The Nuclear Symmetry Energy

Abstract

The nuclear symmetry energy characterizes the variation of the binding energy as the neutron to proton ratio of a nuclear system is varied. This is one of the most important features of nuclear physics in general, since it is just related to the two component nature of the nuclear systems. As such it is one of the most relevant physical parameters that affect the physics of many phenomena and nuclear processes. This review paper presents a survey of the role and relevance of the nuclear symmetry energy in different fields of research and of the accuracy of its determination from the phenomenology and from the microscopic many-body theory. In recent years, a great interest was devoted not only to the Nuclear Matter symmetry energy at saturation density but also to its whole density dependence, which is an essential ingredient for our understanding of many phenomena. We analyze the nuclear symmetry energy in different realms of nuclear physics and astrophysics. In particular we consider the nuclear symmetry energy in relation to nuclear structure, astrophysics of Neutron Stars and supernovae, and heavy ion collision experiments, trying to elucidate the connections of these different fields on the basis of the symmetry energy peculiarities. The interplay between experimental and observational data and theoretical developments is stressed. The expected future developments and improvements are schematically addressed, together with most demanded experimental and theoretical advances for the next few years.

71 pages, 33 figures, accepted for publication by Progress in Particle and Nuclear Physics. arXiv admin note: text overlap with arXiv:1310.2896, arXiv:1205.2585, arXiv:nucl-ex/0610013, arXiv:1407.7625, arXiv:nucl-ex/0310024, arXiv:1101.3648, arXiv:1406.4546, arXiv:1309.5153, arXiv:1401.2074, arXiv:1210.3402, arXiv:1506.04687, arXiv:astro-ph/0407529 by other authors

References in corpus (156)

• Shapiro delay measurement of a two solar mass neutron star
• A Massive Pulsar in a Compact Relativistic Binary
• An accurate nucleon-nucleon potential with charge-independence breaking
• The equation of state for nucleon matter and neutron star structure
• Microscopic Models for Ultrarelativistic Heavy Ion Collisions
• Neutron Star Structure and the Equation of State
• Nuclear ground-state masses and deformations: FRDM(2012)
• Determination of the Equation of State of Dense Matter
• Tidal Love numbers of neutron stars
• Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions
• A unified equation of state of dense matter and neutron star structure
• Constraining neutron star tidal Love numbers with gravitational wave detectors
• Explosion Mechanisms of Core-Collapse Supernovae
• Predictions for the Rates of Compact Binary Coalescences Observable by Ground-based Gravitational-wave Detectors
• Quantum Monte Carlo calculations of nuclei with A \leq 7
• Isospin Asymmetry in Nuclei and Neutron Stars
• The Equation of State from Observed Masses and Radii of Neutron Stars
• Relativistic Equation of State of Nuclear Matter for Supernova and Neutron Star
• Core-collapse supernova equations of state based on neutron star observations
• Constraints on the symmetry energy and neutron skins from experiments and theory
• Reaction Dynamics with Exotic Beams
• Skyrme Interaction and Nuclear Matter Constraints
• Statistical Model for a Complete Supernova Equation of State
• Neutrino Emission from Neutron Stars
• Nuclear symmetry energy probed by neutron skin thickness of nuclei
• Measurement of the Neutron Radius of 208Pb Through Parity-Violation in Electron Scattering
• Towards gravitational-wave asteroseismology
• Complete electric dipole response and the neutron skin in 208Pb
• Relativistic Mean-Field Hadronic Models under Nuclear Matter Constraints
• Constraining the Symmetry Parameters of the Nuclear Interaction
• From low-momentum interactions to nuclear structure
• The maximum mass and radius of neutron stars and the nuclear symmetry energy
