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Neutrino emission and cooling rates of spin-one color superconductors
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Neutrino emission and cooling rates of spin-one color superconductors
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Neutrino emissivities due to direct Urca processes of several spin-one color-superconducting phases of dense quark matter are calculated. In particular, the role of anisotropies and nodes of the gap functions is analyzed. Results for the specific heat as well as for the cooling rates of the color-spin-locked, planar, polar, and {\it A} phases are presented and consequences for the physics of neutron stars are briefly discussed. Furthermore, it is shown that the {\em A} phase exhibits a helicity order, giving rise to a reflection asymmetry in the neutrino emissivity.
Forward citations
Cited by 1 Pith paper
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Neutrino absorption in two-flavor color-superconducting quark matter
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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