Equations of state for supernovae and compact stars

Abstract

We review various theoretical approaches for the equation of state (EoS) of dense matter, relevant for the description of core-collapse supernovae, compact stars and compact star mergers. The emphasis is put on models that are applicable to all of these scenarios. Such EoS models have to cover large ranges in baryon number density, temperature and isospin asymmetry. The characteristics of matter change dramatically within these ranges, from a mixture of nucleons, nuclei, and electrons to uniform, strongly interacting matter containing nucleons, and possibly other particles such as hyperons or quarks. As the development of an EoS requires joint efforts from many directions we consider different theoretical approaches and discuss relevant experimental and observational constraints which provide insights for future research. Finally, results from applications of the discussed EoS models are summarized.

74 pages, 19 figures

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• Effects of Dark Matter on $f$-mode oscillations of Neutron Stars
• Constraints on high density equation of state from maximum neutron star mass
• The baryon coupling scheme in an unified SU(3) and SU(6) symmetry formalism
• Application of artificial intelligence in the determination of impact parameter in heavy-ion collisions at intermediate energies
• Bulk viscosity in neutron stars with hyperon cores
• A pitfall of piecewise-polytropic equation of state inference
• Full distribution of clusters with universal couplings and in-medium effects
• Ruling out the supersoft high-density symmetry energy from the discovery of PSR J0740+6620 with mass $2.14_{-0.09}^{+0.10}{M}_{\odot }$
• The special point on the hybrid star mass--radius diagram and its multi--messenger implications
• Influence of density dependence of symmetry energy in hot and dense matter for supernova simulations
• Muons in the aftermath of neutron star mergers and their impact on trapped neutrinos
• Consistent Skyrme parametrizations constrained by GW170817
• Effects of $\varphi$-meson on properties of hyperon stars in density dependent relativistic mean field model
• Constraining the density dependence of the symmetry energy with nuclear data and astronomical observations in the KIDS framework
• A New Approach to Mass and Radius of Neutron Stars with Supernova Neutrinos
• Towards the understanding of the genuine three-body interaction for p$-$p$-$p and p$-$p$-\Lambda$
• High-momentum components in the ${}^4$He nucleus caused by inter-nucleon correlations
• Hypermassive quark cores
• Bayesian inference of the incompressibility, skewness and kurtosis of nuclear matter from empirical pressures in relativistic heavy-ion collisions
• Supernova Constraints on Dark Flavored Sectors
• The Emission Order of Hydrogen Isotopes via Correlation Functions in 30 MeV/u Ar+Au Reactions
• Role of vector channel in different classes of (non) magnetized neutron stars
• Effect of isovector scalar meson on equation of state of dense matter within relativistic mean field model
• Chiral symmetry restoration and the $\Delta$ matter formation in neutron stars
• Hybrid star models in the light of new multi-messenger data
• $r$-process nucleosynthesis from compact binary mergers
• Exploring thermal effects of the hadron-quark matter transition in neutron star mergers
• Impact of pions on binary neutron star mergers
• EoS constraints from nuclear masses and radii in a meta-modeling approach
• Model-based cross-correlation search for gravitational waves from the low-mass X-ray binary Scorpius X-1 in LIGO O3 data
• Axions: From Magnetars and Neutron Star Mergers to Beam Dumps and BECs
• R-modes and neutron star recycling scenario
• Constraining nuclear parameters using Gravitational waves from f-mode Oscillations in Neutron Stars
• Improved neutrino-nucleon interactions in dense and hot matter for numerical simulations
• GW170817 and the prospect of forming supramassive remnants in neutron star mergers
• Relativistic hybrid stars with sequential first-order phase transitions in light of multimessenger constraints
• Probing high-density nuclear symmetry energy with ${\Xi }^{-}/{\Xi }^0$ ratio in heavy-ion collisions at $\sqrt{s_{NN}}\sim 3$ GeV
• Effect of strong magnetic fields on the crust-core transition and inner crust of neutron stars
• Extended Skyrme interactions for transport model simulations of heavy-ion collisions
• Thermal Relaxation of Dark Matter Admixed Neutron Star
• Phenomenological QCD equations of state for neutron star dynamics: Nuclear-2SC continuity and evolving effective couplings
• Deducing Neutron Star Equation of State Parameters Directly From Telescope Spectra with Uncertainty-Aware Machine Learning
• Can we decipher the composition of the core of a neutron star?