• The Neutron Star Mass-Radius Relation and the Equation of State of Dense Matter
• Neutron skin of 208Pb, nuclear symmetry energy, and the parity radius experiment
• Cooling neutron star in the Cassiopeia~A supernova remnant: Evidence for superfluidity in the core
• Measuring neutron-star properties via gravitational waves from binary mergers
• The information content of a new observable: the case of the nuclear neutron skin
• Parity Violating Measurements of Neutron Densities
• Constraining the neutron-proton effective mass splitting using empirical constraints on the density dependence of nuclear symmetry energy around normal density
• Constraints on the symmetry energy and on neutron skins from the pygmy resonances in 68Ni and 132Sn
• Kaon production in heavy ion reactions at intermediate energies
• The tensor part of the Skyrme energy density functional. I. Spherical nuclei
• Hyperon stars in the Brueckner-Bethe-Goldstone theory
• Strange Stars with Realistic Quark Vector Interaction and Phenomenological Density-dependent Scalar Potential
• Measurement of the pseudorapidity and transverse momentum dependence of the elliptic flow of charged particles in lead-lead collisions at sqrt(s_NN) = 2.76 TeV with the ATLAS detector
• Isotopic Scaling in Nuclear Reactions
• Isospin Fractionation in Nuclear Multifragmentation
• The Expansion Asymmetry and Age of the Cassiopeia A Supernova Remnant
• Nuclear Matter and its Role in Supernovae, Neutron Stars and Compact Object Binary Mergers
• Asymmetric Nuclear Matter from Extended Brueckner-Hartree-Fock Approach
• Spin-Isospin Structure and Pion Condensation in Nucleon Matter
• Symmetry Energy II: Isobaric Analog States
• Microscopic determination of the nuclear incompressibility within the non-relativistic framework
• Cooling neutron stars and superfluidity in their interiors
• Spectral properties of the post-merger gravitational-wave signal from binary neutron stars
• A way forward in the study of the symmetry energy: experiment, theory, and observation
• Symmetry Energy I: Semi-Infinite Matter
• Neutrino-pasta scattering: the opacity of nonuniform neutron-rich matter
• Equation-of-state dependence of the gravitational-wave signal from the ring-down phase of neutron-star mergers
• Constraint Molecular Dynamics approach to Fermionic systems
• Equation of state of asymmetric nuclear matter and collisions of neutron-rich nuclei
• The Giant Dipole Resonance as a quantitative constraint on the symmetry energy
• Neutron Star Masses and Radii from Quiescent Low-Mass X-ray Binaries
• The neutron skin thickness from the measured electric dipole polarizability in ${}^{68}$Ni, ${}^{120}$Sn, and ${}^{208}$Pb
• Gravitational Wave asteroseismology revisited
• Symmetry energy from elliptic flow in 197Au + 197Au
• Determination of the Mean-Field Momentum-Dependence using Elliptic Flow
• Spin-orbit splitting and the tensor component of the Skyrme interaction
• Neutron and Proton Transverse Emission Ratio Measurements and the Density Dependence of the Asymmetry Term of the Nuclear Equation of State
• Effective Nucleon Masses in Symmetric and Asymmetric Nuclear Matter
• Gravitational waves from neutron stars: Promises and challenges
• Systematics of pion emission in heavy ion collisions in the 1A GeV regime
• Incompressibility in finite nuclei and nuclear matter
• Density dependence of the nuclear symmetry energy: a microscopic perspective
• Coupled-cluster calculations of nucleonic matter
• Neutron skin thickness in droplet model with surface width dependence: indications of softness of the nuclear symmetry energy
• Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XI: Stabilizing neutron stars against a ferromagnetic collapse
• Systematics of central heavy ion collisions in the 1A GeV regime
• Probing high-density behavior of symmetry energy from pion emission in heavy-ion collisions
• Equation-of-State Dependent Features in Shock-Oscillation Modulated Neutrino and Gravitational-Wave Signals from Supernovae
