Relativistic Equation of State of Nuclear Matter for Supernova and Neutron Star

Abstract

We construct the equation of state (EOS) of nuclear matter using the relativistic mean field (RMF) theory in the wide density, temperature range with various proton fractions for the use of supernova simulation and the neutron star calculations. We first construct the EOS of homogeneous nuclear matter. We use then the Thomas-Fermi approximation to describe inhomogeneous matter, where heavy nuclei are formed together with free nucleon gas. We discuss the results on free energy, pressure and entropy in the wide range of astrophysical interest. As an example, we apply the resulting EOS on the neutron star properties by using the Oppenheimer-Volkoff equation.

15 pages, LaTeX, 14 ps-figures, accepted for publication in Nucl.Phys.A

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• Possibility of QCD critical point sweep during black hole formation
• Hadron-Quark phase transition in the context of GW190814
• Bayesian parameter estimation of core collapse supernovae using gravitational wave simulations
• Nucleosynthesis in core-collapse supernova explosions triggered by a quark-hadron phase transition
• Application of the Ghosh & Lamb Relation to the Spin-up/down Behavior in the X-ray Binary Pulsar 4U 1626-67
• Quark-meson coupling model for antikaon condensation in neutron star matter with strong magnetic fields
• Hot and Dense Homogeneous Nucleonic Matter Constrained by Observations, Experiment, and Theory
• Phase transition towards strange matter
• Massive Stars and their Supernovae
• Medium modifications for light and heavy nuclear clusters in simulations of core collapse supernovae -- Impact on equation of state and weak interactions
• Lambda hypernuclei and neutron star matter in a chiral SU(3) relativistic mean field model with a logarithmic potential
• Polytropic neutron star - black hole merger simulations with a Paczynski-Wiita potential
• Gravitational wave asteroseismology for low-mass neutron stars
• Critical parameters of liquid-gas phase transition in thermal symmetric and asymmetric nuclear matter
• Accretion-Induced Collapse of Dark Matter Admixed White Dwarfs -- I: Formation of Low-mass Neutron Stars
• Neutron star matter in the quark-meson coupling model in strong magnetic fields
• Searching for New Physics in Ultradense Environment: a Review on Dark Matter Admixed Neutron Stars
• Links between the shock instability in core-collapse supernovae and asymmetric accretions of envelopes
• Explosive nucleosynthesis in the neutrino-driven aspherical supernova explosion of a non-rotating 15$M_{\odot }$ star with solar metallicity
• Observing Supernova Neutrino Light Curves with Super-Kamiokande. II. Impact of the Nuclear Equation of State
• The Hadron-Quark Crossover in Neutron Star within Gaussian Process Regression Method
• Gravitational Wave Signatures of Hyperaccreting Collapsar Disks
• Radial oscillations of quark stars from perturbative QCD
• Effect of Inner Crust EoS on Neutron star properties
• Radial Oscillations in Neutron Stars with Delta Baryons
• Multipole moments and universal relations for scalarized neutron stars
• Gravitational wave asteroseismology on cooling neutron stars
• Estimating the nuclear saturation parameter via low-mass neutron star asteroseismology
• Multidimensional Boltzmann Neutrino Transport Code in Full General Relativity for Core-collapse Simulations
• Application of the nuclear equation of state obtained by the variational method to core-collapse supernovae
• Effects of Nuclear Equation of State on Type-I X-ray Bursts: Interpretation of the X-ray Bursts from GS 1826-24
• Impact of electron capture rates on nuclei far from stability on core-collapse supernovae
• Stellar Core Collapse with Hadron-Quark Phase Transition
• The g-mode Excitation in the Proto Neutron Star by the Standing Accretion Shock Instability
• The Gravitational Wave Signature of Core-Collapse Supernovae
• Numerical Study on Stellar Core Collapse and Neutrino Emission: Probe into the Spherically Symmetric Black Hole Progenitors with 3 - 30Msun Iron Cores
• Pulse profiles from a pulsar in scalar-tensor gravity
• Properties of neutrino transfer in a deformed remnant of neutron star merger
• Threshold Collision Energy of the QCD Phase Diagram Tricritical Endpoint
• On thermal nucleation of quark matter in compact stars
• $\eta$-meson in nuclear matter
