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Symmetry coefficients and incompressibility of clusterized supernova matter

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dc.contributor.authorSamaddar, S. K.
dc.contributor.authorDe, J. N.
dc.contributor.authorViñas Gausí, Xavier
dc.contributor.authorCentelles Aixalà, Mario
dc.date.accessioned2013-08-30T10:33:57Z
dc.date.available2013-08-30T10:33:57Z
dc.date.issued2009
dc.date.updated2013-08-30T10:33:58Z
dc.description.abstractThe symmetry energy coefficients, incompressibility, and single-particle and isovector potentials of clusterized dilute nuclear matter are calculated at different temperatures employing the S-matrix approach to the evaluation of the equation of state. Calculations have been extended to understand the aforesaid properties of homogeneous and clusterized supernova matter in the subnuclear density region. A comparison of the results in the S-matrix and mean-field approach reveals some subtle differences in the density and temperature region we explore.
dc.format.extent11 p.
dc.format.mimetypeapplication/pdf
dc.identifier.idgrec569796
dc.identifier.issn0556-2813
dc.identifier.urihttps://hdl.handle.net/2445/45448
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.isformatofReproducció del document publicat a: http://dx.doi.org/10.1103/PhysRevC.80.03580
dc.relation.ispartofPhysical Review C, 2009, vol. 80, num. 3, p. 035803-1-035803-11
dc.relation.urihttp://dx.doi.org/10.1103/PhysRevC.80.03580
dc.rights(c) American Physical Society, 2009
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)
dc.subject.classificationSupernoves
dc.subject.classificationConstitució de la matèria
dc.subject.classificationFísica nuclear
dc.subject.classificationAstrofísica
dc.subject.otherSupernovae
dc.subject.otherConstitution of matter
dc.subject.otherNuclear physics
dc.subject.otherAstrophysics
dc.titleSymmetry coefficients and incompressibility of clusterized supernova matter
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion

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