• Nonuniform Neutron-Rich Matter and Coherent Neutrino Scattering
• Symmetry energy impact in simulations of core-collapse supernovae
• Gravitational waves from newly born, hot neutron stars
• Revealing the high-density equation of state through binary neutron star mergers
• Symmetry energy of dilute warm nuclear matter
• Unified equation of state for neutron stars on a microscopic basis
• Proto-Neutron Star Cooling with Convection: The Effect of the Symmetry Energy
• Constraining the High-Density Behavior of Nuclear Symmetry Energy with the Tidal Polarizability of Neutron Stars
• Antisymmetrized molecular dynamics with quantum branching processes for collisions of heavy nuclei
• Particle-Number Restoration within the Energy Density Functional Formalism
• Light cluster production in intermediate energy heavy-ion collisions induced by neutron-rich nuclei
• Nuclear Pasta Formation
• On the transverse momentum distribution of strange hadrons produced in relativistic heavy ion collisions
• Constraints on Neutron Star Crusts From Oscillations in Giant Flares
• Constraining the Radii of Neutron Stars with Terrestrial Nuclear Laboratory Data
• Experimental determination of the symmetry energy of a low density nuclear gas
• Microscopic calculations and energy expansions for neutron-rich matter
• The Weak Charge of the Proton and New Physics
• Symmetry energy from the nuclear collective motion: constraints from dipole, quadrupole, monopole and spin-dipole resonances
• Interplay of Neutrino Opacities in Core-collapse Supernova Simulations
• Density dependence of the symmetry energy from neutron skin thickness in finite nuclei
• Accurate nuclear masses from a three parameter Kohn-Sham DFT approach (BCPM)
• Antisymmetrized molecular dynamics of wave packets with stochastic incorporation of Vlasov equation
• Rejecting proposed dense-matter equations of state with quiescent low-mass X-ray binaries
• Nuclear Isospin Diffusivity
• Appearance of Light Clusters in Post-bounce Evolution of Core-Collapse Supernovae
• Properties of the nuclear medium
• The mass and the radius of the neutron star in the transient low mass X-ray binary SAX J1748.9-2021
• Towards a model-independent constraint of the high-density dependence of the symmetry energy
• On the Importance of the Equation of State for the Neutrino-Driven Supernova Explosion Mechanism
• Exploring the extended density-dependent Skyrme effective forces for normal and isospin-rich nuclei to neutron stars
• Information content of the low-energy electric dipole strength: correlation analysis
• Isospin Diffusion and Equilibration for Sn+Sn collisions at E/A=35 MeV
• 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
• Deviation from quark-number scaling of the anisotropy parameter v_2 of pions, kaons, and protons in Au+Au collisions at sqrt(s_NN) = 200 GeV
• Nucleon Superfluidity vs Observations of Cooling Neutron Stars
• The Dependence of the Neutrino Mechanism of Core-Collapse Supernovae on the Equation of State
• Neutron-proton elliptic flow difference as a probe for the high density dependence of the symmetry energy
• On the Maximum Mass of Neutron Stars
• Deep Crustal Heating in a Multicomponent Accreted Neutron Star Crust
• Compatibility of localized wave packets and unrestricted single particle dynamics for cluster formation in nuclear collisions
• Shear viscosity of neutron matter from realistic nucleon-nucleon interactions
• Selecting microscopic Equations of State
• Isospin dependence of nucleon effective mass in Dirac Brueckner-Hartree-Fock approach
• The Nuclear Matter Symmetry Energy at $0.03\le \rho /{\rho }_0\le 0.2$
• Effective Nucleon Masses from Heavy Ion Collisions
• Density-dependent nucleon-nucleon interaction from three-nucleon forces
• Predicting the single-proton/neutron potentials in asymmetric nuclear matter
• Constraints on the inner edge of neutron star crusts from relativistic nuclear energy density functionals
• Theoretical understanding of the nuclear incompressibility: where do we stand ?
