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3. NANOMEMS PHYSICS: Quantum Wave Phenomena                   101


             unraveled by solving the interacting electron problem. The Hamiltonian in
             question, given by (see Appendix B),

                          ° § 1
                                                             +
             H  0  =  2  π v  ­  ¨  + g  · ¸ ¦  ¸  ª 1  N ˆ 2 v  +  ¦  n  q  b  qv  b  qv  º »
                                           «
                          ® ¨
                     L  2  ° ©  g   ¹ v  = L  ,  R  ¬  2  q        ¼    ,  (63)
                          ¯
                      § 1       ª ·                            +  +  º  ½
                                                                      °
                    +  ¨ ¨  − g  ¸ N ˆ  L  N ˆ  R  −  ¦  n  q  (b  qR  b  qL  + b  qR  b  qL  ) ¾
                                                                     »
                                «
                               ¸
                      ©  g      ¬ ¹          q                       ¼  °
                                                                      ¿
             must be diagonalized to determine the pertinent types of solutions holding in
             one dimension.  This  Hamiltonian diagonalization  is facilitated  by the
             procedure of bosonization [137]-[139] discussed in detail in Appendix B. In
             essence,  one-dimensional  bosonization transforms a nondiagonal fermionic
             Hamiltonian into a diagonal bosonic one, with the assumption that the one-
             dimensional  dispersion  relatonship  is  linear,  and  given  by
             E () vk =  =  k −  k   [134]. The nature of this dispersion relation gives rise
                     F      F
             to the transport characterization in terms of spinless left- and right-moving
             electrons with respective electron densities  N  and  N , the parameter g,
                                                     L       R
             which captures the electron-electron interaction strength in the problem, and
             the Fermi velocity  v . Kane  and  Fisher [140]  have captured this
                                  F
             phenomenology with he following set of expressions. The Hamiltonian (63)
             is rewritten as [140], [141],

               H =    v π  [N +  N + 2 λ N  N  ],                                                      (64)
                           2
                                2
                 0     0  R     L       R  L
             with


                       ( ª g  −1  + g )º   ( 1 g−  2 )
               v  = v           ,           λ =   ,                                             (65)
                 0   «         »                2
                                             +
                     ¬    2    ¼           1 g
             with  λ   as  the interaction strength parameter between the  left- and right-
             moving electron species, and g, called the Lüttinger parameter. For  g  =  1
             the interaction is zero, and the Hamiltonian then captures the behavior of a
             noninteracting  electron gas with velocity  equal  to the Fermi  velocity
             v =  v . From (65) it is seen that repulsive  interactions,  which  per  (64)
              0
                   F
             imply  λ >  0 , lead to  g  <  0 , and the opposite is true for attractive
             interactions. In terms of the two-particle interaction potentials, V  and V ,
                                                                     2       4
             between fermions moving in opposite directions, namely, left and right, and
             either both left- or both right-moving, respectively, v and g are given by,
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