Pulsar kicks via spin-1 color superconductivity

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dc.creatorSchmitt, Andreas
dc.creatorShovkovy, Igor A.
dc.creatorWang, Qun
dc.date2005-02-18
dc.date2005-10-04
dc.date.accessioned2026-07-07T06:20:46Z
dc.date.available2026-07-07T06:20:46Z
dc.descriptionWe propose a new neutrino propulsion mechanism for neutron stars which can lead to strong velocity kicks, needed to explain the observed bimodal velocity distribution of pulsars. The spatial asymmetry in the neutrino emission is naturally provided by a stellar core containing spin-1 color-superconducting quark matter in the A phase. The neutrino propulsion mechanism switches on when the stellar core temperature drops below the transition temperature of this phase.
dc.description4 pages, 2 figures. Erratum added
dc.identifierhttps://arxiv.org/abs/hep-ph/0502166
dc.identifierhttp://arxiv.org/abs/hep-ph/0502166
dc.identifierPhys.Rev.Lett. 94 (2005) 211101
dc.identifierdoi:10.1103/PhysRevLett.94.211101
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/95408
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.subjectNuclear Theory
dc.titlePulsar kicks via spin-1 color superconductivity
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