Neutrinos in dense quark matter and cooling of compact stars
arXiv:0912.3075 · doi:10.1016/j.ppnp.2009.12.068
Abstract
We discuss that observational constraints on neutrino cooling processes may restrict the spectrum of quark matter phases admissible for compact star interiors.
3 pages, contribution to International School of Nuclear Physics on "Neutrinos in Cosmology, in Astro-, Particle- and Nuclear Physics, Erice-Sicily, September 16-24, 2009