GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4M_{\odot }$

Abstract

On 2019 April 25, the LIGO Livingston detector observed a compact binary coalescence with signal-to-noise ratio 12.9. The Virgo detector was also taking data that did not contribute to detection due to a low signal-to-noise ratio, but were used for subsequent parameter estimation. The 90% credible intervals for the component masses range from 1.12 to 2.52 $M_{\odot }$ (1.45 to 1.88 $M_{\odot }$ if we restrict the dimensionless component spin magnitudes to be smaller than 0.05). These mass parameters are consistent with the individual binary components being neutron stars. However, both the source-frame chirp mass $1.44_{-0.02}^{+0.02}{M}_{\odot }$ and the total mass $3.4_{-0.1}^{+0.3}{M}_{\odot }$ of this system are significantly larger than those of any other known binary neutron star system. The possibility that one or both binary components of the system are black holes cannot be ruled out from gravitational-wave data. We discuss possible origins of the system based on its inconsistency with the known Galactic binary neutron star population. Under the assumption that the signal was produced by a binary neutron star coalescence, the local rate of neutron star mergers is updated to $250-2810{\text{Gpc}}^{-3}{\text{yr}}^{-1}$.

arXiv comment24 pages, 19 figures, published in ApJL

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• Realistic Finite-Temperature Effects in Neutron Star Merger Simulations
• Neutron Star Mergers and How to Study Them
• Detection of gravitational-wave signals from binary neutron star mergers using machine learning
• All-sky Search for Continuous Gravitational Waves from Isolated Neutron Stars in the Early O3 LIGO Data
• The landscape of disk outflows from black hole - neutron star mergers
• Self-consistent picture of the mass ejection from a one second-long binary neutron star merger leaving a short-lived remnant in general-relativistic neutrino-radiation magnetohydrodynamic simulation
• A Search for Neutron Star-Black Hole Binary Mergers in the Short Gamma-Ray Burst Population
• First Constraints on Nuclear Coupling of Axionlike Particles from the Binary Neutron Star Gravitational Wave Event GW170817
• Holographic modeling of nuclear matter and neutron stars
• Test for the Origin of Solar Mass Black Holes
• Spectral separation of the stochastic gravitational-wave background for LISA: observing both cosmological and astrophysical backgrounds
• Constraints on the maximum mass of neutron stars with a quark core from GW170817 and NICER PSR J0030+0451 data
• Neutron stars in $f(\mathcal{R},\mathcal{T})$ gravity using realistic equations of state in the light of massive pulsars and GW170817
• Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds
• Broad search for gravitational waves from subsolar-mass binaries through LIGO and Virgo's third observing run
• Constraining black hole mimickers with gravitational wave observations
• The Challenges Ahead for Multimessenger Analyses of Gravitational Waves and Kilonova: a Case Study on GW190425
• GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
• The effects of self-interacting bosonic dark matter on neutron star properties
• Numerical relativity simulations of prompt collapse mergers: threshold mass and phenomenological constraints on neutron star properties after GW170817
• Delta baryons and diquark formation in the cores of neutron stars
• Maximum mass of compact stars from gravitational wave events with finite-temperature equations of state
• Simulations of PBH formation at the QCD epoch and comparison with the GWTC-3 catalog
• Modelling neutron star mountains
• Measuring the eccentricity of GW170817 and GW190425
• SN2019dge: a Helium-rich Ultra-Stripped Envelope Supernova
• Incompleteness Matters Not: Inference of $H_0$ from BBH-galaxy cross-correlations
• Can neutron star mergers alone explain the r-process enrichment of the Milky Way?
