Isospin Asymmetry in Nuclei and Neutron Stars

Abstract

The roles of isospin asymmetry in nuclei and neutron stars are investigated using a range of potential and field-theoretical models of nucleonic matter. The parameters of these models are fixed by fitting the properties of homogeneous bulk matter and closed-shell nuclei. We discuss and unravel the causes of correlations among the neutron skin thickness in heavy nuclei, the pressure of beta-equilibrated matter at a density of 0.1 fm${}^{-3}$, the derivative of the nuclear symmetry energy at the same density and the radii of moderate mass neutron stars. Constraints on the symmetry properties of nuclear matter from the binding energies of nuclei are examined. The extent to which forthcoming neutron skin measurements will further delimit the symmetry properties is investigated. The impact of symmetry energy constraints for the mass and moment of inertia contained within neutron star crusts and the threshold density for the nucleon direct Urca process, all of which are potentially measurable, is explored. We also comment on the minimum neutron star radius, assuming that only nucleonic matter exists within the star.

49 pages, 17 figures, Phys. Rep. (in press); made improvements to "RAPR" and corrected transition densities

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• The equation of state for nucleon matter and neutron star structure
• Neutron Star Structure and the Equation of State
• Determination of the Equation of State of Dense Matter
• The Physics of Neutron Stars
• Neutron Star Structure and the Neutron Radius of 208Pb
• Composition and Structure of Protoneutron Stars
• Quantum Monte Carlo Calculations of Light Nuclei
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• Transverse momentum analysis of collective motion in relativistic nuclear collisions
• Relativistic Mean-Field Theory and the High-Density Nuclear Equation of State
• Neutron Radii in Mean-Field Models
• Pulsar Constraints on Neutron Star Structure and Equation of State
• Shape Coexistence and the Effective Nucleon-Nucleon Interaction
• Parity Violating Measurements of Neutron Densities
• Isospin Fractionation in Nuclear Multifragmentation
• Isotopic Scaling in Nuclear Reactions
• Nuclear Matter and its Role in Supernovae, Neutron Stars and Compact Object Binary Mergers
• Spin-Isospin Structure and Pion Condensation in Nucleon Matter
• The neutron radii of Lead and neutron stars
• Momentum dependence of symmetry potential in asymmetric nuclear matter for transport model calculations
• Surface Symmetry Energy
• Effects of momentum-dependent symmetry potential on heavy-ion collisions induced by neutron-rich nuclei
• Isospin fractionation and isoscaling in dynamical nuclear collisions
• Constraining URCA cooling of neutron stars from the neutron radius of 208Pb
• The Thermodynamic Model for Nuclear Multifragmentation
• Discerning the neutron density distribution of 208Pb from nucleon elastic scattering
• Chemical and mechanical instabilities in hot, isospin-asymmetric nuclear matter
• Low densities in nuclear and neutron matters and in the nuclear surface
• Instabilities of infinite matter with effective Skyrme-type interactions
• Neutron Densities from a Global Analysis of Medium Energy Proton Nucleus Elastic Scattering
• Relativistic mean-field study of neutron-rich nuclei
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• Studies of the equation-of-state of nuclear matter by heavy-ion collisions at intermediate energy in the multi-messenger era
• Effect of the momentum dependence of nuclear symmetry potential on the transverse and elliptic flows
• Isobaric incompressibility of the isospin asymmetric nuclear matter
• Beyond-mean-field effects on the symmetry energy and its slope from the low-lying dipole response of ${}^{68}$Ni
• Free spectator nucleons in ultracentral relativistic heavy-ion collisions as a probe of neutron skin
• Decomposition of sensitivity of the symmetry energy observables
• Epicyclic oscillations in the Hartle-Thorne external geometry
