Cooling of a Compact Star with a LOFF Matter Core

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dc.creatorAnglani, Roberto
dc.date2006-10-30
dc.date.accessioned2026-07-07T12:16:51Z
dc.date.available2026-07-07T12:16:51Z
dc.descriptionSpecific heat and neutrino emissivity due to direct URCA processes for quark matter in the color superconductive Larkin-Ovchinnikov-Fulde-Ferrell (LOFF) phase of Quantum-Chromodynamics have been evaluated. The cooling rate of simplified models of compact stars with a LOFF matter core is estimated.
dc.description3 pages, 1 figure, to appear in the proceedings of the Helmoltz International Summer School of Theoretical Physics on Dense Matter in Heavy Ion Collisions and Astrophysics, JINR, Dubna, Russia, 21 Aug - 1 Sep 2006
dc.identifierhttps://arxiv.org/abs/hep-ph/0610404
dc.identifierhttp://arxiv.org/abs/hep-ph/0610404
dc.identifierPhys.Part.Nucl.39:1167-1169,2008
dc.identifierdoi:10.1134/S1063779608070332
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/211936
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleCooling of a Compact Star with a LOFF Matter Core
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