Atoms in Superstrong Magnetic Fields
- 17 August 1970
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 25 (7), 467-469
- https://doi.org/10.1103/physrevlett.25.467
Abstract
In magnetic fields G, characteristic of neutron-star models for pulsars, the ionization energy of atoms is a few hundred electron volts and is a slowly increasing function of . This may greatly affect the nuclear abundances of matter lifted off the stellar surface by electric fields.
Keywords
This publication has 6 references indexed in Scilit:
- One-Dimensional Hydrogen AtomAmerican Journal of Physics, 1969
- Pulsar ElectrodynamicsThe Astrophysical Journal, 1969
- Magnetic Dipole Radiation from PulsarsNature, 1969
- Rotating Neutron Stars and the Nature of PulsarsNature, 1969
- Theory of the absorption edge in semiconductors in a high magnetic fieldJournal of Physics and Chemistry of Solids, 1960
- Theory of the Quadratic Zeeman EffectPhysical Review B, 1939