Pulsar kicks from neutrino oscillations

Simple item page
dc.creatorKusenko, Alexander
dc.creatorSegre, Gino
dc.date1998-11-10
dc.date1998-11-10
dc.date.accessioned2026-07-07T10:31:48Z
dc.date.available2026-07-07T10:31:48Z
dc.descriptionNeutrino oscillations can explain the observed motion of pulsars. We show that two different models of neutrino emission from a cooling neutron star are in good quantitative agreement and predict the same order of magnitude for the pulsar kick velocity, consistent with the data.
dc.descriptionrevtex; 4 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/9811144
dc.identifierhttp://arxiv.org/abs/astro-ph/9811144
dc.identifierPhys.Rev.D59:061302,1999
dc.identifierdoi:10.1103/PhysRevD.59.061302
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178542
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titlePulsar kicks from neutrino oscillations
dc.typetext

Files

Collections

arXiv