Page 165 - Intro to Tensor Calculus
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               which is obtained from equation (1.5.141). Substituting equations (1.5.174) and (1.5.175) into equation
               (1.5.184), rearranging terms and taking the limit we find that

                                                          c 4 c 2
                                                               = h.                                  (1.5.185)
                                                           c 5
               From equations (1.5.183) and (1.5.185) we obtain the results that

                                          c 2         2GM       1                  h
                                     2
                                    c =       ,  c 2 =                ,  c 4 = p                     (1.5.186)
                                     5
                                        1+  E          c 2  1+ E/c 2          c  1+ E/c 2
                                            c 2
               These values substituted into equation (1.5.181) produce the differential equation
                                             2
                                        du       2  2GM      E    2GM        1      3
                                              + u −      u +    =                  u .               (1.5.187)
                                        dφ            h 2    h 2    c 2  1+ E/c 2
                                                    1
               Let α =  c 2 2 =  2GM  and β = c 2 =  2GM  1+E/c 2 ) then the differential equation (1.5.178) can be written as
                                              c 2 (
                       c 4   h 2
                                                      2
                                                     d u      α    3  2
                                                         + u −  =   βu .                             (1.5.188)
                                                     dφ 2      2   2
               We know the solution to equation (1.5.143) is given by

                                                      1
                                                 u =   = A(1 +   cos(φ − φ 0 ))                      (1.5.189)
                                                     ρ
               and so we assume a solution to equation (1.5.188) of this same general form. We know that A is small and so
               we make the assumption that the solution of equation (1.5.188) given by equation (1.5.189) is such that φ 0 is
                                                                                                           0
               approximately constant and varies slowly as a function of Aφ. Observe that if φ 0 = φ 0 (Aφ), then  dφ 0  = φ A
                                                                                                           0
                                                                                                    dφ
                    2
               and  d φ 0  00  2
                    dφ 2 = φ A , where primes denote differentiation with respect to the argument of the function. (i.e.
                           0
               Aφ for this problem.) The derivatives of equation (1.5.189) produce
                                    du
                                                             0
                                       = −  A sin(φ − φ 0 )(1 − φ A)
                                                             0
                                    dφ
                                    2
                                   d u     3                                        2  0 2
                                                                               0
                                       = A sin(φ − φ 0 )φ −  A cos(φ − φ 0 )(1 − 2Aφ + A (φ ) )
                                                       00
                                                                               0
                                                       0
                                                                                      0
                                   dφ 2
                                                                                 3
                                                             2 0
                                       = −  A cos(φ − φ 0 )+2 A φ cos(φ − φ 0 )+ O(A ).
                                                               0
               Substituting these derivatives into the differential equation (1.5.188) produces the equations
                                               α   3β
                           2 0                          2      2             2  2  2               3
                       2 A φ cos(φ − φ 0 )+ A −  =     A +2 A cos(φ − φ 0 )+   A cos (φ − φ 0 ) + O(A ).
                             0
                                               2    2
                                              3
               Now A is small so that terms O(A ) can be neglected. Equating the constant terms and the coefficient of
               the cos(φ − φ 0 ) terms we obtain the equations
                                      α    3β  2                     2   3β  2  2
                                                           2 0
                                  A −    =   A          2 A φ =3β A +        A cos(φ − φ 0 ).
                                                             0
                                       2    2                            2
               Treating φ 0 as essentially constant, the above system has the approximate solutions
                                              α             3β      3β
                                         A ≈           φ 0 ≈   Aφ +    A  sin(φ − φ 0 )              (1.5.190)
                                              2              2       4
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