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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• Constraining the nuclear matter equation of state around twice saturation density
• A New Equation of State for Astrophysical Simulations
• Can very compact and very massive neutron stars both exist?
• The Stability of Nuclear Matter in the Nambu-Jona-Lasinio Model
• Equation of state of fully ionized electron-ion plasmas
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• Evolution of Proto-Neutron Stars with Quarks
• Unified treatment of sub-saturation stellar matter at zero and finite temperature
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• Unified equation of state for neutron stars on a microscopic basis
• Core-collapse supernova explosions triggered by a quark-hadron phase transition during the early post-bounce phase
• Giant Quadrupole Resonances in 208Pb, the nuclear symmetry energy and the neutron skin thickness
• The Progenitor Dependence of the Preexplosion Neutrino Emission in Core-Collapse Supernovae
• High temperature expansion applied to fermions near Feshbach resonance
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• On the appearance of hyperons in neutron stars
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• The Nearest Millisecond Pulsar Revisited with XMM-Newton: Improved Mass-Radius Constraints for PSR J0437-4715
• Structure of the inner crust of neutron stars: crystal lattice or disordered phase ?
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• A nonlocal, covariant generalisation of the NJL model
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• Dynamics and neutrino signal of black hole formation in non-rotating failed supernovae. I. EOS dependence
• Simulation of Transitions between "Pasta" Phases in Dense Matter
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• Nuclear Pasta Formation
• PSR J1311-3430: A Heavyweight Neutron Star with a Flyweight Helium Companion
• Lattice Effective Field Theory for Medium-Mass Nuclei
• Tensor part of the Skyrme energy density functional. II: Deformation properties of magic and semi-magic nuclei
• Covariant representations of the relativistic Brueckner T-matrix and the nuclear matter problem
• Evolution of Proto-Neutron stars with kaon condensates
• Equation of state and thickness of the inner crust of neutron stars
• Modelization of the EOS
• Tables of Hyperonic Matter Equation of State for Core-Collapse Supernovae
• Keplerian frequency of uniformly rotating neutron stars and quark stars
• Strange quark matter with dynamically generated quark masses
• High Density Behaviour of Nuclear Symmetry Energy and High Energy Heavy-Ion Collisions
• Probing the Equation of State of Nuclear Matter via Neutron Star Asteroseismology
• Light nuclei quasiparticle energy shift in hot and dense nuclear matter
• Will black hole-neutron star binary inspirals tell us about the neutron star equation of state?
• PSR J1756$-$2251: a pulsar with a low-mass neutron star companion
• Vector interaction enhanced bag model for astrophysical applications
• Constraints on Neutron Star Crusts From Oscillations in Giant Flares
• The Strange Star Surface: A Crust with Nuggets
• Equation of state of hypernuclear matter: impact of hyperon--scalar-meson couplings
• The Double Pulsar J0737--3039: Testing the Neutron Star Equation of State
• The physics of neutron stars
• Microscopic calculations and energy expansions for neutron-rich matter
• Formation of Nuclear "Pasta" in Supernovae
• Experimental determination of the symmetry energy of a low density nuclear gas
• Effects of hyperons in binary neutron star mergers
• Chiral and deconfinement phase transitions of two-flavour QCD at finite temperature and chemical potential
• Relativistic Hartree-Fock-Bogoliubov theory with Density Dependent Meson-Nucleon Couplings
• Unmasking the nuclear matter equation of state
• Do we understand the incompressibility of neutron-rich matter?
• Cooling of Neutron Stars. Hadronic Model
• Progenitor models of the electromagnetic transient associated with the short GRB 130603B
• The influence of model parameters on the prediction of gravitational wave signals from stellar core collapse
• Impact of the symmetry energy on the outer crust of non-accreting neutron stars
• Evidence for 1122 Hz X-Ray Burst Oscillations from the Neutron-Star X-Ray Transient XTE J1739-285
• Symmetry energy from the nuclear collective motion: constraints from dipole, quadrupole, monopole and spin-dipole resonances
• In-medium chiral perturbation theory beyond the mean-field approximation
• Quark-Hadron Phase Transitions in Young and Old Neutron Stars
• Pushing 1D CCSNe to explosions: model and SN 1987A
• Astrophysical Implications of Equation of State for Hadron-Quark Mixed Phase: Compact Stars and Stellar Collapses
• Quantum Molecular Dynamics Approach to the Nuclear Matter Below the Saturation Density
• Dipole polarizability of 120Sn and nuclear energy density functionals
• Study of the Sigma-nucleus potential by the (pi^-,K^+) reaction on medium-to-heavy nuclear targets
• The physics of dense hadronic matter and compact stars
• Measuring the Cooling of the Neutron Star in Cassiopeia A with all Chandra X-ray Observatory Detectors
• Density dependence of the symmetry energy from neutron skin thickness in finite nuclei
• Constraining hypernuclear density functional with $\Lambda$-hypernuclei and compact stars
• Relativistic Point-Coupling Models as Effective Theories of Nuclei
• Chiral approach to nuclear matter: Role of two-pion exchange with virtual delta-isobar excitation
• A Second Relativistic Mean Field and Virial Equation of State for Astrophysical Simulations
• Hypernuclear matter in a complete SU(3) symmetry group
• Atmospheres and radiating surfaces of neutron stars
• Influence of light nuclei on neutrino-driven supernova outflows
• Upper limits on the observational effects of nuclear pasta in neutron stars
• Accurate nuclear masses from a three parameter Kohn-Sham DFT approach (BCPM)
• Low densities in nuclear and neutron matters and in the nuclear surface
• Application of the density dependent hadron field theory to neutron star matter
• Proton elastic scattering from tin isotopes at 295 MeV and systematic change of neutron density distributions
• Rejecting proposed dense-matter equations of state with quiescent low-mass X-ray binaries
• The effect of accretion on the measurement of neutron star mass and radius in the low-mass X-ray binary 4U 1608-52
• Kaon Condensation in Proto-Neutron Star Matter
• Neutron skin thickness of heavy nuclei with $\alpha$-particle correlations and the slope of the nuclear symmetry energy
• Energy density functional for nuclei and neutron stars
• Appearance of Light Clusters in Post-bounce Evolution of Core-Collapse Supernovae
• Hartree-Fock approach to nuclear matter and finite nuclei with M3Y-type nucleon-nucleon interactions
• Gravitational wave signatures in black-hole-forming core collapse
• Khon-Sham Density Functional Inspired Approach to Nuclear Binding
• Baryon-Baryon Interactions in the Flavor SU(3) Limit from Full QCD Simulations on the Lattice
• Laboratory Tests of Low Density Astrophysical Equations of State
• The Virial Equation of State of Low-Density Neutron Matter
• Shell and isospin effects in nuclear charge radii
• Masses of neutron stars and nuclei
• Accurate determination of the interaction between $\Lambda$ hyperons and nucleons from auxiliary field diffusion Monte Carlo calculations
• Signature of gravitational radiation in afterglow of short Gamma-Ray Bursts?
• Thermodynamic properties of nuclear "pasta" in neutron star crusts
• Spin and spin-isospin instabilities in asymmetric nuclear matter at zero and finite temperatures using Skyrme functionals
• Properties of the nuclear medium
• Thermodynamics of isospin-asymmetric nuclear matter from chiral effective field theory
• New constraints on the cooling of the Central Compact Object in Cas A
• A new equation of state for neutron star matter with nuclei in the crust and hyperons in the core
• Quantum Monte Carlo calculations of neutron matter with non-local chiral interactions
• Hyperon-Nucleon Interactions and the Composition of Dense Nuclear Matter from Quantum Chromodynamics
• Origin of the neutron skin thickness of 208Pb in nuclear mean-field models
• The pasta phase within density dependent hadronic models
• Determining the density content of symmetry energy and neutron skin: an empirical approach
• The Stability of Strange Star Crusts and Strangelets
• The mass and the radius of the neutron star in the transient low mass X-ray binary SAX J1748.9-2021
• Towards a model-independent constraint of the high-density dependence of the symmetry energy
• Auxiliary-Field Quantum Monte Carlo Simulations of Neutron Matter in Chiral Effective Field Theory
• Analysis of bulk and surface contributions in the neutron skin of nuclei
• Hyperon stars at finite temperature in the Brueckner theory
• Hybrid protoneutron stars with the MIT bag model
• New applications of renormalization group methods in nuclear physics
• The Sensitivity of Core-Collapse Supernovae to Nuclear Electron Capture
• Effect of superfluidity on neutron star crustal oscillations
• On the Importance of the Equation of State for the Neutrino-Driven Supernova Explosion Mechanism
• Electric Dipole Polarizability in ${}^{208}$Pb as a Probe of the Symmetry Energy and Neutron Matter around ${\rho }_0/3$
• Beta-decay rates of r-process nuclei in the relativistic quasiparticle random phase approximation
• Nuclear thermodynamics from chiral low-momentum interactions
• Non-congruence of the nuclear liquid-gas and deconfinement phase transitions
• Nuclear symmetry energy at subnormal densities from measured nuclear masses
• On the Cooling of the Neutron Star in Cassiopeia A
• Semi-classical equation of state and specific heats for neutron-star inner crust with proton shell corrections
• Effects of the two-body and three-body hyperon-nucleon interactions in Λ-hypernuclei
• Neutron stars with hyperon cores: stellar radii and EOS near nuclear density
• A new baryonic equation of state at sub-nuclear densities for core-collapse simulations
• Microscopically-based energy density functionals for nuclei using the density matrix expansion: Implementation and pre-optimization
• Comparative study of neutron and nuclear matter with simplified Argonne nucleon-nucleon potentials