• Relativistic Structure of the Nucleon Self-Energy in Asymmetric Nuclei
• Oscillations of hot, young neutron stars: Gravitational wave frequencies and damping times
• The equation of state and symmetry energy of low density nuclear matter
• New parameterization of Skyrme's interaction for regularized multi-reference energy density functional calculations
• Thomas-Fermi theory for atomic nuclei revisited
• KRATTA, a versatile triple telescope array for charged reaction products
• Constraining the symmetry energy content of nuclear matter from nuclear masses: a covariance analysis
• Cassiopeia A and direct URCA cooling
• Probing the high-density behavior of symmetry energy with gravitational waves
• The neutron star in Cassiopeia A: equation of state, superfluidity, and Joule heating
• Isospin dependence of relative yields of $K^{+}$ and $K^0$ mesons at 1.528 AGeV
• Revisit of the neutron/proton ratio puzzle in intermediate-energy heavy-ion collisions
• Flow probe of symmetry energy in relativistic heavy-ion reactions
• Quantum Simulations of Nuclei and Nuclear Pasta with the Multi-resolution Adaptive Numerical Environment for Scientific Simulations
• Neutron-proton effective mass splitting in neutron-rich matter and its impacts on nuclear reactions
• From the crust to the core of Neutron Stars on a microscopic basis
• Correlations between the nuclear matter symmetry energy, its slope, and curvature from a nonrelativistic solvable approach and beyond
• Simple regularization scheme for multi-reference density functional theories
• Nuclear matter equation of state from a quark-model nucleon-nucleon interaction
• ${}^3$H/${}^3$He ratio as a probe of the nuclear symmetry energy at sub-saturation densities
• Nuclear Matter from Effective Quark-Quark Interaction
• Role of the symmetry energy on the neutron-drip transition in accreting and nonaccreting neutron stars
• Stability of the mixed phase in hybrid stars
• Quantum Monte Carlo calculations of the thermal conductivity of neutron star crusts
• Novel technique to extract experimental symmetry free energy information of nuclear matter

Cited by in corpus (152)

• GW170817: Measurements of Neutron Star Radii and Equation of State
• Origin of the Heaviest Elements: the Rapid Neutron-Capture Process
• Neutron Stars and the Nuclear Equation of State
• Nuclear Equation of State from ground and collective excited state properties of nuclei
• Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817
• Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy
• Nucleon Effective Masses in Neutron-Rich Matter
• Average CsI neutron density distribution from COHERENT data
• Neutron skins of atomic nuclei: per aspera ad astra
• Extracting Nuclear Symmetry Energies at High Densities from Observations of Neutron Stars and Gravitational Waves
• Bayesian Inference of High-density Nuclear Symmetry Energy from Radii of Canonical Neutron Stars
• Effects of dark matter on the nuclear and neutron star matter
• GW190814's secondary component with mass $(2.50-2.67)$ M${}_{\odot }$ as a super-fast pulsar
• Heavy Baryons in Compact Stars
• 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
• Cosmic-ray propagation with DRAGON2: II. Nuclear interactions with the interstellar gas
• Exploring QCD matter in extreme conditions with Machine Learning
• Probing the neutron skin with ultrarelativistic isobaric collisions
• Optimizing the relativistic energy density functional with nuclear ground state and collective excitation properties
• Nuclear Equation of state for Compact Stars and Supernovae
• Feasability of constraining the curvature parameter of the symmetry energy using elliptic flow data
• Nuclear Symmetry Energy Extracted from Laboratory Experiments
• Relativistic hybrid stars in light of the NICER PSR J0740+6620 radius measurement
• Imprints of the nuclear symmetry energy on the tidal deformability of neutron stars
• Liquid-Gas phase transition in nuclei
• How tightly is nuclear symmetry energy constrained by unitary Fermi gas?
• Reinterpreting the weak mixing angle from atomic parity violation in view of the Cs neutron rms radius measurement from COHERENT
• Constraints on the nuclear symmetry energy from asymmetric-matter calculations with chiral NN and 3N interactions
• Constraints on the Symmetry Energy from PREX-II in the Multimessenger Era
• The QCD phase diagram and Beam Energy Scan physics: a theory overview
• Collision dynamics at medium and relativistic energies
• Multi-messenger and multi-physics Bayesian inference for GW170817 binary neutron star merger
• Delineating Effects of Nuclear Symmetry Energy on the Radii and Tidal Polarizabilities of Neutron Stars
• Constraints on the skewness coefficient of symmetric nuclear matter within the nonlinear relativistic mean field model
• Constraining hadron-quark phase transition parameters within the quark-mean-field model using multimessenger observations of neutron stars
• Uncertainties in the pasta-phase properties of catalysed neutron stars
• Constraints on the nuclear equation of state and the neutron star structure from crustal torsional oscillations
• Effects of Chiral Effective Field Theory Equation of State on Binary Neutron Star Mergers
• Symmetry energy at supra-saturation densities via the Gravitational Waves from GW170817
• Sensitivity of Au+Au collisions to the symmetric nuclear matter equation of state at 2 -- 5 nuclear saturation densities
