Modern compact star observations and the quark matter EoS
核理论
2008-11-26 v1
摘要
A hybrid equation of state for dense matter is presented that satisfies phenomenological constraints from modern compact star observations which indicate high maximum masses of about 2 M_sun and large radii of R> 12 km. The corresponding isospin symmetric equation of state is consistent with flow data analyses of heavy-ion collisions. The transition from nuclear to two-flavor color superconducting quark matter at n approximately 0.55 fm^{-3} is almost a crossover.
引用
@article{arxiv.nucl-th/0611078,
title = {Modern compact star observations and the quark matter EoS},
author = {T. Klahn},
journal= {arXiv preprint arXiv:nucl-th/0611078},
year = {2008}
}
备注
2 pages, 2 figures; Proceedings of the Erice School on 'Radioactive Beams, Nuclear Dynamics and Astrophysics' to be published in 'Prog. Part. Nucl. Phys.'