Synchrotron radiation of neutrino pairs in neutron stars

Details Synchrotron radiation of neutrino pairs in neutron stars Synchrotron radiation of neutrino pairs in neutron stars

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pazh...17.1090k&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 17, Dec. 1991, p. 1090-1100. In Russian. In Russian.

Statistics

Computation

5

Neutrinos, Neutron Stars, Nuclear Astrophysics, Synchrotron Radiation, Annihilation Reactions, Computational Astrophysics, Relativistic Electron Beams, Stellar Magnetic Fields

Scientific paper

The neutrino energy loss rate is calculated and fitted by a simple formula for the synchrotron radiation of neutrino pairs by electrons in a degenerate relativistic electron gas with a magnetic field under the condition that the electrons populate many Landau levels. In a wide range of parameters the loss rate does not depend on the electron number density. In envelopes of neutron stars at densities of about 10 exp 7 to 10 exp 14 g/cu cm, at temperatures of 10 exp 8 to 10 exp 10 K, and magnetic fields of 10 exp 12 to 10 exp 14 G, the synchrotron losses are comparable to or exceed other neutron energy losses.

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