Structure and cooling of compact stars with color superconductivity

Details Structure and cooling of compact stars with color superconductivity Structure and cooling of compact stars with color superconductivity

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jhw..confe...3b&link_type=abstract

Proceedings of the 29th Johns Hopkins Workshop on current problems in particle theory: strong matter in the heavens. 1-3 August,

Computer Science

Scientific paper

We review the status of research on the cooling of compact stars with special emphasis on possible color superconducting quark matter phases in the stars interior. Although a consistent microscopic approach is not yet available severe constraints for the phase structure of compact star matter at high densities come from recent mass and cooling observations. PACS: 12.38.Mh, 26.60.+c, 95.85.Nv, 97.60.Jd

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