• Nuclear collective dynamics in transport model with the lattice Hamiltonian method
• Nuclear in-medium and isospin effects on subthreshold kaon production in heavy-ion collisions
• Stability of the $\beta$-equilibrated dense matter and core-crust transition in neutron stars
• Collective flows of pions in Au+Au collisions at energies 1.0 and 1.5 GeV/nucleon
• From neutron skins and neutron matter to the neutron star crust
• Influence of differential elastic nucleon-nucleon cross section on stopping and collective flows in heavy-ion collisions at intermediate energies
• Warm asymmetric quark matter and proto-quark stars within the confined-isospin-density-dependent mass model
• Pion condensation in a soft-wall AdS/QCD model
• Relativistic r-modes and Shear viscosity: regularizing the continuous spectrum
• Hot and Dense Matter Equation of State Probability Distributions for Astrophysical Simulations
• Properties of binary components and remnant in GW170817 using equations of state in finite temperature field theory models
• Gravitational waves from isolated neutron stars: mass dependence of r-mode instability
• Generalized isobaric multiplet mass equation and its application to the Nolen-Schiffer anomaly
• Dark Lepton Superfluid in Proto-Neutron Stars
• Constraints on the nuclear symmetry energy and its density slope from the α decay process
• Role of nonlinear vector meson interactions in hyperon stars
• Observing the Ping-pong Modality of Isospin Degree of Freedom in Cluster Emission from Heavy Ion Reactions
• Constraining the nonanalytic terms in the isospin-asymmetry expansion of the nuclear equation of state
• Effects of nuclear symmetry energy and in-medium NN cross section in heavy-ion collisions at beam energies below the pion production threshold
• Thermal properties of the nuclear surface
• Effects of the U-boson on the inner edge of neutron star crusts
• Nuclear in-medium effects on $\eta$ dynamics in proton-nucleus collisions
• Correlations among symmetry energy elements in Skyrme models
• Properties of Nuclear and Neutron Matter and Thermodynamic Consistency in a Nonlinear Mean-field Approximation
• The effect of internal magnetic field on collective flow in heavy ion collisions at intermediate energies
• Novel Scalings of Neutron Star Properties from Analyzing Dimensionless Tolman--Oppenheimer--Volkoff Equations
• Effects of symmetry energy in ${}^{132}\mathrm{Sn}{+}^{124}\mathrm{Sn}$ reaction at 300 MeV/nucleon
• Impact of the nuclear equation of state on the formation of twin stars
• Effective surface properties of light, heavy, and super-heavy nuclei
• The kinks in charge radii across $N$ = 82 and 126 revisited
• Relationship between the symmetry energy and the single-nucleon potential in isospin-asymmetric nucleonic matter
• Low density expansion and isospin dependence of nuclear energy functional: comparison between relativistic and Skyrme models
• Constraining models of twin peak quasi-periodic oscillations with realistic neutron star equations of state
• Symmetry energy dependence of long timescale isospin transport
• Hot and dense matter beyond relativistic mean field theory
• New quantification of symmetry energy from neutron skin thicknesses of ${}^{48}$Ca and ${}^{208}$Pb
• Shear modulus of the hadron-quark mixed phase
• Symmetry energy of dense matter in holographic QCD
• Low-momentum interactions with Brown-Rho-Ericson scalings and the density dependence of the nuclear symmetry energy
• Isospin dependent properties of the isotopic chain of Scandium and Titanium nuclei within the relativistic mean-field formalism
• Quantifying Correlations Between Isovector Observables and the Density Dependence of Nuclear Symmetry Energy away from Saturation Density
• Roles of isoscalar hyperons in probing the density dependence of the nuclear symmetry energy
• Application of the coherent density fluctuation model to study the nuclear matter properties of finite nuclei within the relativistic mean-field formalism
• Isotropic and anisotropic neutron star structure in 4D Einstein Gauss Bonnet Gravity
