Page 237 - PRINCIPLES OF QUANTUM MECHANICS as Applied to Chemistry and Chemical Physics
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228                      Systems of identical particles
                                                            8ðv
                                                     E tot ˆ    (2m e ) 3=2  E F 5=2
                                                            5h 3
                             which may be simpli®ed to
                                                                 3
                                                           E tot ˆ  NE F                       (8:62)
                                                                 5
                             The average energy E per electron is, then
                                                              E tot  3
                                                          E ˆ     ˆ   E F                      (8:63)
                                                               N    5
                               Equations (8.57) and (8.58) are valid only for values of E suf®ciently large
                             and for energy levels suf®ciently close together that E can be treated as a
                                                                                   3
                             continuous variable. For a metallic crystal of volume 1 cm , the lowest energy
                             level is about 10 ÿ14  eV and the spacing between levels is likewise of the order
                             of 10 ÿ14  eV. Since metals typically possess about 10 22  to 10 23  free electrons
                                   3
                             per cm , the Fermi energy E F is about 1.5 to 8 eVand the average energy E per
                             electron is about 1 to 5 eV. Thus, for all practical purposes, the energy of the
                             lowest level may be taken as zero and the energy values may be treated as
                             continuous.
                               The smooth surface of the spherical octant in n-space which de®nes the
                             Fermi energy cuts through some of the unit cubic cells that represent single-
                             particle states. The replacement of what should be a ragged surface by a
                             smooth surface results in a negligible difference because the density of single-
                             particle states near the Fermi energy E F is so large that E is essentially
                             continuous. At the Fermi energy E F , the density of single-particle states is
                                                                           1=3
                                                             2ðvm e 3N
                                                     ù(E F ) ˆ                                 (8:64)
                                                                h 2   ðv
                             which typically is about 10 22  to 10 23  states per eV. Thus, near the Fermi energy
                             E F , a differential energy range dE of 10 ÿ10  eV contains about 10 11  to 10 12
                             doubly occupied single-particle states.
                               Since the potential energy of the electrons in the free-electron gas is assumed
                             to be zero, all the energy of the mobile electrons is kinetic. The electron
                             velocity u F at the Fermi level E F is given by
                                                           1    2                              (8:65)
                                                                F
                                                           2  m e u ˆ E F
                             and the average electron velocity u is given by
                                                         1   2        3                        (8:66)
                                                          m e u ˆ E ˆ E F
                                                         2            5
                                                                                     8
                                                                                           ÿ1
                             For electrons in a metal, these velocities are on the order of 10 cm s .
                               The Fermi temperature T F is de®ned by the relation
                                                            E F ˆ k B T F                      (8:67)
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