Constraints on the symmetry energy and neutron skins from experiments and theory

Abstract

The symmetry energy contribution to the nuclear Equation of State (EoS) impacts various phenomena in nuclear astrophysics, nuclear structure, and nuclear reactions. Its determination is a key objective of contemporary nuclear physics with consequences for the understanding of dense matter within neutron stars. We examine the results of laboratory experiments that have provided initial constraints on the nuclear symmetry energy and its density dependence at and somewhat below normal nuclear matter density. Some of these constraints have been derived from properties of nuclei. Others have been derived from the nuclear response to electroweak and hadronic probes. We also examine the most frequently used theoretical models that predict the symmetry energy and its slope. By comparing existing constraints on the symmetry pressure to theories, we demonstrate how the contribution of the three-body force, an essential ingredient in neutron matter models, can be determined.

28 pages, 4 figures

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Cited by in corpus (435)

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• Equations of state for supernovae and compact stars
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• Coupled-cluster computations of atomic nuclei
• Relativistic Mean-Field Hadronic Models under Nuclear Matter Constraints
• Accurate nuclear radii and binding energies from a chiral interaction
• Neutron skins and neutron stars in the multi-messenger era
• The Neutron Star Mass-Radius Relation and the Equation of State of Dense Matter
• Measuring the neutron star equation of state using X-ray timing
• Constraining the neutron-proton effective mass splitting using empirical constraints on the density dependence of nuclear symmetry energy around normal density
• Quarkyonic Matter and Neutron Stars
• Neutron star radii and crusts: uncertainties and unified equations of state
• Analytical representations of unified equations of state for neutron-star matter
• Symmetry Energy II: Isobaric Analog States
• The Nuclear Symmetry Energy
• A way forward in the study of the symmetry energy: experiment, theory, and observation
• Neutron star tidal deformability and equation of state constraints
• Ab initio predictions link the neutron skin of ${}^{208}$Pb to nuclear forces
• Global performance of covariant energy density functionals: ground state observables of even-even nuclei and the estimate of theoretical uncertainties
• Nuclear Equation of State from ground and collective excited state properties of nuclei
• The neutron skin thickness from the measured electric dipole polarizability in ${}^{68}$Ni, ${}^{120}$Sn, and ${}^{208}$Pb
• Constraining the Mass and Radius of Neutron Stars in Globular Clusters
• Gravitational waves from neutron star mergers and their relation to the nuclear equation of state
• Neutron skin of ${}^{208}$Pb from Coherent Pion Photoproduction
• Nuclear forces and their impact on neutron-rich nuclei and neutron-rich matter
• Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817
• Incompressibility in finite nuclei and nuclear matter
• Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy
• Nucleon Effective Masses in Neutron-Rich Matter
• Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of ${}^{208}$Pb with Minimal Modeling Assumptions
• Coupled-cluster calculations of nucleonic matter
• Electric dipole polarizability of ${}^{48}$Ca and implications for the neutron skin
• Constraining the symmetry energy at subsaturation densities using isotope binding energy difference and neutron skin thickness
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• Electric Dipole Polarizability in ${}^{208}$Pb: insights from the Droplet Model
• Constraining twin stars with GW170817
• Constraining the nuclear matter equation of state around twice saturation density
• Using Neutron Star Observations to Determine Crust Thicknesses, Moments of Inertia, and Tidal Deformabilities
• Probing the Symmetry Energy with the Spectral Pion Ratio
• Improved Mass and Radius Constraints for Quiescent Neutron Stars in Omega Cen and NGC 6397
• Unified equation of state for neutron stars on a microscopic basis
• Giant Quadrupole Resonances in 208Pb, the nuclear symmetry energy and the neutron skin thickness
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• Constraining the High-Density Behavior of Nuclear Symmetry Energy with the Tidal Polarizability of Neutron Stars
