Symmetry energy from elliptic flow in 197Au + 197Au
arXiv:1101.2361 · doi:10.1016/j.physletb.2011.02.033
Abstract
The elliptic-flow ratio of neutrons with respect to protons or light complex particles in reactions of neutron-rich systems at relativistic energies is proposed as an observable sensitive to the strength of the symmetry term in the equation of state at supra-normal densities. The results obtained from the existing FOPI/LAND data for 197Au + 197Au collisions at 400 MeV/nucleon in comparison with the UrQMD model favor a moderately soft symmetry term with a density dependence of the potential term proportional to rho/rho_0^gamma with gamma = 0.9 +- 0.4.
arXiv comment13 pages, 5 figures, submitted to Phys. Lett. B
References in corpus (34)
- Microscopic Models for Ultrarelativistic Heavy Ion Collisions
- Determination of the Equation of State of Dense Matter
- Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions
- Neutron Star Structure and the Neutron Radius of 208Pb
- Constraints on the density dependence of the symmetry energy
- Nuclear symmetry energy probed by neutron skin thickness of nuclei
- Constraints on the high-density nuclear equation of state from the phenomenology of compact stars and heavy-ion collisions
- Circumstantial evidence for a soft nuclear symmetry energy at supra-saturation densities
- Evolution of Nuclear Spectra with Nuclear Forces
- Nuclear Matter and its Role in Supernovae, Neutron Stars and Compact Object Binary Mergers
- Probing the High Density Behaviour of Nuclear Symmetry Energy with High Energy Heavy-Ion Collisions
- Systematics of pion emission in heavy ion collisions in the 1A GeV regime
- Probing high-density behavior of symmetry energy from pion emission in heavy-ion collisions
- Central Collisions of Au on Au at 150, 250 and 400 A MeV
- Excitation function of elliptic flow in Au+Au collisions and the nuclear matter equation of state
- Isospin effects on sub-threshold kaon production at intermediate energies
- Modelization of the EOS
- High Density Behaviour of Nuclear Symmetry Energy and High Energy Heavy-Ion Collisions
- Elliptic flow and system size dependence of transition energies at intermediate energies
- Systematics of Stopping and Flow in Au+Au Collisions
- Isospin emission and flows at high baryon density: a test of the symmetry potential
- Probing the equation of state with pions
- Statistical approach for supernova matter
- Relativistic effects in the search for high density symmetry energy
- Formation of hot heavy nuclei in supernova explosions
- Why is the nuclear symmetry energy so uncertain at supra-saturation densities?
- Medium modifications of the nucleon-nucleon elastic cross section in neutron-rich intermediate energy HICs
- Probing the density dependence of the symmetry potential in intermediate energy heavy ion collisions
- Double neutron-proton differential transverse flow as a probe for the high-density behavior of the nuclear symmetry energy
- Isospin dependence of relative yields of and mesons at 1.528 AGeV
- Differential Neutron-Proton Squeeze-out
- A model comparison of resonance lifetime modifications, a soft equation of state and non-Gaussian effects on correlations at FAIR/AGS energies
- The symmetry energy in nuclear reactions
- Probing the momentum dependence of medium modifications of the nucleon-nucleon elastic cross sections
Cited by in corpus (119)
- Equations of state for supernovae and compact stars
- Constraints on the symmetry energy and neutron skins from experiments and theory
- Constraining Neutron-Star Matter with Microscopic and Macroscopic Collisions
- Symmetry Energy II: Isobaric Analog States
- The Nuclear Symmetry Energy
- A way forward in the study of the symmetry energy: experiment, theory, and observation
- Results of the ASY-EOS experiment at GSI: The symmetry energy at suprasaturation density
- Strangeness in Nuclei and Neutron Stars
- Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817
- Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy
- Dense Nuclear Matter Equation of State from Heavy-Ion Collisions
- Constraining the High-Density Behavior of Nuclear Symmetry Energy with the Tidal Polarizability of Neutron Stars
- 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
- GW190814's secondary component with mass M as a super-fast pulsar
- Towards a model-independent constraint of the high-density dependence of the symmetry energy
- Bayesian Inference of the Symmetry Energy of Super-Dense Neutron-Rich Matter from Future Radius Measurements of Massive Neutron Stars
