Explanations of pulsar velocities

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dc.creatorKusenko, Alexander
dc.date1999-03-11
dc.date.accessioned2026-07-07T02:30:47Z
dc.date.available2026-07-07T02:30:47Z
dc.descriptionSeveral 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.
dc.description7 pages, revtex, epsf, two figures included, talk presented at APS Division of Particles and Fields Conference (DPF'99), UCLA, January 5-9, 1999
dc.identifierhttps://arxiv.org/abs/astro-ph/9903167
dc.identifierhttp://arxiv.org/abs/astro-ph/9903167
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13935
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleExplanations of pulsar velocities
dc.typetext

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