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Diquark Condensates and Compact Star Cooling

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arxiv astro-ph/9908334 v4 pith:A2NN7UXH submitted 1999-08-30 astro-ph nucl-th

D. Blaschke , T. Klaehn , D.N. Voskresensky This is my paper
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keywords starscolorcoolingcrustdataquarkcooldown
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The effect of color superconductivity on the cooling of quark stars and neutron stars with large quark cores is investigated. Various known and new quark-neutrino processes are studied. As a result, stars being in the color flavor locked (CFL) color superconducting phase cool down extremely fast. Quark stars with no crust cool down too rapidly in disagreement with X-ray data. The cooling of stars being in the N_f =2 color superconducting (2SC) phase with a crust is compatible with existing X-ray data. Also the cooling history of stars with hypothetic pion condensate nuclei and a crust does not contradict the data.

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Cited by 1 Pith paper

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  1. Neutrino absorption in two-flavor color-superconducting quark matter

    nucl-th 2025-09 conditional novelty 7.0 of 10

    In 2SC quark matter, neutrino absorption is dominated by strange-quark capture at low temperature, and a degenerate neutrino gas at electron lepton fraction 0.1 has a mean free path of meters or less.

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