Determination of the Equation of State of Dense Matter
arXiv:nucl-th/0208016 · doi:10.1126/science.1078070
Abstract
Nuclear collisions can compress nuclear matter to densities achieved within neutron stars and within core-collapse supernovae. These dense states of matter exist momentarily before expanding. We analyzed the flow of matter to extract pressures in excess of 10^34 pascals, the highest recorded under laboratory-controlled conditions. Using these analyses, we rule out strongly repulsive nuclear equations of state from relativistic mean field theory and weakly repulsive equations of state with phase transitions at densities less than three times that of stable nuclei, but not equations of state softened at higher densities because of a transformation to quark matter.
26 pages, 6 figures; final version
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- Sensitivity of neutron to proton ratio toward the high density behavior of symmetry energy in heavy-ion collisions
- Neutron stars: from the inner crust to the core with the (Extended) Nambu-Jona-Lasinio model
- Efficacy of crustal superfluid neutrons in pulsar glitch models
- Enhancement of elliptic flow can signal a first order phase transition in high energy heavy ion collisions
- First analysis of anisotropic flow with Lee--Yang zeroes
- Volume and surface contributions to the nuclear symmetry energy within the coherent density fluctuation model
- Nuclear matter at high density: Phase transitions, multiquark states, and supernova outbursts
- How strange are compact star interiors ?
- Isospin observables from fragment energy spectra
- Structure in the speed of sound: from neutron stars to heavy-ion collisions
- Dense Matter in Neutron Stars with eXTP
- Relevance of equilibrium in multifragmentation
- Light cluster production at NICA
- Exact versus Taylor-expanded energy density in the study of the neutron star crust-core transition
- Neutron star cooling - a challenge to the nuclear mean field
- Bayesian inference of multimessenger astrophysical data: Joint and coherent inference of gravitational waves and kilonovae
- Hadron-Quark phase transition in the context of GW190814
- On attributes of a Rotating Neutron star with a Hyperon core
- Isospin effects on two-particle correlation functions in E/A = 61 MeV 36Ar + 112,124Sn reactions
- Toward relativistic mean-field description of -nucleus reactions
- Testing the phase transition parameters inside neutron stars with the production of protons and lambdas in relativistic heavy-ion collisions
- CREX- and PREX-II-motivated relativistic interactions and their implications for the bulk properties of nuclear matter and neutron stars
- Constraining three-nucleon forces with multimessenger data
- Hyperonic neutron stars: reconciliation between nuclear properties and NICER and LIGO/VIRGO results
- Nuclear matter equation of state from a quark-model nucleon-nucleon interaction
- Implications of comprehensive nuclear and astrophysics data on the equations of state of neutron star matter
- Folding model study of the charge-exchange scattering to the isobaric analog state and implication for the nuclear symmetry energy
- Double strangeness production as a probe of nuclear equation of state at high densities
- Nuclear matter fourth-order symmetry energy in non-relativistic mean-field models
- Asymmetric Nuclear Matter and Neutron Star Properties in Relativistic ab initio Theory in the Full Dirac Space
- Lambda hypernuclei and neutron star matter in a chiral SU(3) relativistic mean field model with a logarithmic potential
- Nuclear incompressibility and sound speed in uniform matter and finite nuclei
- QCD phase transition drives supernova explosion of a very massive star
- Delineating effects of tensor force on the density dependence of nuclear symmetry energy
- Cooling of neutron stars in "nuclear medium cooling scenario" with stiff equation of state including hyperons
- Diquark Bose-Einstein Condensation and Nuclear Matter
- Parity Violating Electron Scattering Measurements of Neutron Densities
- Nuclear symmetry energy and the role of three-body forces
- Transport model study of nuclear stopping in heavy ion collisions over an energy range from 0.09A GeV to 160A GeV
- Neutron-skin thickness of finite nuclei in relativistic mean-field models with chiral limits
- Dynamical properties of nuclear and stellar matter and the symmetry energy
- Shear viscosity from nuclear stopping
- Relativistic Mean Field Model parameterizations in the light of GW170817, GW190814, and PSR J0740 + 6620
- A method to test the coupling strength of the linear and nonlinear contributions to higher-order flow harmonics via Event Shape Engineering