• Spin transport in intermediate-energy heavy-ion collisions as a probe of in-medium spin-orbit interactions
• Bayesian inference of neutron-skin thickness and neutron-star observables based on effective nuclear interactions
• Pre-equilibrium effects in charge-asymmetric low-energy reactions
• Appearance of peak in symmetry energy at N = 126 for Pb isotopic chain within relativistic energy density functional
• Systematic study of surface properties for Ne, Na, Mg, Al and Si isotopes in a coherent density fluctuation model using the relativistic mean field formalism
• Auxiliary Function Approach for Determining Symmetry Energy at Supra-saturation Densities
• Symmetry energy properties of neutron-rich nuclei from the coherent density fluctuation model applied to nuclear matter calculations with Bonn potentials
• Effects of retarded electrical fields on observables sensitive to the high-density behavior of nuclear symmetry energy in heavy-ion collisions at intermediate energies
• Preequilibrium particle emissions and in-medium effects on the pion production in heavy-ion collisions
• Properties of quark-matter cores in massive hybrid stars
• Neutron-skin values and matter and neutron radii determined from reaction cross sections of proton scattering on ${}^{12}$C, ${}^{40,48}$Ca, ${}^{58}$Ni, ${}^{208}$Pb
• Nucleon Effective E-Mass in Neutron-Rich Matter from the Migdal-Luttinger Jump
• Symmetry energy at subsaturation densities and the neutron skin thickness of 208Pb
• Coherent-Nuclear Pion Photoproduction and Neutron Radii
• Symmetry coefficients and incompressibility of clusterized supernova matter
• Limiting symmetry energy elements from empirical evidence
• Experimental study of the ${}^{40,48}$Ca+ ${}^{40,48}$Ca reactions at 35 MeV/nucleon
• Compressibility and equation of state of finite nuclei
• Dynamics of strangeness production in heavy-ion collisions near threshold energies
• Plasmon excitations in homogeneous neutron star matter
• Nuclear expansion and symmetry energy of hot nuclei
• Temperature and density dependence of asymmetric nuclear matter and protoneutron star properties within an extended relativistic mean field model
• Charged pion production from Au + Au collisions at $\sqrt{s_{NN}}=2.4$ GeV in the Relativistic Vlasov-Uehling-Uhlenbeck model
• Nuclear Symmetry Energy and Neutron Skin Thickness of ${}^{208}Pb$ using a finite range effective interaction
• Equation of State of Neutron-Rich Matter in $d$-Dimensions
• Nuclear matter symmetry energy from generalized polarizabilities: dependences on momentum, isospin, density and temperature
• High $p_t$ squeezed-out n/p ratio as a probe of $K_{\mathrm{sym}}$ of the symmetry energy
• Nuclear condensation and symmetry energy of dilute nuclear matter: an S-matrix approach
• Beam energy dependence of the relativistic retardation effects of electrical fields on the ${\pi }^{-}/{\pi }^{+}$ ratio in heavy-ion collisions
• Nuclear breathing mode in neutron-rich Nickel isotopes: sensitivity to the symmetry energy and the role of the continuum
• Relativistic self-energy decomposition of nuclear symmetry energy and equation of state of neutron matter within QCD sum rules
• Symmetry-energy dependence of the dynamical dipole mode in the Boltzmann-Uehling-Uhlenbeck model
• Constraints on the Nuclear Symmetry Energy from Experiments, Theory and Observations
• Accurate nuclear symmetry energy at finite temperature within a BHF approach
• Determination of the density region of the symmetry energy probed by the ${\pi }^{-}/{\pi }^{+}$ ratio
• From nuclear reactions to compact stars: a unified approach
• Nuclear symmetry energy and proton-rich reactions at intermediate energies
• Flavor Symmetry and Topology Change in Nuclear Symmetry Energy for Compact Stars
• Influence of density dependent symmetry energy on Elliptical flow
• Determining the density dependence of the nuclear symmetry energy using heavy-ion reactions
• Effects of incompressibility $K_0$ in heavy-ion collisions at intermediate energies
• Core-crust transition properties of neutron stars within systematically varied extended relativistic mean-field model