• Relativistic stars with purely toroidal magnetic fields with realistic equations of state
• Pasta phases within the QMC model
• Neutrino - nucleon reaction rates in the supernova core in the relativistic random phase approximation
• Constraining relativistic models through heavy ion collisions
• Stiffness effects on the dynamics of the bar-mode instability of Neutron Stars in full General Relativity
• Magnetar QPOs and neutron star crust elasticity
• Ensemble in-equivalence in supernova matter within a simple model
• Nuclei embedded in an electron gas
• Nuclear pasta and supernova neutrinos at late times
• Properties of neutron star described by a relativistic $abinitio$ model
• Nuclear matter at finite temperature and static properties of proto-neutron star
• Stability of the protoneutron stars toward black hole formation
• Nuclei in Core-Collapse Supernovae Engine
• Observing cosmological binary mergers with next generation neutrino and gravitational wave detectors
• Composition of nuclear matter with light clusters and Bose-Einstein condensation of $\alpha$ particles
• Probing the metastability of protoneutron star with hyperon in core-collapse supernova
• Uniqueness of the Inflationary Higgs Scalar for Neutron Stars and Failure of non-inflationary Approximations
• Large-scale calculations of supernova neutrino-induced reactions in Z=8-82 target nuclei
• Open Problems in $\alpha$ Particle Condensation
• Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations
• Hot and Dense Matter Equation of State Probability Distributions for Astrophysical Simulations
• $\omega N$ scattering length from $\omega$ photoproduction on the proton near the threshold
• Temperature Effects on Core g-modes of Neutron Stars
• An Entropy-Area Law for Neutron Stars Near the Black Hole Threshold
• Caloric curve for finite nuclei in relativistic models
• Diffuse neutrino background from past core-collapse supernovae
• Relativistic hybrid stars with super-strong toroidal magnetic fields: An evolutionary track with QCD phase transition
• Constraining the density dependence of the nuclear symmetry energy from an X-ray bursting neutron star
• Properties of nuclear matter in relativistic Brueckner-Hartree-Fock model with high-precision charge-dependent potentials
• Medium effects in supernovae constraints on light mediators
• Magnetorotational Mechanism of the Explosion of Core-Collapse Supernovae
• Dark Stars and Gravitational Waves: Topical Review
• Impact of late-time neutrino emission on the diffuse supernova neutrino background
• Tetraneutron condensation in neutron rich matter
• Pasta fluctuations in symmetric matter at finite temperature
• Radial oscillations in neutron stars from QCD
• Towards generating a new supernova equation of state: A systematic analysis of cold hybrid stars
• Hot and dense matter beyond relativistic mean field theory
• Neutron stars formation and Core Collapse Supernovae
• On the importance of progenitor asymmetry to shock revival in core-collapse supernovae
• Computational Models of Stellar Collapse and Core-Collapse Supernovae
• The reaction $\pi N\to \omega N$ in a dynamical coupled-channel approach
• Neutron Star instabilities in full General Relativity using a $\Gamma =2.75$ ideal fluid
• Perturbation Analysis of a General Polytropic Homologously Collapsing Stellar Core
• Effects of nuclear matter properties in neutron star mergers
• Asymmetric Nuclear Light Clusters In Supernova Matter
• Impact of Rotation on Neutrino Emission and Relic Neutrino Background from Population III Stars
• Finite-temperature effects in dynamical-spacetime binary neutron star merger simulations: Validation of the parametric approach
• Light clusters in warm stellar matter: calibrating the cluster couplings
• Self consistent calculation of the nuclear composition in hot and dense stellar matter
• Equation of State Dependence of Nonlinear Mode-tide Coupling in Coalescing Binary Neutron Stars
• Hadron-Quark Phase Transitions in Hyperon Stars
• Constraining Axion Mass through Gamma-ray Observations of Pulsars
• Impact of nuclear matter properties on the nucleosynthesis and the kilonova from binary neutron star merger ejecta
• Effects of nuclear matter and composition in core-collapse supernovae and long-term proto-neutron star cooling
• Cautionary tales on heating-rate prescriptions in kilonovae
