Cooling of a New Born Compact Star with QCD Phase Transition

Details Cooling of a New Born Compact Star with QCD Phase Transition Cooling of a New Born Compact Star with QCD Phase Transition

2004-05-29

arxiv.org/abs/astro-ph/0405601v2

Phys.Rev. D70 (2004) 063004

Astronomy and Astrophysics

Astrophysics

12 pages, 11 figures, 4 tables. Deleted a section related to static structure.Very minor updated the results without changing

Scientific paper

10.1103/PhysRevD.70.063004

We study the cooling behaviour of an isolated strange quark star, using an equation of state derived from perturbative QCD up to second order in strong coupling constant, and we compare it with that of a neutron star. After an initial rapid cooling, a quark star may undergo the QCD phase transition to become a neutron star. We propose several signatures for such a scenario: a large amount of energy can be released due to latent heat, a long duration $\gamma$-ray source, and a second neutrino burst after a supernova explosion.

Affiliated with

Also associated with

No associations

Rating

Cooling of a New Born Compact Star with QCD Phase Transition 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 Cooling of a New Born Compact Star with QCD Phase Transition, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cooling of a New Born Compact Star with QCD Phase Transition will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-136547