• Simultaneous Extraction of the Weak Radius and the Weak Mixing Angle from Parity-Violating Electron Scattering on ${}^{12}\mathrm{C}$
• 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
• Supernova Neutrinos as a Precise Probe of Nuclear Neutron Skin
• Symmetry energy in cold dense matter
• Role of isospin physics in supernova matter and neutron stars
• Peeling away neutron skin in ultracentral collisions of relativistic nuclei
• Linear response theory in asymmetric nuclear matter for Skyrme functionals including spin-orbit and tensor terms II: Charge Exchange
• Topology change and nuclear symmetry energy in compact-star matter
• The nuclear symmetry energy from relativistic Brueckner-Hartree-Fock model
• Symmetry energy and neutron-proton radii studies with a Wigner-Heisenberg monopole-monopole interaction
• Initialization effect in heavy-ion collisions at intermediate energies
• Uncertainty Quantification for Neutrino Opacities in Core-Collapse Supernovae and Neutron Star Mergers
• Comment on "New formulas for the (-2) moment of the photoabsorption cross section, σ_(-2)"
• Finite particle number description of neutron matter using the unitary correlation operator and high-momentum pair methods
• Symmetry energy of super-dense neutron-rich matter from integrating barotropic pressures in neutron stars and heavy-ion reactions
• From noise to information: The transfer function formalism for uncertainty quantification on nuclear density reconstruction
• Neutron star crustal properties from relativistic mean-field models and bulk parameters effects
• Effect of Wigner energy on the symmetry energy coefficient in nuclei
• Revisiting the isospin relaxation time in intermediate-energy heavy-ion collisions
• Disentangling effects of collision geometry and symmetry energy in U+U collisions
• Can the nuclear symmetry potential at supra-saturation densities be negative?
• The nuclear symmetry energy and the neutron skin thickness in nuclei
• Ab initio computations of the fourth-order charge density moments of ${}^{48}$Ca and ${}^{208}$Pb
• Symmetry energy effects on isovector properties of neutron rich nuclei with a Thomas-Fermi approach
• Isoscaling in statistical fragment emission in an extended compound nucleus model
• Symmetry potentials and in-medium nucleon-nucleon cross sections within the Nambu-Jona-Lasinio model in relativistic impulse approximation
• Pure Neutron Matter Constraints and Nuclear Symmetry Energy
• Triton-3He relative and differential flows and the high density behavior of nuclear symmetry energy
• Nuclear energy density functional and the nuclear alpha decay
• Parity Violation, the Neutron Radius of Lead, and Neutron Stars
• Landau parameters for isospin asymmetric nuclear matter based on a relativistic model of composite and finite extension nucleons
• The nucleardatapy toolkit for simple access to experimental nuclear data, astrophysical observations, and theoretical predictions
• Correlation between the charge radii difference in mirror partner nuclei and the symmetry energy slope
• Symmetry Energy from Holographic QCD
• Electric dipole polarizability constraints on neutron skin and symmetry energy
• A study of nuclear radii and neutron skin thickness of neutron-rich nuclei near the neutron drip line
• A new probe to study symmetry energy at low density by deuteron breakup reaction
• Density dependence of symmetry energy and neutron skin thickness revisited using relativistic mean field models with nonlinear couplings
• Isospin Constraints on the Parametric Coupling Model for Nuclear Matter
• Pairing effects on neutron matter equation of state and symmetry energy at subsaturation densities
• Elementary excitations in homogeneous superfluid neutron star matter: role of the neutron-proton coupling
• Neutron star cooling with a dynamic stellar structure
• Blind spots of probing the high-density symmetry energy in heavy-ion collisions
• How accurately can the Extended Thomas-Fermi method describe the inner crust of a neutron star?
