Investigations of instabilities in nuclear matter in stochastic relativistic models

dc.authorid0000-0002-8290-434X
dc.contributor.authorAyık, S.
dc.contributor.authorYılmaz, O.
dc.contributor.authorAcar, F.
dc.contributor.authorDanışman, B.
dc.contributor.authorEr, Nuray
dc.date.accessioned2021-06-23T19:28:02Z
dc.date.available2021-06-23T19:28:02Z
dc.date.issued2011
dc.departmentBAİBÜ, Fen Edebiyat Fakültesi, Fizik Bölümüen_US
dc.description.abstractThe spinodal instabilities for symmetric nuclear matter at finite temperature are studied within different relativistic mean-field models in the semi-classical approximation and the relativistic results are compared with Skyrme type non-relativistic calculations. Qualitatively similar results appear in the unstable response of the system in both non-relativistic and relativistic descriptions. Furthermore, the early growth of baryon, scalar and current density correlation functions are calculated for hot symmetric nuclear matter. (C) 2011 Elsevier B.V. All rights reserved.en_US
dc.identifier.doi10.1016/j.nuclphysa.2011.04.004
dc.identifier.endpage86en_US
dc.identifier.issn0375-9474
dc.identifier.issue1en_US
dc.identifier.scopus2-s2.0-79957790662en_US
dc.identifier.scopusqualityQ2en_US
dc.identifier.startpage73en_US
dc.identifier.urihttps://doi.org/10.1016/j.nuclphysa.2011.04.004
dc.identifier.urihttps://hdl.handle.net/20.500.12491/6939
dc.identifier.volume859en_US
dc.identifier.wosWOS:000292430300007en_US
dc.identifier.wosqualityQ3en_US
dc.indekslendigikaynakWeb of Scienceen_US
dc.indekslendigikaynakScopusen_US
dc.institutionauthorEr, Nuray
dc.language.isoenen_US
dc.publisherElsevier Science Bven_US
dc.relation.ispartofNuclear Physics Aen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.subjectSpinodal Instabilityen_US
dc.subjectStochastic Mean-fielden_US
dc.titleInvestigations of instabilities in nuclear matter in stochastic relativistic modelsen_US
dc.typeArticleen_US

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