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arXiv:astro-ph/9903167·v1·Astrophysics

Explanations of pulsar velocities

Alexander Kusenko (UCLA)🇺🇸

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Abstract

Several mechanisms based on neutrino oscillations can explain the observed motions of pulsars if the magnetic field in their interiors is of order 10^{14}-10^{15} G.

Comments: 7 pages, revtex, epsf, two figures included, talk presented at APS Division of Particles and Fields Conference (DPF'99), UCLA, January 5-9, 1999

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