• Information content of the low-energy electric dipole strength: correlation analysis
• Isospin Diffusion and Equilibration for Sn+Sn collisions at E/A=35 MeV
• Hybrid stars with the Dyson-Schwinger quark model
• Extended-soft-core Baryon-Baryon Model I. Nucleon-Nucleon Scattering (ESC04) Extended-soft-core Baryon-Baryon Model I. Nucleon-Nucleon Scattering (ESC04)
• Statistical approach for supernova matter
• Phase diagram of nuclear "pasta" and its uncertainties in supernova cores
• A Metal-Rich Low-Gravity Companion to a Massive Millisecond Pulsar
• Constraints on symmetry energy and nucleon effective mass splitting with Heavy Ion Collisions
• The Fate of the Compact Remnant in Neutron Star Mergers
• Warm pasta phase in the Thomas-Fermi approximation
• Thermodynamic functions of harmonic Coulomb crystals
• A New Code for Proto-Neutron Star Evolution
• Role of isospin in the nuclear liquid-gas phase transition
• Partial Wave Analysis of Nucleon-Nucleon Scattering below pion production threshold
• Power Counting of Contact-Range Currents in Effective Field Theory
• Entrainment coefficient and effective mass for conduction neutrons in neutron star crust: simple microscopic models
• Formation of black hole and accretion disk in a massive high-entropy stellar core collapse
• New equations of state based on the liquid drop model of heavy nuclei and quantum approach to light nuclei for core-collapse supernova simulations
• Linear response theory and neutrino mean free path using Brussels-Montreal Skyrme functionals
• The neutron star inner crust and symmetry energy
• Phase separation in the crust of accreting neutron stars
• Thermal properties of hot and dense matter with finite range interactions
• Charge screening effect in the hadron-quark mixed phase
• Evidence for 6ΛH
• Neutron star properties and the equation of state of neutron-rich matter
• Isovector properties of the Gogny interaction
• Entrainment parameters in cold superfluid neutron star core
• Deconfinement Phase Transition in Compact Stars : Maxwell vs. Gibbs Construction of the Mixed Phase
• Parametrization of light nuclei quasiparticle energy shifts and composition of warm and dense nuclear matter
• Nuclear matter symmetry energy and the symmetry energy coefficient in the mass formula
• Thermal properties of supernova matter: The bulk homogeneous phase
• Non-perturbative methods for a chiral effective field theory of finite density nuclear systems
• Hot neutron matter from a Self-Consistent Green's Functions approach
• Relativistic nuclear model with point-couplings constrained by QCD and chiral symmetry
• Statistical description of complex nuclear phases in supernovae and proto-neutron stars
• Possible Constraints on the Density Dependence of the Nuclear Symmetry Energy from Quasiperiodic Oscillations in Soft Gamma Repeaters
• Neutron-proton elliptic flow difference as a probe for the high density dependence of the symmetry energy
• Supernova neutrinos and nucleosynthesis
• Quantum Monte Carlo approaches to nuclear and atomic physics
• Formation of hot heavy nuclei in supernova explosions
• Nuclear matter in the crust of neutron stars
• The Burst Spectra of EXO 0748-676 during a Long 2003 XMM-Newton Observation
• Measurement of the Xi-p Scattering Cross Sections at Low Energy
• EMMI Rapid Reaction Task Force Meeting on 'Quark Matter in Compact Star'
• Hyperons in neutron stars and supernova cores
• Relativistic nuclear energy density functional constrained by low-energy QCD
• Variational study for the equation of state of asymmetric nuclear matter at finite temperatures
• Accurate calibration of relativistic mean-field models: correlating observables and providing meaningful theoretical uncertainties
• The Neutron Star Crust: Nuclear Physics Input
• Nuclear Waffles
• Effects of color superconductivity on the nucleation of quark matter in neutron stars
• Conditions for Phase Equilibrium in Supernovae, Proto-Neutron and Neutron Stars
• Appearance of the Single Gyroid Network Phase in Nuclear Pasta Matter
• Color-superconductivity in the strong-coupling regime of Landau gauge QCD
• Recent breakthroughs in Skyrme-Hartree-Fock-Bogoliubov mass formulas
• The tensor part of the Skyrme energy density functional. III. Time-odd terms at high spin
• The Microscopic Approach to Nuclear Matter and Neutron Star Matter
• A comparative study of statistical models for nuclear equation of state of stellar matter
• Generalized Beth--Uhlenbeck approach to mesons and diquarks in hot, dense quark matter
• The entrainment matrix of a superfluid neutron-proton mixture at a finite temperature
• Spurious finite-size instabilities in nuclear energy density functionals
• Coupled-cluster studies of infinite nuclear matter
• Symmetry energy of deformed neutron-rich nuclei
• Dirac-Brueckner-Hartree-Fock versus chiral effective field theory
• An Upper Bound on Neutron Star Masses from Models of Short Gamma-ray Bursts
• Neutrino Breakup of A=3 Nuclei in Supernovae
• Density dependence of nuclear symmetry energy constrained by mean-field calculations
• The Mass and Radius of the Neutron Star in the Bulge Low-Mass X-ray Binary KS 1731-260
• Time-Dependent Hartree-Fock Approach to Nuclear Pasta at Finite Temperature
• Experimental Determination of In-Medium Cluster Binding Energies and Mott Points in Nuclear Matter
• Semiclassical Distorted Wave Model Analysis of the $({\pi }^{-},K^{+})$ $\Sigma$ Formation Inclusive Spectrum
• On the relativistic Thomas-Fermi treatment of compressed atoms and compressed nuclear matter cores of stellar dimensions
• Nuclear matter in the crust of neutron stars derived from realistic NN interactions
• Microscopic Study of Slablike and Rodlike Nuclei: Quantum Molecular Dynamics Approach
• An extended equation of state for core-collapse simulations
• Thermal properties of asymmetric nuclear matter with an improved isospin- and momentum-dependent interaction
• Experimental effects on dynamics and thermodynamics in nuclear reactions on the symmetry energy as seen by the CHIMERA 4$\pi$ detector
• Light clusters, pasta phases and phase transitions in core-collapse supernova matter
• Symmetric and asymmetric nuclear matter in the relativistic approach at finite temperatures
• Quark-Meson Coupling Model, Nuclear Matter Constraints and Neutron Star Properties
• The Nuclear Matter Symmetry Energy at $0.03\le \rho /{\rho }_0\le 0.2$
• Effective Nucleon Masses from Heavy Ion Collisions
• Many-body forces in the equation of state of hyperonic matter
• The statistical multifragmentation model for liquid-gas phase transition with a compressible nuclear liquid
• The hyperon-nucleon interaction: conventional versus effective field theory approach
• Phases of hot nuclear matter at subnuclear densities
• Mass and radius formulas for low-mass neutron stars
• Chiral thermodynamics of nuclear matter
• Cluster formation in compact stars: relativistic versus Skyrme models
• Equation of state of classical Coulomb plasma mixtures
• Constraining supernova equations of state with equilibrium constants from heavy-ion collisions
• Chemical potential and the gap equation
• Entrainment coefficient and effective mass for conduction neutrons in neutron star crust: II Macroscopic treatment
• Compact stars in a SU(3) Quark-Meson Model
• Quark deconfinement transition in hyperonic matter
• Equation of State of Dense Matter from a density dependent relativistic mean field model
• Rapid cooling of the compact star in Cassiopea A as a phase transition in dense QCD
• The Neutrino Response of Low-Density Neutron Matter from the Virial Expansion
• Topological characterization of neutron star crusts
• Constraints on the Mass and Radius of the Neutron Star XTE J1807-294
• Nuclear symmetry energy and the r-mode instability of neutron stars
• Liquid-gas phase transition in nuclear matter from realistic many-body approaches
• Sensitivity of the neutron star r-mode instability window to the density dependence of the nuclear symmetry energy
• Symmetry energy in nuclear density functional theory
• Protoneutron stars within the Brueckner-Bethe-Goldstone theory
• Emergence of hyperons in failed supernovae: trigger of the black hole formation
• Nuclear Matter EOS with a Three-body Force
• The Shear Viscosity and Thermal Conductivity of Nuclear Pasta
• Three dimensional structure of low-density nuclear matter
• Nuclear energy density functional from chiral pion-nucleon dynamics
• Hybrid protoneutron stars with the Dyson-Schwinger quark model
• Probing isospin- and momentum-dependent nuclear effective interactions in neutron-rich matter
• Phase diagrams in nonlocal PNJL models constrained by Lattice QCD results
• Gyroid Phase in Nuclear Pasta
• Search for ${}_{\Lambda }^6$H hypernucleus by the ${}^6$Li$({\pi }^{-},K^{+})$ reaction at $p_{{\pi }^{-}}$ = 1.2 GeV/$c$
• Effects of the liquid-gas phase transition and cluster formation on the symmetry energy
• Electric dipole response of 208Pb from proton inelastic scattering: constraints on neutron skin thickness and symmetry energy
• The relativistic entrainment matrix of a superfluid nucleon-hyperon mixture at zero temperature
• Detecting the QCD phase transition in the next Galactic supernova neutrino burst
• Addendum to "Equation of state of classical Coulomb plasma mixtures"
• The equation of state and composition of hot, dense matter in core-collapse supernovae
• Constraining mean-field models of the nuclear matter equation of state at low densities
• Effects of mesonic correlations in the QCD phase transition
• The influence of inelastic neutrino reactions with light nuclei on the standing accretion shock instability in core-collapse supernovae
• Light nuclei in supernova envelopes: a quasiparticle gas model
• On the unlocking of color and flavor in color-superconducting quark matter
• Light clusters in nuclear matter: Excluded volume versus quantum many-body approaches
• Neutron matter at finite temperature
• Lepton effects on the proto-neutron stars with the hadron-quark mixed phase in the Nambu-Jona-Lasinio model
• Influence of pions and hyperons on stellar black hole formation
• Constraining the gravitational binding energy of PSR J0737-3039B using terrestrial nuclear data
• Densities and energies of nuclei in dilute matter
• Thermal Properties of Asymmetric Nuclear Matter
• Nucleon-Nucleon Potentials in Comparison: Physics or Polemics?
