Vacuum Energy, EoS, and the Gluon Condensate at Finite Baryon Density in QCD

dc.creatorZhitnitsky, Ariel
dc.date2007-01-09
dc.date.accessioned2026-07-07T10:22:16Z
dc.date.available2026-07-07T10:22:16Z
dc.descriptionThe Equation of States (EoS) plays the crucial role in all studies of neutron star properties. Still, a microscopical understanding of EoS remains largely an unresolved problem. We use 2-color QCD as a model to study the dependence of vacuum energy (gluon condensate in QCD) as function of chemical potential μ\ll Λ_{QCD} where we find very strong and unexpected dependence on $μ$. We present the arguments suggesting that similar behavior may occur in 3-color QCD in the color superconducting phases. Such a study may be of importance for analysis of EoS when phenomenologically relevant parameters (within such models as MIT Bag model or NJL model) are fixed at zero density while the region of study lies at much higher densities not available for terrestrial tests.
dc.descriptionTalk at " Quark Confinement and the Hadron Spectrum VII", Ponta Delgada, September 2-7, 2006
dc.identifierhttps://arxiv.org/abs/hep-ph/0701065
dc.identifierhttp://arxiv.org/abs/hep-ph/0701065
dc.identifierAIPConf.Proc.892:518-520,2007
dc.identifierdoi:10.1063/1.2714459
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175458
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleVacuum Energy, EoS, and the Gluon Condensate at Finite Baryon Density in QCD
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