Anisotropic neutrino emission from beta-decays in a strong magnetic field

Journal Article · Fri Mar 01 00:00:00 EST 1985 · Sov. Astron. Lett. (Engl. Transl.); (United States)

OSTI ID:5215041

Dorofeev, O F; Rodionov, V N; Ternov, I M

Estimates are obtained for the maximum momentum that could be imparted to a collapsing star because of the anisotropic emission of neutrinos when free nucleons undergo Urca processes at high temperatures and densities in a strong magnetic field.

• Research Organization: Moscow University
• OSTI ID: 5215041
• Journal Information: Sov. Astron. Lett. (Engl. Transl.); (United States), Vol. 11:2
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
COSMIC NEUTRINOS
PARTICLE PRODUCTION
STARS
GRAVITATIONAL COLLAPSE
ANISOTROPY
BETA DECAY
ENERGY LOSSES
MAGNETIC FIELDS
NUCLEONS
POLARIZATION
BARYONS
COSMIC RADIATION
DECAY
ELEMENTARY PARTICLES
FERMIONS
HADRONS
IONIZING RADIATIONS
LEPTONS
LOSSES
MASSLESS PARTICLES
NEUTRINOS
RADIATIONS
640102* - Astrophysics & Cosmology- Stars & Quasi-Stellar
Radio & X-Ray Sources