The equation of state for nucleon matter and neutron star structure

Abstract

Properties of dense nucleon matter and the structure of neutron stars are studied using variational chain summation methods and the new Argonne v18 two-nucleon interaction. The neutron star gravitational mass limit obtained with this interaction is 1.67 M_{solar}. Boost corrections to the two-nucleon interaction, which give the leading relativistic effect of order (v/c)^2, as well as three-nucleon interactions, are also included in the nuclear Hamiltonian. Their successive addition increases the mass limit to 1.80 and 2.20 M_{solar}. Hamiltonians including a three-nucleon interaction predict a transition in neutron star matter to a phase with neutral pion condensation at a baryon number density of 0.2 fm^{-3}. We also investigate the possibility of dense nucleon matter having an admixture of quark matter, described using the bag model equation of state. Neutron stars of 1.4 M_{solar} do not appear to have quark matter admixtures in their cores. However, the heaviest stars are predicted to have cores consisting of a quark and nucleon matter mixture. These admixtures reduce the maximum mass of neutron stars from 2.20 to 2.02 (1.91) M_{solar} for bag constant B = 200 (122) MeV/fm^3. Stars with pure quark matter in their cores are found to be unstable. We also consider the possibility that matter is maximally incompressible above an assumed density, and show that realistic models of nuclear forces limit the maximum mass of neutron stars to be below 2.5 M_{solar}. The effects of the phase transitions on the composition of neutron star matter and its adiabatic index are discussed.

39 pages RevTeX including 12 tables. 21 postscript figures. Submitted to Phys. Rev. C

References in corpus (16)

• An accurate nucleon-nucleon potential with charge-independence breaking
• Construction of high-quality Nucleon-Nucleon potential models
• Quantum Monte Carlo calculations of nuclei with A \leq 7
• Quantum Monte Carlo Calculations of $A\le 6$ Nuclei
• The Maximum Mass of a Neutron Star
• Spin-Isospin Structure and Pion Condensation in Nucleon Matter
• From Kaon-Nuclear Interactions to Kaon Condensation
• The masses of the millisecond pulsar J1012+5307 and its white-dwarf companion
• Triton calculations with the new Nijmegen potentials
• Neutron Star Masses and Radii as Inferred from kilo-Hertz QPOs
• Kaon Energies in Dense Matter
• Modern nucleon-nucleon potentials and symmetry energy in infinite matter
• Strong-field general relativity and quasi-periodic oscillations in x-ray binaries
• Variational Monte Carlo Calculations of ${}^3$H and ${}^4$He with a relativistic Hamiltonian - II
• Variational calculations of the $\Lambda$-seperation energy of the ${}_{\Lambda }^{17}$O hypernucleus
• The three-baryon $\Lambda NN$ potential

Cited by in corpus (1596)

• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
• GW170817: Measurements of Neutron Star Radii and Equation of State
• Modern Theory of Nuclear Forces
• PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
• Testing General Relativity with Present and Future Astrophysical Observations
• Determination of the Equation of State of Dense Matter
• Color superconductivity in dense quark matter
• Neutron Star Observations: Prognosis for Equation of State Constraints
• Masses, Radii, and Equation of State of Neutron Stars
• Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions
• A unified equation of state of dense matter and neutron star structure
• Properties of the binary neutron star merger GW170817
• A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy
• Equations of state for supernovae and compact stars
• Relativistic Continuum Hartree Bogoliubov Theory for Ground State Properties of Exotic Nuclei
• Tidal deformability of neutron stars with realistic equations of state and their gravitational wave signatures in binary inspiral
• Isospin Asymmetry in Nuclei and Neutron Stars
• The Equation of State from Observed Masses and Radii of Neutron Stars
• Strange Quark Matter and Compact Stars
• Constraints on a phenomenologically parameterized neutron-star equation of state
• Quantum Monte Carlo methods for nuclear physics
• From hadrons to quarks in neutron stars: a review
• Hybrid stars that masquerade as neutron stars
• Reaction Dynamics with Exotic Beams
• Evidence for quark-matter cores in massive neutron stars
• New parametrization for the nuclear covariant energy density functional with point-coupling interaction
• Skyrme Interaction and Nuclear Matter Constraints
• Millisecond Oscillations in X-Ray Binaries
• Relativistic Nuclear Energy Density Functionals: Mean-Field and Beyond
• Improved nuclear matter calculations from chiral low-momentum interactions
• The Einstein Toolkit: A Community Computational Infrastructure for Relativistic Astrophysics
• Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XII: Stiffness and stability of neutron-star matter
• Minimal Cooling of Neutron Stars: A New Paradigm
• Realistic models of pion-exchange three-nucleon interactions
• Binary neutron-star mergers: a review of Einstein's richest laboratory
• The mass ejection from the merger of binary neutron stars
• Relativistic Nuclear Energy Density Functionals: adjusting parameters to binding energies
• I-Love-Q Relations in Neutron Stars and their Applications to Astrophysics, Gravitational Waves and Fundamental Physics
• Cold Quark Matter
• I-Love-Q
• Skyrme-Hartree-Fock-Bogoliubov nuclear mass formulas: Crossing the 0.6 MeV threshold with microscopically deduced pairing
• Gravitational Wave Tests of General Relativity with Ground-Based Detectors and Pulsar Timing Arrays
• Neutron Radii in Mean-Field Models
• Modeling GW170817 based on numerical relativity and its implications
• Pairing in nuclear systems: from neutron stars to finite nuclei
• Rapid Cooling of the Neutron Star in Cassiopeia A Triggered by Neutron Superfluidity in Dense Matter
• Sonic-Point Model of Kilohertz Quasi-Periodic Brightness Oscillations in Low-Mass X-ray Binaries
• Measurability of the tidal polarizability of neutron stars in late-inspiral gravitational-wave signals
• The Skyrme Interaction in finite nuclei and nuclear matter
• The maximum mass and radius of neutron stars and the nuclear symmetry energy
• Measuring the neutron star equation of state using X-ray timing
• New effective interactions in RMF theory with non-linear terms and density-dependent meson-nucleon coupling
• Chiral three-nucleon forces and neutron matter
• Neutron matter at next-to-next-to-next-to-leading order in chiral effective field theory
• The Dense Matter Equation of State from Neutron Star Radius and Mass Measurements
• Astrophysical Measurement of the Equation of State of Neutron Star Matter
• Identifying a first-order phase transition in neutron star mergers through gravitational waves
• Generic conditions for stable hybrid stars
• Constraints on the high-density nuclear equation of state from the phenomenology of compact stars and heavy-ion collisions
• Cooling neutron star in the Cassiopeia~A supernova remnant: Evidence for superfluidity in the core
• Merger of binary neutron stars to a black hole: Disk mass, short gamma-ray bursts, and quasinormal mode ringing
• Measuring neutron-star properties via gravitational waves from binary mergers
• Relativistic Fluid Dynamics: Physics for Many Different Scales
• Approximate Universal Relations for Neutron Stars and Quark Stars
• On the Maximum Mass of Differentially Rotating Neutron Stars
• Circumstantial evidence for a soft nuclear symmetry energy at supra-saturation densities
• Quarkyonic Matter and Neutron Stars
• Kaon production in heavy ion reactions at intermediate energies
• Constraining the Equation of State of Neutron Stars from Binary Mergers
• Maximum mass, moment of inertia and compactness of relativistic stars
• Effects of Strong Magnetic Fields on Neutron Star Structure
• The tensor part of the Skyrme energy density functional. I. Spherical nuclei
• The Progenitors of Short Gamma-Ray Bursts
• Remnant massive neutron stars of binary neutron star mergers: Evolution process and gravitational waveform
• Models of Pulsar Glitches
• Binary Neutron Star Mergers: Dependence on the Nuclear Equation of State
• Analytical representations of unified equations of state for neutron-star matter
• A Hydrogen Atmosphere Spectral Model Applied to the Neutron Star X7 in the Globular Cluster 47 Tucanae
• Symmetry Energy II: Isobaric Analog States
• Born-Infeld inspired modifications of gravity
• Symmetry Parameter Constraints From A Lower Bound On The Neutron-Matter Energy
• Probing the High Density Behaviour of Nuclear Symmetry Energy with High Energy Heavy-Ion Collisions
• Binary Neutron Star Mergers
• Neutron Stars as Dark Matter Probes
• Neutron stars - cooling and transport
• The Nuclear Symmetry Energy
• Spectral properties of the post-merger gravitational-wave signal from binary neutron stars
• A NICER view of PSR J0030+0451: Implications for the dense matter equation of state
• Neutron Stars and the Nuclear Equation of State
• Quark Matter In Massive Compact Stars
• Pulsar glitches: The crust is not enough
• Connecting Neutron Star Observations to Three-Body Forces in Neutron Matter and to the Nuclear Symmetry Energy
• Relativistic neutron star merger simulations with non-zero temperature equations of state I. Variation of binary parameters and equation of state
• Equation-of-state dependence of the gravitational-wave signal from the ring-down phase of neutron-star mergers
• The Millisecond Magnetar Central Engine in short GRBs
• Surface Symmetry Energy
• Measuring a cosmological distance-redshift relationship using only gravitational wave observations of binary neutron star coalescences
• Quark phases in neutron stars and a "third family" of compact stars as a signature for phase transitions
• Constraining neutron star matter with QCD
• Stellar structure models in modified theories of gravity: lessons and challenges
• A new quark-hadron hybrid equation of state for astrophysics - I. High-mass twin compact stars
• Implications from GW170817 and I-Love-Q relations for relativistic hybrid stars
• Gravitational waves from instabilities in relativistic stars
• Evidence for a maximum mass cut-off in the neutron star mass distribution and constraints on the equation of state
• Nucleon and hadron structure changes in the nuclear medium and impact on observables
• Interacting quark matter equation of state for compact stars
• On the importance of viscous dissipation and heat conduction in binary neutron-star mergers
• Density dependence of the symmetry energy and the nuclear equation of state: A Dynamical and Statistical model perspective
• Gravitational waves from neutron star mergers and their relation to the nuclear equation of state
• Cluster Formation and The Virial Equation of State of Low-Density Nuclear Matter
• Gravitational Wave asteroseismology revisited
• Mapping crustal heating with the cooling lightcurves of quasi-persistent transients
• Testing the black hole "no-hair" hypothesis
• Neutron matter from chiral effective field theory interactions
• Bayesian analysis of neutrinos observed from supernova SN 1987A
• Inclusive quasi-elastic electron-nucleus scattering
• Effects of Strong and Electromagnetic Correlations on Neutrino Interactions in Dense Matter
• Core-crust transition in neutron stars: predictivity of density developments
• Estimating the Contribution of Dynamical Ejecta in the Kilonova Associated with GW170817
• The outer crust of non-accreting cold neutron stars
• Nuclear forces and their impact on neutron-rich nuclei and neutron-rich matter
• Neutron conduction in the inner crust of a neutron star in the framework of the band theory of solids
• Neutron Star Asteroseismology. Axial Crust Oscillations in the Cowling Approximation
• Dense Matter in Compact Stars: Theoretical Developments and Observational Constraints
• Strongly paired fermions: Cold atoms and neutron matter
• Low-density neutron matter
• Hyperons in neutron-star cores and two-solar-mass pulsar
• Compact stars with color superconducting quark matter
• Simulating coalescing compact binaries by a new code SACRA
• Gravitational-wave signal from binary neutron stars: a systematic analysis of the spectral properties
• Observational constraints on hyperons in neutron stars
• Higher-order effects on the incompressibility of isospin asymmetric nuclear matter
• Neutrino Emission from Cooper Pairs and Minimal Cooling of Neutron Stars
• Heating in the Accreted Neutron Star Ocean: Implications for Superburst Ignition
• Density dependence of the nuclear symmetry energy: a microscopic perspective
• Is nuclear matter perturbative with low-momentum interactions?
• Constraints on Einstein-Æther theory and Horava gravity from binary pulsar observations
• Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy
• Medium modification of the charged current neutrino opacity and its implications
• Nucleon Effective Masses in Neutron-Rich Matter
• Gravitational wave asteroseismology of fast rotating neutron stars with realistic equations of state
• Renormalization group approach to neutron matter: quasiparticle interactions, superfluid gaps and the equation of state
• Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XI: Stabilizing neutron stars against a ferromagnetic collapse
• Nuclear equation of state for core-collapse supernova simulations with realistic nuclear forces
• Moments of inertia for neutron and strange stars: limits derived for the Crab pulsar
• Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. II: Role of the effective mass
• High-resolution magnetohydrodynamics simulation of black hole-neutron star merger: Mass ejection and short gamma-ray burst
• Dark Matter Effects On Neutron Star Properties
• The realistic models of relativistic stars in f(R) = R + alpha R^2 gravity
• General relativistic magnetohydrodynamic simulations of binary neutron star mergers forming a long-lived neutron star
• Isovector splitting of nucleon effective masses, ab-initio benchmarks and extended stability criteria for Skyrme energy functionals
• Dynamical mass ejection from black hole-neutron star binaries
• Relativistic Lines and Reflection from the Inner Accretion Disks Around Neutron Stars
• Equilibrium models of relativistic stars with a toroidal magnetic field
• Interplay of Three-Body Interactions in the EOS of Nuclear Matter
• New Neutron Star Equation of State with Quark-Hadron Crossover
• Quantum Monte Carlo calculation of the equation of state of neutron matter
• Quantum Monte Carlo Calculations of Neutron Matter
• Quasi-Normal Modes and Gravitational Wave Astronomy
• Symmetry energy impact in simulations of core-collapse supernovae
• Hyperon-hyperon interactions and properties of neutron matter
• Chiral Dynamics and Nuclear Matter
• Evolution of magnetized, differentially rotating neutron stars: Simulations in full general relativity
• Dark-Matter Admixed Neutron Stars
• Chiral Effective Field Theory and the High-Density Nuclear Equation of State
• Compact stars in alternative theories of gravity. Einstein-Dilaton-Gauss-Bonnet gravity
• Can very compact and very massive neutron stars both exist?