• Understanding transport simulations of heavy-ion collisions at 100 and 400 AMeV: Comparison of heavy ion transport codes under controlled conditions
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• Average CsI neutron density distribution from COHERENT data
• Three-Nucleon Forces: Implementation and Applications to Atomic Nuclei and Dense Matter
• The equation of state of neutron matter, symmetry energy, and neutron star structure
• (No) neutron star maximum mass constraint from hypernuclei
• Direct Astrophysical Tests of Chiral Effective Field Theory at Supranuclear Densities
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• Pulsar Glitches: The Crust may be Enough
• Extracting Nuclear Symmetry Energies at High Densities from Observations of Neutron Stars and Gravitational Waves
• Constraining the equation of state of high-density cold matter using nuclear and astronomical measurements
• Equation of State for Nucleonic and Hyperonic Neutron Stars with Mass and Radius Constraints
• Bayesian Inference of High-density Nuclear Symmetry Energy from Radii of Canonical Neutron Stars
• New relativistic effective interaction for finite nuclei, infinite nuclear matter and neutron stars
• Towards order-by-order calculations of the nuclear and neutron matter equations of state in chiral effective field theory
• Density dependence of the symmetry energy from neutron skin thickness in finite nuclei
• Equation of state for neutron stars in SU(3) flavor symmetry
• Symmetric nuclear matter from the strong interaction
• Hypernuclear matter in a complete SU(3) symmetry group
• Accurate nuclear masses from a three parameter Kohn-Sham DFT approach (BCPM)
• Neutron Star Mass-Radius Constraints of the Quiescent Low-mass X-ray Binaries X7 and X5 in the Globular Cluster 47 Tuc
• Delta isobars and nuclear saturation
• Neutron skin thickness of heavy nuclei with $\alpha$-particle correlations and the slope of the nuclear symmetry energy
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• GW190814's secondary component with mass $(2.50-2.67)$ M${}_{\odot }$ as a super-fast pulsar
• Quadrupole moments of rotating neutron stars and strange stars
• Heavy Baryons in Compact Stars
• Nuclear and neutron-star matter from local chiral interactions
• On the Induced Gravitational Collapse of a Neutron Star to a Black Hole by a Type Ib/c Supernova
• New equations of state constrained by nuclear physics, observations, and QCD calculations of high-density nuclear matter
• Equation of state effects in core-collapse supernovae
• Critical Density and Impact of $\Delta (1232)$ Resonance Formation in Neutron Stars
• Strong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturation
• Towards a model-independent constraint of the high-density dependence of the symmetry energy
• A Detailed Examination of Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of ${}^{208}$Pb with Minimal Modeling Assumptions
• The Vlasov formalism for extended relativistic mean field models: the crust-core transition and the stellar matter equation of state
• Electric Dipole Polarizability in ${}^{208}$Pb as a Probe of the Symmetry Energy and Neutron Matter around ${\rho }_0/3$
• Bayesian Inference of the Symmetry Energy of Super-Dense Neutron-Rich Matter from Future Radius Measurements of Massive Neutron Stars
• Dynamics of clusters and fragments in heavy-ion collisions
• Chiral EFT based nuclear forces: Achievements and challenges
• Treating quarks within neutron stars
• Determination of the Equation of State from Nuclear Experiments and Neutron Star Observations
• Constraints on symmetry energy and nucleon effective mass splitting with Heavy Ion Collisions
• Correlations between emission timescale of fragments and isospin dynamics in ${}^{124}$Sn+${}^{64}$Ni and ${}^{112}$Sn+${}^{58}$Ni reactions at 35 AMeV
• Symmetry Energy III: Isovector Skins
• Determine the neutron skin type by relativistic isobaric collisions
• Bayesian analysis of the crust-core transition with a compressible liquid-drop model
• Constraints on the symmetry energy and its associated parameters from nuclei to neutron stars
• Towards grounding nuclear physics in QCD
• Is a Trineutron Resonance Lower in Energy than a Tetraneutron Resonance?
• Extreme Matter meets Extreme Gravity: Ultra-heavy neutron stars with crossovers and first-order phase transitions
• Equation of state constraints from nuclear physics, neutron star masses, and future moment of inertia measurements
• Decoding the Density Dependence of the Nuclear Symmetry Energy
• Thermal properties of hot and dense matter with finite range interactions
• Has a thick neutron skin in ${}^{208}$Pb been ruled out?
