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Statistics
                                               ∏
                                          Q =
                                                             i
                                                                   i
                                                i  ∑  exp  ( – (  βE +  α)n )     (5.22)
                                                   n i
                                                                 i
                             The product in (5.22) accounts for all states   accessible to the system,
                             while the sum over  n   depends on how many particles may occupy a
                                               i
                             state . i
                             5.2 Particle Statistics: Counting Particles

                             Different statistical properties of the system arise from the many ways
                             that the sum in (5.13) and (5.22) has to be performed. Summation over all
                                         i
                             possible states   in turn implies summation over all possible values of
                             n  . We now consider these cases.
                              i
                            fE()                            fE()

                                 B
                                                                         Bose-Einstein
                                    Bose-Einstein
                                    Maxwell-Boltzmann                    Fermi-
                                    µ =  0                               Dirac
                                                                          µ >  0




                                                     E                              E

                Figure 5.2. Maxwell-Boltzmann, Bose-Einstein, and Fermi-Dirac distributions.



                             5.2.1 Maxwell-Boltzmann Statistics

                             Suppose that there are N   distinguishable and noninteracting particles in
                             the system. Then, for a given implementation  n n …,{  ,  }  , n   particles
                                                                    1  2       j
                             have the energy E  , to which we must add the constraint that Σ n =  N  .
                                           j                                   k k
                             According to (B 5.1.2) there are  N! (⁄  n !n !…)   possibilities to distrib-
                                                             1  2
                                   N
                             ute the   particles among all available states. This way of counting dis-
                             tinguishes the individual particles, but not their ordering once they

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