Neutrino emission from compact stars and inhomogeneous color superconductivity

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

16 pages, 5 figures, revtex4 style. Version accepted for publication in Phys. Rev. D

Scientific paper

10.1103/PhysRevD.74.074005

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.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Neutrino emission from compact stars and inhomogeneous color superconductivity does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Neutrino emission from compact stars and inhomogeneous color superconductivity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Neutrino emission from compact stars and inhomogeneous color superconductivity will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-33365

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.