High squeezed-out n/p ratio as a probe of of the symmetry energy
arXiv:1810.13172 · doi:10.1103/PhysRevC.100.014617
Abstract
By involving the constraints of the slope of nuclear symmetry energy into the question of determination of the high-density symmetry energy, one needs to probe the curvature of nuclear symmetry energy . Based on the Isospin-dependent Boltzmann-Uehling-Uhlenbeck (IBUU) transport model, effects of the curvature of nuclear symmetry energy on the squeezed-out nucleons are demonstrated in the semi-central Au+Au reaction at 400 and 600 MeV/nucleon. It is shown that the squeezed-out isospin-dependent nucleon emissions at high transverse momenta are sensitive to the curvature of nuclear symmetry energy. The curvature of nuclear symmetry energy at saturation density thus can be determined by the high momentum squeezed-out isospin-dependent nucleon emissions experiments from the semi-central Au+Au reaction at 400 or 600 MeV/nucleon.
arXiv comment6 pages, 4 figures, Physical Review C, in press
References in corpus (59)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- GW170817: Measurements of Neutron Star Radii and Equation of State
- Neutron Star Structure and the Equation of State
- Determination of the Equation of State of Dense Matter
- The Physics of Neutron Stars
- Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions
- Equations of state for supernovae and compact stars
- Gravitational-wave constraints on the neutron-star-matter Equation of State
- Isospin Asymmetry in Nuclei and Neutron Stars
- Flow Study in Relativistic Nuclear Collisions by Fourier Expansion of Azimuthal Particle Distributions
- Reaction Dynamics with Exotic Beams
- Systematics of dynamical mass ejection, nucleosynthesis, and radioactively powered electromagnetic signals from neutron-star mergers
- Nuclear symmetry energy probed by neutron skin thickness of nuclei
- R-Process Nucleosynthesis in Dynamically Ejected Matter of Neutron Star Mergers
- Complete electric dipole response and the neutron skin in 208Pb
- Probing Cold Dense Nuclear Matter
- Neutron skin of 208Pb, nuclear symmetry energy, and the parity radius experiment
- Identifying a first-order phase transition in neutron star mergers through gravitational waves
- Signatures of quark-hadron phase transitions in general-relativistic neutron-star mergers
- The information content of a new observable: the case of the nuclear neutron skin
- Constraining the neutron-proton effective mass splitting using empirical constraints on the density dependence of nuclear symmetry energy around normal density
- Momentum sharing in imbalanced Fermi systems
- Symmetry Parameter Constraints From A Lower Bound On The Neutron-Matter Energy
- Electric dipole polarizability and the neutron skin
- Results of the ASY-EOS experiment at GSI: The symmetry energy at suprasaturation density
- The neutron skin thickness from the measured electric dipole polarizability in Ni, Sn, and Pb
- Effects of momentum-dependent symmetry potential on heavy-ion collisions induced by neutron-rich nuclei
- Density dependence of the nuclear symmetry energy: a microscopic perspective
- Multi-messenger picture of compact binary mergers
- Disappearance of Elliptic Flow: A New Probe for the Nuclear Equation of State
- Incompressibility of neutron-rich matter
- Revealing the high-density equation of state through binary neutron star mergers
- Nuclear Equation of State from Observations of Short Gamma-Ray Burst Remnants
- Near-threshold pion production with radioactive beams at the Rare Isotope Accelerator
- Dipole polarizability of 120Sn and nuclear energy density functionals
- Density dependence of the symmetry energy from neutron skin thickness in finite nuclei
- Isospin emission and flows at high baryon density: a test of the symmetry potential
- Discovery of the Neutron Star Spin Frequency in EXO 0748-676
- Double neutron/proton ratio of nucleon emissions in isotopic reaction systems as a robust probe of nuclear symmetry energy
- SRIT: A time-projection chamber for symmetry-energy studies
- Relativistic effects in the search for high density symmetry energy
- Proton Differential Elliptic Flow and the Isospin-Dependence of the Nuclear Equation of State
- Feasability of constraining the curvature parameter of the symmetry energy using elliptic flow data
- How tightly is nuclear symmetry energy constrained by unitary Fermi gas?
- Insights on Skyrme parameters from GW170817
- Constraining the equation of state of nuclear matter with gravitational wave observations: Tidal deformability and tidal disruption
- Pygmy and core polarization dipole modes in Pb: connecting nuclear structure to stellar nucleosynthesis
- Effective Nucleon Masses from Heavy Ion Collisions
- Difference in proton radii of mirror nuclei as a possible surrogate for the neutron skin
- Gravitational Waves from Compact Dark Objects in Neutron Stars
- The neutron/proton ratio of squeezed-out nucleons and the high density behavior of the nuclear symmetry energy
- The interplay of short-range correlations and nuclear symmetry energy in hard photon productions from heavy-ion reactions at Fermi energies
- Modeling pion production in heavy-ion collisions at intermediate energies
- Normal or abnormal isospin-fractionation as a qualitative probe of nuclear symmetry energy at supradensities
- Cross-checking the symmetry energy at high densities
- Constraining nucleon high momentum in nuclei
- Dynamics and Afterglow Light Curves of GRB Blast Waves Encountering a Density Bump or Void
- Azimuthal asymmetry of direct photons in intermediate energy heavy-ion collisions
- Probing the density dependence of the symmetry energy by nucleon flow
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- Initialization effects of nucleon profile on the yields in heavy-ion collisions at medium energies
- Probing in-medium nucleon-nucleon inelastic scattering cross section by using energetic n/p ratio
- Isospin blocking and its effects in heavy-ion collisions