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J. Chem. Phys. 99, 1271 (1993); http://dx.doi.org/10.1063/1.465371 (7 pages)

The low lying electronic states of O3

Wolfram Koch1, Gernot Frenking2, G. Steffen2, D. Reinen2, M. Jansen3, and W. Assenmacher3

1Institut für Organische Chemie, Technische Universität Berlin, Strasse des 17. Juni 135, D‐1000 Berlin 12, Germany
2Fachbereich Chemie, Philipps‐Universität Marburg, Hans‐Meerwein‐Strasse, D‐3550 Marburg, Germany
3Institut für Anorganische Chemie der Universität, D‐5300 Bonn, Germany

(Received 26 February 1993; accepted 5 April 1993)

The energies of the three lowest lying excited states of the ozonide anion (1 2B2, 1 2A1, 1 2A2) at the optimized geometry of the X2B1 ground state are theoretically predicted at the MRCI‐SD level of theory using large atomic natural basis sets. The calculated vertical excitation energy Tv=2.85 eV for the 1 2A2X2B1 transition, which has a large transition moment, is in good agreement with the experimental results for the isolated O3 anion in host matrices and solution between 2.69–2.81 eV. The state symmetry forbidden transition 1 2B2X2B1 is calculated with Tv=2.26 eV. The excitation energy for the 1 2A1X2B1 transition is theoretically predicted with Tv=2.28 eV and a very low transition moment. The theoretical results are also discussed in comparison with recently observed low lying absorption bands of O3.

KEYWORDS and PACS

PACS

  • 33.70.Ca

    Oscillator and band strengths, lifetimes, transition moments, and Franck-Condon factors

  • 31.50.Df

    Potential energy surfaces for excited electronic states

ARTICLE DATA

PUBLICATION DATA

ISSN

0021-9606 (print)  
1089-7690 (online)

For access to fully linked references, you need to log in.
    The Quantum-Chemistry Literature Data Bank, edited by K. Ohno, K. Morokuma, and H. Hosoya (JAICI, Tokyo, 1990) shows in its 1990 edition 103 entries for ab initio calculations of O3. The following references (Refs. 1–5) are just the latest studies which are relevant for the present paper: S. M. Adler-Golden, S. R. Langhoff, C. W. Bauschlicher, and G. D. Carney, J. Chem. Phys. 83, 255 (1985JCPSA6000074000011006096000001).

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    (b) D. H. Magers, W. N. Lipscomb, R. J. Bartlett, and J. F. Stanton, ibid. 91, 1945 (1989JCPSA6000091000003001945000001).

    T. J. Lee and G. E. Scuseria, J. Chem. Phys. 93, 489 (1990JCPSA6000093000001000489000001).

    K. Ohta, H. Nakatsuiji, K. Hirao, and T. Yonezawa, J. Chem. Phys. 73, 1770 (1980JCPSA6000073000004001770000001).

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    P. C. Cosby, J. T. Moseley, J. R. Peterson, and J. H. Ling, J. Chem. Phys. 69, 2771 (1978JCPSA6000069000006002771000001).

    S. E. Novick, P. C. Engelking, P. L. Jones, J. H. Futrell, and W. C. Lineberger, J. Chem. Phys. 70, 2652 (1979JCPSA6000070000006002652000001).

    L. J. Wang, S. B. Woo, and E. M. Helmy, Phys. Rev. A 35, 759 (1987).

    J. Almlöf and P. R. Taylor, J. Chem. Phys. 86, 4070 (1987JCPSA6000086000007004070000001).

    W. J. Hehre, R. Ditchfield, and J. A. Pople, J. Chem. Phys. 56, 2257 (1972JCPSA6000056000005002257000001).

    R. Krishnan, J. S. Binkley, R. Seeger, and J. A. Pople, J. Chem. Phys. 72, 650 (1980JCPSA6000072000001000650000001).


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