Neutrino emissivity and bulk viscosity of iso-CSL quark matter in neutron stars

Details Neutrino emissivity and bulk viscosity of iso-CSL quark matter in neutron stars Neutrino emissivity and bulk viscosity of iso-CSL quark matter in neutron stars

2007-10-27

arxiv.org/abs/0710.5243v1

AIPConf.Proc.964:290-295,2007

Physics

High Energy Physics

High Energy Physics - Phenomenology

6 pages, 2 figures, to appear in the proceedings of QCD@Work 2007, Martina Franca (Italy)

Scientific paper

10.1063/1.2823866

We present results for neutrino emissivities and bulk viscosities of a two-flavor color superconducting quark matter phase with isotropic color-spin-locked (iso-CSL) single-flavor pairing which fulfill the constraints on quark matter derived from cooling and rotational evolution of compact stars. We compare with results for the phenomenologically successful, but yet heuristic 2SC+X phase.

Affiliated with

Also associated with

No associations

Rating

Neutrino emissivity and bulk viscosity of iso-CSL quark matter in neutron stars 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 emissivity and bulk viscosity of iso-CSL quark matter in neutron stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Neutrino emissivity and bulk viscosity of iso-CSL quark matter in neutron stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-469146