Communications
1767
trum in good signal-to-noise ratio. For other fragment mea-
surements, the power was reduced to 50 J.
2
According to the linewidth measurements of the
1
1
ϩ
4
pL ⌸(vϭ0)←3sB ⌺ (vϭ0) transition reported by
7 4–6
Drabbels et al. and by the group of Ubachs, the linewidth
of the Q branch (f-symmetry component͒ is independent of
J, while those of the P and R branches (e-symmetry com-
ponent͒ increase proportionally with J(Jϩ1). The J depen-
dence suggests that the e-symmetry component of the
1
1
ϩ
4
pL ⌸(vϭ0) state predissociates to the repulsive ⌺
1
ϩ
potential surface, that is, DЈ ⌺ state, and that the predis-
sociation of the f-symmetry component of the 4pL ⌸(v
ϭ0) state dissociates to the repulsive ⌸ state, that is the
1
1
1
13,17
2
⌸ state.
By assuming that the radiative decay rates of
the Rydberg states are much smaller than the predissociation
rates, the total quantum yield to the singlet and triplet disso-
ciation channels is considered to be unity. As a consequence,
the change of the predissociation rate to the singlet channel
leads to the change in the quantum yield of the triplet chan-
FIG. 3. Photofragment yield and simulated spectra of 4pL 1⌸(v
1
ϩ
3
1
ϭ0)←3sB ⌺ (vϭ0) transition of CO. ͑a͒ C( P) and ͑b͒ C( D) frag-
ment monitored spectra.
1
cluded that the predissociation of the 4pL ⌸(vϭ0) state
1
to the triplet channel competes with that to the singlet chan-
nel with comparable rate.
nel product, that is C( D). Thus the observed dependence
3
1
1
for the C( P) and C( D) products for the 4pL ⌸(v
ϭ0) state can be explained by that the predissociation pro-
cesses to the singlet and triplet channels are competing with
the similar rate and the rotational dependence is due to that
of the predissociation rate to the singlet channel.
Furthermore, it is suggested that the predissociation rate
1
of the 3dLЈ ⌸(vϭ1) to the triplet channel is also com-
1
parable to that to the singlet channel because the C( D) sig-
1
nal intensity of 3dLЈ ⌸(vϭ1) is similar to that of
1
4
3
ϳ10
pL ⌸(vϭ0). Estimated predissociation rate of the
We estimated the predissociation rates to the singlet and
triplet channels from the observed photofragment yield spec-
tra and from the reported total decay rate, k, of each rota-
tional levels obtained from the linewidth measurement. Here
1
dLЈ ⌸(vϭ1) state to the triplet channel is kT
11
Ϫ1
s .
Shafer III et al. calculated several valence states for the
triplet repulsive states to which the Rydberg states predisso-
the total decay rates are the sum of the singlet (k ) and triplet
s
3
ϩ
3
Ϫ
3
ciate. According to their calculation, ⌺ , ⌺ , and ⌸
states are known to cross the potential curves of the Rydberg
states at relatively low energy region. At this stage, we can
not predict which state is mainly responsible for the predis-
sociation. More detailed analysis is in progress, which in-
cludes the rotational and vibrational dependencies of the pre-
dissociation rates.
(
kT) dissociation rates. For the e-symmetry component, the
predissociation rate to the singlet manifold is expressed as
the sum of the J independent and dependent terms,
e
S
k ϭk ϩk J͑Jϩ1͒.
͑1͒
0
J
For the f-symmetry component, on the other hand, the rate
includes only J independent term,
f
ACKNOWLEDGMENTS
k ϭk .
͑2͒
S
0
The authors would like to thank Dr. Asuka Fujii and Dr.
Haruki Ishikawa for their helpful discussions and T. Ebata
would like to thank Professor Robert W. Field for his interest
of this work and valuable suggestions.
For the triplet channel, we assumed that k is independent of
T
J, since the spin–orbit coupling does not include J. Though
this assumption is rather crude, the simulated photofragment
yield spectrum well reproduced the observed spectra. The
observed signal intensities are given by
1
C. Letzelter, M. Eidelsberg, F. Rostas, J. Breton, and B. Thieblemont,
kT
Chem. Phys. 114, 273 ͑1987͒.
M. Eidersberg, J. Y. Roncin, A. Le Floch, F. Launay, C. Letzelter, and J.
Rostas, J. Mol. Spectrosc. 121, 309 ͑1987͒.
M. Eidelsberg, J. J. Benayoun, Y. Viala, and F. Rostas, Astron. Astro-
phys., Suppl. Ser. 90, 231 ͑1991͒.
P. F. Levelt, W. Ubachs, and W. Hogervorst, J. Chem. Phys. 97, 7160
1
2
I͑ D͒ϭS
ϫ
ϫ
,
͑3͒
͑4͒
J J
Ј Љ
kSϩkT
3
kS
3
I͑ P͒ϭS
,
4
J J
Ј Љ
kSϩkT
͑
1992͒.
5
6
7
K. S. E. Eikema, W. Hogervorst, and W. Ubachs, Chem. Phys. 181, 217
͑1994͒.
W. Ubachs, K. S. E. Eikema, P. F. Levelt, W. Hogervorst, M. Drabbels,
W. L. Meerts, and J. J. ter Meulen, Astrophys. J. 427, 55 ͑1994͒.
M. Drabbels, J. Heinze, J. J. ter Meulen, and W. L. Meerts, J. Chem. Phys.
1
1
ϩ
where S
is the 4pL ⌸(vЈϭ0,JЈ)←B ⌺ (vЉϭ0,JЉ)
J J
Ј Љ
transition intensity. From the linewidth measurements by
Drabbels et al., kJϭ1.2ϫ109
7
s
Ϫ1
,
and k ϩk ϭ1.9
0 T
9
Ϫ1
ϫ10
s . By changing the value of k , we found the simu-
lated spectra well reproduce the observed ones for k ϭ1.4
T
99, 5701 ͑1993͒.
8
9
T
N. Hosoi, T. Ebata, and M. Ito, J. Phys. Chem. 95, 4182 ͑1991͒.
M. Komatsu, T. Ebata, and N. Mikami, J. Chem. Phys. 99, 9350 ͑1993͒.
9
Ϫ1
ϫ10
s
, as shown in Fig. 3. From these results, it is con-
J. Chem. Phys., Vol. 108, No. 5, 1 February 1998
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