- Phase transition from quark-meson coupling hyperonic matter to deconfined quark matter
- Effect of isospin asymmetry in nuclear system
- Breaking the EOS-Gravity Degeneracy with Masses and Pulsating Frequencies of Neutron Stars
- Symmetry energy effects on the properties of hybrid stars
- Empirical information on nuclear matter fourth-order symmetry energy from an extended nuclear mass formula
- The roles of deformation and orientation in heavy-ion collisions induced by light deformed nuclei at intermediate energy
- Differential isospin-fractionation in dilute asymmetric nuclear matter
- The induced surface tension contribution for the equation of state of neutron stars
- Charged -meson condensation in neutron stars
- From quarks and gluons to color superconductivity at supranuclear densities
- Symmetry energy extracted from the SRIT pion data in Sn+Sn systems
- Shear viscosity to entropy density ratio in nuclear multifragmentation
- Tidal Deformation of Neutron Stars from Microscopic Models of Nuclear Dynamics
- Extended Skyrme Equation of State in asymmetric nuclear matter
- Constraints on nuclear matter parameters of an Effective Chiral Model
- Probing in-medium spin-orbit potential with intermediate-energy heavy-ion collisions
- Energy, centrality and momentum dependence of dielectron production at collider energies in a coarse-grained transport approach
- Nonrelativistic nucleon effective masses in nuclear matter: BHF versus RHF
- Isospin-asymmetric nuclear matter
- Role of the symmetry energy on the neutron-drip transition in accreting and nonaccreting neutron stars
- Quark mean-field model for nuclear matter with or without bag
- Indirect methods in nuclear astrophysics with relativistic radioactive beams
- Phenomenological QCD equations of state for neutron stars
- Isospin splitting of pion elliptic flow in relativistic heavy-ion collisions
- Theoretical predictions of experimental observables sensitive to the symmetry energy: Results of the SMF transport model
- Isoscaling and the nuclear EOS
- Isovector Channel Role of Relativistic Mean Field Models in the Neutrino Mean Free Path
- Links Between Heavy Ion and Astrophysics
- Low density nuclear matter with light clusters in a generalized nonlinear relativistic mean-field model
- Investigation of collective radial expansion and stopping in heavy ion collisions at Fermi energies
- Nuclear symmetry energy effects on liquid-gas phase transition in hot asymmetric nuclear matter
- Proton and neutron density distributions at supranormal density in low- and medium-energy heavy-ion collisions
- Temperature dependence of single-particle properties in nuclear matter
- Deformation properties with a finite range simple effective interaction
- Repulsive properties of hadrons in lattice QCD data and neutron stars
- BigApple force and its implications to finite nuclei and astrophysical objects
- Hyperonic Neutron Star Matter in Light of GW170817
- Application of density dependent parametrization models to asymmetric nuclear matter
- Hyperon bulk viscosity and -modes of neutron stars
- Density-dependent van der Waals model under the GW170817 constraint
- Influence of charge asymmetry and isospin dependent cross-section on nuclear stopping
- Excitation of soft dipole modes in electron scattering
- Bayesian uncertainty quantification for nuclear matter incompressibility
- Nuclear collective dynamics in the lattice Hamiltonian Vlasov method
- Correlations between bulk parameters in relativistic and nonrelativistic hadronic mean-field models
- Observational constraint from the heaviest pulsar PSR J0952-0607 on the equation of state of dense matter in relativistic mean field model
- Collective flow and correlations measurements with HADES in Au+Au collisions at 1.23 AGeV
- Determining impact parameters of heavy-ion collisions at low-intermediate incident energies using deep learning with convolutional neural network
- Neutron star matter in an effective model
- Anisotropic Collective Flow of Lambda Hyperons Produced in C + C Collisions at 4.2 AGeV/c
- Effect of the momentum dependence of nuclear symmetry potential on pion-/pion+ ratio in heavy-ion collisions
- Compact Object and Neutron Stars within Eddington-Inspired Born-Infeld Theory of Gravity
- Neutron star, -stable ring-diagram equation of state and Brown-Rho scaling
- Study of spin polarized nuclear matter and finite nuclei with finite range simple effective interaction
- Comparison between the Thomas-Fermi and Hartree-Fock-Bogoliubov Methods in the Inner Crust of a Neutron Star: The Role of Pairing Correlations
- A phenomenological equation of state for isospin asymmetric nuclear matter
