QCD at high density: Equation of state for nuclear collisions and neutron stars
arXiv:1809.02000 · doi:10.1016/j.nuclphysa.2018.11.028
Abstract
A unified chiral mean field approach is presented for QCD thermodynamics in a wide range of temperatures and densities. The model simultaneously gives a satisfactory description of lattice QCD thermodynamics and fulfills nuclear matter and astrophysical constraints. The resulting equation of state can be incorporated in relativistic fluid-dynamical simulations of heavy-ion collisions and neutron stars mergers. Access to different regions of the QCD phase diagram can be obtained in simulations of heavy-ion data and observations of neutron star mergers.
arXiv comment4 pages, 2 figures. Contribution to the Quark Matter 2018 conference proceedings
References in corpus (18)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- The equation of state in (2+1)-flavor QCD
- Full result for the QCD equation of state with 2+1 flavors
- Chiral effective model with the Polyakov loop
- Phases of QCD: lattice thermodynamics and a field theoretical model
- Using gravitational-wave observations and quasi-universal relations to constrain the maximum mass of neutron stars
- New constraints on radii and tidal deformabilities of neutron stars from GW170817
- The QCD Equation of State to from Lattice QCD
- Nuclei in a chiral SU(3) model
- van der Waals Interactions in Hadron Resonance Gas: From Nuclear Matter to Lattice QCD
- Rotational properties of hypermassive neutron stars from binary mergers
- The hadronic SU(3) Parity Doublet Model for Dense Matter, its extension to quarks and the strange equation of state
- An effective chiral Hadron-Quark Equation of State
- Higher order quark number fluctuations via imaginary chemical potentials in QCD
- Nuclear Matter and Neutron stars in a Parity Doublet Model
- Cluster Expansion Model for QCD Baryon Number Fluctuations: No Phase Transition at
- Higher-order baryon number susceptibilities: interplay between the chiral and the nuclear liquid-gas transitions
- Critical point of nuclear matter and beam energy dependence of net proton number fluctuations
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- Probing neutron-star matter in the lab: similarities and differences between binary mergers and heavy-ion collisions
- Toward a unified equation of state for multi-messenger astronomy
- Coalescence, the thermal model and multi-fragmentation: The energy and volume dependence of light nuclei production in heavy ion collisions
- Bosonic dark matter dynamics in hybrid neutron stars
- Phase transition amplification of proton number fluctuations in nuclear collisions from a transport model approach
- Hagedorn bag-like model with a crossover transition meets lattice QCD
- Interplay between chiral dynamics and repulsive interactions