index  change.  FBGs  are  found  to  be
                      highly  stable  at  room  temperature,  though  they  can  be  erased  at
                      elevated temperatures.  Most FBGs will be erased at temperatures
                                          58
                      above 400°C, and FBGs with improved temperature stability can be
                      made using special writing processes. One unique aspect that makes
                      FBGs possible is that silica glass in the cladding is not photosensi-
                      tive,  which  allows  the  UV  beam  to  reach  the  core  glass  without
                      being absorbed.
                         In an FBG, due to momentum conservation, we have
                                             k =  k −  k                  (15.35)
                                              g  f   b

                      This leads to a relation between peak wavelength  λ  and grating
                                                                    0
                      pitch Λ.
                                             λ =  2n Λ                    (15.36)
                                              0    0
                      where n  is effective mode index. For a uniform grating, reflectivity
                             0
                      can be analytically determined:

                                              κ  2  h κ sin  2 (  L)
                                  R =                                     (15.37)
                                           2
                                                            2
                                      δ  2  h (  L +κ sin  2  − κ )(  δ  2 )cos h κ (  L)
                      where L is grating length. The coupling coefficient is defined as

                                                π ∆n
                                            κ=     g  η                   (15.38)
                                                     g
                                                 λ 0
                      where η  is the spatial modal overlap with the grating. It is also the
                             g
                      proportion of modal power in the core if the FBG is written uniformly
                      over the core; 2∆n  is the peak-to-peak refractive index modulation.
                                     g
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