Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.117...47k&link_type=abstract
Astrophysics and Space Science (ISSN 0044-640X), vol. 117, no. 1, Dec. 1985, p. 47-64.
Astronomy and Astrophysics
Astrophysics
20
Hydrogen Ions, Molecular Ions, Molecular Rotation, Neutron Stars, Stellar Magnetic Fields, Electron Energy, Molecular Structure, Perturbation Theory
Scientific paper
The paper discusses the structure and energies of rotational-vibrational levels of a molecular ion H2(+) in a strong magnetic field typical of neutron stars, B = 10 to the 12th-10 to the 13th G. The study is based on the calculations of the potential energy surface of this molecular ion presented in the paper by Khersonskii (1984). The energies of the rovibrational levels are calculated with the aid of the perturbation theory. The numbers of levels in a H2(+) potential hole is determined at different magnetic intensities. In particular, it is ascertained that the number of levels decreases as the strength of the magnetic field increases. The effect of nuclear spins on the structure of the rotational levels is considered.
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