Nuclear dipole polarizability from mean-field modeling constrained by chiral effective field theory
arXiv:1703.00866 · doi:10.1016/j.physletb.2017.12.012
Abstract
We construct a new Skyrme interaction Skm by fitting the equation of state and nucleon effective masses in asymmetric nuclear matter from chiral two- and three-body forces as well as the binding energies of finite nuclei. Employing this interaction to study the electric dipole polarizabilities of Ca, Ni, Sn, and Pb in the random-phase approximation, we find that the theoretical predictions are in good agreement with experimentally measured values without additional fine tuning of the Skyrme interaction, thus confirming the usefulness of the new Skyrme interaction in studying the properties of nuclei. We further use this interaction to study the neutron skin thicknesses of Ca and Pb, and they are found to be consistent with the experimental data.
Significantly revised, 7 pages, 4 figures. Published version in PLB
References in corpus (8)
- 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
- Electric dipole polarizability of Ca and implications for the neutron skin
- Neutron skins and neutron stars
- Neutron star crusts from mean field models constrained by chiral effective field theory
- Constraining the density slope of nuclear symmetry energy at subsaturation densities using electric dipole polarizability in Pb
- Low Momentum Nucleon-Nucleon Interactions and Shell-Model Calculations
- Information and statistics: a new paradigm in theoretical nuclear physics
Cited by in corpus (23)
- Nucleon Effective Masses in Neutron-Rich Matter
- Neutron star tidal deformabilities constrained by nuclear theory and experiment
- Dense Nuclear Matter Equation of State from Heavy-Ion Collisions
- Laser Spectroscopy for the Study of Exotic Nuclei
- Bayesian modeling of the nuclear equation of state for neutron star tidal deformabilities and GW170817
- Optimizing the relativistic energy density functional with nuclear ground state and collective excitation properties
- Implications of parity-violating electron scattering experiments on Ca (CREX) and Pb (PREX-II) for nuclear energy density functionals
- Tides in merging neutron stars: Consistency of the GW170817 event with experimental data on finite nuclei
- Systematic Matter and Binding-Energy Distributions from a Dispersive Optical Model Analysis
- Nuclear matter properties at finite temperatures from effective interactions
- Entrainment effects in neutron-proton mixtures within the nuclear-energy density functional theory. I. Low-temperature limit
- Constraining nuclear matter parameters from correlation systematics:a mean-field perspective
- The nucleon effective mass and its isovector splitting
- Hot and Dense Matter Equation of State Probability Distributions for Astrophysical Simulations
- Tensor Fermi liquid parameters in nuclear matter from chiral effective field theory
- Bayesian inference on the isospin splitting of nucleon effective mass from giant resonances in Pb
- Empirical neutron star mass formula based on experimental observables
- Nuclear giant quadruple resonance within transport approach and its constraint on nucleon effective mass
- Neutron-skin values and matter and neutron radii determined from reaction cross sections of proton scattering on C, Ca, Ni, Pb
- Nuclear Symmetry Energy and Neutron Skin Thickness of using a finite range effective interaction
- Constraining neutron-proton effective mass splitting through nuclear giant dipole resonance within transport approach
- In-medium potential, pion production in heavy-ion collisions and the symmetry energy
- Transport Model Comparison Studies of Intermediate-Energy Heavy-Ion Collisions