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Photodissociation of NaH

Anindita BhattacharjeeDepartment of Spectroscopy, Indian Association for the Cultivation of Science, Calcutta 700032, IndiaKrishna Rai DastidarDepartment of Spectroscopy, Indian Association for the Cultivation of Science, Calcutta 700032, India
2002en
ABI

Abstract

We have calculated the photodissociation cross section of NaH through the $B{}^{1}\ensuremath{\Pi}$ state. We have solved the time-dependent Schr\"odinger equation by using the Chebyshev-polynomial scheme and Fourier grid Hamiltonian method. We have used four different sets of potential-energy curves for $X{}^{1}{\ensuremath{\Sigma}}^{+}$ and $B{}^{1}\ensuremath{\Pi}$ states [E. S. Sachs, J. Hinze, and N. H. Sabelli, J. Chem. Phys. 62, 3367 (1975); R. E. Olson and B. Liu, J. Chem. Phys. 73, 2817 (1980); W. C. Stwalley, W. T. Zemke, and S. C. Yang, J. Phys. Chem. Ref. Data 20, 156 (1991)]. We have found that the values of maximum photodissociation cross section and the corresponding photon energy depend on the choice of the potential-energy curves. But all these results differ significantly from an earlier calculation [K. Kirby and A. Dalgarno, Astrophys. J. 224, 444 (1978)]. We have also found that the photodissociation occurs mainly due to the Franck-Condon transitions.

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