• Isovector properties of the Gogny interaction
• Low-energy electric dipole response in 120Sn
• Thermal properties of supernova matter: The bulk homogeneous phase
• Probing the neutron skin with ultrarelativistic isobaric collisions
• Possible Constraints on the Density Dependence of the Nuclear Symmetry Energy from Quasiperiodic Oscillations in Soft Gamma Repeaters
• Nuclear Equation of state for Compact Stars and Supernovae
• Higher-order symmetry energy and neutron star core-crust transition with Gogny forces
• Symmetry energy of cold nucleonic matter within a relativistic mean field model encapsulating effects of high momentum nucleons induced by short-range correlations
• Tomography of Ultra-relativistic Nuclei with Polarized Photon-gluon Collisions
• Charge radii in covariant density functional theory: a global view
• Evaluated Experimental Isobaric Analogue States from $T=1/2$ to $T=3$ and associated IMME coefficients
• Feasability of constraining the curvature parameter of the symmetry energy using elliptic flow data
• Electric dipole polarizability from first principles calculations
• Hyperonic stars and the symmetry energy
• Perturbative QCD and the Neutron Star Equation of State
• Low-energy dipole strength in 112,120Sn
• A lower limit on the heat capacity of the neutron star core
• Selecting microscopic Equations of State
• Functional renormalization group studies of nuclear and neutron matter
• Probing neutron-proton dynamics by pions
• Cooling of hypernuclear compact stars
• From asymmetric nuclear matter to neutron stars: a functional renormalization group study
• Imprints of the nuclear symmetry energy on the tidal deformability of neutron stars
• Reinterpreting the weak mixing angle from atomic parity violation in view of the Cs neutron rms radius measurement from COHERENT
• Probing mass-radius relation of protoneutron stars from gravitational-wave asteroseismology
• Relativistic Mean-Field Models with Scaled Hadron Masses and Couplings: Hyperons and Maximum Neutron Star Mass
• Electric and magnetic dipole modes in high-resolution inelastic proton scattering at $0^{\circ }$
• How tightly is nuclear symmetry energy constrained by unitary Fermi gas?
• Generic Constraints on the Relativistic Mean-Field and Skyrme-Hartree-Fock Models from the Pure Neutron Matter Equation of State
• Constraints on the nuclear symmetry energy from asymmetric-matter calculations with chiral NN and 3N interactions
• Medium effects on pion production in heavy ion collisions
• An Upper Bound on Neutron Star Masses from Models of Short Gamma-ray Bursts
• Dirac-Brueckner-Hartree-Fock versus chiral effective field theory
• Constraining the density slope of nuclear symmetry energy at subsaturation densities using electric dipole polarizability in ${}^{208}$Pb
• Equation of state for neutron stars with hyperons and quarks in relativistic Hartree-Fock approximation
• Progress of Quantum Molecular Dynamics model and its applications in Heavy Ion Collisions
• The surface properties of neutron-rich exotic nuclei within relativistic mean field formalisms
• Experimental effects on dynamics and thermodynamics in nuclear reactions on the symmetry energy as seen by the CHIMERA 4$\pi$ detector
• Delineating Effects of Nuclear Symmetry Energy on the Radii and Tidal Polarizabilities of Neutron Stars
• Computational Nuclear Quantum Many-Body Problem: The UNEDF Project
• Quark-Meson Coupling Model, Nuclear Matter Constraints and Neutron Star Properties
• Constraints on the skewness coefficient of symmetric nuclear matter within the nonlinear relativistic mean field model
• Cooling of Small and Massive Hyperonic Stars
• EoS for massive neutron stars
• Constraining the high-density nuclear symmetry energy with the transverse-momentum dependent elliptic flow
• Effective Nucleon Masses from Heavy Ion Collisions
• Quantum Nuclear Pasta and Nuclear Symmetry Energy
• Imprint of the symmetry energy on the inner crust and strangeness content of neutron stars
• Symmetry Energy Constraints from Giant Resonances: A Theoretical Overview
• Imposing multi-physics constraints at different densities on the Neutron Star Equation of State
• On the effect of high order empirical parameters on the nuclear equation of state
• Constraints on the nuclear equation of state and the neutron star structure from crustal torsional oscillations
• Possible identifications of newly observed magnetar quasi-periodic oscillations as crustal shear modes
• Effects of short-range correlation reduced kinetic symmetry energy in heavy-ion collisions at intermediate energies
• Crustal heating in accreting neutron stars from the nuclear energy-density functional theory. I. Proton shell effects and neutron-matter constraint
• Constraints on the symmetry energy from observational probes of the neutron star crust
• Trends of Neutron Skins and Radii of Mirror Nuclei from First Principles
• Neutron skins of ${}^{208}$Pb and ${}^{48}$Ca from pionic probes
• Giant Pulsar Glitches and the Inertia of Neutron-Star Crusts
• Neutrino emission from binary neutron star mergers: characterizing light curves and mean energies
• The neutron skin thickness of ${}^{48}$Ca from a nonlocal-dispersive-optical-model analysis
• Electric and magnetic dipole strength in 112,114,116,118,120,124Sn
• Symmetry energy: nuclear masses and neutron stars
• Extended Skyrme interactions for nuclear matter, finite nuclei and neutron stars
• Symmetry energy in nuclear density functional theory
• Difference in proton radii of mirror nuclei as a possible surrogate for the neutron skin
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• The role of strangeness in hybrid stars and possible observables
• Probing nuclear bubble structure via neutron star asteroseismology
• Constraining compact star properties with nuclear saturation parameters
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• Electric dipole response of 208Pb from proton inelastic scattering: constraints on neutron skin thickness and symmetry energy
• Effects of the liquid-gas phase transition and cluster formation on the symmetry energy
• Are nuclear matter properties correlated to neutron star observables ?
