Cooling of Color Superconducting Compact Stars

Details Cooling of Color Superconducting Compact Stars Cooling of Color Superconducting Compact Stars

2006-03-26

arxiv.org/abs/nucl-th/0603063v1

Physics

Nuclear Physics

Nuclear Theory

11 pages, 9 figures, to be published in the Proceedings of the Johns Hopkins Workshop on 'Strong Matter in the Heaven', Budape

Scientific paper

We review the status of research on the cooling of compact stars, with
emphasis on the influence of color superconducting quark matter phases.
Although a consistent microscopic approach is not yet available, severe
constraints on the phase structure of matter at high densities come from recent
mass and cooling observations of compact stars.

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