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dc.date.accessioned2020-05-20T18:34:30Z
dc.date.available2020-05-20T18:34:30Z
dc.date.created2020-01-15T09:21:27Z
dc.date.issued2019
dc.identifier.citationKaya, L. Görgen, Andreas Sahin, Eda et al, et al, et al . Isomer spectroscopy in 133Ba and high-spin structure of 134Ba. Physical Review C. 2019, 100
dc.identifier.urihttp://hdl.handle.net/10852/76017
dc.description.abstractThe transitional nuclei 134 Ba and 133 Ba are investigated after multinucleon transfer employing the high-resolution Advanced GAmma Tracking Array coupled to the magnetic spectrometer PRISMA at the Laboratori Nazionali di Legnaro, Italy, and after fusion-evaporation reaction at the FN tandem accelerator of the University of Cologne, Germany. The Jπ = 19 / 2 + state at 1942 keV in 133 Ba is identified as an isomer with a half-life of 66.6 ( 20 ) ns corresponding to a B(E1) value of 7.7 ( 4 ) × 10 − 6 e 2 fm 2 for the Jπ = 19 / 2 + to Jπ = 19 / 2 − transition. The level scheme of 134 Ba above the Jπ = 10 + isomer is extended to approximately 6 MeV. A pronounced backbending is observed at ℏ ω = 0.38 MeV along the positive-parity yrast band. The results are compared to the high-spin systematics of the Z=56 isotopes. Large-scale shell-model calculations employing the GCN50:82, SN100PN, SNV, PQM130, Realistic SM, and EPQQM interactions reproduce the experimental findings and elucidate the structure of the high-spin states. The shell-model calculations employing the GCN50:82 and PQM130 interactions reproduce alignment properties and provide detailed insight into the microscopic origin of this phenomenon in transitional 134 Ba .en_US
dc.languageEN
dc.publisherAmerican Physical Society
dc.titleIsomer spectroscopy in 133Ba and high-spin structure of 134Baen_US
dc.typeJournal articleen_US
dc.creator.authorKaya, L.
dc.creator.authorGörgen, Andreas
dc.creator.authorSahin, Eda
dc.creator.authoret al, et al, et al
cristin.unitcode185,15,4,20
cristin.unitnameKjerne- og energifysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1773315
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Physical Review C&rft.volume=100&rft.spage=&rft.date=2019
dc.identifier.jtitlePhysical Review C
dc.identifier.volume100
dc.identifier.issue2
dc.identifier.doihttps://doi.org/10.1103/PhysRevC.100.024323
dc.identifier.urnURN:NBN:no-79135
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn2469-9985
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/76017/1/PhysRevC.100.024323.pdf
dc.type.versionPublishedVersion
cristin.articleid024323
dc.relation.projectNFR/263030


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