• Nuclear symmetry energy from the Fermi-energy difference in nuclei
• Neutron star structure and collective excitations of finite nuclei
• Covariant density functional theory: The role of the pion
• Triton-${}^3$He relative and differential flows as probes of the nuclear symmetry energy at supra-saturation densities
• New parameterization of Skyrme's interaction for regularized multi-reference energy density functional calculations
• Probing nuclear symmetry energy at high densities using pion, kaon, eta and photon productions in heavy-ion collisions
• From supernovae to neutron stars
• Strangeness-driven phase transition in (proto)- neutron star matter
• Symmetry energy, neutron skin, and neutron star radius from chiral effective field theory interactions
• Electron screening in the liquid-gas mixed phases of nuclear matter
• Light clusters and the pasta phase
• Next Generation Relativistic Models
• Towards a metallurgy of neutron star crusts
• Rotational Corrections to Neutron-Star Radius Measurements from Thermal Spectra
• In-medium nuclear cluster energies within the Extended Thomas-Fermi approach
• The relativistic Feynman-Metropolis-Teller treatment at finite temperatures
• Thermodynamic consistency for nuclear matter calculations
• The influence of Coulomb on the liquid-gas phase transition and nuclear multifragmentation
• The relativistic entrainment matrix of a superfluid nucleon-hyperon mixture. II. Effect of finite temperatures
• Impact of Quarks and Pions on Dynamics and Neutrino Signal of Black Hole Formation in Non-rotating Stellar Core Collapse
• Nuclear Partition Functions at Temperatures Exceeding 10^10 K
• Nuclear Masses and Neutron Stars
• Nuclear Many-Body Dynamics constrained by QCD and Chiral Symmetry
• Anomalous thermodynamics and phase transitions of neutron-star matter
• $\alpha$ particles and the pasta phase
• The structure of accreted neutron star crust
• Origin of symmetry energy in finite nuclei and density dependence of nuclear matter symmetry energy from measured alpha-decay energies
• Cluster formation in asymmetric nuclear matter: semi-classical and quantal approaches
• Hyperon Matter and Black Hole Formation in Failed Supernovae
• Hybrid neutron stars with the Dyson-Schwinger quark model and various quark-gluon vertices
• Dyson-Schwinger approach to color superconductivity at finite temperature and density
• Tabulated equation of state for supernova matter including full nuclear ensemble
• Nucleon-Meson Coupling Constants and Form Factors in the Quark Model
• Density dependent hadronic models and the relation between neutron stars and neutron skin thickness
• Liquid-gas coexistence vs. energy minimization with respect to the density profile in the inhomogeneous inner crust of neutron stars
• Post-shock-revival evolutions in the neutrino-heating mechanism of core-collapse supernovae
• Liquid-Gas Phase Transition of Supernova Matter and Its Relation to Nucleosynthesis
• Clusterized nuclear matter in the (proto-)neutron star crust and the symmetry energy
• Equation of state for $\beta$-stable hot nuclear matter
• Dilute resonating gases and the third virial coefficient
• Exploration of a modified density dependence in the Skyrme functional
• On the temperature dependence of the symmetry energy
• Revisit of the neutron/proton ratio puzzle in intermediate-energy heavy-ion collisions
• The QCD phase diagram from Schwinger-Dyson Equations
• Flow probe of symmetry energy in relativistic heavy-ion reactions
• Extended Skyrme interaction (II): ground state of nuclei and of nuclear matter
• Nuclear liquid-gas phase transition and supernovae evolution
• A Comparative study of hyperon equations of state in supernova simulations
• Effect of BCS pairing on entrainment in neutron superfluid current in neutron star crust
• Isospin Dynamics in Heavy Ion Collisions: from Coulomb Barrier to Quark Gluon Plasma
• Spin-orbit and tensor interactions in homogeneous matter of nucleons: accuracy of modern many-body theories
• The breathing-mode giant monopole resonance and the surface compressibility in the relativistic mean-field theory
• Momentum dependent mean-field dynamics of compressed nuclear matter and neutron stars
• Effect of Coulomb Screening Length on Nuclear Pasta Simulations
• Temperature and thermodynamic instabilities in heavy ion collisions
• Soft nuclear equation-of-state from heavy-ion data and implications for compact stars
• Sigma exchange in the nuclear force and effective field theory
• Strange quark matter in explosive astrophysical systems
• Surface effects in color superconducting strange-quark matter
• Limiting temperature from microscopic equation of state
• From the crust to the core of Neutron Stars on a microscopic basis
• Comparison of statistical treatments for the equation of state for core-collapse supernovae
• Cold quarks in medium: an equation of state
• Baryon formation and dissociation in dense hadronic and quark matter
• On the consistency of neutron-star radius measurements from thermonuclear bursts
• Exploring Hadron Physics in Black Hole Formations: a New Promising Target of Neutrino Astronomy
• Isospin-rich nuclei in neutron star matter
• Narrow Atomic Features from Rapidly Spinning Neutron Stars
• Phase transitions in Core-Collapse Supernova Matter at sub-saturation densities
• The Incompatibility of Rapid Rotation with Narrow Photospheric X-ray Lines in EXO 0748-676
• Modification of magicity towards the dripline and its impact on electron-capture rates for stellar core-collapse
• Extended Skyrme interaction (I): spin fluctuations in dense matter
• Extended Skyrme pseudo-potential deduced from infinite matter properties
• Phase transition towards strange matter
• Nucleosynthesis in core-collapse supernova explosions triggered by a quark-hadron phase transition
• Toward relativistic mean-field description of $\bar{\text{N}}$-nucleus reactions
• Non-Linear derivative interactions in relativistic hadrodynamics
• Symmetry energy of warm nuclear systems
• Low-momentum Hyperon-Nucleon Interactions
• Proton fraction in the inner neutron-star crust
• Beyond Nuclear Pasta: Phase Transitions and Neutrino Opacity of Non-Traditional Pasta
• Application of the nuclear equation of state obtained by the variational method to core-collapse supernovae
• Relativistic Mean Field Model with Generalized Derivative Nucleon-Meson Couplings
• The Negele-Vautherin density matrix expansion applied to the Gogny force
• Curvature effect on nuclear pasta: Is it helpful for gyroid appearance?
• Exotic nuclear phases in the inner crust of neutron stars in the light of Skyrme-Hartree-Fock theory
• Stellar Core Collapse with Hadron-Quark Phase Transition
• S-matrix approach to equation of state of nuclear matter
• Chiral Effective Field Theory for Nuclear Matter with long- and short-range Multi-Nucleon Interactions
• Isospin effects and symmetry energy studies with INDRA
• Ising analogue to compact-star matter
• Spin instabilities of infinite nuclear matter and effective tensor interactions
• Core collapse supernovae in the QCD phase diagram
• Instabilities in the Nuclear Energy Density Functional
• Hadron-Quark Crossover and Hot Neutron Stars at Birth
• Heavy-ion Collisions: Direct and indirect probes of the density and temperature dependence of Esym
• Effects of Electron Band Structure on Neutrino Pair Bremsstrahlung in Neutron Star Crusts
• Local energy-density functional approach to many-body nuclear systems with s-wave pairing
• Molecular Dynamics for Dense Matter
• Pasta phases in neutron star studied with extended relativistic mean field models
• Supernova Equation of State with an extended SU(3) Quark-Meson Model
• Reexamining the neutron skin thickness within a density dependent hadronic model
• Energy Dependent Isospin Asymmetry in Mean-Field Dynamics
• Quantum Monte Carlo study of dilute neutron matter at finite temperatures
• Hyperon-nucleon single-particle potentials with low-momentum interactions
• The High-Density Symmetry Energy in Heavy Ion Collisions
• The ASY-EOS experiment at GSI: investigating the symmetry energy at supra-saturation densities
• Classical Nucleation Theory of the One-Component Plasma
• Spin-orbit correlation energy in neutron matter
• Thermodynamics of clusterized matter
• Relativistic equation of state at subnuclear densities in the Thomas-Fermi approximation
• Low-momentum interactions for nuclei
• Pasta Structures of Quark-Hadron Phase Transition in Proto-Neutron Stars
• Finite size effects in Neutron Star and Nuclear matter simulations
• Neutron star equations of state with optical potential constraint
• EOSDB: The Database for Nuclear EoS
• Corrections to linear mixing in binary ionic mixtures and plasma screening at zero separation
• Constraints on possible phase transitions above the nuclear saturation density
• Strange matter in core-collapse supernovae
• Charged Ising Model of Neutron Star Matter
• Medium modification of two-particle scattering in nonideal Bose systems
• Self-consistent Green's functions with three-body forces
• Towards a quantal dynamical simulation of the neutron-star crust
• Shear Viscosity of the outer crust of Neutron stars: Ion Contribution
• Excluded-Volume Approximation for Supernova Matter
• Ordered bicontinuous double-diamond morphology in subsaturation nuclear matter
• A doubly-periodic structure for the study of inhomogeneous bulk fermion matter with spatial localizations
• The Quest for the Nuclear Equation of State
• Path Integral Variational Methods for Strongly Correlated Systems
• On the convergence of multi-channel effective interactions
• Understanding nuclear "pasta": current status and future prospects
• Fully antisymmetrised dynamics for bulk fermion systems
• Microscopic Study of Nuclear "Pasta" by Quantum Molecular Dynamics

Cited by in corpus (720)

• GW170817: Measurements of Neutron Star Radii and Equation of State
• A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
• GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4M_{\odot }$
• A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy
• Using gravitational-wave observations and quasi-universal relations to constrain the maximum mass of neutron stars
• Origin of the Heaviest Elements: the Rapid Neutron-Capture Process
• Neutron-star radius constraints from GW170817 and future detections
• Challenges and Opportunities of Gravitational Wave Searches at MHz to GHz Frequencies
• Neutron Star Mergers and Nucleosynthesis of Heavy Elements
• Nonparametric constraints on neutron star matter with existing and upcoming gravitational wave and pulsar observations
• Symmetry Parameter Constraints From A Lower Bound On The Neutron-Matter Energy
• A NICER view of PSR J0030+0451: Implications for the dense matter equation of state
• Neutron star tidal deformability and equation of state constraints
• Neutron Stars and the Nuclear Equation of State
• GW170817: constraining the nuclear matter equation of state from the neutron star tidal deformability
• Nuclear Equation of State from ground and collective excited state properties of nuclei
• Evidence for a maximum mass cut-off in the neutron star mass distribution and constraints on the equation of state
• Gravitational waves from neutron star mergers and their relation to the nuclear equation of state
• Estimating the Contribution of Dynamical Ejecta in the Kilonova Associated with GW170817
• Strangeness in Nuclei and Neutron Stars
• Constraining the dense matter equation of state with joint analysis of NICER and LIGO/Virgo measurements
• The Dynamics of Binary Neutron Star Mergers and of GW170817
• Rotating Stars in Relativity
• Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817
• Impact of the PSR J0740+6620 radius constraint on the properties of high-density matter
• Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy
• Nucleon Effective Masses in Neutron-Rich Matter
• Hydrodynamics of core-collapse supernovae and their progenitors
