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Please use this identifier to cite or link to this item: https://hdl.handle.net/2445/10989
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dc.contributor.authorDe, J. N.cat
dc.contributor.authorViñas Gausí, Xaviercat
dc.contributor.authorPatra, S. K.cat
dc.contributor.authorCentelles Aixalà, Mariocat
dc.date.accessioned2010-01-28T17:01:55Z-
dc.date.available2010-01-28T17:01:55Z-
dc.date.issued2001cat
dc.identifier.issn0556-2813cat
dc.identifier.urihttps://hdl.handle.net/2445/10989-
dc.description.abstractIn the Thomas-Fermi model, calculations are presented for nuclei beyond the nuclear drip line at zero temperature. These nuclei are in equilibrium by the presence of an external gas, as may be envisaged in the astrophysical scenario. We find that there is a limiting asymmetry beyond which these nuclei can no longer be made stable.eng
dc.format.extent4 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.64.057306cat
dc.relation.ispartofPhysical Review C, 2001, vol. 64, núm. 5, p. 057306-1-057306-4ca
dc.relation.urihttp://dx.doi.org/10.1103/PhysRevC.64.057306-
dc.rights(c) The American Physical Society, 2001cat
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)-
dc.subject.classificationEstructura nuclearcat
dc.subject.classificationFísica nuclearcat
dc.subject.otherNuclear structureeng
dc.subject.otherNuclear physicseng
dc.titleNuclei beyond the drip lineeng
dc.typeinfo:eu-repo/semantics/articleeng
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.identifier.idgrec187584cat
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
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