Thermal effects of nonequilibrium beta-processes in a strong magnetic field

Details Thermal effects of nonequilibrium beta-processes in a strong magnetic field Thermal effects of nonequilibrium beta-processes in a strong magnetic field

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991azh....68..984s&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 68, Sept.-Oct. 1991, p. 984-991. In Russian.

Astronomy and Astrophysics

Astronomy

Degenerate Matter, Stellar Interiors, Stellar Magnetic Fields, Thermal Energy, Weak Interactions (Field Theory), Electron Gas, Neutrinos, Nonequilibrium Conditions, Relativistic Electron Beams

Scientific paper

The present study determines the thermal energy which is released by the nonequilibrium beta-capture of ultrarelativistic electrons by nuclei in the partially degenerate matter of equilibrium stars in the quantum limit of the magnetic field frozen into their interiors. It is shown that, taking the number of quantum states of the partially degenerate ultrarelativistic electron gas into consideration, the thermal energy release differs quantitatively from the one due to nonequilibrium beta-capture processes in the matter of degenerate magnetic stars.

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