- Nuclear matter fourth-order symmetry energy in the relativistic mean field models
- Determination of the Equation of State from Nuclear Experiments and Neutron Star Observations
- Influence of Transport Variables on Isospin Transport Ratios
- The impact of energy conservation in transport models on the multiplicity ratio in heavy-ion collisions and the symmetry energy
- Decoding the Density Dependence of the Nuclear Symmetry Energy
- Neutron-proton elliptic flow difference as a probe for the high density dependence of the symmetry energy
- EMMI Rapid Reaction Task Force Meeting on 'Quark Matter in Compact Star'
- Transport approaches for the Description of Intermediate-Energy Heavy-Ion Collisions
- The Present and Future of QCD
- Feasability of constraining the curvature parameter of the symmetry energy using elliptic flow data
- Nuclear in-medium effects and collective flows in heavy-ion collisions at intermediate energies
- Elliptic flow and the symmetry energy at supra-saturation density
- Collision dynamics at medium and relativistic energies
- Progress of Quantum Molecular Dynamics model and its applications in Heavy Ion Collisions
- Equation of state of dense matter in the multimessenger era
- Experimental effects on dynamics and thermodynamics in nuclear reactions on the symmetry energy as seen by the CHIMERA 4 detector
- Constraining the high-density nuclear symmetry energy with the transverse-momentum dependent elliptic flow
- Symmetry energy constraints from GW170817 and laboratory experiments
- Hypernuclear stars from relativistic Hartree-Fock density functional theory
- Transverse emission of isospin ratios as a probe of high-density symmetry energy in isotopic nuclear reactions
- Effective mass splitting of neutron and proton and isospin emission in heavy-ion collisions
- Are nuclear matter properties correlated to neutron star observables ?
- Energy dependence of pion in-medium effects on π^-/π^+ ratio in heavy-ion collisions
- Constraining the density dependence of the symmetry energy using the multiplicity and average ratios of charged pions
- Impact of the equation-of-state -- gravity degeneracy on constraining the nuclear symmetry energy from astrophysical observables
- Probing the density dependence of symmetry energy via multifragmentation at sub-saturation densities
- Nuclear symmetry energy from the Fermi-energy difference in nuclei
- Pion Production in Rare Isotope Collisions
- Probing nuclear symmetry energy at high densities using pion, kaon, eta and photon productions in heavy-ion collisions
- KRATTA, a versatile triple telescope array for charged reaction products
- Bayesian reconstruction of nuclear matter parameters from the equation of state of neutron star matter
- Probing the high-density behavior of symmetry energy with gravitational waves
- Symmetry potential of resonance and its effects on the ratio in heavy-ion collisions near the pion production threshold
- Symmetry energy systematics and its high density behavior
- Ruling out the supersoft high-density symmetry energy from the discovery of PSR J0740+6620 with mass
- Clusterized nuclear matter in the (proto-)neutron star crust and the symmetry energy
- Flow probe of symmetry energy in relativistic heavy-ion reactions
- Cross-checking the symmetry energy at high densities
- Normal or abnormal isospin-fractionation as a qualitative probe of nuclear symmetry energy at supradensities
- Lorentz covariant nucleon self-energy decomposition of the nuclear symmetry energy
- Probing high-density nuclear symmetry energy with ratio in heavy-ion collisions at GeV
- Extended Skyrme interactions for transport model simulations of heavy-ion collisions
- Effects of in-medium nucleon-nucleon cross section on collective flow and nuclear stopping in heavy-ion collisions in the Fermi-energy domain
- Structure in the speed of sound: from neutron stars to heavy-ion collisions
- The isospin dependent nucleon-nucleon inelastic cross section in the nuclear medium
- Sensitivity of neutron to proton ratio toward the high density behavior of symmetry energy in heavy-ion collisions
- Efficacy of crustal superfluid neutrons in pulsar glitch models
- Implications of comprehensive nuclear and astrophysics data on the equations of state of neutron star matter
- H/He ratio as a probe of the nuclear symmetry energy at sub-saturation densities
- Effects of nuclear symmetry energy on eta meson production and its rare decay to the dark U-boson in heavy-ion reactions
- Understanding the symmetry energy using data from the ALADIN-2000 Collaboration taken at the GSI Large Neutron Detector
