Show simple item record

dc.contributor.authorBa̧czyk, P.
dc.contributor.authorDobaczewski, Jacek
dc.contributor.authorKonieczka, M.
dc.contributor.authorSatuła, W.
dc.contributor.authorNakatsukasa, T.
dc.contributor.authorSato, K.
dc.date.accessioned2018-02-14T10:36:17Z
dc.date.available2018-02-14T10:36:17Z
dc.date.issued2018
dc.identifier.citationBa̧czyk, P., Dobaczewski, J., Konieczka, M., Satuła, W., Nakatsukasa, T., & Sato, K. (2018). Isospin-symmetry breaking in masses of N ≃ Z nuclei. <i>Physics Letters B</i>, <i>778</i>, 178-183. <a href="https://doi.org/10.1016/j.physletb.2017.12.068" target="_blank">https://doi.org/10.1016/j.physletb.2017.12.068</a>
dc.identifier.otherCONVID_27856953
dc.identifier.otherTUTKAID_76571
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/57059
dc.description.abstractEffects of the isospin-symmetry breaking (ISB) beyond mean-field Coulomb terms are systematically studied in nuclear masses near the N = Z line. The Coulomb exchange contributions are calculated exactly. We use extended Skyrme energy density functionals (EDFs) with proton–neutron-mixed densities, to which we add new terms breaking the isospin symmetry. Two parameters associated with the new terms are determined by fitting mirror and triplet displacement energies (MDEs and TDEs) of isospin multiplets. The new EDFs reproduce MDEs for the T = 1 2 doublets and T = 1 triplets, and TDEs for the T = 1 triplets. Relative strengths of the obtained isospin-symmetry-breaking terms are not consistent with the differences in the N N scattering lengths, ann, app , and anp. Based on low-energy experimental data, it seems thus impossible to delineate the strong-force ISB effects from beyond-mean-field Coulomb-energy corrections.
dc.language.isoeng
dc.publisherElsevier B.V.
dc.relation.ispartofseriesPhysics Letters B
dc.subject.othernuclear density functional theory (DFT)
dc.subject.otherenergy density functional (EDF)
dc.subject.otherproton–neutron mixing
dc.subject.otherisospin symmetry breaking (ISB)
dc.subject.othermirror displacement energy (MDE)
dc.subject.othertriplet displacement energy (TDE)
dc.titleIsospin-symmetry breaking in masses of N ≃ Z nuclei
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201802131479
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2018-02-13T13:15:12Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.format.pagerange178-183
dc.relation.issn0370-2693
dc.relation.numberinseries0
dc.relation.volume778
dc.type.versionpublishedVersion
dc.rights.copyright© 2018 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license. Funded by SCOAP3.
dc.rights.accesslevelopenAccessfi
dc.subject.ysoydinfysiikka
dc.subject.ysotiheys
dc.subject.ysotiheysfunktionaaliteoria
dc.subject.ysoenergia
dc.subject.ysoprotonit
dc.subject.ysoneutronit
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
jyx.subject.urihttp://www.yso.fi/onto/yso/p14628
jyx.subject.urihttp://www.yso.fi/onto/yso/p28852
jyx.subject.urihttp://www.yso.fi/onto/yso/p1310
jyx.subject.urihttp://www.yso.fi/onto/yso/p12428
jyx.subject.urihttp://www.yso.fi/onto/yso/p15394
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1016/j.physletb.2017.12.068
dc.type.okmA1


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record

© 2018 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license. Funded by SCOAP3.
Except where otherwise noted, this item's license is described as © 2018 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license. Funded by SCOAP3.