Chiral NNLOsat descriptions of nuclear multipole resonances within the random-phase approximation

Q. Wu, B. S. Hu, F. R. Xu, Y. Z. Ma, S. J. Dai, Z. H. Sun, and G. R. Jansen
Phys. Rev. C 97, 054306 – Published 3 May 2018

Abstract

We study nuclear multipole resonances in the framework of the random-phase approximation by using the chiral potential NNLOsat. This potential includes two- and three-body terms that have been simultaneously optimized to low-energy nucleon-nucleon scattering data and selected nuclear structure data. Our main focuses have been the isoscalar monopole, isovector dipole, and isoscalar quadrupole resonances of the closed-shell nuclei, He4, O16,22,24, and Ca40,48. These resonance modes have been widely observed in experiment. In addition, we use a renormalized chiral potential Vlow-k, based on the N3LO two-body potential by Entem and Machleidt [Phys. Rev. C 68, 041001 (2011)]. This introduces a dependency on the cutoff parameter used in the normalization procedure as reported in previous works by other groups. While NNLOsat can reasonably reproduce observed multipole resonances, it is not possible to find a single cutoff parameter for the Vlow-k potential that simultaneously describes the different types of resonance modes. The sensitivity to the cutoff parameter can be explained by missing induced three-body forces in the calculations. Our results for neutron-rich O22,24 show a mixing nature of isoscalar and isovector resonances in the dipole channel at low energies. We predict that O22 and O24 have low-energy isoscalar quadrupole resonances at energies lower than 5 MeV.

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  • Received 11 January 2018

DOI:https://doi.org/10.1103/PhysRevC.97.054306

©2018 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

Q. Wu1, B. S. Hu1, F. R. Xu1,*, Y. Z. Ma1, S. J. Dai1, Z. H. Sun1,2,3, and G. R. Jansen3,4

  • 1School of Physics, and State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871, China
  • 2Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USA
  • 3Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
  • 4National Center for Computational Sciences, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA

  • *frxu@pku.edu.cn

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Issue

Vol. 97, Iss. 5 — May 2018

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