Gravitational-wave constraints on the neutron-star-matter Equation of State

Abstract

The LIGO/Virgo detection of gravitational waves originating from a neutron-star merger, GW170817, has recently provided new stringent limits on the tidal deformabilities of the stars involved in the collision. Combining this measurement with the existence of two-solar-mass stars, we generate a generic family of neutron-star-matter Equations of State (EoSs) that interpolate between state-of-the-art theoretical results at low and high baryon density. Comparing the results to ones obtained without the tidal-deformability constraint, we witness a dramatic reduction in the family of allowed EoSs. Based on our analysis, we conclude that the maximal radius of a 1.4-solar-mass neutron star is 13.6 km, and that smallest allowed tidal deformability of a similar-mass star is $\Lambda (1.4M_{\odot })=120$.

6 pages, 4 figures; v2: results and discussion updated, version accepted to PRL

References in corpus (26)

• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Shapiro delay measurement of a two solar mass neutron star
• A Massive Pulsar in a Compact Relativistic Binary
• Multi-messenger Observations of a Binary Neutron Star Merger
• Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
• Tidal Love numbers of neutron stars
• Constraining neutron star tidal Love numbers with gravitational wave detectors
• Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source
• The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models
• Constraining the Maximum Mass of Neutron Stars From Multi-Messenger Observations of GW170817
• Using gravitational-wave observations and quasi-universal relations to constrain the maximum mass of neutron stars
• The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Dark Energy Camera Discovery of the Optical Counterpart
• The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. IV. Detection of Near-infrared Signatures of r-process Nucleosynthesis with Gemini-South
• GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations
• Neutron-star radius constraints from GW170817 and future detections
• Cold Quark Matter
• The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. III. Optical and UV Spectra of a Blue Kilonova From Fast Polar Ejecta
• GW170817, General Relativistic Magnetohydrodynamic Simulations, and the Neutron Star Maximum Mass
• Neutron matter at next-to-next-to-next-to-leading order in chiral effective field theory
• The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. V. Rising X-ray Emission from an Off-Axis Jet
• Constraining the Mass and Radius of Neutron Stars in Globular Clusters
• Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra
• Merging Strangeon Stars
• Neutron-star radii based on realistic nuclear interactions
• I-Love-Q Relations for Neutron Stars in dynamical Chern Simons Gravity
• Uniformly rotating, axisymmetric and triaxial quark stars in general relativity

Cited by in corpus (635)

• GW170817: Measurements of Neutron Star Radii and Equation of State
• A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
• GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4M_{\odot }$
• Origin of the Heaviest Elements: the Rapid Neutron-Capture Process
• New constraints on radii and tidal deformabilities of neutron stars from GW170817
• Evidence for quark-matter cores in massive neutron stars
• Binary Neutron Star Mergers: Mass Ejection, Electromagnetic Counterparts and Nucleosynthesis
• Signatures of quark-hadron phase transitions in general-relativistic neutron-star mergers
• Constraining the speed of sound inside neutron stars with chiral effective field theory interactions and observations
• Nonparametric constraints on neutron star matter with existing and upcoming gravitational wave and pulsar observations
• Quarkyonic Matter and Neutron Stars
• A critical examination of constraints on the equation of state of dense matter obtained from GW170817
• Constraining Neutron-Star Matter with Microscopic and Macroscopic Collisions
• A NICER view of PSR J0030+0451: Implications for the dense matter equation of state
• Neutron star tidal deformability and equation of state constraints
• Neutron Stars and the Nuclear Equation of State
• Stellar structure models in modified theories of gravity: lessons and challenges
• Gravitational waves from neutron star mergers and their relation to the nuclear equation of state
• Revisiting the mechanical properties of the nucleon
• Constraining the dense matter equation of state with joint analysis of NICER and LIGO/Virgo measurements
• Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations
• Multimessenger Parameter Estimation of GW170817
• 50 Years of Quantum Chromodynamics
• Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817
• Nonparametric Inference of Neutron Star Composition, Equation of State, and Maximum Mass with GW170817
• Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy
• GW190814: Impact of a 2.6 solar mass neutron star on nucleonic equations of state
• Neutron star tidal deformabilities constrained by nuclear theory and experiment
• Postmerger Gravitational-Wave Signatures of Phase Transitions in Binary Mergers
• Dark Matter Effects On Neutron Star Properties
• Dense Nuclear Matter Equation of State from Heavy-Ion Collisions
• How perturbative QCD constrains the Equation of State at Neutron-Star densities
• Constraining twin stars with GW170817
• Chiral Effective Field Theory and the High-Density Nuclear Equation of State
• A lower bound on the maximum mass if the secondary in GW190814 was once a rapidly spinning neutron star
• Equation of state sensitivities when inferring neutron star and dense matter properties
• Multimessenger constraints for ultra-dense matter
• NNNLO pressure of cold quark matter: leading logarithm
• Strongly interacting matter exhibits deconfined behavior in massive neutron stars
• The electromagnetic counterparts of compact binary mergers
• A General-relativistic Determination of the Threshold Mass to Prompt Collapse in Binary Neutron Star Mergers
• 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
• Tidal deformability with sharp phase transitions in (binary) neutron stars
• Neutron Star Equation of State in light of GW190814
• Revisiting the lower bound on tidal deformability derived by AT 2017gfo
• Perturbative Thermal QCD: Formalism and Applications
• Soft interactions in cold quark matter
• The Multi-Messenger Matrix: the Future of Neutron Star Merger Constraints on the Nuclear Equation of State
• Direct Astrophysical Tests of Chiral Effective Field Theory at Supranuclear Densities
• First observation of an attractive interaction between a proton and a multi-strange baryon
• A long-lived remnant neutron star after GW170817 inferred from its associated kilonova
• Third family of compact stars within a nonlocal chiral quark model equation of state
• Asymmetric Dark Stars and Neutron Star Stability
• Ab-initio QCD calculations impact the inference of the neutron-star-matter equation of state
• On the maximum mass of neutron stars and GW190814
• Extracting Nuclear Symmetry Energies at High Densities from Observations of Neutron Stars and Gravitational Waves
• Constraining the equation of state of high-density cold matter using nuclear and astronomical measurements
• Interpreting Binary Neutron Star Mergers: Describing the Binary Neutron Star Dynamics, Modelling Gravitational Waveforms, and Analyzing Detections
• Beyond second-order convergence in simulations of magnetised binary neutron stars with realistic microphysics
• Relativistic parameterizations of neutron matter and implications for neutron stars
• Are small radii of compact stars ruled out by GW170817/AT2017gfo?
