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dc.contributor.authorPrassa, Vaia
dc.contributor.authorNikšic, T.
dc.contributor.authorVretenar, D.
dc.date.accessioned2016-01-28T08:19:30Z
dc.date.available2016-01-28T08:19:30Z
dc.date.issued2013
dc.identifier.citationPrassa, V., Nikšic, T., & Vretenar, D. (2013). Structure of transactinide nuclei with relativistic energy density functionals. <i>Physical Review C</i>, <i>88</i>(4), Article 044324. <a href="https://doi.org/10.1103/PhysRevC.88.044324" target="_blank">https://doi.org/10.1103/PhysRevC.88.044324</a>
dc.identifier.otherCONVID_23227345
dc.identifier.otherTUTKAID_60709
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/48497
dc.description.abstractA microscopic theoretical framework based on relativistic energy density functionals (REDFs) is applied to studies of shape evolution, excitation spectra, and decay properties of transactinide nuclei. Axially symmetric and triaxial relativistic Hartree-Bogoliubov (RHB) calculations, based on the functional DD-PC1 and with a separable pairing interaction, are performed for the even-even isotopic chains between Fm and Fl. The occurrence of a deformed shell gap at neutron number N = 162 and its role on the stability of nuclei in the region around Z = 108 is investigated. A quadrupole collective Hamiltonian, with parameters determined by self-consistent constrained triaxial RHB calculations, is used to examine low-energy spectra of No, Rf, Sg, Hs, and Ds with neutron number in the interval 158 N 170. In particular, we analyze the isotopic dependence of several observables that characterize the transitions between axially symmetric rotors, γ -soft rotors, and spherical vibrators. An interesting example of a possible occurrence of shape-phase transitions and critical-point phenomena in this mass region is explored.
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review C
dc.relation.urihttp://link.aps.org/doi/10.1103/PhysRevC.88.044324
dc.subject.otherTheoretical nuclear physics
dc.titleStructure of transactinide nuclei with relativistic energy density functionals
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201601281305
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineFysiikkafi
dc.contributor.oppiainePhysicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2016-01-28T07:15:06Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn0556-2813
dc.relation.numberinseries4
dc.relation.volume88
dc.type.versionpublishedVersion
dc.rights.copyright© 2013 American Physical Society. Published in this repository with the kind permission of the publisher.
dc.rights.accesslevelopenAccessfi
dc.relation.doi10.1103/PhysRevC.88.044324
dc.type.okmA1


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