• Weak Polarized Electron Scattering
• Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence
• Determining the nuclear neutron distribution from Coherent Elastic neutrino-Nucleus Scattering: current results and future prospects
• Low-mass neutron stars: universal relations, the nuclear symmetry energy and gravitational radiation
• Insights into nuclear saturation density from parity violating electron scattering
• Implications of parity-violating electron scattering experiments on ${}^{48}$Ca (CREX) and ${}^{208}$Pb (PREX-II) for nuclear energy density functionals
• Tidal deformations of neutron stars with elastic crusts
• Nuclear matter properties with nucleon-nucleon forces up to fifth order in the chiral expansion
• The scenario of two families of compact stars 1. Equations of state, mass-radius relations and binary systems
• Broken SU(6) symmetry and massive hybrid stars
• A Neutron Star is born
• Model dependence of the neutron-skin thickness on the symmetry energy
• Impact of the equation-of-state -- gravity degeneracy on constraining the nuclear symmetry energy from astrophysical observables
• Computing the dipole polarizability of 48Ca with increased precision
• Reconciling Nuclear and Astrophysical Constraints
• Neutron star structure and collective excitations of finite nuclei
• Nuclear isospin asymmetry in $\alpha$ decays of heavy nuclei
• Pion Production in Rare Isotope Collisions
• Probing nuclear structure with mean transverse momentum in relativistic isobar collisions
• Probing nuclear symmetry energy at high densities using pion, kaon, eta and photon productions in heavy-ion collisions
• A dispersive optical model analysis of ${}^{208}$Pb generating a neutron-skin prediction beyond the mean field
• Nuclear charge radii of silicon isotopes
• Asymmetric nuclear matter in relativistic mean-field models with isoscalar- and isovector-meson mixing
• Nucleon self-energies for supernova equations of state
• Covariance Analysis of Symmetry Energy Observables from Heavy Ion Collision
• The $d^{\ast }(2380)$ in neutron stars - a new degree of freedom?
• In-medium nuclear cluster energies within the Extended Thomas-Fermi approach
• The nuclear symmetry energy from neutron skins and pure neutron matter in a Bayesian framework
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• Measurement of the nuclear symmetry energy parameters from gravitational wave events
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• Constraining the symmetry energy content of nuclear matter from nuclear masses: a covariance analysis
• Observational constraints on neutron star crust-core coupling during glitches
• Electroweak probes of ground state densities
• Density-dependent symmetry energy at subsaturation densities from nuclear mass differences
• Probing the high-density behavior of symmetry energy with gravitational waves
• The Radius of PSR J0740+6620 from NICER and XMM-Newton Data
• Nuclear fourth-order symmetry energy and its effects on neutron star properties in the relativistic Hartree-Fock theory
• The scenario of two families of compact stars 2. Transition from hadronic to quark matter and explosive phenomena
• Positioning the neutron drip line and the r-process paths in the nuclear landscape
• The interplay of short-range correlations and nuclear symmetry energy in hard photon productions from heavy-ion reactions at Fermi energies
• Constraints on the Neutron Skin and the Symmetry Energy from the Anti-analog Giant Dipole Resonance in 208Pb
• Insights on pion production mechanism and symmetry energy at high density
• Influence of neutron-skin thickness on ${\pi }^{-}/{\pi }^{+}$ ratio in Pb+Pb collisions
• Symmetry potential of $\Delta (1232)$ resonance and its effects on the ${\pi }^{-}/{\pi }^{+}$ ratio in heavy-ion collisions near the pion production threshold
• Application of machine learning in the determination of impact parameter in the ${}^{132}$Sn+${}^{124}$Sn system
• Constraining nuclear symmetry energy with the charge radii of mirror-pair nuclei
• Symmetry energy systematics and its high density behavior
• Consistent Skyrme parametrizations constrained by GW170817
• Radii of neutron drops probed via the neutron skin thickness of nuclei
• Flow probe of symmetry energy in relativistic heavy-ion reactions
• Temperature dependence of the symmetry energy and neutron skins in Ni, Sn, and Pb isotopic chains
• Cooling of hypernuclear compact stars: Hartree-Fock models and high-density pairing
• EoS constraints from nuclear masses and radii in a meta-modeling approach
• Resonant Shattering Flares as Multimessenger Probes of the Nuclear Symmetry Energy