• On the nature of GW190814 and its impact on the understanding of supranuclear matter
• Signals in the tidal deformability for phase transitions in compact stars with constraints from GW170817
• Continuous gravitational waves from neutron stars: current status and prospects
• Bayesian modeling of the nuclear equation of state for neutron star tidal deformabilities and GW170817
• Phases of dense matter in compact stars
• AT2017gfo: Bayesian inference and model selection of multi-component kilonovae and constraints on the neutron star equation of state
• Neutron star equation of state from the quark level in the light of GW170817
• Inferring neutron star properties from GW170817 with universal relations
• Reaching percolation and conformal limits in neutron stars
• The Science of the Einstein Telescope
• Equation of state for hot QCD and compact stars from a mean field approach
• New equations of state constrained by nuclear physics, observations, and QCD calculations of high-density nuclear matter
• Confronting gravitational-wave observations with modern nuclear physics constraints
• On the Deconfinement Phase Transition in Neutron-Star Mergers
• Combining Electromagnetic and Gravitational-Wave Constraints on Neutron-Star Masses and Radii
• Towards asteroseismology of core-collapse supernovae with gravitational-wave observations - II. Spacetime perturbations
• Constraining nuclear matter parameters with GW170817
• Observing the post-merger signal of GW170817-like events with improved gravitational-wave detectors
• Prospects for axion searches with Advanced LIGO through binary mergers
• Cold quark matter at N3LO: soft contributions
• PSR J0030+0451, GW170817 and the nuclear data: joint constraints on equation of state and bulk properties of neutron stars
• Nuclear equation of state for arbitrary proton fraction and temperature based on chiral effective field theory and a Gaussian process emulator
• A Parametrized Equation of State for Neutron Star Matter with Continuous Sound Speed
• Studying strong phase transitions in neutron stars with gravitational waves
• GW190814: Spin and equation of state of a neutron star companion
• Theoretical and Experimental Constraints for the Equation of State of Dense and Hot Matter
• Fast-transient Searches in Real Time with ZTFReST: Identification of Three Optically-discovered Gamma-ray Burst Afterglows and New Constraints on the Kilonova Rate
• A new public code for initial data of unequal-mass, spinning compact-object binaries
• Implications from GW170817 for $\Delta$-isobar admixed hypernuclear compact stars
• Cool baryon and quark matter in holographic QCD
• The tidal deformability of an anisotropic compact star: Implications of GW170817
• Holographic QCD in the Veneziano limit and neutron stars
• Waveform systematics in the gravitational-wave inference of tidal parameters and equation of state from binary neutron star signals
• Constraints on the symmetry energy and its associated parameters from nuclei to neutron stars
• Towards grounding nuclear physics in QCD
• Unified Interacting Quark Matter and its Astrophysical Implications
• The possibility of the secondary object in GW190814 as a neutron star
• Comparing two models for measuring the neutron star equation of state from gravitational-wave signals
• Constraining the neutron star equation of state using multi-band independent measurements of radii and tidal deformabilities
• Spin effects on neutron star fundamental-mode dynamical tides: phenomenology and comparison to numerical simulations
• An updated nuclear-physics and multi-messenger astrophysics framework for binary neutron star mergers
• Hybrid equation of state with pasta phases and third family of compact stars
• Equation-of-state insensitive relations after GW170817
• Relativistic hybrid stars with sequential first-order phase transitions and heavy-baryon envelopes
• Tidal deformability of dressed black holes and tests of ultralight bosons in extended mass ranges
• Tidal Deformability of Dark Matter Admixed Neutron Stars
• Equation of state and speed of sound of isospin-asymmetric QCD on the lattice
• On gravitational echoes from ultracompact exotic stars
• Post-Newtonian spin-tidal couplings for compact binaries
• Twin stars and the stiffness of the nuclear equation of state: ruling out strong phase transitions below $1.7n_0$ with the new NICER radius measurements
• Empirical relations for gravitational-wave asteroseismology of binary neutron star mergers
• What do we learn about vector interactions from GW170817?
• Gravitational Waves from Holographic Neutron Star Mergers
• Bosonic Dark Matter in Light of the NICER Precise Mass-Radius Measurements
• Phase transitions in neutron stars and their links to gravitational waves
• Holographic modeling of nuclear matter and neutron stars
• Holographic compact stars meet gravitational wave constraints
• Impact of the neutron star crust on the tidal polarizability
• Tidal Love numbers of neutron stars in $f(R)$ gravity
• Relativistic hybrid stars in light of the NICER PSR J0740+6620 radius measurement
• Quark-nuclear hybrid equation of state for neutron stars under modern observational constraints
• Gravitational Wave Signal for Quark Matter with Realistic Phase Transition
• Neutron stars in $f(\mathcal{R},\mathcal{T})$ gravity using realistic equations of state in the light of massive pulsars and GW170817
• Hyperonic stars and the symmetry energy
• Perturbative QCD and the Neutron Star Equation of State
• Hybrid and quark star matter based on a non-perturbative equation of state
• Unified weak/strong coupling framework for nuclear matter and neutron stars
• Chiral symmetry restoration by parity doubling and the structure of neutron stars
• Oscillation modes of hybrid stars within the relativistic Cowling approximation
• Constraining strangeness in dense matter with GW170817
• The effects of self-interacting bosonic dark matter on neutron star properties
• Hot quark matter and (proto-) neutron stars
• Measuring the eccentricity of GW170817 and GW190425
• Investigating Signatures of Phase Transitions in Neutron-Star Cores
• Imprints of the nuclear symmetry energy on the tidal deformability of neutron stars
• Waveform systematics for binary neutron star gravitational wave signals: effects of the point-particle baseline and tidal descriptions
• Emergence of microphysical bulk viscosity in binary neutron star post-merger dynamics
• Insights on Skyrme parameters from GW170817
• Neutron star universal relations with microscopic equations of state
• Relevance of tidal effects and post-merger dynamics for binary neutron star parameter estimation
• Tidal deformability and other global parameters of compact stars with strong phase transitions
• Modelling frequency-dependent tidal deformability for environmental black-hole mergers
• GW170817 implications on the frequency and damping time of f-mode oscillations of neutron stars
• Relativistic rotating vector model for X-ray millisecond pulsars
• Lensing of gravitational waves as a probe of compact dark matter
• Uncertainty limits on neutron star radius measurements with gravitational waves
• Multi-messenger and multi-physics Bayesian inference for GW170817 binary neutron star merger
• Equation of state of dense matter in the multimessenger era
• Delineating Effects of Nuclear Symmetry Energy on the Radii and Tidal Polarizabilities of Neutron Stars
• What neutron stars tell about the hadron-quark phase transition: a Bayesian study
• Equation of State of Cold Quark Matter to $O({\alpha }_s^3\ln {\alpha }_s)$
• Impacts of dark matter on the $f$-mode oscillation of hyperon star
• Cooling of Small and Massive Hyperonic Stars
• Updated observing scenarios and multi-messenger implications for the International Gravitational-wave Network's O4 and O5
• Comparing inclination dependent analyses of kilonova transients
• Effects of spin on magnetized binary neutron star mergers and jet launching
• Can a black hole-neutron star merger explain GW170817, AT2017gfo, GRB170817A?