- Constraints on neutron skin thickness in 208Pb and density-dependent symmetry energy
- Hyperon threshold and stellar radii
- Stopping effects in U+U collisions with a beam energy of 520 MeV/nucleon
- Relativistic approach for the determination of nuclear and neutron star properties in consideration of PREX-II results
- Probing phase transition in neutron stars via the crust-core interfacial mode
- Dense nuclear matter and symmetry energy in strong magnetic fields
- Nuclear Incompressibility in Asymmetric Systems at Finite Temperature and Entropy
- Studies of the equation-of-state of nuclear matter by heavy-ion collisions at intermediate energy in the multi-messenger era
- Imprints of Nuclear Symmetry Energy on Properties of Neutron Stars
- Effect of nucleon effective mass and symmetry energy on the neutrino mean free path in a neutron star
- Nuclear matter properties at finite temperatures from effective interactions
- Symmetry energy and neutron star properties in the saturated Nambu-Jona-Lasinio model
- Perturbation Theory of Nuclear Matter with a Microscopic Effective Interaction
- Decomposition of sensitivity of the symmetry energy observables
- Isobaric incompressibility of the isospin asymmetric nuclear matter
- Effect of the momentum dependence of nuclear symmetry potential on the transverse and elliptic flows
- Spin-orbit coupling and the up-down differential transverse flow in intermediate-energy heavy-ion collisions
- Feasibility of dark matter admixed neutron star based on recent observational constraints
- Infinite matter properties and zero-range limit of nonrelativistic finite-range interactions
- Symmetry energy at subnuclear densities deduced from nuclear masses
- Nuclear matter at finite temperature and static properties of proto-neutron star
- Heavy-ion Collisions: Direct and indirect probes of the density and temperature dependence of Esym
- Repulsive potentials in dense neutron star matter and binding energy of in hypernuclei
- Impacts of symmetry energy slope on the oscillation frequencies of neutron stars with short-range correlation and admixed dark matter
- Correlation between elliptic flow and shear viscosity in intermediate-energy heavy-ion collisions
- Effects of sequential decay on collective flows and nuclear stopping power in heavy-ion collisions at intermediate energies
- Nuclear collective dynamics in transport model with the lattice Hamiltonian method
- Properties of quark matter and hybrid stars from a quasiparticle model
- Isothermal compressibility of hadronic matter formed in relativistic nuclear collisions
- Coulomb corrections to density and temperature of bosons in heavy ion collisions
- Effects of the Symmetry Energy and its Slope on Neutron Star Properties
- Nucleon radius effects on neutron stars in quark mean field model
- Constraining nuclear matter parameters from correlation systematics:a mean-field perspective
- Stability of the -equilibrated dense matter and core-crust transition in neutron stars
- The Statistical Multifragmentation Model with Skyrme Effective Interactions
- Role of nonlinear vector meson interactions in hyperon stars
- Energy release from hadron-quark phase transition in neutron stars and the axial -mode of gravitational waves
- Quarkyonic matter state of neutron stars
- Gravitational waves from isolated neutron stars: mass dependence of r-mode instability
- Effects of hadron-quark phase transition on properties of Neutron Stars
- The nucleon effective mass and its isovector splitting
- Probing Nuclear Symmetry Energy and its Imprints on Properties of Nuclei, Nuclear Reactions, Neutron Stars and Gravitational Waves
- Equation of state of nuclear matter and neutron stars: Quark mean-field model versus relativistic mean-field model
- The enhancement of in nuclear collisions at the highest densities signals a first order phase transition
- Dynamical effects of spin-dependent interactions in low- and intermediate-energy heavy-ion reactions
- Mean free path and shear viscosity in central Xe+Sn collisions below 100 MeV/nucleon
- Constraints on Skyrme Equations of State from Doubly Magic Nuclei, Ab-Initio Calculations of Low-Density Neutron Matter, and Neutron Stars
- Novel Scalings of Neutron Star Properties from Analyzing Dimensionless Tolman--Oppenheimer--Volkoff Equations
- Relationship between the symmetry energy and the single-nucleon potential in isospin-asymmetric nucleonic matter
- Spin-polarized neutron matter, the maximum mass of neutron stars, and GW170817
- Strangeness production in heavy ion reactions at intermediate energies
- What if GW190425 did not produce a black hole promptly?
