7483
J. Chem. Phys., Vol. 115, No. 16, 22 October 2001
Photodissociation of CH Cl
2
TABLE I. Calculated rotational energies for selected ͑N,K͒ levels of the two
Since CH is a near-prolate top in both the ground and
the 3p-Rydberg states, the energy levels for a prolate top are
2
˜
3
photon transition to the 3p Rydberg state of CH (X B ).
2
1
used in the calculations of the rotational energies with Bavg
⌬rot /cmϪ1
Erot /cmϪ1
͑
N,K͒
ϭ0.5(BϩC). The rotational selection rules for a two-photon
͑
͑
0,0͒
1,0͒
2,0͒
1,1͒
3,0͒
2,1͒
4,0͒
3,1͒
4,1͒
5,0͒
5,1͒
2,2͒
3,2͒
4,2͒
5,2͒
3,3͒
4,3͒
5,3͒
6,3͒
4,4͒
5,4͒
6,4͒
5,5͒
6,5͒
0.0
Ϫ0.8
Ϫ2.4
Ϫ0.3
Ϫ4.9
Ϫ2.0
Ϫ8.1
Ϫ4.4
Ϫ7.6
Ϫ12.1
Ϫ11.7
Ϫ0.5
Ϫ2.9
Ϫ6.2
Ϫ10.2
Ϫ0.6
Ϫ3.8
Ϫ7.8
Ϫ12.7
Ϫ0.5
Ϫ4.5
Ϫ9.4
Ϫ0.2
Ϫ5.1
0
15
44
81
89
transition are: ⌬Nϭ0, Ϯ1, Ϯ2; ⌬Kϭ0, Ϯ1, Ϯ2. If we con-
Q
sider only transitions with ⌬Nϭ0, ⌬Kϭ0 ͑ Q branch͒, then
͑
͑
͑
͑
͑
͑
͑
͑
͑
͑
͑
͑
͑
͑
͑
͑
͑
͑
͑
͑
͑
͑
the rotational contribution to the total rovibronic transition
energy is given by
111
148
155
215
222
289
310
355
414
488
687
746
821
910
1212
1286
1375
1884
1973
⌬
ϭ͑BЈ ϪBЉ ͒N͑Nϩ1͒
rot
avg avg
2
ϩ͓͑AЈϪBЈ ͒Ϫ͑AЉϪBЉ ͔͒K .
avg
avg
Table I shows ⌬rot for transitions originating from selected
N, K͒ levels, along with their rotational energies. Clearly,
͑
Ϫ1
many rotational levels have ⌬rot within 10 cm . Taking
into account the fact that the transitions are broadened by
intramolecular interactions,19 we expect simultaneous excita-
tion of these levels with the detection at 311.8 nm.
1
B. J. Finlayson-Pitts and J. N. Pitts, Jr., Chemistry of the Upper and Lower
Atmosphere: Theory, Experiments, and Applications ͑Academic, New
York, 2000͒.
C. Sandorfy, Top. Curr. Chem. 86, 91 ͑1979͒.
2
3
S. V. Levchenko and A. I. Krylov, J. Chem. Phys. 115, 7485 ͑2001͒,
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4
P. B. Roussel, P. D. Lightfoot, F. Caralp, V. Catoire, R. Lesclaux, and W.
Forst, J. Chem. Soc., Faraday Trans. 87, 2367 ͑1991͒.
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5
6
2
The participation of the 2 A (3s) state in the dissocia-
1
W. G. Mallard, Gas-Phase Ion and Neutral Thermochemistry ͓J. Phys.
Chem. Ref. Data, Suppl. 17, 1 ͑1988͔͒.
NIST Chemistry WebBook: NIST Standard Reference Database No. 69
tion is not yet clear, as is the role of possible surface cross-
ings. More theoretical work on the ground and excited state
potential energy surfaces is clearly needed. On the experi-
mental front, a search of other dissociation channels is now
in progress.
7
͑
February 2000 Release͒; http://webbook.nist.gov/chemistry/
8
J. J. DeCorpo, D. A. Bafus, and J. L. Franklin, J. Chem. Thermodyn. 3,
25 ͑1971͒.