• Hadron-quark Pasta Phase in Massive Neutron Stars
• Impact of updated Multipole Love numbers and f-Love Universal Relations in the context of Binary Neutron Stars
• Isospin symmetry breaking in the charge radius difference of mirror nuclei
• Thermal behavior as indicator for hyperons in binary neutron star merger remnants
• Inference of the neutron star equation of state from cosmological distances
• Dense Matter in Neutron Stars with eXTP
• Extracting nuclear matter properties from the neutron star matter equation of state using deep neural networks
• Inference of neutron-star properties with unified crust-core equations of state for parameter estimation
• Reconciling multi-messenger constraints with chiral symmetry restoration
• $R$-mode Stability of GW190814's Secondary Component as a Supermassive and Superfast Pulsar
• The effect of the energy functional on the pasta-phase properties of catalysed neutron stars
• The equation of state and some key parameters of neutron stars: constraints from GW170817, the nuclear data and the low mass X-ray binary data
• Neutron star mass formula with nuclear saturation parameters for asymmetric nuclear matter
• Structure of Quark Star: A Comparative Analysis of Bayesian Inference and Neural Network Based Modeling
• Bayesian inference of neutron-star observables based on effective nuclear interactions
• Hadron matter in neutron stars in view of gravitational wave observations
• Constraints on the muon fraction and density profile in neutron stars
• Impact of Symmetry Energy on Sound Speed and Spinodal Decomposition in Dense Neutron-Rich Matter
• Progenitor Dependence of Hadron-quark Phase Transition in Failing Core-collapse Supernovae
• Constraining isovector nuclear interactions with giant resonances within a Bayesian approach
• Neutron Star Structure in the Presence of Nonminimally Coupled Scalar Fields
• CREX- and PREX-II-motivated relativistic interactions and their implications for the bulk properties of nuclear matter and neutron stars
• g-mode Oscillations in Neutron Stars with Hyperons
• Nuclear matter fourth-order symmetry energy in non-relativistic mean-field models
• Delta baryons in neutron stars
• Equation of state and composition of proto-neutron stars and merger remnants with hyperons
• Hot and Dense Homogeneous Nucleonic Matter Constrained by Observations, Experiment, and Theory
• Baryonic models of ultra-low-mass compact stars for the central compact object in HESS J1731-347
• Double strangeness ${\Xi }^{-}$ production as a probe of nuclear equation of state at high densities
• Hyperonic neutron stars: reconciliation between nuclear properties and NICER and LIGO/VIRGO results
• Universal relations for compact stars with heavy baryons
• Determination of the symmetry energy from the neutron star equation of state
• Asymmetric Nuclear Matter and Neutron Star Properties in Relativistic ab initio Theory in the Full Dirac Space
• Medium modifications for light and heavy nuclear clusters in simulations of core collapse supernovae -- Impact on equation of state and weak interactions
• Searching for New Physics in Ultradense Environment: a Review on Dark Matter Admixed Neutron Stars
• Symmetry energy effect on the secondary component of GW190814 as a neutron star
• Fluctuations and phases in baryonic matter
• Observing Supernova Neutrino Light Curves with Super-Kamiokande. II. Impact of the Nuclear Equation of State
• From bare interactions, low--energy constants and unitary gas to nuclear density functionals without free parameters: application to neutron matter
• Constraining equation of state of nuclear matter by charge-changing cross section measurements of mirror nuclei
• Critical parameters of liquid-gas phase transition in thermal symmetric and asymmetric nuclear matter
• Covariant Density Functional Theory with Localized Exchange Terms
• Camouflage of the Phase Transition to Quark Matter in Neutron Stars
• Crust-core transition of a neutron star: effects of the symmetry energy and temperature under strong magnetic fields
• XTE J1814-338 as a dark matter admixed neutron star
• Relativistic Mean Field Model parameterizations in the light of GW170817, GW190814, and PSR J0740 + 6620
• Neutron star mass-radius constraints using the high-frequency QPOs of GRB 200415A
• GW170817 constraints analyzed with Gogny forces and momentum-dependent interactions
• Constraining neutron superfluidity with $r$-mode physics
• Symmetry energy effects on the properties of hybrid stars
• Radial Oscillations in Neutron Stars with Delta Baryons
• Symmetry energy extracted from the S$\pi$RIT pion data in Sn+Sn systems
• Vector-Interaction-Enhanced Bag Model
• Addition of tabulated equation of state and neutrino leakage support to IllinoisGRMHD
• Finite-size effects on the Phase Structure of the Walecka Model
• Electric dipole polarizability in neutron-rich Sn isotopes as a probe of nuclear isovector properties
• Empirical information on nuclear matter fourth-order symmetry energy from an extended nuclear mass formula
• Unified nuclear matter EOSs constrained by the in-medium balance in density-dependent covariant density functionals
• Nuclear pasta structures and symmetry energy
• Superfluid Phase Transitions and Effects of Thermal Pairing Fluctuations in Asymmetric Nuclear Matter
• Indirect methods in nuclear astrophysics with relativistic radioactive beams
• Nucleus giant resonances from an improved isospin-dependent Boltzmann-Uehling-Uhlenbeck transport approach
• Pulse profiles from a pulsar in scalar-tensor gravity
• Astrophysics and Nuclear Physics Informed Interactions in Dense Matter: Inclusion of PSR J0437-4715
