Neutron skin systematics from microscopic equations of state
arXiv:2203.09753 · doi:10.1103/PhysRevC.105.064303
Abstract
This paper presents an analysis of neutron skins based on fully microscopic equations of state, including chiral two- and three-nucleon forces consistently at N3LO. Other theoretical predictions and recent constraints are also addressed, such as those from the PREX II experiment and the latest parity-violating electron scattering measurement of the 27Al neutron skin.
arXiv commentRevised version, to appear in Physical Review C
References in corpus (25)
- Constraints on the symmetry energy and neutron skins from experiments and theory
- Constraints on the density dependence of the symmetry energy
- Implications of PREX-II on the equation of state of neutron-rich matter
- Accurate nuclear radii and binding energies from a chiral interaction
- Neutron skin of 208Pb, nuclear symmetry energy, and the parity radius experiment
- Three-Body Interactions Among Nucleons and Pions
- Charge, neutron, and weak size of the atomic nucleus
- High-quality two-nucleon potentials up to fifth order of the chiral expansion
- Chiral interactions up to next-to-next-to-next-to-leading order and nuclear saturation
- Symmetry Energy II: Isobaric Analog States
- The Nuclear Symmetry Energy
- Results of the ASY-EOS experiment at GSI: The symmetry energy at suprasaturation density
- Local chiral effective field theory interactions and quantum Monte Carlo applications
- Neutron skin thickness in droplet model with surface width dependence: indications of softness of the nuclear symmetry energy
- Chiral Effective Field Theory and the High-Density Nuclear Equation of State
- Accurate bulk properties of nuclei from to from potentials with isobars
- Proton elastic scattering from tin isotopes at 295 MeV and systematic change of neutron density distributions
- Bayesian modeling of the nuclear equation of state for neutron star tidal deformabilities and GW170817
- Relativistic Brueckner-Hartree-Fock in nuclear matter without the average momentum approximation
- Universal correlations in the nuclear symmetry energy, slope parameter, and curvature
- Neutron rich matter in heaven and on Earth
- Analysis of the neutron matter equation of state and the symmetry energy up to fourth order of chiral effective field theory
- First Determination of the 27Al Neutron Distribution Radius from a Parity-Violating Electron Scattering Measurement
- Correlations among symmetry energy elements in Skyrme models
- The Equation of State of Neutron-Rich Matter at Fourth Order of Chiral Effective Field Theory and the Radius of a Medium-Mass Neutron Star