Page 109 - High Power Laser Handbook
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78   G a s , C h e m i c a l , a n d F r e e - E l e c t r o n L a s e r s     High-Power Fr ee-Electr on Lasers     79


                      In fact, if the process is permitted to continue, the electrons can travel
                      up the other side of the well and take energy back from the wave. A
                      net transfer of energy from the electrons to the wave can only happen
                      if the electrons are moving slightly faster than the ponderomotive
                      wave.  In  this  case,  the  electrons  “surf”  the  wave  but  with  roles
                      reversed, as if the surfer were pushing the ocean wave rather than the
                      other way around. The speed of this wave is wavelength dependent.
                      The resonant wavelength (the one in which the electrons are traveling
                      at the same velocity) is given by

                                               l
                                                      2
                                           l =  s  w  1 (  +  K )           (4.1)
                                                g 2  2
                      where l  is the radiated wavelength; l  is the wiggler wavelength; and
                             s
                                                     w
                      K is the strength parameter of the wiggler field, given by K = 93.4B rms (T)
                      l (m), with B being the rms wiggler field (K is of order 1 and compen-

                       w
                      sates for the fact that the electron trajectories in the wiggler are not
                      exactly parallel to the axis). For example, if B rms = 0.2T and l  = 0.05 m,
                                                                       w
                      the resonant wavelength would be around 1.2 µm for an electron energy
                      of 100 MeV. The resonant wavelength turns out to be the one in which
                      the electrons slip backward exactly one optical wavelength for each
                      wiggler period. When this occurs, a net transfer of energy between the
                      electrons and the optical wave can occur, because the electrons’ direction
                      of transverse motion ends up always in the same direction as the trans-
                      verse field of the optical wave (qE·dl is always positive; see Fig. 4.2).
                         In practical terms, K is a measure of the strength on the wiggler
                      interaction and needs to be of order 1 to give reasonable gain.
                         It can be seen from a cursory examination of Eq. (4.1) that once
                      constructed with a fixed wavelength, the wiggler has a limited range
                      of control over the output wavelength either through the field strength
                      in K by means of a power supply (if the wiggler is electromagnetic) or
                      by  changing  the  gap  of  a  permanent  magnet  wiggler.  The  output
                      wavelength can also be controlled through the input electron beam
                      energy—hence,  the  statement  that  FELs  can  provide  lasing  at  any
                      wavelength. There are, however, practical and physics performance
                      limitations to the operating range, which will become clearer in the
                      discussions that follow.
                      4.2.3  Gain and Bandwidth
                      The small signal gain of an FEL is given by
                                                   2
                                      g = 31.8 (I/I )(N /g)Bη η η           (4.2)
                                                A
                                                         I f µ
                                                              2
                                                                      2
                                                     2
                      where I = 17 kA, B = 4ξ[J (ξ) – J (ξ)] , and ξ = K /[2(1 + K )]. The last
                                            0
                            A
                                                 1
                      three terms are degradations due to finite emittance, energy spread,
                      and optical electron beam overlap. Here I is the peak current, N is the
                      number of wiggler periods, and J is a Bessel function.
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