Neutrino emission and cooling rates of spin-one color superconductors

Details Neutrino emission and cooling rates of spin-one color superconductors Neutrino emission and cooling rates of spin-one color superconductors

2005-10-26

arxiv.org/abs/hep-ph/0510347v2

Phys.Rev. D73 (2006) 034012

Physics

High Energy Physics

High Energy Physics - Phenomenology

25 pages, 6 figures, v2: minor modifications, several references added, version to appear in Phys. Rev. D

Scientific paper

10.1103/PhysRevD.73.034012

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.

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