• Dense Nuclear Matter Equation of State from Heavy-Ion Collisions
• Superfluidity in nuclear systems and neutron stars
• How perturbative QCD constrains the Equation of State at Neutron-Star densities
• Anisotropic Compact stars in the Buchdahl model: A comprehensive study
• Chiral Effective Field Theory and the High-Density Nuclear Equation of State
• Grand Unified Neutrino Spectrum at Earth: Sources and Spectral Components
• Thermodynamics conditions of matter in neutron star mergers
• Combined Constraints on the Equation of State of Dense Neutron-Rich Matter from Terrestrial Experiments and Observations of Neutron Stars
• Astronuclear Physics: a Tale of the Atomic Nuclei in the Skies
• p-p, p-$\Lambda$ and $\Lambda$-$\Lambda$ correlations studied via femtoscopy in pp reactions at $\sqrt{s}$ = 7 TeV
• Information content of the parity-violating asymmetry in ${}^{208}$Pb
• Equation of state constraints from the threshold binary mass for prompt collapse of neutron star mergers
• A New Open-Source Nuclear Equation of State Framework based on the Liquid-Drop Model with Skyrme Interaction
• Towards the global description of nuclear charge radii: exploring the Fayans energy density functional
• Inferring the post-merger gravitational wave emission from binary neutron star coalescences
• Muons in supernovae: implications for the axion-muon coupling
• Neutron Star Merger Remnants
• Extracting Nuclear Symmetry Energies at High Densities from Observations of Neutron Stars and Gravitational Waves
• Study of the $\Lambda$-$\Lambda$ interaction with femtoscopy correlations in pp and p-Pb collisions at the LHC
• The Radius of PSR J0740+6620 from NICER with NICER Background Estimates
• Competition between delta isobars and hyperons and properties of compact stars
• Relativistic parameterizations of neutron matter and implications for neutron stars
• Bayesian Inference of High-density Nuclear Symmetry Energy from Radii of Canonical Neutron Stars
• Correlated Signatures of Gravitational-Wave and Neutrino Emission in Three-Dimensional General-Relativistic Core-Collapse Supernova Simulations
• A new temperature dependent hyperonic equation of state: application to rotating neutron star models and I-Q-relations
• Equation of state of dense nuclear matter and neutron star structure from nuclear chiral interactions
• GW190814's secondary component with mass $(2.50-2.67)$ M${}_{\odot }$ as a super-fast pulsar
• Heavy Baryons in Compact Stars
• Phases of dense matter in compact stars
• The Science of the Einstein Telescope
• A systematic study of proto-neutron star convection in three-dimensional core-collapse supernova simulations
• Proto-neutron stars with heavy baryons and universal relations
• Constraining nuclear matter parameters with GW170817
• Observing the post-merger signal of GW170817-like events with improved gravitational-wave detectors
• Beta equilibrium in neutron star mergers
• PSR J0030+0451, GW170817 and the nuclear data: joint constraints on equation of state and bulk properties of neutron stars
• Equation of state effects in the core collapse of a $20$-$M_{\odot }$ star
• Bayesian Inference of the Symmetry Energy of Super-Dense Neutron-Rich Matter from Future Radius Measurements of Massive Neutron Stars
• Dynamics of clusters and fragments in heavy-ion collisions
• Effects of symmetry energy on equation of state for simulations of core-collapse supernovae and neutron-star mergers
• A Parametrized Equation of State for Neutron Star Matter with Continuous Sound Speed
• Observational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger S190814bv
• GW190814: Spin and equation of state of a neutron star companion
• Theoretical and Experimental Constraints for the Equation of State of Dense and Hot Matter
• Treating quarks within neutron stars
• Equation of State Dependent Dynamics and Multimessenger Signals from Stellar-mass Black Hole Formation
• Towards mitigation of apparent tension between nuclear physics and astrophysical observations by improved modeling of neutron star matter
• Pions in hot dense matter and their astrophysical implications
• Constraining bosonic asymmetric dark matter with neutron star mass-radius measurements
• Exploring QCD matter in extreme conditions with Machine Learning
• Magnetic neutron star cooling and microphysics
• Bayesian Inference of Dense Matter Equation of State within Relativistic Mean Field Models using Astrophysical Measurements
• Bayesian analysis of the crust-core transition with a compressible liquid-drop model
• Comparison of Heavy-Ion Transport Simulations: Mean-field Dynamics in a Box
• Relativistic Anisotropic Fluid Spheres Satisfying a Non-Linear Equation of State
• Damping of density oscillations in neutrino-transparent nuclear matter
• Systematics of prompt black-hole formation in neutron star mergers
• The APR equation of state for simulations of supernovae, neutron stars and binary mergers
• $Abinitio$ constraints on thermal effects of the nuclear equation of state
• Neutrino emission characteristics of black hole formation in three-dimensional simulations of stellar collapse
• Implications of the mass $M=2.17_{-0.10}^{+0.11}$M${}_{\odot }$ of PSR~J0740+6620 on the Equation of State of Super-Dense Neutron-Rich Nuclear Matter
• Equation-of-state insensitive relations after GW170817
• A new equation of state for core-collapse supernovae based on realistic nuclear forces and including a full nuclear ensemble
• Higher-order symmetry energy and neutron star core-crust transition with Gogny forces
• Realistic Finite-Temperature Effects in Neutron Star Merger Simulations
• Inference of the sound speed and related properties of neutron stars
• Nuclear Equation of state for Compact Stars and Supernovae
• Coalescence of black hole--neutron star binaries
• Supernova Simulations Confront SN 1987A Neutrinos
• Holographic modeling of nuclear matter and neutron stars
• Equation of State Dependence of Gravitational Waves in Core-Collapse Supernovae
• Relativistic hybrid stars in light of the NICER PSR J0740+6620 radius measurement
• Relativistic hypernuclear compact stars with calibrated equations of state
• Hyperonic stars and the symmetry energy
• Semi-analytic derivation of the threshold mass for prompt collapse in binary neutron star mergers
• Hybrid and quark star matter based on a non-perturbative equation of state
• New Gogny interaction suitable for astrophysical applications
• Fast neutrino flavor conversions in one-dimensional core-collapse supernova models with and without muon creation
• Maximum mass of compact stars from gravitational wave events with finite-temperature equations of state
• Plausible presence of new state in neutron stars with masses above $0.98M_{\mathrm{TOV}}$
• The Tarantula Massive Binary Monitoring VI: Characterisation of hidden companions in 51 single-lined O-type binaries, a flat mass-ratio distribution, and black-hole binary candidates
• Chiral symmetry restoration by parity doubling and the structure of neutron stars
• Constraining the Neutron Star Mass--Radius Relation and Dense Matter Equation of State with NICER. III. Model Description and Verification of Parameter Estimation Codes
• Diffuse Supernova Neutrino Background from extensive core-collapse simulations of $8$-$100{\mathrm{M}}_{\odot }$ progenitors
• Towards an Understanding of the Resolution Dependence of Core-Collapse Supernova Simulations
• How tightly is nuclear symmetry energy constrained by unitary Fermi gas?
• Emergence of microphysical bulk viscosity in binary neutron star post-merger dynamics
• Bayesian Inference of the Symmetry Energy and the Neutron Skin in ${}^{48}$Ca and ${}^{208}$Pb from CREX and PREX-2
• Future Physics Perspectives on the Equation of State from Heavy Ion Collisions to Neutron Stars
• Medium effects on pion production in heavy ion collisions
• Stiffening of matter in quark-hadron continuity
• Constraints on the nuclear symmetry energy from asymmetric-matter calculations with chiral NN and 3N interactions
• Constraints on the Symmetry Energy from PREX-II in the Multimessenger Era
• GW170817 implications on the frequency and damping time of f-mode oscillations of neutron stars
• Uncertainty limits on neutron star radius measurements with gravitational waves
• What neutron stars tell about the hadron-quark phase transition: a Bayesian study
• Delineating Effects of Nuclear Symmetry Energy on the Radii and Tidal Polarizabilities of Neutron Stars
• Equation of state of dense matter in the multimessenger era
• Constraints on the skewness coefficient of symmetric nuclear matter within the nonlinear relativistic mean field model
• Cooling of Small and Massive Hyperonic Stars
• Comparing treatments of weak reactions with nuclei in simulations of core-collapse supernovae
• The nuclear symmetry energy and the breaking of the isospin symmetry: how do they reconcile with each other?
• Constraining hadron-quark phase transition parameters within the quark-mean-field model using multimessenger observations of neutron stars
• Microscopic equation of state of hot nuclear matter for numerical relativity simulations
• Status and perspectives of Continuous Gravitational Wave searches
• Hyperons in hot dense matter: what do the constraints tell us for equation of state?
• Imposing multi-physics constraints at different densities on the Neutron Star Equation of State
• Probing the incompressibility of nuclear matter at ultra-high density through the prompt collapse of asymmetric neutron star binaries
• A NICER view of the 1.4 solar-mass edge-on pulsar PSR J0614-3329
• Constraining the relativistic mean-field model equations of state with gravitational wave observations
• Equation-of-state Constraints and the QCD Phase Transition in the Era of Gravitational-Wave Astronomy
• Curvature-slope correlation of nuclear symmetry energy and its imprints on the crust-core transition, radius and tidal deformability of canonical neutron stars
• Spectral classification of gravitational-wave emission and equation of state constraints in binary neutron star mergers
• Equations of state for hot neutron stars -- II. The role of exotic particle degrees of freedom
• Sexaquark dilemma in neutron stars and its solution by quark deconfinement
• Massive $\Delta$-resonance admixed hypernuclear stars with anti-kaon condensations
• Sensitivity of Au+Au collisions to the symmetric nuclear matter equation of state at 2 -- 5 nuclear saturation densities
• Horizons: Nuclear Astrophysics in the 2020s and Beyond
• Multi-physics constraints at different densities to probe nuclear symmetry energy in hyperonic neutron stars
• Hypernuclear stars from relativistic Hartree-Fock density functional theory
• Bayesian model-selection of neutron star equation of state using multi-messenger observations
• On the minimum radius of very massive neutron stars
• Compact body in a tidal environment: New types of relativistic Love numbers, and a post-Newtonian operational definition for tidally induced multipole moments
• Thermal evolution and quiescent emission of transiently accreting neutron stars
• Rapidly rotating $\Delta$-resonance-admixed hypernuclear compact stars
• Nonperturbative quark matter equations of state with vector interactions
• Bayesian inference of nuclear symmetry energy from measured and imagined neutron skin thickness in ${}^{116,118,120,122,124,130,132}$Sn, ${}^{208}$Pb, and ${}^{48}$Ca
• Role of vector self-interaction in Neutron Star properties
• Constraining compact star properties with nuclear saturation parameters
• Heat blanketing envelopes of neutron stars
• Reconstructing the neutron star equation of state from observational data via automatic differentiation
• Magnetic field distribution in magnetars
• Bayesian nonparametric inference of neutron star equation of state via neural network
• Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence
• Dense and Hot QCD at Strong Coupling
• Are nuclear matter properties correlated to neutron star observables ?