- The influence of the symmetry energy on the cone-azimuthal emission
- Analysis of the neutron matter equation of state and the symmetry energy up to fourth order of chiral effective field theory
- Theoretical predictions of experimental observables sensitive to the symmetry energy: Results of the SMF transport model
- Nuclear collective dynamics in the lattice Hamiltonian Vlasov method
- Model dependence of isospin sensitive observables at high densities
- Feasibility of dark matter admixed neutron star based on recent observational constraints
- Imprints of Nuclear Symmetry Energy on Properties of Neutron Stars
- 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
- Symmetry energy and neutron star properties in the saturated Nambu-Jona-Lasinio model
- Nuclear collective dynamics in transport model with the lattice Hamiltonian method
- Influence of differential elastic nucleon-nucleon cross section on stopping and collective flows in heavy-ion collisions at intermediate energies
- Probing Nuclear Symmetry Energy and its Imprints on Properties of Nuclei, Nuclear Reactions, Neutron Stars and Gravitational Waves
- Charged particle track reconstruction with SRIT Time Projection Chamber
- Effect of energy conservation on in-medium $\mbox{NN}\to \mbox{N}Δ$ cross section in isospin-asymmetric nuclear matter
- Effects of the U-boson on the inner edge of neutron star crusts
- Effects of nuclear symmetry energy and in-medium NN cross section in heavy-ion collisions at beam energies below the pion production threshold
- The effect of internal magnetic field on collective flow in heavy ion collisions at intermediate energies
- Exploiting neutron-rich radioactive ion beams to constrain the symmetry energy
- Effect of the -cut potential on the properties of neutron stars with or without a hyperonic core
- The ASY-EOS experiment at GSI: investigating the symmetry energy at supra-saturation densities
- The density- and isospin- dependent -formation cross section and its decay width
- KATANA - a charge-sensitive triggering system for the SRIT experiment
- Estimation of the slope of nuclear symmetry energy via charge radii of mirror nuclei
- Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Nucleonic models
- Nuclear Symmetry Energy and Neutron Skin Thickness of using a finite range effective interaction
- The cumulants of the baryon number from central Au+Au collision at = 1.23 GeVnucleon reveal the nuclear mean-field potentials
- Constraining nucleon effective masses with flow and stopping observables from the SRIT experiment
- Symmetry energy and nucleon-nucleon cross sections
- Neutron recognition in the LAND detector for large neutron multiplicity
- Beam energy dependence of the relativistic retardation effects of electrical fields on the ratio in heavy-ion collisions
- Delineating the properties of matter in cold, dense QCD
- High Density with Elliptic Flows
- Symmetry energy softening in nuclear matter with non-nucleonic constituents
- Symmetry energy of super-dense neutron-rich matter from integrating barotropic pressures in neutron stars and heavy-ion reactions
- The nuclear symmetry energy and the neutron skin thickness in nuclei
- Isospin diffusion from CaCa experimental data at Fermi energies: Direct comparisons with transport model calculations
- Disentangling effects of collision geometry and symmetry energy in U+U collisions
- Experimental nuclear astrophysics in Italy
- The nucleardatapy toolkit for simple access to experimental nuclear data, astrophysical observations, and theoretical predictions
- Aspects of approximation in modelling of the symmetry energy
- Correlation and isospin dynamics of participant-spectator matter in neutron-rich colliding nuclei at 50 MeV/nucleon
- Neutron Star Radii from Laboratory Experiments
- Correlation between nuclear temperatures and symmetry energy in sub-saturation
- Three-body Force Effects on the Properties of Neutron-rich Nuclear Matter
- In-medium potential, pion production in heavy-ion collisions and the symmetry energy
- Ground-state properties of light kaonic nuclei signaling symmetry energy at high densities
- Correlations between isospin dynamics and Intermediate Mass Fragments emission time scales: a probe for the symmetry energy in asymmetric nuclear matter
- Origins and Impacts of High-Density Symmetry Energy
- In-medium pion dispersion relation and medium correction of near the threshold energy of pion production
- Toward a Unified Understanding of the Dense Matter Equation of State