• Neutron star properties with careful parameterization in the (axial)vector meson extended linear sigma model
• Central Speed of Sound, Trace Anomaly and Observables of Neutron Stars from Perturbative Analyses of Scaled TOV Equations
• Dense matter equation of state for neutron star mergers
• Low density nuclear matter with light clusters in a generalized nonlinear relativistic mean-field model
• The Role of Baryon Structure in Neutron Stars
• Glitch Behavior of Pulsars and Contribution from Neutron Star Crust
• Finding quark content of neutron stars in light of GW170817
• Revisiting the Equation of State of Hybrid Stars in the Dyson-Schwinger Equation Approach to QCD
• Bayesian Inference of Fine-Features of Nuclear Equation of State from Future Neutron Star Radius Measurements to 0.1km Accuracy
• Setting nonperturbative uncertainties on finite-temperature properties of neutron matter
• Tidal heating as a direct probe of strangeness inside neutron stars
• Bayesian uncertainty quantification for nuclear matter incompressibility
• Bulk viscosity from Urca processes: $npe\mu$ matter in the neutrino-transparent regime
• Collective flow and correlations measurements with HADES in Au+Au collisions at 1.23 AGeV
• Constraining the equation of state of hybrid stars using recent information from multidisciplinary physics
• Density-dependent van der Waals model under the GW170817 constraint
• Nuclear collective dynamics in the lattice Hamiltonian Vlasov method
• 3D code for MAgneto-Thermal evolution in Isolated Neutron Stars, MATINS: thermal evolution and lightcurves
• X-PSI Parameter Recovery for Temperature Map Configurations Inspired by PSR J0030+0451
• Influence of the interactions of scalar mesons on the behavior of the symmetry energy
• Axion emission from strange matter in core-collapse SNe
• Massive neutron star with strangeness in a relativistic mean-field model with a high-density cut-off
• Bayesian model averaging for nuclear symmetry energy from effective proton-neutron chemical potential difference of neutron-rich nuclei
• Magnetar QPOs and neutron star crust elasticity
• Microscopic nuclear equation of state at finite temperature and stellar stability
• Quick Guides for Use of the CompOSE Data Base
• Hot neutron stars and their equation of state
• Constraining isovector nuclear interactions with giant dipole resonance and neutron skin in ${}^{208}$Pb from a Bayesian approach
• Hybrid Equations of State for Neutron Stars with Hyperons and Deltas
• Detectability of a phase transition in neutron star matter with third-generation gravitational wave interferometers
• Thermodynamics from the quark condensate
• Pasta phases within the QMC model
• Axion effects in the stability of hybrid stars
• Probing phase transition in neutron stars via the crust-core interfacial mode
• Neutron star equation of state and GW170817
• Nuclear matter at finite temperature and static properties of proto-neutron star
• Measuring deformed neutron skin with free spectator nucleons in relativistic heavy-ion collisions
• A bag model of matter condensed by the strong interaction
• Stability of the protoneutron stars toward black hole formation
• Effects of the equation of state on the core-crust interface of slowly rotating neutron stars
• Numerical Study of Stellar Core Collapse and Neutrino Emission Using the Nuclear Equation of State Obtained by the Variational Method
• Composition of nuclear matter with light clusters and Bose-Einstein condensation of $\alpha$ particles
• Feasibility of dark matter admixed neutron star based on recent observational constraints
• Beyond-mean-field effects on the symmetry energy and its slope from the low-lying dipole response of ${}^{68}$Ni
• Repulsive $\Lambda$ potentials in dense neutron star matter and binding energy of $\Lambda$ in hypernuclei
• Nonparametric model for the equations of state of neutron star from deep neural network
• Supercritically charged objects and electron-positron pair creation
• $Abinitio$ thermodynamics of one-component plasma for astrophysics of white dwarfs and neutron stars
• Frequencies of $f$- and $p$-oscillation modes in cold and hot compact stars
• Studies of the equation-of-state of nuclear matter by heavy-ion collisions at intermediate energy in the multi-messenger era
• Nuclei in Core-Collapse Supernovae Engine
• In medium properties of $K^0$ and $\varphi$ mesons under an external magnetic field
• Masquerading hybrid stars with dark matter
• Nuclear collective dynamics in transport model with the lattice Hamiltonian method
• Temperature and Strong Magnetic Field Effects in Dense Matter
• Constraining nuclear matter parameters from correlation systematics:a mean-field perspective
• Constraining dense matter physics using f-mode oscillations in neutron stars
• New covariant density functionals of nuclear matter for compact star simulations
• Impacts of symmetry energy slope on the oscillation frequencies of neutron stars with short-range correlation and admixed dark matter
• From NS observations to nuclear matter properties: a machine learning approach
• Bayesian inference of the dense matter equation of state built upon extended Skyrme interactions
• Multilayer neutron stars with scalar mesons crossing term
• Hyperons in the pasta phase
• Properties of binary components and remnant in GW170817 using equations of state in finite temperature field theory models
• Bayesian inference of finite-nuclei observables based on the KIDS model
• Thermodynamics of Hot Neutron Stars and Universal Relations
• Medium Effects in MIT Bag Model for quark matter: Self consistent thermodynamical treatment
• Bayesian constraints on covariant density functional equations of state of compact stars with new NICER mass-radius measurements
