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arXiv · hep-ph/0303073

Impact of CFL Quark Matter on the Cooling of Compact Stars

Igor A. Shovkovy·Paul J. Ellis
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Abstract

The cooling mechanism of compact stars with quark cores in the color-flavor locked phase is discussed. It is argued that the high thermal conductivity of the quark core plays a key role in the stellar cooling. It implies that the cooling time of compact stars with color-flavor locked quark cores is similar to that of ordinary neutron stars, unless the star is almost completely made of color-flavor locked quark matter.

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BibTeXRIS

Igor A. Shovkovy, Paul J. Ellis. 2003-03-10. Impact of CFL Quark Matter on the Cooling of Compact Stars. https://doi.org/10.1142/9789812795120_0019

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