- Bayesian inference of in-medium baryon-baryon scattering cross sections from HADES proton flow data
- Neutrino Electromagnetic Form Factors Effect on the Neutrino Cross Section in Dense Matter
- Effects of the U-boson on the inner edge of neutron star crusts
- The kinks in charge radii across = 82 and 126 revisited
- Exploiting neutron-rich radioactive ion beams to constrain the symmetry energy
- The effect of internal magnetic field on collective flow in heavy ion collisions at intermediate energies
- Small radii of neutron stars as an indication of novel in-medium effects
- Hadronic freeze-out in an effective relativistic mean field model
- Energy Dependent Isospin Asymmetry in Mean-Field Dynamics
- Effects of symmetry energy in reaction at 300 MeV/nucleon
- Effects of the high-momentum tail of nucleon momentum distribution on the isospin-sensitive observables
- Warm unstable asymmetric nuclear matter: critical properties and the density dependence of the symmetry energy
- Nuclear symmetry energy with mesonic cross-couplings in the effective chiral model
- Astrophysics with heavy-ion beams
- Diversities in the properties of neutron stars at a fixed neutron-skin thickness in Pb nucleus
- Effects of nuclear matter properties in neutron star mergers
- Low-momentum interactions with Brown-Rho-Ericson scalings and the density dependence of the nuclear symmetry energy
- Might Normal Nuclear Matter be Quarkyonic?
- Decoding the flow evolution in Au+Au reactions at GeV using hadron flow correlations and dileptons
- Beam energy dependence of rapidity-even dipolar flow in Au+Au collisions
- Symmetry energy of dense matter in holographic QCD
- Nambu-Jona-Lasinio description of hadronic matter from a Bayesian approach
- Spin transport in intermediate-energy heavy-ion collisions as a probe of in-medium spin-orbit interactions
- Neutron stars meet constraints from high and low energy nuclear physics
- Hard-core Radius of Nucleons within the Induced Surface Tension Approach
- From finite nuclei to neutron stars : the essential role of high-order density dependence in effective forces
- Examination of an isospin-dependent single-nucleon momentum distribution for the isospin-asymmetric nuclear matter in heavy-ion collisions
- The neutron star inner crust: an empirical essay
- The ASY-EOS experiment at GSI: investigating the symmetry energy at supra-saturation densities
- Remarks on the origin of Castillejo-Dalitz-Dyson poles
- Prospects for Direct Detection of Black Hole Formation in Neutron Star Mergers with Next-Generation Gravitational-Wave Detectors
- Properties of strange quark stars with isovector interactions
- A CsI hodoscope on CSHINE for Bremsstrahlung γ-rays in Heavy Ion Reactions
- Minimal Length, Nuclear Matter, and Neutron Stars
- Quark matter in high-mass neutron stars?
- Dark matter admixed neutron stars with a realistic nuclear equation of state from chiral nuclear interactions
- Effects of the QCD phase transition on hadronic observables in relativistic hydrodynamic simulations of heavy-ion reactions in the FAIR/NICA energy regime
- From chiral EFT to perturbative QCD: a Bayesian model mixing approach to symmetric nuclear matter
- Symmetry coefficients and incompressibility of clusterized supernova matter
- Probing dense QCD matter in the laboratory: The CBM experiment at FAIR
- Effects of chiral symmetry restoration on meson and dilepton production in relativistic heavy-ion collisions
- Symmetry energy at subsaturation densities and the neutron skin thickness of 208Pb
- Elliptic flow in heavy-ion collisions at intermediate energy: the role of impact parameter, mean field potential, and collision term
- Constraints of the variation of fundamental couplings and sensitivity of the equation of state of dense matter
- Exploring hybrid star matter at NICA and FAIR
- Properties of Neutron Stars with hyperon cores in parameterized hydrostatic conditions
- Heavy Ion Physics at RHIC
- Hadron-quark phase transition: the QCD phase diagram and stellar conversion
- Criteria for nonlinear parameters of relativistic mean field models
- Flow and Equation of State of nuclear matter at /A=0.25-1.5 GeV with the SMASH transport approach
- Properties of quark-matter cores in massive hybrid stars
- Quarkyonic matter and quarkyonic stars in an extended RMF model
- High-Order Multipole and Binary Love Number Universal Relations
- Nucleon Effective E-Mass in Neutron-Rich Matter from the Migdal-Luttinger Jump
- Experimental study of the Ca+ Ca reactions at 35 MeV/nucleon
- Effects of the momentum dependence of nuclear symmetry potential on pion observables in Sn + Sn collisions at 270 MeV/nucleon
- Neutron star structure with a new force between quarks
- Constraining the onset density for the QCD phase transition with the neutrino signal from core-collapse supernovae
- Equation of State of Neutron-Rich Matter in -Dimensions
- Probing the momentum dependence of medium modifications of the nucleon-nucleon elastic cross sections
- Constraining nucleon effective masses with flow and stopping observables from the SRIT experiment
- Role of dense matter in tidal deformations of inspiralling neutron stars and in gravitational waveform with unified equations of state
- Constraints and correlations of nuclear matter parameters from a density-dependent van der Waals model
