Cooling of Color Superconducting Compact Stars
Nuclear Theory
2007-05-23 v1
Abstract
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.
Keywords
Cite
@article{arxiv.nucl-th/0603063,
title = {Cooling of Color Superconducting Compact Stars},
author = {David Blaschke},
journal= {arXiv preprint arXiv:nucl-th/0603063},
year = {2007}
}
Comments
11 pages, 9 figures, to be published in the Proceedings of the Johns Hopkins Workshop on 'Strong Matter in the Heaven', Budapest, August 1-3, 2005