• Role of vector channel in different classes of (non) magnetized neutron stars
• Constraints on Nuclear Saturation Properties from Terrestrial Experiments and Astrophysical Observations of Neutron Stars
• Correlation of the neutron star crust-core properties with the slope of the symmetry energy and the lead skin thickness
• Probing high-density nuclear symmetry energy with ${\Xi }^{-}/{\Xi }^0$ ratio in heavy-ion collisions at $\sqrt{s_{NN}}\sim 3$ GeV
• Relativistic Effects and Three-Nucleon Forces in Nuclear Matter and Nuclei
• Tensor force effects and high-momentum components in the nuclear symmetry energy
• Volume and surface contributions to the nuclear symmetry energy within the coherent density fluctuation model
• From the crust to the core of Neutron Stars on a microscopic basis
• Efficacy of crustal superfluid neutrons in pulsar glitch models
• The effect of isoscalar-isovector coupling in infinite nuclear matter
• Isospin symmetry breaking in the charge radius difference of mirror nuclei
• Isospin observables from fragment energy spectra
• Exact versus Taylor-expanded energy density in the study of the neutron star crust-core transition
• Mass and radius relations of quarkyonic stars using an excluded volume model
• Phase transitions in Core-Collapse Supernova Matter at sub-saturation densities
• Hyperon star in a modified quark meson coupling model
• Modification of magicity towards the dripline and its impact on electron-capture rates for stellar core-collapse
• Asymmetric Nuclear Matter and Neutron Star Properties in Relativistic ab initio Theory in the Full Dirac Space
• Determination of the symmetry energy from the neutron star equation of state
• Probing crustal structures from neutron star compactness
• Nuclear matter equation of state from a quark-model nucleon-nucleon interaction
• Hot and Dense Homogeneous Nucleonic Matter Constrained by Observations, Experiment, and Theory
• Implications of comprehensive nuclear and astrophysics data on the equations of state of neutron star matter
• Delta baryons in neutron stars
• ${}^3$H/${}^3$He ratio as a probe of the nuclear symmetry energy at sub-saturation densities
• Constraining equation of state of nuclear matter by charge-changing cross section measurements of mirror nuclei
• Nuclear symmetry energy and the role of three-body forces
• Timescale for equilibration of N/Z gradients in dinuclear systems
• Effect of isospin asymmetry in nuclear system
• Search for the chiral magnetic effect in collisions between two isobars with deformed and neutron-rich nuclear structures
• Charge-exchange scattering to the isobaric analog state at medium energies as a probe of the neutron skin
• Crust-core transition of a neutron star: effects of the symmetry energy and temperature under strong magnetic fields
• Anti-analog giant dipole resonances and the neutron skin of nuclei
• Measuring neutron skin by grazing isobaric collisions
• Pasta properties of the neutron star within effective relativistic mean-field model
• Symmetry energy effects on the properties of hybrid stars
• Numerical models for stationary superfluid neutron stars in general relativity with realistic equations of state
• Crustal properties of a neutron star within an effective relativistic mean-field model
• Neutron Density Distributions of Neutron-Rich Nuclei Studied with the Isobaric Yield Ratio Difference
• Effects of nuclear symmetry energy on eta meson production and its rare decay to the dark U-boson in heavy-ion reactions
• Proton and neutron density distributions at supranormal density in low- and medium-energy heavy-ion collisions
• Theoretical predictions of experimental observables sensitive to the symmetry energy: Results of the SMF transport model
• Role of the symmetry energy on the neutron-drip transition in accreting and nonaccreting neutron stars
• Analysis of the neutron matter equation of state and the symmetry energy up to fourth order of chiral effective field theory
• Emulating \emph{ab initio} computations of infinite nucleonic matter
• Isospin effects and symmetry energy studies with INDRA
• Neutron-skin effect in direct-photon and charged hadron-production in Pb+Pb collisions at the LHC
• Effect of nuclear saturation parameters on possible maximum mass of neutron stars
• Second and fourth moments of the charge density and neutron-skin thickness of atomic nuclei
• Constraints on neutron skin thickness in 208Pb and density-dependent symmetry energy
• Influence of the treatment of initialization and mean-field potential on the neutron to proton yield ratios
• Magnetar QPOs and neutron star crust elasticity