- Limiting symmetry energy elements from empirical evidence
- Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis
- Nuclear matter symmetry energy from generalized polarizabilities: dependences on momentum, isospin, density and temperature
- Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Nucleonic models
- Saturation properties of nuclear matter in the presence of strong magnetic field
- Introduction to low-momentum effective interactions with Brown-Rho scaling and three-nucleon forces
- Energy-dependent existence of soliton in the synthesis of chemical elements
- Hadron-string cascade versus hydrodynamics in Cu+Cu collisions at GeV
- Rapidly rotating axisymmetric neutron stars with quark cores
- Nuclear Chemical and Mechanical Instability and the Liquid-Gas Phase Transition in Nuclei
- When cold, dense quarks in 1+1 and 3+1 dimensions are not a Fermi liquid
- Influence of the nuclear matter equation of state on the r-mode instability using the finite-range simple effective interaction
- Unraveling the global behavior of equation of state by explicit finite nuclei constraints
- Beam energy dependence of the relativistic retardation effects of electrical fields on the ratio in heavy-ion collisions
- High squeezed-out n/p ratio as a probe of of the symmetry energy
- Deconfinement of non-strange hadronic matter with nucleons and baryons to quark matter in neutron stars
- Relativistic self-energy decomposition of nuclear symmetry energy and equation of state of neutron matter within QCD sum rules
- Isospin asymmetric nuclear matter and properties of axisymmetric neutron stars
- Constraining Bag constant for Hybrid Neutron stars
- Neutron stars in accreting systems -- signatures of the QCD phase transition
- Symmetry energy and nucleon-nucleon cross sections
- Accurate nuclear symmetry energy at finite temperature within a BHF approach
- Accreting neutron stars from the nuclear energy-density functional theory. II. Equation of state and global properties
- From nuclear reactions to compact stars: a unified approach
- Determining the density dependence of the nuclear symmetry energy using heavy-ion reactions
- Constraining the relativistic mean-field models from PREX-2 data: Effective forces revisited
- Directed and elliptic flows of protons and deuterons in HADES Au+Au collisions at GeV
- Probing the incompressibility of dense hadronic matter near QCD phase transition in relativistic heavy-ion collisions
- Nuclear Incompressibility at Finite Temperature and Entropy
- Towards a new quark-nuclear matter EoS for applications in astrophysics and heavy-ion collisions
- Influence of density dependent symmetry energy on Elliptical flow
- Nuclear symmetry energy and proton-rich reactions at intermediate energies
- Fragment Formation in Central Heavy Ion Collisions at Relativistic Energies
- Quarkyonic Percolation and deconfinement at finite density and number of colors
- High Density with Elliptic Flows
- Role of isospin physics in supernova matter and neutron stars
- meson effects on neutron stars in the modified quark-meson coupling model
- Shell States of Neutron Rich Matter
- Probing the EOS of dense neutron-rich matter with high-energy radioactive beams
- Delineating the properties of matter in cold, dense QCD
- Competition between fermions and bosons in nuclear matter at low densities and finite temperatures
- Equation of state and hybrid star properties with the weakly interacting light U-boson in relativistic models
- Effects of incompressibility in heavy-ion collisions at intermediate energies
- Equation of state for dense supernova matter
- A model investigation of the longitudinal broadening of the transverse momentum two-particle correlator
- The influence of reconstruction criteria on the sensitive probes of the symmetry potential
- A comparative study of model ingredients: fragmentation in heavy-ion collisions using quantum molecular dynamics model
- Nuclear Matter and Nuclear Dynamics
- The Auxiliary Field Diffusion Monte Carlo Method for Nuclear Physics and Nuclear Astrophysics
- Supernova Neutrinos as a Precise Probe of Nuclear Neutron Skin
- Neutron stars: A novel equation of state with induced surface tension
- Momentum correlation of light nuclei in Au + Au collisions at = 2.0 7.7 GeV
- Quark condensate and chiral symmetry restoration in neutron stars
- Charged-particle multiplicity fluctuations in Pb-Pb collisions at = 2.76 TeV
- Intrinsic Correlations Among Characteristics of Neutron-rich Matter Imposed by the Unbound Nature of Pure Neutron Matter
- Astrophysics in the Laboratory: The CBM Experiment at FAIR
- Effects of mean-field and the softening of equation of state on elliptic flow in Au+Au collision at = 5 GeV from JAM model
- The attribute of rotational profile to the hyperon puzzle in the prediction of heaviest compact star
- Landau quantization and neutron emissions by nuclei in the crust of a magnetar
- Current Status of Nuclear Physics Research
- Cooling of neutron stars and hybrid stars with a stiff hadronic EoS
- Probing the nuclear EOS with fragment production
- Equation of state at high densities and modern compact star observations
- Proton-nucleus elastic scattering and the equation of state of nuclear matter
- Can the nuclear symmetry potential at supra-saturation densities be negative?
