Core-collapse supernova equations of state based on neutron star observations

Abstract

Many of the currently available equations of state for core-collapse supernova simulations give large neutron star radii and do not provide large enough neutron star masses, both of which are inconsistent with some recent neutron star observations. In addition, one of the critical uncertainties in the nucleon-nucleon interaction, the nuclear symmetry energy, is not fully explored by the currently available equations of state. In this article, we construct two new equations of state which match recent neutron star observations and provide more flexibility in studying the dependence on nuclear matter properties. The equations of state are also provided in tabular form, covering a wide range in density, temperature and asymmetry, suitable for astrophysical simulations. These new equations of state are implemented into our spherically symmetric core-collapse supernova model, which is based on general relativistic radiation hydrodynamics with three-flavor Boltzmann neutrino transport. The results are compared with commonly used equations of state in supernova simulations of 15 and 40 solar mass progenitors. We do not find any simple correlations between individual nuclear matter properties at saturation and the outcome of these simulations. However, the new equations of state lead to the most compact neutron stars among the relativistic mean-field models which we considered. The new models also obey the previously observed correlation between the time to black hole formation and the maximum mass of an s=4 neutron star.

10 pages, 7 figures

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• Numerical Inside View of Hypermassive Remnant Models for GW170817
• Modern nuclear and astrophysical constraints of dense matter in a renormalized chiral approach
• Hot and dense matter beyond relativistic mean field theory
• Geometric and thermodynamic characterization of binary neutron star accretion discs
• On the importance of progenitor asymmetry to shock revival in core-collapse supernovae
• Systematic errors due to quasi-universal relations in binary neutron stars and their correction for unbiased model selection
• Prospects for Distinguishing Supernova Models Using a Future Neutrino Signal
• A Generalized Kompaneets Formalism for Inelastic Neutrino-Nucleon Scattering in Supernova Simulations
• Effects of nuclear matter and composition in core-collapse supernovae and long-term proto-neutron star cooling
• Light clusters in warm stellar matter: calibrating the cluster couplings
• Actinide-boosting r Process in Black Hole-Neutron Star Merger Ejecta
• Tabulated Equations of State From Models Informed by Chiral Effective Field Theory
• A Force Explosion Condition for Spherically Symmetric Core-collapse Supernovae
• thornado-hydro: a discontinuous Galerkin method for supernova hydrodynamics with nuclear equations of state
• Impact of nuclear matter properties on the nucleosynthesis and the kilonova from binary neutron star merger ejecta
• Three-Dimensional General-Relativistic Simulations of Neutrino-Driven Winds from Rotating Proto-Neutron Stars
• Calibration of the Advanced Spectral Leakage scheme for neutron star merger simulations, and extension to smoothed-particle hydrodynamics
• Prospects for optical detections from binary neutron star mergers with the next-generation multi-messenger observatories
• On the Role of Muons in Binary Neutron Star Mergers: First Simulations
• Gamma-ray Diagnostics of r-process Nucleosynthesis in the Remnants of Galactic Binary Neutron-Star Mergers
• Variability in Short Gamma-ray Bursts: Gravitationally Unstable Tidal Tails
• Visualizing convolutional neural network for classifying gravitational waves from core-collapse supernovae
• Probing nuclear physics with supernova gravitational waves and machine learning
• Diffuse supernova neutrino background with up-to-date star formation rate measurements and long-term multidimensional supernova simulations
• Low-Energy Supernovae Bounds on Sterile Neutrinos
• Angle-dependent in-situ fast flavor transformations in post-neutron star merger disks
• The Neutrino Signal From Pair Instability Supernovae
• Effects of Different Closure Choices in Core-Collapse Supernova Simulations
• Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis
• Comparison of simulated neutrino emission models with data on Supernova 1987A
• Fully general relativistic simulations of rapidly rotating quark stars: Oscillation modes and universal relations
• Thermal effects on tidal deformability in the last orbits of an inspiraling binary neutron star system
• Neutrino-driven Core-collapse Supernova Yields in Galactic Chemical Evolution
• The Force Explosion Condition is Consistent with Spherically Symmetric CCSN Explosions
• Influence of effective nucleon mass on equation of state for supernova simulations and neutron stars
• Sensitivity of nuclear statistical equilibrium to nuclear uncertainties during stellar core collapse
• Inferring the Equation of State from Neutron Star Observables via Machine Learning
• Accurate nuclear symmetry energy at finite temperature within a BHF approach
• Investigating the role of nuclear parameters on oscillation modes in hot Neutron Stars
• Constraining the supersaturation density equation of state from core-collapse supernova simulations - Excluded volume extension of the baryons
• Accretion-Induced Collapse of Dark Matter Admixed White Dwarfs -- II: Rotation and Gravitational-wave Signals
• The collimation of relativistic jets in post-neutron star binary merger simulations
• Mass and tidal parameter extraction from gravitational waves of binary neutron stars mergers using deep learning
• Phase-transition-induced collapse of proto-compact stars and its implication for supernova explosions
• Nonparametric extensions of nuclear equations of state: probing the breakdown scale of relativistic mean-field theory
• Nuclear pasta in hot and dense matter and its influence on the equation of state for astrophysical simulations
• A New Constraint on the Nuclear Equation of State from Statistical Distributions of Compact Remnants of Supernovae
• Normalizing flows for microscopic many-body calculations: an application to the nuclear equation of state
• Equation of state in neutron stars and supernovae
• Cocoon shock breakout emission from binary neutron star mergers
• Do Finite Density Effects Jeopardize Axion Nucleophobia in Supernovae?
