Equation of state of hot, dense stellar matter. Finite temperature nuclear Thomas-Fermi approach

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dc.contributor.authorBarranco Gómez, Manuelcat
dc.contributor.authorBuchler, Jean-Robertcat
dc.date.accessioned2010-04-22T11:56:21Z-
dc.date.available2010-04-22T11:56:21Z-
dc.date.issued1981-
dc.description.abstractThe properties of hot, dense stellar matter are investigated with a finite temperature nuclear Thomas-Fermi model.eng
dc.format.extent12 p.-
dc.format.mimetypeapplication/pdf-
dc.identifier.idgrec75989-
dc.identifier.issn0556-2813-
dc.identifier.urihttps://hdl.handle.net/2445/12235-
dc.language.isoengeng
dc.publisherThe American Physical Societyeng
dc.relation.isformatofReproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevC.24.1191cat
dc.relation.ispartofPhysical Review C, 1981, vol. 24, núm. 3, p. 1191-1202cat
dc.relation.urihttp://dx.doi.org/10.1103/PhysRevC.24.1191
dc.rights(c) The American Physical Society, 1981eng
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)
dc.subject.classificationEstructura nuclearcat
dc.subject.classificationAstrofísica nuclearcat
dc.subject.classificationEcuacions d'estatcat
dc.subject.otherNuclear structureeng
dc.subject.otherNuclear astrophysicseng
dc.subject.otherEquations of stateeng
dc.titleEquation of state of hot, dense stellar matter. Finite temperature nuclear Thomas-Fermi approacheng
dc.typeinfo:eu-repo/semantics/articleeng
dc.typeinfo:eu-repo/semantics/publishedVersion

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