• Probing planetary-mass primordial black holes with continuous gravitational waves
• Quasi-universal behaviour of the threshold mass in unequal-mass, spinning binary neutron-star mergers
• Impact of Dynamical Tides on the Reconstruction of the Neutron Star Equation of State
• Listening to the Universe with Next Generation Ground-Based Gravitational-Wave Detectors
• Emergence of microphysical bulk viscosity in binary neutron star post-merger dynamics
• X-Shooting ULLYSES: massive stars at low metallicity. I. Project Description
• Neural networks reconstruction of the dense-matter equation of state from neutron-star parameters
• Constraining the Hubble constant to a precision of about 1% using multi-band dark standard siren detections
• Primordial black holes and secondary gravitational waves from natural inflation
• Detection and Parameter Estimation of Gravitational Waves from Binary Neutron-Star Mergers in Real LIGO Data using Deep Learning
• Rapid Parameter Estimation of Gravitational Waves from Binary Neutron Star Coalescence using Focused Reduced Order Quadrature
• Kilonova Detectability with Wide-Field Instruments
• Black holes in the low mass gap: Implications for gravitational wave observations
• Bayesian analysis of the spin distribution of LIGO/Virgo black holes
• Modelling Double Neutron Stars: Radio and Gravitational Waves
• Uncertainty limits on neutron star radius measurements with gravitational waves
• New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
• High rate of gravitational waves mergers from flyby perturbations of wide black-hole triples in the field
• A brief overview of black hole-neutron star mergers
• Constraints on the time variation of the gravitational constant using gravitational-wave observations of binary neutron stars
• Combined search for anisotropic birefringence in the gravitational-wave transient catalog GWTC-1
• Unified model for the LISA measurements and instrument simulations
• Impact of the equation of state on $f$- and $p$- mode oscillations of neutron stars
• PSR J2222--0137. I. Improved physical parameters for the system
• Impacts of dark matter on the $f$-mode oscillation of hyperon star
• Detecting the anisotropic astrophysical gravitational wave background in the presence of shot noise through cross-correlations
• Possible Causes of False General Relativity Violations in Gravitational Wave Observations
• The effect of $f(R,T)$ modified gravity on mass and radius of pulsar HerX1
• Stellar Evolution in the Disks of Active Galactic Nuclei Produces Rapidly Rotating Massive Stars
• Ranking Love numbers for the neutron star equation of state: The need for third-generation detectors
• Updated observing scenarios and multi-messenger implications for the International Gravitational-wave Network's O4 and O5
• Shock-powered radio precursors of neutron star mergers from accelerating relativistic binary winds
• Short gamma-ray bursts within 200 Mpc
• Constraints on the distance duality relation with standard sirens
• Gravitational wave sources in our Galactic backyard: Predictions for BHBH, BHNS and NSNS binaries detectable with LISA
• Constraining hadron-quark phase transition parameters within the quark-mean-field model using multimessenger observations of neutron stars
• Status and perspectives of Continuous Gravitational Wave searches
• Microscopic equation of state of hot nuclear matter for numerical relativity simulations
• Speed of sound constraints from tidal deformability of neutron stars
• Primordial black holes and secondary gravitational waves from the Higgs field
• Phase Transition Phenomenology with Nonparametric Representations of the Neutron Star Equation of State
• Primordial black holes and scalar induced gravitational waves from the $E$ model with a Gauss-Bonnet term
• Assessing the impact of transient orbital resonances
• Probing the incompressibility of nuclear matter at ultra-high density through the prompt collapse of asymmetric neutron star binaries
• A new spin on LIGO-Virgo binary black holes
• Tests of general relativity in the nonlinear regime: a parametrized plunge-merger-ringdown gravitational waveform model
• Updated Parameter Estimates for GW190425 Using Astrophysical Arguments and Implications for the Electromagnetic Counterpart
• A NICER view of the 1.4 solar-mass edge-on pulsar PSR J0614-3329
• Binary Neutron Star Merger Simulations with a Calibrated Turbulence Model
• Maximum mass cutoff in the neutron star mass distribution and the prospect of forming supramassive objects in the double neutron star mergers
• Generic searches for alternative gravitational wave polarizations with networks of interferometric detectors
• Target of Opportunity Observations of Gravitational Wave Events with Vera C. Rubin Observatory
• Formation and Evolution of Binary Neutron Stars: Mergers and Their Host Galaxies
• Astrophysical constraints on compact objects in 4D Einstein-Gauss-Bonnet gravity
• Multi-physics constraints at different densities to probe nuclear symmetry energy in hyperonic neutron stars
• Gravitational axial perturbations of Schwarzschild-like black holes in dark matter halos
• Gravitational-Wave Implications for the Parity Symmetry of Gravity at GeV Scale
