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dc.date.accessioned2019-02-19T14:22:06Z
dc.date.available2019-02-19T14:22:06Z
dc.date.created2016-06-22T10:02:12Z
dc.date.issued2016
dc.identifier.citationWiedeking, Mathis Krtička, M. Bernstein, L. A. Allmond, J. M. Basunia, M. S. Bleuel, Darren L. Burke, J. T. Daub, B. H. Fallon, Paul Firestone, R.B. Goldblum, Bethany L. Hatarik, R. Lake, P. T. Larsen, Ann-Cecilie Lee, I.-Y. Lescher, S. R. Paschalis, S. Petri, M. Phair, L. Scielzo, N. D. Volya, A. . γ-ray decay from neutron-bound and unbound states in Mo 95 and a novel technique for spin determination. Physical Review C. Nuclear Physics. 2016, 93(2)
dc.identifier.urihttp://hdl.handle.net/10852/66658
dc.description.abstractThe emission of γ rays from neutron-bound and neutron-unbound states in 95 Mo , populated in the 94 Mo ( d , p ) reaction, has been investigated. Charged particles and γ radiation were detected with arrays of annular silicon and Clover-type high-purity Germanium detectors, respectively. Utilizing p− γ and p− γ − γ coincidences, the 95 Mo level scheme was greatly enhanced with 102 new transitions and 43 new states. It agrees well with shell model calculations for excitation energies below ≈ 2 MeV. From p− γ coincidence data, a new method for the determination of spins of discrete levels is proposed. The method exploits the suppression of high-angular momentum neutron emission from levels with high spins populated in the (d,p) reaction above the neutron separation energy. Spins for almost all 95 Mo levels below 2 MeV (and for a few levels above) have been determined with this method.en_US
dc.languageEN
dc.publisherAmerican Physical Society
dc.titleγ-ray decay from neutron-bound and unbound states in Mo 95 and a novel technique for spin determinationen_US
dc.typeJournal articleen_US
dc.creator.authorWiedeking, Mathis
dc.creator.authorKrtička, M.
dc.creator.authorBernstein, L. A.
dc.creator.authorAllmond, J. M.
dc.creator.authorBasunia, M. S.
dc.creator.authorBleuel, Darren L.
dc.creator.authorBurke, J. T.
dc.creator.authorDaub, B. H.
dc.creator.authorFallon, Paul
dc.creator.authorFirestone, R.B.
dc.creator.authorGoldblum, Bethany L.
dc.creator.authorHatarik, R.
dc.creator.authorLake, P. T.
dc.creator.authorLarsen, Ann-Cecilie
dc.creator.authorLee, I.-Y.
dc.creator.authorLescher, S. R.
dc.creator.authorPaschalis, S.
dc.creator.authorPetri, M.
dc.creator.authorPhair, L.
dc.creator.authorScielzo, N. D.
dc.creator.authorVolya, A.
cristin.unitcode185,15,4,20
cristin.unitnameKjerne- og energifysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode0
dc.identifier.cristin1363174
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. Nuclear Physics&rft.volume=93&rft.spage=&rft.date=2016
dc.identifier.jtitlePhysical Review C. Nuclear Physics
dc.identifier.volume93
dc.identifier.issue2
dc.identifier.pagecount11
dc.identifier.doihttp://dx.doi.org/10.1103/PhysRevC.93.024303
dc.identifier.urnURN:NBN:no-69839
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn0556-2813
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/66658/1/Wiedeking_PhysRevC.93.024303.pdf
dc.type.versionPublishedVersion
cristin.articleid024303


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