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Por favor, use este identificador para citar o enlazar a este item: http://hdl.handle.net/10261/142501
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dc.contributor.authorVogt, A.-
dc.contributor.authorBirkenbach, B.-
dc.contributor.authorReiter, P.-
dc.contributor.authorBlazhev, A.-
dc.contributor.authorSiciliano, M.-
dc.contributor.authorGadea, Andrés-
dc.contributor.authorGeibel, K.-
dc.contributor.authorGelletly, W.-
dc.contributor.authorGengelbach, A.-
dc.contributor.authorJungclaus, Andrea-
dc.contributor.authorKorten, W.-
dc.contributor.authorMontanari, D.-
dc.contributor.authorNapoli, D.-
dc.date.accessioned2017-01-13T12:36:46Z-
dc.date.available2017-01-13T12:36:46Z-
dc.date.issued2016-05-25-
dc.identifierdoi: 10.1103/PhysRevC.93.054325-
dc.identifierissn: 1089-490X-
dc.identifier.citationPhysical Review C - Nuclear Physics 93: 054325 (2016)-
dc.identifier.urihttp://hdl.handle.net/10261/142501-
dc.descriptionA. Vogt et al. ; 12 págs.; 9 figs.; 1 tab.-
dc.description.abstractDetailed spectroscopic information on the N∼82 nuclei is necessary to benchmark shell-model calculations in the region. The nuclear structure above long-lived isomers in Xe134 is investigated after multinucleon transfer (MNT) and actinide fission. Xenon-134 was populated as (i) a transfer product in Xe136+U238 and Xe136+Pb208 MNT reactions and (ii) as a fission product in the Xe136+U238 reaction employing the high-resolution Advanced Gamma Tracking Array (AGATA). Trajectory reconstruction has been applied for the complete identification of beamlike transfer products with the magnetic spectrometer PRISMA. The Xe136+Pt198 MNT reaction was studied with the γ-ray spectrometer GAMMASPHERE in combination with the gas detector array Compact Heavy Ion Counter (CHICO). Several high-spin states in Xe134 on top of the two long-lived isomers are discovered based on γγ-coincidence relationships and information on the γ-ray angular distributions as well as excitation energies from the total kinetic energy loss and fission fragments. The revised level scheme of Xe134 is extended up to an excitation energy of 5.832 MeV with tentative spin-parity assignments up to 16+. Previous assignments of states above the 7- isomer are revised. Latest shell-model calculations employing two different effective interactions reproduce the experimental findings and support the new spin and parity assignments.-
dc.description.sponsorshipThe research leading to these results has received funding from the German BMBF under Contract No. 05P12PKFNE TP4, from the European Union Seventh Framework Programme FP7/2007–2013 under Grant Agreement No. 262010 - ENSAR, from the Spanish Ministerio de Ciencia e Innovación under Contract No. FPA2011-29854-C04, from the Spanish Ministerio de Economía y Competitividad under Contract No. FPA2014-57196-C5, from the Bonn-Cologne Graduate School of Physics and Astronomy (BCGS), from the UK Science and Technology Facilities Council (STFC), and from the US National Science Foundation (NSF). One of the authors (A. Gadea) has been supported by the Generalitat Valenciana, Spain, under Grant No. PROMETEOII/2014/019 and EU under the FEDER program.-
dc.languageeng-
dc.publisherAmerican Physical Society-
dc.relationinfo:eu-repo/grantAgreement/EC/FP7/262010-
dc.relationinfo:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/FPA2014-57196-C5-4-P-
dc.relation.isversionofPublisher's version-
dc.rightsopenAccess-
dc.titleHigh-spin structure of Xe 134-
dc.typeartículo-
dc.identifier.doi10.1103/PhysRevC.93.054325-
dc.relation.publisherversionhttps://doi.org/10.1103/PhysRevC.93.054325-
dc.date.updated2017-01-13T12:36:50Z-
dc.description.versionPeer Reviewed-
dc.contributor.funderFederal Ministry of Education and Research (Germany)-
dc.contributor.funderEuropean Commission-
dc.contributor.funderMinisterio de Ciencia e Innovación (España)-
dc.contributor.funderMinisterio de Economía y Competitividad (España)-
dc.contributor.funderBonn-Cologne Graduate School of Physics and Astronomy-
dc.contributor.funderScience and Technology Facilities Council (UK)-
dc.contributor.funderNational Science Foundation (US)-
dc.contributor.funderGeneralitat Valenciana-
dc.relation.csicSí-
dc.identifier.funderhttp://dx.doi.org/10.13039/501100002347es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000780es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100004837es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003329es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000271es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/100000001es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003359es_ES
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.fulltextWith Fulltext-
item.openairetypeartículo-
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