• Modern compact star observations and the quark matter equation of state
• Relativistic iron emission lines in neutron star low-mass X-ray binaries as probes of neutron star radii
• Differential Rotation in Neutron Stars: Magnetic Braking and Viscous Damping
• Observing Gravitational Waves From The Post-Merger Phase Of Binary Neutron Star Coalescence
• Rotational properties of hypermassive neutron stars from binary mergers
• Using Neutron Star Observations to Determine Crust Thicknesses, Moments of Inertia, and Tidal Deformabilities
• Constraining the Neutron Star Mass-Radius Relation and Dense Matter Equation of State with NICER. II. Emission from Hot Spots on a Rapidly Rotating Neutron Star
• Recent Progress in Neutron Star Theory
• Two-Body Correlations in Nuclear Systems
• The Galactic Population of Low- and Intermediate-Mass X-ray Binaries
• Phenomenological QCD equation of state for massive neutron stars
• The Massive Pulsar PSR J1614-2230: Linking Quantum Chromodynamics, Gamma-ray Bursts, and Gravitational Wave Astronomy
• Constraints on binary neutron star merger product from short GRB observations
• Cold uniform matter and neutron stars in the quark-mesons-coupling model
• Neutron Stars in Rastall Gravity
• Longterm general relativistic simulation of binary neutron stars collapsing to a black hole
• Pulsars as Astrophysical Laboratories for Nuclear and Particle Physics
• From Brueckner Approach to Skyrme-type Energy Density Functional
• Slowly rotating neutron and strange stars in $R^2$ gravity
• General relativistic simulations of compact binary mergers as engines of short gamma-ray bursts
• Numerical relativity simulations of binary neutron stars
• Multi-resonance orbital model of high-frequency quasi-periodic oscillations: possible high-precision determination of black hole and neutron star spin
• Non-perturbative and self-consistent models of neutron stars in R-squared gravity
• Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations I: Black Hole-Neutron Star Mergers
• Strong Binary Pulsar Constraints on Lorentz Violation in Gravity
• Dark halos around neutron stars and gravitational waves
• Torsional Oscillations of Relativistic Stars with Dipole Magnetic Fields
• Nuclear Equation of State from Observations of Short Gamma-Ray Burst Remnants
• On the appearance of hyperons in neutron stars
• Hadron-Quark Crossover and Massive Hybrid Stars
• The Oblate Schwarzschild Approximation for Light Curves of Rapidly Rotating Neutron Stars
• On the nuclear symmetry energy and the neutron skin in neutron-rich nuclei
• Neutron-star Radius from a Population of Binary Neutron Star Mergers
• Neutron Matter from Low to High Density
• Trace anomaly as signature of conformality in neutron stars
• Model comparison from LIGO-Virgo data on GW170817's binary components and consequences for the merger remnant
• Constraints on interquark interaction parameters with GW170817 in a binary strange star scenario
• Magnetar heating
• Neutron star cooling after deep crustal heating in the X-ray transient KS 1731-260
• Structure of cold nuclear matter at subnuclear densities by Quantum Molecular Dynamics
• Inferring physical parameters of compact stars from their f-mode gravitational wave signals
• Structure and deformations of strongly magnetized neutron stars with twisted torus configurations
• Gravitational Microlensing Events Due to Stellar Mass Black Holes
• How Gravitational-wave Observations Can Shape the Gamma-ray Burst Paradigm
• First 100 ms of a long-lived magnetized neutron star formed in a binary neutron star merger
• Three-Nucleon Forces: Implementation and Applications to Atomic Nuclei and Dense Matter
• Forecasting the detection capabilities of third-generation gravitational-wave detectors using $\text{GWFAST}$
• Slowly rotating neutron stars in the nonminimal derivative coupling sector of Horndeski gravity
• The equation of state of neutron matter, symmetry energy, and neutron star structure
• Effective No-Hair Relations for Neutron Stars and Quark Stars: Relativistic Results
• Modelization of the EOS
• Toward ab initio density functional theory for nuclei
• Equation of state constraints from the threshold binary mass for prompt collapse of neutron star mergers
• Gravitational waves from relativistic neutron star mergers with nonzero-temperature equations of state
• Coalescing neutron stars - a step towards physical models III. Improved numerics and different neutron star masses and spins
• Challenging the Presence of Scalar Charge and Dipolar Radiation in Binary Pulsars
• An abrupt drop in the coherence of the lower kilohertz QPO in 4U 1636-536
• Magneto-elastic oscillations of neutron stars with dipolar magnetic fields
• Effectively universal behavior of rotating neutron stars in general relativity makes them even simpler than their Newtonian counterparts
• Merger of black hole-neutron star binaries in full general relativity
• Merger of black hole and neutron star in general relativity: Tidal disruption, torus mass, and gravitational waves
• High Density Behaviour of Nuclear Symmetry Energy and High Energy Heavy-Ion Collisions
• On neutron stars in f(R) theories: small radii, large masses and large energy emitted in a merger
• Keplerian frequency of uniformly rotating neutron stars and quark stars
• Prospects of Detecting Baryon and Quark Superfluidity from Cooling Neutron Stars
• Measurability of the tidal deformability by gravitational waves from coalescing binary neutron stars
• On the History of Dibaryons and their Final Observation
• Relativistic models of magnetars: the twisted-torus magnetic field configuration
• Will black hole-neutron star binary inspirals tell us about the neutron star equation of state?
• Neutron stars exclude light dark baryons
• Constraints on Neutron Star Crusts From Oscillations in Giant Flares
• I-Q relation for rapidly rotating neutron stars
• Surface Emission from Neutron Stars and Implications for the Physics of their Interiors
• Neutron-proton asymmetry dependence of spectroscopic factors in Ar isotopes
• Third family of compact stars within a nonlocal chiral quark model equation of state
• Gravitational waves from black hole-neutron star binaries I: Classification of waveforms
• Spin susceptibility of neutron matter at zero temperature
• Magnetized hypermassive neutron star collapse: a central engine for short gamma-ray bursts
• Constraining the Radii of Neutron Stars with Terrestrial Nuclear Laboratory Data
• Tests of the nuclear equation of state and superfluid and superconducting gaps using the Cassiopeia A neutron star
• Short-living supermassive magnetar model for the early X-ray flares following short GRBs
• Light Curves for Rapidly-Rotating Neutron Stars
• The physics of neutron stars
• Microscopic calculations and energy expansions for neutron-rich matter
• R-Modes in Superfluid Neutron Stars
• Spontaneous scalarization
• Extracting Nuclear Symmetry Energies at High Densities from Observations of Neutron Stars and Gravitational Waves
• Cooling of Neutron Stars. Hadronic Model
• Upper Limit on the QCD Axion Mass from Isolated Neutron Star Cooling
• Magnetohydrodynamics in full general relativity: Formulation and tests
• On the universality of I-Love-Q relations in magnetized neutron stars
• Merger of black hole-neutron star binaries: nonspinning black hole case
• Solution of the Hyperon Puzzle within a Relativistic Mean-Field Model
• Improved Treatment of Dark Matter Capture in Neutron Stars
• Exploring the sensitivity of gravitational wave detectors to neutron star physics
• Cooling rates of neutron stars and the young neutron star in the Cassiopeia A supernova remnant
• High Resolution Calculations of Merging Neutron Stars I: Model Description and Hydrodynamic Evolution
• Real-Time Detection of Gravitational Waves from Binary Neutron Stars using Artificial Neural Networks
• Shear viscosity in neutron star cores
• Isolated and Binary Neutron Stars in Dynamical Chern-Simons Gravity
• Finite-size effects at the hadron-quark transition and heavy hybrid stars
• Are small radii of compact stars ruled out by GW170817/AT2017gfo?
• Effects of dark matter on the nuclear and neutron star matter
• Phase Transitions in Neutron Stars and Maximum Masses
• Relativistic Charged Spheres II: Regularity and Stability
• Mapping neutron star data to the equation of state using the deep neural network
• Astrophysical Axion Bounds: The 2024 Edition
• Limit on the Axion Decay Constant from the Cooling Neutron Star in Cassiopeia A
• A new temperature dependent hyperonic equation of state: application to rotating neutron star models and I-Q-relations
• Coalescing Binary Neutron Stars
• Jets, winds and bursts from coalescing neutron stars
• Chiral approach to nuclear matter: Role of two-pion exchange with virtual delta-isobar excitation
• Cold neutrons trapped in external fields
• Accurate nuclear masses from a three parameter Kohn-Sham DFT approach (BCPM)
• Hyperon-nucleon three-body forces and strangeness in neutron stars
• Surface Symmetry Energy of Nuclear Energy Density Functionals
• Cooling of Neutron Stars with Color Superconducting Quark Cores
• Precessing flaring magnetar as a source of repeating FRB 180916.J0158+65
• Application of the density dependent hadron field theory to neutron star matter
• Binary Love Relations
• The coherence of kHz quasi-periodic oscillations in the X-rays from accreting neutron stars
• Neutron Star Mass-Radius Constraints of the Quiescent Low-mass X-ray Binaries X7 and X5 in the Globular Cluster 47 Tuc
• The Dipole Magnetic Field and Spin-down Evolutions of The High Braking Index Pulsar PSR J1640-4631
• Equation of state of dense nuclear matter and neutron star structure from nuclear chiral interactions
• The imprint of the equation of state on the axial w-modes of oscillating neutron stars
• Black Hole Formation in Core-Collapse Supernovae and Time-of-Flight Measurements of the Neutrino Masses
• Density Dependence of the Symmetry energy and the Equation of State of Isospin Asymmetric Nuclear Matter
• The neutron drip line: single-particle degrees of freedom and pairing properties as sources of theoretical uncertainties
• Kaon Condensation in Proto-Neutron Star Matter
• Fundamental oscillation modes of neutron stars: validity of universal relations
• Nuclear heating and melted layers in the inner crust of an accreting neutron star
• The nuclear symmetry energy and stability of matter in neutron star
• GW190814's secondary component with mass $(2.50-2.67)$ M${}_{\odot }$ as a super-fast pulsar
• Quadrupole moments of rotating neutron stars and strange stars
• Multipole Love Relations
• Khon-Sham Density Functional Inspired Approach to Nuclear Binding
• Nuclear chiral dynamics and thermodynamics
• Masses of neutron stars and nuclei
• The Virial Equation of State of Low-Density Neutron Matter
• Internal Heating of Old Neutron Stars: Contrasting Different Mechanisms
• The rotational modes of relativistic stars: Numerical results
• Nuclear and neutron-star matter from local chiral interactions
• Quaking Neutron Stars
• Kilonova/Macronova Emission from Compact Binary Mergers
• Neutron stars in Einstein-aether theory
• Constraints on Axion-like Particles and Nucleon Pairing in Dense Matter from the Hot Neutron Star in HESS J1731-347
• Properties of the nuclear medium
• Essential elements for nuclear binding
• Thermodynamics of isospin-asymmetric nuclear matter from chiral effective field theory
• The Science of the Einstein Telescope
• Effect of Differential Rotation on the Maximum Mass of Neutron Stars: Realistic Nuclear Equations of State
• Constraining the onset density of the hadron-quark phase transition with gravitational-wave observations
• Dark stars: gravitational and electromagnetic observables
• Testing dark decays of baryons in neutron stars
• Quantum Monte Carlo calculations of neutron matter with non-local chiral interactions
• Strong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturation
• Exploring tidal effects of coalescing binary neutron stars in numerical relativity
• Rapidly rotating neutron stars in $R$-squared gravity
• Love can be Tough to Measure
• Gravitational-Wave Asteroseismology with Fundamental Modes from Compact Binary Inspirals
• Evidence for a three-nucleon-force effect in proton-deuteron elastic scattering
• Constraints on Neutron Star Parameters from Burst Oscillation Light Curves of the Accreting Millisecond Pulsar XTE J1814-338
• Relativistic models of magnetars: structure and deformations
• New applications of renormalization group methods in nuclear physics
• Pinning down the superfluid and measuring masses using pulsar glitches
• Forecasting neutron star temperatures: predictability and variability
• Beta equilibrium in neutron star mergers
• Prospects For High Frequency Burst Searches Following Binary Neutron Star Coalescence With Advanced Gravitational Wave Detectors
• Roles of Hyperons in Neutron Stars
• Asymmetric nuclear matter in a parity doublet model with hidden local symmetry
• Magnetars oscillations in the presence of a crust
• The spin parameter of uniformly rotating compact stars
• Changing Frequency Separation of Kilohertz Quasi-Periodic Oscillations in the Sonic-Point Beat-Frequency Model
• Electric Dipole Polarizability in ${}^{208}$Pb as a Probe of the Symmetry Energy and Neutron Matter around ${\rho }_0/3$
• Oscillations of General Relativistic Superfluid Neutron Stars
• On the Cooling of the Neutron Star in Cassiopeia A
• Nuclear symmetry energy and the role of the tensor force
• Relativistic fluid dynamics: physics for many different scales
• Gravitational effects of condensate dark matter on compact stellar objects
• Theoretical and Experimental Constraints for the Equation of State of Dense and Hot Matter
• Chiral EFT based nuclear forces: Achievements and challenges
• Collimated outflows from long-lived binary neutron star merger remnants
• Dark matter interactions with muons in neutron stars
• 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
• Hybrid stars with the color dielectric and the MIT bag models
• Neutron matter at zero temperature with auxiliary field diffusion Monte Carlo
• Numerical relativity confronts compact neutron star binaries: a review and status report
• Treating quarks within neutron stars
• Effects of the two-body and three-body hyperon-nucleon interactions in Λ-hypernuclei
• Chiral dynamics of few- and many-nucleon systems
• Microscopically-based energy density functionals for nuclei using the density matrix expansion: Implementation and pre-optimization
• Neutron stars in Horndeski gravity
• Cooling of Akmal-Pandharipande-Ravenhall neutron star models
• Ground state energy of dilute neutron matter at next-to-leading order in lattice chiral effective field theory
• Hybrid stars with the Dyson-Schwinger quark model
• Elliptic flow in intermediate energy heavy ion collisions and in-medium effects
• General Relativistic Binary Merger Simulations and Short Gamma Ray Bursts
• A Comprehensive Study of Young Black Hole Populations
• Isospin Diffusion in Heavy-Ion Collisions and the Neutron Skin Thickness of Lead
• Why I-Love-Q
• From Neutron Star Observables to the Equation of State. I. An Optimal Parametrization
• Magnetars: super(ficially) hot and super(fluid) cool
• Black hole-neutron star mergers and short GRBs: a relativistic toy model to estimate the mass of the torus
• I-Love-Q anisotropically: Universal relations for compact stars with scalar pressure anisotropy
• Towards mitigation of apparent tension between nuclear physics and astrophysical observations by improved modeling of neutron star matter
• Covariant energy density functionals: nuclear matter constraints and global ground state properties
• All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run
• General Relativistic Magnetohydrodynamic Simulations of Binary Neutron Star Mergers with the APR4 Equation of State
• Observable signatures of enhanced axion emission from protoneutron stars
• Reaction rates and transport in neutron stars
• Constraint on energy-momentum squared gravity from neutron stars and its cosmological implications
• Bayesian Inference of Dense Matter Equation of State within Relativistic Mean Field Models using Astrophysical Measurements
• Was GW170817 a canonical neutron star merger? Bayesian analysis with a third family of compact stars
• Magnetic neutron star cooling and microphysics
• Relativistic stars in scalar-tensor theories with disformal coupling
• The High-Density Symmetry Energy and Direct Urca
• Magnetic field growth in young glitching pulsars with a braking index
• Phase transitions in dense matter and the maximum mass of neutron stars
• Dirac-Brueckner-Hartree-Fock calculations for isospin asymmetric nuclear matter based on improved approximation schemes
• Neutron star bulk viscosity, "spin-flip" and GW emission of newly born magnetars
• Constraints on the dense matter EOS from the measurements of PSR J0737-3039A moment of inertia and PSR J0751+1807 mass
• Impact of PREX-II and combined Radio/NICER/XMM-Newton's mass-radius measurement of PSRJ0740+6620 on the dense matter equation of state
• The possibility of the secondary object in GW190814 as a neutron star
• Linear response theory and neutrino mean free path using Brussels-Montreal Skyrme functionals
• Magneto-elastic oscillations and the damping of crustal shear modes in magnetars
• Antikaon condensation in neutron stars
• Approximate Matching of Analytic and Numerical Solutions for Rapidly Rotating Neutron Stars
• Constraining values of bag constant for strange star candidates
• Low-energy collective excitations in the neutron star inner crust
• A Hard Look at the Neutron Stars and Accretion Disks in 4U 1636-53, GX 17+2, and 4U 1705-44 with $\text{NuSTAR}$
• Constraining the neutron star equation of state using multi-band independent measurements of radii and tidal deformabilities
• Rotochemical Heating in Millisecond Pulsars. Formalism and Non-superfluid case
• Systematics of prompt black-hole formation in neutron star mergers
• Exploring binary-neutron-star-merger scenario of short-gamma-ray bursts by gravitational-wave observation
• Implications of NICER for neutron star matter: the QHC21 equation of state
• Scale-Invariant Hidden Local Symmetry, Topology Change and Dense Baryonic Matter II
• The APR equation of state for simulations of supernovae, neutron stars and binary mergers
• Variational calculation of the ground state of closed-shell nuclei up to $A=40$
