Sensitivity of Au+Au collisions to the symmetric nuclear matter equation of state at 2 -- 5 nuclear saturation densities
arXiv:2208.11996 · doi:10.1103/PhysRevC.108.034908
Abstract
We demonstrate that proton and pion flow measurements in heavy-ion collisions at incident energies ranging from 1 to 20 GeV per nucleon in the fixed target frame can be used for an accurate determination of the symmetric nuclear matter equation of state at baryon densities equal 2--4 times nuclear saturation density . We simulate Au+Au collisions at these energies using a hadronic transport model with an adjustable vector mean-field potential dependent on baryon density . We show that the mean field can be parametrized to reproduce a given density-dependence of the speed of sound at zero temperature , which we vary independently in multiple density intervals to probe the differential sensitivity of heavy-ion observables to the equation of state at these specific densities. Recent flow data from the STAR experiment at the center-of-mass energies GeV can be described by our model, and a Bayesian analysis of these data indicates a hard equation of state at and a possible phase transition at . More data at GeV, as well as a more thorough analysis of the model systematic uncertainties will be necessary for a more precise conclusion.
26 pages, 18 figures, accepted to publication in Phys Rev C, minor fixes
References in corpus (26)
- Shapiro delay measurement of a two solar mass neutron star
- A Massive Pulsar in a Compact Relativistic Binary
- A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy
- Refined Mass and Geometric Measurements of the High-Mass PSR J0740+6620
- Accurate Determination of the Neutron Skin Thickness of Pb through Parity-Violation in Electron Scattering
- Transverse momentum analysis of collective motion in relativistic nuclear collisions
- Sound velocity bound and neutron stars
- Incompressibility in finite nuclei and nuclear matter
- Phenomenological constraints on the transport properties of QCD matter with data-driven model averaging
- Direct Astrophysical Tests of Chiral Effective Field Theory at Supranuclear Densities
- Ab-initio QCD calculations impact the inference of the neutron-star-matter equation of state
- Dynamical phase trajectories for relativistic nuclear collisions
- Reaching percolation and conformal limits in neutron stars
- Comparison of Heavy-Ion Transport Simulations: Mean-field Dynamics in a Box
- Directed Flow Indicates a Crossover Deconfinement Transition in Relativistic Nuclear Collisions
- Flow and interferometry results from Au+Au collisions at = 4.5 GeV
- Momentum-dependent potential and collective flows within the relativistic quantum molecular dynamics approach based on relativistic mean-field theory
- Collision dynamics at medium and relativistic energies
- Mean-field update in the JAM microscopic model: Mean-field effects on collective flow in high-energy heavy-ion collisions at GeV energies
- "Smashing more than two": Deuteron production in relativistic heavy ion collisions via stochastic multi-particle reactions
- Phase transitions and critical behavior in hadronic transport with a relativistic density functional equation of state
- The high-density equation of state in heavy-ion collisions: Constraints from proton flow
- Effects of a phase transition on two-pion interferometry in heavy-ion collisions at GeV
- The Radius of PSR J0740+6620 from NICER and XMM-Newton Data
- The role of proton-antiproton regeneration in the late stages of heavy-ion collisions
- Impact of the Coulomb field on charged-pion spectra in few-GeV heavy-ion collisions
Cited by in corpus (26)
- Theoretical and Experimental Constraints for the Equation of State of Dense and Hot Matter
- Determination of the Equation of State from Nuclear Experiments and Neutron Star Observations
- The QCD phase diagram and Beam Energy Scan physics: a theory overview
- QCD Equation of State of Dense Nuclear Matter from a Bayesian Analysis of Heavy-Ion Collision Data
- Structure in the speed of sound: from neutron stars to heavy-ion collisions
- Applications of emulation and Bayesian methods in heavy-ion physics
- Novel Scalings of Neutron Star Properties from Analyzing Dimensionless Tolman--Oppenheimer--Volkoff Equations
- Flow and Equation of State of nuclear matter at /A=0.25-1.5 GeV with the SMASH transport approach
- Strong Gravity Extruding Peaks in Speed of Sound Profiles of Massive Neutron Stars
- Anti-flow of Mesons in the High Baryon Density Region
- Unraveling Trace Anomaly of Supradense Matter via Neutron Star Compactness Scaling
- Examination of STAR fixed-target data on directed flow at 3 and 4.5 GeV
- Ultra fast, event-by-event heavy-ion simulations for next generation experiments
- Bayesian inference of nuclear incompressibility from collective flow in mid-central Au+Au collisions at 400--1500 MeV/nucleon
- Shell quenching in nuclear charge radii based on Monte Carlo dropout Bayesian neural network
- Toward a foundation model for heavy-ion collision experiments based on point-cloud diffusion
- Novel features of asymmetric nuclear matter from terrestrial experiments and astrophysical observations of neutron stars
- SMASH as an event generator for heavy-ion collisions
- Extension of the integrated hydrokinetic model to nuclear collision energies relevant for the RHIC Beam-Energy Scan program and the research program at GSI-FAIR
- Is The Trace Anomaly at its Minimum Value at Neutron Star Centers?
- Heavy Neutron Star Phenomenology with an H-dibaryon
- production as a probe of equation of state of dense matter near the QCD phase transition in relativistic heavy-ion collisions
- The time evolution of light nuclei cumulants and ratios with a first-order phase transition in the UrQMD transport model
- Predictions of baryon directed flow in heavy-ion collisions at high baryon density
- Covariant formulation of relativistic quantum molecular dynamics for a system of interacting wave packets
- Toward a Unified Understanding of the Dense Matter Equation of State