Page 232 - Principles and Applications of NanoMEMS Physics
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222                                                    Appendix A

             So, the  eigenvalue of  N is  n. For  fermion operators,  the  pertinent
             anticommutation relations and number operator are,
                                               +
                                            +
                                                            +
               a α a β  + a β a α  =  { ,aa α  β } 0= , { ,aa α  β } 0= { ,aa α  β } 0=  ,           (A.40a)
                                                     ,
                 +  +                      +
               a α a α  =  0 , a α a α  =  0, N =  a α a ,                                              (A.40b)
                                             α
                                     α
               N =   a α a α a α a =  a α ( −  a α a α )a =  a α a =  N .                       (A.41)
                      +
                                        +
                                                   +
                           +
                                  +
                 2
                                    1
                             α
                 α
                                             α
                                                     α
                                                          α
               The  second  quantization  formalism is completed by the  necessary
             expressions for operators, which upon acting on the wavefunction will
             measure certain quantities of interest. In this context,  the  quantities  to  be
             measured are classified according to the  number  of  fundamental  particles
             producing it. For instance, in a noninteracting system, these quantities may
             depend  on individual particles, where each  particle contributes  its share
             independently from the others. An example of such a quantity is the kinetic
             energy  of the system. On the other  hand, quantities such as the Coulomb
             interaction energy, in  an  interacting system, depend  on  two-particle
             potentials, thus two-particle operators must be employed. Next, expressions
             for one- and two-particle operators are presented.
               A typical one-particle operator is the  kinetic  energy.  For  a  bosonic
             system, this is obtained by counting the number of particles in a given state,
             multiplying this number by the energy of each particle, and then adding the
             energies of all states. If an arbitrary particle occupies state α, following this
             prescription, then the one-particle operator is given by,
               H =  ¦  α K  α N =      α K  α a α a .                                       (A.42)
                ˆ
                                               +
                                α ¦
                                                  α
                    α               α
             In this expression,  α K  α  is the state energy, given by,
                                              º
                                             2
               E α  = α K α  = φ +  () −r G  ª = 2  ∇ φ  () rdr G  G  ,                                   (A.43)
                                     «
                                              » α
                               ³ α
                                     ¬  2 m   ¼
                                                   G
             where  m is the particle  mass, and  φ α () r  is the  configuration  space
             representation of the wavefunction. Notice, that  α K  α  may be computed
             in any convenient basis in which the wavefunction are available. Thus, in
             momentum-space basis we would have,
                                                   G
                                        2
                                          º
                                    G
                                              G
                                           φ
               E α  = α K  α  = φ +  () p  ª p  » α () p  p d  3  .                                 (A.44)
                                      «
                               ³ α
                                                 2π
                                      ¬ 2m ¼     ( )
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