• Thermal properties of hot and dense matter with finite range interactions
• Evidence against a strong first-order phase transition in neutron star cores: impact of new data
• X-ray Studies of Two Neutron Stars in 47 Tucanae: Toward Constraints on the Equation of State
• Neutrino emission due to Cooper-pair recombination in neutron stars revisited
• Improved Treatment of Dark Matter Capture in Neutron Stars II: Leptonic Targets
• From Neutron Star Observables to the Equation of State. II. Bayesian Inference of Equation of State Pressures
• Benchmark calculations of pure neutron matter with realistic nucleon-nucleon interactions
• Explaining observations of rapidly rotating neutron stars in LMXBs
• Thermal properties of supernova matter: The bulk homogeneous phase
• Non-perturbative methods for a chiral effective field theory of finite density nuclear systems
• Measurement of neutron star parameters: a review of methods for low-mass X-ray binaries
• NS 1987A in SN 1987A
• Tidal capture of a primordial black hole by a neutron star: implications for constraints on dark matter
• Nuclear and neutron matter $G$-matrix calculations with Ch-EFT potential including effects of three-nucleon interaction
• Delta isobars in relativistic mean-field models with $\sigma$-scaled hadron masses and couplings
• Interdependence of different symmetry energy elements
• Lattice QCD and baryon-baryon interactions: HAL QCD method
• A new equation of state for core-collapse supernovae based on realistic nuclear forces and including a full nuclear ensemble
• Frequency domain model of $f$-mode dynamic tides in gravitational waveforms from compact binary inspirals
• On the Maximum Mass of Neutron Stars
• Dark Matter Heating vs. Rotochemical Heating in Old Neutron Stars
• Coalescence of black hole--neutron star binaries
• Nuclear Equation of state for Compact Stars and Supernovae
• Tidal Deformability of Dark Matter Admixed Neutron Stars
• Dense baryonic matter: constraints from recent neutron star observations
• Relativistic Mean-Field Models with Effective Hadron Masses and Coupling Constants, and rho^- Condensation
• Inference of the sound speed and related properties of neutron stars
• On the Quasi-Periodic Oscillations of Magnetars
• Deep Crustal Heating in a Multicomponent Accreted Neutron Star Crust
• On the metallicity dependence of HMXBs
• On the Ambiguity in Relativistic Tidal Deformability
• Rotating proto-neutron stars: spin evolution, maximum mass and I-Love-Q relations
• Confronting Neutron Star Cooling Theories with New Observations
• Relativistic nuclear energy density functional constrained by low-energy QCD
• Empirical relations for gravitational-wave asteroseismology of binary neutron star mergers
• A general, scale-independent description of the sound speed in neutron stars
• Finite-temperature extension for cold neutron star equations of state
• Exploring tidal effects of coalescing binary neutron stars in numerical relativity II: Longterm simulations
• Variational study for the equation of state of asymmetric nuclear matter at finite temperatures
• Microscopic calculation of the equation of state of nuclear matter and neutron star structure
• R-mode frequencies of slowly rotating relativistic neutron stars with realistic equations of state
• Radial oscillations and stability of compact stars in Eddington-inspired Born-Infeld gravity
• Large amplitude behavior of the bulk viscosity of dense matter
• Discriminating hadronic and quark stars through gravitational waves of fluid pulsation modes
• Thin accretion disks around neutron and quark stars
• The Neutron Star Crust: Nuclear Physics Input
• Probing the Internal Composition of Neutron Stars with Gravitational Waves
• Axion Emission Can Explain a New Hard $X$-ray Excess from Nearby Isolated Neutron Stars
• Holographic modeling of nuclear matter and neutron stars
• Limits on Mass and Radius for the ms-Period X-ray Pulsar SAX J1808.4-3658
• Radial oscillations and stability of compact stars in $f(R,T)=R+2\beta T$ gravity
• The merger of binary white dwarf-neutron stars: Simulations in full general relativity
• Tidal Love numbers of neutron stars in $f(R)$ gravity
• Universal I-Q relations for rapidly rotating neutron and strange stars in scalar-tensor theories
• On the possibility of GW190425 being a black hole--neutron star binary merger
• Assessing theoretical uncertainties in fission barriers of superheavy nuclei
• The Moment of Inertia of the Binary Pulsar J0737-3039A: Constraining the Nuclear Equation of State
• Magnetars as cooling neutron stars with internal heating
• Bounds on the speed of sound in dense matter, and neutron star structure
• Equation of state of low--density neutron matter and the ${}^1{S}_0$ pairing gap
• Magneto-elastic oscillations of neutron stars: exploring different magnetic field configurations
• Equation of state for neutron stars with hyperons by the variational method
• Quark-nuclear hybrid equation of state for neutron stars under modern observational constraints
• Neutron stars in $f(\mathcal{R},\mathcal{T})$ gravity using realistic equations of state in the light of massive pulsars and GW170817
• Post-Newtonian SPH calculations of binary neutron star coalescence. I. Method and first results
• Neutron stars in $f(\mathtt{R},{\mathtt{L}}_{\mathtt{m}})$ gravity with realistic equations of state: joint-constrains with GW170817, massive pulsars, and the PSR J0030+0451 mass-radius from $NICER$ data
• Constraining color flavor locked strange stars in the gravitational wave era
• Mirror model for sterile neutrinos
• Two-fluid models of superfluid neutron star cores
• The Microscopic Approach to Nuclear Matter and Neutron Star Matter
• Unified weak/strong coupling framework for nuclear matter and neutron stars
• Emerging Anisotropic Compact Stars in $f(\mathcal{G},T)$ Gravity
• Properties of trapped neutrons interacting with realistic nuclear Hamiltonians
• The contrasting magnetic fields of superconducting pulsars and magnetars
• Semi-analytic derivation of the threshold mass for prompt collapse in binary neutron star mergers
• Plausible presence of new state in neutron stars with masses above $0.98M_{\mathrm{TOV}}$
• Selecting microscopic Equations of State
• Approximate Universal Relations among Tidal Parameters for Neutron Star Binaries
• Electromagnetic Structure of Few-Nucleon Ground States
• Perturbative approach to the structure of rapidly rotating neutron stars
• Functional renormalization group studies of nuclear and neutron matter
• Chiral symmetry restoration by parity doubling and the structure of neutron stars
• Asymmetric Type-Ia supernova origin of W49B as revealed from spatially resolved X-ray spectroscopic study
• Reducing orbital eccentricity in initial data of binary neutron stars
• Shear viscosity of neutron matter from realistic nucleon-nucleon interactions
• Maximum mass of compact stars from gravitational wave events with finite-temperature equations of state
• 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
• Impact of Dynamical Tides on the Reconstruction of the Neutron Star Equation of State
• Waveform systematics for binary neutron star gravitational wave signals: effects of the point-particle baseline and tidal descriptions
• Imprints of the nuclear symmetry energy on the tidal deformability of neutron stars
• From asymmetric nuclear matter to neutron stars: a functional renormalization group study
• Equation of State of Nuclear Matter at high baryon density
• Dark-matter admixed white dwarfs
• Effects of Rapid Stellar Rotation on Equation of State Constraints Derived from Quasi-Periodic Brightness Oscillations
• Compact Stars for Undergraduates
• Bayesian Inference of the Symmetry Energy and the Neutron Skin in ${}^{48}$Ca and ${}^{208}$Pb from CREX and PREX-2
• Relativistic Mean-Field Models with Scaled Hadron Masses and Couplings: Hyperons and Maximum Neutron Star Mass
• On mass-constraints implied by the relativistic precession model of twin-peak quasi-periodic oscillations in Circinus X-1
• Equation of State and Progenitor Dependence of Stellar-Mass Black-Hole Formation
• Structure of Stable Binary Neutron Star Merger Remnants: Role of Initial Spin
• Superburst Ignition and Implications for Neutron Star Interiors
• Stellar matter with a strong magnetic field within density-dependent relativistic models
• Neural networks reconstruction of the dense-matter equation of state from neutron-star parameters
• Stiffening of matter in quark-hadron continuity
• Quasiequilibrium sequences of binary neutron stars undergoing dynamical scalarization
• Generic Constraints on the Relativistic Mean-Field and Skyrme-Hartree-Fock Models from the Pure Neutron Matter Equation of State
• Neutron star universal relations with microscopic equations of state
• Detection and Parameter Estimation of Gravitational Waves from Binary Neutron-Star Mergers in Real LIGO Data using Deep Learning
• Linear response of homogeneous nuclear matter with energy density functionals
• Electron-muon heat conduction in neutron star cores via the exchange of transverse plasmons
• Constraints on the nuclear symmetry energy from asymmetric-matter calculations with chiral NN and 3N interactions
• Extensive Studies of the Neutron Star Equation of State from the Deep Learning Inference with the Observational Data Augmentation
• Black hole-neutron star mergers are unlikely multi-messenger sources
• In medium T-matrix for nuclear matter with three-body forces - binding energy and single particle properties
• Skyrme-Hartree-Fock-Bogoliubov mass models on a 3D Mesh: Effect of triaxial shape
• Galactic Populations of Ultracompact Binaries
• Effects of Differential Rotation on the Maximum Mass of Neutron Stars
• Hyperon Puzzle, Hadron-Quark Crossover and Massive Neutron Stars
• Equilibrium Structure and Radial Oscillations of Dark Matter Admixed Neutron Stars
• Progress of Quantum Molecular Dynamics model and its applications in Heavy Ion Collisions
• Heating and cooling of magnetars with accreted envelopes
• Nuclear medium cooling scenario in the light of new Cas A cooling data and the 2 M_sun pulsar mass measurements
• Viscous damping of r-modes: Small amplitude instability
• Effects of the equation of state on the bulk properties of maximally-rotating neutron stars
• Large Sound Speed in Dense Matter and the Deformability of Neutron Stars
• Maximum Baryon Masses for Static Neutron Stars in $f(R)$ Gravity
• Static and slowly rotating neutron stars in scalar-tensor theory with self-interacting massive scalar field
• Equation of state of the neutron star matter, and the nuclear symmetry energy
• Wavefunction matching for solving quantum many-body problems
• What neutron stars tell about the hadron-quark phase transition: a Bayesian study
• Proto-neutron star evolution with improved charged-current neutrino-nucleon interactions
• Quark-Meson Coupling Model, Nuclear Matter Constraints and Neutron Star Properties
• Ground State Correlations in 16O and 40Ca
• GRMHD simulations of neutron-star mergers with weak interactions: r-process nucleosynthesis and electromagnetic signatures of dynamical ejecta
• Impact of high-order tidal terms on binary neutron-star waveforms
• Imprints of superfluidity on magneto-elastic QPOs of SGRs
• Magnetic Field Evolution in Neutron Stars: One-Dimensional Multi-Fluid Model
• Constraining the equation of state of nuclear matter with gravitational wave observations: Tidal deformability and tidal disruption
• Diffusive nuclear burning in cooling simulations and application to new temperature data of the Cassiopeia A neutron star
• Density-dependent nucleon-nucleon interaction from three-nucleon forces
• EoS for massive neutron stars
• Gravitational waves from transient neutron star f-mode oscillations
• Relativistic stars in 4D Einstein-Gauss-Bonnet gravity
• Cooling of Dark-Matter Admixed Neutron Stars with density-dependent Equation of State
• Ranking Love numbers for the neutron star equation of state: The need for third-generation detectors
• Classifications of Twin Star Solutions for a Constant Speed of Sound Parameterized Equation of State
• Mass and radius formulas for low-mass neutron stars
• Speed of sound constraints from tidal deformability of neutron stars
• Spin Polarized Asymmetric Nuclear Matter and Neutron Star Matter Within the Lowest Order Constrained Variational Method
• Cluster formation in compact stars: relativistic versus Skyrme models
• Microscopic equation of state of hot nuclear matter for numerical relativity simulations
• Impact of the nuclear equation of state on the last orbits of binary neutron stars
• Imposing multi-physics constraints at different densities on the Neutron Star Equation of State
• Maximum mass cutoff in the neutron star mass distribution and the prospect of forming supramassive objects in the double neutron star mergers
• Constraints on Skyrme Equations of State from Properties of Doubly Magic Nuclei and Ab-Initio Calculations of Low-Density Neutron Matter
• Constraints on the Properties of the Neutron Star XTE J1814-338 from Pulse Shape Models
• Symmetry energy at supra-saturation densities via the Gravitational Waves from GW170817
• Dense matter equation of state of a massive neutron star with anti-kaon condensation
• Bounds on Compactness for LMXB Neutron Stars from X-ray Burst Oscillations
• Quantum Monte Carlo calculations of symmetric nuclear matter
• Modeling dynamical scalarization with a resummed post-Newtonian expansion
• Resummation of fermionic in-medium ladder diagrams to all orders
• Thermal emission of neutron stars with internal heaters
• Chandra Phase-Resolved X-ray Spectroscopy of the Crab Pulsar II
• Effects of Chiral Effective Field Theory Equation of State on Binary Neutron Star Mergers
• Neutron star tidal disruption in mixed binaries: the imprint of the equation of state
• Constraining a possible time-variation of the gravitational constant through "gravitochemical heating" of neutron stars
• Constraints on the Mass and Radius of the Neutron Star XTE J1807-294
• Hubble Space Telescope non-detection of PSR J2144-3933: the coldest known neutron star
• Nuclear matter properties from local chiral interactions with $\Delta$ isobar intermediate states
• Constraints on the symmetry energy from observational probes of the neutron star crust
• Giant Pulsar Glitches and the Inertia of Neutron-Star Crusts
• Crustal heating in accreting neutron stars from the nuclear energy-density functional theory. I. Proton shell effects and neutron-matter constraint
• First-order phase transition from hypernuclear matter to deconfined quark matter obeying new constraints from compact star observations
• Estimating the maximum gravitational mass of nonrotating neutron stars from the GW170817/GRB 170817A/AT2017gfo observation
• New Ideas in Constraining Nuclear Forces
• Polarized thermal emission from X-ray Dim Isolated Neutron Stars: the case of RX J1856.5-3754
• Binary Pulsar constraints on massless scalar-tensor theories using Bayesian statistics
• A Semi-relativistic Model for Tidal Interactions in BH-NS Coalescing Binaries
• Versatility of field theory motivated nuclear effective Lagrangian approach
• Density dependent hadron field theory for neutron stars with antikaon condensates
• Bayesian model-selection of neutron star equation of state using multi-messenger observations
• The Hyperon Puzzle in Neutron Stars
• Transport parameters in neutron stars from in-medium NN cross sections
• Crustal failure during binary inspiral
• Flux tubes and the type-I/type-II transition in a superconductor coupled to a superfluid
• Orbital and epicyclic frequencies around rapidly rotating compact stars in scalar-tensor theories of gravity
• Symmetry energy: nuclear masses and neutron stars
• Extended Skyrme interactions for nuclear matter, finite nuclei and neutron stars
• Scalarization of neutron stars with realistic equations of state
• Thermal evolution and quiescent emission of transiently accreting neutron stars
• Density dependence of the nuclear energy-density functional
• Chiral Fermi liquid approach to neutron matter
• Ferromagnetic neutron stars: axial anomaly, dense neutron matter, and pionic wall
• Probing the equation of state of neutron star matter with gravitational waves from binary inspirals in light of GW170817: a brief review
• Nuclear symmetry energy and the r-mode instability of neutron stars
• Post-Newtonian SPH calculations of binary neutron star coalescence. II. Binary mass ratio, equation of state, and spin dependence
• Anisotropic pressure in dense neutron matter under the presence of a strong magnetic field
• Superfluid Fermi atomic gas as a quantum simulator for the study of neutron-star equation of state
• Equilibrium Configurations of Strongly Magnetized Neutron Stars with Realistic Equations of State
• Probing the nuclear equation of state from the existence of a $\sim 2.6M_{\odot }$ neutron star: the GW190814 puzzle
• Quark deconfinement in neutron star cores: The effects of spin-down
• Protoneutron stars within the Brueckner-Bethe-Goldstone theory
• Nuclear Matter EOS with a Three-body Force
• Impact of Rotation-Driven Particle Repopulation on the Thermal Evolution of Pulsars
• Influence of momentum-dependent interactions on balance energy and mass dependence
• Non-conformally flat initial data for binary compact objects
• Probing isospin- and momentum-dependent nuclear effective interactions in neutron-rich matter
• Semi-realistic nucleon-nucleon interactions with improved neutron-matter properties
• Constraints on the inner edge of neutron star crusts from relativistic nuclear energy density functionals
• ${}^3{P}_2$-${}^3{F}_2$ Pairing in Dense Neutron Matter: The Spectrum of Solutions
• Negative Kaons in Dense Baryonic Matter
• Hierarchical Inference of Binary Neutron Star Mass Distribution and Equation of State with Gravitational Waves
• Composition temperature-dependent g-modes in superfluid neutron stars
• Hybrid protoneutron stars with the Dyson-Schwinger quark model
• Heat blanketing envelopes of neutron stars
• Quark formation and phenomenology in binary neutron-star mergers using V-QCD
• Tidal Deformabilities of Neutron Stars in scalar-Gauss-Bonnet Gravity and Their Applications to Multimessenger Tests of Gravity
• Dense and Hot QCD at Strong Coupling
• Viscous damping of r-modes: Large amplitude saturation
• Are nuclear matter properties correlated to neutron star observables ?
