Abstract
Neutron stars can have magnetic fields as strong as 1012-1013 G. We review here some recent experiments that provide a direct determination of the field strength, and some calculations on radiative cross sections and radiation transport in magnetized neutron stars. The magnetic field-induced vacuum polarization effect and its detectability, are discussed.
Original language | English (US) |
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Pages (from-to) | 1551-1554 |
Number of pages | 4 |
Journal | Journal of Magnetism and Magnetic Materials |
Volume | 15-18 |
Issue number | PART 3 |
DOIs | |
State | Published - 1980 |
All Science Journal Classification (ASJC) codes
- Electronic, Optical and Magnetic Materials
- Condensed Matter Physics