Neutron stars and quark matter

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dc.creatorBaym, Gordon
dc.date2006-12-05
dc.date.accessioned2026-07-07T10:22:40Z
dc.date.available2026-07-07T10:22:40Z
dc.descriptionRecent observations of neutron star masses close to the maximum predicted by nucleonic equations of state begin to challenge our understanding of dense matter in neutron stars, and constrain the possible presence of quark matter in their deep interiors.
dc.descriptionTo be published in the proceedings of Quark Confinement and the Hadron Spectrum VII, Sept. 2006, Ponta Delgada, Azores. 7 pages, 3 figures, aiproc
dc.identifierhttps://arxiv.org/abs/nucl-th/0612021
dc.identifierhttp://arxiv.org/abs/nucl-th/0612021
dc.identifierAIPConf.Proc.892:8-14,2007
dc.identifierdoi:10.1063/1.2714340
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175592
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleNeutron stars and quark matter
dc.typetext

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