• Triplet Pairing in Neutron Matter
• Skyrme-Hartree-Fock-Bogoliubov mass models on a 3D mesh: II. Time-reversal symmetry breaking
• Lattice Calculation of Thermal Properties of Low-Density Neutron Matter with Pionless NN Effective Field Theory
• Constraints on Axions and Axionlike Particles from Fermi Large Area Telescope Observations of Neutron Stars
• Realistic Exact Solution for the Exterior Field of a Rotating Neutron Star
• Viscosity of neutron star matter and $r$-modes in rotating pulsars
• Frequency deviations in universal relations of isolated neutron stars and postmerger remnants
• Rapidly Spinning Compact Stars with Deconfinement Phase Transition
• Strangeons constitute bulk strong matter-- To test using GW170817
• Are pulsars born with a hidden magnetic field?
• EoS for hot neutron stars
• Entrainment in Superfluid Neutron Star Crusts: Hydrodynamic Description and Microscopic Origin
• Spectral analysis of gravitational waves from binary neutron star merger remnants
• Relativistic Brueckner-Hartree-Fock in nuclear matter without the average momentum approximation
• Role of the symmetry energy and the neutron-matter stiffness on the tidal deformability of a neutron star with unified equations of state
• Nuclear physics constraints from binary neutron star mergers in the Einstein Telescope era
• Large and massive neutron stars: Implications for the sound speed in dense QCD
• Static Response of Neutron Matter
• The physics of Core-Collapse Supernovae: explosion mechanism and explosive nucleosynthesis
• Twin peak quasi-periodic oscillations as signature of oscillating cusp torus
• A new method to constrain neutron star structure from quasi-periodic oscillations
• Dark matter seeding and the kinematics and rotation of neutron stars
• Neutron matter at finite temperature
• Magnetars: Time Evolution, Superfluid Properties, and Mechanism of Magnetic Field Decay
• Auxiliary Field Diffusion Monte Carlo calculation of ground state properties of neutron drops
• Microscopic study of neutrino trapping in hyperon stars
• Probing the isospin dependence of the in-medium nucleon-nucleon cross sections with radioactive beams
• Neutron star crust cooling in KS 1731-260: the influence of accretion outburst variability on the crustal temperature evolution
• Neutron star cooling constraints for color superconductivity in hybrid stars
• Viscous damping of r-mode oscillations in compact stars with quark matter
• Quasinormal modes of compact objects in alternative theories of gravity
• Cooling of Neutron Stars with Strong Toroidal Magnetic Fields
• $R^p$ Attractors Static Neutron Star Phenomenology
• Neutron Stars with Baryon Number Violation, Probing Dark Sectors
• The Role of the Dilaton in Dense Skyrmion Matter
• Remarks on nuclear matter: how an ${\omega }_0$ condensate can spike the speed of sound, and a model of $Z(3)$ baryons
• Equation of State for Nucleonic Matter and its Quark Mass Dependence from the Nuclear Force in Lattice QCD
• Comparative study of three-nucleon potentials in nuclear matter
• Finite temperature effects on anisotropic pressure and equation of state of dense neutron matter in an ultrastrong magnetic field
• Benchmark calculations of infinite neutron matter with realistic two- and three-nucleon potentials
• Differentially rotating neutron stars in scalar-tensor theories of gravity
• Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects
• Neutron star structure and collective excitations of finite nuclei
• Constraining Superfluidity in Dense Matter from the Cooling of Isolated Neutron Stars
• R-modes of neutron stars with the superfluid core
• The Gravity Collective: A Search for the Electromagnetic Counterpart to the Neutron Star-Black Hole Merger GW190814
• Universal Inflationary Attractors Implications on Static Neutron Stars
• Astrophysical science metrics for next-generation gravitational-wave detectors
• In-medium enhancement of the modified Urca neutrino reaction rates
• LOCV calculation for Beta-stable matter at finite temperature
• Inflationary Attractors Predictions for Static Neutron Stars in the Mass-Gap Region
• New binary pulsar constraints on Einstein-æther theory after GW170817
• Microscopic Vortex Velocity in the Inner Crust and Outer Core of Neutron Stars
• Phase Transitions in Nucleonic Matter and Neutron-Star Cooling
• Polarized Neutron Matter: A Lowest Order Constrained Variational Approach
• Observable effects of symmetry energy in heavy-ion collisions at RIA energies
• Magnetic field evolution and equilibrium configurations in neutron star cores: the effect of ambipolar diffusion
• Constraining the properties of neutron star crusts with the transient low-mass X-ray binary Aql X-1
• Crust structure and thermal evolution of neutron stars in soft X-ray transients
• Chaotic dynamics around astrophysical objects with nonisotropic stresses
• Probing nuclear symmetry energy at high densities using pion, kaon, eta and photon productions in heavy-ion collisions
• Medium Effects in Cooling of Neutron Stars and $3P_2$ Neutron Gap
• Variational Theory of Hot Nucleon Matter II : Spin-Isospin Correlations and Equation of State of Nuclear and Neutron Matter
• Universal relations for rapidly rotating cold and hot hybrid star
• From the microscopic to the macroscopic world: from nucleons to neutron stars
• Post-Tolman-Oppenheimer-Volkoff formalism for relativistic stars
• Head-on collisions of binary white dwarf--neutron stars: Simulations in full general relativity
• Energy density functional on a microscopic basis
• A systematic study of the ${\pi }^{-}/{\pi }^{+}$ ratio in heavy-ion collisions with the same neutron/proton ratio but different masses
• Prompt Mergers of Neutron Stars with Black Holes
• Connecting neutron star observations to the high density equation of state of quasi-particle model
• Symmetry energy, neutron skin, and neutron star radius from chiral effective field theory interactions
• Multi-epoch Analysis of Pulse Shapes from the Neutron Star SAX J1808.4-3658
• Unveiling the universality of I-Love-Q relations
• Effective density functionals beyond mean field
• Variational Calculation for the Equation of State of Nuclear Matter at Finite Temperatures
• Neutron Stars in Scalar-tensor Gravity with Quartic Order Scalar Potential
• Improved Analytic Modeling of Neutron Star Interiors
• Distinguishing high-mass binary neutron stars from binary black holes with second- and third-generation gravitational wave observatories
• A cooling neutron star crust after recurrent outbursts: Modelling the accretion outburst history of Aql X-1
• Holographic approach to compact stars and their binary mergers
• Nuclear equation of state at high baryonic density and compact star constraints
• Thermodynamical Description of Hot, Rapidly Rotating Neutron Stars, Protoneutron Stars, and Neutron Star Merger Remnants
• Studying the onset of deconfinement with multi-messenger astronomy of neutron stars
• Hydrostatic Expansion and Spin Changes During Type I X-Ray Bursts
• Nuclear Masses and Neutron Stars
• General-relativistic treatment of tidal $g$-mode resonances in coalescing binaries of neutron stars. I. Theoretical framework and crust breaking
• Influence of the stiffness of the equation of state and in-medium effects on the cooling of compact stars
• Finite tidal effects in GW170817: Observational evidence or model assumptions?
• Chiral condensate in neutron matter
• Translating neutron star observations to nuclear symmetry energy via artificial neural networks
• Tidal deformations of compact stars with crystalline quark matter
• Systematic study on the quark-hadron mixed phase in compact stars
• Non-strange Dibaryon Resonances Observed in the $\gamma d\to {\pi }^0{\pi }^{0}d$ Reaction
• Ultra-Dense Neutron Star Matter, Strange Quark Stars, and the Nuclear Equation of State
• Pulsar spin-down luminosity: Simulations in general relativity
• Structures of the Vela pulsar and the glitch crisis from the Brueckner theory
• Predicting magic numbers of nuclei with semi-realistic nucleon-nucleon interactions
• Strong-coupling corrections to ground-state properties of a superfluid Fermi gas
• Sound velocity in dense stellar matter with strangeness and compact stars
• Deep Learning Detection and Classification of Gravitational Waves from Neutron Star-Black Hole Mergers
• Neutron stars and the dense matter equation of state: from microscopic theory to macroscopic observations
• Static Neutron Stars Perspective of Quadratic and Induced Inflationary Attractor Scalar-tensor Theories
• From homogeneous matter to finite nuclei: Role of the effective mass
• Phenomenological Relations for Axial Quasi-normal Modes of Neutron Stars with Realistic Equations of State
• Crustal Oscillations of Slowly Rotating Relativistic Stars
• Multimessenger Binary Mergers Containing Neutron Stars: Gravitational Waves, Jets, and $\mathbf{\gamma }$-Ray Bursts
• Consequences of neutron decay inside neutron stars
• Drop of coherence of the lower kilo-Hz QPO in neutron stars: is there a link with the innermost stable circular orbit?
• Variational Theory of Hot Nucleon Matter
• Probing the Nuclear Symmetry Energy with Heavy-Ion Reactions Induced by Neutron-Rich Nuclei
• New equation of states for postmerger supramassive quark stars
• Toward Realistic and Practical No-Hair Relations for Neutron Stars in the Non-Relativistic Limit
• Self-consistent Continuum Random Phase Approximation calculations with finite-range interactions
• Quantum gravity effects on compact star cores
• The chiral quark condensate and pion decay constant in nuclear matter at next-to-leading order
• Phenomenological neutron star equations of state: 3-window modeling of QCD matter
• The 2016 Vela glitch: a key to neutron star internal structure and dynamics
• Hybrid neutron stars with the Dyson-Schwinger quark model and various quark-gluon vertices
• Rotochemical heating in millisecond pulsars: modified Urca reactions with uniform Cooper pairing gaps
• Super-Eddington fluxes during thermonuclear X-ray bursts
• Gravitational-wave spin-down and stalling lower limits on the electrical resistivity of the accreted mountain in a millisecond pulsar
• Fast Radio Burst Trains from Magnetar Oscillations
• Strange Quark Matter in Stars: A General Overview
• From dilute matter to the equilibrium point in the energy--density--functional theory
• Probing the interior of neutron stars with gravitational waves
• Equations of state and stability of color-superconducting quark matter cores in hybrid stars
• Resummation of in-medium ladder diagrams: s-wave effective range and p-wave interaction
• Constraining properties of high-density matter in neutron stars with magneto-elastic oscillations
• Cosmography with next-generation gravitational wave detectors
• Neutron-star radii based on realistic nuclear interactions
• Reanalysis of the binary neutron star mergers GW170817 and GW190425 using numerical-relativity calibrated waveform models
• Constraining equation of state groups from $g$-mode asteroseismology
• Constraining properties of rapidly rotating neutron stars using data from heavy-ion collisions
• Cassiopeia A and direct URCA cooling
• The Renormalization Group in Nuclear Physics
• Nuclear fourth-order symmetry energy and its effects on neutron star properties in the relativistic Hartree-Fock theory
• Timescale of twin-peak quasi-periodic oscillations and mass of accreting neutron stars
• Equation of state of cold and dense QCD matter in resummed perturbation theory
• Equation of State for Hot and Dense Matter: $\sigma$-$\omega$-$\rho$ Model with Scaled Hadron Masses and Couplings
• Postglitch exponential relaxation of radio pulsars and magnetars in terms of vortex creep across flux tubes
• Neutron-proton effective mass splitting and thermal evolution in neutron rich matter
• Cooling of young neutron stars and dark gauge bosons
• The massive neutron star or low-mass black hole in 2S0921-630
• I-Love relation for incompressible stars and realistic stars
• Relating Follicly-Challenged Compact Stars to Bald Black Holes
• On the validity of the adiabatic approximation in compact binary inspirals
• The neutron star in Cassiopeia A: equation of state, superfluidity, and Joule heating
• Dilute neutron matter on the lattice at next-to-leading order in chiral effective field theory
• Constraining the nuclear symmetry energy and properties of neutron star from GW170817 by Bayesian analysis
• Axial quasi-normal modes of Einstein-Gauss-Bonnet-dilaton neutron stars
• Improved Universality in the Neutron Star Three-Hair Relations
• Effect of spin on the inspiral of binary neutron stars
• Binary Neutron Stars in Quasi-equilibrium
• Studies of two-solar-mass hybrid stars within the framework of Dyson-Schwinger equations
• Asymptotic behavior of Nambu-Bethe-Salpeter wave functions for multi-particles in quantum field theories
• I-Love-Q Relations for Neutron Stars in dynamical Chern Simons Gravity
• Role of nucleonic Fermi surface depletion in neutron star cooling
• Binary neutron star mergers as a probe of quark-hadron crossover equations of state
• Ruling out the supersoft high-density symmetry energy from the discovery of PSR J0740+6620 with mass $2.14_{-0.09}^{+0.10}{M}_{\odot }$
• A pitfall of piecewise-polytropic equation of state inference
• kHz Quasi-Periodic Oscillations in the low-mass X-ray binary 4U 0614+09
• The special point on the hybrid star mass--radius diagram and its multi--messenger implications
• Low densities in asymmetric nuclear matter
• Axial quasi-normal modes of neutron stars: Accounting for the superfluid in the crust
• Bulk viscosity in neutron stars with hyperon cores
• Cooling Theory Faced with Old Warm Neutron Stars: Role of Non-Equilibrium Processes with Proton and Neutron Gaps
• Lowest Order Constrained Variational Calculation of the Polarized Nuclear Matter with the Modern $A{V}_{18}$ Potential
• Thermalization and Annihilation of Dark Matter in Neutron Stars
• The surface of rapidly-rotating neutron stars: implications to neutron star parameter estimation
• Equation of state for $\beta$-stable hot nuclear matter
• Three-dimensional non-vacuum pulsar outer-gap model: Localized acceleration electric field in the higher altitudes
• Imprints of the nuclear symmetry energy on gravitational waves from the axial w-modes of neutron stars
• 3+1 geodesic equation and images in numerical spacetimes
• Relativistic mean field model for ultra-compact low mass neutron star of HESS J1731-347
• Capture of Electroweak Multiplet Dark Matter in Neutron Stars
• Can chiral EFT give us satisfaction?
