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dc.contributor.authorYilmaz, O.en_US
dc.contributor.authorAyik, S.en_US
dc.contributor.authorAcar, F.en_US
dc.contributor.authorSaatci, S.en_US
dc.contributor.authorGokalp, A.en_US
dc.date.accessioned2015-07-28T11:56:53Z
dc.date.available2015-07-28T11:56:53Z
dc.date.issued2013en_US
dc.identifier.issn1434-6001
dc.identifier.urihttp://hdl.handle.net/11693/11110
dc.description.abstractEarly development of spinodal instabilities and density correlation functions in asymmetric nuclear matter are investigated in the stochastic extension of the Walecka-type relativistic mean field including coupling with rho meson. Calculations are performed under typical conditions encountered in heavy-ion collisions and in the crusts of neutron stars. In general, growth of instabilities occur relatively slower for increasing charge asymmetry of matter. At higher densities around rho = 0.4 rho(0) fluctuations grow relatively faster in the quantal description than those found in the semi-classical limit. Typical sizes of early condensation regions extracted from density correlation functions are consistent with those found from dispersion relations of the unstable collective modes.en_US
dc.language.isoEnglishen_US
dc.source.titleEuropean Physical Journal A : Hadrons and Nucleien_US
dc.relation.isversionofhttp://dx.doi.org/10.1140/epja/i2013-13033-8en_US
dc.subjectMean-field Theoryen_US
dc.subjectInstabilitiesen_US
dc.subjectDensityen_US
dc.titleInvestigations of spinodal dynamics in asymmetric nuclear matter within a stochastic relativistic modelen_US
dc.typeArticleen_US
dc.departmentDepartment of Physicsen_US
dc.citation.spage1en_US
dc.citation.epage11en_US
dc.citation.volumeNumber49en_US
dc.citation.issueNumber3en_US
dc.identifier.doi10.1140/epja/i2013-13033-8en_US
dc.publisherSpringer-Verlagen_US
dc.identifier.eissn1434-601X


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