Neutron Star Structure and the Neutron Radius of 208Pb

Abstract

We study relationships between the neutron-rich skin of a heavy nucleus and the properties of neutron-star crusts. Relativistic effective field theories with a thicker neutron skin in ${}^{208}$Pb have a larger electron fraction and a lower liquid-to-solid transition density for neutron-rich matter. These properties are determined by the density dependence of the symmetry energy which we vary by adding nonlinear couplings between isoscalar and isovector mesons. An accurate measurement of the neutron radius in ${}^{208}$Pb---via parity violating electron scattering---may have important implications for the structure of neutron stars.

5 pages 3 figures, added additional evidence of model independence, Phys. Rev. Letters in press

References in corpus (3)

• Neutron Star Structure and the Equation of State
• Parity Violating Measurements of Neutron Densities
• Inner edge of neutron-star crust with SLy effective nucleon-nucleon interactions

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• Effects of finite size and symmetry energy on the phase transition of stellar matter at subnuclear densities
• Standard cooling of rapidly rotating isolated neutron stars in 2D
• Determining the neutron skin thickness by relativistic semi-isobaric collisions
• The influence of the enhanced vector meson sector on the properties of the matter of neutron stars
• Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Nucleonic models
• Evolution of nuclear charge radii in copper and indium isotopes
• Study of hot thermally fissile nuclei using relativistic mean field theory
• Nuclear pasta and symmetry energy in the relativistic point-coupling model
• Hyperonic uncertainties in neutron stars, mergers and supernovae
• A multi-reflection time-of-flight mass spectrometer for the offline ion source of the PUMA experiment
• Crust-core interface and bulk neutron star properties
• Constraining the relativistic mean-field models from PREX-2 data: Effective forces revisited
• Constraining Bag constant for Hybrid Neutron stars
• Strong magnetic fields and pasta phases revisited
• Analyzing the dense matter equation of states in the light of the compact object HESS J1731-347
• Thermal effects in hot and dilute homogeneous asymmetric nuclear matter
• Neutron density distribution and neutron skin thickness of ${}^{208}$Pb
• From nuclear reactions to compact stars: a unified approach
• Nuclear breathing mode in neutron-rich Nickel isotopes: sensitivity to the symmetry energy and the role of the continuum
• Probing the momentum-dependence of the symmetry potential by the free n/p ratio of preequilibrium emission
• Nuclear condensation and symmetry energy of dilute nuclear matter: an S-matrix approach
• Emergence of low-energy monopole strength in the neutron-rich calcium isotopes
• Neutrino diffusion in the pasta phase matter within the Thomas-Fermi approach
• Multi-messenger observations of neutron rich matter
• Pasta phases in neutron stars under strong magnetic fields
• Strong magnetic fields: neutron stars with an extended inner crust
• Cold dilute nuclear matter with $\alpha$-particle condensation in a generalized nonlinear relativistic mean-field model
• Crust-core transition of a neutron star: effect of the temperature under strong magnetic fields
• Role of isospin physics in supernova matter and neutron stars
• Thermal x-ray studies of neutron stars and the equation of state
• Simultaneous Extraction of the Weak Radius and the Weak Mixing Angle from Parity-Violating Electron Scattering on ${}^{12}\mathrm{C}$
• Nuclear pasta in hot and dense matter and its influence on the equation of state for astrophysical simulations
• The symmetry energy $\gamma$ parameter of relativistic mean-field models
• Core-crust transition properties of neutron stars within systematically varied extended relativistic mean-field model
• Equation of state and hybrid star properties with the weakly interacting light U-boson in relativistic models
• Moving Beyond Chi-Squared in Nuclei and Neutron Stars
• The effect of self interacting isoscalar-vector meson on finite nuclei and infinite nuclear matter
• Peeling away neutron skin in ultracentral collisions of relativistic nuclei
• Symmetry energy softening in nuclear matter with non-nucleonic constituents
• Quark condensate and chiral symmetry restoration in neutron stars
• Sensitivity of neutron radii in the $""sup208_{P}bnucleusandaneutronstartonucleon-$ sigma_-$ rho_ coupling corrections in relativistic mean field theory
• Deep crustal heating by neutrinos from the surface of accreting neutron stars
• Correlation between the symmetry energy slope and the deconfinement phase transition
• The attribute of rotational profile to the hyperon puzzle in the prediction of heaviest compact star
• Effects of the symmetry energy on the kaon condensates in the QMC Model
• Finite particle number description of neutron matter using the unitary correlation operator and high-momentum pair methods
• Electromagnetic Interactions in a Chiral Effective Lagrangian for Nuclei
• Ensembles of unified crust and core equations of state in a nuclear-multimessenger astrophysics environment
• The nuclear symmetry energy and the neutron skin thickness in nuclei
• Softness of Sn isotopes in relativistic semi-classical approximation
• Superfluidity of $\Lambda$ hyperons in warm strange hadronic star matter
• Effect of Wigner energy on the symmetry energy coefficient in nuclei
• Ab initio computations of the fourth-order charge density moments of ${}^{48}$Ca and ${}^{208}$Pb
• Can the nuclear symmetry potential at supra-saturation densities be negative?
• From noise to information: The transfer function formalism for uncertainty quantification on nuclear density reconstruction
• Detecting Hyperons in neutron stars -- a machine learning approach
• Neutron star equation of state: identifying hadronic matter characteristics
• Quark matter symmetry energy effect on equation of state for neutron stars
