Neutron-skin values and matter and neutron radii determined from reaction cross sections of proton scattering on C, Ca, Ni, Pb
arXiv:2211.16688 · doi:10.1103/PhysRevC.107.024608
Abstract
Very lately, the PREX and the CREX collaboration present skin values, and , respectively. We recently determined a neutron-skin value fm from measured reaction cross sections of p+Pb scattering in a range of incident energies $10 \lsim E_{\rm in} \lsim 100$ MeV where the chiral (Kyushu) -matrix folding model is reliable for C+C scattering. The data are available for proton scattering on Ni, Ca, C targets. Our first aim is to test the Kyushu -matrix folding model for p+Pb scattering in $20 \lsim E_{\rm in} \lsim 180$ MeV. Our second aim is to determine skin values and matter and neutron radii, and , for Pb, Ni, Ca, C from the . Our method is the Kyushu -matrix folding model with the densities scaled from the D1S-GHFB+AMP densities, where D1S-GHFB+AMP stands for Gogny-D1S HFB (GHFB) with the angular momentum projection (AMP). As for proton scattering, we find that our model is reliable in $20 \lsim E_{\rm in} \lsim 180$ MeV. For Pb, the skin value deduced from in $20 \lsim E_{\rm in} \lsim 180$ MeV is fm. Our results on are compared with the previous works. Our result fm agrees with fm. In addition, our result fm is consistent with the CREX value.
References in corpus (51)
- The equation of state for nucleon matter and neutron star structure
- Equations of state for supernovae and compact stars
- Isospin Asymmetry in Nuclei and Neutron Stars
- Skyrme Interaction and Nuclear Matter Constraints
- Accurate Determination of the Neutron Skin Thickness of Pb through Parity-Violation in Electron Scattering
- Measurement of the Neutron Radius of 208Pb Through Parity-Violation in Electron Scattering
- Implications of PREX-II on the equation of state of neutron-rich matter
- Complete electric dipole response and the neutron skin in 208Pb
- Neutron skin of 208Pb, nuclear symmetry energy, and the parity radius experiment
- Parity Violating Measurements of Neutron Densities
- Neutron star radii and crusts: uncertainties and unified equations of state
- Precision Determination of the Neutral Weak Form Factor of Ca
- Density slope of the nuclear symmetry energy from the neutron skin thickness of heavy nuclei
- Neutron skin of Pb from Coherent Pion Photoproduction
- Electric dipole polarizability of Ca and implications for the neutron skin
- Weak charge form factor and radius of 208Pb through parity violation in electron scattering
- Neutron skins of atomic nuclei: per aspera ad astra
- Dipole polarizability of 120Sn and nuclear energy density functionals
- Charge radii of exotic neon and magnesium isotopes
- Determination of the structure of Ne by full-microscopic framework
- Origin of the neutron skin thickness of 208Pb in nuclear mean-field models
- Ground-state properties of neutron-rich Mg isotopes
- Effects of symmetry energy on equation of state for simulations of core-collapse supernovae and neutron-star mergers
- Nuclear symmetry energy and core-crust transition in neutron stars: a critical study
- Deformation of Ne isotopes in the island-of-inversion region
- Has a thick neutron skin in Pb been ruled out?
- Isovector properties of the Gogny interaction
- The Brieva-Rook Localization of the Microscopic Nucleon-Nucleus Potential
- Nuclear and neutron matter -matrix calculations with Ch-EFT potential including effects of three-nucleon interaction
- Higher-order symmetry energy and neutron star core-crust transition with Gogny forces
- New Gogny interaction suitable for astrophysical applications
- Validating relativistic models of nuclear structure against theoretical, experimental, and observational constraints
- Constraining the high-density nuclear symmetry energy with the transverse-momentum dependent elliptic flow
- Constraints on Skyrme Equations of State from Properties of Doubly Magic Nuclei and Ab-Initio Calculations of Low-Density Neutron Matter
- Microscopic optical potentials for He scattering
- Are nuclear matter properties correlated to neutron star observables ?
- Microscopic calculations based on chiral two- and three-nucleon forces for proton- and He-nucleus scattering
- Kaon Condensation in Neutron Stars with Skyrme-Hartree-Fock Models
- A dispersive optical model analysis of Pb generating a neutron-skin prediction beyond the mean field
- Nuclear dipole polarizability from mean-field modeling constrained by chiral effective field theory
- Sensitivity of the fusion cross section to the density dependence of the symmetry energy
- Neutron rich matter in the laboratory and in the heavens after GW170817
- Radii of neutron drops probed via the neutron skin thickness of nuclei
- Neutron skin thickness of Pb determined from reaction cross section for proton scattering
- GW170817 constraints analyzed with Gogny forces and momentum-dependent interactions
- -matrix folding-model approach to reaction cross sections for scattering of Ca isotopes on a C target
- Constraining slope parameter of symmetry energy from nuclear structure
- Roles of chiral three-nucleon forces in nucleon-nucleus scattering
- Neutron skin thickness of Pb, Sn, and Ca determined from reaction cross sections of He scattering
- Constraints on Skyrme Equations of State from Doubly Magic Nuclei, Ab-Initio Calculations of Low-Density Neutron Matter, and Neutron Stars
- EOSDB: The Database for Nuclear EoS
Cited by in corpus (3)
- Design and characterisation of an antiproton deceleration beamline for the PUMA experiment
- C+C scattering as the reference system for reaction cross section
- Determination of matter radius and neutron-skin thickness of Ni from reaction cross section of proton scattering on Ni targets (published in Results in Physics)