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dc.contributor.authorMarcos Marcos, Saturnino 
dc.contributor.authorNiembro Bárcena, Ramón 
dc.contributor.authorLópez Quelle, Mercedes 
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2025-03-03T17:18:37Z
dc.date.available2025-03-03T17:18:37Z
dc.date.issued2024-07
dc.identifier.issn0375-9474
dc.identifier.issn1873-1554
dc.identifier.urihttps://hdl.handle.net/10902/35834
dc.description.abstractWithin the relativistic mean field approximation, we analyse the kink effect (KE) in the evolution of the charge radius isotope shift of lead isotopes as a function of the neutron number N. We show that if the interactions between neutron and proton states responsible for the KE are assumed to be proportional either to the overlaps of their corresponding wave functions or to those of their corresponding probability density distributions, it is not possible, by themselves, to explain the KE. However, we find that the small component of the single-particle Dirac spinors plays a relevant role in the kink formation. By considering the contribution of the N − 126 valence neutrons to the proton central potential, we can explain the generation of the KE and why neutrons in the 1i₁₁∕₂ orbital are more kinky than when they are in the 2g₉∕₂ orbital.es_ES
dc.format.extent11 p.es_ES
dc.language.isoenges_ES
dc.publisherElsevieres_ES
dc.rights© 2024 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY-NC license (http://creativecommons.org/licenses/by-nc/4.0/).es_ES
dc.rights.urihttp://creativecommons.org/licenses/by-nc/4.0/*
dc.sourceNuclear Physics A, 2024, 1047, 122883es_ES
dc.subject.otherNuclear charge radiuses_ES
dc.subject.otherKink effectes_ES
dc.subject.otherRelativistic nuclear modelses_ES
dc.titleKink of the nuclear charge radius isotope shift and overlaps of the neutron and proton orbitals in leades_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://doi.org/10.1016/j.nuclphysa.2024.122883es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1016/j.nuclphysa.2024.122883
dc.type.versionpublishedVersiones_ES


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© 2024 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY-NC license (http://creativecommons.org/licenses/by-nc/4.0/).Excepto si se señala otra cosa, la licencia del ítem se describe como © 2024 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY-NC license (http://creativecommons.org/licenses/by-nc/4.0/).