Electromagnetic transitions for the hydrogen atom in strong magnetic fields

Details Electromagnetic transitions for the hydrogen atom in strong magnetic fields Electromagnetic transitions for the hydrogen atom in strong magnetic fields

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...242..828w&link_type=abstract

Astrophysical Journal, Part 1, vol. 242, Dec. 1, 1980, p. 828-842. Research supported by the Deutsche Forschungsgemeinschaft.

Astronomy and Astrophysics

Astrophysics

27

Electromagnetic Interactions, Hydrogen Atoms, Neutron Stars, Stellar Magnetic Fields, Stellar Structure, Transition Probabilities, Adiabatic Equations, Atomic Structure, Field Strength, Radiative Transfer, Wave Functions

Scientific paper

Relevant formulas for electromagnetic transitions in strong magnetic fields are provided, and applied to the hydrogen atom. For magnetic field strengths in the range 235 billion to 4.7 trillion gauss, which are characteristic of neutron stars, dipole strengths, oscillator strengths, sum rules, asymptotic formulae, transition probabilities, lifetimes, and intensities are calculated.

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