Dissociation energy of the ground state of the CuH molecule

Details Dissociation energy of the ground state of the CuH molecule Dissociation energy of the ground state of the CuH molecule

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981jqsrt..25..547r&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer, vol. 25, June 1981, p. 547-549. Research supported by the Universi

Computer Science

6

Gas Dissociation, Late Stars, Metallic Stars, Molecular Spectra, Stellar Spectra, Sunspots, Copper Compounds, Correlation Coefficients, Curve Fitting, Diatomic Molecules, Extrapolation, Ground State, Metal Hydrides, Potential Energy, Wentzel-Kramer-Brillouin Method

Scientific paper

The dissociation energy of the ground state of the CuH molecule, which is observed in sun spots and in 19 Piscium, is evaluated by fitting the Hulburt-Hirschfelder function to the RKRV curve. The Hulburt-Hirschfelder potential is shown to reproduce the true curve more accurately than does the Lippincott function. The value obtained for the dissociation energy is 2.84 eV, while the values reported by Herzberg (1950) and Beckel et al. (1971) are less than 2.89 eV and 2.80 + or - 0.12 eV, respectively.

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