• Ranking Love numbers for the neutron star equation of state: The need for third-generation detectors
• Merger of compact stars in the two-families scenario
• Constraining hadron-quark phase transition parameters within the quark-mean-field model using multimessenger observations of neutron stars
• Building a realistic neutron star from holography
• Speed of sound constraints from tidal deformability of neutron stars
• Analytic I-Love-C relations for realistic neutron stars
• Imposing multi-physics constraints at different densities on the Neutron Star Equation of State
• Constraining the relativistic mean-field model equations of state with gravitational wave observations
• Updated Parameter Estimates for GW190425 Using Astrophysical Arguments and Implications for the Electromagnetic Counterpart
• Binary Neutron Star Merger Simulations with a Calibrated Turbulence Model
• Symmetry energy at supra-saturation densities via the Gravitational Waves from GW170817
• Target of Opportunity Observations of Gravitational Wave Events with Vera C. Rubin Observatory
• Discontinuity gravity modes in hybrid stars: assessing the role of rapid and slow phase conversions
• Finite-temperature Equations of State for Neutron Star Mergers
• Dynamical ejecta and nucleosynthetic yields from eccentric binary neutron-star mergers
• Excluded-volume model for quarkyonic Matter: Three-flavor baryon-quark Mixture
• Horizons: Nuclear Astrophysics in the 2020s and Beyond
• The impact of the crust equation of state on the analysis of GW170817
• New Ideas in Constraining Nuclear Forces
• Multi-physics constraints at different densities to probe nuclear symmetry energy in hyperonic neutron stars
• First-order phase transition from hypernuclear matter to deconfined quark matter obeying new constraints from compact star observations
• Hypernuclear stars from relativistic Hartree-Fock density functional theory
• Universal relation for supernova gravitational waves
• On the minimum radius of very massive neutron stars
• Updated universal relations for tidal deformabilities of neutron stars from phenomenological equations of state
• Axion star collisions with black holes and neutron stars in full 3D numerical relativity
• Numerical-relativity simulations of long-lived remnants of binary neutron star mergers
• Binary neutron star mergers: Effects of spin and post-merger dynamics
• Constraining self-interacting fermionic dark matter in admixed neutron stars using multimessenger astronomy
• Constraints on the hybrid equation of state with a crossover hadron-quark phase transition in the light of GW170817
• New constraints on the nuclear equation of state from the thermal emission of neutron stars in quiescent low-mass X-ray binaries
• Radial Oscillations of Dark Matter admixed Neutron Stars
• GW170817 constraints on the properties of a neutron star in the presence of WIMP dark matter
• Effects of dark matter on the in-spiral properties of the binary neutron stars
• Reconstructing the neutron star equation of state from observational data via automatic differentiation
• Constraining compact star properties with nuclear saturation parameters
• Dense and Hot QCD at Strong Coupling
• Are nuclear matter properties correlated to neutron star observables ?
• Tidal Deformabilities of Neutron Stars in scalar-Gauss-Bonnet Gravity and Their Applications to Multimessenger Tests of Gravity
• Lensed or not lensed: Determining lensing magnifications for binary neutron star mergers from a single detection
• Maximum mass and universal relations of rotating relativistic hybrid hadron-quark stars
• General-relativistic hydrodynamics of non-perfect fluids: 3+1 conservative formulation and application to viscous black-hole accretion
• Rapidly Spinning Compact Stars with Deconfinement Phase Transition
• Do the current astronomical observations exclude the existence of non-strange quark stars?
