Color superconducting quark matter in compact stars
高能物理 - 唯象学
2007-05-23 v1 核理论
摘要
When nuclear matter reaches a high enough density, we expect that the nucleons will overlap so much as to lose their separate identities, and merge into quark matter. In this talk I will review some theoretical expectations and speculations about quark matter, focusing on the phenomenon of quark pair condensation (color superconductivity) and its application to compact stars.
引用
@article{arxiv.hep-ph/0110150,
title = {Color superconducting quark matter in compact stars},
author = {Mark Alford},
journal= {arXiv preprint arXiv:hep-ph/0110150},
year = {2007}
}
备注
Invited talk at the Conference on Compact Stars in the QCD Phase Diagram, Copenhagen, August 15-18, 2001. LaTeX with eps figs, 12 pages