• Massive $\Delta$-resonance admixed hypernuclear stars with anti-kaon condensations
• Bayesian inference of strange star equation of state using the GW170817 and GW190425 data
• Numerical simulation of sky localization for LISA-TAIJI joint observation
• Thermal Effects in Binary Neutron Star Mergers
• Bayesian model-selection of neutron star equation of state using multi-messenger observations
• On the minimum radius of very massive neutron stars
• Gravitational wave detectors with broadband high frequency sensitivity
• Deep-Learning Continuous Gravitational Waves: Multiple detectors and realistic noise
• Compact body in a tidal environment: New types of relativistic Love numbers, and a post-Newtonian operational definition for tidally induced multipole moments
• Neutrino emission from binary neutron star mergers: characterizing light curves and mean energies
• Impact of eccentricity on the gravitational wave searches for binary black holes: High mass case
• Detecting a stochastic gravitational-wave background in the presence of correlated magnetic noise
• Impact of astrophysical binary coalescence timescales on the rate of lensed gravitational wave events
• Kilonova Emission From Black Hole-Neutron Star Mergers. I. Viewing-Angle-Dependent Lightcurves
• Double-peaked inflation model: Scalar induced gravitational waves and primordial-black-hole suppression from primordial non-Gaussianity
• Testing General Relativity with Gravitational Waves: An Overview
• Tidal Love Numbers of Novel and Admixed Celestial Objects
• Constraining self-interacting fermionic dark matter in admixed neutron stars using multimessenger astronomy
• Measuring precession in asymmetric compact binaries
• A scalable random forest regressor for combining neutron-star equation of state measurements: A case study with GW170817 and GW190425
• Constraining scalar-tensor theories by neutron star-balck hole gravitational wave events
• Real-time gravitational-wave inference for binary neutron stars using machine learning
• Effect of data gaps on the detectability and parameter estimation of massive black hole binaries with LISA
• Nonperturbative quark matter equations of state with vector interactions
• Rapidly rotating $\Delta$-resonance-admixed hypernuclear compact stars
• Quiescent and active galactic nuclei as factories of merging compact objects in the era of gravitational-wave astronomy
• The role of supernova convection for the lower mass gap in the isolated binary formation of gravitational wave sources
• Constraining the Kilonova Rate with Zwicky Transient Facility Searches Independent of Gravitational Wave and Short Gamma-ray Burst Triggers
• Multi-messenger Detection Rates and distributions of Binary Neutron Star Mergers and Their Cosmological Implications
• Constraints on the maximum densities of neutron stars from postmerger gravitational waves with third-generation observations
• Targeted Sub-threshold Search for Strongly-lensed Gravitational-wave Events
• Standard-siren cosmology using gravitational waves from binary black holes
• Accretion-Induced Collapse of Neutron Stars in the Disks of Active Galactic Nuclei
• Radius Constraints from Reflection Modeling of Cygnus X-2 with NuSTAR and NICER
• Gravity in the infrared and effective nonlocal models
• Importance nested sampling with normalising flows
• Impact of Rastall gravity on mass, radius and sound speed of the pulsar PSR J0740+6620
• Hierarchical Inference of Binary Neutron Star Mass Distribution and Equation of State with Gravitational Waves
• Astrophysical implications on hyperon couplings and hyperon star properties with relativistic equations of states
• Modelling neutron star mountains in relativity
• Primordial black holes and scalar-induced gravitational waves from the generalized Brans-Dicke theory
• Measuring eccentricity of binary black holes in GWTC-1 by using inspiral-only waveform
• Bayesian nonparametric inference of neutron star equation of state via neural network
• Tight constraints on Einstein-dilation-Gauss-Bonnet gravity from GW190412 and GW190814
• Estimating outflow masses and velocities in merger simulations: impact of r-process heating and neutrino cooling
• Accurate modeling and mitigation of overlapping signals and glitches in gravitational-wave data
• Frequency deviations in universal relations of isolated neutron stars and postmerger remnants
• Strong lensing as a giant telescope to localize the host galaxy of gravitational wave event
• Lensed or not lensed: Determining lensing magnifications for binary neutron star mergers from a single detection
• Gravitational Wave observatories may be able to detect hyperbolic encounters of Black Holes
• Search for gravitational waves from high-mass-ratio compact-binary mergers of stellar mass and sub-solar mass black holes
• Bridging the gap: spectral distortions meet gravitational waves
• A surrogate model for gravitational waveforms of spin-aligned binary black holes with eccentricities
• Gravitational-Wave Signatures from Compact Object Binaries in the Galactic Center
• Validity of common modelling approximations for precessing binary black holes with higher-order modes
• Parameter estimation of stellar-mass black hole binaries with LISA
• Towards the routine use of subdominant harmonics in gravitational-wave inference: re-analysis of GW190412 with generation X waveform models
