Results of the ASY-EOS experiment at GSI: The symmetry energy at suprasaturation density
arXiv:1608.04332 · doi:10.1103/PhysRevC.94.034608
Abstract
Directed and elliptic flows of neutrons and light charged particles were measured for the reaction 197Au+197Au at 400 MeV/nucleon incident energy within the ASY-EOS experimental campaign at the GSI laboratory. The detection system consisted of the Large Area Neutron Detector LAND, combined with parts of the CHIMERA multidetector, of the ALADIN Time-of-flight Wall, and of the Washington-University Microball detector. The latter three arrays were used for the event characterization and reaction-plane reconstruction. In addition, an array of triple telescopes, KRATTA, was used for complementary measurements of the isotopic composition and flows of light charged particles. From the comparison of the elliptic flow ratio of neutrons with respect to charged particles with UrQMD predictions, a value γ= 0.72 \pm 0.19 is obtained for the power-law coefficient describing the density dependence of the potential part in the parametrization of the symmetry energy. It represents a new and more stringent constraint for the regime of supra-saturation density and confirms, with a considerably smaller uncertainty, the moderately soft to linear density dependence deduced from the earlier FOPI-LAND data. The densities probed are shown to reach beyond twice saturation.
25 pages, 22 figures, accepted for publication in Physical Review C
References in corpus (18)
- Neutron Star Observations: Prognosis for Equation of State Constraints
- Transverse momentum analysis of collective motion in relativistic nuclear collisions
- Probing Cold Dense Nuclear Matter
- Momentum sharing in imbalanced Fermi systems
- Constraints on the Symmetry Energy Using the Mass-Radius Relation of Neutron Stars
- Symmetry energy from elliptic flow in 197Au + 197Au
- Systematics of pion emission in heavy ion collisions in the 1A GeV regime
- Symmetry Energy of Nucleonic Matter With Tensor Correlations
- Systematics of Stopping and Flow in Au+Au Collisions
- Isospin dependent multifragmentation of relativistic projectiles
- Constraining the high-density nuclear symmetry energy with the transverse-momentum dependent elliptic flow
- Effects of short-range correlation reduced kinetic symmetry energy in heavy-ion collisions at intermediate energies
- Thermal and Chemical Freeze-out in Spectator Fragmentation
- Double neutron-proton differential transverse flow as a probe for the high-density behavior of the nuclear symmetry energy
- KRATTA, a versatile triple telescope array for charged reaction products
- Normal or abnormal isospin-fractionation as a qualitative probe of nuclear symmetry energy at supradensities
- A model comparison of resonance lifetime modifications, a soft equation of state and non-Gaussian effects on correlations at FAIR/AGS energies
- Decomposition of sensitivity of the symmetry energy observables
Cited by in corpus (95)
- Constraining Neutron-Star Matter with Microscopic and Macroscopic Collisions
- Neutron star tidal deformability and equation of state constraints
- Neutron Stars and the Nuclear Equation of State
- Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817
- Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy
- Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of Pb with Minimal Modeling Assumptions
- Dense Nuclear Matter Equation of State from Heavy-Ion Collisions
- A Detailed Examination of Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of Pb with Minimal Modeling Assumptions
- 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
- Determination of the Equation of State from Nuclear Experiments and Neutron Star Observations
- Constraints on the symmetry energy and its associated parameters from nuclei to neutron stars
- Decoding the Density Dependence of the Nuclear Symmetry Energy
- An updated nuclear-physics and multi-messenger astrophysics framework for binary neutron star mergers
- Transport approaches for the Description of Intermediate-Energy Heavy-Ion Collisions
- 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
- Ranking Love numbers for the neutron star equation of state: The need for third-generation detectors
- Imposing multi-physics constraints at different densities on the Neutron Star Equation of State
- Symmetry energy constraints from GW170817 and laboratory experiments
- Horizons: Nuclear Astrophysics in the 2020s and Beyond
- Multi-physics constraints at different densities to probe nuclear symmetry energy in hyperonic neutron stars
- Impact of the neutron-star deformability on equation of state parameters
- Probing Quarkyonic Matter in Neutron Stars with the Bayesian Nuclear-Physics Multi-Messenger Astrophysics Framework
- Bayesian reconstruction of nuclear matter parameters from the equation of state of neutron star matter
- The interplay of short-range correlations and nuclear symmetry energy in hard photon productions from heavy-ion reactions at Fermi energies
- Insights on pion production mechanism and symmetry energy at high density
- Quantifying modeling uncertainties when combining multiple gravitational-wave detections from binary neutron star sources
- Constraints on Nuclear Saturation Properties from Terrestrial Experiments and Astrophysical Observations of Neutron Stars
- Probing high-density nuclear symmetry energy with ratio in heavy-ion collisions at GeV
- Structure in the speed of sound: from neutron stars to heavy-ion collisions
- Bayesian inference of multimessenger astrophysical data: Joint and coherent inference of gravitational waves and kilonovae