• On the nature of the mass-gap object in the GW190814 event
• Towards a Unified Quark-Hadron Matter Equation of State for Applications in Astrophysics and Heavy-Ion Collisions
• Strangeons constitute bulk strong matter-- To test using GW170817
• Role of the symmetry energy and the neutron-matter stiffness on the tidal deformability of a neutron star with unified equations of state
• Probing neutron-star matter in the lab: similarities and differences between binary mergers and heavy-ion collisions
• Investigating Dark Matter-Admixed Neutron Stars with NITR Equation of State in Light of PSR J0952-0607
• Constraints on strong phase transitions in neutron stars
• A Neutron Star is born
• The Deconfinement Phase Transition in Proto-Neutron-Star Matter
• Extreme Gravity and Fundamental Physics
• Probing up-down quark matter via gravitational waves
• Dimension dependence of numerical simulations on gravitational waves from protoneutron stars
• Differentially rotating neutron stars in scalar-tensor theories of gravity
• Supermassive Neutron Stars Rule Out Twin Stars
• Probing Quarkyonic Matter in Neutron Stars with the Bayesian Nuclear-Physics Multi-Messenger Astrophysics Framework
• $I-$Love$-C$ relation for an anisotropic neutron star
• Computing Fast and Reliable Gravitational Waveforms of Binary Neutron Star Merger Remnants
• Non-strange quark stars from NJL model with proper-time regularisation
• Magnetised hybrid stars: effects of slow and rapid phase transitions at the quark-hadron interface
• Holographic approach to compact stars and their binary mergers
• Effects of nuclear symmetry energy and equation of state on neutron star properties
• Transport in strongly coupled quark matter
• Tides in merging neutron stars: Consistency of the GW170817 event with experimental data on finite nuclei
• Gravitational wave echoes from strange stars
• Excluded-volume model for quarkyonic matter II: Three-flavor shell-like distribution of baryons in phase space
• Two-moment scheme for general-relativistic radiation hydrodynamics: a systematic description and new applications
• Waveform systematics for binary neutron star gravitational wave signals: Effects of spin, precession, and the observation of electromagnetic counterparts
• Isovector Effects in Neutron Stars, Radii and the GW170817 Constraint
• Neutron star matter with strange interactions in a relativistic quark model
• Anisotropic compact stars: Constraining model parameters to account for physical features of tidal Love numbers
• Neutron star asteroseismology and nuclear saturation parameter
• Studying the onset of deconfinement with multi-messenger astronomy of neutron stars
• Translating neutron star observations to nuclear symmetry energy via artificial neural networks
• Excitation of f-modes during mergers of spinning binary neutron star
• Probing internal dissipative processes of neutron stars with gravitational waves during the inspiral of neutron star binaries
• Neutron stars and the dense matter equation of state: from microscopic theory to macroscopic observations
• Bayesian Inference of the Dense Matter Equation of State built upon Covariant Density Functionals
• Two novel approaches to the hadron-quark mixed phase in compact stars
• Tidal deformations of hybrid stars with sharp phase transitions and elastic crusts
• Constraints on the curvature of nuclear symmetry energy from recent astronomical data within the KIDS framework
• Impact of extreme spins and mass ratios on the post-merger observables of high-mass binary neutron stars
• A model-agnostic analysis of hybrid stars with reactive interfaces
• Neutron star collapse and gravitational waves with a non-convex equation of state
• New constraints on the neutron-star mass and radius relation from terrestrial nuclear experiments
• Constraining the neutron star equation of state using Pulse Profile Modeling
• Future Prospects for Constraining Nuclear Matter Parameters with Gravitational Waves
• R-modes as a New Probe of Dark Matter in Neutron Stars
• Recovering the conformal limit of color superconducting quark matter within a confining density functional approach
• Reanalysis of the binary neutron star mergers GW170817 and GW190425 using numerical-relativity calibrated waveform models
• Spin-Precessing Black Hole Binaries in Dynamical Chern-Simons Gravity
• Holographic Bjorken flow of a hot and dense fluid in the vicinity of a critical point
• The Radius of PSR J0740+6620 from NICER and XMM-Newton Data
• Detection and parameter estimation of binary neutron star merger remnants
• Very long baseline astrometry of PSR J1012+5307 and its implications on alternative theories of gravity
• Isospin asymmetry in holographic baryonic matter
• Empirical constraints on the high-density equation of state from multi-messenger observables
• Differentially rotating strange star in general relativity
• Common-envelope Dynamics of a Stellar-mass Black Hole: General Relativistic Simulations
• GW190814: Circumstantial Evidence for Up-Down Quark Star
• Constraining the nuclear symmetry energy and properties of neutron star from GW170817 by Bayesian analysis
• A Bayesian Approach to Matching Thermonuclear X-ray Burst Observations with Models
• Insights on pion production mechanism and symmetry energy at high density
• Exploring strong-field deviations from general relativity via gravitational waves
• Effect of spin on the inspiral of binary neutron stars
• Constraint on phase transition with the multimessenger data of neutron stars
• Holographic approach to transport in dense QCD matter
• Binary neutron star mergers as a probe of quark-hadron crossover equations of state
• The special point on the hybrid star mass--radius diagram and its multi--messenger implications
• A pitfall of piecewise-polytropic equation of state inference
• Impact of high spins on the ejection of mass in GW170817
• Nuclear and Hybrid Equations of State in Light of the Low-Mass Compact Star in HESS J1731-347
• Probing hybrid stars with gravitational waves via interfacial modes
• Neutron rich matter in heaven and on Earth
• Consistent Skyrme parametrizations constrained by GW170817
• Low-latency gravitational wave alert products and their performance at the time of the fourth LIGO-Virgo-KAGRA observing run
• Quantifying modeling uncertainties when combining multiple gravitational-wave detections from binary neutron star sources
• Relativistic mean field model for ultra-compact low mass neutron star of HESS J1731-347
• Insights on the peak in the speed of sound of ultradense matter
• nEoS: Neutron Star Equation of State from hadron physics alone
• Hybrid stars with sequential phase transitions: the emergence of the g${}_2$ mode
• Radial oscillations of quark stars admixed with dark matter
• Binary White Dwarfs as Laboratories for Extreme Gravity with LISA
• Can the GW190814 secondary component be a bosonic dark matter admixed compact star?
