Color superconducting quark matter in compact stars

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dc.creatorAlford, Mark
dc.date2001-10-11
dc.date.accessioned2026-07-07T03:45:31Z
dc.date.available2026-07-07T03:45:31Z
dc.descriptionWhen nuclear matter reaches a high enough density, we expect that the nucleons will overlap so much as to lose their separate identities, and merge into quark matter. In this talk I will review some theoretical expectations and speculations about quark matter, focusing on the phenomenon of quark pair condensation (color superconductivity) and its application to compact stars.
dc.descriptionInvited talk at the Conference on Compact Stars in the QCD Phase Diagram, Copenhagen, August 15-18, 2001. LaTeX with eps figs, 12 pages
dc.identifierhttps://arxiv.org/abs/hep-ph/0110150
dc.identifierhttp://arxiv.org/abs/hep-ph/0110150
dc.identifiereConf C010815 (2002) 137-148
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/40952
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectNuclear Theory
dc.titleColor superconducting quark matter in compact stars
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