• Nuclear matter properties from local chiral interactions with $\Delta$ isobar intermediate states
• Bayesian inference of nuclear symmetry energy from measured and imagined neutron skin thickness in ${}^{116,118,120,122,124,130,132}$Sn, ${}^{208}$Pb, and ${}^{48}$Ca
• Probing nuclear bubble structure via neutron star asteroseismology
• Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence
• Dense and Hot QCD at Strong Coupling
• Nuclear symmetry energy and hadron-quark mixed phase in neutron stars
• Tidal deformations of neutron stars with elastic crusts
• Impact of NICER's Radius Measurement of PSR J0740+6620 on Nuclear Symmetry Energy at Suprasaturation Densities
• Skyrme functional with tensor terms from \textit{ab initio} calculations of neutron-proton drops
• Impact of the neutron-star deformability on equation of state parameters
• New insights into nuclear physics and weak mixing angle using electroweak probes
• Thermodynamical Description of Hot, Rapidly Rotating Neutron Stars, Protoneutron Stars, and Neutron Star Merger Remnants
• Translating neutron star observations to nuclear symmetry energy via artificial neural networks
• Constraints on the curvature of nuclear symmetry energy from recent astronomical data within the KIDS framework
• Electric dipole strength and dipole polarizability in ${}^{48}$Ca within a fully self-consistent second random-phase approximation
• Determining the temperature in heavy-ion collisions with multiplicity distribution
• The interplay of short-range correlations and nuclear symmetry energy in hard photon productions from heavy-ion reactions at Fermi energies
• Ruling out the supersoft high-density symmetry energy from the discovery of PSR J0740+6620 with mass $2.14_{-0.09}^{+0.10}{M}_{\odot }$
• Constraining nuclear symmetry energy with the charge radii of mirror-pair nuclei
• Warm dense matter and cooling of supernovae remnants
• Influence of density dependence of symmetry energy in hot and dense matter for supernova simulations
• Consistent Skyrme parametrizations constrained by GW170817
• Hybrid stars in light of the HESS J1731-347 remnant and the PREX-II experiment
• Constraining the density dependence of the symmetry energy with nuclear data and astronomical observations in the KIDS framework
• Neutron Star Matter as a Relativistic Fermi Liquid
• Probing high-density nuclear symmetry energy with ${\Xi }^{-}/{\Xi }^0$ ratio in heavy-ion collisions at $\sqrt{s_{NN}}\sim 3$ GeV
• Relativistic hybrid stars with sequential first-order phase transitions in light of multimessenger constraints
• Extended Skyrme interactions for transport model simulations of heavy-ion collisions
• Constraints on Nuclear Saturation Properties from Terrestrial Experiments and Astrophysical Observations of Neutron Stars
• Dense Matter in Neutron Stars with eXTP
• The isospin dependent nucleon-nucleon inelastic cross section in the nuclear medium
• Isospin symmetry breaking in the charge radius difference of mirror nuclei
• Structure in the speed of sound: from neutron stars to heavy-ion collisions
• $R$-mode Stability of GW190814's Secondary Component as a Supermassive and Superfast Pulsar
• First results from the INDRA-FAZIA apparatus on isospin diffusion in ${}^{58,64}$Ni+${}^{58,64}$Ni systems at Fermi energies
• Equilibrium constants of Hydrogen and Helium isotopes at low nuclear densities
• Nuclear matter fourth-order symmetry energy in non-relativistic mean-field models
• Fluctuations and phases in baryonic matter
• Nuclear symmetry energy and the role of three-body forces
• Constraining equation of state of nuclear matter by charge-changing cross section measurements of mirror nuclei
• Empirical information on nuclear matter fourth-order symmetry energy from an extended nuclear mass formula
• Symmetry energy effects on the properties of hybrid stars
• BigApple force and its implications to finite nuclei and astrophysical objects
• Analysis of the neutron matter equation of state and the symmetry energy up to fourth order of chiral effective field theory
• Nuclear collective dynamics in the lattice Hamiltonian Vlasov method
• Density-dependent van der Waals model under the GW170817 constraint
• Second and fourth moments of the charge density and neutron-skin thickness of atomic nuclei
• Bayesian model averaging for nuclear symmetry energy from effective proton-neutron chemical potential difference of neutron-rich nuclei
• Massive neutron star with strangeness in a relativistic mean-field model with a high-density cut-off
• Nuclear matter at finite temperature and static properties of proto-neutron star
• Effects of the equation of state on the core-crust interface of slowly rotating neutron stars
• Effect of nucleon effective mass and symmetry energy on the neutrino mean free path in a neutron star
• Perturbation Theory of Nuclear Matter with a Microscopic Effective Interaction
• Properties of neutron star described by a relativistic $abinitio$ model
• Collective flows of pions in Au+Au collisions at energies 1.0 and 1.5 GeV/nucleon
• Isotopic shift and search of magic number in the superheavy region
• Effects of Coulomb and isospin symmetry breaking interactions on neutron-skin thickness
• Properties of nuclear matter in relativistic Brueckner-Hartree-Fock model with high-precision charge-dependent potentials
• Supernovae and Weinberg's Higgs Portal Dark Radiation and Dark Matter
• Might Normal Nuclear Matter be Quarkyonic?
