Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/10967
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dc.contributor.authorCentelles Aixalà, Mariocat
dc.contributor.authorViñas Gausí, Xaviercat
dc.contributor.authorSchuck, Petercat
dc.date.accessioned2010-01-28T16:28:42Z-
dc.date.available2010-01-28T16:28:42Z-
dc.date.issued1996cat
dc.identifier.issn0556-2813cat
dc.identifier.urihttp://hdl.handle.net/2445/10967-
dc.description.abstractThe difficulties arising in the calculation of the nuclear curvature energy are analyzed in detail, especially with reference to relativistic models. It is underlined that the implicit dependence on curvature of the quantal wave functions is directly accessible only in a semiclassical framework. It is shown that also in the relativistic models quantal and semiclassical calculations of the curvature energy are in good agreement.eng
dc.format.extent4 p.cat
dc.format.mimetypeapplication/pdfeng
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/cat
dc.relation.ispartofPhysical Review C, 1996, vol. 53, núm. 2, p. 1018-1021eng
dc.rights(c) The American Physical Society, 1996eng
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)-
dc.subject.classificationEstructura nuclearcat
dc.subject.classificationRelativitat (Física)cat
dc.subject.classificationModels nuclearscat
dc.subject.otherNuclear structureeng
dc.subject.otherRelativity (Physics)eng
dc.subject.otherNuclear modelseng
dc.titleNuclear curvature energy in relativistic modelseng
dc.typeinfo:eu-repo/semantics/articleeng
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.identifier.idgrec112677cat
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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