• Detection of Gravitational Waves Using Bayesian Neural Networks
• Tidal deformations of neutron stars with elastic crusts
• Dynamics of binary black holes in low-mass young star clusters
• Probing Kilonova Ejecta Properties Using a Catalog of Short Gamma-Ray Burst Observations
• Gravitational tuning forks and hierarchical triple systems
• Convolutional neural networks for the detection of the early inspiral of a gravitational-wave signal
• Compact object scalarization with general relativity as a cosmic attractor
• Identifying when Precession can be Measured in Gravitational Waveforms
• Primordial black holes and secondary gravitational waves from chaotic inflation
• Investigating Dark Matter-Admixed Neutron Stars with NITR Equation of State in Light of PSR J0952-0607
• Nuclear physics constraints from binary neutron star mergers in the Einstein Telescope era
• Population properties and multimessenger prospects of neutron star-black hole mergers following GWTC-3
• Dark Matter Effects on the Compact Star Properties
• Analytic models of the spectral properties of gravitational waves from neutron star merger remnants
• A Neutron Star is born
• Pre-merger localization of compact-binary mergers with third generation observatories
• A Late-time Radio Survey of Short GRBs at $z<0.5$: New Constraints on the Remnants of Neutron Star Mergers
• Bimodal black-hole mass distribution and chirp masses of binary black-hole mergers
• $g$-modes of neutron stars with hadron-to-quark crossover transitions
• Implicit correlations within phenomenological parametric models of the neutron star equation of state
• Neutron Stars with Baryon Number Violation, Probing Dark Sectors
• Bayesian Metric Reconstruction with Gravitational Wave Observations
• Heavy double neutron stars: birth, mid-life and death
• Linking the rates of neutron star binaries and short gamma-ray bursts
• Recognizing black holes in gravitational-wave observations: Challenges in telling apart impostors in mass-gap binaries
• Swift-XRT follow-up of gravitational wave triggers during the third aLIGO/Virgo observing run
• Assessing the Readiness of Numerical Relativity for LISA and 3G Detectors
• Searching for the radio remnants of short duration gamma-ray bursts
• Colour-Flavour Locked Quark Stars in Light of the Compact Object in HESS J1731-347 and the GW190814 Event
• Subtracting Compact Binary Foregrounds to Search for Subdominant Gravitational-Wave Backgrounds in Next-Generation Ground-Based Observatories
• Primordial black holes and secondary gravitational waves from string inspired general no-scale supergravity
• Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects
• Third post-Newtonian effective-one-body Hamiltonian in scalar-tensor and Einstein-scalar-Gauss-Bonnet gravity
• MOCCA SURVEY Database I: Binary Black Hole Mergers from Globular Clusters with Intermediate Mass Black Holes
• Impact of the neutron-star deformability on equation of state parameters
• Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift During the LIGO-Virgo Run O3a
• On the diversity of magnetar-driven kilonovae
• Does GW190425 require an alternative formation pathway than a fast-merging channel?
• Radiation hydrodynamics modeling of kilonovae with SNEC
• Probing Quarkyonic Matter in Neutron Stars with the Bayesian Nuclear-Physics Multi-Messenger Astrophysics Framework
• Fast, faithful, frequency-domain effective-one-body waveforms for compact binary coalescences
• Gas Assisted Binary Black Hole Formation in AGN Discs
• Signature of Collective Plasma Effects in Beam-Driven QED Cascades
• Estimating Satellite Orbital Drag During Historical Magnetic Superstorms
• Improved deep learning techniques in gravitational-wave data analysis
• NANOGrav signal and LIGO-Virgo Primordial Black Holes from the Higgs field
• Gravitational-wave Merger Forecasting: Scenarios for the early detection and localization of compact-binary mergers with ground based observatories
• Poking Holes: Looking for Gaps in LIGO/Virgo's Black Hole Population
• Effects of High Density Phase Transitions on Neutron Star Dynamics
• Early warning of coalescing neutron-star and neutron-star-black-hole binaries from nonstationary noise background using neural networks
• Stringent Search for Precursor Emission in Short GRBs from Fermi/GBM data and Physical Implications
• Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): Observations and Analysis from Advanced LIGO/Virgo's Third Observing Run
• Excluded-volume model for quarkyonic matter II: Three-flavor shell-like distribution of baryons in phase space
• New models with independent dynamical torsion and nonmetricity fields
• Distinguishing high-mass binary neutron stars from binary black holes with second- and third-generation gravitational wave observatories
• High accuracy post-Newtonian and numerical relativity comparisons involving higher modes for eccentric binary black holes and a dominant mode eccentric inspiral-merger-ringdown model
• Holographic approach to compact stars and their binary mergers
• Thermodynamical Description of Hot, Rapidly Rotating Neutron Stars, Protoneutron Stars, and Neutron Star Merger Remnants
