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arXiv · hep-ph/0610404

Cooling of a Compact Star with a LOFF Matter Core

Roberto Anglani
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Abstract

Specific 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.

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Roberto Anglani. 2006-10-30. Cooling of a Compact Star with a LOFF Matter Core. https://doi.org/10.1134/s1063779608070332

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