dc.date.accessioned | 2020-05-20T18:34:30Z | |
dc.date.available | 2020-05-20T18:34:30Z | |
dc.date.created | 2020-01-15T09:21:27Z | |
dc.date.issued | 2019 | |
dc.identifier.citation | Kaya, 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.uri | http://hdl.handle.net/10852/76017 | |
dc.description.abstract | The 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.language | EN | |
dc.publisher | American Physical Society | |
dc.title | Isomer spectroscopy in 133Ba and high-spin structure of 134Ba | en_US |
dc.type | Journal article | en_US |
dc.creator.author | Kaya, L. | |
dc.creator.author | Görgen, Andreas | |
dc.creator.author | Sahin, Eda | |
dc.creator.author | et al, et al, et al | |
cristin.unitcode | 185,15,4,20 | |
cristin.unitname | Kjerne- og energifysikk | |
cristin.ispublished | true | |
cristin.fulltext | original | |
cristin.qualitycode | 1 | |
dc.identifier.cristin | 1773315 | |
dc.identifier.bibliographiccitation | info: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.jtitle | Physical Review C | |
dc.identifier.volume | 100 | |
dc.identifier.issue | 2 | |
dc.identifier.doi | https://doi.org/10.1103/PhysRevC.100.024323 | |
dc.identifier.urn | URN:NBN:no-79135 | |
dc.type.document | Tidsskriftartikkel | en_US |
dc.type.peerreviewed | Peer reviewed | |
dc.source.issn | 2469-9985 | |
dc.identifier.fulltext | Fulltext https://www.duo.uio.no/bitstream/handle/10852/76017/1/PhysRevC.100.024323.pdf | |
dc.type.version | PublishedVersion | |
cristin.articleid | 024323 | |
dc.relation.project | NFR/263030 | |