• Probing fermionic asymmetric dark matter cores using global neutron star properties
• The Influence of Muons, Pions, and Trapped Neutrinos on Neutron Star Mergers
• Universal relations for compact stars with exotic degrees of freedom
• Hubble constant and nuclear equation of state from kilonova spectro-photometric light curves
• Embedding short-range correlations in relativistic density functionals through quasi-deuterons
• Quarkyonic matter state of neutron stars
• Studying the parameters of the extended $\sigma$-$\omega$ model for neutron star matter
• Quantifying the uncertainties on spinodal instability in stellar matter through meta-modeling
• Gravitational waves from isolated neutron stars: mass dependence of r-mode instability
• Rotating hybrid stars with the Dyson-Schwinger quark model
• Neutron star-black hole coalescence rate inferred from macronova/kilonova observations
• Nuclear skin and the curvature of the symmetry energy
• Properties of nuclear matter in relativistic Brueckner-Hartree-Fock model with high-precision charge-dependent potentials
• Critical mass, moment of inertia and universal relations of rapidly rotating neutron stars with exotic matter
• New equation of state involving Bose-Einstein condensate of antikaon for supernova and neutron star merger simulations
• The Equation of State of Neutron-Rich Matter at Fourth Order of Chiral Effective Field Theory and the Radius of a Medium-Mass Neutron Star
• Properties of First-Order Hadron-Quark Phase Transition from Inverting Neutron Star Observables
• Novel Scalings of Neutron Star Properties from Analyzing Dimensionless Tolman--Oppenheimer--Volkoff Equations
• Gray Two-moment Neutrino Transport: Comprehensive Tests and Improvements for Supernova Simulations
• Observing the Ping-pong Modality of Isospin Degree of Freedom in Cluster Emission from Heavy Ion Reactions
• Precursor of Superfluidity in a Strongly Interacting Fermi Gas with Negative Effective Range
• Topology change, emergent symmetries and compact star matter
• Short range correlations in the extended quantum molecular dynamics model
• Impact of the nuclear equation of state on the formation of twin stars
• Correlations among symmetry energy elements in Skyrme models
• Unitary $p$-wave Fermi gas in one dimension
• Intersections of ultracold atomic polarons and nuclear clusters: How is a chart of nuclides modified in dilute neutron matter?
• Binding two and three $\alpha$ particles in cold neutron matter
• Confronting new NICER mass-radius measurements with phase transition in dense matter and twin compact stars
• Late time supernova neutrino signal and proto-neutron star radius
• Massive relativistic compact stars from SU(3) symmetric quark models
• Imprints of the nuclear symmetry energy slope in gravitational wave signals emanating from neutron stars
• Many-body approximations to the superfluid gap and critical temperature in pure neutron matter
• Neutron stars formation and Core Collapse Supernovae
• Warm unstable asymmetric nuclear matter: critical properties and the density dependence of the symmetry energy
• Nonparametric Representation of Neutron Star Equation of State Using Variational Autoencoder
• Asymmetric Nuclear Light Clusters In Supernova Matter
• QCD-like phase diagram with Efimov trimers and Cooper pairs in resonantly interacting SU(3) Fermi gases
• Improved method for the experimental determination of in-medium effects from heavy-ion collisions
• Role of the symmetry energy slope in neutron stars: exploring the model-dependency
• Pulse Profile Modeling of Thermonuclear Burst Oscillations I: The Effect of Neglecting Variability
• Baryonic dense matter in view of gravitational-wave observations
• Relativistic correction to the r-mode frequency in light of multi-messenger constraints
• Extended NJL model for baryonic matter and quark matter
• Prospects for optical detections from binary neutron star mergers with the next-generation multi-messenger observatories
• Effects of nuclear matter and composition in core-collapse supernovae and long-term proto-neutron star cooling
• Shear oscillations in neutron stars and the nuclear symmetry energy
• Finite-temperature effects in dynamical-spacetime binary neutron star merger simulations: Validation of the parametric approach
• Polytropic fits of modern and unified equations of state
• Bayesian inference of neutron-skin thickness and neutron-star observables based on effective nuclear interactions
• Nambu-Jona-Lasinio description of hadronic matter from a Bayesian approach
• Light clusters in warm stellar matter: calibrating the cluster couplings
• The $\Xi N$ interaction constrained by recent ${\Xi }^{-}$ hypernuclei experiments
• From finite nuclei to neutron stars : the essential role of high-order density dependence in effective forces
• thornado-hydro: a discontinuous Galerkin method for supernova hydrodynamics with nuclear equations of state
• The proto-neutron star inner crust in the liquid phase
• Minimal Length, Nuclear Matter, and Neutron Stars
• The neutron star inner crust: an empirical essay
• Actinide-boosting r Process in Black Hole-Neutron Star Merger Ejecta
• Multi-messenger observations of core-collapse supernovae: Exploiting the standing accretion shock instability
• Decoding rotating neutron stars: Role of the symmetry energy slope
• Properties of quark-matter cores in massive hybrid stars
• Gravitational-wave imprints of non-convex dynamics in binary neutron star mergers
• Quarkyonic matter and quarkyonic stars in an extended RMF model
• Probing short-range correlations in asymmetric nuclei with quasi-free pair knockout reactions
