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dc.contributor.authorShi, Yue
dc.contributor.authorDobaczewski, Jacek
dc.contributor.authorGreenlees, Paul
dc.date.accessioned2014-09-10T13:49:30Z
dc.date.available2014-09-10T13:49:30Z
dc.date.issued2014
dc.identifier.citationShi, Y., Dobaczewski, J., & Greenlees, P. (2014). Rotational properties of nuclei around 254 No investigated using a spectroscopic-quality Skyrme energy density functional. <i>Physical Review C</i>, <i>89</i>(3), Article 034309. <a href="https://doi.org/10.1103/PhysRevC.89.034309" target="_blank">https://doi.org/10.1103/PhysRevC.89.034309</a>
dc.identifier.otherCONVID_23729292
dc.identifier.otherTUTKAID_62172
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/44236
dc.description.abstractAbstract. Background: Nuclei in the Z≈100 mass region represent the heaviest systems where detailed spectroscopic information is experimentally available. Although microscopic-macroscopic and self-consistent models have achieved great success in describing the data in this mass region, a fully satisfying precise theoretical description is still missing. Purpose: By using fine-tuned parametrizations of the energy density functionals, the present work aims at an improved description of the single-particle properties and rotational bands in the nobelium region. Such locally optimized parametrizations may have better properties when extrapolating towards the superheavy region. Methods: Skyrme Hartree-Fock-Bogolyubov and Lipkin-Nogami methods were used to calculate the quasiparticle energies and rotational bands of nuclei in the nobelium region. Starting from the most recent Skyrme parametrization, UNEDF1, the spin-orbit coupling constants and pairing strengths have been tuned, so as to achieve a better agreement with the excitation spectra and odd-even mass differences in 251Cf and 249Bk. Results: The quasiparticle properties of 251Cf and 249Bk were very well reproduced. At the same time, crucial deformed neutron and proton shell gaps open up at N=152 and Z=100, respectively. Rotational bands in Fm, No, and Rf isotopes, where experimental data are available, were also fairly well described. To help future improvements towards a more precise description, small deficiencies of the approach were carefully identified. Conclusions: In the Z≈100 mass region, larger spin-orbit strengths than those from global adjustments lead to improved agreement with data. Puzzling effects of particle-number restoration on the calculated moment of inertia, at odds with the experimental behavior, require further scrutiny.fi
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review C
dc.subject.othersuperheavy elements
dc.subject.othermean-field
dc.subject.otherfission
dc.titleRotational properties of nuclei around 254 No investigated using a spectroscopic-quality Skyrme energy density functional
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201409092754
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.updated2014-09-09T03:30:10Z
dc.type.coarjournal article
dc.description.reviewstatuspeerReviewed
dc.relation.issn0556-2813
dc.relation.numberinseries3
dc.relation.volume89
dc.type.versionpublishedVersion
dc.rights.copyright© 2014 American Physical Society. This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
dc.rights.accesslevelopenAccessfi
dc.subject.ysoisotoopit
jyx.subject.urihttp://www.yso.fi/onto/yso/p6387
dc.rights.urlhttp://creativecommons.org/licenses/by/3.0/
dc.relation.doi10.1103/PhysRevC.89.034309


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© 2014 American Physical Society. This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Except where otherwise noted, this item's license is described as © 2014 American Physical Society. This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.