Page 191 - Chemical equilibria Volume 4
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Appendix 2     167
                             We can see that this limiting case keeps the formula of the Maxwell–
                           Boltzmann distribution. The value of  α  is therefore determined  by the
                           relation:
                                            N
                                 exp( α  ) ≅  A                                         [A2.15]
                                    −
                                       A
                                            z A
                             We can show that in this case. We also have the condition:
                                 N <<  g i                                              [A2.16]


                             This means that the number of particles is much less than the number of
                           possible states.


                           A2.2. Partition functions of a molecule object

                           A2.2.1. Definition

                             The partition function of  molecule object of a  collection is the sum  z
                           defined by:

                                            ⎛   ε ⎞
                                            ⎜ ∑
                                                              ( ε β
                                 z =  g i  exp −  i  ⎟  = ∑  g  i exp −  i  )           [A2.17]
                                                B ⎠
                                     i      ⎝  k T     i
                             The sum is extended to all the energy levels which that object can attain.


                           A2.2.2. Independence of energy values


                             The complete partition function for a system includes terms which refer
                           to the different forms of energy: nuclear, electronic, molecule vibration,
                           rotation, translation and the energy of interaction  between the different
                           molecules.

                             For simplicity’s sake, we accept the hypothesis that those different forms
                           of energy, for a molecule, are independent.

                             In these conditions, we can write the total energy of a molecule as the
                           sum of the  different contributions of the forms  of energy: nuclear  ε ,
                                                                                             n
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