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dc.date.accessioned2020-05-20T18:35:53Z
dc.date.available2020-05-20T18:35:53Z
dc.date.created2020-01-15T11:44:17Z
dc.date.issued2019
dc.identifier.citationKaya, L. Vogt, A Reiter, P Müller-Gatermann, C. Gargano, A Coraggio, L Itaco, N Blazhev, A Arnswald, K. Bazzacco, D Birkenbach, B Bracco, A Bruyneel, B Corradi, L Crespi, F.C.L. De Angelis, G Droste, M. Eberth, J Farnea, E Fioretto, E Fransen, C Gadea, A Giaz, A Görgen, Andreas Gottardo, A Hadynska-Klek, Katarzyna Hess, H Hetzenegger, R. Hirsch, R John, P.R. Jolie, J Jungclaus, A Korten, W Leoni, S Lewandowski, L. Lunardi, S Menegazzo, R Mengoni, D Michelagnoli, C Mijatovic, T Montagnoli, G Montanari, D Napoli, D Podolyák, Zs Pollarolo, G Recchia, F Rosiak, D. Saed-Samii, N. Sahin, Eda Siciliano, M Scarlassara, F Seidlitz, M Söderström, P.-A. Stefanini, AM Stezowski, O Szilner, S Szpak, B Ur, C Valiente-Dobón, JJ Weinert, M Wolf, K Zell, KO . Identification of high-spin proton configurations in 136Ba and 137Ba. Physical Review C. 2019, 99(1)
dc.identifier.urihttp://hdl.handle.net/10852/76018
dc.description.abstractThe high-spin structures of 136 Ba and 137 Ba are investigated after multinucleon-transfer (MNT) and fusion-evaporation reactions. 136 Ba is populated in a 136 Xe + 238 U MNT reaction employing the high-resolution Advanced GAmma Tracking Array (AGATA) coupled to the magnetic spectrometer PRISMA at the Laboratori Nazionali di Legnaro, Italy, and in two 9Be + 130 Te fusion-evaporation reactions using the High-efficiency Observatory for γ -Ray Unique Spectroscopy (HORUS) at the FN tandem accelerator of the University of Cologne, Germany. Furthermore, both isotopes are populated in an elusive reaction channel in the 11 B + 130 Te fusion-evaporation reaction utilizing the HORUS γ -ray array. The level scheme above the Jπ = 10 + isomer in 136 Ba is revised and extended up to an excitation energy of approximately 5.5 MeV. From the results of angular-correlation measurements, the Ex=3707 - and Ex=4920 -keV states are identified as the bandheads of positive- and negative-parity cascades. While the high-spin regimes of both 132 Te and 134 Xe are characterized by high-energy 12 + → 10 + transitions, the 136 Ba E 2 ground-state band is interrupted by negative-parity states only a few hundred keV above the Jπ = 10 + isomer. Furthermore, spins are established for several hitherto unassigned high-spin states in 137 Ba . The new results close a gap along the high-spin structure of N<82 Ba isotopes. Experimental results are compared to large-scale shell-model calculations employing the GCN50:82, Realistic SM, PQM130, and SN100PN interactions. The calculations suggest that the bandheads of the positive-parity bands in both isotopes are predominantly of proton character.en_US
dc.languageEN
dc.publisherAmerican Physical Society
dc.titleIdentification of high-spin proton configurations in 136Ba and 137Baen_US
dc.typeJournal articleen_US
dc.creator.authorKaya, L.
dc.creator.authorVogt, A
dc.creator.authorReiter, P
dc.creator.authorMüller-Gatermann, C.
dc.creator.authorGargano, A
dc.creator.authorCoraggio, L
dc.creator.authorItaco, N
dc.creator.authorBlazhev, A
dc.creator.authorArnswald, K.
dc.creator.authorBazzacco, D
dc.creator.authorBirkenbach, B
dc.creator.authorBracco, A
dc.creator.authorBruyneel, B
dc.creator.authorCorradi, L
dc.creator.authorCrespi, F.C.L.
dc.creator.authorDe Angelis, G
dc.creator.authorDroste, M.
dc.creator.authorEberth, J
dc.creator.authorFarnea, E
dc.creator.authorFioretto, E
dc.creator.authorFransen, C
dc.creator.authorGadea, A
dc.creator.authorGiaz, A
dc.creator.authorGörgen, Andreas
dc.creator.authorGottardo, A
dc.creator.authorHadynska-Klek, Katarzyna
dc.creator.authorHess, H
dc.creator.authorHetzenegger, R.
dc.creator.authorHirsch, R
dc.creator.authorJohn, P.R.
dc.creator.authorJolie, J
dc.creator.authorJungclaus, A
dc.creator.authorKorten, W
dc.creator.authorLeoni, S
dc.creator.authorLewandowski, L.
dc.creator.authorLunardi, S
dc.creator.authorMenegazzo, R
dc.creator.authorMengoni, D
dc.creator.authorMichelagnoli, C
dc.creator.authorMijatovic, T
dc.creator.authorMontagnoli, G
dc.creator.authorMontanari, D
dc.creator.authorNapoli, D
dc.creator.authorPodolyák, Zs
dc.creator.authorPollarolo, G
dc.creator.authorRecchia, F
dc.creator.authorRosiak, D.
dc.creator.authorSaed-Samii, N.
dc.creator.authorSahin, Eda
dc.creator.authorSiciliano, M
dc.creator.authorScarlassara, F
dc.creator.authorSeidlitz, M
dc.creator.authorSöderström, P.-A.
dc.creator.authorStefanini, AM
dc.creator.authorStezowski, O
dc.creator.authorSzilner, S
dc.creator.authorSzpak, B
dc.creator.authorUr, C
dc.creator.authorValiente-Dobón, JJ
dc.creator.authorWeinert, M
dc.creator.authorWolf, K
dc.creator.authorZell, KO
cristin.unitcode185,15,4,20
cristin.unitnameKjerne- og energifysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1773544
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=99&rft.spage=&rft.date=2019
dc.identifier.jtitlePhysical Review C
dc.identifier.volume99
dc.identifier.issue1
dc.identifier.pagecount19
dc.identifier.doihttps://doi.org/10.1103/PhysRevC.99.014301
dc.identifier.urnURN:NBN:no-79147
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn2469-9985
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/76018/2/PhysRevC.99.014301.pdf
dc.type.versionPublishedVersion
cristin.articleid014301
dc.relation.projectNFR/263030
dc.relation.projectNFR/240104


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