Neutron star interiors and the equation of state of ultra-dense matter

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dc.creatorWeber, F.
dc.creatorNegreiros, R.
dc.creatorRosenfield, P.
dc.creatorCuadrat, Andreu Torres i
dc.date2006-12-05
dc.date.accessioned2026-07-07T10:21:09Z
dc.date.available2026-07-07T10:21:09Z
dc.descriptionThere has been much recent progress in our understanding of quark matter, culminating in the discovery that if such matter exists in the cores of neutron stars it ought to be in a color superconducting state. This paper explores the impact of superconducting quark matter on the properties (e.g., masses, radii, surface gravity, photon emission) of compact stars.
dc.description3 pages, 4 figures; Paper presented at the Int. Conf. on Quark Confinement and the Hadron Spectrum VII, Ponta Delgada, Acores, 2-7 September 2006; to be published by AIP
dc.identifierhttps://arxiv.org/abs/astro-ph/0612132
dc.identifierhttp://arxiv.org/abs/astro-ph/0612132
dc.identifierAIPConf.Proc.892:515-517,2007
dc.identifierdoi:10.1063/1.2714458
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175082
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectNuclear Theory
dc.titleNeutron star interiors and the equation of state of ultra-dense matter
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