Neutrino Emission From Inhomogeneous Pion Condensed Quark Matter

Details Neutrino Emission From Inhomogeneous Pion Condensed Quark Matter Neutrino Emission From Inhomogeneous Pion Condensed Quark Matter

2007-10-19

arxiv.org/abs/0710.3634v3

Int.J.Mod.Phys.E17:1906-1916,2008

Physics

High Energy Physics

High Energy Physics - Phenomenology

10 pages, 5 figures. A new reference added,published version

Scientific paper

10.1142/S021830130801088X

It is believed that quark matter can exist in neutron star interior if the baryon density is high enough. When there is a large isospin density, quark matter could be in a pion condensed phase. We compute neutrino emission from direct Urca processes in such a phase, particularly in the inhomogeneous Larkin-Ovchinnikov-Fulde-Ferrell (LOFF) states. The neutrino emissivity and specific heat are obtained, from which the cooling rate is estimated.

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