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A. Khachatrian, P.J. Dagdigian / Chemical Physics Letters 402 (2005) 265–269
statistical distribution. This good agreement of the
experimental and prior state distributions is consistent
with formation and decay of an energized CD3SD com-
plex in the dynamics of the S(1D) + CD4 reaction.
While there is sufficient energy to populate SD rota-
tional levels up to J = 25.5–27.5, the experimental and
statistical rotational state distributions peak at much
lower values of J. It is also interesting to note that the
degree of rotational excitation of the SD product from
the S(1D) + CD4 reaction is much less than that
for the SD product of the S(1D) + D2 reaction [12], de-
spite the fact that both reactions proceed by formation
and decay of an energized complex and the energy avail-
able to the former reaction is significantly greater than
for the latter. This reflects the approximately statistical
partitioning of the available energy into the SD and
CD3 internal degrees of freedom.
spin–orbit constant A and the rotational constant B
(A/B = ꢀ7.5 and ꢀ76.9, respectively [22,28]). The small
value of this ratio for OH(X2P) implies that this state
approaches the HundÕs case (b) limit at fairly low values
of J. Within the case (b) limit, the K doublet levels can
display different symmetries of the electronic wave func-
tion with respect to the plane of molecular rotation, and
collisional K doublet propensities can be anticipated
[29]. By contrast, SD(X2P) remains near the HundÕs
case (a) limit for all rotational levels energetically acces-
sible in the S(1D) + CD4 reaction.
Acknowledgement
This research has been supported by the National Sci-
ence Foundation under Grant No. CHE-0413743.
We observe in Fig. 2 that a slight preference for for-
mation of the lower-energy F1 fine-structure manifold
over that for the F2 manifold is predicted in the prior
distribution. The ratio of the total populations in the
F1 to F2 manifolds is computed for the prior distribution
to equal 1.64. The slightly unequal populations result
from the slightly greater energy available to relative
translational energy and CD3 internal energy in the case
of SD products formed in the F1 manifold, and resulting
larger density of available states, than for products
formed in the F2 manifold. Our experimentally deter-
mined SD(X2P) internal state distribution displays an
even greater propensity for formation of products in
the F1 manifold. As noted above, we determine the
fine-structure branching ratio to equal 3.23 0.13.
This fine-structure propensity contrasts with the lack
of such a propensity in the isoelectronic O(1D) + CH4
reaction [1,2]. The exothermicity of this reaction
ðDHo0 ¼ ꢀ191:3 ꢁ 1:2 kJ molꢀ1Þ is much greater than
that of the S(1D) + CH4 reaction. Moreover, the spin–
orbit constant A for OH(X2P) is much less than for
SH(X2P) (A = ꢀ139 and ꢀ377 cmꢀ1, respectively [28]).
Thus, the fine-structure splitting is a much smaller frac-
tion of the total energy available to the products of
O(1D) + CH4 than for S(1D) + CH4. The observed
enhancement of the production of SD in the lower, F1
fine-structure manifold over that predicted by the prior
distribution could be the result of a tendency of the ener-
gized CD3SD complex to dissociate adiabatically to the
lowest fine-structure state.
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