J. Chem. Phys., Vol. 114, No. 19, 15 May 2001
Photolysis of jet-cooled OClO
8345
2
2
from the initial ( A � B ) electronic excitation. Further-
correspond to a very long dissociation lifetime in the order of
17 ps which is completely unexpected in case of the highly
excited 21,0,0 level. Should OClO decay from a near-linear
geometry, max will be close to 2. Since max is reduced by
a factor of 4 as a result of a long lifetime and a rotational
period of OClO in the order of ϳ1.6 ps,14 the measured 
parameter of 0.4 ͑Table I͒ gives further evidence for a near-
2
1
more, the various impulsive models describing the expected
distributions of the surplus energy over the fragment degrees
of freedom in triatomic decay49,50 are far from sufficient to
account for the observed high percentages of vibrational en-
ergy in the ClO photofragments. As a consequence, impul-
sive fragment recoil is not capable of generating the ob-
served kinetic energy distributions and must at least be
accompanied by an additional mechanism to become a
source of the almost entirely inverted ClO vibrational state
populations which are seen at short photolysis wavelengths
below 280 nm.
2
linear decay along the A1 surface.
Both the trimodality of the vibrational distributions ob-
3
served in the O ( P2) kinetic energy curves, and the substan-
tially altered kinetic energy distributions resulting from prob-
3
3
ing the O ( P1) and O ( P0) fragments indicate that the
2
In view of these considerations, very recent ab initio
predissociative decay of OClO( A2 1Ͼ20,0,0) proceeds via
more than one pathway. Similar O ( P) spin–orbit level-
2
3
theoretical calculations addressing the OClO A potential
2
energy surface reported by Xie and Guo36 appear remarkably
helpful with respect to a rational explanation of the observed
energy partitioning. Their results show that significant in-
dependent kinetic energy release has been observed recently
by Gericke and co-workers6 in the OClO decay at
ϭ308 nm and also in the short-wavelength photolysis of O3
investigated by Houston and co-workers.52 No detailed mod-
els are currently available in describing these exit channel
separable amplitudes of antisymmetric stretching motion
prevail due to anharmonicity of the A state potential. Al-
though the OClO parent is in the first step excited to a purely
symmetric stretch vibronic level of the A state and the A
2
2
correlation effects and further theoretical work is demanded.
2
2
2
Given the strong fragment recoil anisotropy, the A surface
1
2
2
is nonetheless likely to act as the main exit channel at the
employed wavelengths thereby imprinting its near-linear
equilibrium angle on the fragmenting triatomic parent.
potential exhibits only a single C2v minimum, the wave
function has significant non-C2v symmetry. This is calcu-
2
lated to be the case for ( A Ͼ4,0,0) vibronic levels of
2
1
OClO. The coupling between symmetric and antisymmetric
stretching coordinate is already clearly visible as a bifurca-
tion in the wave function calculated for the relatively low
V. CONCLUSION
2
36
With the blue wing OClO dissociation study reported in
this article, virtually the entire spectral region of the
lying A 5,0,0 vibronic level of OClO. As a consequence,
2
2
the initial OClO( A Ͼ20,0,0) parent geometry is far off
2
1
2
2
UV( A � B ) absorption band of the OClO molecule has
2
1
from C2v with largely unequal Cl–O bond distances. Ac-
cordingly, the transition dipole and recoil vector become
closer to parallel, resulting in a higher beta value. The initial
asymmetric stretching motion of vibronically excited
been covered to date by the various state-to-state investiga-
2
tions of the nascent photoproducts ClO(X ⌸ ,v,J) and O
⍀
3
(
P ). Although available theory ͑see for example Refs. 34,
J
2
35, and 36, and references therein͒ is suitable to explain
much of the observations, there is a clear need for more
refined theory which can account for spin–orbit correlation
effects.
Summarizing, the observed very high anisotropy param-
eters and extreme channeling of available energy show a
fundamental change of the fragmentation dynamics of OClO
OClO( A Ͼ20,0,0) exceeds the bond dissociation energy
2
1
with the O fragment asymptotically released at the outer
turning point. This rationale agrees with the observed paucity
2
of fragment kinetic and rotational energy. OClO( A
2
1
Ͼ20,0,0) with an expected severely distorted symmetry is
initially prepared, undergoes fast coupling to the near-
2
degenerate A surface, and subsequently decays under a
1
17
prevalent in the hitherto disregarded blue end of the OClO
near-linear geometry.
near UV absorption band. Furthermore, the amount of vibra-
tionally hot ClO radicals generated from OClO at short pho-
tolysis wavelengths should be scrutinized in light of possible
atmospheric mechanisms due to both their increased reactiv-
ity and absorptivity.
As obvious from Figs. 3 and 4, the kinetic energy distri-
butions obtained from OClO photodissociation at somewhat
longer photolysis wavelengths, namely, at 292.5 and 293 nm,
are the sum of three different contributions. As to the slowest
fraction, the decrease in the corresponding  parameters with
increasing dissociation wavelength ͑see Table I͒ is presum-
ably due to a longer dissociation lifetime rather than the
ACKNOWLEDGMENTS
2
2
result of fast dissociation via the more bent A2 and B2
R.F.D. and A.T.J.B.S acknowledge financial support by
the European Union TMR program IMAGINE, Contract No.
ERB 4061 PL 97-0264. Technical assistance by Cor Sikkens
and Chris Timmer is gratefully acknowledged. We thank I.
Szydtowska, Dr. W. L. Meerts, and Dr. K. Remmers for
providing us with their polyatomic spectra fitting program.
states, respectively. This reasoning is supported by the recur-
rence of rotational resolution at high energies visible in the
photofragment yield spectrum of the 21,0,0 vibronic level
͑
Fig. 6͒ which is in the first instance quite puzzling with
5
1
regard to earlier work reported by Richard and Vaida. In
their high-resolution absorption study the rotational state
2
vanished for the OClO( A 8,0,0) band which is in agree-
2
1
A. Wahner, G. S. Tyndall, and A. R. Ravishankara, J. Phys. Chem. 91,
ment with the unresolved 12,0,0 band structure depicted in
2
734 ͑1987͒.
Fig. 6 ͑middle͒. The rotational linewidths of the 0,0,0 and of
2
M. B. McElroy, R. J. Salawitch, S. C. Wofsy, and J. A. Logan, Nature
Ϫ1
the 21,0,0 band shown in Fig. 6 are about 0.3 cm and
͑London͒ 321, 759 ͑1986͒.
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