Page 125 - Mechanism and Theory in Organic Chemistry
P. 125

Let us assume that we have two isomeric substances A and B in equilibrium
                at very low temperature, so that we can say that for practical purposes all mole-
                cules are in  their lowest  energy states.  Then we  could regard  A and B as two
                energy  states of  a  system, and  since  there  are only  two  populated  states,  the
                equilibrium constant K, the ratio of the number of B molecules to the number of A
                molecules, would be given by Equation A1.2,
                                                   [ - (€0; ;
                                           NB               €01)
                                              =
                                       K  = - exp              I
                                           NA
               The quantity E,,  is the energy of the lowest state of B, and E,,   is the energy of the
               lowest state of A. As it is more convenient to have energies on a molar basis, we
               multiply  the energies and the Boltzmann  constant by Avagadro's  number,  No,
               and  since kNo is  equal to the gas constant R,  1.986 cal OK  mole-l,  we  obtain
                Equation A1.3 :


                                        K  = exp
                                                     RT

                E:  is  the standard state energy at O°K.  Equation A1.3  may be  written  in  the
               form  A1.4,  and  since  at  absolute  zero  AE:  = AH:  = AG,", this  equation  is

                                             - AE:  = RTln K                       (A1.4)

               indeed the familiar thermodynamic expression for the equilibrium constant.

               The Partition Function
               The example we have used is of course unrealistic; we are interested in what goes   : .
               on at temperatures above absolute zero, where many energy levels of the mole-
                                                                                          '
               cules are populated. All we need do to correct our equilibrium constant A1.3 is
               to find out how many molecules of A and of B are in each energy level at the
                temperature of interest. The total number of molecules of A,  NA, is the sum of
                numbers of molecules in each energy state,



                So far we have assumed that each state has a different energy, but this will not
                always be true. We have to allow for degeneracies, that is, groups of more than one
               state at the same energy. When two states have the same energy, their populations
                must be identical; we  therefore modify Equation A1.5 to A1.6, where g,,  is the



                number of states that have energy E~A, and n,,  is the number of molecules occupy-
               ing a single state of energy €,,.   Since the Boltzmann distribution deals with ratios
               of numbers in various states, we divide both sides of Equation A1.6  by no,  and
                                                                                            .
               obtain Equation A1.7, which gives the ratio of the total number of molecules to
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