1. DIGITAL.CSIC
  2. Ciencia y Tecnologías Físicas
  3. Centro de Física Miguel A. Catalán - Instituto de Estructura de la Materia (CFMAC-IEM)
  4. (CFMAC-IEM) Artículos
Por favor, use este identificador para citar o enlazar a este item: http://hdl.handle.net/10261/161174
COMPARTIR / EXPORTAR:
logo share SHARE logo core CORE BASE

Comparte tu historia
de Acceso Abierto
Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL | DATACITE

Invitar a revisión por pares abierta
Campo DC Valor Lengua/Idioma
dc.contributor.authorVogt, A.-
dc.contributor.authorSiciliano, M.-
dc.contributor.authorBirkenbach, B.-
dc.contributor.authorReiter, P.-
dc.contributor.authorGadea, Andrés-
dc.contributor.authorGelletly, W.-
dc.contributor.authorGiaz, A.-
dc.contributor.authorGörgen, A.-
dc.contributor.authorJungclaus, Andrea-
dc.contributor.authorMacchiavelli, A.O.-
dc.date.accessioned2018-02-22T08:57:41Z-
dc.date.available2018-02-22T08:57:41Z-
dc.date.issued2017-08-24-
dc.identifierdoi: 10.1103/PhysRevC.96.024321-
dc.identifierissn: 2469-9993-
dc.identifier.citationPhysical Review C 96: 024321 (2017)-
dc.identifier.urihttp://hdl.handle.net/10261/161174-
dc.descriptionA. Vogt et al. -- 14 pags., 10 figs.-
dc.description.abstractThe transitional nuclei Xe132 and Xe133 are investigated after multinucleon-transfer (MNT) and fusion-evaporation reactions. Both nuclei are populated (i) in Xe136+Pb208 MNT reactions employing the high-resolution Advanced GAmma Tracking Array (AGATA) coupled to the magnetic spectrometer PRISMA, (ii) in the Xe136+Pt198 MNT reaction employing the GAMMASPHERE spectrometer in combination with the gas-detector array CHICO, and (iii) as an evaporation residue after a Te130(α,xn)Xe134-xn fusion-evaporation reaction employing the HORUS γ-ray array at the University of Cologne. The high-spin level schemes are considerably extended above the Jπ=(7-) and (10+) isomers in Xe132 and above the 11/2- isomer in Xe133. The results are compared to the high-spin systematics of the Z=54 as well as the N=78 and N=79 chains. Furthermore, evidence is found for a long-lived (T1/2â‰1μs) isomer in Xe133 which closes a gap along the N=79 isotones. Shell-model calculations employing the SN100PN and PQM130 effective interactions reproduce the experimental findings and provide guidance to the interpretation of the observed high-spin features.-
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 UK Science and Technology Facilities Council (STFC), and from the US National Science Foundation (NSF). E.T. and N.Y. were supported by a Grant-in-Aid for Japan Society for the Promotion of Science (JSPS) Fellows (Grant No. 26.10429). A.V. and L.K. thank the Bonn-Cologne Graduate School of Physics and Astronomy (BCGS) for financial support. One of the authors (A. Gadea) has been supported by the GeneralitatValenciana, Spain, under the grant PROMETEOII/2014/019 and by the EU under the FEDER program.-
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 structures in Xe 132 and Xe 133 and evidence for isomers along the N=79 isotones-
dc.typeartículo-
dc.identifier.doi10.1103/PhysRevC.96.024321-
dc.relation.publisherversionhttps://doi.org/10.1103/PhysRevC.96.024321-
dc.date.updated2018-02-22T08:57:42Z-
dc.description.versionPeer Reviewed-
dc.language.rfc3066eng-
dc.contributor.funderJapan Society for the Promotion of Science-
dc.contributor.funderBonn-Cologne Graduate School of Physics and Astronomy-
dc.contributor.funderGeneralitat Valenciana-
dc.contributor.funderNational Science Foundation (US)-
dc.contributor.funderScience and Technology Facilities Council (UK)-
dc.contributor.funderMinisterio de Ciencia e Innovación (España)-
dc.contributor.funderEuropean Commission-
dc.contributor.funderFederal Ministry of Education and Research (Germany)-
dc.contributor.funderMinisterio de Economía y Competitividad (España)-
dc.relation.csicSí-
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000271es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003359es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100004837es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000780es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100001691es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100002347es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003329es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/100000001es_ES
dc.type.coarhttp://purl.org/coar/resource_type/c_6501es_ES
item.openairetypeartículo-
item.grantfulltextopen-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
Aparece en las colecciones: (IFIC) Artículos
(CFMAC-IEM) Artículos
Ficheros en este ítem:
Fichero Descripción Tamaño Formato
High-spin.pdf1,51 MBAdobe PDFVista previa
Visualizar/Abrir
Show simple item record

CORE Recommender

SCOPUSTM   
Citations

13
checked on 12-abr-2024

WEB OF SCIENCETM
Citations

15
checked on 26-feb-2024

Page view(s)

338
checked on 19-abr-2024

Download(s)

201
checked on 19-abr-2024

Google ScholarTM

Check

Altmetric

Altmetric


NOTA: Los ítems de Digital.CSIC están protegidos por copyright, con todos los derechos reservados, a menos que se indique lo contrario.