• nEoS: Neutron Star Equation of State from hadron physics alone
• Consistent accretion-induced heating of the neutron-star crust in MXB 1659-29 during two different outbursts
• Binary neutron star merger simulations with different initial orbital frequency and equation of state
• Model-Independent Inference of Neutron Star Radii from Moment of Inertia Measurements
• Gravitational Waveforms for Precessing, Quasicircular Compact Binaries with Multiple Scale Analysis: Small Spin Expansion
• The Black Hole Remnant of Black Hole-Neutron Star Coalescing Binaries
• Nuclear limits on gravitational waves from elliptically deformed pulsars
• Mass-angular-momentum relations implied by models of twin peak quasi-periodic oscillations
• Constraining the density dependence of the symmetry energy with nuclear data and astronomical observations in the KIDS framework
• Lattice QCD Constraints on Hybrid and Quark Stars
• Can the GW190814 secondary component be a bosonic dark matter admixed compact star?
• Ab initio and phenomenological studies of the static response of neutron matter
• Rotochemical heating of millisecond and classical pulsars with anisotropic and density-dependent superfluid gap models
• Binary White Dwarfs as Laboratories for Extreme Gravity with LISA
• The axial anomaly and the phases of dense QCD
• A chiral lagrangian with Broken Scale: testing the restoration of symmetries in astrophysics and in the laboratory
• Diffusive heat blanketing envelopes of neutron stars
• Short gamma-ray burst jet propagation in binary neutron star merger environments
• Torsional oscillations of neutron stars in scalar-tensor theory of gravity
• Nuclear equation of state at high density and the properties of neutron stars
• Single-particle potential of the $\Lambda$ hyperon in nuclear matter with chiral effective field theory NLO interactions including effects of YNN three-baryon interactions
• Gamma-Ray Bursts via the Neutrino Emission from Heated Neutron Stars
• Isospin dependent properties of asymmetric nuclear matter
• Sloppy nuclear energy density functionals: effective model reduction
• Constraining a possible time variation of the gravitational constant G with terrestrial nuclear laboratory data
• Impact of pions on binary neutron star mergers
• Neutron Star Matter as a Relativistic Fermi Liquid
• Constraining the Origin of Magnetar Flares
• Microscopic calculations of transport properties of neutron matter
• Cooling of hypernuclear compact stars: Hartree-Fock models and high-density pairing
• Axisymmetric models for neutron star merger remnants with realistic thermal and rotational profiles
• X-ray bounds on cooling, composition, and magnetic field of the Cassiopeia A neutron star and young central compact objects
• Bayesian timing analysis of giant flare of SGR 1806-20 by RXTE PCA
• Correlations between charge radii differences of mirror nuclei and stellar observables
• Quantum Monte Carlo Studies of Relativistic Effects in Light Nuclei
• Degeneracy in the inference of phase transitions in the neutron star equation of state from gravitational wave data
• Spontaneous scalarization with an extremely massive field and heavy neutron stars
• Near-Infrared Light Curves of the Black Hole Binary A0620-00
• An Infrared Search for Kilonovae with the WINTER Telescope. I. Binary Neutron Star Mergers
• Neutron star-black hole mergers in next generation gravitational-wave observatories
• Soft nuclear equation-of-state from heavy-ion data and implications for compact stars
• Thin accretion disks around cold Bose-Einstein Condensate stars
• A Generalized Semi-Analytic Model for Magnetar-Driven Supernovae
• Weak response of cold symmetric nuclear matter at three-body cluster level
• Constraints on the Steady-State R-mode Amplitude in Neutron Star Transients
• Thermal evolution of neo-neutron stars. I: envelopes, Eddington luminosity phase and implications for GW170817
• Phenomenological QCD equations of state for neutron star dynamics: Nuclear-2SC continuity and evolving effective couplings
• Rotation at 1122 Hz and the neutron star structure
• The equation of state and radial oscillations of neutron stars
• Axial quasi-normal modes of scalarized neutron stars with massive self-interacting scalar field
• Coherent magneto-elastic oscillations in superfluid magnetars
• Reexamining the relation between the binding energy of finite nuclei and the equation of state of infinite nuclear matter
• Temperature effects in pulsating superfluid neutron stars
• Two-layer compact stars with crystalline quark matter: Screening effect on the tidal deformability
• Probing Matter Radii of Neutron-Rich Nuclei by Antiproton Scattering
• GW170817 and the prospect of forming supramassive remnants in neutron star mergers
• Many-body correlations in Semiclassical Molecular Dynamics and Skyrme interaction
• Modulating the magnetosphere of magnetars by internal magneto-elastic oscillations
• Energy-density functionals inspired by effective-field theories: Applications to neutron drops
• Implementing chiral three-body forces in terms of medium-dependent two-body forces
• Impact of updated Multipole Love numbers and f-Love Universal Relations in the context of Binary Neutron Stars
• Future Prospects for Probing Scalar-Tensor Theories with Gravitational Waves from Mixed Binaries
• Pulse profiles of highly compact pulsars in general relativity
• Effect of the Nuclear Equation of State on Relativistic-Turbulence Induced Core-Collapse Supernovae
• Chiral four-body interactions in nuclear matter
• The Barcelona-Catania-Paris-Madrid functional with a realistic effective mass
• Nuclear matter at high density: Phase transitions, multiquark states, and supernova outbursts
• Maximally incompressible neutron star matter
• Quasi-normal modes of superfluid neutron stars
• Intrinsic properties of the engine and jet that powered the short gamma-ray burst associated with GW170817
• Thermal behavior as indicator for hyperons in binary neutron star merger remnants
• Temperature dependence of magnetic susceptibility of nuclear matter: lowest order constrained variational calculations
• Speed of sound constraints on maximally rotating neutron stars
• Lowest order constrained variational calculation of polarized neutron matter at finite temperature
• Tensor force effects and high-momentum components in the nuclear symmetry energy
• Isospin coupling-channel decomposition of nuclear symmetry energy in covariant density functional theory
• Comparison of statistical treatments for the equation of state for core-collapse supernovae
• Scalarized neutron stars in massive scalar-tensor gravity: X-ray pulsars and tidal deformability
• Constraints on Phase Transitions in Neutron Star Matter
• Exact versus Taylor-expanded energy density in the study of the neutron star crust-core transition
• The existence of a two-solar mass neutron star constrains the gravitational constant G_N at strong field
• Two-fluid simulations of the magnetic field evolution in neutron star cores in the weak-coupling regime
• Universal relations for the Keplerian sequence of rotating neutron stars
• Mass and radius relations of quarkyonic stars using an excluded volume model
• Studies of the hybrid star structure within 2+1 flavors NJL model
• On attributes of a Rotating Neutron star with a Hyperon core
• General-relativistic treatment of tidal $g$-mode resonances in coalescing binaries of neutron stars. II. As triggers for precursor flares of short gamma-ray bursts
• Hyperon star in a modified quark meson coupling model
• Constraints on the equation of state from the stability condition of neutron stars
• A new consistent Neutron Star Equation of State from a Generalized Skyrme model
• The Shapes of Atomic Lines from the Surfaces of Weakly Magnetic Rotating Neutron Stars and Their Implications
• Newtonian View of General Relativistic Stars
• Structure of the hadron-quark mixed phase in protoneutron stars
• Non-perturbative Extraction of the Effective Mass in Neutron Matter
• Millisecond radio pulsars with known masses: parameter values and equation of state models
• Distinguishing double neutron star from neutron star-black hole binary populations with gravitational wave observations
• Black hole - neutron star mergers: The first mass gap and kilonovae
• Possibility of s-wave pion condensates in neutron stars revisited
• Hadron matter in neutron stars in view of gravitational wave observations
• Neutron star cooling - a challenge to the nuclear mean field
• Dissipation in relativistic superfluid neutron stars
• The equation of state and some key parameters of neutron stars: constraints from GW170817, the nuclear data and the low mass X-ray binary data
• The first five years of gravitational-wave astrophysics
• Application of the Ghosh & Lamb Relation to the Spin-up/down Behavior in the X-ray Binary Pulsar 4U 1626-67
• Cold Atom Quantum Simulator for Dilute Neutron Matter
• Nuclear matter equation of state from a quark-model nucleon-nucleon interaction
• Collapse of magnetized hypermassive neutron stars in general relativity: Disk evolution and outflows
• Superfluid Phase Transitions in Dense Neutron Matter
• Structure, Deformations and Gravitational Wave Emission of Magnetars
• Holographic QCD in the NICER era
• Nuclear Matter and Neutron Stars from Relativistic Brueckner-Hartree-Fock Theory
• Comparing the inspiral of irrotational and corotational binary neutron stars
• Nuclear chiral dynamics and phases of QCD
• Distinguishing the nature of ''ambiguous'' merging systems hosting a neutron star: GW190425 in low-latency
• Axial quasi-normal modes of neutron stars in $R^2$ gravity
• Constraining three-nucleon forces with multimessenger data
• Detecting resonant tidal excitations of Rossby modes in coalescing neutron-star binaries with third-generation gravitational-wave detectors
• From bare interactions, low--energy constants and unitary gas to nuclear density functionals without free parameters: application to neutron matter
• Axial Quasi-Normal Modes of Scalarized Neutron Stars with Realistic Equations of State
• Quark matter imprint on Gravitational Waves from oscillating stars
• Rearrangement of the Fermi Surface of Dense Neutron Matter and Direct Urca Cooling of Neutron Stars
• Radial Oscillations of Hybrid Stars
• Lambda hypernuclei and neutron star matter in a chiral SU(3) relativistic mean field model with a logarithmic potential
• A Gravitational Wave Detector for Post Merger Neutron Stars: Beyond the Quantum Loss Limit of Michelson Fabry Perot Interferometer
• Shear viscosity due to phonons in superfluid neutron stars
• Probing Mechanical and Chemical Instabilities in Neutron-Rich Matter
• Analysis of nuclear structure in a converging expansion scheme
• Effect of three-body forces on response functions in infinite neutron matter
• Hunting for Orphaned Central Compact Objects among Radio Pulsars
• Mixed-phase induced core-quakes and the changes in neutron star parameters
• Cooling of neutron stars in "nuclear medium cooling scenario" with stiff equation of state including hyperons
• Fluctuations and phases in baryonic matter
• Dark gauge boson production from neutron stars via nucleon-nucleon bremsstrahlung
• Gravitational wave probes of particle dark matter: a review
• Improved Constraints on Modified Gravity with Eccentric Gravitational Waves
• Constraining neutron superfluidity with $r$-mode physics
• Kaon Condensation in Dense Matter
• Radial oscillations of quark stars from perturbative QCD
• Bose-Einstein condensation in dense nuclear matter and strong magnetic fields
• Properties of exotic nuclei and their linkage to the nucleonic interaction
• A Comparison of Measured Crab and Vela Glitch Healing Parameters with Predictions of Neutron Star Models
• Skyrme forces with extended density dependence
• Quasi-periodic oscillations in precursor flares via seismic aftershocks from resonant shattering
• Nuclear Matter from Effective Quark-Quark Interaction
• Impacts of anomaly on nuclear and neutron star equation of state based on a parity doublet model
• Revisiting the maximum mass of differentially rotating neutron stars in general relativity: Übermassive stars with realistic equations of state
• Deformed crystals and torsional oscillations of neutron star crust
• Hybrid star structure with the Field Correlator Method
• Covariant Density Functional Theory with Localized Exchange Terms
• Neutron Star in Covariant $f(Q)$ gravity
• XTE J1814-338: A potential hybrid star candidate
• GW170817 and GW190425 as Hybrid Stars of Dark and Nuclear Matters
• Oscillating magnetised hybrid stars under the magnifying glass of multi-messenger observations
• Application of the nuclear equation of state obtained by the variational method to core-collapse supernovae
• Stellar Hydrostatic Equilibrium Compact Structures in $f(\mathcal{G},T)$ Gravity
• Nuclear Matter Spectral Functions by Transport Theory
• Novel neutron decay mode inside neutron stars
• The relativistic self-energy in nuclear dynamics
• Deformation and crustal rigidity of rotating neutron stars
• Accretion disks around neutron and strange stars in ${\mathcal{R}}^2$ gravity
• Superfluid Phase Transitions and Effects of Thermal Pairing Fluctuations in Asymmetric Nuclear Matter
• The induced surface tension contribution for the equation of state of neutron stars
• Cooper Triples in Attractive Three-Component Fermions: Implication for Hadron-Quark Crossover
• Tidal Deformation of Neutron Stars from Microscopic Models of Nuclear Dynamics
• Inertial modes of neutron stars with the superfluid core
• Nuclear symmetry energy in presence of hyperons in the nonrelativistic Thomas-Fermi approximation
• Nuclear symmetry energy effects on neutron stars properties
• Finite-size effects on the Phase Structure of the Walecka Model
• Multipole moments and universal relations for scalarized neutron stars
• Evolutionary implications of a magnetar interpretation for GLEAM-X J162759.5-523504.3
• Extended Skyrme Equation of State in asymmetric nuclear matter
• Charged $\rho$-meson condensation in neutron stars
• Two steps forward and one step sideways: the propagation of relativistic jets in realistic binary neutron star merger ejecta
• Constraining neutron star properties with a new equation of state insensitive approach
• Strangeness Balance in HADES Experiments and the Xi- Enhancement
• Central Speed of Sound, Trace Anomaly and Observables of Neutron Stars from Perturbative Analyses of Scaled TOV Equations
• Constraints on the merging binary neutron star mass distribution and equation of state based on the incidence of jets in the population
• Topological neutron stars in tensor-multi-scalar theories of gravity
• Black hole remnant of black hole-neutron star coalescing binaries with arbitrary black hole spin
• Contribution of isovector mesons to the symmetry energy in a microscopic model
• Finding quark content of neutron stars in light of GW170817
• Ground state of finite nuclei evaluated from realistic interactions
• Dense matter equation of state for neutron star mergers
• Deformation properties with a finite range simple effective interaction
• S-matrix approach to equation of state of nuclear matter
• Analysis of the neutron matter equation of state and the symmetry energy up to fourth order of chiral effective field theory
• Cooling of neutron stars in soft X-ray transients
• Neutron Star Mergers Chirp About Vacuum Energy
• Revisiting the Equation of State of Hybrid Stars in the Dyson-Schwinger Equation Approach to QCD
• Temperature dependence of single-particle properties in nuclear matter
• How far is normal nuclear matter from the chiral symmetry restoration?
