Three-dimensional equation of state extension of quark matter in Fermi-liquid theory

Abstract

The cold, dense matter equation of state (EoS) determines crucial global properties of neutron stars (NSs), including the mass, radius and tidal deformability. However, a one-dimensional (1D), cold, and $\beta$-equilibrated EoS is insufficient to fully describe the interactions or capture the dynamical processes of dense matter as realized in binary neutron star (BNS) mergers or core-collapse supernovae (CCSNe), where thermal and out-of-equilibrium effects play important roles. We develop a method to self-consistently extend a 1D cold and $\beta$-equilibrated EoS of quark matter to a full three-dimensional (3D) version, accounting for density, temperature, and electron fraction dependencies, within the framework of Fermi-liquid theory (FLT), incorporating both thermal and out-of-equilibrium contributions. We compare our FLT-extended EoS with the original bag model and find that our approach successfully reproduces the contributions of thermal and compositional dependencies of the 3D EoS. Furthermore, we construct a 3D EoS with a first-order phase transition (PT) by matching our 3D FLT-extended quark matter EoS to the hadronic DD2 EoS under Maxwell construction, and test it through the GRHD simulations of the TOV-star and CCSN explosion. Both simulations produce consistent results with previous studies, demonstrating the effectiveness and robustness of our 3D EoS construction with PT.

17 pages, 10 figures

References in corpus (53)

• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
• A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
• A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy
• The Combined Ultraviolet, Optical, and Near-Infrared Light Curves of the Kilonova Associated with the Binary Neutron Star Merger GW170817: Unified Data Set, Analytic Models, and Physical Implications
• Signals of the QCD phase transition in core-collapse supernovae
• A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715
• On the importance of viscous dissipation and heat conduction in binary neutron-star mergers
• Impact of the PSR J0740+6620 radius constraint on the properties of high-density matter
• Equation-of-State Dependent Features in Shock-Oscillation Modulated Neutrino and Gravitational-Wave Signals from Supernovae
• How perturbative QCD constrains the Equation of State at Neutron-Star densities
• On r-process nucleosynthesis from matter ejected in binary neutron starmergers
• Limiting masses and radii of neutron stars and their implications
• Skye: A Differentiable Equation of State
• Mass Ejection by Strange Star Mergers and Observational Implications
• Theoretical and Experimental Constraints for the Equation of State of Dense and Hot Matter
• Merger and post-merger of binary neutron stars with a quark-hadron crossover equation of state
• Self-consistent picture of the mass ejection from a one second-long binary neutron star merger leaving a short-lived remnant in general-relativistic neutrino-radiation magnetohydrodynamic simulation
• Finite-temperature extension for cold neutron star equations of state
• Relativistic hybrid stars in light of the NICER PSR J0740+6620 radius measurement
• Core-collapse supernova simulations and the formation of neutron stars, hybrid stars, and black holes
• Emergence of microphysical bulk viscosity in binary neutron star post-merger dynamics
• Merger of two neutron stars: predictions from the two-families scenario
• Gravitational-wave Signature of a First-order Quantum Chromodynamics Phase Transition in Core-Collapse Supernovae
• Constraining hadron-quark phase transition parameters within the quark-mean-field model using multimessenger observations of neutron stars
• Phase Transition Phenomenology with Nonparametric Representations of the Neutron Star Equation of State
• Thermal Effects in Binary Neutron Star Mergers
• Jet Launching from Binary Neutron Star Mergers: Incorporating Neutrino Transport and Magnetic Fields
• On the minimum radius of very massive neutron stars
• Large and massive neutron stars: Implications for the sound speed in dense QCD
• Strange quark stars in binaries: formation rates, mergers and explosive phenomena
• Constraint on phase transition with the multimessenger data of neutron stars
• The Role of the Hadron-Quark Phase Transition in Core-Collapse Supernovae
• Exploring thermal effects of the hadron-quark matter transition in neutron star mergers
• Impact of bulk viscosity on the post-merger gravitational-wave signal from merging neutron stars
• Progenitor Dependence of Hadron-quark Phase Transition in Failing Core-collapse Supernovae
• Estimate for the bulk viscosity of strongly coupled quark matter using perturbative QCD and holography
• Numerical modelling of bulk viscosity in neutron stars
• Evolution of equal mass binary bare quark stars in full general relativity: could a supramassive merger remnant experience prompt collapse?
• The Influence of Muons, Pions, and Trapped Neutrinos on Neutron Star Mergers
• Reverse phase transitions in binary neutron-star systems with exotic-matter cores
• Performance-Portable Binary Neutron Star Mergers with AthenaK
• Evolution of bare quark stars in full general relativity: Single star case
• A hybrid approach to long-term binary neutron-star simulations
• Long-lived neutron-star remnants from asymmetric binary neutron star mergers: element formation, kilonova signals and gravitational waves
• Black Hole Supernovae, their Equation of State Dependence and Ejecta Composition
• Fully general relativistic simulations of rapidly rotating quark stars: Oscillation modes and universal relations
• Impact of Rotation on the Multimessenger Signatures of a Hadron-quark Phase Transition in Core-collapse Supernovae
• Fermi-liquid theory of imbalanced quark matter
• Thermal Effects in Dense Matter Beyond Mean Field Theory
• Non-Fermi Liquid Effective Field Theory of Dense QCD Matter
• Long-term impact of the magnetic-field strength on the evolution and electromagnetic emission by neutron-star merger remnants
• General relativistic hydrodynamic simulations of binary strange star mergers