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Neutrino luminosity of magnetic stars in renormalizable models

Journal Article · · Astrophysics (Engl. Transl.); (United States)
DOI:https://doi.org/10.1007/BF01004380· OSTI ID:6865814

The cross section of neutrino photoproduction is calculated, and the contribution of this process to the neutrino luminosity of magnetic stars is estimated. Calculations were made using the renormalizable Weinberg-Salam field theory model.

OSTI ID:
6865814
Journal Information:
Astrophysics (Engl. Transl.); (United States), Journal Name: Astrophysics (Engl. Transl.); (United States) Vol. 15:3; ISSN ATPYA
Country of Publication:
United States
Language:
English

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Related Subjects

640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
BASIC INTERACTIONS
COSMIC NEUTRINOS
COSMIC RADIATION
CROSS SECTIONS
ELECTROMAGNETIC INTERACTIONS
ELEMENTARY PARTICLES
FERMIONS
FIELD THEORIES
INTERACTIONS
IONIZING RADIATIONS
LEPTONS
LUMINOSITY
MAGNETIC STARS
MASSLESS PARTICLES
NEUTRINOS
NEUTRON STARS
OPTICAL PROPERTIES
PARTICLE PRODUCTION
PHOTOPRODUCTION
PHYSICAL PROPERTIES
RADIATIONS
STARS