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Neutrino emission from compact stars and inhomogeneous color superconductivity

2006/07/31 by R. Anglani, M. Mannarelli, Giuseppe Nardulli +4 · 3 citations
Physics and Astronomy · #Astrophysics #Cold Atom Physics and Bose-Einstein Condensates #Color superconductivity #Condensed matter physics #Emissivity #Fermion #Neutrino #Nuclear physics #Pairing #Particle physics #Physics #Pulsars and Gravitational Waves Research #Quantum Chromodynamics and Particle Interactions #Quantum chromodynamics #Quantum mechanics #Quark #Quark star #Stars #Strange matter #Superconductivity #hep-ph

paper · pdf · doi:10.1103/physrevd.74.074005

published as Phys.Rev. D74 (2006) 074005 · 16 pages, 5 figures, revtex4 style. Version accepted for publication in Phys. Rev. D

arxiv created 2006/09/25 · openalex publication_date 2006/10/11 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We discuss specific heat and neutrino emissivity due to direct Urca processes for quark matter in the color superconductive Larkin-Ovchinnikov-Fulde-Ferrell (LOFF) phase of quantum chromodynamics. We assume that the three light quarks u, d, s are in a color and electrically neutral state and interact by a four-fermion Nambu--Jona-Lasinio coupling. We study a LOFF state characterized by a single plane wave for each pairing. From the evaluation of neutrino emissivity and fermionic specific heat, the cooling rate of simplified models of compact stars with a quark core in the LOFF state is estimated.

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