• Second virial coefficients of light nuclear clusters and their chemical freeze-out in nuclear collisions
• Diffuse supernova neutrino background with up-to-date star formation rate measurements and long-term multidimensional supernova simulations
• Frozen and $\beta$-equilibrated $f$ and $p$ modes of cold neutron stars: nuclear metamodel predictions
• Variability in Short Gamma-ray Bursts: Gravitationally Unstable Tidal Tails
• Electron-positron energy deposition rate from neutrino pair annihilation on the rotation axis of neutron and quark stars
• Neutron Stars and Gravitational Waves: the Key Role of Nuclear Equation of State
• Quenched Λ spin-orbit splitting by relativistic Fock diagram in single-Λ hypernuclei
• Low-Energy Supernovae Bounds on Sterile Neutrinos
• Quark Matter Equation of State from Perturbative QCD
• Influence of effective nucleon mass on equation of state for supernova simulations and neutron stars
• An "archaeological" quest for galactic supernova neutrinos
• An approach toward the successful supernova explosion by physics of unstable nuclei
• Is a soft nuclear equation of state extracted from heavy-ion data incompatible with pulsar data?
• Investigating the role of nuclear parameters on oscillation modes in hot Neutron Stars
• Parametrization of the surface energy in the ETF approximation
• Neutrino emission from the collapse of $\sim 10^4$ $M_{\odot }$ population III supermassive stars
• Multi-messenger observations of neutron rich matter
• Shell States of Neutron Rich Matter
• Statistical treatment of nuclear clusters in the continuum
• Nuclear pasta in hot and dense matter and its influence on the equation of state for astrophysical simulations
• Strong magnetic fields: neutron stars with an extended inner crust
• Neutron star mass formula with nuclear saturation parameters
• Electron-positron energy deposition rate from neutrino pair annihilation in the equatorial plane of rapidly rotating neutron and quark stars
• Effects of finite sizes of atomic nuclei on shear modulus and torsional oscillations in neutron stars
• Equilibrium nuclear ensembles taking into account vaporization of hot nuclei in dense stellar matter
• Normalizing flows for microscopic many-body calculations: an application to the nuclear equation of state
• Quark matter with strong magnetic field and possibility of the third family of compact stars
• The infrared counterpart and proper motion of magnetar SGR0501+4516
• Slowly-Rotating Neutron Stars in Massive Bigravity
• Nuclear matter from the ladder resummation in terms of the experimental nucleon-nucleon scattering amplitudes
• Neutrino oscillation and expected event rate of supernova neutrinos in adiabatic explosion model
• Light clusters in the liquid proto-neutron star inner crust
• Superfluidity of $\Lambda$ hyperons in warm strange hadronic star matter
• Isotopic equilibrium constants for very low-density and low-temperature nuclear matter
• Relativistic Thomas-Fermi description of Sm isotopes at finite temperature
• Influence of the tetraneutron on the EoS under core-collapse supernovae and heavy-ion collisions conditions
• Cooling the Shock: New Supernova Constraints on Dark Photons
• Critical properties of calibrated relativistic mean-field models for the transition to warm, non-homogeneous nuclear matter
• Cooling of Isolated Neutron Stars with Pion Condensation: Possible Fast Cooling in a Low-Symmetry-Energy Model
• Dirac-Neutrino Magnetic Moment and the Dynamics of a Supernova Explosion
• Lepton-rich cold QCD matter in protoneutron stars
• Equation of State for Neutralino Star as a Form of Cold Dark Matter
• Equation of state and neutrino transfer in supernovae and neutron stars
• From Microscales to Macroscales in 3D: Selfconsistent Equation of State for Supernova and Neutron Star Models
• Quark-hadron mixed phases in protoneutron stars
• Appearance of a quark matter phase in hybrid stars
• Pseudo Nambu-Goldstone modes in neutron stars
• Dependence of postmerger properties on the thermal heating efficiency in neutron star mergers
• Equation of State of Hot Neutron Star Matter using Finite Range Simple Effective Interaction
• Spontaneous Scalarization in Proto-neutron Stars
• Methods for relativistic self-gravitating fluids: From binary neutron stars to black hole-disks and magnetized rotating neutron stars
• Exploring Radial Oscillations in Slow Stable and Hybrid Neutron Stars
• How Well Do We Know The Supernova Equation of State?