• Systematic analysis of inner crust composition using the extended Thomas-Fermi approximation with pairing correlations
• Temperature dependence of the volume and surface contributions to the nuclear symmetry energy within the coherent density fluctuation model
• First Determination of the 27Al Neutron Distribution Radius from a Parity-Violating Electron Scattering Measurement
• Strange Hadron Spectroscopy with Secondary KL Beam in Hall D
• Beyond-mean-field effects on the symmetry energy and its slope from the low-lying dipole response of ${}^{68}$Ni
• Decomposition of sensitivity of the symmetry energy observables
• Heavy-ion Collisions: Direct and indirect probes of the density and temperature dependence of Esym
• Studies of the equation-of-state of nuclear matter by heavy-ion collisions at intermediate energy in the multi-messenger era
• Collective flows of pions in Au+Au collisions at energies 1.0 and 1.5 GeV/nucleon
• From NS observations to nuclear matter properties: a machine learning approach
• Effects of the Symmetry Energy and its Slope on Neutron Star Properties
• Properties of quark matter and hybrid stars from a quasiparticle model
• Influence of differential elastic nucleon-nucleon cross section on stopping and collective flows in heavy-ion collisions at intermediate energies
• Constraining nuclear matter parameters from correlation systematics:a mean-field perspective
• From neutron skins and neutron matter to the neutron star crust
• Studying the parameters of the extended $\sigma$-$\omega$ model for neutron star matter
• Properties of Hybrid Stars with Density Dependent Bag Model
• Theoretical tools for neutrino scattering: interplay between lattice QCD, EFTs, nuclear physics, phenomenology, and neutrino event generators
• Constraining the density dependence of the nuclear symmetry energy from an X-ray bursting neutron star
• Impact parameter smearing effects on isospin sensitive observables in heavy ion collisions
• Constraints on the nuclear symmetry energy and its density slope from the α decay process
• Effects of hadron-quark phase transition on properties of Neutron Stars
• Neutron-skin thickness of 208Pb from the energy of the anti-analog giant dipole resonance
• Nuclear skin and the curvature of the symmetry energy
• Exploiting neutron-rich radioactive ion beams to constrain the symmetry energy
• Small radii of neutron stars as an indication of novel in-medium effects
• Microscopic approach to the nucleon-nucleon effective interaction and nucleon-nucleon scattering in symmetric and isospin-asymmetric nuclear matter
• 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
• The effect of internal magnetic field on collective flow in heavy ion collisions at intermediate energies
• Bayesian Inference of dense matter equation of state of neutron star with antikaon condensation
• Effects of nuclear symmetry energy and in-medium NN cross section in heavy-ion collisions at beam energies below the pion production threshold
• Variation of delta baryon mass and hybrid star properties in static and rotating conditions
• Constraints on the dense matter equation of state and neutron star properties from NICER's mass-radius estimate of PSR J0740+6620 and multimessenger observations
• The kinks in charge radii across $N$ = 82 and 126 revisited
• The effect of Lorentz-like force on collective flows of K${}^{+}$ in Au+Au collisions at 1.5 GeV/nucleon}{The effect of Lorentz-like force on collective flows of $K^{+}$ in Au+Au collisions at 1.5 GeV/nucleon
• Competition between Coulomb and Symmetry Potential in Semi-peripheral Heavy-ion Collisions
• Nuclear symmetry energy with mesonic cross-couplings in the effective chiral model
• Solving Tolman-Oppenheimer-Volkoff equations in f(T) gravity: a novel approach applied to some realistic equations of state
• Symmetry energy dependence of long timescale isospin transport
• Effects of nuclear matter properties in neutron star mergers
• Impact of initial fluctuations and nuclear deformations in isobar collisions
• Light clusters in warm stellar matter: calibrating the cluster couplings
• Symmetry energy, unstable nuclei, and neutron star crusts
• The neutron star inner crust: an empirical essay
• Neutron skin systematics from microscopic equations of state
• Polytropic fits of modern and unified equations of state
• 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
• Application of the coherent density fluctuation model to study the nuclear matter properties of finite nuclei within the relativistic mean-field formalism
• The ASY-EOS experiment at GSI: investigating the symmetry energy at supra-saturation densities