• Supernova axions convert to gamma-rays in magnetic fields of progenitor stars
• Frequency deviations in universal relations of isolated neutron stars and postmerger remnants
• On the nature of the mass-gap object in the GW190814 event
• Implications of parity-violating electron scattering experiments on ${}^{48}$Ca (CREX) and ${}^{208}$Pb (PREX-II) for nuclear energy density functionals
• Thermal evolution of relativistic hyperonic compact stars with calibrated equations of state
• Tidal deformations of neutron stars with elastic crusts
• Simultaneous Inference of Neutron Star Equation of State and the Hubble Constant with a Population of Merging Neutron Stars
• Nuclear symmetry energy and hadron-quark mixed phase in neutron stars
• EoS for hot neutron stars
• Cooling timescale for protoneutron stars and properties of nuclear matter: Effective mass and symmetry energy at high densities
• $\Delta$-admixed neutron stars: spinodal instabilities and dUrca processes
• Impact of NICER's Radius Measurement of PSR J0740+6620 on Nuclear Symmetry Energy at Suprasaturation Densities
• Phenomenological quark-hadron equations of state with first-order phase transitions for astrophysical applications
• Broken SU(6) symmetry and massive hybrid stars
• Unified neutron star EOSs and neutron star structures in RMF models
• A Neutron Star is born
• Implicit correlations within phenomenological parametric models of the neutron star equation of state
• Information content of the differences in the charge radii of mirror nuclei
• Constraining the Properties of the Thermonuclear Burst Oscillation Source XTE J1814-338 Through Pulse Profile Modelling
• Universal relations for rapidly rotating cold and hot hybrid star
• From the microscopic to the macroscopic world: from nucleons to neutron stars
• Nucleon effective mass in hot dense matter
• Effects of nuclear symmetry energy and equation of state on neutron star properties
• Translating neutron star observations to nuclear symmetry energy via artificial neural networks
• Short-range correlations effects on the deformability of neutron stars
• QCD constraints on isospin-dense matter and the nuclear equation of state
• Kinetic approach of light-nuclei production in intermediate-energy heavy-ion collisions
• Determination of properties of protoneutron stars toward black hole formation via gravitational wave observations
• Formulating bulk viscosity for neutron star simulations
• Systematic study on the quark-hadron mixed phase in compact stars
• Isovector Effects in Neutron Stars, Radii and the GW170817 Constraint
• Bayesian Inference of the Dense Matter Equation of State built upon Covariant Density Functionals
• Toward a unified equation of state for multi-messenger astronomy
• Neutron stars and the dense matter equation of state: from microscopic theory to macroscopic observations
• Dissipative Magnetohydrodynamics for Non-Resistive Relativistic Plasmas
• Sound velocity in dense stellar matter with strangeness and compact stars
• Measurement of the nuclear symmetry energy parameters from gravitational wave events
• Directed flow of $\Lambda$ in high-energy heavy-ion collisions and $\Lambda$ potential in dense nuclear matter
• Constraints on the curvature of nuclear symmetry energy from recent astronomical data within the KIDS framework
• General relativistic dynamical tides in binary inspirals, without modes
• Nuclear fourth-order symmetry energy and its effects on neutron star properties in the relativistic Hartree-Fock theory
• Constraining the neutron star equation of state using Pulse Profile Modeling
• Hadron-quark mixed phase in the quark-meson coupling model
• Exploring the distribution and impact of bosonic dark matter in neutron stars
• R-modes as a New Probe of Dark Matter in Neutron Stars
• New constraints on the neutron-star mass and radius relation from terrestrial nuclear experiments
• Future Prospects for Constraining Nuclear Matter Parameters with Gravitational Waves
• Constraining the nuclear symmetry energy and properties of neutron star from GW170817 by Bayesian analysis
• Study of the core-crust transition in neutron stars with finite-range interactions: the dynamical method
• Effects of Dark Matter on $f$-mode oscillations of Neutron Stars
• Constraints on high density equation of state from maximum neutron star mass
• Equation of State table with hyperon and antikaon for supernova and neutron star merger
• Empirical constraints on the high-density equation of state from multi-messenger observables
• The baryon coupling scheme in an unified SU(3) and SU(6) symmetry formalism
• The interplay of short-range correlations and nuclear symmetry energy in hard photon productions from heavy-ion reactions at Fermi energies
• A pitfall of piecewise-polytropic equation of state inference
• Ruling out the supersoft high-density symmetry energy from the discovery of PSR J0740+6620 with mass $2.14_{-0.09}^{+0.10}{M}_{\odot }$
• Bulk viscosity in neutron stars with hyperon cores
• The special point on the hybrid star mass--radius diagram and its multi--messenger implications
• Full distribution of clusters with universal couplings and in-medium effects
• Application of artificial intelligence in the determination of impact parameter in heavy-ion collisions at intermediate energies
• Muons in the aftermath of neutron star mergers and their impact on trapped neutrinos
• Effects of $\varphi$-meson on properties of hyperon stars in density dependent relativistic mean field model
• Consistent Skyrme parametrizations constrained by GW170817
• Influence of density dependence of symmetry energy in hot and dense matter for supernova simulations
• Towards the understanding of the genuine three-body interaction for p$-$p$-$p and p$-$p$-\Lambda$
• A New Approach to Mass and Radius of Neutron Stars with Supernova Neutrinos
• Constraining the density dependence of the symmetry energy with nuclear data and astronomical observations in the KIDS framework
• The Emission Order of Hydrogen Isotopes via Correlation Functions in 30 MeV/u Ar+Au Reactions
• Bayesian inference of the incompressibility, skewness and kurtosis of nuclear matter from empirical pressures in relativistic heavy-ion collisions
• Hypermassive quark cores
• Supernova Constraints on Dark Flavored Sectors
• High-momentum components in the ${}^4$He nucleus caused by inter-nucleon correlations
• Model-based cross-correlation search for gravitational waves from the low-mass X-ray binary Scorpius X-1 in LIGO O3 data
• Effect of isovector scalar meson on equation of state of dense matter within relativistic mean field model
• Role of vector channel in different classes of (non) magnetized neutron stars
• Impact of pions on binary neutron star mergers
• EoS constraints from nuclear masses and radii in a meta-modeling approach
• Chiral symmetry restoration and the $\Delta$ matter formation in neutron stars
• Hybrid star models in the light of new multi-messenger data
• Exploring thermal effects of the hadron-quark matter transition in neutron star mergers
• $r$-process nucleosynthesis from compact binary mergers
• R-modes and neutron star recycling scenario
• Thermal Relaxation of Dark Matter Admixed Neutron Star
• Probing high-density nuclear symmetry energy with ${\Xi }^{-}/{\Xi }^0$ ratio in heavy-ion collisions at $\sqrt{s_{NN}}\sim 3$ GeV
• Constraining nuclear parameters using Gravitational waves from f-mode Oscillations in Neutron Stars
• Relativistic hybrid stars with sequential first-order phase transitions in light of multimessenger constraints
• Axions: From Magnetars and Neutron Star Mergers to Beam Dumps and BECs
• Phenomenological QCD equations of state for neutron star dynamics: Nuclear-2SC continuity and evolving effective couplings
• Improved neutrino-nucleon interactions in dense and hot matter for numerical simulations
• Extended Skyrme interactions for transport model simulations of heavy-ion collisions
• GW170817 and the prospect of forming supramassive remnants in neutron star mergers
• Effect of strong magnetic fields on the crust-core transition and inner crust of neutron stars
• Inference of neutron-star properties with unified crust-core equations of state for parameter estimation
• Isospin symmetry breaking in the charge radius difference of mirror nuclei
• Hadron-quark Pasta Phase in Massive Neutron Stars
• Can we decipher the composition of the core of a neutron star?