- Strangeness thermodynamic instabilities in hot and dense nuclear matter
- Critical Properties of Symmetric Nuclear Matter in Low-Density Regime Using Effective-Relativistic Mean Field Formalism
- Neutron star structure in an in-medium modified chiral soliton model
- Disentangling effects of collision geometry and symmetry energy in U+U collisions
- Pygmy resonances probed with electron scattering
- Alternative Formulation of the Induced Surface and Curvature Tensions Approach
- Effect of Wigner energy on the symmetry energy coefficient in nuclei
- Exploring sensitivity of charge-exchange () reactions to the neutron density distribution
- The effect of inclusion of resonances in relativistic mean-field model with scaled hadron masses and coupling constants
- Symmetry energy effects on isovector properties of neutron rich nuclei with a Thomas-Fermi approach
- Hyperon puzzle and the RMF model with scaled hadron masses and coupling constants
- Quark deconfinement in neutron star cores and the ground state of neutral matter
- RMF models with -scaled hadron masses and couplings for description of heavy-ion collisions below 2A GeV
- Multi-Strangeness Production in Hadron Induced Reactions
- Baryonic matter and the medium modification of the baryon masses
- The finite range simple effective interaction including tensor terms
- Symmetry energy of super-dense neutron-rich matter from integrating barotropic pressures in neutron stars and heavy-ion reactions
- Production and rescattering of strange baryons at SPS energies in a transport model with hadron potentials
- Elliptic flow splitting between protons and antiprotons from hadronic potentials
- Effect of the spin-orbit interaction on flows in heavy-ion collisions at intermediate energies
- Bayesian analysis of a relativistic hadronic model constrained by recent astrophysical observations
- An Undergraduate Approach to the Quantum Hadrodynamics and the Physics of Neutron Stars
- Symmetry potentials and in-medium nucleon-nucleon cross sections within the Nambu-Jona-Lasinio model in relativistic impulse approximation
- Effects of medium-induced meson mixing on the equation of state in isospin-asymmetric nuclear matter
- The neutron and proton mass radii from the vector meson photoproduction data on the deuterium target
- Density-dependent quark mean-field model for nuclear matter and neutron stars
- Examination of STAR fixed-target data on directed flow at 3 and 4.5 GeV
- Isospin Constraints on the Parametric Coupling Model for Nuclear Matter
- Neutron star equation of state and tidal deformability with nuclear energy density functionals
- Triton-3He relative and differential flows and the high density behavior of nuclear symmetry energy
- Symmetry Energy from Holographic QCD
- Role of s in determining the properties of Neutron Stars in parameterized hydrostatic equilibrium
- The Equation of State of Dense Matter : from Nuclear Collisions to Neutron Stars
- The nucleardatapy toolkit for simple access to experimental nuclear data, astrophysical observations, and theoretical predictions
- Principal Component Analysis of Azimuthal Flow in Intermediate-Energy Heavy-Ion Reactions
- Nuclear Matter and Finite Nuclei in the Effective Chiral Model
- Novel technique to extract experimental symmetry free energy information of nuclear matter
- Pseudo Nambu-Goldstone modes in neutron stars
- Nuclear medium effect on nuclear modification factor of protons and pions in intermediate-energy heavy ion collisions
- Neutron star cooling within the equation of state with induced surface tension
- Pure Neutron Matter Constraints and Nuclear Symmetry Energy
- Evolutions of in-medium baryon-baryon scattering cross sections and stiffness of dense nuclear matter from Bayesian analyses of FOPI proton flow excitation functions
- Quark-Meson Coupling model based upon the Nambu-Jona Lasinio model
- Constraining the Skyrme effective interactions and the neutron skin thickness of nuclei using isospin diffusion data from heavy ion collisions
- Study of nuclear matter properties for Hybrid EoS
- Azimuthal dependence of two-particle transverse momentum current correlations
- Neutron-proton differential transverse flow in Sn + Sn collisions at 270 MeV/nucleon
- How do mirror charge radii constrain density dependence of the symmetry energy?
- Alpha Cluster Model of Atomic Nuclei
- How Well Do We Know The Supernova Equation of State?