- Asymmetric Nuclear Matter and Neutron Star Properties in Relativistic ab initio Theory in the Full Dirac Space
- Implications of comprehensive nuclear and astrophysics data on the equations of state of neutron star matter
- Constraining three-nucleon forces with multimessenger data
- Fluctuations and phases in baryonic matter
- Symmetry energy extracted from the SRIT pion data in Sn+Sn systems
- 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
- Neutron star matter based on a parity doublet model including the meson
- Nuclear collective dynamics in the lattice Hamiltonian Vlasov method
- Influence of the treatment of initialization and mean-field potential on the neutron to proton yield ratios
- Effect of nucleon effective mass and symmetry energy on the neutrino mean free path in a neutron star
- Feasibility of dark matter admixed neutron star based on recent observational constraints
- Perturbation Theory of Nuclear Matter with a Microscopic Effective Interaction
- Studies of the equation-of-state of nuclear matter by heavy-ion collisions at intermediate energy in the multi-messenger era
- Nuclear collective dynamics in transport model with the lattice Hamiltonian method
- Constraining nuclear matter parameters from correlation systematics:a mean-field perspective
- Bayesian inference of the dense matter equation of state built upon extended Skyrme interactions
- Embedding short-range correlations in relativistic density functionals through quasi-deuterons
- Equation of state of nuclear matter and neutron stars: Quark mean-field model versus relativistic mean-field model
- Novel Scalings of Neutron Star Properties from Analyzing Dimensionless Tolman--Oppenheimer--Volkoff Equations
- The effect of internal magnetic field on collective flow in heavy ion collisions at intermediate energies
- Properties of nuclear matter in relativistic Brueckner-Hartree-Fock model with high-precision charge-dependent potentials
- Effect of the -cut potential on the properties of neutron stars with or without a hyperonic core
- Nuclear symmetry energy with mesonic cross-couplings in the effective chiral model
- Effects of nuclear matter properties in neutron star mergers
- Astrophysics with heavy-ion beams
- Experimental study of the isospin transport with 40,48 Ca+ 40,48 Ca reactions at 35 MeV/nucleon
- A CsI hodoscope on CSHINE for Bremsstrahlung γ-rays in Heavy Ion Reactions
- Prospects for Direct Detection of Black Hole Formation in Neutron Star Mergers with Next-Generation Gravitational-Wave Detectors
- Neutron skin systematics from microscopic equations of state
- Elliptic flow in heavy-ion collisions at intermediate energy: the role of impact parameter, mean field potential, and collision term
- Probing dense QCD matter in the laboratory: The CBM experiment at FAIR
- Experimental study of the Ca+ Ca reactions at 35 MeV/nucleon
- Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Nucleonic models
- Effects of the momentum dependence of nuclear symmetry potential on pion observables in Sn + Sn collisions at 270 MeV/nucleon
- Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis
- Nuclear Symmetry Energy and Neutron Skin Thickness of using a finite range effective interaction
- Constraining nucleon effective masses with flow and stopping observables from the SRIT experiment
- Investigating the role of nuclear parameters on oscillation modes in hot Neutron Stars
- Astrophysics in the Laboratory: The CBM Experiment at FAIR
- The nuclear symmetry energy from relativistic Brueckner-Hartree-Fock model
- Intrinsic Correlations Among Characteristics of Neutron-rich Matter Imposed by the Unbound Nature of Pure Neutron Matter
- Isospin diffusion from CaCa experimental data at Fermi energies: Direct comparisons with transport model calculations
- Bayesian Analysis of the Neutron Star Equation of State and Model Comparison: Insights from PSR J0437+4715, PSR J0614+3329, and Other Multi-Physics Data
- The nuclear symmetry energy and the neutron skin thickness in nuclei
- The nucleardatapy toolkit for simple access to experimental nuclear data, astrophysical observations, and theoretical predictions
- From masses and radii of neutron stars to EOS of nuclear matter through neural network
- Experimental nuclear astrophysics in Italy
- Necessity of selfconsistent calculations for the electromagnetic field in probing the nuclear symmetry energy using pion observables in heavy-ion collisions
- Probing in-medium nucleon-nucleon inelastic scattering cross section by using energetic n/p ratio
- Neutron Star Radii from Laboratory Experiments
- -mode oscillations in hot Neutron Stars: Effect of hyperons and neutrino trapping
- In-medium potential, pion production in heavy-ion collisions and the symmetry energy
- Light and heavy hyperclusters in nuclear matter with relativistic-mean-field models
- Nucleon- elastic cross section in isospin-asymmetric nuclear medium with inclusion of scalar-isovector meson field
- Determination of energy-dependent neutron backgrounds using shadow bars
- Toward a Unified Understanding of the Dense Matter Equation of State
- Universal relation between dipole polarizability of finite nuclei and neutron-star compactness
- Transport Model Comparison Studies of Intermediate-Energy Heavy-Ion Collisions
- Isospin blocking and its effects in heavy-ion collisions
- Constraining the Phase-Transition EoS using the Energy Dependence of Directed Flow
- Investigating the mass-ratio dependence of the prompt-collapse threshold with numerical-relativity simulations