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238                                                    Appendix B


             Clearly, all the A  = 1 and  B  =  0 . These examples together with Figs. B-1
                           n          n
             and B-2 should provide an  intuitive  way of assimilating  the  concept  of
             bosonization. What we will do next is to finally present an example of the
             bosonization procedure, namely, their Delft and Scholler’s [139] application
             of the procedure to a Hamiltonian with a linear dispersion.
               They begin by assuming a linear dispersion of the form,  () vkE  =  k = ,
                                                                          F
             which measures all energies in units v  = , where the total Hamiltonian is,
                                             F
               H   ≡  ¦  H  ,                                                                                    (B.44)
                 0        0 η
                     η
             with,

                       ∞
               H    ≡  ¦ k  + c +  c  +
                 0 η      + kη  kη +
                      k = −∞
                                            .                                                     (B.45)
                     L 2/  dx
                               +
                    =  ³    + + ψ η () ∂ix  x ψ η () x  + +
                     −L 2/  2 π

             Then,  the  fact  that the Hamiltonian commutes with  the number operator
             [H 0η , N ˆ  ' η ] 0=  for all  ,ηη  ', is exploited as an argument to justify that any
              G
             N -particle ground state  is  an eigenstate  of  H  0 η , in  particular,
                  G       G  G
                          N
             H 0η  N  =  E 0η  N  . The eigenvalue is obtained by adding the energy of
                    0          0
             all levels,

                               ­  N η       1  2  1
                                                     ( δ
                                     −
                               ° ¦
                                                                   0
                                                    η
                                                                η
                                               η
                                       b
               G        G   2 π °  (n δ 2/  ) =  N +  N 1 −  b ) for  N ≥ ,
             E =  N  H  N =    ®  n=1       2     2
              N
                                 0
               η 0
                 0    η 0  0  L  °  ¦ − (n δ 2/  ) =  1 N +  1  N 1 −  ) for  N < 0 .  (B.46)
                                      −
                                                       ( δ
                                                2
                                                η
                                                                  η
                                                      η
                               ¯ n ° = N η +1  b  2  2    b
                           =  2 π 1  N η (N +1 − δ b )
                                    η
                             L 2
             This gives the ground state energy of  H  . When the system is excited, its
                                                0 η
             eigenstate energy  E ,  may increase  in  units of q. This follows from the
             commutation relations,
                               δ
               [H 0η ,b q +  ' η ]= qb q + η ' ηη '  ,                                                                      (B.4 )
                                                                            7
             and its consequence,
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