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dc.contributor.authorRodríguez-Tajes, C.-
dc.contributor.authorGarcía Borge, María José-
dc.contributor.authorPascual-Izarra, C.-
dc.contributor.authorPerea, Ángel-
dc.contributor.authorTengblad, Olof-
dc.contributor.authorZhukov, M.V.-
dc.date.accessioned2012-11-16T12:20:24Z-
dc.date.available2012-11-16T12:20:24Z-
dc.date.issued2011-
dc.identifierdoi: 10.1103/PhysRevC.83.064313-
dc.identifierissn: 0556-2813-
dc.identifier.citationPhysical Review C - Nuclear Physics 83 (2011)-
dc.identifier.urihttp://hdl.handle.net/10261/60480-
dc.description.abstractOne-neutron knockout data for N18-22 are analyzed in the eikonal approximation of the Glauber model. The role of the s-d shell and the crossing of the N=14 neutron subshell are discussed. Of particular interest is the nucleus N22, where the knockout data provide a sensitive experimental test for a possible halo structure of its ground state. The observation of a narrow momentum distribution of the N21 fragments, together with an essential 1s 1/2 contribution needed to describe the observed longitudinal- momentum distribution, allow the firm conclusion that the ground state of N22 is a well-developed nuclear halo. The results also show that the N=14 subshell in N22 is somewhat reduced as compared to that of O23. © 2011 American Physical Society.-
dc.description.sponsorshipThis work was supported by: GSI, via Hochschulzusammenarbeitsvereinbarungen under Contracts No. DA RICK, No. OF ELZ, and No. MZ KRAK; German BMBF; the DFG Cluster of Excellence, Origin and Structure of the Universe; FBR under Contract No. 08-02-012244; EC under Contract No. ERBCHGE-CT92-003; Ministerio de Ciencia e Innovacion under Project No. FPA2009-14604-602-01; ´ Ministerio de Educacion under Grant No. FPU-AP2005-3308, ´ and the Galician Conseller´ıa de Educacion e Ordenaci ´ on´ Universitaria, Consolidacion e Estructuraci ´ on de Unidades ´ Competitivas 2010/57.-
dc.language.isoeng-
dc.publisherAmerican Physical Society-
dc.rightsopenAccess-
dc.titleStructure of N22 and the N=14 subshell-
dc.typeartículo-
dc.identifier.doi10.1103/PhysRevC.83.064313-
dc.date.updated2012-11-16T12:20:24Z-
dc.description.versionPeer Reviewed-
dc.type.coarhttp://purl.org/coar/resource_type/c_6501es_ES
item.grantfulltextopen-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.languageiso639-1en-
item.fulltextWith Fulltext-
item.openairetypeartículo-
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