Modern compact star observations and the quark matter EoS
| dc.creator | Klahn, T. | |
| dc.date | 2006-11-22 | |
| dc.date.accessioned | 2026-07-07T10:38:31Z | |
| dc.date.available | 2026-07-07T10:38:31Z | |
| dc.description | 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. | |
| dc.description | 2 pages, 2 figures; Proceedings of the Erice School on 'Radioactive Beams, Nuclear Dynamics and Astrophysics' to be published in 'Prog. Part. Nucl. Phys.' | |
| dc.identifier | https://arxiv.org/abs/nucl-th/0611078 | |
| dc.identifier | http://arxiv.org/abs/nucl-th/0611078 | |
| dc.identifier | Prog.Part.Nucl.Phys.59:196-198,2007 | |
| dc.identifier | doi:10.1016/j.ppnp.2006.12.015 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/180747 | |
| dc.subject | Nuclear Theory | |
| dc.title | Modern compact star observations and the quark matter EoS | |
| dc.type | text |