• Modified Urca neutrino emissivity at finite temperature
• Revisiting the post-glitch relaxation of the 2000 Vela glitch with the neutron star equation of states in the Brueckner and relativistic Brueckner theories
• A Generalized Double Chaplygin Model for Anisotropic Matter: The Newtonian Case
• Bayesian analysis of hybrid neutron star EOS constraints within an instantaneous nonlocal chiral quark matter model
• Neutron-skin values and matter and neutron radii determined from reaction cross sections of proton scattering on ${}^{12}$C, ${}^{40,48}$Ca, ${}^{58}$Ni, ${}^{208}$Pb
• Bayesian inference of strangeon matter using the measurements of PSR J0437-4715 and GW190814
• Estimation of the slope of nuclear symmetry energy via charge radii of mirror nuclei
• Premerger phenomena in neutron-star binary coalescences
• Auxiliary Function Approach for Determining Symmetry Energy at Supra-saturation Densities
• Effects of retarded electrical fields on observables sensitive to the high-density behavior of nuclear symmetry energy in heavy-ion collisions at intermediate energies
• Anomalous quartic term in the expansion of the symmetry energy
• Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars
• Nuclear Symmetry Energy and Neutron Skin Thickness of ${}^{208}Pb$ using a finite range effective interaction
• Density of States of a Coupled-Channel System
• Partially accreted crusts of neutron stars
• Neutron star inner crust: effects of rotation and magnetic fields
• Effects of the momentum dependence of nuclear symmetry potential on pion observables in Sn + Sn collisions at 270 MeV/nucleon
• Interfacing branching random walks with Metropolis sampling: constraint release in auxiliary-field quantum Monte Carlo
• Hyperonic uncertainties in neutron stars, mergers and supernovae
• Kerr-Enhanced Optical Spring
• Cost of inferred nuclear parameters towards the f-mode dynamical tide in binary neutron stars
• Influence of the nuclear symmetry energy slope on observables of compact stars with $\Delta$-admixed hypernuclear matter
• Nuclear pasta and symmetry energy in the relativistic point-coupling model
• Equation of State of Neutron-Rich Matter in $d$-Dimensions
• Neutron Skins: Weak Elastic Scattering and Neutron Stars
• The proto-neutron star inner crust in a multi-component plasma approach
• Pulse Profile Modelling of Thermonuclear Burst Oscillations II: Handling variability
• Compact Objects in close orbits as Gravitational Wave Sources: Formation Scenarios and Properties
• Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Nucleonic models
• Phenomenological Equation of State of Strongly Interacting Matter with First-Order Phase Transitions and Critical Points
• Influence of effective nucleon mass on equation of state for supernova simulations and neutron stars
• High $p_t$ squeezed-out n/p ratio as a probe of $K_{\mathrm{sym}}$ of the symmetry energy
• Accretion-Induced Collapse of Dark Matter Admixed White Dwarfs -- II: Rotation and Gravitational-wave Signals
• Problematic systematics in neutron-star merger simulations
• Strong magnetic fields and pasta phases revisited
• Directed and elliptic flows of protons and deuterons in HADES Au+Au collisions at $\sqrt{s_{\mathrm{NN}}}=2.4$ GeV
• Impact of ground-state properties and collective excitations on the Skyrme ansatz: a Bayesian study
• Investigating the role of nuclear parameters on oscillation modes in hot Neutron Stars
• Nuclear physics with gravitational waves from neutron stars disrupted by black holes
• Effect of the crust on neutron star empirical relations
• Employing ternary fission of ${}^{242}$Pu as a probe of very neutron rich matter
• Sensitivity of nuclear statistical equilibrium to nuclear uncertainties during stellar core collapse
• Collisional dynamics of polaronic clouds immersed in a Fermi sea
• Accurate nuclear symmetry energy at finite temperature within a BHF approach
• Relativistic self-energy decomposition of nuclear symmetry energy and equation of state of neutron matter within QCD sum rules
• Nuclear pasta in hot and dense matter and its influence on the equation of state for astrophysical simulations
• Strong Gravity Extruding Peaks in Speed of Sound Profiles of Massive Neutron Stars
• Properties of ${}^{208}$Pb predicted from the relativistic equation of state in the full Dirac space
• Parametrization of the surface energy in the ETF approximation
• High Density with Elliptic Flows
• Sensitivity of the evaporation residue observables to the symmetry energy
• Impact of strong magnetic fields on the inner crust of neutron stars
• Neutron star cooling and mass distributions
• Effects of incompressibility $K_0$ in heavy-ion collisions at intermediate energies
• Neutron star mass formula with nuclear saturation parameters
• Strong magnetic fields: neutron stars with an extended inner crust
• Quiescent luminosities of accreting neutron stars with different equation of states
• Polaronic Proton and Diproton Clustering in Neutron-Rich Matter
• Universal relations to measure neutron star properties from targeted r-mode searches
• The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy
• Phase-transition-induced collapse of proto-compact stars and its implication for supernova explosions
• Evidence for strong isovector nuclear spin-orbit interaction
• Quark condensate and chiral symmetry restoration in neutron stars
• Neutron star deformability with hyperonization in density-dependent relativistic mean-field models
• Hyperons during proto-neutron star deleptonization and the emission of dark flavoured particles
• Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities
• What can be learned from a proto-neutron star's mass and radius?