• 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
• Neutron skin systematics from microscopic equations of state
• Nambu-Jona-Lasinio description of hadronic matter from a Bayesian approach
• Effects of retarded electrical fields on observables sensitive to the high-density behavior of nuclear symmetry energy in heavy-ion collisions at intermediate energies
• Auxiliary Function Approach for Determining Symmetry Energy at Supra-saturation Densities
• Estimation of the slope of nuclear symmetry energy via charge radii of mirror nuclei
• Nuclear pasta and symmetry energy in the relativistic point-coupling model
• Charged pion production from Au + Au collisions at $\sqrt{s_{NN}}=2.4$ GeV in the Relativistic Vlasov-Uehling-Uhlenbeck model
• Effects of the momentum dependence of nuclear symmetry potential on pion observables in Sn + Sn collisions at 270 MeV/nucleon
• Neutron Stars and Gravitational Waves: the Key Role of Nuclear Equation of State
• Symmetry energy in holographic QCD
• Constraints and correlations of nuclear matter parameters from a density-dependent van der Waals model
• Accreting neutron stars from the nuclear energy-density functional theory. II. Equation of state and global properties
• Accurate nuclear symmetry energy at finite temperature within a BHF approach
• Relativistic self-energy decomposition of nuclear symmetry energy and equation of state of neutron matter within QCD sum rules
• Accelerated detection of the binary neutron star gravitational-wave background
• Impact of ground-state properties and collective excitations on the Skyrme ansatz: a Bayesian study
• Supernova Neutrinos as a Precise Probe of Nuclear Neutron Skin
• The symmetry energy $\gamma$ parameter of relativistic mean-field models
• Effects of incompressibility $K_0$ in heavy-ion collisions at intermediate energies
• Uncertainty Quantification for Neutrino Opacities in Core-Collapse Supernovae and Neutron Star Mergers
• Intrinsic Correlations Among Characteristics of Neutron-rich Matter Imposed by the Unbound Nature of Pure Neutron Matter
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• Revisiting the isospin relaxation time in intermediate-energy heavy-ion collisions
• The nuclear symmetry energy and the neutron skin thickness in nuclei
• Modeling Neutron Star Matter in the Age of Multimessenger Astrophysics
• Effects of nucleon-nucleon short-range correlation and symmetry energy on the evolution of newly born magnetars
• Necessity of selfconsistent calculations for the electromagnetic field in probing the nuclear symmetry energy using pion observables in heavy-ion collisions
• Nuclear matter calculations with the phenomenological three-nucleon interaction
• Constraining neutron star properties through parity-violating electron scattering experiments and relativistic point coupling interactions
• Neutron star calculations with the phenomenological three-nucleon force
• Approaching the conformal limit of quark matter with different chemical potentials
• High-order isospin-dependent surface tension contribution to the fourth-order symmetry energy of finite nuclei
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• Impact of choices for center-of-mass correction energy on the surface energy of Skyrme energy density functionals
• Fast neutron star cooling in light of the PREX-2 experiment
• Neutron Star Radii from Laboratory Experiments
• Probing small neutron skin variations in isotope pairs by hyperon-antihyperon production in antiproton--nucleus interactions
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• Investigating the possibility of extracting neutron-skin thickness in nuclei by their collisions at intermediate energies
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