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dc.contributor.authorGreenlees, Paul
dc.contributor.authorRubert, J.
dc.contributor.authorPiot, J.
dc.contributor.authorGall, Benoit
dc.contributor.authorAndersson, L.L.
dc.contributor.authorAsai, M.
dc.contributor.authorAsfari, Z.
dc.contributor.authorCox, D.M.
dc.contributor.authorDechery, F.
dc.contributor.authorDorvaux, Olivier
dc.contributor.authorGrahn, Tuomas
dc.contributor.authorHauschild, Karl
dc.contributor.authorHenning, G.
dc.contributor.authorHerzan, Andrej
dc.contributor.authorHerzberg, Rolf-Dietmar
dc.contributor.authorHessberger, Fritz Peter
dc.contributor.authorJakobsson, Ulrika
dc.contributor.authorJones, Peter
dc.contributor.authorJulin, Rauno
dc.contributor.authorJuutinen, Sakari
dc.contributor.authorKetelhut, Steffen
dc.contributor.authorKhoo, Teng Lek
dc.contributor.authorLeino, Matti
dc.contributor.authorLjungvall, J.
dc.contributor.authorLopez-Martens, Araceli
dc.contributor.authorLozeva, R.
dc.contributor.authorNieminen, Päivi
dc.contributor.authorPakarinen, Janne
dc.contributor.authorPapadakis, P.
dc.contributor.authorParr, E.
dc.contributor.authorPeura, Pauli
dc.contributor.authorRahkila, Panu
dc.contributor.authorRinta-Antila, Sami
dc.contributor.authorRuotsalainen, Panu
dc.contributor.authorSandzelius, Mikael
dc.contributor.authorSarén, Jan
dc.contributor.authorScholey, Catherine
dc.contributor.authorSeweryniak, D.
dc.contributor.authorSorri, Juha
dc.contributor.authorSulignano, B.
dc.contributor.authorTheisen, Ch
dc.contributor.authorUusitalo, Juha
dc.contributor.authorVenhart, Martin
dc.date.accessioned2016-02-08T05:55:03Z
dc.date.available2016-02-08T05:55:03Z
dc.date.issued2012
dc.identifier.citationGreenlees, P., Rubert, J., Piot, J., Gall, B., Andersson, L. L., Asai, M., . . . Venhart, M. (2012). Shell-Structure and Pairing Interaction in Superheavy Nuclei: Rotational Properties of the Z=104 Nucleus 256Rf. <em>Physical Review Letters</em>, 109 (1), 012501. <a href="http://dx.doi.org/10.1103/PhysRevLett.109.012501">doi:10.1103/PhysRevLett.109.012501</a> Retrieved from <a href="http://prl.aps.org/abstract/PRL/v109/i1/e012501">http://prl.aps.org/abstract/PRL/v109/i1/e012501</a>
dc.identifier.otherTUTKAID_55642
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/48665
dc.description.abstractThe rotational band structure of the Z ¼ 104 nucleus 256Rf has been observed up to a tentative spin of 20@ using state-of-the-art -ray spectroscopic techniques. This represents the first such measurement in a superheavy nucleus whose stability is entirely derived from the shell-correction energy. The observed rotational properties are compared to those of neighboring nuclei and it is shown that the kinematic and dynamic moments of inertia are sensitive to the underlying single-particle shell structure and the specific location of high-j orbitals. The moments of inertia therefore provide a sensitive test of shell structure and pairing in superheavy nuclei which is essential to ensure the validity of contemporary nuclear models in this mass region. The data obtained show that there is no deformed shell gap at Z ¼ 104, which is predicted in a number of current self-consistent mean-field models.
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review Letters
dc.subject.otherKokeellinen ydinfysiikka
dc.subject.otherExperimental nuclear physics
dc.titleShell-Structure and Pairing Interaction in Superheavy Nuclei: Rotational Properties of the Z=104 Nucleus 256Rf
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201602051456
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineFysiikka
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2016-02-05T07:15:05Z
dc.type.coarjournal article
dc.description.reviewstatuspeerReviewed
dc.format.pagerange12501
dc.relation.issn0031-9007
dc.relation.volume109
dc.type.versionpublishedVersion
dc.rights.copyright© 2012 the Authors. Published by the American Physical Society under the terms of the Creative Commons Attribution 3.0 License.
dc.rights.accesslevelopenAccessfi
dc.rights.urlhttp://creativecommons.org/licenses/by/3.0/
dc.relation.doi10.1103/PhysRevLett.109.012501


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© 2012 the Authors. Published by the American Physical Society under the terms of the Creative Commons Attribution 3.0 License.
Except where otherwise noted, this item's license is described as © 2012 the Authors. Published by the American Physical Society under the terms of the Creative Commons Attribution 3.0 License.