• The Diffuse Supernova Neutrino Background in the Standard and Double Collapse Models
• Pure Neutron Matter Constraints and Nuclear Symmetry Energy
• Triton-3He relative and differential flows and the high density behavior of nuclear symmetry energy
• Symmetry potentials and in-medium nucleon-nucleon cross sections within the Nambu-Jona-Lasinio model in relativistic impulse approximation
• Experimental nuclear astrophysics in Italy
• An Undergraduate Approach to the Quantum Hadrodynamics and the Physics of Neutron Stars
• Isospin Constraints on the Parametric Coupling Model for Nuclear Matter
• A study of nuclear radii and neutron skin thickness of neutron-rich nuclei near the neutron drip line
• Density dependence of symmetry energy and neutron skin thickness revisited using relativistic mean field models with nonlinear couplings
• Parity Violation, the Neutron Radius of Lead, and Neutron Stars
• A new probe to study symmetry energy at low density by deuteron breakup reaction
• Density dependence of isospin observables in spinodal decomposition
• Design and characterisation of an antiproton deceleration beamline for the PUMA experiment
• On the possible existence of a soft dipole mode in 8He
• Connecting Relativistic Density Functional Theory to Microscopic Calculations
• Pygmy resonances and symmetry energy
• Neutron stars in general relativity and scalar-tensor theory of gravity
• Study of nuclear matter properties for Hybrid EoS
• Low-Density Instability of Multi-Component Matter with Trapped Neutrinos
• Pairing effects on neutron matter equation of state and symmetry energy at subsaturation densities
• Strongly interacting matter in extreme magnetic fields
• Aspects of approximation in modelling of the symmetry energy
• Novel effects of electromagnetic interaction on the correlation of nucleons in nuclear matter
• Sensitivity of deexcitation energies of superdeformed secondary minima to the density dependence of symmetry energy with the relativistic mean-field theory
• Pygmies, giants, and skins as laboratory constraints on the equation of state of neutron-rich matter
• Dense Hadronic Matter in Neutron Stars
• Strong correlation of the neutron star core-crust transition density with the $\sigma$-meson mass via vacuum polarization
• Novel features of asymmetric nuclear matter from terrestrial experiments and astrophysical observations of neutron stars
• Electric dipole response of sd-shell nuclei within the Configuration-Interaction Shell Model approach
• Neutron stars as a dense liquid drop at equilibrium within the effective surface approximation
• Novel halos in light kaonic nuclei as an indicator of nuclear equation of state at supra-normal densities
• Neutron Star Radii from Laboratory Experiments
• Direct Inference of Nuclear Equation-of-State Parameters from Gravitational-Wave Observations
• Elimination of influence of neutron-skin size difference of initial colliding nuclei in Pb+Pb collisions
• Properties of glitching pulsars in the Skyrme-Hartree-Fock framework
• Many Facets of Strangeness Nuclear Physics with Stored Antiprotons
• Density Dependence of Nuclear Symmetry Energy
• Neutron rich matter, neutron stars, and their crusts
• Can a hybrid star with constant sound speed parametrization explain the new NICER mass-radius measurements ?
• Pygmies, Giants, and Skins
• New solution to the hyperon puzzle of neutron stars: Quantum many-body effects
• Probing small neutron skin variations in isotope pairs by hyperon-antihyperon production in antiproton--nucleus interactions
• Investigation of ground state properties and shape evolution in Hf isotopes using the CDFT approach
• Microscopic Investigation of Ground State Properties and Shape Evolution in Osmium Isotopes
• Neutron stars with Bogoliubov quark-meson coupling model
• Neutron star properties: Constraining the nuclear matter EoS
• Characterization of the inner edge of the neutron star crust
• Model-independent determination of nuclear charge radii from Li-like ions
• Rotating Neutron Stars with Dark Matter Halos
• Landau parameters and entrainment matrix of cold stellar matter: effect of the symmetry energy and strong magnetic fields
• Light clusters as a possible source of crustal impurities: a quasi-particle approach
• Origins and Impacts of High-Density Symmetry Energy
• Ground-state properties of light kaonic nuclei signaling symmetry energy at high densities
• Compact Stars in Hadron and Quark-Hadron Models
• Finite particle-number description of symmetric nuclear matter with spin excitations of high-momentum pairs induced by tensor force
• Modeling Ultra-High-Energy Cosmic Rays propagation using the input from Configuration Interaction Shell Model
• Leptodermic corrections to the TOV equations and nuclear astrophysics within the effective surface approximation
• Investigating the possibility of extracting neutron-skin thickness in nuclei by their collisions at intermediate energies
• Influence of hyperon-hyperon interaction on the properties of neutron stars
• Learning about neutron star composition from the slope of the mass-radius diagram
• The pygmy dipole strength, the neutron radius of ${}^{208}$Pb and the symmetry energy
• The Nuclear Physics of Neutron Stars
• Macroscopic approaches to rotating neutron stars
• Investigating the weak charge of ${}^{48}$Ca using a dispersive optical model
• Effects of isoscalar- and isovector-scalar meson mixing on neutron star structure
• Unified Equation of State for Neutron Stars Based on the Gogny Interaction
• Detectability of continuous gravitational waves from magnetically deformed neutron stars
• Recent applications of the subtracted second RPA method
• Toward a Unified Understanding of the Dense Matter Equation of State
• Isentropic thermodynamics across the hadron-quark mixed phase in a two-phase model with a PNJL quark description
• A neutron star model in the nonlinear Relativistic Mean-Field Theory
• Low Density Neutron Star Matter with Quantum Molecular Dynamics: The Role of Vector Interactions