• Formation of quark phases in protoneutron stars: the transition from the 2SC to the normal quark phase
• Self-consistent single-nucleon potential at positive energy produced by semi-realistic interaction and its examination via nucleon-nucleus elastic scattering
• $f$-mode oscillations in hot Neutron Stars: Effect of hyperons and neutrino trapping
• A Parametric Study of the Acoustic Mechanism for Core-Collapse Supernovae
• Properties of the Initial Participant Matter Interaction Zone in Near Fermi-Energy Heavy Ion Collisions
• Preliminary EoS for core-collapse supernova simulations with the QMC model
• The Strange Prospects for Astrophysics
• Adaptive Mesh Refinement for Astrophysics Applications with ParalleX
• An Investigation into Surface Temperature Distributions of High-B Pulsars
• Modification of the universal relation between mass, radius and nonradial $f$-mode oscillation in proto-neutron stars
• Universal relations between the quasinormal modes of neutron stars and magnetic tidal deformability
• Inner crust equations of state for CompOSE
• In-medium Properties of ${\Theta }^{+}$ as a K$\pi$N structure in Relativistic Mean Field Theory
• Thermal properties of hot and dense medium in interacting hadron resonance gas model
• Measuring the Low-Energy Weak Mixing Angle with Supernova Neutrinos
• Short gamma-ray bursts and the decompression of neutron star matter in tidal streams
• Alpha clustering in warm and dense nuclear matter from heavy-ion collisions
• Core-Collapse Supernovae at the Threshold
• General relativistic magnetohydrodynamics simulations for binary neutron star mergers
• Neutron Star Evolutions using Tabulated Equations of State with a New Execution Model
• Limitations in constraining neutron star radii and nuclear properties from inspiral gravitational wave detections
• Fermi operator expansion method for nuclei and inhomogeneous matter with nuclear energy density functional
• Phase-space excluded-volume approach for light clusters in nuclear medium
• Interacting quark matter effects on the structure of compact stars
• Equation of state for hot hyperonic neutron star matter
• Updates of the nuclear equation of state for core-collapse supernovae and neutron Stars: effects of 3-body forces, QCD, and magnetic fields
• Occurrence of fast neutrino flavor conversions in QCD phase-transition supernovae
• Impact of Rotation on Quark-Hadron Hybrid Stars
• Properties of rapidly rotating hot neutron stars within Brueckner theory
• Rotating NSs/QSs and recent astrophysical observations
• Can a supernova bang twice?
• Quantum corrections to the Relativistic mean-field theory
• Hadronic matter phases and their application to rapidly rotating neutron stars
• Nuclear Drip Line and the Composition of Supernova Matter
• Numerical modeling of core-collapse supernovae and compact objects
• Assessing the Distance for Probing the Nuclear Equation of State with Supernova Gravitational Waves
• Light hyperclusters and hyperons in low-density hot stellar matter
• Toward Radiation-Magnetohydrodynamic Simulations in Core-Collapse Supernovae
• The thermal index of neutron-star matter in the virial approximation
• Constraints on the Neutron Star Equation of State from GW170817
• Formation of large chunk of nuclear matter in heavy-ion collisions
• From pQCD to neutron stars: matching equations of state to constrain global star properties
• Heavy baryons in hot stellar matter with light nuclei and hypernuclei
• EstrellaNueva: an open-source software to study the interactions and detection of neutrinos emitted by supernovae
• Bare Collapse, Formation of Neutron Star Binaries and Fast Optical Transients
• Bremsstrahlung emission from nuclear reactions in compact stars
• New Insights into Uncertainties in the Relic Neutrino Background and Effects from the Nuclear Equation of State