• Correlation between the symmetry energy slope and the deconfinement phase transition
• Intrinsic Correlations Among Characteristics of Neutron-rich Matter Imposed by the Unbound Nature of Pure Neutron Matter
• Equation of state in neutron stars and supernovae
• Measuring spin in coalescing binaries of neutron stars showing double precursors
• The nuclear symmetry energy from relativistic Brueckner-Hartree-Fock model
• Study of ($p,n$)IAS and (${}^3$He,$t$)IAS charge-exchange reactions with the $G$-matrix folding method
• Equilibrium nuclear ensembles taking into account vaporization of hot nuclei in dense stellar matter
• The outer crust of a cold, non-accreting neutron star within the Quark-Meson Coupling (QMC) model
• Critical behaviour of an effective relativistic mean field model in the presence of magnetic background and boundaries
• Optimized Statistical Approach for Comparing Multi-Messenger Neutron Star Data
• Hyperonization in compact stars
• QCD phase transition and equation of state of stellar strong interaction matter via Dyson-Schwinger equation approach
• The impact of hyperons on neutron star mergers: gravitational waves, mass ejection and black hole formation
• Treating divergence in quark matter by using energy projectors
• Nuclear matter from the ladder resummation in terms of the experimental nucleon-nucleon scattering amplitudes
• Hybrid stars within the framework of the Sigma-Omega-Rho model combined with the MIT and NJL models
• Light clusters in the liquid proto-neutron star inner crust
• Virialized equation of state for warm and dense stellar plasmas in proto-neutron stars and Supernova matter
• Impact of Hot Inner Crust on Compact Stars at Finite Temperature
• Role of local anisotropy in hybrid stars
• Unraveling Trace Anomaly of Supradense Matter via Neutron Star Compactness Scaling
• The nuclear symmetry energy and the neutron skin thickness in nuclei
• Rotating Neutron Stars with the Relativistic Ab Initio Calculations
• Isotopic equilibrium constants for very low-density and low-temperature nuclear matter
• Critical properties of calibrated relativistic mean-field models for the transition to warm, non-homogeneous nuclear matter
• Bayesian inference of neutron star crust properties using an ab initio-benchmarked meta-model
• Composition of scalar mesons and their effects on nuclear matter properties in an extended linear sigma model
• Symmetry energy of super-dense neutron-rich matter from integrating barotropic pressures in neutron stars and heavy-ion reactions
• Towards a unified hadron-quark equation of state for neutron stars within the relativistic mean-field model
• Crust (Unified) Tool for Equation-of-state Reconstruction (CUTER) v2
• Influence of the tetraneutron on the EoS under core-collapse supernovae and heavy-ion collisions conditions
• RMF models with $\sigma$-scaled hadron masses and couplings for description of heavy-ion collisions below 2A GeV
• Bayesian analysis of a relativistic hadronic model constrained by recent astrophysical observations
• Phase transitions and latent heat in magnetized matter
• Revisiting the isospin relaxation time in intermediate-energy heavy-ion collisions
• Cooling of Isolated Neutron Stars with Pion Condensation: Possible Fast Cooling in a Low-Symmetry-Energy Model
• Neutron star crustal properties from relativistic mean-field models and bulk parameters effects
• Neutron Stars: Laboratories for fundamental physics under extreme astrophysical conditions
• Finite-temperature infinite matter with effective-field-theory-inspired energy-density functionals
• Investigating the role of nuclear parameters in Neutron Star oscillations: a model comparison
• From masses and radii of neutron stars to EOS of nuclear matter through neural network
• Direct nonparametric multimessenger constraints on the equation of state of cold dense nuclear matter
• Implementing advanced trial wave functions in fermion quantum Monte Carlo via stochastic sampling
• Density dependence of symmetry energy and neutron skin thickness revisited using relativistic mean field models with nonlinear couplings
• An Undergraduate Approach to the Quantum Hadrodynamics and the Physics of Neutron Stars
• Equation of state and neutrino transfer in supernovae and neutron stars
• Neutron-star seismology with realistic, finite-temperature nuclear matter
• Investigating the Impact of Higher-Order Phase Transitions in Binary Neutron-Star Mergers
• Cooling of the Cassiopeia A neutron star and the effect of diffusive nuclear burning
• Experimental nuclear astrophysics in Italy
• Nucleon momentum gap in asymmetric nuclear matter
• Neutron star cooling within the equation of state with induced surface tension
• Non-Radial Oscillation Modes in Hybrid Stars with Hyperons and Delta Baryons
• Effects of inner crusts on $g$-mode oscillations in neutron stars
• Explosive Nucleosynthesis: What we learned and what we still do not understand
• Neutron-proton differential transverse flow in ${}^{132}$Sn + ${}^{124}$Sn collisions at 270 MeV/nucleon
• Revisit to the yield ratio of triton and ${}^3$He as an indicator of neutron-rich neck emission
• Tidal deformability of neutron stars with exotic particles within a density dependent relativistic mean field model in R-squared gravity
• Simple fits for the neutrino luminosities from protoneutron star cooling
• Resonance-to-bound transition of ${}^5$He in neutron matter and its analogy with heteronuclear Feshbach molecule
• Equation of State of Hot Neutron Star Matter using Finite Range Simple Effective Interaction
• Effects of phase transition in hybrid stars from quark-meson coupling hadronic matter to deconfined quark matter
• Reexamination of ${}^6$Li scattering as a Probe to Investigate the Isoscalar Giant Resonances in Nuclei
• Construction of energy density functional for arbitrary spin polarization using functional renormalization group
• Study of nuclear matter properties for Hybrid EoS
• Bayesian Inference of Hybrid Star Properties from Future High-Precision Measurements of Their Radii
• Strong toroidal magnetic fields sustained by the elastic crust in a neutron star
• I-C-Q relations for rapidly rotating stable hybrid stars
• Quark deconfinement in compact stars through sexaquark condensation
• Perturbed nuclear matter studied within Density Functional Theory with a finite number of particles
• Dependence of postmerger properties on the thermal heating efficiency in neutron star mergers
• Strange matter in compact stars
• Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches
• Suitable resolution for EOS tables in neutron star investigation
• Probing Strange Dark Matter through $f$-mode Oscillations of Neutron Stars with Hyperons and Quark Matter
• Nucleon Short-Range Correlations and High-Momentum Dynamics: Implications on the Equation of State of Dense Matter
• Comparing strange and non-strange quark stars within resummed QCD at NLO
• How do mirror charge radii constrain density dependence of the symmetry energy?
