Comment on "Pulsar kicks via spin-1 color superconductivity"

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dc.creatorKusenko, Alexander
dc.date2005-08-10
dc.date.accessioned2026-07-07T03:55:22Z
dc.date.available2026-07-07T03:55:22Z
dc.descriptionIn a recent paper, Phys. Rev. Lett. 94, 211101 (2005) [hep-ph/0502166], Schmitt et al. have proposed a new mechanism to explain the observed velocities of pulsars. The proposed explanation is based on anisotropic emission of neutrinos from a cooling neutron star at temperatures below 0.1 MeV, thousands of years after the supernova. However, while neutrinos are copiously produced during the first minute of the supernova explosion, at later times the neutrino emission is negligible. Therefore, the proposed mechanism is not viable.
dc.description1 page, no figures
dc.identifierhttps://arxiv.org/abs/hep-ph/0508124
dc.identifierhttp://arxiv.org/abs/hep-ph/0508124
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/44535
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleComment on "Pulsar kicks via spin-1 color superconductivity"
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