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Fig. 3.2 Gibbs energy
change during a reaction
D G m
G m
G m +
D G m
REACTION COORDINATE
where the fc ðÞ are now taken to represent an amount or concentration of potential
reaction species subject to fluctuations of energy, m is the frequency of the fluc-
tuations (the suffixes +,- distinguish the forward and reverse cases, respectively),
and exp G m = R ð Þ is the probability that a given fluctuation will reach G m : Under
the assumptions that the ''attempt'' rates f þ c ðÞ m þ and f c ðÞ m in the two direc-
tions are the same (they must be so at equilibrium, when DG m ¼ 0 ; ) the net rate of
reaction
n ¼ n þ n will be given by
n ¼ n þ 1 e DG m
ð 3 : 10a Þ
RT
(See Lasaga 1981 for a more satisfying derivation of 3.10 using transition state
theory). In the case DG RT ; we then have
n n þ DG m
RT ¼ fc ðÞ DG m
me G RT
ð 3 : 10b Þ
RT
or substituting ( 3.8 ) and dropping the suffixes, the rate coefficient, now also the
specific rate, is given by
n
fc ðÞ DG m
me G RT
k ¼
ð 3 : 11 Þ
RT
This case thus corresponds to the ''near to equilibrium'' linear case discussed
earlier in connection with ( 3.4 ).
The above argument is put on a somewhat sounder basis in transition state
theory, although still under the assumption that there is a thermodynamically
definable intermediate state, known as the activated complex, which is in equi-
librium with the reactants in a steady-state reaction. On statistical mechanical
grounds (Atkins 1978 , Chap. 27; Christian 1975 , Chap. 3; Flynn 1972 , Chap. 7;
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