The Flow Constraint Influence on the Properties of Nuclear Matter Critical Endpoint
arXiv:1710.08218 · doi:10.1103/PhysRevC.97.064905
Abstract
We propose a novel family of equations of state for symmetric nuclear matter based on the induced surface tension concept for the hard-core repulsion. It is shown that having only four adjustable parameters the suggested equations of state can, simultaneously, reproduce not only the main properties of the nuclear matter ground state, but the proton flow constraint up its maximal particle number densities. Varying the model parameters we carefully examine the range of values of incompressibility constant of normal nuclear matter and its critical temperature which are consistent with the proton flow constraint. This analysis allows us to show that the physically most justified value of nuclear matter critical temperature is 15.5-18 MeV, the incompressibility constant is 270-315 MeV and the hard-core radius of nucleons is less than 0.4 fm.
8 pages, 3 figures
References in corpus (7)
- Relativistic Mean-Field Hadronic Models under Nuclear Matter Constraints
- Constraints on the high-density nuclear equation of state from the phenomenology of compact stars and heavy-ion collisions
- Incompressibility in finite nuclei and nuclear matter
- Critical temperature for the nuclear liquid-gas phase transition (from multifragmentation and fission)
- Correlations between critical parameters and bulk properties of nuclear matter
- Nuclear multifragmentation and fission: similarity and differences
- Hadron Resonance Gas Model for An Arbitrarily Large Number of Different Hard-Core Radii
Cited by in corpus (24)
- Bosonic Dark Matter in Neutron Stars and its Effect on Gravitational Wave Signal
- Neutron stars: new constraints on asymmetric dark matter
- What is the nature of the HESS J1731-347 compact object?
- The effects of self-interacting bosonic dark matter on neutron star properties
- Asteroseismology: radial oscillations of neutron stars with realistic equation of state
- Chirally improved quark Pauli blocking in nuclear matter and applications to quark deconfinement in neutron stars
- Rapid neutron star cooling triggered by dark matter
- Hadron resonance gas with van der Waals interactions
- The induced surface tension contribution for the equation of state of neutron stars
- Neutron stars meet constraints from high and low energy nuclear physics
- Hard-core Radius of Nucleons within the Induced Surface Tension Approach
- Self-consistent Treatment of Quantum Gases of D-dimensional Hard Spheres Beyond the Van der Waals Approximation
- On separate chemical freeze-outs of hadrons and light (anti)nuclei in high energy nuclear collisions
- Alternative Formulation of the Induced Surface and Curvature Tensions Approach
- The concept of induced surface and curvature tensions and a unified description of the gas of hard discs and hard spheres
- Relativistic energy density functional from momentum space to coordinate space within a coherent density fluctuation model
- Resolution of hyper-triton chemical freeze-out puzzle in high energy nuclear collisions
- Neutron star cooling within the equation of state with induced surface tension
- Thermal production of sexaquarks in heavy-ion collisions
- Tidal Deformability as a Probe of Dark Matter in Neutron Stars
- On relation between bulk, surface and curvature parts of nuclear binding energy within the model of hexagonal clusters
- Classical excluded volumes of loosely bound light (anti)nuclei and their chemical freeze-out in heavy ion collisions
- Induced Surface and Curvature Tensions Equation of State of Hadrons with Relativistic Excluded Volumes and its Relation to Morphological Thermodynamics
- Induced surface and curvature tensions equation of state of hard spheres and its virial coefficients