• The reliability of the low-latency estimation of binary neutron star chirp mass
• Rotochemical Heating of Neutron Stars: Rigorous Formalism with Electrostatic Potential Perturbations
• Isovector Channel Role of Relativistic Mean Field Models in the Neutrino Mean Free Path
• Recent progress constraining the nuclear equation of state from astrophysics and heavy ion reactions
• Role of the symmetry energy on the neutron-drip transition in accreting and nonaccreting neutron stars
• Models of binary neutron star remnants with tabulated equations of state
• Phenomenological QCD equations of state for neutron stars
• Neutron Star Mass-Radius Constraints using Evolutionary Optimization
• Short-range correlations in isospin symmetric and asymmetric nuclear matter: a microscopic perspective
• Neutron Stars in frames of $R^2$-gravity and Gravitational Waves
• Non-topological spontaneously scalarized neutron stars in tensor-multi-scalar theories of gravity
• Do Neutron Star Gravitational Waves Carry Superfluid Imprints?
• Neutron star matter in an effective model
• Perturbative Analysis of Universality and Individuality in Gravitational Waves from Neutron Stars
• Chandra Phase-Resolved Spectroscopy of the High Magnetic Field Pulsar B1509-58
• The highest-frequency kHz QPOs in neutron star low mass X-ray binaries
• Decoupling of superfluid and normal modes in pulsating neutron stars
• Constraining the Neutron Star Radius with Joint Gravitational-Wave and Short Gamma-Ray Burst Observations of Neutron Star-Black Hole Coalescing Binaries
• Searching for exotic cores with binary neutron star inspirals
• The role of binding energies of neutron stars on the accretion driven evolution
• Relativistic stars with purely toroidal magnetic fields with realistic equations of state
• Using Gray Sirens to Resolve the Hubble-Lemaître Tension
• Shear viscosity and the r-mode instability window in superfluid neutron stars
• Soft Modes, Resonances and Quantum Transport
• X-ray bounds on the r-mode amplitude in millisecond pulsars
• Quasi-universality of the magnetic deformation of neutron stars in general relativity and beyond
• Are fast radio bursts the most likely electromagnetic counterpart of neutron star mergers resulting in prompt collapse?
• Hot neutron stars and their equation of state
• Velocity-dependent energy gaps and dynamics of superfluid neutron stars
• Ways to constrain neutron star equation of state models using relativistic disc lines
• Three-body spin-orbit forces from chiral two-pion exchange
• Nonequilibrium Weak Processes in Kaon Condensation II - Kinetics of condensation ---
• Diagrammatic calculation of thermodynamical quantities in nuclear matter
• Disc-oscillation resonance and neutron star QPOs: 3:2 epicyclic orbital model
• Self-similarity relations for cooling superfluid neutron stars
• Study of spin polarized nuclear matter and finite nuclei with finite range simple effective interaction
• Thermal evolution of neutron stars in soft X-ray transients with thermodynamically consistent models of the accreted crust
• Gravitational wave constraints on the shape of neutron stars
• Two coexisting families of compact stars: observational implications for millisecond pulsars
• Reinvestigation of the electron fraction and electron Fermi energy of neutron star
• Probing phase transition in neutron stars via the crust-core interfacial mode
• Universal relations for innermost stable circular orbits around rapidly rotating neutron stars
• A phenomenological equation of state for isospin asymmetric nuclear matter
• Momentum distributions and spectroscopic factors of doubly-closed shell nuclei in correlated basis function theory
• Temperature dependence of the volume and surface contributions to the nuclear symmetry energy within the coherent density fluctuation model
• Microscopic nuclear equation of state at finite temperature and stellar stability
• New Bayesian analysis of hybrid EoS constraints with mass-radius data for compact stars
• Exploring universal characteristics of neutron star matter with relativistic \textit{ab initio} equations of state
• Gravitational waves from neutron star excitations in binary inspirals
• Mixed phase transition from hypernuclear matter to deconfined quark matter fulfilling mass-radius constraints of neutron stars
• Nuclei in Core-Collapse Supernovae Engine
• Effect of nucleon effective mass and symmetry energy on the neutrino mean free path in a neutron star
• Probing Strange Stars with Advanced Gravitational Wave Detectors
• Properties of scalar wave emission in a scalar-tensor theory with kinetic screening
• Jet-environment interplay in magnetized binary neutron star mergers
• Supernova Neutrino-Effects on R-Process Nucleosynthesis in Black Hole Formation
• Neutrino luminosities and heat capacities of neutron stars in analytic form
• Perturbation Theory of Nuclear Matter with a Microscopic Effective Interaction
• Nonparametric model for the equations of state of neutron star from deep neural network
• Numerical Study of Stellar Core Collapse and Neutrino Emission Using the Nuclear Equation of State Obtained by the Variational Method
• Core States of Neutron Stars from Anatomizing their Scaled Structure Equations
• Correlations in Nuclear Matter
• Properties of neutron star described by a relativistic $abinitio$ model
• Universal properties of maximum-mass neutron stars: a new tool to explore superdense matter
• Acceptability Conditions and Relativistic Barotropic Equations of State
• Constraining the equation of state in modified gravity via universal relations
• Thermodynamic Properties of Holographic Multiquark and the Multiquark Star
• Tidal deformability and gravitational-wave phase evolution of magnetised compact-star binaries
• Constraints on temporal variation of fundamental constants from GRBs
• Superfluid nucleon matter in and out of equilibrium and weak interactions
• Localization of Compact Binary Sources with Second Generation Gravitational-wave Interferometer Networks
• Mass and radius constraints for compact stars and the QCD phase diagram
• Studies of the equation-of-state of nuclear matter by heavy-ion collisions at intermediate energy in the multi-messenger era
• Spin-orbit induced backflow in neutron matter with auxiliary field diffusion Monte Carlo
• Magnetic excitations in nuclei with neutron excess
• Spindown of Isolated Neutron Stars: Gravitational Waves or Magnetic Braking?
• Temperature-dependent r-modes in superfluid neutron stars stratified by muons
• Epicyclic oscillations in the Hartle-Thorne external geometry
• Transport coefficients of leptons in superconducting neutron star cores
• N-Body Nuclear Forces at Short Distances in Holographic QCD
• Weak response of neutron matter at low momentum transfer
• Thermal conductivity due to phonons in the core of superfluid neutron stars
• Stability of the $\beta$-equilibrated dense matter and core-crust transition in neutron stars
• Constraining nuclear matter parameters from correlation systematics:a mean-field perspective
• Dineutron correlations in quasi two-dimensional systems in a simplified model and possible relation to neutron-rich nuclei
• Parameters of rotating neutron stars with and without hyperons
• Microscopic Study of ${}^1{S}_0$ Superfluidity in Dilute Neutron Matter
• S-pairing in neutron matter. I. Correlated Basis Function Theory
• Local energy-density functional approach to many-body nuclear systems with s-wave pairing
• Surrogate light curve models for kilonovae with comprehensive wind ejecta outflows and parameter estimation for AT2017gfo
• Uniqueness of the Inflationary Higgs Scalar for Neutron Stars and Failure of non-inflationary Approximations
• Dynamical onset of superconductivity and retention of magnetic fields in cooling neutron stars
• Fast cooling and internal heating in hyperon stars
• Rotating hybrid stars with the Dyson-Schwinger quark model
• Cosmological and Astrophysical Probes of Vacuum Energy
• Gravitational waves from isolated neutron stars: mass dependence of r-mode instability
• Implications of latest NICER data for the neutron star equation of state
• A strange star scenario for the formation of isolated millisecond pulsars
• Role of nonlinear vector meson interactions in hyperon stars
• Relativistic hybrid stars with super-strong toroidal magnetic fields: An evolutionary track with QCD phase transition
• Quasi-elastic electron scattering with KIDS nuclear energy density functional
• Modeling Mergers of Known Galactic Systems of Binary Neutron Stars
• Constraining free parameters of a color superconducting non-local Nambu-Jona-Lasinio model using Bayesian analysis of neutron stars mass and radius measurements
• Rearrangement term in the nonlocal folding model of the nucleon optical potential
• Nonradial superfluid modes in oscillating neutron stars
• Three-nucleon forces and superfluidity in neutron matter
• Thermodynamics of Hot Neutron Stars and Universal Relations
• Measuring Masses and Radii of Neutron Stars in Low-Mass X-ray Binaries: Effects of Atmospheric Composition and Touchdown Radius
• Large enhancement of total reaction cross sections at the edge of the island of inversion in Ti, Cr, and Fe isotopes
• Strengthening the bounds on the r-mode amplitude with X-ray observations of millisecond pulsars
• Relativistic r-modes and Shear viscosity: regularizing the continuous spectrum
• Compression of matter in the center of accreting neutron stars
• Neutron skin thickness of ${}^{208}$Pb, ${}^{116,120,124}$Sn, and ${}^{40}$Ca determined from reaction cross sections of ${}^4$He scattering
• Temperature Effects on Core g-modes of Neutron Stars
• The final phase of inspiral of neutron stars: realistic equations of state
• Stability of the mixed phase in hybrid stars
• Embedding short-range correlations in relativistic density functionals through quasi-deuterons
• Three-body forces and Efimov physics in nuclei and atoms
• An Entropy-Area Law for Neutron Stars Near the Black Hole Threshold
• Mean-field calculations of exotic nuclei ground states
• Phenomenological Lambda-Nuclear Interactions
• Fast rotation of neutron stars and equation of state of dense matter
• Dark Stars and Gravitational Waves: Topical Review
• Radial oscillations in neutron stars from QCD
• Observational signatures of neutron stars in low-mass X-ray binaries climbing a stability peak
• The stochastic background of gravitational waves due to the f-mode instability in neutron stars
• Neutrino Electromagnetic Form Factors Effect on the Neutrino Cross Section in Dense Matter
• Prospects of constraining $f(T)$ gravity with the third-generation gravitational-wave detectors
• $R^2$-gravity quark stars from perturbative QCD
• Torsional oscillations of crystalline color-superconducting hybrid stars: Possible sources for Advanced LIGO?
• Properties of Nuclear and Neutron Matter and Thermodynamic Consistency in a Nonlinear Mean-field Approximation
• Recent progresses in strange quark stars
• Improved early warning of compact binary mergers using higher modes of gravitational radiation: A population study
• Novel Scalings of Neutron Star Properties from Analyzing Dimensionless Tolman--Oppenheimer--Volkoff Equations
• Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants
• In medium T matrix for neutron matter
• Finite temperature calculations for the spin polarized asymmetric nuclear matter with the LOCV method
• Constructing Love-Q-Relations with Gravitational Wave Detections
• Evolution of bare quark stars in full general relativity: Single star case
• Isospin Symmetry Breaking Effects on the Properties of Asymmetrical Nuclear Matter and $\beta$-Stable Matter
• Studying the Landau mass parameter of the extended $\sigma$-$\omega$ model for neutron star matter
• Structure formation during phase transitions in strongly interacting matter
• Implications of the measured parameters of PSR J1903+0327 for its progenitor neutron star
• Effect of the $\sigma$-cut potential on the properties of neutron stars with or without a hyperonic core
• "Sloppy" nuclear energy density functionals (II): Finite nuclei
• Ultrarelativistic heavy ion collisions: the first billion seconds
• Low density expansion and isospin dependence of nuclear energy functional: comparison between relativistic and Skyrme models
• Speed of sound bounds and first-order phase transitions in compact stars
• Properties of nuclear matter in relativistic Brueckner-Hartree-Fock model with high-precision charge-dependent potentials
• Quark-Novae in Low-Mass X-ray Binaries with massive neutron stars: A universal model for short-hard Gamma-Ray Bursts
• Gravitational wave asteroseismology limits from low density nuclear matter and perturbative QCD
• Radial and Non-Radial Oscillations of Inverted Hybrid Stars
• The Properties of Matter in White Dwarfs and Neutron Stars
• Leading bounds on micro- to picometer fifth forces from neutron star cooling
• Quark-hadron pasta phase in neutron stars: the role of medium-dependent surface and curvature tensions
• Surface gravity of neutron stars and strange stars
• Nuclear response functions in homogeneous matter with finite range effective interactions
• Spin-polarized neutron matter at different orders of chiral effective field theory
• Linear Response Theory with finite-range interactions
• Compact astrophysical objects in modified gravity
• The entrainment matrix of a superfluid nucleon mixture at finite temperatures
• Baryonic dense matter in view of gravitational-wave observations
• Accretion onto black holes inside neutron stars with piecewise-polytropic equations of state: analytic and numerical treatments
• Tidal Deformability Doppelgangers: Implications of a low-density phase transition in the neutron star equation of state
• Systematic errors due to quasi-universal relations in binary neutron stars and their correction for unbiased model selection
• Hot and dense matter beyond relativistic mean field theory
• Constraints on conformal ultralight dark matter couplings from the European Pulsar Timing Array
• Exploring the QCD phase diagram with compact stars
• Phase separation in low-density neutron matter
• Universal Relations for rapidly rotating neutron stars using supervised machine-learning techniques
• QCD-like phase diagram with Efimov trimers and Cooper pairs in resonantly interacting SU(3) Fermi gases
• Maximum Mass Of Differentially Rotating Strange Quark Stars
• Gravitomagnetic effect in magnetized neutron stars
• Constraining models of twin peak quasi-periodic oscillations with realistic neutron star equations of state
• Quantifying Correlations Between Isovector Observables and the Density Dependence of Nuclear Symmetry Energy away from Saturation Density
• Mean Field Calculation of Thermal Properties of Simple Nucleon Matter on a Lattice
• Constraining Gravity with Eccentric Gravitational Waves: Projected Upper Bounds and Model Selection
• Neutron Star QPOs from Oscillating, Precessing Hot, Thick Flow
• Stability of topological neutron stars
• Scalar Charges and Scaling Relations in Massless Scalar-Tensor Theories
• Mixed configurations of tensor-multi-scalar solitons and neutron stars
• Quark-quark interaction and quark matter in neutron stars
• Dark matter admixed neutron stars with a realistic nuclear equation of state from chiral nuclear interactions
• Detecting dense-matter phase transition signatures in neutron star mass-radius measurements as data anomalies using normalising flows
• Detectability of Sub-Solar Mass Neutron Stars Through a Template Bank Search
• Short-range correlations in asymmetric nuclear matter
• Bridging the gap by shaking superfluid matter
• Neutron stars meet constraints from high and low energy nuclear physics
• Total Energy in Supernova Neutrinos and the Tidal Deformability and Binding Energy of Neutron Stars
• Magnetically supramassive neutron stars
• Equation of State Dependence of Nonlinear Mode-tide Coupling in Coalescing Binary Neutron Stars
• Effects of nuclear matter and composition in core-collapse supernovae and long-term proto-neutron star cooling
• Prospects for optical detections from binary neutron star mergers with the next-generation multi-messenger observatories
