Color Superconductivity in Compact Stars

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dc.creatorAlford, Mark
dc.creatorBowers, Jeffrey A.
dc.creatorRajagopal, Krishna
dc.date2000-09-29
dc.date.accessioned2026-07-07T10:52:09Z
dc.date.available2026-07-07T10:52:09Z
dc.descriptionAfter a brief review of the phenomena expected in cold dense quark matter, color superconductivity and color-flavor locking, we sketch some implications of recent developments in our understanding of cold dense quark matter for the physics of compact stars. We give a more detailed summary of our recent work on crystalline color superconductivity and the consequent realization that (some) pulsar glitches may originate in quark matter.
dc.description19 pages. 2 figures. To appear in the proceedings of the ECT Workshop on Neutron Star Interiors, Trento, Italy, June 2000. Shorter versions contributed to the proceedings of Strong and Electroweak Matter 2000, Marseille, France, June 2000 and to the proceedings of Strangeness 2000, Berkeley, CA, July 2000. KR was the speaker at all three meetings
dc.identifierhttps://arxiv.org/abs/hep-ph/0009357
dc.identifierhttp://arxiv.org/abs/hep-ph/0009357
dc.identifierJ.Phys.G27:541-556,2001; Lect.NotesPhys.578:235-252,2001
dc.identifierdoi:10.1088/0954-3899/27/3/335
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/185064
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleColor Superconductivity in Compact Stars
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