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dc.creatorSingh, Gagandeepes
dc.creatorSingh, Jagjites
dc.creatorCasal Berbel, Jesúses
dc.creatorFortunato, L.es
dc.date.accessioned2023-01-20T12:36:36Z
dc.date.available2023-01-20T12:36:36Z
dc.date.issued2022
dc.identifier.citationSingh, G., Singh, J., Casal Berbel, J. y Fortunato, L. (2022). Exploring the halo character and dipole response in the dripline nucleus F 31. Physical Review C, 105 (1), 014328. https://doi.org/10.1103/PhysRevC.105.014328.
dc.identifier.issn2469-9985es
dc.identifier.issn2469-9993es
dc.identifier.urihttps://hdl.handle.net/11441/141639
dc.description.abstractBackground: Lying at the lower edge of the “island of inversion,” neutron-rich fluorine isotopes ( 29 – 31 F ) provide a curious case to study the configuration mixing in this part of the nuclear landscape. Recent studies have suggested that a prospective two-neutron halo in the dripline nucleus 31 F could be linked to the occupancy of the p f intruder configurations. Purpose: Focusing on configuration mixing, matter radii, and neutron-neutron ( n n ) correlations in the ground state of 31 F , we explore various scenarios to analyze its possible halo nature as well as the low-lying electric dipole ( E 1 ) response within a three-body approach. Method: We use an analytical, transformed harmonic oscillator basis under the aegis of a hyperspherical formalism to construct the ground-state three-body wave function of 31 F . The n n interaction is defined by the Gogny-Pires-Tourreil potential that includes the central, spin-orbit, and tensor terms, while the different two-body potentials to describe the core + n subsystems are constrained by the different possible scenarios considered. Results: The 31 F ground-state configuration mixing and its matter radius are computed for different choices of the 30 F structure coupled to the valence neutron. The admixture of p 3 / 2 , d 3 / 2 , and f 7 / 2 components is found to play an important role, favoring the dominance of inverted configurations with dineutron spreads for two-neutron halo formation. The increase in matter radius with respect to the core radius, Δ r ≳ 0.30 fm and the dipole distributions along with the integrated B ( E 1 ) strengths of ⩾ 2.6 e 2 fm 2 are large enough to be compatible with other two-neutron halo nuclei.es
dc.description.sponsorshipScuola Italiana Design (SID) de la Università degli Studi di Padova-CASA_SID19_01es
dc.formatapplication/pdfes
dc.format.extent14 p.es
dc.language.isoenges
dc.publisherAmerican Physical Societyes
dc.relation.ispartofPhysical Review C, 105 (1), 014328.
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internacional*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.titleExploring the halo character and dipole response in the dripline nucleus F 31es
dc.typeinfo:eu-repo/semantics/articlees
dcterms.identifierhttps://ror.org/03yxnpp24
dc.type.versioninfo:eu-repo/semantics/publishedVersiones
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses
dc.contributor.affiliationUniversidad de Sevilla. Departamento de Física Atómica, Molecular y Nucleares
dc.relation.projectIDCASA_SID19_01es
dc.relation.publisherversionhttps://doi.org/10.1103/PhysRevC.105.014328es
dc.identifier.doi10.1103/PhysRevC.105.014328es
dc.journaltitlePhysical Review Ces
dc.publication.volumen105es
dc.publication.issue1es
dc.publication.initialPage014328es
dc.contributor.funderUniversità degli Studi di Padova. Italyes

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