• Extracting nuclear matter properties from the neutron star matter equation of state using deep neural networks
• Deducing Neutron Star Equation of State Parameters Directly From Telescope Spectra with Uncertainty-Aware Machine Learning
• Impact of updated Multipole Love numbers and f-Love Universal Relations in the context of Binary Neutron Stars
• Thermal behavior as indicator for hyperons in binary neutron star merger remnants
• Dense Matter in Neutron Stars with eXTP
• Reconciling multi-messenger constraints with chiral symmetry restoration
• Inference of the neutron star equation of state from cosmological distances
• Neutron star mass formula with nuclear saturation parameters for asymmetric nuclear matter
• Impact of Symmetry Energy on Sound Speed and Spinodal Decomposition in Dense Neutron-Rich Matter
• Bayesian inference of neutron-star observables based on effective nuclear interactions
• 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
• Structure of Quark Star: A Comparative Analysis of Bayesian Inference and Neural Network Based Modeling
• $R$-mode Stability of GW190814's Secondary Component as a Supermassive and Superfast Pulsar
• Hadron matter in neutron stars in view of gravitational wave observations
• The effect of the energy functional on the pasta-phase properties of catalysed neutron stars
• Constraints on the muon fraction and density profile in neutron stars
• Double strangeness ${\Xi }^{-}$ production as a probe of nuclear equation of state at high densities
• g-mode Oscillations in Neutron Stars with Hyperons
• Determination of the symmetry energy from the neutron star equation of state
• Hyperonic neutron stars: reconciliation between nuclear properties and NICER and LIGO/VIRGO results
• Neutron Star Structure in the Presence of Nonminimally Coupled Scalar Fields
• Asymmetric Nuclear Matter and Neutron Star Properties in Relativistic ab initio Theory in the Full Dirac Space
• 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
• Constraining isovector nuclear interactions with giant resonances within a Bayesian approach
• Progenitor Dependence of Hadron-quark Phase Transition in Failing Core-collapse Supernovae
• Delta baryons in neutron stars
• CREX- and PREX-II-motivated relativistic interactions and their implications for the bulk properties of nuclear matter and neutron stars
• Nuclear matter fourth-order symmetry energy in non-relativistic mean-field models
• Universal relations for compact stars with heavy baryons
• Equation of state and composition of proto-neutron stars and merger remnants with hyperons
• Observing Supernova Neutrino Light Curves with Super-Kamiokande. II. Impact of the Nuclear Equation of State
• Fluctuations and phases in baryonic matter
• 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
• Medium modifications for light and heavy nuclear clusters in simulations of core collapse supernovae -- Impact on equation of state and weak interactions
• Critical parameters of liquid-gas phase transition in thermal symmetric and asymmetric nuclear matter
• Symmetry energy effect on the secondary component of GW190814 as a neutron star
• Searching for New Physics in Ultradense Environment: a Review on Dark Matter Admixed Neutron Stars
• Constraining neutron superfluidity with $r$-mode physics
• GW170817 constraints analyzed with Gogny forces and momentum-dependent interactions
• Neutron star mass-radius constraints using the high-frequency QPOs of GRB 200415A
• Crust-core transition of a neutron star: effects of the symmetry energy and temperature under strong magnetic fields
• Relativistic Mean Field Model parameterizations in the light of GW170817, GW190814, and PSR J0740 + 6620
• XTE J1814-338 as a dark matter admixed neutron star
• Covariant Density Functional Theory with Localized Exchange Terms
• Camouflage of the Phase Transition to Quark Matter in Neutron Stars
• Empirical information on nuclear matter fourth-order symmetry energy from an extended nuclear mass formula
• Nuclear pasta structures and symmetry energy
• Symmetry energy extracted from the S$\pi$RIT pion data in Sn+Sn systems
• Vector-Interaction-Enhanced Bag Model
• Symmetry energy effects on the properties of hybrid stars
• Radial Oscillations in Neutron Stars with Delta Baryons
• Unified nuclear matter EOSs constrained by the in-medium balance in density-dependent covariant density functionals
• Addition of tabulated equation of state and neutrino leakage support to IllinoisGRMHD
• Finite-size effects on the Phase Structure of the Walecka Model
• Superfluid Phase Transitions and Effects of Thermal Pairing Fluctuations in Asymmetric Nuclear Matter
• Electric dipole polarizability in neutron-rich Sn isotopes as a probe of nuclear isovector properties
• Finding quark content of neutron stars in light of GW170817
• Astrophysics and Nuclear Physics Informed Interactions in Dense Matter: Inclusion of PSR J0437-4715
• Nucleus giant resonances from an improved isospin-dependent Boltzmann-Uehling-Uhlenbeck transport approach
• Revisiting the Equation of State of Hybrid Stars in the Dyson-Schwinger Equation Approach to QCD
• Low density nuclear matter with light clusters in a generalized nonlinear relativistic mean-field model
• Glitch Behavior of Pulsars and Contribution from Neutron Star Crust
• Dense matter equation of state for neutron star mergers
• Central Speed of Sound, Trace Anomaly and Observables of Neutron Stars from Perturbative Analyses of Scaled TOV Equations
• Pulse profiles from a pulsar in scalar-tensor gravity
• Indirect methods in nuclear astrophysics with relativistic radioactive beams
• Bayesian Inference of Fine-Features of Nuclear Equation of State from Future Neutron Star Radius Measurements to 0.1km Accuracy
• The Role of Baryon Structure in Neutron Stars
• Neutron star properties with careful parameterization in the (axial)vector meson extended linear sigma model
• Tidal heating as a direct probe of strangeness inside neutron stars
• Setting nonperturbative uncertainties on finite-temperature properties of neutron matter
• Bulk viscosity from Urca processes: $npe\mu$ matter in the neutrino-transparent regime
• Bayesian uncertainty quantification for nuclear matter incompressibility
• 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
• 3D code for MAgneto-Thermal evolution in Isolated Neutron Stars, MATINS: thermal evolution and lightcurves
• Axion emission from strange matter in core-collapse SNe
• Influence of the interactions of scalar mesons on the behavior of the symmetry energy
• X-PSI Parameter Recovery for Temperature Map Configurations Inspired by PSR J0030+0451
• Density-dependent van der Waals model under the GW170817 constraint
• Nuclear collective dynamics in the lattice Hamiltonian Vlasov method
• Probing phase transition in neutron stars via the crust-core interfacial mode
• Constraining isovector nuclear interactions with giant dipole resonance and neutron skin in ${}^{208}$Pb from a Bayesian approach
• Pasta phases within the QMC model
• Hot neutron stars and their equation of state
• Axion effects in the stability of hybrid stars
• Magnetar QPOs and neutron star crust elasticity
• Detectability of a phase transition in neutron star matter with third-generation gravitational wave interferometers
• Quick Guides for Use of the CompOSE Data Base
• Hybrid Equations of State for Neutron Stars with Hyperons and Deltas
• Microscopic nuclear equation of state at finite temperature and stellar stability
• Bayesian model averaging for nuclear symmetry energy from effective proton-neutron chemical potential difference of neutron-rich nuclei
• Thermodynamics from the quark condensate
• Massive neutron star with strangeness in a relativistic mean-field model with a high-density cut-off
• Nuclear matter at finite temperature and static properties of proto-neutron star
• Numerical Study of Stellar Core Collapse and Neutrino Emission Using the Nuclear Equation of State Obtained by the Variational Method
• Feasibility of dark matter admixed neutron star based on recent observational constraints
• Composition of nuclear matter with light clusters and Bose-Einstein condensation of $\alpha$ particles
• Effects of the equation of state on the core-crust interface of slowly rotating neutron stars
• Neutron star equation of state and GW170817
• In medium properties of $K^0$ and $\varphi$ mesons under an external magnetic field
• Repulsive $\Lambda$ potentials in dense neutron star matter and binding energy of $\Lambda$ in hypernuclei
• Masquerading hybrid stars with dark matter
• Nonparametric model for the equations of state of neutron star from deep neural network
• Stability of the protoneutron stars toward black hole formation
• Frequencies of $f$- and $p$-oscillation modes in cold and hot compact stars
• Nuclei in Core-Collapse Supernovae Engine
• Supercritically charged objects and electron-positron pair creation
• Beyond-mean-field effects on the symmetry energy and its slope from the low-lying dipole response of ${}^{68}$Ni
• Studies of the equation-of-state of nuclear matter by heavy-ion collisions at intermediate energy in the multi-messenger era
• Measuring deformed neutron skin with free spectator nucleons in relativistic heavy-ion collisions
• $Abinitio$ thermodynamics of one-component plasma for astrophysics of white dwarfs and neutron stars
• A bag model of matter condensed by the strong interaction
• From NS observations to nuclear matter properties: a machine learning approach
• Constraining dense matter physics using f-mode oscillations in neutron stars
• New covariant density functionals of nuclear matter for compact star simulations
• Bayesian inference of the dense matter equation of state built upon extended Skyrme interactions
• Temperature and Strong Magnetic Field Effects in Dense Matter
• Impacts of symmetry energy slope on the oscillation frequencies of neutron stars with short-range correlation and admixed dark matter
• Constraining nuclear matter parameters from correlation systematics:a mean-field perspective
• Nuclear collective dynamics in transport model with the lattice Hamiltonian method
• Quantifying the uncertainties on spinodal instability in stellar matter through meta-modeling
• Thermodynamics of Hot Neutron Stars and Universal Relations
• Hubble constant and nuclear equation of state from kilonova spectro-photometric light curves
• Rotating hybrid stars with the Dyson-Schwinger quark model
• Studying the parameters of the extended $\sigma$-$\omega$ model for neutron star matter
• 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
• Bayesian constraints on covariant density functional equations of state of compact stars with new NICER mass-radius measurements
• Medium Effects in MIT Bag Model for quark matter: Self consistent thermodynamical treatment
• The Influence of Muons, Pions, and Trapped Neutrinos on Neutron Star Mergers
• Multilayer neutron stars with scalar mesons crossing term
• Quarkyonic matter state of neutron stars
• Gravitational waves from isolated neutron stars: mass dependence of r-mode instability
• Neutron star-black hole coalescence rate inferred from macronova/kilonova observations
• Hyperons in the pasta phase
• Universal relations for compact stars with exotic degrees of freedom
• Probing fermionic asymmetric dark matter cores using global neutron star properties
• Embedding short-range correlations in relativistic density functionals through quasi-deuterons
• Late time supernova neutrino signal and proto-neutron star radius
• Binding two and three $\alpha$ particles in cold neutron matter
• Impact of the nuclear equation of state on the formation of twin stars
• Nuclear skin and the curvature of the symmetry energy
• Massive relativistic compact stars from SU(3) symmetric quark models
• 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
• Correlations among symmetry energy elements in Skyrme models
• Short range correlations in the extended quantum molecular dynamics model
• Critical mass, moment of inertia and universal relations of rapidly rotating neutron stars with exotic matter
• Topology change, emergent symmetries and compact star matter
• Intersections of ultracold atomic polarons and nuclear clusters: How is a chart of nuclides modified in dilute neutron matter?
