Asymmetric neutrino emision and formation of rapidly moving pulsars

Details Asymmetric neutrino emision and formation of rapidly moving pulsars Asymmetric neutrino emision and formation of rapidly moving pulsars

1997-07-10

arxiv.org/abs/astro-ph/9707120v1

Astron.Astrophys.Trans. 3 (1993) 287-294

Astronomy and Astrophysics

Astrophysics

8 pages, TeX, No figures. No macroses

Scientific paper

The neutron star formation during the collapse with the strong magnetic field
may lead to a mirror symmetry violation and formation of an asymmetric magnetic
field. Dependence of the week interaction cross-section on the magnetic field
strength lead to the asymmetric neutrino flux and formation of rapidly mooving
pulsars due to the recoil action as well as rapidly moving black holes.

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