Matter and Radiation in Strong Magnetic Fields of Neutron Stars

Details Matter and Radiation in Strong Magnetic Fields of Neutron Stars Matter and Radiation in Strong Magnetic Fields of Neutron Stars

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jphcs..31...68l&link_type=abstract

Journal of Physics: Conference Series, Volume 31, Issue 1, pp. 68-75 (2006).

Physics

Scientific paper

Neutron stars are found to possess magnetic fields ranging from 108 G to 1015 G, much larger than achievable in terrestrial laboratories. Understanding the properties of matter and radiative transfer in strong magnetic fields is essential for the proper interpretation of various observations of magnetic neutron stars, including radio pulsars and magnetars. This paper reviews the atomic/molecular physics and condensed matter physics in strong magnetic fields, as well as recent works on modeling radiation from magnetized neutron star atmospheres/surface layers.

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