(
)
316
D.W. Arnold et al.rChemical Physics Letters 282 1998 313–317
2 P3r2 states, respectively. These values are compa-
spin–orbit population ratios are different than in both
gas-phase CID and collisionless unimolecular de-
composition, and depend on Einc. These differences
suggest that product state distributions are influenced
by exit channel interactions between the decompos-
ing NO2 andror its fragments with the surface.
From the many studies of photoinitiated uni-
molecular decomposition of gaseous NO2 , a robust
rable to, or slightly lower than, those obtained in
scattering from MgO 100 at 1940 cmy1 1 and
Ž
.
w x
w
x
with gas-phase colliders 3,4 .
By summing the populations of all rotational lev-
els in each NO spin–orbit state, the ratio
2
2
w
x w
x
P1r2 r P3r2 ;0.4"0.05 is obtained. This
value lies between the unity ratio obtained in
molecule–surface CID at Einc s1940 cmy1 1 and
signature has emerged: the P3r2 r P1r2 ratio of
2
2
w x
w
x w
x
the ratios obtained in the gas-phase experiments
the NO product is always smaller than the statistical
w
x
w x
3,4 . It is also slightly higher than the ratio of
approximately 0.3 obtained in the unimolecular de-
value of unity 11,12 . This propensity is also present
Ž
in gas phase CID with small collision partners e.g.,
composition of NO2 at excess energy ;2000 cmy1
Ar 3 , and is in qualitative agreement with the
. w x
w
x
11 .
picture of collisional activation followed by uni-
molecular decomposition. However, when CID devi-
ates from the separable, two-step process described
above, significant interactions between the collision
partner and the CID products can affect energy
partitioning, resulting, for example in more ‘equi-
4. Discussion
w
x
The present results, taken together with the gas-
librated’ NO spin–orbit populations 3,4 .
w
x
phase CID studies 2–4 and the molecule–surface
w x
Exit-channel interactions are more complex in the
molecule–surface CID of NO2) than in gas-phase
CID. Molecule–surface binding energies of the par-
CID results obtained at Einc s1940 cmy1 1 , enable
Ž
.
us to obtain a more complete albeit still qualitative
Ž
.
picture of the reaction mechanism. It is therefore
useful to summarize the previous studies.
ent and its fragments are significant, and energy
transfer to the surface may be substantial. In addi-
tion, molecule–surface forces are likely to be stronger
and longer-range for highly excited molecules than
for unexcited molecules. Thus, one cannot assume a
priori that decomposition following collision with
MgO proceeds in a way that parallels gas phase CID.
Measurements at different collision energies reveal
the influence of molecule–surface exit channel inter-
actions on the state distributions of the NO product.
It is probable that some fraction of the NO will
interact strongly with the surface, since its binding
Gas-phase CID can be described as a two-step
Ž .
process: 1 collisional activation creates a distribu-
Ž .
tion of excited NO2 levels above D0 and 2 subse-
quent unimolecular decomposition yields NOqO.
The collider plays mostly a spectator role, and a
statistical model, based on the assumption that the
fractional population of NO2 above D0 decreases
exponentially with increasing energy, reproduces the
w x
experimental observations rather well 3 . Indications
of minor exit-channel interactions with the collider
are revealed mainly through the dependence of the
NO spin–orbit ratio on the nature of the collider.
The average energy transferred per collision depends
on the stiffness of the collision partner, with Ar
w
x
energy is ;0.2 eV 14 . For example, suppose some
of the post-collision NO2 molecules rebound from
˚
the surface with speeds ;6 Arps, and recall that
the NO2 collision-free unimolecular decomposition
rate several hundred cmy1 above D0 is ;1012 sy1
²
:
exhibiting the largest D E values, while poly-
w
x
13 . In this case, some decomposition occurs before
the parent and fragments are free from the surface.
Moreover, studies of expansion-cooled NO scattering
Ž
.
The molecule–surface results reveal some intrigu-
from M gO 100
have shown that the
2
2
Ž .
w
x w
x
ing differences: i the amount of energy transferred
P3r2 r P1r2 ratio for the scattered NO is near
Ž .
w
x
per collision is smaller than in the gas phase; ii
rotational excitation does not increase and may even
the statistical value of unity 15 . This is similar to
the value obtained in NO2) CID on MgO 100 at
Ž
Ž
.
Einc s1940 cmy1, but in contrast to the lower value
.
Ž .
decrease with increasing Einc; and iii the NO