- Nucleon Short-Range Correlations and High-Momentum Dynamics: Implications on the Equation of State of Dense Matter
- N/Z and N/A dependence of balance energy as a probe of symmetry energy in heavy-ion collisions
- New Insights into Supradense Matter from Dissecting Scaled Stellar Structure Equations
- Nuclear collision in strong magnetic field
- Thermal fluctuations of matter composition and quark nucleation in compact stars
- Unveiling a universal relationship between the f(R) parameter and neutron star properties
- Correlation and isospin dynamics of participant-spectator matter in neutron-rich colliding nuclei at 50 MeV/nucleon
- Beam energy and system dependence of rapidity-even dipolar flow
- Recent astrophysical observations reproduced by a short-range correlated van der Waals-type model?
- Blind spots of probing the high-density symmetry energy in heavy-ion collisions
- Temperature dependence of nuclear matter generalized isovector symmetry energy with Skyrme-type interactions
- Dense matter equation of state and neutron star properties from nuclear theory and experiment
- Do short range correlations inhibit the appearance of the nuclear pasta?
- Spinodal Instability at the Onset of Collective Expansion in Nuclear Collisions
- Novel effects of electromagnetic interaction on the correlation of nucleons in nuclear matter
- Implications of PREX--2 data on the electron--neutrino opacity in dense matter
- Necessity of selfconsistent calculations for the electromagnetic field in probing the nuclear symmetry energy using pion observables in heavy-ion collisions
- An effective Nuclear Model: from Nuclear Matter to Finite Nuclei
- Properties of the Object HESS J1731-347 as a Twin Compact Star
- Neutron Star Radii from Laboratory Experiments
- Symmetry Energy and Universality classes of holographic QCD
- High-order isospin-dependent surface tension contribution to the fourth-order symmetry energy of finite nuclei
- Probing Fundamental Physics with Gravitational Waves
- The nuclear symmetry energy and other isovector observables from the point of view of nuclear structure
- Density Functional Equation of State and Its Application to the Phenomenology of Heavy-Ion Collisions
- Reaction mechanisms in transport theories: a test of the nuclear effective interaction
- Framework for phase transitions between the Maxwell and Gibbs constructions at finite temperature
- Nuclear equation of state and finite nucleon volumes
- Equation of state for hyperonic neutron-star matter in SU(3) flavor symmetry
- Effect of liquid drop model parameters on nuclear liquid gas phase transition
- Skewness of nuclear matter and three-particle correlations
- Elimination of influence of neutron-skin size difference of initial colliding nuclei in Pb+Pb collisions
- Level inversion in kaonic nuclei and the high-density nuclear equation of state
- Effect of isoscalar and isovector scalar fields on baryon semileptonic decays in nuclear matter
- Novel features of asymmetric nuclear matter from terrestrial experiments and astrophysical observations of neutron stars
- Novel halos in light kaonic nuclei as an indicator of nuclear equation of state at supra-normal densities
- Sensitive dependence of isotope and isobar distribution of limiting temperatures on symmetry energy
- Three-body Force Effects on the Properties of Neutron-rich Nuclear Matter
- Probing the symmetry energy with isospin ratio from nucleons to fragments
- From nuclear structure to neutron stars
- Recent progress on superstrange dynamics
- Constraint on the internal structure of a neutron star from Vela pulsar glitches
- Note on neutron star equation of state in the light of GW170817
- Exotic Fluids Matching the Stress-Energy Tensor of Alcubierre Warp Drive Spacetimes
- Asymmetric nuclear matter : a variational approach
- Probing the symmetry energy at high baryon density with heavy ion collisions
- Structure and cooling of compact stars
- Chiral condensate in nuclear matter with vacuum corrections
- Singly heavy baryons in nuclear matter from an SU(3) chiral soliton model
- Tension between implications from PREX-2 data and gravitational tidal response on dense matter equation of state
- Antineutrino Opacity in Neutron Stars in the Models Constrained by Recent Terrestrial Experiments and Astrophysical Observations
- Measurement of Kaon Directed Flow in Au+Au Collisions in the High Baryon Density Region
- Constraining properties of neutron stars with heavy-ion reactions in terrestrial laboratories
- Properties and microscopic structures of dense stellar matter in RMF models
- Bayesian inference favors quark matter in neutron star interiors
- Weak Charge Form Factor Determination at the Electron-Ion Collider
- Imprints of high-density nuclear symmetry energy on the crustal fraction of neutron star moment of inertia