• Self consistent calculation of the nuclear composition in hot and dense stellar matter
• Measuring the surface thickness of the weak charge density of nuclei
• Nucleon Effective E-Mass in Neutron-Rich Matter from the Migdal-Luttinger Jump
• Elliptic flow in heavy-ion collisions at intermediate energy: the role of impact parameter, mean field potential, and collision term
• Properties of Neutron Stars with hyperon cores in parameterized hydrostatic conditions
• The full weak charge density distribution of 48Ca from parity violating electron scattering
• Auxiliary Function Approach for Determining Symmetry Energy at Supra-saturation Densities
• Effects of neutron-skin thickness on direct hard photon emission from reactions induced by the neutron-rich projectile ${}^{50}$Ca
• KATANA - a charge-sensitive triggering system for the S$\pi$RIT experiment
• Effects of retarded electrical fields on observables sensitive to the high-density behavior of nuclear symmetry energy in heavy-ion collisions at intermediate energies
• Coherent-Nuclear Pion Photoproduction and Neutron Radii
• Properties of quark-matter cores in massive hybrid stars
• Isospin dependence of nucleon Correlations in ground state nuclei
• Nuclear Symmetry Energy and Neutron Skin Thickness of ${}^{208}Pb$ using a finite range effective interaction
• Determining the neutron skin thickness by relativistic semi-isobaric collisions
• Limiting symmetry energy elements from empirical evidence
• On the possibility of rho-meson condensation in neutron stars
• Accreting neutron stars from the nuclear energy-density functional theory. II. Equation of state and global properties
• Neutron density distribution and neutron skin thickness of ${}^{208}$Pb
• Probing the momentum-dependence of the symmetry potential by the free n/p ratio of preequilibrium emission
• Relativistic self-energy decomposition of nuclear symmetry energy and equation of state of neutron matter within QCD sum rules
• Accurate nuclear symmetry energy at finite temperature within a BHF approach
• Pairing effects on spinodal decomposition of asymmetric nuclear matter
• Deconfinement of non-strange hadronic matter with nucleons and $\Delta$ baryons to quark matter in neutron stars
• Impact of the neutron matter equation of state on neutron skin and neutron drip lines in chiral effective field theory
• The Radius of PSR J0437-4715 from NICER Data
• Testing the formation scenarios of binary neutron star systems with measurements of the neutron star moment of inertia
• Neutrino diffusion in the pasta phase matter within the Thomas-Fermi approach
• Exploring pathways to forming twin stars
• Probing the density dependence of the symmetry energy by nucleon flow
• Sensitivity of the evaporation residue observables to the symmetry energy
• Properties of ${}^{208}$Pb predicted from the relativistic equation of state in the full Dirac space
• EOSDB: The Database for Nuclear EoS
• Equation of state in neutron stars and supernovae
• The nuclear symmetry energy from relativistic Brueckner-Hartree-Fock model
• Optimized Statistical Approach for Comparing Multi-Messenger Neutron Star Data
• Effects of the symmetry energy on the kaon condensates in the QMC Model
• Ensembles of unified crust and core equations of state in a nuclear-multimessenger astrophysics environment
• Investigation of constraints on few-neutron forces in neutron matter by empirical information on the neutron skin of 48Ca and 208Pb
• Symmetry energy softening in nuclear matter with non-nucleonic constituents
• Recent progress on the determination of the symmetry Energy
• Multi-Strangeness Production in Hadron Induced Reactions
• Isospin diffusion from ${}^{40,48}$Ca${+}^{40,48}$Ca experimental data at Fermi energies: Direct comparisons with transport model calculations
• Photoneutron cross section measurements on ${}^{208}$Pb in the Giant Dipole Resonance region
• Symmetry energy effects on isovector properties of neutron rich nuclei with a Thomas-Fermi approach
• Analytical mass formula and nuclear surface properties in the ETF approximation
• Critical properties of calibrated relativistic mean-field models for the transition to warm, non-homogeneous nuclear matter
• Exploring sensitivity of charge-exchange ($p,n$) reactions to the neutron density distribution
• New Skyrme energy density functional for a better description of the Gamow-Teller Resonance
• Baryonic matter and the medium modification of the baryon masses
• Constraints on the symmetry energy from neutron star observations
• Symmetry energy of super-dense neutron-rich matter from integrating barotropic pressures in neutron stars and heavy-ion reactions
