Matter distribution and spin-orbit force in spherical nuclei

G. Co', M. Anguiano, V. De Donno, and A. M. Lallena
Phys. Rev. C 97, 034313 – Published 12 March 2018

Abstract

We investigate the possibility that some nuclei show density distributions with a depletion in the center, a semibubble structure, by using a Hartree-Fock plus Bardeen-Cooper-Schrieffer approach. We separately study the proton, neutron, and matter distributions in 37 spherical nuclei mainly in the sd shell region. We found a relation between the semibubble structure and the energy splitting of spin-orbit partner single particle levels. The presence of semibubble structure reduces this splitting, and we study its consequences on the excitation spectrum of the nuclei under investigation by using a quasiparticle random-phase-approximation approach. The excitation energies of the low-lying 4+ states can be related to the presence of semibubble structure in nuclei.

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  • Received 6 December 2017
  • Revised 29 January 2018

DOI:https://doi.org/10.1103/PhysRevC.97.034313

©2018 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

G. Co'1,2, M. Anguiano3, V. De Donno1, and A. M. Lallena3

  • 1Dipartimento di Matematica e Fisica “E. De Giorgi”, Università del Salento, I-73100 Lecce, Italy
  • 2INFN Sezione di Lecce, Via Arnesano, I-73100 Lecce, Italy
  • 3Departamento de Física Atómica, Molecular y Nuclear, Universidad de Granada, E-18071 Granada, Spain

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Issue

Vol. 97, Iss. 3 — March 2018

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