• Parameter estimation for strong phase transitions in supranuclear matter using gravitational-wave astronomy
• Cooling of hypernuclear compact stars: Hartree-Fock models and high-density pairing
• Phase Transitions in Neutron Stars
• Neutron Star Matter as a Relativistic Fermi Liquid
• Resonant Shattering Flares as Multimessenger Probes of the Nuclear Symmetry Energy
• Degeneracy in the inference of phase transitions in the neutron star equation of state from gravitational wave data
• Phenomenological QCD equations of state for neutron star dynamics: Nuclear-2SC continuity and evolving effective couplings
• Constraints on Nuclear Saturation Properties from Terrestrial Experiments and Astrophysical Observations of Neutron Stars
• Systematic biases due to waveform mismodeling in parametrized post-Einsteinian tests of general relativity: The impact of neglecting spin precession and higher modes
• Hybrid neutron stars in the mass-radius diagram
• Relativistic hybrid stars with sequential first-order phase transitions in light of multimessenger constraints
• Impact of bulk viscosity on the post-merger gravitational-wave signal from merging neutron stars
• Two-layer compact stars with crystalline quark matter: Screening effect on the tidal deformability
• A pseudo-conformal structure in dense baryonic matter
• Implementing chiral three-body forces in terms of medium-dependent two-body forces
• Cool quark matter with perturbative quark masses
• Dense Matter in Neutron Stars with eXTP
• Pulse profiles of highly compact pulsars in general relativity
• Gravitational-Wave and X-ray Probes of the Neutron Star Equation of State
• Reconciling multi-messenger constraints with chiral symmetry restoration
• Hadron matter in neutron stars in view of gravitational wave observations
• Optimal neutron-star mass ranges to constrain the equation of state of nuclear matter with electromagnetic and gravitational-wave observations
• 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
• Optimizing Serendipitous Detections of Kilonovae: Cadence and Filter Selection
• Neutron star mass formula with nuclear saturation parameters for asymmetric nuclear matter
• Mass and radius relations of quarkyonic stars using an excluded volume model
• Moment of inertia - mass universal relations for neutron stars in scalar-tensor theory with self-interacting massive scalar field
• Astrophysical aspects of general relativistic mass twin stars
• Constraining a relativistic mean field model using neutron star mass-radius measurements II: Hyperonic models
• Unveiling the correlations of tidal deformability with the nuclear symmetry energy parameters
• Optimizing Cadences with Realistic Light Curve Filtering for Serendipitous Kilonova Discovery with Vera Rubin Observatory
• CREX- and PREX-II-motivated relativistic interactions and their implications for the bulk properties of nuclear matter and neutron stars
• Speed of Sound in Hybrid Stars and the Role of Bag Pressure in the Emergence of Special Points on M-R Variation of Hybrid Stars
• Asymmetric Nuclear Matter and Neutron Star Properties in Relativistic ab initio Theory in the Full Dirac Space
• Astrophysical Implications of Neutron Star Inspiral and Coalescence
• Detecting resonant tidal excitations of Rossby modes in coalescing neutron-star binaries with third-generation gravitational-wave detectors
• Constraining three-nucleon forces with multimessenger data
• Cold Atom Quantum Simulator for Dilute Neutron Matter
• Universal relations for compact stars with heavy baryons
• Nuclear Matter and Neutron Stars from Relativistic Brueckner-Hartree-Fock Theory
• Axial Quasi-Normal Modes of Scalarized Neutron Stars with Realistic Equations of State
• Symmetry energy effect on the secondary component of GW190814 as a neutron star
• A Measurement of the Hubble Constant using Gravitational Waves from the Binary Merger GW190814
• Effects of quark-matter symmetry energy on hadron-quark coexistence in neutron-star matter
• Fluctuations and phases in baryonic matter
• Gravitational wave asteroseismology for low-mass neutron stars
• Bayesian Analysis for Extracting Properties of the Nuclear Equation of State from Observational Data including Tidal Deformability from GW170817
• Cooling of neutron stars in "nuclear medium cooling scenario" with stiff equation of state including hyperons
• Effect of Inner Crust EoS on Neutron star properties
• Relativistic Mean Field Model parameterizations in the light of GW170817, GW190814, and PSR J0740 + 6620
• Neutron star mass-radius constraints using the high-frequency QPOs of GRB 200415A
• Probing the Impact of WIMP Dark Matter on Universal Relations, GW170817 Posterior and Radial Oscillations
• Light curves from highly compact neutron stars with spot size effect
• Radial oscillations of quark stars from perturbative QCD
• GW170817 constraints analyzed with Gogny forces and momentum-dependent interactions
• Tidal Love numbers and approximate universal relations for fermion soliton stars
• Gravitational wave asteroseismology on cooling neutron stars
• Estimating the nuclear saturation parameter via low-mass neutron star asteroseismology
• Efficient parameter inference for gravitational wave signals in the presence of transient noises using temporal and time-spectral fusion normalizing flow
• Tidal Deformability of Neutron Stars with Realistic Nuclear Energy Density Functionals
• Effects of Nuclear Equation of State on Type-I X-ray Bursts: Interpretation of the X-ray Bursts from GS 1826-24
• Central Speed of Sound, Trace Anomaly and Observables of Neutron Stars from Perturbative Analyses of Scaled TOV Equations
• Hybrid star phenomenology from the properties of the special point
• Effects of Hadron-Quark Phase Transitions in Hybrid Stars within the NJL Model
• Neutron Star Mergers Chirp About Vacuum Energy
• Evidence for a multipolar magnetic field in SGR J1745-2900 from X-ray light-curve analysis
• Finding quark content of neutron stars in light of GW170817
• Hyperonic Neutron Star Matter in Light of GW170817
• Quark mean-field model for nuclear matter with or without bag
• BigApple force and its implications to finite nuclei and astrophysical objects
• Neutron star properties with careful parameterization in the (axial)vector meson extended linear sigma model
• Observational constraint from the heaviest pulsar PSR J0952-0607 on the equation of state of dense matter in relativistic mean field model
• Constraining the equation of state of hybrid stars using recent information from multidisciplinary physics
• Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity
• Setting nonperturbative uncertainties on finite-temperature properties of neutron matter
• Evidence for the photoionization absorption edge in a photospheric radius expansion X-ray burst from GRS 1747$-$312 in Terzan 6
• Gravitational-wave Emission from a Primordial Black Hole Inspiraling inside a Compact Star: a Novel Probe for Dense Matter Equation of State
• Non-radial oscillations in anisotropic dark energy stars
• Tidal heating as a direct probe of strangeness inside neutron stars
• Searching for exotic cores with binary neutron star inspirals
• The I-Love-Q Relations for Superfluid Neutron Stars
• Pulsar glitches in a strangeon star model. II. The activity
• The fate of twin stars on the unstable branch: implications for the formation of twin stars
• Mixed phase transition from hypernuclear matter to deconfined quark matter fulfilling mass-radius constraints of neutron stars
• Neutron Stars in Scalar-Tensor Theories: Analytic Scalar Charges and Universal Relations
• Magnetar QPOs and neutron star crust elasticity
• Curvature of the energy per particle in neutron stars
• Numerical modelling of bulk viscosity in neutron stars
• Influence of the treatment of initialization and mean-field potential on the neutron to proton yield ratios
• Rapid pre-merger localization of binary neutron stars in third generation gravitational wave detectors
• Relativistic approach for the determination of nuclear and neutron star properties in consideration of PREX-II results
• Exploring universal characteristics of neutron star matter with relativistic \textit{ab initio} equations of state
• Non-strange quark stars within resummed QCD
• Fundamental physics using the temporal gravitational wave background
• Probing phase transition in neutron stars via the crust-core interfacial mode
• Implications of the fermion vacuum term in the extended SU(3) Quark Meson model on compact stars properties
• Investigating the I-Love-Q and w-mode Universal Relations Using Piecewise Polytropes
• Stiff equation of state for a holographic nuclear matter as instanton gas
• Studies of the equation-of-state of nuclear matter by heavy-ion collisions at intermediate energy in the multi-messenger era
• Tidal deformability and gravitational-wave phase evolution of magnetised compact-star binaries
