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Appendix 1

      DERIVATION  OF  THE


      TRANSITION  STATE  THEORY


      EXPRESSION  FOR  A


      RATE  CONSTANTa



















      In order to  analyze the  transition  state equilibrium, we  need  to  know  how  a
      collection of molecules divides up the available energy.

     THE  BOLTZMANN  DISTRIBUTION
      Molecules  distribute  their  total  energy  among  translational,  rotational,  vibra-
      tional, and electronic motions. These motions are all quantized, with energy-level
      separations very small for translation, larger for rotation, still larger for vibration,
      and very large for electronic motion.  There are therefore  many discrete energy
      states available. At very_ low temperature,  approaching absolute zero, nearly all
      the_~o!ecules are in their lowest energy state; but as the temperature is raised,
      the molecules acquire more energy and begin to populate higher states.  The ratio
      of numbers  of molecules in any two states depends on the energy difference be-
      tween the states and on the temperature, and is given by the Boltzmann distribu-
      tion law,




      Here  n,  is  the number of  molecules  in state  1, energy  E,,  n,  is  the  number  of
      molecules in  state 2,  energy  E,,  k  is  the  Boltzmann  constant,  1.3806  x  10-l6
      erg OK-l,  and  T is the absolute temperature in degrees Kel~in.~


      ' Derivations may be found in the sources cited in note 36 of  Chapter 2.
       For  a derivation  see K. B.  Wiberg,  Physical  Organic Chemistry, Wiley, New  York,  1964, p.  21 1, or
      W. J. Moore, Physical Chemistry, 3rd ed.,  Prentice-Hall,  Englewood Cliffs, N.J,,  1962, p.  619.
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