- Physics of Collectivity and EOS from the RHIC Beam Energy Scan Program
- Applications of the Octet Baryon Quark-Meson Coupling Model to Hybrid Stars
- Constraints from the GW170817 merger event on the nuclear matter equation of state
- A microscopic equation of state for neutron-rich matter and its effect on neutron star properties
- Role of thermal fluctuations in nucleation of three-flavor quark matter
- Neutron Star News and Puzzles
- Observability of sharp phase transitions in neutron stars
- K+'s Collective Flow in Heavy-ion Collisions predicted by Covariant Kaon Dynamics
- Isospin Diffusion in Ni-Induced Reactions at Intermediate Energies
- Production Cross Section of Neutron-Rich Calcium Isotopes in Heavy Ion Collisions
- Two-flavor hybrid stars with the Dyson-Schwinger quark model
- Effects of Symmetry Energy in the Reaction 40Ca+124Sn at 140 MeV/nucleon
- Origins and Impacts of High-Density Symmetry Energy
- Harmonic flow correlations in Au+Au reactions at 1.23 AGeV: A new testing ground for the Equation-of-State and expansion geometry
- High density matter
- Density functional approach to finite temperature nuclear properties and the role of a momentum dependent isovector interaction
- Nucleon- elastic cross section in isospin-asymmetric nuclear medium with inclusion of scalar-isovector meson field
- Isotopic Transparency in Central Xe+Sn Collisions at 100 MeV/nucleon
- Neutron-rich nuclei and the equation of state of stellar matter
- production as a probe of equation of state of dense matter near the QCD phase transition in relativistic heavy-ion collisions
- Probing potential at high and low densities via \(^3_Λ\)H production in C+C reactions
- Antikaons in neutron star studied with recent versions of relativistic mean-field models
- Heavy Neutron Star Phenomenology with an H-dibaryon
- How large is "large " for Nuclear matter?
- Light Nuclei and Hyper Nuclei Collectivity Measurements at High Baryon Density Region
- Predictions of baryon directed flow in heavy-ion collisions at high baryon density
- High-density Skyrmion matter and Neutron Stars
- Effective interaction: From nuclear reactions to neutron stars
- Isospin blocking and its effects in heavy-ion collisions
- The Nuclear Physics of Neutron Stars
- Induced surface and curvature tensions equation of state of hard spheres and its virial coefficients
- Equation of state from symmetry
- Effects of isoscalar- and isovector-scalar meson mixing on neutron star structure
- Effects of three-baryon forces on kaon condensation in hyperon-mixed matter
- Bremsstrahlung emission from nuclear reactions in compact stars
- Signatures of deconfined quark phases in binary neutron star mergers
- Unified Equation of State for Neutron Stars Based on the Gogny Interaction
- Modern compact star observations and the quark matter EoS
- Toward a Unified Understanding of the Dense Matter Equation of State
- Investigating the mass-ratio dependence of the prompt-collapse threshold with numerical-relativity simulations
- Probing the density dependence of symmetry energy at subsaturation density with HICs
- Deconfinement, naturalness and the nuclear-quark equation of state
- Incompressibility of asymmetric nuclear matter
- Formation of large chunk of nuclear matter in heavy-ion collisions
- Impact of three-nucleon forces on gravitational wave emission from neutron stars
- Basic quantities of the Equation of State in isospin asymmetric nuclear matter
- Implications of nuclear interaction for nuclear structure and astrophysics within the relativistic mean-field model
- Fragment Distribution in Reactions of Kr+Ta
- Progress Towards Determining the Density Dependence of the Nuclear Symmetry Energy Using Heavy-Ion Reactions
- Rotating NSs/QSs and recent astrophysical observations
- Dilepton production from hydrodynamically expanding fireball
- Constraining the Phase-Transition EoS using the Energy Dependence of Directed Flow
- Quantum corrections to the Relativistic mean-field theory
- Equation of State and Phase Transitions in the Nuclear and Hadronic Systems
- Neutron Star Equation of State with Nucleon Short-Range Correlations: A Concise Review and Open Issues
- Space-time regions of high baryon density and baryon stopping in heavy-ion collisions
- Common Approaches in Description of Ordinary Liquids and Hadronic Matter
- Degenerate limit thermodynamics beyond leading order for models of dense matter
- -delayed -proton decay in Zn: analysis of the charged-particle spectrum
- Isentropic thermodynamics across the hadron-quark mixed phase in a two-phase model with a PNJL quark description
- Quark-Meson Coupling Model in Heavy-Ion Collision Simulations
- A novel filtering method for generating desired density profiles of colliding nuclei