• 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
• Confronting new NICER mass-radius measurements with phase transition in dense matter and twin compact stars
• New equation of state involving Bose-Einstein condensate of antikaon for supernova and neutron star merger simulations
• Observing the Ping-pong Modality of Isospin Degree of Freedom in Cluster Emission from Heavy Ion Reactions
• Unitary $p$-wave Fermi gas in one dimension
• Gray Two-moment Neutrino Transport: Comprehensive Tests and Improvements for Supernova Simulations
• Precursor of Superfluidity in a Strongly Interacting Fermi Gas with Negative Effective Range
• Properties of nuclear matter in relativistic Brueckner-Hartree-Fock model with high-precision charge-dependent potentials
• Asymmetric Nuclear Light Clusters In Supernova Matter
• Neutron stars formation and Core Collapse Supernovae
• Pulse Profile Modeling of Thermonuclear Burst Oscillations I: The Effect of Neglecting Variability
• Many-body approximations to the superfluid gap and critical temperature in pure neutron matter
• Imprints of the nuclear symmetry energy slope in gravitational wave signals emanating from neutron stars
• Baryonic dense matter in view of gravitational-wave observations
• Warm unstable asymmetric nuclear matter: critical properties and the density dependence of the symmetry energy
• Role of the symmetry energy slope in neutron stars: exploring the model-dependency
• QCD-like phase diagram with Efimov trimers and Cooper pairs in resonantly interacting SU(3) Fermi gases
• Nonparametric Representation of Neutron Star Equation of State Using Variational Autoencoder
• Relativistic correction to the r-mode frequency in light of multi-messenger constraints
• Improved method for the experimental determination of in-medium effects from heavy-ion collisions
• Minimal Length, Nuclear Matter, and Neutron Stars
• Polytropic fits of modern and unified equations of state
• The proto-neutron star inner crust in the liquid phase
• Effects of nuclear matter and composition in core-collapse supernovae and long-term proto-neutron star cooling
• Multi-messenger observations of core-collapse supernovae: Exploiting the standing accretion shock instability
• thornado-hydro: a discontinuous Galerkin method for supernova hydrodynamics with nuclear equations of state
• The $\Xi N$ interaction constrained by recent ${\Xi }^{-}$ hypernuclei experiments
• Finite-temperature effects in dynamical-spacetime binary neutron star merger simulations: Validation of the parametric approach
• Prospects for optical detections from binary neutron star mergers with the next-generation multi-messenger observatories
• Shear oscillations in neutron stars and the nuclear symmetry energy
• Bayesian inference of neutron-skin thickness and neutron-star observables based on effective nuclear interactions
• Extended NJL model for baryonic matter and quark matter
• Light clusters in warm stellar matter: calibrating the cluster couplings
• Nambu-Jona-Lasinio description of hadronic matter from a Bayesian approach
• From finite nuclei to neutron stars : the essential role of high-order density dependence in effective forces
• The neutron star inner crust: an empirical essay
• Actinide-boosting r Process in Black Hole-Neutron Star Merger Ejecta
• Estimation of the slope of nuclear symmetry energy via charge radii of mirror nuclei
• Auxiliary Function Approach for Determining Symmetry Energy at Supra-saturation Densities
• Probing short-range correlations in asymmetric nuclei with quasi-free pair knockout reactions
• Quarkyonic matter and quarkyonic stars in an extended RMF model
• Decoding rotating neutron stars: Role of the symmetry energy slope
• 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
• Bayesian inference of strangeon matter using the measurements of PSR J0437-4715 and GW190814
• Revisiting the post-glitch relaxation of the 2000 Vela glitch with the neutron star equation of states in the Brueckner and relativistic Brueckner theories
• 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
• Properties of quark-matter cores in massive hybrid stars
• Modified Urca neutrino emissivity at finite temperature
• Premerger phenomena in neutron-star binary coalescences
• Effects of retarded electrical fields on observables sensitive to the high-density behavior of nuclear symmetry energy in heavy-ion collisions at intermediate energies
• Gravitational-wave imprints of non-convex dynamics in binary neutron star mergers
• Pulse Profile Modelling of Thermonuclear Burst Oscillations II: Handling variability
• Cost of inferred nuclear parameters towards the f-mode dynamical tide in binary neutron stars
• Kerr-Enhanced Optical Spring
• Hyperonic uncertainties in neutron stars, mergers and supernovae
• Interfacing branching random walks with Metropolis sampling: constraint release in auxiliary-field quantum Monte Carlo
• Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Nucleonic models
• Partially accreted crusts of neutron stars
• Effects of the momentum dependence of nuclear symmetry potential on pion observables in Sn + Sn collisions at 270 MeV/nucleon
• Nuclear pasta and symmetry energy in the relativistic point-coupling model
• Compact Objects in close orbits as Gravitational Wave Sources: Formation Scenarios and Properties
• The proto-neutron star inner crust in a multi-component plasma approach
• Nuclear Symmetry Energy and Neutron Skin Thickness of ${}^{208}Pb$ using a finite range effective interaction
• Neutron Skins: Weak Elastic Scattering and Neutron Stars
• Equation of State of Neutron-Rich Matter in $d$-Dimensions
• Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars
• Anomalous quartic term in the expansion of the symmetry energy
• Influence of the nuclear symmetry energy slope on observables of compact stars with $\Delta$-admixed hypernuclear matter
• Neutron star inner crust: effects of rotation and magnetic fields
• Density of States of a Coupled-Channel System
• 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
• Problematic systematics in neutron-star merger simulations
• Collisional dynamics of polaronic clouds immersed in a Fermi sea
• Phenomenological Equation of State of Strongly Interacting Matter with First-Order Phase Transitions and Critical Points
• 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
• Employing ternary fission of ${}^{242}$Pu as a probe of very neutron rich matter
• Effect of the crust on neutron star empirical relations
• Impact of ground-state properties and collective excitations on the Skyrme ansatz: a Bayesian study
• Sensitivity of nuclear statistical equilibrium to nuclear uncertainties during stellar core collapse
• Relativistic self-energy decomposition of nuclear symmetry energy and equation of state of neutron matter within QCD sum rules
• Nuclear physics with gravitational waves from neutron stars disrupted by black holes
• Investigating the role of nuclear parameters on oscillation modes in hot Neutron Stars
• Accretion-Induced Collapse of Dark Matter Admixed White Dwarfs -- II: Rotation and Gravitational-wave Signals
• Accurate nuclear symmetry energy at finite temperature within a BHF approach
• Properties of ${}^{208}$Pb predicted from the relativistic equation of state in the full Dirac space
• The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy
• Parametrization of the surface energy in the ETF approximation
• Polaronic Proton and Diproton Clustering in Neutron-Rich Matter
• Effects of incompressibility $K_0$ in heavy-ion collisions at intermediate energies
• Phase-transition-induced collapse of proto-compact stars and its implication for supernova explosions
• Sensitivity of the evaporation residue observables to the symmetry energy
• High Density with Elliptic Flows
• Neutron star mass formula with nuclear saturation parameters
• Quiescent luminosities of accreting neutron stars with different equation of states
• Strong magnetic fields: neutron stars with an extended inner crust
• Impact of strong magnetic fields on the inner crust of neutron stars
• Neutron star cooling and mass distributions
• Strong Gravity Extruding Peaks in Speed of Sound Profiles of Massive Neutron Stars
• Nuclear pasta in hot and dense matter and its influence on the equation of state for astrophysical simulations
• Universal relations to measure neutron star properties from targeted r-mode searches
• Measuring spin in coalescing binaries of neutron stars showing double precursors
• 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
• Hyperonization in compact stars
• Equilibrium nuclear ensembles taking into account vaporization of hot nuclei in dense stellar matter
• Study of ($p,n$)IAS and (${}^3$He,$t$)IAS charge-exchange reactions with the $G$-matrix folding method
• Hyperons during proto-neutron star deleptonization and the emission of dark flavoured particles
• What can be learned from a proto-neutron star's mass and radius?
• Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities
• The outer crust of a cold, non-accreting neutron star within the Quark-Meson Coupling (QMC) model
• The nuclear symmetry energy from relativistic Brueckner-Hartree-Fock 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
• Equation of state in neutron stars and supernovae
• Intrinsic Correlations Among Characteristics of Neutron-rich Matter Imposed by the Unbound Nature of Pure Neutron Matter
• Evidence for strong isovector nuclear spin-orbit interaction
• Neutron star deformability with hyperonization in density-dependent relativistic mean-field models
• Quark condensate and chiral symmetry restoration in neutron stars
• Correlation between the symmetry energy slope and the deconfinement phase transition
• Revisiting the isospin relaxation time in intermediate-energy heavy-ion collisions
• 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
• Towards a unified hadron-quark equation of state for neutron stars within the relativistic mean-field model
• Hybrid stars within the framework of the Sigma-Omega-Rho model combined with the MIT and NJL models
• RMF models with $\sigma$-scaled hadron masses and couplings for description of heavy-ion collisions below 2A GeV
• Symmetry energy of super-dense neutron-rich matter from integrating barotropic pressures in neutron stars and heavy-ion reactions
• Unraveling Trace Anomaly of Supradense Matter via Neutron Star Compactness Scaling
• Critical properties of calibrated relativistic mean-field models for the transition to warm, non-homogeneous nuclear matter
• Composition of scalar mesons and their effects on nuclear matter properties in an extended linear sigma model
• Treating divergence in quark matter by using energy projectors
• Isotopic equilibrium constants for very low-density and low-temperature nuclear matter
• Virialized equation of state for warm and dense stellar plasmas in proto-neutron stars and Supernova matter
• Nuclear matter from the ladder resummation in terms of the experimental nucleon-nucleon scattering amplitudes
• Light clusters in the liquid proto-neutron star inner crust
• Neutron star crustal properties from relativistic mean-field models and bulk parameters effects
• Rotating Neutron Stars with the Relativistic Ab Initio Calculations
• Bayesian analysis of a relativistic hadronic model constrained by recent astrophysical observations
• The nuclear symmetry energy and the neutron skin thickness in nuclei
• Impact of Hot Inner Crust on Compact Stars at Finite Temperature
• Neutron Stars: Laboratories for fundamental physics under extreme astrophysical conditions
• Bayesian inference of neutron star crust properties using an ab initio-benchmarked meta-model
• Role of local anisotropy in hybrid stars
• Phase transitions and latent heat in magnetized matter
• Cooling of Isolated Neutron Stars with Pion Condensation: Possible Fast Cooling in a Low-Symmetry-Energy Model
• Nucleon momentum gap in asymmetric nuclear matter
• Neutron star cooling within the equation of state with induced surface tension
• Cooling of the Cassiopeia A neutron star and the effect of diffusive nuclear burning
• An Undergraduate Approach to the Quantum Hadrodynamics and the Physics of Neutron Stars
• Non-Radial Oscillation Modes in Hybrid Stars with Hyperons and Delta Baryons
• From masses and radii of neutron stars to EOS of nuclear matter through neural network
• Finite-temperature infinite matter with effective-field-theory-inspired energy-density functionals
• Equation of state and neutrino transfer in supernovae and neutron stars
• Investigating the role of nuclear parameters in Neutron Star oscillations: a model comparison
• Neutron-star seismology with realistic, finite-temperature nuclear matter
• Implementing advanced trial wave functions in fermion quantum Monte Carlo via stochastic sampling
• Explosive Nucleosynthesis: What we learned and what we still do not understand
• Experimental nuclear astrophysics in Italy
• Effects of inner crusts on $g$-mode oscillations in neutron stars
• Investigating the Impact of Higher-Order Phase Transitions in Binary Neutron-Star Mergers
• Density dependence of symmetry energy and neutron skin thickness revisited using relativistic mean field models with nonlinear couplings
• Direct nonparametric multimessenger constraints on the equation of state of cold dense nuclear matter
• Suitable resolution for EOS tables in neutron star investigation
• Quark deconfinement in compact stars through sexaquark condensation
• Simple fits for the neutrino luminosities from protoneutron star cooling
• Reexamination of ${}^6$Li scattering as a Probe to Investigate the Isoscalar Giant Resonances in Nuclei
• Nuclear physics inputs for dense-matter modelling in neutron stars. The nuclear equation of state
• Perturbed nuclear matter studied within Density Functional Theory with a finite number of particles
• How do mirror charge radii constrain density dependence of the symmetry energy?
