8814
J. Chem. Phys., Vol. 112, No. 20, 22 May 2000
Miklavc, Perdih, and Smith
mount the potential energy barrier to reaction. Although, as
pointed out previously, on a simple basis it is difficult to see
be most suitable for comparison with the result of KMM
6
calculations when discussing rotational effects.
In subsequent formulations1
2,13
of the KMM, it was ex-
reactivity can be enhanced in this manner for a reaction
dominated by a collinear minimum energy path, since rota-
tional motion would be orthogonal to the motion along the
reaction coordinate, rotational energy might assist in those
many nonlinear collisions that lead to reaction, even in those
cases where the lowest barrier to reaction is for a collinear
geometry.
Orientational effects of reagent rotation have largely em-
phasized the possibility that increased reagent rotational mo-
tion will disrupt the progress of a trajectory towards the most
tended to include the effects of vibration in the BC molecule.
In these calculations, the barriers at the CDS were calculated
to include not only the electronic energy but also the adia-
batic vibrational energy corresponding to the state of the BC
reagent; i.e., of vϭ0 ͑Ref. 12͒ allowing for changes in the
zero-point energy in passing from isolated AϩBC to the
CDS, and of vϭ1 ͑Ref. 13͒ to explore the effects of vibra-
tional excitation in the BC molecule. These modifications
made it possible to compare the KMM results with the nu-
merous results of quasiclassical trajectories. In the case of
the OϩHCl ͑DCl͒ reactions, reasonably good agreement was
again obtained in regard to the dependence of the reaction
cross-sections on both translational and rotational energy of
the reagents, for both vϭ0 and vϭ1, although the agree-
ment was somewhat less good than in the case of the CT
calculations. This poorer agreement might be due to addi-
tional simplifications introduced in estimating the vibra-
tionally adiabatic barriers and to the neglect of recrossing
effects, which become larger the greater the internal excita-
tion of the BC reagent, particularly for H atom transfer reac-
tions. Of relevance to the present work was the observation
that the reaction cross-sections increased for higher initial j
levels but the enhancement predicted by the KMM calcula-
tions was too weak in all the H atom transfer reactions that
were considered.
favorable, i.e., lowest energy, geometry for reaction. Classi-
cal trajectory ͑CT͒ studies7
–10
have shown that this is par-
ticularly the case for ‘‘oblate’’ PESs on which the long-range
interactions tend to guide the trajectory towards the lowest
energy reaction path, thus increasing the reaction cross-
section above the value it would have in the absence of these
forces and hence in the case of straight line trajectories. Ro-
tational excitation reduces this funneling effect and causes a
decline in reactivity with rotational quantum number in the
case of such PESs.
For several reasons, including the ease with which dif-
ferent dynamical effects can be separated out, calculations
using simplified models have an important part to play in
problems of reaction dynamics. Over the past few years we
1
1–13
have developed
a simple kinematic mass model ͑KMM͒
to treat activated bimolecular reactions which is an extension
In the present work we show, using modified KMM cal-
culations, that the orientational effect associated with reagent
rotation can give rise to an enhancement of the cross-sections
with increasing reagent rotation which can greatly exceed
that due to part of rotational kinetic energy being available
for barrier crossing. The analysis of the reactions
of the angle-dependent line-of-centers ͑ADLOC͒ model
originally proposed by Smith.1
,14
The KMM, like the AD-
LOC treatment, assumes straight line trajectories up to the
CDS on the PES, and then examines whether the energy
associated with some critical component of the velocity of
approach exceeds the potential energy at that point on the
CDS. However, in contrast to the ADLOC treatment, the
effects of the anisotropy of the PES and of BC rotational
motion are included in the KMM.
OϩHCl͑DCl͒ and OϩH which we present clearly demon-
2
strates this behavior and leads to a convincing explanation of
the strong j-dependence of the reaction cross-section.
The KMM was first used to calculate opacities, reaction
cross-sections, and the effects of reagent rotation for the re-
actions OϩHCl͑DCl͒→OH͑OD͒ϩCl and OϩHBr→OH
ϩBr. Calculations for OϩHCl were performed on two
II. THE KINEMATIC MASS MODEL
The KMM has been described in detail elsewhere.11–13
Therefore only an outline of the model will be given in the
present article emphasizing those aspects which are espe-
cially relevant to the present calculations.
1
5,16
PESs,
one oblate, and one prolate, and the model results
9
were compared with the results of CT calculations run on
the same surfaces. When applied to the OϩHCl͑DCl͒ reac-
tions on the oblate surface, the cross-sections were about an
order-of-magnitude smaller than those obtained from the CT
calculation, presumably because of the extensive effects of
funneling. However, the same reactions were modeled quite
satisfactorily by the KMM applied on the prolate PES. In all
cases where a prolate surface was used, both the translational
energy and the j-dependence of the reaction cross-sections
In the KMM, attention is focused on relative motion of
the reagents within a small element of space at the CDS. It is
assumed that the reagents follow straight paths up to this
point. This situation is represented in Fig. 1 where some of
the parameters which are used in the implementation of the
model are illustrated: v is the relative collision velocity; the
coordinates R and ␥ are the values of the Jacobi coordinates
at the point of impact in the collision on the CDS, and n is a
unit vector normal to the equipotential contours at R, ␥. Re-
action is assumed to occur if the kinetic energy associated
with the relative velocity (v*) perpendicular to the equipo-
tential contours at the point of impact on the CDS exceeds
the potential energy barrier or the adiabatic potential energy
barrier (Ebar) at that point, i.e.,
9
were in fair agreement with the CT results, although at high
j the model results were lower than those from the trajecto-
ries. In view of the success in modeling dynamics on prolate
surfaces, only such surfaces have been used in subsequent
work including that reported in the present article. It should
be noted that, in the CT calculations reported in Refs. 7–9,
coplanar collisions were studied, with the vibrational effects
on the barriers and these trajectory results therefore appear to
2
1/2*v* уE
.
͑1͒
bar
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