• Neutron star structure in an in-medium modified chiral soliton model
• CompOSE - CompStar Online Supernovae Equations of State
• Exploring $\Delta$-resonance in neutron stars: implications from astrophysical and nuclear observations
• Role of $\Delta$s in determining the properties of Neutron Stars in parameterized hydrostatic equilibrium
• Equation of state and neutrino transfer in supernovae and neutron stars
• A new probe to study symmetry energy at low density by deuteron breakup reaction
• Effects of pairing correlations on the neutron skin thickness and the symmetry energy
• Electric dipole polarizability constraints on neutron skin and symmetry energy
• Symmetry potentials and in-medium nucleon-nucleon cross sections within the Nambu-Jona-Lasinio model in relativistic impulse approximation
• Persistence of the N = 50 shell closure over the isotopic chains of Sc, Ti, V and Cr nuclei using relativistic energy density functional
• Constraining neutron star properties through parity-violating electron scattering experiments and relativistic point coupling interactions
• On the impact of non-local gravity on compact stars
• Dynamics of one-dimensional correlated nuclear systems within non-equilibrium Green's function theory
• Nucleon Short-Range Correlations and High-Momentum Dynamics: Implications on the Equation of State of Dense Matter
• The nuclear symmetry energy and other isovector observables from the point of view of nuclear structure
• Strong correlation of the neutron star core-crust transition density with the $\sigma$-meson mass via vacuum polarization
• Probing neutron skin and symmetry energy with relativistic isobar collisions
• Sensitive dependence of isotope and isobar distribution of limiting temperatures on symmetry energy
• Density Dependence of Nuclear Symmetry Energy
• Novel features of asymmetric nuclear matter from terrestrial experiments and astrophysical observations of neutron stars
• Constraint on the internal structure of a neutron star from Vela pulsar glitches
• The equation of state of neutron star matter and the symmetry energy
• From nuclear structure to neutron stars
• Analytic insights on the information content of new observables
• Probing small neutron skin variations in isotope pairs by hyperon-antihyperon production in antiproton--nucleus interactions
• In-medium $\Delta (1232)$ potential, pion production in heavy-ion collisions and the symmetry energy
• Nuclear coherent ${\pi }^0$ photoproduction with charge-exchange and spin-flip rescattering
• Nuclear Symmetry Energy: constraints from Giant Quadrupole Resonances and Parity Violating Electron Scattering
• The role of strangeness and isospin in low density expansions of hadronic matter
• High density matter
• Estimation of neutron star mass and radius of FRB 20240114A by identification of crustal oscillations
• Effects of Neutron-Proton Short-Range Correlation on the Equation of State of Dense Neutron-Rich Nucleonic Matter
• Ground-state properties of light kaonic nuclei signaling symmetry energy at high densities
• Neutron-rich nuclei and the equation of state of stellar matter
• Origins and Impacts of High-Density Symmetry Energy
• Chiral nucleon-nucleon forces in nuclear structure calculations
• Correlations between isospin dynamics and Intermediate Mass Fragments emission time scales: a probe for the symmetry energy in asymmetric nuclear matter
• The EOS of neutron matter and the effect of $\Lambda$ hyperons to neutron star structure
• Finding signatures of the nuclear symmetry energy in heavy-ion collisions with deep learning
• Unified Equation of State for Neutron Stars Based on the Gogny Interaction
• European Spallation Source: a future for Coherent Neutrino Nucleus Scattering
• Neutron Star Equation of State with Nucleon Short-Range Correlations: A Concise Review and Open Issues
• Neutron skins probed in proton knockout from neutron-rich nuclei
• Recent applications of the subtracted second RPA method
• Transport Model Comparison Studies of Intermediate-Energy Heavy-Ion Collisions
• Implications of nuclear interaction for nuclear structure and astrophysics within the relativistic mean-field model
• Unlocking the initial neutron density distribution from the two-pion HBT correlation function in heavy-ion collisions
• Study of nucleonic matter with a consistent two- and three-body perturbative chiral interaction
• $\beta$-delayed $\gamma$-proton decay in ${}^{56}$Zn: analysis of the charged-particle spectrum
• Investigating the weak charge of ${}^{48}$Ca using a dispersive optical model