1
9
0
M. Weissman and S. W. Benson, J. Phys. Chem. 87, 243 ͑1983͒.
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J. A. Seetula, Phys. Chem. Chem. Phys. 2, 3807 ͑2000͒.
1
11
ACKNOWLEDGMENTS
1
1
1
2
3
4
Support by the National Science Foundation and the Do-
nors of the Petroleum Research Fund, administered by the
American Chemical Society is gratefully acknowledged. The
authors benefited greatly from discussions with Anna Krylov,
Sergei Levchenko, and Pavel Jungwirth.
D. W. Kohn, H. Clauberg, and P. Chen, Rev. Sci. Instrum. 63, 4003
͑
1992͒.
15
E. Kolodney and A. Amirav, Chem. Phys. 82, 269 ͑1983͒.
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16
17
M. Zyrianov, A. Sanov, Th. Droz-Georget, and H. Reisler, J. Chem. Phys.
1
10, 10774 ͑1999͒.
APPENDIX: REMPI SPECTROSCOPY
18
19
C. E. Moore, Atomic Energy Levels v.I ͑NSRDS-NBS, 1971͒.
K. K. Irikura, R. D. Johnson III, and J. W. Hudgens, J. Phys. Chem. 96,
3
˜
OF THE CH „X B … RADICAL
2
1
6131 ͑1992͒.
20
In order to calculate the positions of the rotational lines
R. N. Bracewell, The Fourier Transform and Its Applications ͑McGraw-
Hill, New York, 1986͒.
K. Mikhaylichenko, C. Riehn, L. Valachovic, A. Sanov, and C. Wittig, J.
Chem. Phys. 105, 6807 ͑1996͒.
M. R. Cameron and S. H. Kable, Rev. Sci. Instrum. 67, 283 ͑1996͒.
A. V. Demyanenko, V. Dribinski, A. B. Potter, and H. Reisler ͑unpub-
lished͒.
R. D. Johnson III, J. Chem. Phys. 96, 4073 ͑1992͒.
M. E. Jacox and D. E. Milligan, J. Chem. Phys. 53, 2688 ͑1970͒.
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F. Temps, H. Gg. Wagner, and M. Wolf, Z. Naturforsch., A: Phys. Sci. 47,
3
˜
of CH (X B ) it is necessary to know the rotational con-
2
1
21
stants for the ground and excited electronic states of the radi-
3
39
22
23
cal. For the ground B state, the rotational constants are
1
AЉϭ73.811 cmϪ1, BЉϭ8.45 cm , CЉϭ7.184 cm . The ro-
tational constants for the excited 3p-Rydberg state of CH2
are not known. However, since the geometry of this state is
Ϫ1
Ϫ1
24
25
26
expected to be close to that of the ground state of the cation
ϩ
2
27
28
29
CH , the rotational constants for the 3p-Rydberg state can
6
͑
3
60 ͑1992͒.
a͒ H. Koch, H. Jørgen, Aa. Jensen, and P. Jørgensen, J. Chem. Phys. 93,
345 ͑1990͒; ͑b͒ J. F. Stanton and R. J. Bartlett, ibid. 98, 7029 ͑1993͒.
be evaluated using the same geometry. Geometry optimiza-
tion was performed with the Q-Chem program package us-
4
0
4
1
ing the DFT method with B3LYP functionals in a 6-311
ϩ,ϩ͒G͑3df,3pd͒ basis set.42,43 The values obtained ͓r͑CH͒
ϭ1.097 Å, HCH angleϭ141.36°͔ agree well with previous
The axis system in the C2v notation used here is the one customary in
spectroscopy, cf. J. M. Hollas, High Resolution Spectroscopy ͑Wiley, New
York, 1998͒, in which the x axis is out-of-plane, and the z axis is along the
C–Cl bond. Note that in the accompanying paper ͑Ref. 3͒, a different axis
system, common in ab initio calculations, is used in which the y axis is
out-of-plane. However, a nonstandard table of C2v characters is used in
͑
4
4
calculations. The corresponding rotational constants are
Ϫ1
Ϫ1
Ϫ1
AЈϭ73.883 cm , BЈϭ7.783 cm , CЈϭ7.042 cm
.
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