Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/11001
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dc.contributor.authorSil, Tapascat
dc.contributor.authorSamaddar, S. K.cat
dc.contributor.authorViñas Gausí, Xaviercat
dc.contributor.authorCentelles Aixalà, Mariocat
dc.contributor.authorAgrawal, B. K.cat
dc.contributor.authorPatra, S. K.cat
dc.date.accessioned2010-01-28T17:16:21Z-
dc.date.available2010-01-28T17:16:21Z-
dc.date.issued2002cat
dc.identifier.issn0556-2813cat
dc.identifier.urihttp://hdl.handle.net/2445/11001-
dc.description.abstractStability of nuclei beyond the drip lines in the presence of an enveloping gas of nucleons and electrons, as prevailing in the inner crust of a neutron star, is studied in the temperature-dependent Thomas-Fermi framework. A limiting asymmetry in the isospin space beyond which nuclei cannot exist emerges from the calculations. The ambient conditions such as temperature, baryon density, and neutrino concentration under which these exotic nuclear systems can be formed are studied in some detail.eng
dc.format.extent9 p.cat
dc.format.mimetypeapplication/pdfeng
dc.language.isoengeng
dc.publisherThe American Physical Societycat
dc.relation.isformatofReproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevC.66.045803cat
dc.relation.ispartofPhysical Review C, 2002, vol. 66, núm. 4, p. 045803-1-045803-9cat
dc.relation.urihttp://dx.doi.org/10.1103/PhysRevC.66.045803-
dc.rights(c) The American Physical Society, 2002cat
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)-
dc.subject.classificationAstrofísica nuclearcat
dc.subject.classificationEstructura nuclearcat
dc.subject.otherNuclear astrophysicseng
dc.subject.otherNuclear structureeng
dc.titleIsospin-rich nuclei in neutron star mattereng
dc.typeinfo:eu-repo/semantics/articleeng
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.identifier.idgrec508593cat
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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