• The impact of hyperons on neutron star mergers: gravitational waves, mass ejection and black hole formation
• Progenitor Dependence of Neutrino-driven Supernova Explosions with the Aid of Heavy Axion-like Particles
• Diagnosing electron-neutrino lepton number crossings in core-collapse supernovae: A comparison of methods
• Equilibrium nuclear ensembles taking into account vaporization of hot nuclei in dense stellar matter
• Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities
• Conditions for the existence of stable strange quark matter
• What can be learned from a proto-neutron star's mass and radius?
• Explosion Energies for Core-collapse Supernovae I: Analytic, Spherically Symmetric Solutions
• Merger of a Neutron Star with a Black Hole: one-family vs. two-families scenario
• Deep-Learning Classification and Parameter Inference of Rotational Core-Collapse Supernovae
• Did a Kilonova Set Off in Our Galactic Backyard 3.5 Myr ago?
• Tight bound on neutron-star radius with quasiperiodic oscillations in short gamma-ray bursts
• Gravitational Wave emission in Binary Neutron Star early post-merger within a dark environment
• Detecting and reconstructing gravitational waves from the next Galactic core-collapse supernova in the Advanced Detector Era
• Cooling the Shock: New Supernova Constraints on Dark Photons
• Supernova Preshock Neutronization Burst as a Probe of Non-Standard Neutrino Interactions
• Critical properties of calibrated relativistic mean-field models for the transition to warm, non-homogeneous nuclear matter
• Neutron stars in the large-$N_c$ limit
• Diffuse Neutrino Background from Magnetorotational Stellar Core Collapses
• Evaluating Machine Learning Models for Supernova Gravitational Wave Signal Classification
• Equation of state and neutrino transfer in supernovae and neutron stars
• Comparison of Electron Capture Rates in the N=50 Region using 1D Simulations of Core-collapse Supernovae
• Equation of State of Hot Neutron Star Matter using Finite Range Simple Effective Interaction
• Massive Computation for Understanding Core-Collapse Supernova Explosions
• Estimate of the Detectability of the Circular Polarisation Signature of Supernova Gravitational Waves Using the Stokes Parameters
• Thermal fluctuations of matter composition and quark nucleation in compact stars
• The internal structure of neutron stars and white dwarfs, and the Jacobi virial equation. II
• Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches
• Simple fits for the neutrino luminosities from protoneutron star cooling
• How Well Do We Know The Supernova Equation of State?
