Modern compact star observations and the quark matter EoS

Details Modern compact star observations and the quark matter EoS Modern compact star observations and the quark matter EoS

2006-11-22

arxiv.org/abs/nucl-th/0611078v1

Prog.Part.Nucl.Phys.59:196-198,2007

Physics

Nuclear Physics

Nuclear Theory

2 pages, 2 figures; Proceedings of the Erice School on 'Radioactive Beams, Nuclear Dynamics and Astrophysics' to be published

Scientific paper

10.1016/j.ppnp.2006.12.015

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.

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