Physics
Scientific paper
Oct 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrvd..46.3256k&link_type=abstract
Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 46, Issue 8, 15 October 1992, pp.3256-3264
Physics
17
Elementary Particle Processes, Neutron Stars
Scientific paper
A general formalism is developed for calculating the neutrino emissivities of synchrotron and e-e+ annihilation radiations in a plasma in the presence of a large magnetic field B~1012-1014 G. As a first step, the formalism is used to calculate the synchrotron and annihilation radiations from a nonrelativistic electron plasma (density ρ<~106 g cm-3, temperature T<~6×109 K) including the cases of nondegenerate and degenerate electrons, and of quantizing and nonquantizing magnetic fields. We conclude that these processes can be important for neutrino production in a hot plasma of neutron star envelopes.
Amsterdamski Piotr
Haensel Pawel
Kaminker A. D.
Levenfish K. P.
Yakovlev Dmitry G.
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