Constraining relativistic models through heavy ion collisions

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dc.creatorMenezes, D. P.
dc.creatorProvidencia, C.
dc.creatorChiapparini, M.
dc.creatorBracco, M. E.
dc.creatorDelfino, A.
dc.creatorMalheiro, M.
dc.date2007-08-24
dc.date.accessioned2026-07-07T11:42:02Z
dc.date.available2026-07-07T11:42:02Z
dc.descriptionRelativistic models can be successfully applied to the description of compact star properties in nuclear astrophysics as well as to nuclear matter and finite nuclei properties, these studies taking place at low and moderate temperatures. Nevertheless, all results are model dependent and so far it is unclear whether some of them should be discarded. Moreover, in the regime of hot hadronic matter very few calculations exist using these relativistic models, in particular when applied to particle yields in heavy ion collisions. In the present work we comment on the known constraints that can help the selection of adequate models in this regime and investigate the main differences that arise when the particle production during a Au+Au collision at RHIC is calculated with different models.
dc.description9 pages, 1 figure, 3 tables
dc.identifierhttps://arxiv.org/abs/0708.3380
dc.identifierhttp://arxiv.org/abs/0708.3380
dc.identifierPhys.Rev.C76:064902,2007
dc.identifierdoi:10.1103/PhysRevC.76.064902
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/200742
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectNuclear Theory
dc.titleConstraining relativistic models through heavy ion collisions
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