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dc.contributor.authorDobaczewski, Jacek
dc.contributor.authorEngel, Jonathan
dc.contributor.authorKortelainen, Markus
dc.contributor.authorBecker, Pierre
dc.date.accessioned2018-12-13T10:46:53Z
dc.date.available2018-12-13T10:46:53Z
dc.date.issued2018
dc.identifier.citationDobaczewski, J., Engel, J., Kortelainen, M., & Becker, P. (2018). Correlating Schiff Moments in the Light Actinides with Octupole Moments. <i>Physical Review Letters</i>, <i>121</i>(23), Article 232501. <a href="https://doi.org/10.1103/physrevlett.121.232501" target="_blank">https://doi.org/10.1103/physrevlett.121.232501</a>
dc.identifier.otherCONVID_28766540
dc.identifier.otherTUTKAID_79779
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/60595
dc.description.abstractTo explore the nature of collective modes in weakly bound nuclei, we have investigated deformation effects and surface flow patterns of isovector dipole modes in a shape-coexisting nucleus, 40Mg. The calculations were done in a fully self-consistent continuum finite-amplitude quasiparticle random phase approximation in a large deformed spatial mesh. An unexpected result of pygmy and giant dipole modes having disproportionate deformation splittings in strength functions was obtained. Furthermore, the transition current densities demonstrate that the long-sought core-halo oscillation in pygmy resonances is collective and compressional, corresponding to the lowest excitation energy and the simplest quantum flow topology. Our calculations show that surface flow patterns become more complicated as excitation energies increase.fi
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review Letters
dc.rightsIn Copyright
dc.subject.othernuclear density functional theory
dc.subject.othernuclear many-body theory
dc.subject.othernuclear structure and decays
dc.subject.othernuclear tests of fundamental interactions
dc.titleCorrelating Schiff Moments in the Light Actinides with Octupole Moments
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201812105032
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2018-12-10T07:15:11Z
dc.description.reviewstatuspeerReviewed
dc.relation.issn0031-9007
dc.relation.numberinseries23
dc.relation.volume121
dc.type.versionpublishedVersion
dc.rights.copyright© 2017 American Physical Society.
dc.rights.accesslevelopenAccessfi
dc.subject.ysoydinfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1103/physrevlett.121.232501


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