• Strongly interacting matter in extreme magnetic fields
• Pairing effects on neutron matter equation of state and symmetry energy at subsaturation densities
• Nuclear physics inputs for dense-matter modelling in neutron stars. The nuclear equation of state
• Exploring nuclear force with pulsar glitch observation
• Gravitation with modified fluid Lagrangian: Variational principle and an early dark energy model
• New Insights into Supradense Matter from Dissecting Scaled Stellar Structure Equations
• $f$-mode oscillations in hot Neutron Stars: Effect of hyperons and neutrino trapping
• Impact of the relativistic Cowling approximation on shear and interface modes of neutron stars
• Excitation of the isoscalar giant monopole resonance using 6Li inelastic scattering
• Constraining the Hadron-Quark Phase Transition Chemical Potential via Astronomical Observation
• Neutron Star Radii from Laboratory Experiments
• Dense Hadronic Matter in Neutron Stars
• Fermi-Dirac Integrals in Degenerate Regimes: A Novel Asymptotic Expansion
• Novel features of asymmetric nuclear matter from terrestrial experiments and astrophysical observations of neutron stars
• Framework for phase transitions between the Maxwell and Gibbs constructions at finite temperature
• The Impact of $f(\mathcal{G},T)$ Gravity on the Evolution of Cavity in the Cluster of Stars
• High-order isospin-dependent surface tension contribution to the fourth-order symmetry energy of finite nuclei
• Modification of hyperon masses in nuclear matter
• Fast neutron star cooling in light of the PREX-2 experiment
• Probing Fundamental Physics with Gravitational Waves
• Stiffening of matter in quark-hadron continuity: a mini-review
• Fluctuations of work in realistic equilibrium states of quantum systems with conserved quantities
• Simulating Binary Neutron Star Mergers with Finite-temperature Equations of State: The influences of the slope of the symmetry energy and artificial heating
• Nuclear mass table in density functional approach inspired by neutron-star observations
• The Yukawa potential under weak magnetic field
• One- and two-argument equation of state parametrizations with continuous sound speed for neutron star simulations
• Quartet correlations near the surface of $N=Z$ nuclei
• Simulating bulk viscosity in neutron stars. I. Formalism
• Strong correlation of the neutron star core-crust transition density with the $\sigma$-meson mass via vacuum polarization
• Nuclear incompressibility from spherical and deformed nuclei
• The origin of the elements and other implications of gravitational wave detection for nuclear physics
• Inner crust equations of state for CompOSE
• Thermal Evolution of Neutron Stars as a Probe of Physics beyond the Standard Model
• Imprints of high-density nuclear symmetry energy on the crustal fraction of neutron star moment of inertia
• Neutron stars from crust to core within the Quark-meson coupling model
• Rotating Neutron Stars with Dark Matter Halos
• Experimental investigation of ground-state properties of ${}^7$H with transfer reactions
• STROBE-X: A probe-class mission for X-ray spectroscopy and timing on timescales from microseconds to years
• Modification of the universal relation between mass, radius and nonradial $f$-mode oscillation in proto-neutron stars
• Finite-temperature equation of state with hyperons
• Properties and microscopic structures of dense stellar matter in RMF models
• Anisotropic pressure effect on central EOS of PSR J0740+6620 in the light of dimensionless TOV equation
• Tension between implications from PREX-2 data and gravitational tidal response on dense matter equation of state
• Neutron star properties: Constraining the nuclear matter EoS
• Properties of fermionic systems with the Path-integral ground state method
• Kaon production in the HADES experiment in Au+Au collisions at $\sqrt{s_{\mathrm{NN}}}=2.4$ GeV
• Dipole Polarizability of Finite Nuclei as a Probe of Neutron Stars
• Joint Inference of Population, Cosmology, and Neutron Star Equation of State from Gravitational Waves of Dark Binary Neutron Stars
• Effect of symmetry energy on properties of rapidly rotating neutron stars and universal relations
• Neutron stars with Bogoliubov quark-meson coupling model
• Dineutron decay into sterile anti-neutrinos in neutron stars and its observable consequences
• Polaronic neutron in dilute alpha matter: A $p$-wave Bose polaron
• New {\em ab initio} constrained extended Skyrme equations of state for simulations of neutron stars, supernovae and binary mergers: I. Subsaturation density domain
• Recent progress on superstrange dynamics
• Finding signatures of the nuclear symmetry energy in heavy-ion collisions with deep learning
• Phase-space excluded-volume approach for light clusters in nuclear medium
• Equation of state for hot hyperonic neutron star matter
• Alpha clustering in warm and dense nuclear matter from heavy-ion collisions
• Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars?