• Isoscalar and isovector giant resonances in 44Ca, 54Fe, 64,68Zn and 56,58,60,68Ni
• Pygmies, giants, and skins as laboratory constraints on the equation of state of neutron-rich matter
• Necessity of selfconsistent calculations for the electromagnetic field in probing the nuclear symmetry energy using pion observables in heavy-ion collisions
• Nuclear collision in strong magnetic field
• Constraining the Skyrme effective interactions and the neutron skin thickness of nuclei using isospin diffusion data from heavy ion collisions
• R-process Nucleosynthesis of Subminimal Neutron Star Explosions
• Revisit to the yield ratio of triton and ${}^3$He as an indicator of neutron-rich neck emission
• New Insights into Supradense Matter from Dissecting Scaled Stellar Structure Equations
• Constraining neutron star properties through parity-violating electron scattering experiments and relativistic point coupling interactions
• Sensitivity of deexcitation energies of superdeformed secondary minima to the density dependence of symmetry energy with the relativistic mean-field theory
• Temperature dependence of nuclear matter generalized isovector symmetry energy with Skyrme-type interactions
• Nucleon Short-Range Correlations and High-Momentum Dynamics: Implications on the Equation of State of Dense Matter
• Persistence of the N = 50 shell closure over the isotopic chains of Sc, Ti, V and Cr nuclei using relativistic energy density functional
• Anatomy of symmetry energy of dilute nuclear matter
• Sensitive dependence of isotope and isobar distribution of limiting temperatures on symmetry energy
• Density and Temperature in Heavy Ion Collisions: A Test of Classical and Quantum Approaches
• Effect of liquid drop model parameters on nuclear liquid gas phase transition
• Symmetry Energy and Universality classes of holographic QCD
• Novel halos in light kaonic nuclei as an indicator of nuclear equation of state at supra-normal densities
• Impact of choices for center-of-mass correction energy on the surface energy of Skyrme energy density functionals
• Van der Waals equation of state for asymmetric nuclear matter
• Properties of glitching pulsars in the Skyrme-Hartree-Fock framework
• Performance study of the Highly Granular Neutron Detector prototype in the BM@N experiment
• Caloric curve for nuclear liquid-gas phase transition in relativistic mean-field hadronic model
• Fluxtube Dynamics in Neutron Star Cores
• Pygmies, Giants, and Skins
• Probing the symmetry energy with isospin ratio from nucleons to fragments
• Three-body Force Effects on the Properties of Neutron-rich Nuclear Matter
• Analysis of critical parameters for nonrelativistic models in symmetric nuclear matter
• Isobaric analog state energy in deformed nuclei: a toy model
• Constraining properties of neutron stars with heavy-ion reactions in terrestrial laboratories
• Isospin Asymmetry in Nuclei, Neutron Stars, and Heavy-Ion Collisions
• Curvature correction term as a constraint for the Skyrme interaction
• Scattering effects on nuclear thermodynamic observables
• 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
• Investigating the possibility of extracting neutron-skin thickness in nuclei by their collisions at intermediate energies
• High-density Skyrmion matter and Neutron Stars
• Origins and Impacts of High-Density Symmetry Energy
• Role of thermal fluctuations in nucleation of three-flavor quark matter
• Observability of sharp phase transitions in neutron stars
• Neutron Star News and Puzzles
• Neutron Star Equation of State with Nucleon Short-Range Correlations: A Concise Review and Open Issues
• Recent applications of the subtracted second RPA method
• Symmetry energy of baryon- and neutron-rich nuclear matter
• Structure of Anisotropic Magnetized Neutron Stars in f(R,T) Gravity with Realistic Equation of State
• Effects of isoscalar- and isovector-scalar meson mixing on neutron star structure
• Investigating the weak charge of ${}^{48}$Ca using a dispersive optical model
• Angular momentum conservation and pion production in intermediate-energy heavy-ion collisions
• Evidence against nuclear polarization as source of fine-structure anomalies in muonic atoms
• Effective interaction: From nuclear reactions to neutron stars
• Probing the density dependence of symmetry energy at subsaturation density with HICs
• Incompressibility of asymmetric nuclear matter
• On the spin-isospin decomposition of nuclear symmetry energy
• Effects of isovector scalar $\delta$-meson on hypernuclei