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Statistics
                             Taking into account that (5.8) is valid for spin up and down particles it
                             must be multiplied by a factor 2.
                             5.1.2 Canonical Ensemble

                                                          A
                             Let us now consider a small system   which stays in contact with a very
                                             R
                             large heat reservoir   (see Figure 5.1b). We only allow   to exchange
                                                                           A
                             heat with  R   (think of a tin-can filled with liquid that is immersed in a
                             lake). In the following we assume that  A «  R  . The total energy of the
                                                                       A
                             system, given by  E  =  E +  E  , is conserved. If   can be found in a
                                            tot    A   R
                             well defined state  A   with energy  E  , then the energy of the heat reser-
                                             i            i
                             voir is given by  E =  E  –  E  . The probability  P   to find exactly an
                                            R    tot   i               i
                             implementation  A  , is proportional to the number of possible implemen-
                                           i
                             tations Ω E(  )  for the heat reservoir  , each of which has energy E
                                                          R
                                       R                                           R
                                                     ⋅
                                                        (
                                               P =  c Ω E   –  E )                 (5.9)
                                                i         tot  i
                             where   is the normalization factor. The prerequisite A «  R   immediately
                                  c
                             implies that  E «  E  . We next expand the logarithm of  Ω   by a Taylor
                                         i  R
                             series about E =  0  , (or about E  ) to obtain a good approximation
                                        i              R
                                                             ∂ lnΩ
                                      (
                                                     (
                                   lnΩ E   –  E ) =  lnΩ E ) –  ------------  E +  …  (5.10)
                                        tot   i        tot   ∂         i
                                                              E
                                                                R  E i =  0
                             Now imagine that, for one specific E i  , the reservoir only has to fulfil the
                             condition that  E =  E  tot  –  E  i  . Due to its huge size compared to  , the
                                                                                  A
                                          R
                             number of implementations of  R   is obviously very large and also
                             increases strongly with increasing energy. Inserting (5.10) in (5.9) yields
                                   ⋅
                             P =  c exp – βE i   and performing the normalization we obtain
                              i
                                                     exp  – (  βE )
                                                             i
                                               P =  -----------------------------------  (5.11)
                                                i
                                                    ∑  exp  – (  βE )
                                                              k
                                                     k
                Temperature  where  ∂ [  lnΩ ∂⁄  E ]  =  β   is independent of the energy  E  .  The
                                           R E i =  0                             i
                                      β
                             parameter   specifies the average energy per degree of freedom of the
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