Pulsar Kicks from Majoron Emission

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dc.creatorFarzan, Y.
dc.creatorGelmini, G.
dc.creatorKusenko, A.
dc.date2005-02-16
dc.date.accessioned2026-07-07T10:29:25Z
dc.date.available2026-07-07T10:29:25Z
dc.descriptionWe show that Majoron emission from a hot nascent neutron star can be anisotropic in the presence of a strong magnetic field. If Majorons carry a non-negligible fraction of the supernova energy, the resulting recoil velocity of a neutron star can explain the observed velocities of pulsars.
dc.description4 pages, no figures
dc.identifierhttps://arxiv.org/abs/hep-ph/0502150
dc.identifierhttp://arxiv.org/abs/hep-ph/0502150
dc.identifierPhys.Lett.B621:22-27,2005
dc.identifierdoi:10.1016/j.physletb.2005.06.060
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/177797
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titlePulsar Kicks from Majoron Emission
dc.typetext

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