• Effects of the symmetry energy slope on magnetized neutron stars
• Heavy Neutron Star Phenomenology with an H-dibaryon
• Series solutions to the TOV equations
• Phase transitions and finite-size effects in integrable virial statistical models
• Estimation of neutron star mass and radius of FRB 20240114A by identification of crustal oscillations
• Is The Trace Anomaly at its Minimum Value at Neutron Star Centers?
• The sharpness of the quark-hadron transition and the properties of hybrid stars
• Investigating the possibility of extracting neutron-skin thickness in nuclei by their collisions at intermediate energies
• Neutron stars as extreme gravity probes
• Impact of hyperons on structural properties of neutron stars and hybrid stars within the regularized four-dimensional Einstein-Gauss-Bonnet gravity
• Gauge invariance of quantum electrodynamics of multi-electron atoms
• Machine learning-driven conservative-to-primitive conversion in hybrid piecewise polytropic and tabulated equations of state
• Rotating neutron stars with chaotic magnetic fields in general relativity and Rastall gravity
• Correlated structure of nuclear symmetry energy from covariant nucleon self-energy
• Landau parameters and entrainment matrix of cold stellar matter: effect of the symmetry energy and strong magnetic fields
• Cosmology from Strong Interactions
• Fermions with long and finite range interactions on a quantum ring
• Role of thermal fluctuations in nucleation of three-flavor quark matter
• Tidal Deformability of Quark Stars with Repulsive Interactions
• Structure of two- and three-alpha systems in cold neutron matter
• Numerical Approach to the Exterior Solution of Spherically Symmetric and Static Configuration in Scalar-Tensor Theories
• Stability of Neutron Star and Cosmological Constant
• Unified Equation of State for Neutron Stars Based on the Gogny Interaction
• The nuclear matter density functional under the nucleonic hypothesis
• Basic quantities of the Equation of State in isospin asymmetric nuclear matter
• Investigating Universal Relations in Compact Stars featuring $\Delta -$Admixed Exotic Dense Matter
• P-stars in the gravitational wave era
• Supernova Constraints on Dark Flavored Sectors
• Formation of large chunk of nuclear matter in heavy-ion collisions
• The thermal index of neutron-star matter in the virial approximation
• Triaxial instabilities in rapidly rotating Neutron Stars
• Updated estimates of post-merger gravitational wave energy released in GW170817 and the maximum neutron star mass
• The Strange Physics of Dark Baryons
• Nuclear Matter and Finite Nuclei: Relativistic Thomas-Fermi Approximation Versus Relativistic Mean-Field Approach
• Equation-of-State Independent Relations in Rapidly Rotating Hybrid Stars
• Angular momentum conservation and pion production in intermediate-energy heavy-ion collisions
• An Undergraduate Approach to the Quantum Hadrodynamics and the Physics of Neutron Stars Part II: Neutron Stars' Exotic Content
• Slowly rotating condensate dark stars beyond the mean-field approximation
• Symmetry energy of baryon- and neutron-rich nuclear matter
• Radial oscillations of quark stars in light of current astrophysical constraints: A comparative study
• Symmetry breaking and restoration on a fermionic quantum ring
• Recent applications of the subtracted second RPA method
• The effect of charm quark on the QCD chiral phase diagram
• Properties of rapidly rotating hot neutron stars within Brueckner theory
• Heavy baryons in hot stellar matter with light nuclei and hypernuclei
• Neutron skins probed in proton knockout from neutron-rich nuclei
• Medium effects on light clusters from heavy-ion collisions within a relativistic mean-field description
• Impact of crust-core connection procedures on the tidal deformability of neutron stars
• Fully general relativistic description of rapidly-rotating axially-symmetric neutron stars for constraining nuclear matter equations of state
• Observation of $\bar{\Lambda }p\to K^{+}{\pi }^{+}{\pi }^{-}{\pi }^0$ and $\bar{\Lambda }p\to K^{+}{\pi }^{+}{\pi }^{-}2{\pi }^0$
• Neutron Star Equation of State with Nucleon Short-Range Correlations: A Concise Review and Open Issues
• Collective effects in an incompressible electronic liquid
• Thermal liquid-gas phase transition in a quasi-one-dimensional dipolar Fermi gas
• Recurring region for neutron-star observables
• Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Influences of parametrizations of density dependent couplings
• Binding energy of compact stars and their non-radial oscillations
• Neutron drop trapped in axially deformed external fields
• Effects of three-baryon forces on kaon condensation in hyperon-mixed matter
• Probing neutron stars with the full pre-merger and post-merger gravitational wave signal from binary coalescences