Color Superconductivity and Blinking Proto-Neutron Stars

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dc.creatorCarter, G. W.
dc.date2001-11-27
dc.date.accessioned2026-07-07T03:45:56Z
dc.date.available2026-07-07T03:45:56Z
dc.descriptionIf quark matter exists in the cores of neutron stars, it is most likely color superconducting. Thus a phase transition from free to paired quark matter might occur during the first minute of proto-neutron star evolution. In this talk I discuss how critical behavior of the medium will modify neutrino diffusion, possibly leading to a short temporal variation in the neutrino signal detected on Earth.
dc.description6 pages, 4 figures, includes econfmacros.tex; talk at "Compact Stars in the QCD Phase Diagram", Nordita, 15-18 August 2001
dc.identifierhttps://arxiv.org/abs/hep-ph/0111353
dc.identifierhttp://arxiv.org/abs/hep-ph/0111353
dc.identifiereConf C010815 (2002) 149-154
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/41108
dc.subjectHigh Energy Physics - Phenomenology
dc.titleColor Superconductivity and Blinking Proto-Neutron Stars
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