• Neutron-proton differential transverse flow in ${}^{132}$Sn + ${}^{124}$Sn collisions at 270 MeV/nucleon
• Strange matter in compact stars
• Construction of energy density functional for arbitrary spin polarization using functional renormalization group
• Dependence of postmerger properties on the thermal heating efficiency in neutron star mergers
• Revisit to the yield ratio of triton and ${}^3$He as an indicator of neutron-rich neck emission
• Bayesian Inference of Hybrid Star Properties from Future High-Precision Measurements of Their Radii
• Equation of State of Hot Neutron Star Matter using Finite Range Simple Effective Interaction
• Nucleon Short-Range Correlations and High-Momentum Dynamics: Implications on the Equation of State of Dense Matter
• Exploring nuclear force with pulsar glitch observation
• Strongly interacting matter in extreme magnetic fields
• Strong toroidal magnetic fields sustained by the elastic crust in a neutron star
• Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches
• Gravitation with modified fluid Lagrangian: Variational principle and an early dark energy model
• New Insights into Supradense Matter from Dissecting Scaled Stellar Structure Equations
• I-C-Q relations for rapidly rotating stable hybrid stars
• Effects of phase transition in hybrid stars from quark-meson coupling hadronic matter to deconfined quark matter
• Pairing effects on neutron matter equation of state and symmetry energy at subsaturation densities
• Probing Strange Dark Matter through $f$-mode Oscillations of Neutron Stars with Hyperons and Quark Matter
• Resonance-to-bound transition of ${}^5$He in neutron matter and its analogy with heteronuclear Feshbach molecule
• Comparing strange and non-strange quark stars within resummed QCD at NLO
• Study of nuclear matter properties for Hybrid EoS
• Tidal deformability of neutron stars with exotic particles within a density dependent relativistic mean field model in R-squared gravity
• Neutron Star Radii from Laboratory Experiments
• One- and two-argument equation of state parametrizations with continuous sound speed for neutron star simulations
• Modification of hyperon masses in nuclear matter
• Excitation of the isoscalar giant monopole resonance using 6Li inelastic scattering
• Probing Fundamental Physics with Gravitational Waves
• Dense Hadronic Matter in Neutron Stars
• Simulating Binary Neutron Star Mergers with Finite-temperature Equations of State: The influences of the slope of the symmetry energy and artificial heating
• Simulating bulk viscosity in neutron stars. I. Formalism
• Fast neutron star cooling in light of the PREX-2 experiment
• The Impact of $f(\mathcal{G},T)$ Gravity on the Evolution of Cavity in the Cluster of Stars
• Fermi-Dirac Integrals in Degenerate Regimes: A Novel Asymptotic Expansion
• Strong correlation of the neutron star core-crust transition density with the $\sigma$-meson mass via vacuum polarization
• $f$-mode oscillations in hot Neutron Stars: Effect of hyperons and neutrino trapping
• Framework for phase transitions between the Maxwell and Gibbs constructions at finite temperature
• Stiffening of matter in quark-hadron continuity: a mini-review
• Nuclear incompressibility from spherical and deformed nuclei
• High-order isospin-dependent surface tension contribution to the fourth-order symmetry energy of finite nuclei
• Fluctuations of work in realistic equilibrium states of quantum systems with conserved quantities
• Impact of the relativistic Cowling approximation on shear and interface modes of neutron stars
• Constraining the Hadron-Quark Phase Transition Chemical Potential via Astronomical Observation
• Quartet correlations near the surface of $N=Z$ nuclei
• Novel features of asymmetric nuclear matter from terrestrial experiments and astrophysical observations of neutron stars
• Nuclear mass table in density functional approach inspired by neutron-star observations
• The Yukawa potential under weak magnetic field
• Finite-temperature equation of state with hyperons
• Kaon production in the HADES experiment in Au+Au collisions at $\sqrt{s_{\mathrm{NN}}}=2.4$ GeV
• New {\em ab initio} constrained extended Skyrme equations of state for simulations of neutron stars, supernovae and binary mergers: I. Subsaturation density domain
• Inner crust equations of state for CompOSE
• Neutron stars from crust to core within the Quark-meson coupling model
• Properties of fermionic systems with the Path-integral ground state method
• Tension between implications from PREX-2 data and gravitational tidal response on dense matter equation of state
• Properties and microscopic structures of dense stellar matter in RMF models
• Modification of the universal relation between mass, radius and nonradial $f$-mode oscillation in proto-neutron stars
• Thermal Evolution of Neutron Stars as a Probe of Physics beyond the Standard Model
• Effect of symmetry energy on properties of rapidly rotating neutron stars and universal relations
• Recent progress on superstrange dynamics
• Rotating Neutron Stars with Dark Matter Halos
• Joint Inference of Population, Cosmology, and Neutron Star Equation of State from Gravitational Waves of Dark Binary Neutron Stars
• The origin of the elements and other implications of gravitational wave detection for nuclear physics
• Experimental investigation of ground-state properties of ${}^7$H with transfer reactions
• Anisotropic pressure effect on central EOS of PSR J0740+6620 in the light of dimensionless TOV equation
• Neutron stars with Bogoliubov quark-meson coupling model
• Polaronic neutron in dilute alpha matter: A $p$-wave Bose polaron
• Imprints of high-density nuclear symmetry energy on the crustal fraction of neutron star moment of inertia
• Dipole Polarizability of Finite Nuclei as a Probe of Neutron Stars
• Neutron star properties: Constraining the nuclear matter EoS
• Dineutron decay into sterile anti-neutrinos in neutron stars and its observable consequences
• STROBE-X: A probe-class mission for X-ray spectroscopy and timing on timescales from microseconds to years
• Cosmology from Strong Interactions
• 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
• Effects of the symmetry energy slope on magnetized neutron stars
• Investigating the possibility of extracting neutron-skin thickness in nuclei by their collisions at intermediate energies
• Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars?
• Neutron stars as extreme gravity probes
• Gauge invariance of quantum electrodynamics of multi-electron atoms
• Alpha clustering in warm and dense nuclear matter from heavy-ion collisions
• Equation of state for hot hyperonic neutron star matter
• Rotating neutron stars with chaotic magnetic fields in general relativity and Rastall gravity
• Machine learning-driven conservative-to-primitive conversion in hybrid piecewise polytropic and tabulated equations of state
• Phase-space excluded-volume approach for light clusters in nuclear medium
• Series solutions to the TOV equations
• Role of thermal fluctuations in nucleation of three-flavor quark matter
• Heavy Neutron Star Phenomenology with an H-dibaryon
• Landau parameters and entrainment matrix of cold stellar matter: effect of the symmetry energy and strong magnetic fields
• Phase transitions and finite-size effects in integrable virial statistical models
• Finding signatures of the nuclear symmetry energy in heavy-ion collisions with deep learning
• Correlated structure of nuclear symmetry energy from covariant nucleon self-energy
• Fermions with long and finite range interactions on a quantum ring
• Impact of hyperons on structural properties of neutron stars and hybrid stars within the regularized four-dimensional Einstein-Gauss-Bonnet gravity
• Estimation of neutron star mass and radius of FRB 20240114A by identification of crustal oscillations
• The thermal index of neutron-star matter in the virial approximation
• Symmetry breaking and restoration on a fermionic quantum ring
• Basic quantities of the Equation of State in isospin asymmetric nuclear matter
• The nuclear matter density functional under the nucleonic hypothesis
• Updated estimates of post-merger gravitational wave energy released in GW170817 and the maximum neutron star mass
• Application and Optimization of the GET Electronics System for Double-Sided Silicon Strip Detector Readout
• Tidal Deformability of Quark Stars with Repulsive Interactions
• Effects of three-baryon forces on kaon condensation in hyperon-mixed matter
• Neutron drop trapped in axially deformed external fields
• Probing neutron stars with the full pre-merger and post-merger gravitational wave signal from binary coalescences
• Triaxial instabilities in rapidly rotating Neutron Stars
• 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
• Fully general relativistic description of rapidly-rotating axially-symmetric neutron stars for constraining nuclear matter equations of state
• Recurring region for neutron-star observables
• Formation of large chunk of nuclear matter in heavy-ion collisions
• Collective effects in an incompressible electronic liquid
• Heavy baryons in hot stellar matter with light nuclei and hypernuclei
• Equation-of-State Independent Relations in Rapidly Rotating Hybrid Stars
• Investigating Universal Relations in Compact Stars featuring $\Delta -$Admixed Exotic Dense Matter
• Binding energy of compact stars and their non-radial oscillations
• The Strange Physics of Dark Baryons
• Supernova Constraints on Dark Flavored Sectors
• Properties of rapidly rotating hot neutron stars within Brueckner theory
• Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Influences of parametrizations of density dependent couplings
• Thermal liquid-gas phase transition in a quasi-one-dimensional dipolar Fermi gas
• Unified Equation of State for Neutron Stars Based on the Gogny Interaction
• Neutron Star Equation of State with Nucleon Short-Range Correlations: A Concise Review and Open Issues
• Observation of $\bar{\Lambda }p\to K^{+}{\pi }^{+}{\pi }^{-}{\pi }^0$ and $\bar{\Lambda }p\to K^{+}{\pi }^{+}{\pi }^{-}2{\pi }^0$
• Impact of crust-core connection procedures on the tidal deformability of neutron stars
• Nuclear Matter and Finite Nuclei: Relativistic Thomas-Fermi Approximation Versus Relativistic Mean-Field Approach
• Symmetry energy of baryon- and neutron-rich nuclear matter
• Slowly rotating condensate dark stars beyond the mean-field approximation
• An Undergraduate Approach to the Quantum Hadrodynamics and the Physics of Neutron Stars Part II: Neutron Stars' Exotic Content
• Medium effects on light clusters from heavy-ion collisions within a relativistic mean-field description
• Neutron skins probed in proton knockout from neutron-rich nuclei
• Radial oscillations of quark stars in light of current astrophysical constraints: A comparative study
• The effect of charm quark on the QCD chiral phase diagram
• Angular momentum conservation and pion production in intermediate-energy heavy-ion collisions
• Recent applications of the subtracted second RPA method
• Stability of Neutron Star and Cosmological Constant
• P-stars in the gravitational wave era