Asymmetry of neutrino emission in a magnetic field and the self-acceleration of neutron stars.

Details Asymmetry of neutrino emission in a magnetic field and the self-acceleration of neutron stars. Asymmetry of neutrino emission in a magnetic field and the self-acceleration of neutron stars.

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mvsfa..30q...3l&link_type=abstract

Moskovskii Universitet, Vestnik, Seriia 3 - Fizika, Astronomiia (ISSN 0579-9392), vol. 30, Sept.-Oct. 1989, p. 3-7. In Russian.

Physics

Neutrinos, Neutron Stars, Stellar Magnetic Fields, Acceleration (Physics), Angular Distribution, Magnetic Field Configurations, Symmetry

Scientific paper

The magnetic-field-induced asymmetry of neutrino emission in a dense
nucleon medium is analyzed. The results obtained are used to analyze the
self-acceleration of a neutron star due to the recoil resulting from a
neutrino burst connected with the neutronization of the matter.

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