• Nuclei in Core-Collapse Supernovae Engine
• Core States of Neutron Stars from Anatomizing their Scaled Structure Equations
• Fundamental oscillation modes of scalar bosonic dark stars
• Exploring the ${\Sigma }^{+}p$ interaction by measurements of the correlation function
• The heavier the better: how to constrain mass ratios and spins of high-mass neutron-star mergers
• Bayesian inference of the dense matter equation of state built upon extended Skyrme interactions
• A Bayesian study of quark models in view of recent astrophysical constraints
• Renormalization group improved pressure for cold and dense QCD
• Constraining dense matter physics using f-mode oscillations in neutron stars
• Maximally local two-nucleon interactions at N${}^3$LO in $\Delta$-less chiral effective field theory
• Bulk Strong Matter: the Trinity
• A Detailed Analysis of the Special Points on $M-R$ Solutions of Hybrid (Twin) Stars
• Impacts of symmetry energy slope on the oscillation frequencies of neutron stars with short-range correlation and admixed dark matter
• Constraining nuclear matter parameters from correlation systematics:a mean-field perspective
• Rotating Love: The dynamical tides of spinning Newtonian stars
• Dynamic Scheduling: Target of Opportunity Observations of Gravitational Wave Events
• The Masses of Isolated Neutron Stars Inferred from the Gravitational Redshift Measurements
• Analyzing the speed of sound in neutron star with machine learning
• Universal behavior of compact star based upon gravitational binding energy
• Studying VLOCV twin compact stars with binary mergers
• The Influence of Muons, Pions, and Trapped Neutrinos on Neutron Star Mergers
• Holographic cold dense matter constrained by neutron stars
• Strange magnetars admixed with fermionic dark matter
• Hubble constant and nuclear equation of state from kilonova spectro-photometric light curves
• Quarkyonic matter state of neutron stars
• Increasing the Accuracy of Binary Neutron Star Simulations with an improved Vacuum Treatment
• Merging strangeon stars II: the ejecta and light curves
• Constraint on the radius of five-dimensional dS spacetime with GW170817 and GRB 170817A
• Quasi-normal Modes of Static Spherically Symmetric Black Holes in $f(R)$ Theory
• Constructing Love-Q-Relations with Gravitational Wave Detections
• Accretion-induced collapse to third family compact stars as trigger for eccentric orbits of millisecond pulsars in binaries
• Novel Scalings of Neutron Star Properties from Analyzing Dimensionless Tolman--Oppenheimer--Volkoff Equations
• The Equation of State of Neutron-Rich Matter at Fourth Order of Chiral Effective Field Theory and the Radius of a Medium-Mass Neutron Star
• Spin-polarized neutron matter, the maximum mass of neutron stars, and GW170817
• Constraining neutron star matter from the slope of the mass-radius curves
• Analytical expressions for pulse profile of neutron stars in plasma environments
• Hybrid Stars Built with Density Dependent Models
• $R^2$-gravity quark stars from perturbative QCD
• Evolution of bare quark stars in full general relativity: Single star case
• Charged neutron stars and observational tests of a dark force weaker than gravity
• Holographic QCD and magnetic fields
• Radial oscillations in neutron stars from QCD
• Rotational-tidal phasing of the binary neutron star waveform
• Relativistic correction to the r-mode frequency in light of multi-messenger constraints
• Role of the symmetry energy slope in neutron stars: exploring the model-dependency
• Emergence of new oscillation modes in dark matter admixed neutron stars
• Tidal Deformability of Strange Quark Planets and Strange Dwarfs
• Neutron matter from local chiral effective field theory interactions at large cutoffs
• A mixing interpolation method to mimic pasta phases in compact star matter
• Five-dimensional compact stars in Einstein-Gauss-Bonnet gravity
• Empirical neutron star mass formula based on experimental observables
• The orbital-decay test of general relativity to the 2% level with 6-year VLBA astrometry of the double neutron star PSR J1537+1155
• Shear and interface modes in neutron stars with pasta structures
• A Deeply Bound Dibaryon is Incompatible with Neutron Stars and Supernovae
• Neutron stars and stellar mergers as a laboratory for dense QCD matter
• Degenerate fermionic matter at N${}^3$LO: Quantum Electrodynamics
• Nonparametric Representation of Neutron Star Equation of State Using Variational Autoencoder
• Differentially rotating scalarized neutron stars with realistic post-merger profile
• Shear oscillations in neutron stars and the nuclear symmetry energy
• Effects of Onset of Phase Transition on Binary Neutron Star Mergers
• Hard-core Radius of Nucleons within the Induced Surface Tension Approach
• Estimating the EOS from the measurement of NS radii with 5% accuracy
• Impact of nuclear matter properties on the nucleosynthesis and the kilonova from binary neutron star merger ejecta
• Web application for galaxy-targeted follow-up of electromagnetic counterparts to gravitational wave sources
• Average speed of sound in neutron stars
• Scale symmetry and composition of compact star matter
• Holographic dense QCD in the Veneziano limit
• The study of nonstrange quark stars within a modified NJL model
• Cold and dense perturbative QCD in a very strong magnetic background
• Hybrid star within the framework of a lowest-order constraint variational method
• Properties of quark-matter cores in massive hybrid stars
• Universality in quasinormal modes of neutron stars with quark-hadron crossover
• Consequences of Fine-Tuning for Fifth Force Searches
• On the Role of Muons in Binary Neutron Star Mergers: First Simulations
• Decoding Long-duration Gravitational Waves from Binary Neutron Stars with Machine Learning: Parameter Estimation and Equations of State
• Bayesian analysis of hybrid neutron star EOS constraints within an instantaneous nonlocal chiral quark matter model
• Comprehensive Analysis of Constructing Hybrid Stars with an RG-consistent NJL Model
• Spin-down induced quark-hadron phase transition in cold isolated neutron stars
• Hidden symmetry between rotational tidal Love numbers of spinning neutron stars
• Case for quarkyoniclike matter from a constituent quark model
• Neutron star matter equation of state including $d^{\ast }$-hexaquark degrees of freedom
• High-accuracy high-mass ratio simulations for binary neutron stars and their comparison to existing waveform models
• Neutron Stars and Gravitational Waves: the Key Role of Nuclear Equation of State
• Cost of inferred nuclear parameters towards the f-mode dynamical tide in binary 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
• Asymptotically conformal CFL quark matter within a nonlocal chiral quark model
• Neutron Skins: Weak Elastic Scattering and Neutron Stars
• The rate of iPTF 14gqr like ultra-stripped supernovae and binary evolution leading to double neutron star formation
• Compact Objects in close orbits as Gravitational Wave Sources: Formation Scenarios and Properties
• Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Nucleonic models
• High $p_t$ squeezed-out n/p ratio as a probe of $K_{\mathrm{sym}}$ of the symmetry energy
• Structure and tidal deformability of a hybrid star within the framework of the field correlator method
• An in-medium chiral power counting for nuclear matter and some applications
• When cold, dense quarks in 1+1 and 3+1 dimensions are not a Fermi liquid
• The radius of a typical-mass neutron star and chiral effective field theory
• Investigating the role of nuclear parameters on oscillation modes in hot Neutron Stars
• On the energy budget of the transition of a neutron star into the third family branch
• Constraining the properties of dense matter and neutron stars by combining nuclear physics and gravitational waves from GW170817
• Effect of the crust on neutron star empirical relations
• The Critical Role of LIGO-India in the Era of Next-Generation Observatories
• Confining density functional approach for color superconducting quark matter and mesonic correlations
• Hadron-quark phase transition in neutron star by combining the relativistic Brueckner-Hartree-Fock theory and Dyson-Schwinger equation approach
• Deeper, Wider, Sharper: Next-Generation Ground-Based Gravitational-Wave Observations of Binary Black Holes
• Nuclear-Physics Multi-Messenger Astrophysics Constraints on the Neutron-Star Equation of State: Adding NICER's PSR J0740+6620 Measurement
• The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy
• Neutron star mass formula with nuclear saturation parameters
• Locating the special point of hybrid neutron stars
• Strong Gravity Extruding Peaks in Speed of Sound Profiles of Massive Neutron Stars
• What if the neutron star maximum mass is beyond $\sim 2.3M_{\odot }$?
