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228                                                    Appendix B


             fashion the procedure of bosonization, and we follow their exposition
             closely.
               In general, bosonizing a theory involving M species of fermions may be
             accomplished when a fix specific set of conditions are met, in particular:
                1) The theory can be formulated in terms of a set of fermion creation and
                                   +       +
             annihilation operators,  c  and  c ,  which obey  the following canonical
                                  kq       kq
             anti-commutation relations
                     +
                            δ
               { c kη ,c kη } δ=  ηη ' kk '  ,                                                                              (B.2)
             where the index  η =  1 ,... M  labels M different  species, which  might be
                                     −
             present, and the index  ∈k  [ ∞, ∞ ] is a discrete, unbounded wave number
             of the form,
                    π
                            1
               k  =  2 § ¨n k  − δ b  · , ¸  with n k  ∈  Z  and δ b  ∈  [ ) 2,0  ,                 (B.3)
                    L  ©    2   ¹

             with  n  are integers, L is a length associated with the size of the system, and
                  k
             δ  is a parameter that embodies the nature of the boundary conditions of the
              b
             fermion fields, i.e., whether they periodic or fixed. According to Delft and
             Scholler [139], in typical examples Ș can denote electron spin: Ș = (Ĺ, Ļ), in
             which case M = 2, or it distinguishes left-moving from right-moving spinless
             electrons, as found in a one-dimensional wire, in which case: Ș = (L,R), and
             M = 2. k refers to the momentum index that labels the energy states,  E , of a
                                                                         k
             free noninteracting Fermi gas, defined with respect to the Fermi energy, so
             that E =  E . The discrete and unbounded nature of k are needed in order to
                  0    F
             enable  the systematic accounting  of the  states, on  the one  hand, and  the
             proper definition of bosonic operators, oh the other.

               2) The fermion fields are defined in terms of the creation and annihilation
             operators as follows,

                             ∞
               ψ  () =x  2 π ¦ e −ikx c  ,                                                                  (B.4)
                 η
                         L  k = −∞  kη
             with inverse,   L  2 /

                              ikx
               c kη =  1    ³ e ψ η ()dxx  ,                                                              (B.5)
                       π
                      2 L  − /  2
                           L
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