Transition probabilities and dissociation energy of astrophysical molecule GeH

Details Transition probabilities and dissociation energy of astrophysical molecule GeH Transition probabilities and dissociation energy of astrophysical molecule GeH

Jan 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ap%26ss.271...59r&link_type=abstract

Astrophysics and Space Science, v. 271, Issue 1, p. 59-63 (2000).

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

The Franck-Condon factors and r-centroids, which are very closely related to vibrational transition probabilities, have been evaluated by the more reliable numerical integration procedure for the bands of A 2 Δ - X2 πr system of astrophysical molecule GeH, using a suitable potential. The dissociation energy for the electronic ground state of astrophysical molecule GeH has been estimated precisely as D 0 0 = 2.69 ± 0.05 eV by fitting the empirical potential function to the experimental potential energy curve using correlation coefficient.

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