• A closer look at the Yukawa's interaction from a symmetry group perspective
• Multimessenger signal from phase transition of neutron star to quark star
• Measuring spin in coalescing binaries of neutron stars showing double precursors
• Maximal Mass Neutron Star as a Key to Superdense Matter Physics
• Equation of state in neutron stars and supernovae
• Effect of Scalar Boson on Fermionic Dark Star
• Radius and equation of state constraints from massive neutron stars and GW190814
• From QCD Symmetries to Nuclei and Neutron Stars
• Improved Analytic Love-C Relations for Neutron Stars
• Effects of finite sizes of atomic nuclei on shear modulus and torsional oscillations in neutron stars
• QCD phase transition and equation of state of stellar strong interaction matter via Dyson-Schwinger equation approach
• Equation of state of asymmetric nuclear matter and the tidal deformability of neutron star
• Universal relation involving fundamental modes in two-fluid dark matter admixed neutron stars
• Optimized Statistical Approach for Comparing Multi-Messenger Neutron Star Data
• Investigating magnetically-induced distortions of neutron stars through gamma-ray burst X-ray plateaus
• Dense Baryonic Matter and Strangeness in Neutron Stars
• Unraveling Trace Anomaly of Supradense Matter via Neutron Star Compactness Scaling
• Quark matter symmetry energy effect on equation of state for neutron stars
• Detecting Hyperons in neutron stars -- a machine learning approach
• Rotating Neutron Stars with the Relativistic Ab Initio Calculations
• Bayesian inference of neutron star crust properties using an ab initio-benchmarked meta-model
• Nonradial oscillations of stratified neutron stars with solid crusts: Mode characterization and tidal resonances in coalescing binaries
• Subtleties in constraining gravity theories with mass-radius data
• Phase transition and stiffer core fluid in neutron stars: Effects on stellar configurations, dynamical stability, and tidal deformability
• Observability of dynamical tides in merging eccentric neutron star binaries
• Neutron stars and the cosmological constant problem
• CLAP for modified gravity: scalar instabilities in binary black hole spacetimes
• Tidal dissipation in binary neutron star inspirals from hyperon bulk viscosity: Phase modeling and parameter estimation bias
• Direct nonparametric multimessenger constraints on the equation of state of cold dense nuclear matter
• Equation of State Independent Determination on the Radius of a 1.4 $M_{\odot }$ Neutron Star Using Mass-Radius Measurements
• Maximum mass of hybrid star formed via shock induced phase transition in cold neutron stars
• Conformality and percolation threshold in neutron stars
• Fundamental-mode eigenfrequencies of neutral and charged twin neutron stars
• Finite size effects on the light curves of slowly-rotating neutron stars
• Model-Independent Determination of the Tidal Deformability of a 1.4 $M_{\odot }$ Neutron Star from Gravitational-Wave Measurements
• Investigating the role of nuclear parameters in Neutron Star oscillations: a model comparison
• Comparing strange and non-strange quark stars within resummed QCD at NLO
• Equation of states in the curved spacetime of slowly rotating degenerate stars
• Dense matter equation of state and neutron star properties from nuclear theory and experiment
• Applicability of Relativistic Point-Coupling Models to Neutron Star Physics
• Effects of multidimensional treatment of gravity in simulations on supernova gravitational waves
• Quark deconfinement in compact stars through sexaquark condensation
• Role of the Symmetry Energy on the Structure of Neutron Stars with Unified Equations of State
• Suitable resolution for EOS tables in neutron star investigation
• Study of hybrid stars with nonstrange quark matter cores
• Data-driven approach for modeling the temporal and spectral evolution of kilonova systematic uncertainties
• Gravitational wave asteroseismology of accreting neutron stars in a steady state
• Love-C relations for elastic hybrid stars
• On the impact of non-local gravity on compact stars
• Neutron stars in general relativity and scalar-tensor theory of gravity
• Constraining neutron star properties through parity-violating electron scattering experiments and relativistic point coupling interactions
• Gravitation with modified fluid Lagrangian: Variational principle and an early dark energy model
• New modeling for hybrid stars with an elastic quark core
• Strongly interacting matter in extreme magnetic fields
• Semi Universal relation to understand matter properties at neutron star interiors
• Confronting recent light compact star observations with color-flavor locked quark matter
• Probing Fundamental Physics with Gravitational Waves
• Bayesian analysis of multimessenger M-R data with interpolated hybrid EoS
• Stellar Initial Mass Function (IMF) Probed with Supernova Rates and Neutrino Background: Cosmic Average IMF Slope is $\simeq 2-3$ Similar to the Salpeter IMF
• Sequency Hierarchy Truncation (SeqHT) for Adiabatic State Preparation and Time Evolution in Quantum Simulations
• Constraining the Hadron-Quark Phase Transition Chemical Potential via Astronomical Observation
• Improved Treatment of Bosonic Dark Matter Dynamics in Neutron Stars: Consequences and Constraints
• Level inversion in kaonic nuclei and the high-density nuclear equation of state
• Impact of the relativistic Cowling approximation on shear and interface modes of neutron stars
• Novel features of asymmetric nuclear matter from terrestrial experiments and astrophysical observations of neutron stars
• A holographic study on QCD phase transition and neutron star properties
• Properties of the Object HESS J1731-347 as a Twin Compact Star
• Direct Inference of Nuclear Equation-of-State Parameters from Gravitational-Wave Observations
• $f$-mode oscillations in hot Neutron Stars: Effect of hyperons and neutrino trapping
• Strange Matter
• Thermodynamics of strongly magnetized dense quark matter from hard dense loop perturbation theory
