Photodissociation Dynamics of Cl2O
J. Phys. Chem. A, Vol. 108, No. 39, 2004 7963
V. Conclusion
excitations out of the four highest occupied molecular orbitals
(2a2)2 (9a1)2 (7b2)2 (3b1)2 into the lowest unoccupied (10a1)
molecular orbital. This series would consist of a sequence of
transitions to the 1B1, 1B2, and 2A1 states (numbers 1, 2, and
4 in Table 1) with corresponding â* parameters -1, +1, and
0. However, the excitation dynamics must be more complex
than that. The energetic separation of the four highest occupied
molecular orbital is well-known from photoelectron spectros-
copy and covers an energy range of only 2.8 eV. This
contradiction becomes apparent when individual theoretical
results are compared to experimental data. Whereas the predic-
tions of Nickolaisen et al. agree well with the observed
fragmentation dynamics for excitation energies around 5 eV,
their assignment of the first small absorption feature around 3
eV as resulting from triplet r singlet excitation must be
regarded as erroneous. On the other hand, the assignment of
this feature to the 10a1 r 3b1 excitation agrees very well the
experiments of Davis et al. and of Aures et al., but goes along
with incorrect predictions of the fragmentation dynamics around
5 eV. For this energy range, predicted zero or negative â
parameter values are in marked contrast with the experimentally
observed positive values. Considering the second series of one-
electron excitations into the second lowest unoccupied molecular
orbital (8b2) results in a sequence of transitions to 3A1, 2B2,
and 3B1 states (numbers 7, 8, and 9 in Table 1) with
corresponding â* parameters 0, +1, and -1. In fact, this
explanation extends the range where positive â parameters will
be observed well into the energy range above 6 eV and matches
the experimental observations well. In this case, energies and
oscillator strengths for the 2B2 and 3B1 states as calculated by
Tomasello et al. are in much better agreement with experimental
observations than the data published by Toniolo et al. In any
case, the influence of the 2B1 state, which both authors calculate
to lie between the two one-electron sequences into the 10a1 and
8b2 orbitals, respectively, has not been observed experimentally.
Either this state, being the first involving higher excitations than
the 8b2 molecular orbital, mixes strongly with other high-lying
excited states or the rather small oscillator strength, in combina-
tion with unfavorable Franck-Condon factors, might reduce
the intensity of this perpendicular transition to such an extent
that it is too small to be experimentally observable.
The photodissociation of Cl2O has been investigated by
resonance-enhanced multiphoton ionization in combination with
time-of-flight measurements for the excitation energies 5.3 eV
(235 nm) and 6.0 eV (207 nm) in adjacent regions of the first
and the second absorption bands. At 5.3 eV, the main primary
dissociation channel is ClO + Cl(2P1/2). A significant portion
of Cl(2P1/2) undergoes conversion to ground-state Cl(2P3/2) during
fragmentation. The decay is characterized by a positive anisot-
ropy parameter of 0.7 ( 0.2. Excitation proceeds via the
transitions 10a1 r 7b2 and 10a1 r 9a1. At 6.0 eV, the main
dissociation channel is the three-body decay into 2Cl + O. The
decay mechanism is of an asynchronous concerted type, possibly
with ClO(A2Π) as intermediate fragment. The decay is char-
acterized by a small positive anisotropy parameter of 0.2 ( 0.2.
Excitation proceeds mainly via the transition 8b2 r 7b2.
Acknowledgment. The authors thank Professor Kawasaki
for fruitful discussions. The work was supported by the Deutsche
Forschungsgemeinschaft. M.R. thanks the Fonds der Chemis-
chen Industrie for fellowship support.
References and Notes
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Hence, we conclude that at 235 nm Cl2O excitation mainly
occurs via the transitions 10a1 r 7b2 and 10a1 r 9a1. The
observed â parameter of +0.7 suggests that the former makes
the dominant contribution. Its large oscillator strength might
easily compensate for the somewhat larger deviation of its
calculated excitation energy from the photon energy. The
situation can largely be rationalized by the assignment depicted
in Figure 1. According to Tanaka et al., the 1B2 state correlates
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M. J. Chemical Kinetics and Photochemical Data for Use in Stratospheric