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J. Chem. Phys., Vol. 119, No. 14, 8 October 2003
Qiao et al.
970Ϯ60 cmϪ1 and a long vibrational progression is the sec-
ond band of H2O. The abnormally high intensity of the sixth,
seventh, and eighth vibrational peaks of the second band of
H2O is attributed to overlapping with the bands of other
species. The remaining four bands at 10.73, 11.56, 14.20,
14.74 are attributed to the PE spectrum of HOBr. The band at
the lowest energy 10.73 eV is the first PE band of HOBr
because the adiabatic ionization energy at 10.64 eV is in
excellent agreement with and thus confirms the reported ex-
perimental values 10.617 eV,19͑a͒ 10.638 eV,19͑b͒ and a calcu-
lated value 10.65 eV.19͑c͒ The present PES value is equivalent
to our G2 calculated value of 10.645 eV and matches well
the OVGF value 10.689 ͑see Table I͒. The third vibrational
peak at 10.82 eV on the first band has the highest intensity
because the  peak of He I radiation for the first band at
12.61 eV of H2O overlaps on the third vibrational peak of
the first band of HOBr. The vibrational spacing 750Ϯ60
cmϪ1 is larger than the reported value of 620 cmϪ1 ͑Ref. 20͒
for the Br–O stretch model of the neutral HOBr molecule
͑see Table II͒. This shows that ionization corresponding to
the first band is the result of removal of the electron of an
antibonding orbital. This is not only consistent with the char-
tion energy side.17 That is, the PE spectrum of HOBr consists
of at least four bands at 10.73, 11.56, 14.20, and 14.74 eV.
The ͑c͒ of both Figs. 1 and 2 are PE spectra of a mixture
of BrOBr and HOBr which were synthesized without remov-
ing moisture from bromine. It further demonstrates that the
͑a͒ of Figs. 1 and 2 are the PE spectra of pure BrOBr and the
͑b͒ of Figs. 1 and 2 are the PE spectra of pure HOBr.
ACKNOWLEDGMENTS
This project was supported by the National Natural Sci-
ence Foundation of China ͑Contract Nos. 29973051 and
20073052͒ and the Basic Bureau of Chinese Academy of
Sciences ͑No. KJCXZ-HZ-01͒. Z.Q., S.S., and Q.S. thanks
the Chinese Academy of Sciences for a scholarship during
the period of this work.
1 J. G. Anderson, D. W. Toohey, and W. H. Brune, Science 251, 39 ͑1991͒.
2
¨
H. S. P. Muller, C. E. Miller, and E. A. Cohen, Angew. Chem., Int. Ed.
Engl. 35, 2129 ͑1996͒.
3 K. Yagi, J. Williams, N. Y. Wang, and R. J. Cicerone, Science 267, 1979
͑1995͒.
4 M. W. Chase, J. Phys. Chem. Ref. Data 25, 1069 ͑1996͒.
5 R. R. Garcia and S. Solomon, J. Geophys. Res., ͓Space Phys.͔ 99, 12937
͑1994͒.
6 J. C. McConnell, G. S. Henderson, L. Barrie, J. Bottenhiem, H. Niki, C.
H. Langford, and E. M. J. Templeton, Nature ͑London͒ 355, 150 ͑1992͒.
7 S.-M. Fan and D. J. Jacob, Nature ͑London͒ 359, 522 ͑1992͒.
8 WMO, Scientific Assessment of Ozone Depletion: 1994, WMO Global
Ozone Research and Monitoring Project-Report No. 37 ͑WMO, Geneva,
1995͒, and references therein.
acter of the HOMO 6a in which there has been the contri-
Љ
bution of dominant Br and O atoms ͑see Table I͒, but also
this assignment is further supported by the calculated vibra-
tional frequency 626.38 cmϪ1 ͑B3P86͒, 606.03 cmϪ1
͑B3LYP͒, and 623.20 cmϪ1 ͑B3PW91͒ for the Br–O stretch
model of the HOBr ͑see Table II͒.
9 S. Solomon, M. Mills, L. E. Heidt, W. H. Pollock, and A. F. Tuck, J.
Geophys. Res., ͓Space Phys.͔ 97, 825 ͑1992͒.
The band at 11.56 eV with a vibrational spacing of
10 M. K. W. Ko, N. D. Sze, C. Scott, J. M. Rodriquez, D. K. Weisenstein, and
S. P. Sander, J. Geophys. Res., ͓Space Phys.͔ 103, 28187 ͑1998͒.
11 D. X. Wang, P. Jiang, X. M. Qian, and G. Y. Hong, J. Chem. Phys. 106,
3003 ͑1997͒, and references therein.
650Ϯ60 cmϪ1 is the second PE band of HOBr. It results
from ionization of the electron of the 16a , because its value
Ј
matches the computed values of 11.254 eV ͑OVGF͒ and
12 L. A. Curtiss, L. D. Kock, and J. A. Pople, J. Chem. Phys. 95, 4040
͑1991͒.
**
11.804 eV ͑HF/6-311ϩϩG ͒ ͑see Table I͒. The band at
13 W. Von Niessen, J. Schirmer, and L. S. Cederbaum, Comput. Phys. Rep. 1,
57 ͑1984͒.
12.61 eV is the first band of H2O, because the PE spectrum
of HOBr is obtained under condition of H2O existence for
reaction ͑2͒. In fact, the bands of H2O are also used as a
calibration for the PE spectrum of the new species.
The bands in the high ionization energy region ͑Ͼ13.50
eV͒ are the overlapping bands of HOBr and H2O. A clear
shoulder at 14.20 eV is designated as the third band of
HOBr, because there is no band of H2O in this region.17 This
band corresponds to ionization of the electron of the
14 J. Kolm, O. Schrems, and P. Beichert, J. Phys. Chem. A 102, 1083 ͑1998͒.
15 L. T. Chu and Z. Li, Chem. Phys. Lett. 330, 68 ͑2000͒.
16 J. J. Orlando and J. B. Burkholder, J. Phys. Chem. 99, 1143 ͑1995͒.
17 K. Kimura, S. Katsumata, Y. Achiba, and T. Yamazaki, Handbook of HeI
Photoelectron Spectron Spectra ͑New York, 1981͒.
18
͑a͒ R. P. Thorn, Jr., P. S. Monks, L. J. Stief, S.-C. Kuo, Z. Zhang, and R.
B. Klemm, J. Phys. Chem. 100, 12199 ͑1996͒; ͑b͒ I. Novak, Struct. Chem.
3, 377 ͑1992͒.
͑a͒ P. S. Monks, L. J. Stief, M. Krauss, S. C. Kuo, and R. B. Klemm, J.
19
Chem. Phys. 100, 1902 ͑1994͒; ͑b͒ B. Ruscic and J. Berkowitz, ibid. 101,
7795 ͑1994͒; ͑c͒ M. N. Glukhovtsev, A. Pross, and L. Radom, J. Phys.
Chem. 100, 3498 ͑1996͒.
15a (20) orbital. An obvious high intensity band at 14.74 eV
Ј
is the result of overlapping of the bands of both HOBr and
H2O because the band centered near 14.74 eV of H2O should
have a symmetrical shape, the same as with its low ioniza-
20 I. Barnes, V. Bastian, K. H. Becker, R. Overath, and T. Zhu, Int. J. Chem.
Kinet. 21, 499 ͑1989͒.
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