Neutrino Emission From Direct Urca Processes in Pion Condensed Quark Matter

Details Neutrino Emission From Direct Urca Processes in Pion Condensed Quark Matter Neutrino Emission From Direct Urca Processes in Pion Condensed Quark Matter

2007-06-29

arxiv.org/abs/0706.4381v2

Phys.Rev.D76:094008,2007

Physics

High Energy Physics

High Energy Physics - Phenomenology

12 pages,6 figures, published version

Scientific paper

10.1103/PhysRevD.76.094008

We study neutrino emission from direct Urca processes in pion condensed quark matter. In compact stars with high baryon density, the emission is dominated by the gapless modes of the pion condensation which leads to an enhanced emissivity. While for massless quarks the enhancement is not remarkable, the emissivity is significantly larger and the cooling of the condensed matter is considerably faster than that in normal quark matter when the mass difference between $u$- and $d$-quarks is sizable.

Affiliated with

Also associated with

No associations

Rating

Neutrino Emission From Direct Urca Processes in Pion Condensed Quark Matter 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 Direct Urca Processes in Pion Condensed Quark Matter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Neutrino Emission From Direct Urca Processes in Pion Condensed Quark Matter will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-681695