Constraining isovector nuclear interactions with giant resonances within a Bayesian approach
arXiv:2006.05217 · doi:10.1016/j.physletb.2020.135820
Abstract
We put a stringent constraint on the isovector nuclear interactions in the Skyrme-Hartree-Fock model from the centroid energy of the isovector giant dipole resonance in Pb as well as its electric polarizability . Using the Bayesian analysis method, and are found to be mostly determined by the nuclear symmetry energy at about fm and the isovector nucleon effective mass at the saturation density. At confidence level, we obtain MeV and .
5 pages, 5 figures
References in corpus (6)
- Neutron Star Observations: Prognosis for Equation of State Constraints
- Constraints on the Symmetry Energy Using the Mass-Radius Relation of Neutron Stars
- The Giant Dipole Resonance as a quantitative constraint on the symmetry energy
- Nuclear symmetry energy and its density slope at normal density extracted from global nucleon optical potentials
- Giant Quadrupole Resonances in 208Pb, the nuclear symmetry energy and the neutron skin thickness
- Constraining the density slope of nuclear symmetry energy at subsaturation densities using electric dipole polarizability in Pb
Cited by in corpus (4)
- Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817
- Comparison of Heavy-Ion Transport Simulations: Mean-field Dynamics in a Box
- Bayesian inference of finite-nuclei observables based on the KIDS model
- Finding signatures of the nuclear symmetry energy in heavy-ion collisions with deep learning