Cooling of Color Superconducting Compact Stars

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dc.creatorBlaschke, David
dc.date2006-03-26
dc.date.accessioned2026-07-07T07:07:33Z
dc.date.available2026-07-07T07:07:33Z
dc.descriptionWe review the status of research on the cooling of compact stars, with emphasis on the influence of color superconducting quark matter phases. Although a consistent microscopic approach is not yet available, severe constraints on the phase structure of matter at high densities come from recent mass and cooling observations of compact stars.
dc.description11 pages, 9 figures, to be published in the Proceedings of the Johns Hopkins Workshop on 'Strong Matter in the Heaven', Budapest, August 1-3, 2005
dc.identifierhttps://arxiv.org/abs/nucl-th/0603063
dc.identifierhttp://arxiv.org/abs/nucl-th/0603063
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/110433
dc.subjectNuclear Theory
dc.titleCooling of Color Superconducting Compact Stars
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