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Interpretation of Rate Constants  95

       T is the temperature in degrees Kelvin. The units of A, called  the pre-exponential
      factor,  are the same as those of k,,,:   for a first-order rate constant,  time-';  for a
      second-order rate constant, 1 mole-'  time-'.  We use the notation k,,,   to empha-
      size that the equation applies to the observed rate constant, which  may or may
      not  be  simply related  to  the microscopic k's  characterizing  the individual steps
      of a reaction sequence.
           If we write Equation  2.50 in  the form of Equation 2.51, we  see at once a
      resemblance to the familiar relation  2.52 between  the equilibrium constant of a
                                             C)
                                 -E,  = RTln  -
                                  -AGO  = RTln K                          (2.52)
      reaction  and its free-energy  change. Hence it  is  natural  to  interpret  E,  as  an
      energy.  This  energy is  called  the Arrhenius activation energy,  or  simply  activation
      energy,  and may  be  crudely interpreted as the height  of an energy barrier over
      which reactants must pass on their way to products. Yet because k,,,  will not in
      general correspond to the microscopic constant for a single step, the origin of the
      activation  energy on the molecular  level is not well defined.  To obtain a more
      precise idea of the dynamic behavior  of molecules during a reaction, we turn to
      the transition-state  theory.

      Transition State Theory36
      The transition state theory is  confined  to consideration of single elementary re-
      action  steps, and is meaningful only when  applied to a  single microscopic rate
      constant.  The theory  postulates  that  when  two  molecules  come  together  in  a
      collision that leads to products (or when a single molecule in a unimolecular step
      follows the motions  that cause the chemical change), they  pass  through a  con-
      figuration  of  maximum  potential  energy  called  the transition state.  In order  to
      understand this concept fully, we must first digress to consider some ideas about
      potential energy surfaces.


           Potential energy surfaces  Because each of the Natoms in a molecule can
      move  in  three  mutually perpendicular  and  therefore  independent directions,  a
      molecule has a total of 3N degrees of freedom. But since we think of a molecule
      as a unit, it is useful to divide these degrees of freedom into three categories.  If
      the atoms were fixed relative to each other, the position of the rigid molecule in
      space would  be defined by specifying six quantities: the three  cartesian  coordi-
      nates of its center of mass and three rotational angles to indicate its orientation
      in  space.  Hence  there  remain  3N - 6  degrees  of  freedom  which  are  internal
      vibrational motions of the atoms with  respect to each other.  (A linear molecule


        Transition state theory is discussed in standard texts on physical  chemistry, kinetics,  and physical
      organic chemistry.  See, for  example,  (a) W. J.  Moore,  Physical  Chemistry,  3rd  ed.,  Prentice-Hall,
      Englewood  Cliffs,  N.J.,  1962, p.  296;  (b) S. W. Benson,  Thermochemical  Kinetics,  Wiley,  New  York,
      1968; (c) K. J. Laidler, Chemical Kinetics, 2nd ed., McGraw-Hill, New York,  1965; (d) K. B. Wiberg,
      Physical  Organic  Chemistry,  Wiley,  New  York,  1964;  (e) L.  P.  Hammett, Physical  Organic  Chemistry,
      2nd  ed.,  McGraw-Hill,  New  York,  1970.  For  a  different  approach  to  chemical  dynamics,  see
      (f) D.  L. Bunker, Accts.  Chem. Res., 7, 195 (1974).
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