Por favor, use este identificador para citar o enlazar a este item: http://hdl.handle.net/10261/31800
COMPARTIR / EXPORTAR:
logo share SHARE logo core CORE BASE
Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL | DATACITE

Invitar a revisión por pares abierta
Título

Structural evolution in Pt isotopes with the interacting boson model Hamiltonian derived from the Gogny energy density functional

AutorNomura, K.; Otsuka, T.; Rodríguez-Guzmán, R. CSIC; Robledo, Luis Miguel; Sarriguren, Pedro CSIC ORCID
Palabras claveInteracting Boson Model
Gogny Energy Density Functional
Platinum isotopes
Fecha de publicación25-ene-2011
EditorAmerican Physical Society
CitaciónPHYSICAL REVIEW C 83, 014309 (2011)
ResumenSpectroscopic calculations are carried out for the description of the shape/phase transition in Pt nuclei in terms of the interacting boson model (IBM) Hamiltonian derived from (constrained) Hartree-Fock-Bogoliubov (HFB) calculations with the finite range and density-dependent Gogny-D1S energy density functional. Assuming that the many-nucleon driven dynamics of nuclear surface deformation can be simulated by effective bosonic degrees of freedom, the Gogny-D1S potential energy surface (PES) with quadrupole degrees of freedom is mapped onto the corresponding PES of the IBM. By using this mapping procedure, the parameters of the IBM Hamiltonian, relevant to the low-lying quadrupole collective states, are derived as functions of the number of valence nucleons. Merits of both Gogny-HFB and IBM approaches are utilized so that the spectra and the wave functions in the laboratory system are calculated precisely. The experimental low-lying spectra of both ground-state and sideband levels are well reproduced. From the systematics of the calculated spectra and the reduced E2 transition probabilities B(E2), the prolate-to-oblate shape/phase transition is shown to take place quite smoothly as a function of neutron number N in the considered Pt isotopic chain, for which the γ softness plays an essential role. All of these spectroscopic observables behave consistently with the relevant PES and the derived parameters of the IBM Hamiltonian as functions of N. Spectroscopic predictions are also made for those nuclei that do not have enough experimental E2 data.
Versión del editorhttp://dx.doi.org/10.1103/PhysRevC.83.014309
URIhttp://hdl.handle.net/10261/31800
DOI10.1103/PhysRevC.83.014309
Aparece en las colecciones: (CFMAC-IEM) Artículos




Ficheros en este ítem:
Fichero Descripción Tamaño Formato
sarri_prc83_nomura.pdf747,24 kBAdobe PDFVista previa
Visualizar/Abrir
Mostrar el registro completo

CORE Recommender

SCOPUSTM   
Citations

48
checked on 09-abr-2024

WEB OF SCIENCETM
Citations

52
checked on 29-feb-2024

Page view(s)

280
checked on 17-abr-2024

Download(s)

247
checked on 17-abr-2024

Google ScholarTM

Check

Altmetric

Altmetric


NOTA: Los ítems de Digital.CSIC están protegidos por copyright, con todos los derechos reservados, a menos que se indique lo contrario.