• A metric on the space of neutron star models in general relativity and modified gravity
• Imprints of high-density nuclear symmetry energy on the crustal fraction of neutron star moment of inertia
• Analytic insights on the information content of new observables
• Probing the equation of state of neutron stars with captured primordial black holes
• Correlation between the curvature and some properties of the neutron star
• Astrophysical constraints on the cold equation of state of the strongly interacting matter
• Modification of the universal relation between mass, radius and nonradial $f$-mode oscillation in proto-neutron stars
• Dipole Polarizability of Finite Nuclei as a Probe of Neutron Stars
• Neutron Star Mergers and the Quark Matter Equation of State
• An Online Framework for Fitting Fast Transient Lightcurves
• The mixed phase quark core in massive hybrid stars
• Universal relations between the quasinormal modes of neutron stars and magnetic tidal deformability
• General relativistic calculation of magnetic field and Power loss for a misaligned pulsar
• Detectability of Population III stellar remnants as X-ray binaries from tidal captures in the local Universe
• Fully general-relativistic simulations of isolated and binary strange quark stars
• Projecting the likely importance of weak-interaction-driven bulk viscosity in neutron star mergers
• Early deconfinement of asymptotically conformal color-superconducting quark matter in neutron stars
• Binary neutron star mergers within kaon condensation: GW170817
• Gravitational wave signatures of phase transition from hadronic to quark matter in isolated neutron stars and binaries
• Bayesian inference favors quark matter in neutron star interiors
• Note on neutron star equation of state in the light of GW170817
• ASAS-SN search for optical counterparts of gravitational-wave events from the third observing run of Advanced LIGO/Virgo
• Quark flavors in hot and dense holographic QCD: setup and comparison to data
• Limitations in constraining neutron star radii and nuclear properties from inspiral gravitational wave detections
• Towards asteroseismology of neutron stars with physics-informed neural networks
• Mergers of binary neutron star systems: a multi-messenger revolution
• Effects of the symmetry energy slope on magnetized neutron stars
• Estimation of neutron star mass and radius of FRB 20240114A by identification of crustal oscillations
• Is The Trace Anomaly at its Minimum Value at Neutron Star Centers?
• The role of equation of state on the spin-up of millisecond pulsars
• Fine structure of giant resonances: What can be learned
• The effect of multiple extra dimensions on the maximal mass of compact stars in Kaluza-Klein space-time
• Constraining the Equation of State of Neutron Stars through GRB X-Ray Plateaus
• Instability of holographic cold compact stars with a color superconducting core
• Constraints from the GW170817 merger event on the nuclear matter equation of state
• Challenging theories of gravitation: dark matter, compact objects and gravitational waves
• Interacting quark matter effects on the structure of compact stars
• Identifying the QCD Phase Transitions via the Gravitational Wave Frequency from Supernova Explosion
• Tidal deformations of compact objects and gravitational wave emission
• Effects of a Brueckner-Hartree-Fock-corrected effective mass on speed of sound, conformality, and observables of dark matter-admixed neutron stars
• The $g$-mode frequencies in cold neutron stars and nuclear saturation parameters
• Universality of dual mass-scaled fundamental modes in two-fluid neutron stars with mirror dark matter
• Isentropic thermodynamics across the hadron-quark mixed phase in a two-phase model with a PNJL quark description
• A new class of hybrid EoS with multiple critical endpoints for simulations of supernovae, neutron stars and their mergers
• Impact and detectability of spin-tidal couplings in neutron star inspirals
• Tidal Deformability of Quark Stars with Repulsive Interactions
• Non-perturbative Aspects of Quantum Field Theories from Holography
• Realistic Equations of State Informing Neutron Star Post-Merger Gravitational-Wave Frequencies
• Gravitational waves from deformed neutron stars: mountains and tides
• The nuclear matter density functional under the nucleonic hypothesis
• Constraining Hamiltonians from chiral effective field theory with neutron-star data
• Constraints on the Neutron Star Equation of State from GW170817
• Density functional approach to quark matter with confinement and color superconductivity
• Investigating the mass-ratio dependence of the prompt-collapse threshold with numerical-relativity simulations
• Unified nonparametric equation-of-state inference from the neutron-star crust to perturbative-QCD densities
• Holography in Quark-Gluon Plasma and Neutron Stars
• Combining simulation-based inference and universal relations for precise and accurate neutron star science
• Improving the cold quark-matter pressure via soft interactions at N3LO
• Lattice QCD at nonzero temperature and density
• Examining the possibility of a thick crust in the compact stellar object HESS J1731-347
• What We Have Learned from NICER About Neutron Star Radii
• Towards a novel energy density functional for beyond-mean-field calculations with pairing and deformation
• Properties of H particle-admixed compact star
• Implications of nuclear interaction for nuclear structure and astrophysics within the relativistic mean-field model
• Incorporating a radiative hydrodynamics scheme in the numerical-relativity code BAM
• Massive Neutron Stars and White Dwarfs as Noncommutative Fuzzy Spheres
• Impact of Higher-order Tidal Corrections on the Measurement Accuracy of Neutron Star Tidal Deformability
• In-medium pion dispersion relation and medium correction of $N\pi \leftrightarrow \Delta$ near the threshold energy of pion production
• Early Warning From Eccentric Compact Binaries: Template Initialization And Sub-dominant Mode Effects