• Magnetic Field Strength Effects on Nucleosynthesis from Neutron Star Merger Outflows
• Unveiling a universal relationship between the f(R) parameter and neutron star properties
• Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state
• Suitable resolution for EOS tables in neutron star investigation
• Explosion Dynamics of Parametrized Spherically Symmetric Core-Collapse Supernova Simulations
• Neutron Stars in Mimetic Gravity
• Estimates of the early EM emission from compact binary mergers
• Connecting Relativistic Density Functional Theory to Microscopic Calculations
• Effects of multidimensional treatment of gravity in simulations on supernova gravitational waves
• Insights into Binary Neutron Star Merger Simulations: A Multi-Code Comparison
• Electron-neutrino lepton number crossings: Variations with the supernova core physics
• Black Hole-Neutron Star Binaries near Neutron Star Disruption Limit in the Mass Regime of Event GW230529
• R-process heating implementation in hydrodynamic simulations with neural networks
• Numerical Relativity Estimates of the Remnant Recoil Velocity in Binary Neutron Star Mergers
• Simulating Binary Neutron Star Mergers with Finite-temperature Equations of State: The influences of the slope of the symmetry energy and artificial heating
• $f$ and $p$ mode oscillation of proto-neutron stars with systematic variation of the nucleon effective mass
• Preliminary EoS for core-collapse supernova simulations with the QMC model
• Multi-dimensional Core-Collapse Supernova Simulations with Neutrino Transport
• Gravitational-wave model for neutron star merger remnants with supervised learning
• Nonlinear mode-tide coupling in coalescing binary neutron stars with relativistic corrections
• Fundamental quantum limits for detecting ultrahigh frequency gravitational waves
• Effect of spin in binary neutron star mergers
• $f$-mode oscillations of compact stars with realistic equations of state in dynamical spacetime
• Astrophysical constraints on the cold equation of state of the strongly interacting matter
• A constraint on superheavy elements of the GRB-kilonova AT 2023vfi
• Dynamical ejecta of neutron star mergers with nucleonic weak processes I: Nucleosynthesis
• Do black holes remember what they are made of?
• Axion-like Particles from Hypernovae
• Rapidly rotating neutron stars with realistic nuclear matter equation of state
• Modification of the universal relation between mass, radius and nonradial $f$-mode oscillation in proto-neutron stars
• Time integration for neutrino radiation transport using minimally implicit Runge-Kutta methods
• Observability of sharp phase transitions in neutron stars
• Collapsar Disk Outflows III: Detectable Neutrino and Gravitational Wave Signatures
• Neutron matter with chiral EFT interactions: Perturbative and first QMC calculations
• Constraints from the GW170817 merger event on the nuclear matter equation of state
• The Gravitational Wave Memory from Binary Neutron Star Mergers
• Occurrence of fast neutrino flavor conversions in QCD phase-transition supernovae
• Matter- and magnetically-driven flavor conversion of neutrinos in magnetorotational collapses
• Neutrino flavor instabilities in neutron star mergers with moment transport: Slow, fast, and collisional modes
• Role of thermal fluctuations in nucleation of three-flavor quark matter
• Toward First-Principles Multi-Messenger Predictions: Coupling Nuclear Networks with GR Radiation-MHD in {\tt Gmunu}
• Neutrino emission, Equation of State and the role of strong gravity
• Limitations in constraining neutron star radii and nuclear properties from inspiral gravitational wave detections
• General relativistic magnetohydrodynamics simulations for binary neutron star mergers
• Hyperboloidal neutron star and black hole initial data in spherical symmetry
• Phenomenological QCD equations of state for neutron star mergers, a talk presented at CPOD17
• Stochastic Gravitational-Wave Background from Stellar Core-Collapse Events
• Extract non-Gaussian Features in Gravitational Wave Observation Data Using Self-Supervised Learning
• Incorporating a radiative hydrodynamics scheme in the numerical-relativity code BAM
• Nuclear Matter and Finite Nuclei: Relativistic Thomas-Fermi Approximation Versus Relativistic Mean-Field Approach
• Maximal mass of neutron stars constrained by neutron star observations
• Trends in gravitational wave emission in axisymmetric simulations of rotating core-collapse supernovae
• libyt: an In Situ Interface Connecting Simulations with yt, Python, and Jupyter Workflows
• New Insights into Uncertainties in the Relic Neutrino Background and Effects from the Nuclear Equation of State
• Uncertainties in the production of iron-group nuclides in core-collapse supernovae from Monte Carlo variations of reaction rates
• Light hyperclusters and hyperons in low-density hot stellar matter
• Assessing the Distance for Probing the Nuclear Equation of State with Supernova Gravitational Waves
• EstrellaNueva: an open-source software to study the interactions and detection of neutrinos emitted by supernovae
• Parity-doubled nucleons can rapidly cool neutron stars
• Properties of rapidly rotating hot neutron stars within Brueckner theory
• The thermal index of neutron-star matter in the virial approximation
• The Strange Physics of Dark Baryons
• Triaxial instabilities in rapidly rotating Neutron Stars