• Low-mass X-ray Binaries with Strange Quark Stars
• Inclusive electron scattering in the quasielastic region with Korea-IBS-Daegu-SKKU density functional
• The Effect of Neutron Star Binding Energy on Gravitational-Radiation-Driven Mass-Transfer Binaries
• Constraining Axion Mass through Gamma-ray Observations of Pulsars
• Neutron star pulse profile observations as extreme gravity probes
• Reconstruction of the neutron star equation of state from $w$-quasinormal modes spectra with a piecewise polytropic meshing and refinement method
• Hadron-Quark Phase Transitions in Hyperon Stars
• Pulse profile variability associated with the glitch of PSR J1048$-$5832
• 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
• Supramassive dark objects with neutron star origin
• Criteria for nonlinear parameters of relativistic mean field models
• Bayesian analysis of hybrid neutron star EOS constraints within an instantaneous nonlocal chiral quark matter model
• Neutron Fraction and Neutrino Mean Free Path Predictions in Relativistic Mean Field Models
• Constraints of the variation of fundamental couplings and sensitivity of the equation of state of dense matter
• Spin-orbit correlation energy in neutron matter
• Second look to the Polyakov Loop Nambu-Jona-Lasinio model at finite baryonic density
• The exterior spacetime of relativistic stars in scalar-Gauss-Bonnet gravity
• Toward a systematic strategy for defining power counting in the construction of the energy density functional theory
• On the frequency correlations of low-frequency QPOs with kilohertz QPOs in accreting millisecond X-ray pulsars
• Neutron star structure in a quark model with excluded volume correction
• Premerger phenomena in neutron-star binary coalescences
• Short-range correlations in low-lying nuclear excited states
• Neutron Star Structure in Hořava-Lifshitz Gravity
• Holographic dense QCD in the Veneziano limit
• Reconciling light nuclei and nuclear matter: relativistic $abinitio$ calculations
• Non-radial oscillations and gravitational wave emission of hybrid neutron stars
• Prospects of constraining the dense matter equation of state from the timing analysis of pulsars in double neutron star binaries: the cases of PSR J0737-3039A and PSR J1757-1854
• Signature of hadron-quark crossover in binary-neutron-star mergers
• Phenomenological model of gravitational self-force enhanced tides in inspiralling binary neutron stars
• Standard cooling of rapidly rotating isolated neutron stars in 2D
• Long-term temperature evolution of neutron stars undergoing episodic accretion outbursts
• Application of an ab-initio-inspired energy density functional to nuclei: impact of the effective mass and the slope of the symmetry energy on bulk and surface properties
• Bulk viscosity coefficients due to phonons in superfluid neutron stars
• A tight universal relation between the shape eccentricity and the moment of inertia for rotating neutron stars
• Lee-Yang-inspired energy-density functional including contributions from $p$-wave scattering
• Phase diagram determination at fivefold nuclear compression
• Determination of the internal structure of neutron stars from gravitational wave spectra
• Scales in nuclear matter: Chiral dynamics with pion nucleon form factors
• Constraining Palatini gravity with GR-independent equations of state for neutron stars
• Constraints on kHz QPO models and stellar EOSs from SAX J1808.4-3658, Cyg X-2 and 4U 1820-30
• Hidden symmetry between rotational tidal Love numbers of spinning neutron stars
• Neutron star structure with a new force between quarks
• Breakdown of the tensor component in the Skyrme energy density functional
• Limiting symmetry energy elements from empirical evidence
• Scalar quanta in Fermi liquids: zero sounds, instabilities, Bose condensation, and a metastable state in dilute nuclear matter
• Neutron star matter equation of state including $d^{\ast }$-hexaquark degrees of freedom
• Cost of inferred nuclear parameters towards the f-mode dynamical tide in binary neutron stars
• Neutron Stars in Teleparallel Gravity
• Role of dense matter in tidal deformations of inspiralling neutron stars and in gravitational waveform with unified equations of state
• The power of binary pulsars in testing Gauss-Bonnet gravity
• Neutron Stars and Gravitational Waves: the Key Role of Nuclear Equation of State
• Nuclear matter properties, phenomenological theory of clustering at the nuclear surface, and symmetry energy
• Deep learning inference of the neutron star equation of state
• Crust effects and the cooling relaxation time in highly magnetized neutron stars
• Electron-positron energy deposition rate from neutrino pair annihilation on the rotation axis of neutron and quark stars
• Kilonova constraints for the LIGO/Virgo/KAGRA neutron star merger candidate S250206dm: GW-MMADS observations
• Cosmology and nuclear-physics implications of a subsolar gravitational-wave event
• Nuclear matter with JISP16 NN interaction
• Satisfying the compressibility sum rule in neutron matter
• The optimized point-coupling interaction for the relativistic energy density functional of Hartree-Bogoliubov approach quantifying the nuclear bulk properties
• Influence of the nuclear matter equation of state on the r-mode instability using the finite-range simple effective interaction
• Roles of crust and core in the tidal deformability of neutron stars
• Where Are the r-modes? Chandra Observations of Millisecond Pulsars
• Gravitational waves from glitch-induced f-mode oscillations in quark and neutron stars
• Black hole-neutron star mergers with massive neutron stars in numerical relativity
• High-frequency behavior of w-mode pulsations of compact stars
• The Critical Role of LIGO-India in the Era of Next-Generation Observatories
• Mechanism of r-mode stability in young rapidly rotating pulsars
• Long-period thermal oscillations in superfluid millisecond pulsars
• Spin-polarized low-density neutron matter
• Short distance repulsion in 3 nucleon forces from perturbative QCD
• From nuclear reactions to compact stars: a unified approach
• Prospects for the inference of inertial modes from hypermassive neutron stars with future gravitational-wave detectors
• Follow-up analyses of the binary-neutron-star signals GW170817 and GW190425 by using post-Newtonian waveform models
• Probing the incompressibility of dense hadronic matter near QCD phase transition in relativistic heavy-ion collisions
• Accreting neutron stars from the nuclear energy-density functional theory. II. Equation of state and global properties
• Analyzing the dense matter equation of states in the light of the compact object HESS J1731-347
• Quark-Novae in Neutron Star-White-Dwarf Binaries: A model for luminous (spin-down powered) sub-Chandrasekhar-mass Type Ia Supernovae ?
• Rapidly rotating axisymmetric neutron stars with quark cores
• Implications of Fermionic Dark Matter Interactions on Anisotropic Neutron Stars
• Electron-neutron scattering and transport properties of neutron stars
• When cold, dense quarks in 1+1 and 3+1 dimensions are not a Fermi liquid
• Neutron Stars In $f(R,T)$ Theory: Slow Rotation Approximation
• Probing dark gauge boson with observations from neutron stars
• Generalized Crossover in Interacting Fermions within the Low-Energy Expansion
• Relativistic self-energy decomposition of nuclear symmetry energy and equation of state of neutron matter within QCD sum rules
• Neutron density distribution and neutron skin thickness of ${}^{208}$Pb
• Rotational parameters of strange stars in comparison with neutron stars
• An in-medium chiral power counting for nuclear matter and some applications
• Black hole pulsars and monster shocks as outcomes of black hole--neutron star mergers
• Effects of magnetic field topology in black hole-neutron star mergers: Long-term simulations
• Refinement of the timing-based estimator of pulsar magnetic fields
• Delineating the properties of matter in cold, dense QCD
• Temperature-dependent oscillation modes in rotating superfluid neutron stars
• Ladder resummation of spin 1/2 fermion many-body systems with arbitrary partial-wave content
• Constraints on possible phase transitions above the nuclear saturation density
• Discriminating same-mass Neutron Stars and Black Holes gravitational wave-forms
• Tensor optimized Fermi sphere method for nuclear matter -- power series correlated wave function and a cluster expansion
• Role of isospin physics in supernova matter and neutron stars
• Locating the special point of hybrid neutron stars
• Transport coefficients of magnetized neutron star cores
• Dense Stellar Matter with Strange Quark Matter Driven by Kaon Condensation
• Exploring pathways to forming twin stars
• Bayesian Analysis of Hybrid EoS based on Astrophysical Observational Data
• A brief account of Steven Weinberg's legacy in ab initio many-body theory
• The Auxiliary Field Diffusion Monte Carlo Method for Nuclear Physics and Nuclear Astrophysics
• Probing the physics of newly born magnetars through observation of superluminous supernovae
• Electron-positron energy deposition rate from neutrino pair annihilation in the equatorial plane of rapidly rotating neutron and quark stars
• Resonance suppression of the r-mode instability in superfluid neutron stars: Accounting for muons and entrainment
• Neutron stars with spin polarized self-interacting dark matter
• Strong Gravity Extruding Peaks in Speed of Sound Profiles of Massive Neutron Stars
• Neutron Stars in f(R)-Gravity and Its Extension with a Scalar Axion Field
• Faddeev Calculation of ${}_{\Lambda }^3$H incorporating 2π-exchange $\Lambda$NN Interaction
• Folding model analysis of ${}^{12}C{-}^{12}C$ and ${}^{16}O{-}^{16}O$ elastic scattering using the density-dependent LOCV averaged effective interaction
• The Effect of Quantum Fluctuations in the High-Energy Cold Nuclear Equation of State and in Compact Star Observables
• Anderson-Bogoliubov phonon in inner crust of neutron stars: Dipole excitation in spherical Wigner-Seitz cell
• Crust Cooling Models are Insensitive to the Crust-Core Transition Pressure for Realistic Equations of State
• The impact of hyperons on neutron star mergers: gravitational waves, mass ejection and black hole formation
• One possible mechanism for massive neutron star supported by soft EOS
• Hadron Interactions from lattice QCD
• Revealing Dark Matter's Role in Neutron Stars Anisotropy: A Bayesian Approach Using Multi-messenger Observations
• Simulating neutron stars with a flexible enthalpy-based equation of state parametrization in SpECTRE
• Equation of state of asymmetric nuclear matter and the tidal deformability of neutron star
• The nuclear symmetry energy from relativistic Brueckner-Hartree-Fock model
• Neutrino beaming in ultraluminous X-ray pulsars as a result of gravitational lensing by neutron stars
• Equation of state in neutron stars and supernovae
• Self-consistent Green's functions with three-body forces
• Unifying Nucleon and Quark Dynamics at Finite Baryon Number Density
• Color Ferromagnetic Quark Matter in Neutron Stars
• Optimized Statistical Approach for Comparing Multi-Messenger Neutron Star Data
• The attribute of rotational profile to the hyperon puzzle in the prediction of heaviest compact star
• The role of General Relativity in the evolution of Low Mass X-ray Binaries
• Breaking black-hole uniqueness at supermassive scales
• Equation of state at high densities and modern compact star observations
• Evolution of newborn rapidly rotating magnetars: effects of r-mode and fall-back accretion
• Sign-Problem-Free Nuclear Quantum Monte Carlo Simulation
• Universal relations for quasinormal modes of neutron stars in $R^2$ gravity
• The nuclear symmetry energy and the neutron skin thickness in nuclei
• KIDS density functional for deformed nuclei: Examples of the even-even Nd isotopes
• Relativistic stars in mass-varying massive gravity
• Crust (Unified) Tool for Equation-of-state Reconstruction (CUTER) v2
• Modeling Neutron Star Matter in the Age of Multimessenger Astrophysics
• Hybrid stars and QCD phase transition with a NJL-like model
• From Nuclear to Unnuclear Physics
• Transport coefficients of hyperonic neutron star cores
• Hybrid Stars
• Unraveling Trace Anomaly of Supradense Matter via Neutron Star Compactness Scaling
• Neutron-quark stars: Discerning viable alternatives for the higher-density part of the equation of state of compact stars
• Rotating Neutron Stars with the Relativistic Ab Initio Calculations
• Spin-polarized $\beta$-stable neutron star matter: the nuclear symmetry energy and GW170817 constraint
• Superfluidity of $\Lambda$ hyperons in warm strange hadronic star matter
• Holographic equations of state and astrophysical compact objects
• Merger of a Neutron Star with a Black Hole: one-family vs. two-families scenario
• Superfluid effects on gauging core temperatures of neutron stars in low-mass X-ray binaries
• The hadron-quark phase transition in neutron stars
• Bayesian inference of neutron star crust properties using an ab initio-benchmarked meta-model
• Slowly-Rotating Neutron Stars in Massive Bigravity
• Neutron star structure in an in-medium modified chiral soliton model
• Compact stars in the standard model - and beyond
• The infrared counterpart and proper motion of magnetar SGR0501+4516
• The finite range simple effective interaction including tensor terms
• Which is which? Identification of the two compact objects in gravitational-wave binaries
• Torsional oscillations of magnetized neutron stars with mixed poloidal-toroidal fields
• Partial-wave expansion of $\Lambda NN$ three-baryon interactions in chiral effective field theory
• Mechanisms driving alteration of the Landau state in the vicinity of a second-order phase transition
• Constraining gravity with hadron physics: neutron stars, modified gravity and gravitational waves
• Magnetars From Magnetized Cores Created by a Strong Interaction Phase Transition
• Probing Dark Star Parameters Through $f$-Mode Gravitational Wave Signals
• Thermal effects on nuclear matter properties
• A method for probing the formation of quark matter
• Investigating Time Evolution of Thermal Emission from the Putative Neutron Star in SN 1987A for 50+ Years
• Baryonic matter and the medium modification of the baryon masses
• Effective lagrangian for the macroscopic motion of fermionic matter
• Treating divergence in quark matter by using energy projectors
• Orbital and epicyclic frequencies in massive scalar-tensor theory with self-interaction
• The Lagrangian Numerical Relativity code SPHINCS_BSSN_v1.0
• Neutron Stars: Recent Developments
• Dark I-Love-Q
• Pure Neutron Matter Constraints and Nuclear Symmetry Energy
• Influence of the effective mass on the properties of nuclear matter at finite density and temperature
• Direct nonparametric multimessenger constraints on the equation of state of cold dense nuclear matter
• Moment of Inertia for Axisymmetric Neutron Stars in the Standard-Model Extension
• Different scenarios of topological phase transitions in homogeneous neutron matter
• Neutron stars and the cosmological constant problem
• Density-dependent quark mean-field model for nuclear matter and neutron stars
• Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression
• Deuteron distribution in nuclei and the Levinger's factor
• r-mode instability of neutron stars in low-mass X-ray binaries: effects of Fermi surface depletion and superfluidity of dense matter
• New Skyrme parametrizations to describe finite nuclei and neutron star matter with realistic effective masses
• Test of the string loop oscillation model using kHz quasiperiodic oscillations in a neutron star binary
• Quasi-normal f-modes of anisotropic quark stars in full general relativity
• Neutron star equation of state and tidal deformability with nuclear energy density functionals
• Melting of antikaon condensate in protoneutron stars
• Compact Star Matter: EoS with New Scaling Law
• Slowly rotating topological neutron stars -- universal relations and epicyclic frequencies
• Enforcing causality in nonrelativistic equations of state at finite temperature
• Can we constrain the aftermath of binary neutron star mergers with short gamma-ray bursts?
