Neutron Star Structure with Hyperons and Quarks

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dc.creatorBaldo, M.
dc.creatorBurgio, G. F.
dc.creatorSchulze, H. -J.
dc.date2003-12-17
dc.date.accessioned2026-07-07T02:11:37Z
dc.date.available2026-07-07T02:11:37Z
dc.descriptionWe discuss the high-density nuclear equation of state within the Brueckner-Hartree-Fock approach. Particular attention is paid to the effects of nucleonic three-body forces, the presence of hyperons, and the joining with an eventual quark matter phase. The resulting properties of neutron stars, in particular the mass-radius relation, are determined. It turns out that stars heavier than 1.3 solar masses contain necessarily quark matter.
dc.description21 pages, 12 figures, Talk given at the NATO Advanced Research Workshop on Superdense QCD Matter and Compact Stars, 27 Sep - 4 Oct 2003, Yerevan, Armenia
dc.identifierhttps://arxiv.org/abs/astro-ph/0312446
dc.identifierhttp://arxiv.org/abs/astro-ph/0312446
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7158
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleNeutron Star Structure with Hyperons and Quarks
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