• Constraining the density dependence of the symmetry energy in the nuclear equation of state using heavy ion beams
• Generalised Inverse-Cowling Approximation for Polar $w$-mode Oscillations of Neutron Stars
• Internal heating and thermal emission from old neutron stars: Constraints on dense-matter and gravitational physics
• Exposing Gravitational Waves below the Quantum Shot Noise
• The nucleardatapy toolkit for simple access to experimental nuclear data, astrophysical observations, and theoretical predictions
• Cooling of the Cassiopeia A neutron star and the effect of diffusive nuclear burning
• Chiral approach to nuclear matter: Role of explicit short-range NN-terms
• ${}^1{S}_0$ pairing for neutrons in dense neutron matter induced by a soft pion
• The Equation of State of Dense Matter : from Nuclear Collisions to Neutron Stars
• Pseudo Nambu-Goldstone modes in neutron stars
• Magneto-elastic torsional oscillations of magnetars
• Finite-temperature infinite matter with effective-field-theory-inspired energy-density functionals
• Observability of dynamical tides in merging eccentric neutron star binaries
• Next-generation global gravitational-wave detector network: Impact of detector orientation on compact binary coalescence and stochastic gravitational-wave background searches
• Neutron Star Radius-to-mass Ratio from Partial Accretion Disc Occultation as Measured through Fe K$\alpha$ Line Profiles
• Solar system tests and neutron stars in $f(R)$ gravity revisited
• New modeling for hybrid stars with an elastic quark core
• Testing merging of Dark Exotic Stars from Gravitational Waves in the Multi-messenger approach
• Distinct Classes of Compact Stars Based On Geometrically Deduced Equations of State
• New Insights into Supradense Matter from Dissecting Scaled Stellar Structure Equations
• A Time Dependent Local Isospin Density Approximation Study of Asymmetric Nuclear Matter
• Neutron star cooling with a dynamic stellar structure
• Probing three-nucleon-force effects via (p,2p) reactions
• Transport properties of superfluid phonons in neutron stars
• Exploring Radial Oscillations in Slow Stable and Hybrid Neutron Stars
• Neutron matter within QCD sum rules
• Selfsimilarity relations for torsional oscillations of neutron stars
• Tests of gravitational scalar polarization and constraints of chameleon $f(R)$ gravity from comprehensive analysis of binary pulsars
• Study of hybrid stars with nonstrange quark matter cores
• Shear viscosity in antikaon condensed matter
• Superfluid dark stars
• Rotational Properties of Inverted Hybrid Stars
• A Strange Star Scenario for the Formation of Eccentric Millisecond Pulsar PSR J1946+3417
• The internal structure of neutron stars and white dwarfs, and the Jacobi virial equation. II
• $M/R$ estimates for two neutron stars in LMXBs with possible r-mode frequencies detected
• Probing Strong Field $f(R)$ Gravity and Ultra-Dense Matter with the Structure and Thermal Evolution of Neutron Stars
• Construction of energy density functional for arbitrary spin polarization using functional renormalization group
• Nucleon Short-Range Correlations and High-Momentum Dynamics: Implications on the Equation of State of Dense Matter
• Equation of State of Hot Neutron Star Matter using Finite Range Simple Effective Interaction
• Suitable resolution for EOS tables in neutron star investigation
• Determination of hadron-quark phase transition line from lattice QCD and two-solar-mass neutron star observations
• Long term evolution of CFS-unstable neutron stars and role of differential rotation on short time-scales
• Detection of simultaneous QPO triplets in 4U 1728-34 and constraining the neutron star mass and moment of inertia
• Love-C relations for elastic hybrid stars
• Role of the Symmetry Energy on the Structure of Neutron Stars with Unified Equations of State
• Strongly interacting matter in extreme magnetic fields
• Nuclear matter calculations with the phenomenological three-nucleon interaction
• Members of the double pulsar system PSR J0737-3039 : neutron stars or strange stars ?
• Spacetime Curvature as a Probe of Exotic Core Phases in Neutron Stars within Modified Gravity
• Effective Field Theories for Neutron Stars Physics
• An effective Nuclear Model: from Nuclear Matter to Finite Nuclei
• Stiffening of matter in quark-hadron continuity: a mini-review
• Dense Hadronic Matter in Neutron Stars
• Neutron Stars, Supernova Explosions and the Transition to Quark Matter
• Superfluid Neutrons in the Core of the Neutron Star in Cassiopeia A
• Application of Kaluza-Klein Theory in Modeling Compact Stars: Exploring Extra Dimensions
• Gravitational-wave model for neutron star merger remnants with supervised learning
• Neutron stars as a dense liquid drop at equilibrium within the effective surface approximation
• Deriving Neutron Star Equation of State from AdS/QCD
• Ferromagnetism of electron gas
• One- and two-argument equation of state parametrizations with continuous sound speed for neutron star simulations
• Pulsar as a Weber detector of gravitational waves and a probe to its internal phase transitions
• Novel halos in light kaonic nuclei as an indicator of nuclear equation of state at supra-normal densities
• Level inversion in kaonic nuclei and the high-density nuclear equation of state
• Early evolution of newly born proto-neutron stars
• Evaluations of uncertainties in simulations of propagation of ultrahigh-energy cosmic-ray nuclei derived from microscopic nuclear models
• Three-Nucleon Forces
• Dilute Nuclear Matter in Chiral Perturbation Theory
• Ab initio calculations on nuclear matter properties including the effects of three-nucleons interaction
• Signal of quark deconfinement in thermal evolution neutron stars with deconfinement heating
• Resonance states below pion-nucleon threshold and their consequences for nuclear systems
• The Role of Strangeness in Astrophysics - an Odyssey through Strange Phases
• Bayesian analysis of multimessenger M-R data with interpolated hybrid EoS
• Probing Fundamental Physics with Gravitational Waves
• Fundamental and higher-order excited modes of radial oscillation of neutron stars for various types of cold nucleonic and hyperonic matter
• Reducing orbital eccentricity in initial data of black hole--neutron star binaries in the puncture framework
• Crust composition and the Shallow Heat Source in KS 1731-260
• Structure and cooling of compact stars
• Thermal Evolution of Neutron Stars as a Probe of Physics beyond the Standard Model
• $f$-mode oscillations of compact stars with realistic equations of state in dynamical spacetime
• Asymmetric nuclear matter : a variational approach
• IGR J17480-2446: a new class of accreting binaries?
• Viscous damping of r-modes and emission of gravitational waves
• Isospin-Asymmetry Dependence of the Thermodynamic Nuclear Equation of State in Many-Body Perturbation Theory
• Hydrostatic equilibrium of causally consistent and dynamically stable neutron star models
• Three-body Force Effects on the Properties of Neutron-rich Nuclear Matter
• Neutron Star Mergers and the Quark Matter Equation of State
• Note on neutron star equation of state in the light of GW170817
• Inferring jet physics from neutron star - black hole mergers with gravitational waves
• XMM-Newton observations of PSR J0554+3107: pulsing thermal emission from a cooling high-mass neutron star
• Star Log-extended eMulation: a method for efficient computation of the Tolman-Oppenheimer-Volkoff equations
• Anisotropic pressure effect on central EOS of PSR J0740+6620 in the light of dimensionless TOV equation
• Phenomenological QCD equations of state for neutron star mergers
• X-ray Timing beyond the Rossi X-ray Timing Explorer
• $\varphi$-modes of neutron stars in a massless scalar-tensor theory
• Neutron stars within relativistic central variational method
• The equation of state of neutron star matter and the symmetry energy
• Relativistic disc line: a tool to constrain neutron star equation of state models
• Properties and microscopic structures of dense stellar matter in RMF models
• Dineutron decay into sterile anti-neutrinos in neutron stars and its observable consequences
• Rapid Hierarchical Inference of Neutron Star Equation of State from multiple Gravitational Wave Observations of Binary Neutron Star Coalescences
• Experimental investigation of ground-state properties of ${}^7$H with transfer reactions
• Accretion-caused deceleration of a gravitationally powerful compact stellar object moving within a dense Fermi gas
• Skyrme-based extrapolation for the static response of neutron matter
• Tunable Fujita-Miyazawa-Type Three-Body Force in Ultracold Atoms
• Gravitational Redshift for Rapidly Rotating Neutron Stars
• Singly heavy baryons in nuclear matter from an SU(3) chiral soliton model
• Estimating the variation of neutron star observables by symmetric dense nuclear matter properties
• Nuclear interactions with modern three-body forces lead to the instability of neutron matter and neutron stars
• I-Love irrotationally
• Theoretical constraints on properties of low-mass neutron stars from EOS of inner crust matters
• Exploring the Strongly-Interacting Regime of Effective Multi-Body Interactions in a Trapped Ultracold Atom System
• Neutron matter at the interface(s): static response and effective mass
• Constraining properties of neutron stars with heavy-ion reactions in terrestrial laboratories
• More than the sum of its parts: combining parameterized tests of extreme gravity
• Leading-order nucleon self-energy in relativistic chiral effective field theory
• Correlations in the properties of static and rapidly rotating compact stars
• Neutron stars and supernova explosions in the framework of Landau's theory
• Magnetic amplification in premerger neutron stars through resonance-induced magnetorotational instabilities
• From nuclear structure to neutron stars
• Recent progress on superstrange dynamics
• Isospin Asymmetry in Nuclei, Neutron Stars, and Heavy-Ion Collisions
• Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia
• Constraints from the GW170817 merger event on the nuclear matter equation of state
• Tidal deformations of compact objects and gravitational wave emission
• High-density Skyrmion matter and Neutron Stars
• SU(2) Chiral Sigma Model Study of Phase Transition in Hybrid Stars
• ${\Omega }^{-}$ production as a probe of equation of state of dense matter near the QCD phase transition in relativistic heavy-ion collisions
• Cooling of Hybrid Stars with Spin Down Compression
• The EOS of neutron matter and the effect of $\Lambda$ hyperons to neutron star structure
• Interacting quark matter effects on the structure of compact stars
• First detection of X-ray pulsations and spectrum of the high Galactic latitude pulsar PSR J0837-2454 and direct Urca cooling implications
• General relativistic magnetohydrodynamics simulations for binary neutron star mergers
• Relativistic Corrections to the CBF Effective Nuclear Hamiltonian
• Non-linear saturation of gravito-inertial modes excited by tidal resonances in binary neutron stars
• Inferring neutron star properties through gravitational waves from r-modes and their relativistic counterparts
• Finite particle-number description of symmetric nuclear matter with spin excitations of high-momentum pairs induced by tensor force
• The effect of multiple extra dimensions on the maximal mass of compact stars in Kaluza-Klein space-time
• Maximal mass of the neutron star with a deconfined quark core
• Neutron stars as extreme gravity probes
• Effects of light-mass fermionic dark matter on the equilibrium and stability of white dwarfs
• Is The Trace Anomaly at its Minimum Value at Neutron Star Centers?
• Quantum Monte Carlo study of inhomogeneous neutron matter
• Axial $w$-modes of anisotropic neutron stars
• Rapidly Rotating Neutron Star Collapse in Massive Scalar-Tensor Theories
• Series solutions to the TOV equations
• Illuminating the Mass Gap Through Deep Optical Constraint on a Neutron Star Merger Candidate S250206dm
• Mass-Radius Constraints for 2S 0918-549 from an RXTE Superexpansion Burst: A Direct Cooling-Tail Analysis
• Few-baryon interactions from lattice QCD
• The Golden Era of Neutron Stars: from Hadrons to Quarks
• Constraints on gravitational waves from the 2024 Vela pulsar glitch
• Restrictions to neutron star properties based on twin-peak quasi-periodic oscillations
• Probing millisecond magnetar formation in binary neutron star mergers through X-ray follow-up of gravitational wave alerts
• Neutron star heating vs. HST observations
• Neutron stars can shine a light on elusive lepton-flavor-violating dark matter
• Axion Emission from Proton Cooper Pairs in Neutron Stars
• Primordial black holes versus their impersonators at gravitational wave observatories
• Methods for Estimating Neutron Star Parameters using Multiple Mechanisms for Gravitational Wave Emission Associated with Pulsar Glitches
• Observational bounds on Dark Matter Admixed Neutron Stars from Gravitational Wave Data
• Quark flavors in hot and dense holographic QCD: setup and comparison to data
• Static charged fluid around a massive magnetic dipole
• Neutron Star News and Puzzles
• Spontaneous Scalarization in Scalar-Tensor Theories with Conformal Symmetry as an Attractor
• Inertial modes in stratified rotating neutron stars : An evolutionary description
• Resolving the fastest ejecta from binary Neutron Star mergers: implications for electromagnetic counterparts
• Vanishing Compactness Gap and Fermionic Compact Dark Matter in Hořava-Lifshitz Gravity
• Twin stars: probe of phase transition from hadronic to quark matter
• Examining the possibility of a thick crust in the compact stellar object HESS J1731-347
• Universal Relations for the Increase in the Mass and Radius of a Rotating Neutron Star
• Prospects for detecting and localizing short-duration transient gravitational waves from glitching neutron stars without electromagnetic counterparts
• Neutron Star Equation of State with Nucleon Short-Range Correlations: A Concise Review and Open Issues
• Topological Shell Structures in Neutron Stars: Effects on Equilibrium, Oscillations, and Gravitational-Wave Signatures
• Prospects for distinguishing dynamical tides in inspiralling binary neutron stars with third generation gravitational-wave detectors
• The Influence of Magnetic Field Geometry in Neutron Stars Crustal Oscillations
• Tracing the Trace Anomaly of Dense Matter inside Neutron Stars
• Structural Properties of Magnetized Neutron Stars under f (R, T ) Gravity Framework
• I-Love-Q Relations of Fermion-Boson Stars
• Tidal effect on the gyroscopic precession around a compact star
• Impact of Higher-order Tidal Corrections on the Measurement Accuracy of Neutron Star Tidal Deformability
• Sco X-1 as a continuous gravitational waves source: modelling the secular evolution using MESA
• Gravitational-wave asteroseismology with f-modes from neutron star binaries at the merger phase
• Inferring neutron-star Love-Q relations from gravitational waves in the hierarchical Bayesian framework
• Impact of three-nucleon forces on gravitational wave emission from neutron stars
• SpecGrav -- Detection of Gravitational Waves using Deep Learning
• Detectability of continuous gravitational waves from magnetically deformed neutron stars
• Some properties of doubly-degenerate stars
• Exotic atoms at extremely high magnetic fields: the case of neutron star atmosphere
• Binding energy of compact stars and their non-radial oscillations
• Uncertainty in predicting the stochastic gravitational wave background from compact binary coalescences
• The stochastic gravitational wave background from magnetars
• Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars
• Functional renormalization group study of nuclear and neutron matter
• A Pseudo su(1,1)-Algebraic Deformation of the Cooper-Pair in the su(2)-Algebraic Many-Fermion Model
• SU(3)_f Constraints on Hypernuclear Energy Density Functionals
• Comparative folding-model study of low-energy elastic scattering and fusion of the ${}^{12}$C+${}^{12}$C and ${}^{16}$O+${}^{16}$O systems
• Measurement of 3He analyzing power for p-3He scattering using the polarized 3He target
• Study of Some Aspects of Astronuclear System
• A "Hyperburst" in the MAXI J0556-332 Neutron Star: Evidence for a New Type of Thermonuclear Explosion
• Novae breves from magnetar giant flares: Potential probes of neutron star crusts
• Strongly Interacting Dark Matter admixed Neutron Stars
• Exact solution of equations for proton localization in neutron star matter
• 1122 Hz rotation of XTE J1739-285 as a probe of quark matter in the interior of the neutron star
• Constraining the parameterized neutron star equation of state with astronomical observations
• Many-body correlations in Semiclassical Molecular Dynamics and Skyrme forces for symmetric Nuclear Matter
• Formation of millisecond pulsars - NS initial mass and EOS constraints
• Effective interaction: From nuclear reactions to neutron stars
• Predictions on observing hot holographic quark star with gravitational waves
• Convective stability analysis of massive neutron stars formed in binary mergers
• Impact and detectability of spin-tidal couplings in neutron star inspirals
• Constraints on the Neutron Star Equation of State from GW170817