• A Search for Gravitational Waves from Binary Mergers with a Single Observatory
• Translating neutron star observations to nuclear symmetry energy via artificial neural networks
• New limits on the Lorentz/CPT symmetry through fifty gravitational-wave events
• NuRIA: Numerical Relativity Injection Analysis of spinning binary black hole signals in Advanced LIGO data
• Stochastic gravitational wave background: methods and Implications
• Intensity and anisotropies of the stochastic Gravitational Wave background from merging compact binaries in galaxies
• Toward a unified equation of state for multi-messenger astronomy
• Bayesian Inference of the Dense Matter Equation of State built upon Covariant Density Functionals
• Deep Learning Detection and Classification of Gravitational Waves from Neutron Star-Black Hole Mergers
• The role of core-collapse physics in the observability of black-hole neutron-star mergers as multi-messenger sources
• Gravitational-wave constraints on the GWTC-2 events by measuring the tidal deformability and the spin-induced quadrupole moment
• Relativistic effective action of dynamical gravitomagnetic tides for slowly rotating neutron stars
• Probing internal dissipative processes of neutron stars with gravitational waves during the inspiral of neutron star binaries
• Excitation of f-modes during mergers of spinning binary neutron star
• Cosmography using strongly lensed gravitational waves from binary black holes
• Neutron stars and the dense matter equation of state: from microscopic theory to macroscopic observations
• Prospects for multi-messenger detection of binary neutron star mergers in the fourth LIGO-Virgo-KAGRA observing run
• Tidal deformations of hybrid stars with sharp phase transitions and elastic crusts
• Implementation of advanced Riemann solvers in a neutrino-radiation magnetohydrodynamics code in numerical relativity and its application to a binary neutron star merger
• Search for Continuous Gravitational Waves from the Central Compact Objects in Supernova Remnants Cassiopeia A, Vela Jr. and G347.3-0.5
• On the moment of inertia of PSR J0737-3039 A from LIGO/Virgo and NICER
• Detectability of kilonovae in optical surveys: $post$-$mortem$ examination of the LVC O3 run follow-up
• Algorithm for TDI numerical simulation and sensitivity investigation
• Impact of extreme spins and mass ratios on the post-merger observables of high-mass binary neutron stars
• Dark matter component in hadronic models with short-range correlations
• Constraints on the curvature of nuclear symmetry energy from recent astronomical data within the KIDS framework
• GW241011 and GW241110: Exploring Binary Formation and Fundamental Physics with Asymmetric, High-Spin Black Hole Coalescence
• Comprehensive analysis of the tidal effect in gravitational waves and implication for cosmology
• Bayesian reconstruction of nuclear matter parameters from the equation of state of neutron star matter
• A model-agnostic analysis of hybrid stars with reactive interfaces
• Generalized Rastall's gravity and its effects on compact objects
• Discovery of Three Candidate Magnetar-powered Fast X-ray Transients from Chandra Archival Data
• Reanalysis of the binary neutron star mergers GW170817 and GW190425 using numerical-relativity calibrated waveform models
• Detection and parameter estimation of binary neutron star merger remnants
• Hadron-quark mixed phase in the quark-meson coupling model
• Tidal Love numbers of Proca stars
• Gravitational waves from binary black hole mergers surrounded by scalar field clouds: Numerical simulations and observational implications
• The Radius of PSR J0740+6620 from NICER and XMM-Newton Data
• Quantum nucleation of up-down quark matter and astrophysical implications
• Inferring the neutron star maximum mass and lower mass gap in neutron star-black hole systems with spin
• Multimessenger parameter estimation of GW170817: from jet structure to the Hubble constant
• Effects of Dark Matter on $f$-mode oscillations of Neutron Stars
• A gravitational-wave limit on the Chandrasekhar mass of dark matter
• Probing gravity and growth of structure with gravitational waves and galaxies' peculiar velocity
• Novel Model of an Ultra-stripped Supernova Progenitor of a Double Neutron Star
• Constraining properties of asymmetric dark matter candidates from gravitational-wave observations
• Dynamics of binary black holes in young star clusters: the impact of cluster mass and long-term evolution
• Nearly model-independent constraints on dense matter equation of state in a Bayesian approach
• Inferring the maximum and minimum mass of merging neutron stars with gravitational waves
• Bayesian inference of quark star equation of state using the NICER PSR J0030+0451 data
• Assessing the compact-binary merger candidates reported by the MBTA pipeline in the LIGO-Virgo O3 run: probability of astrophysical origin, classification, and associated uncertainties
• Mock data study for next-generation ground-based detectors: The performance loss of matched filtering due to correlated confusion noise
• Dark particle mass effects on neutron star properties from a short-range correlated hadronic model
• Quasinormal modes in the field of a dyon-like dilatonic black hole
• Discovery of the optical afterglow and host galaxy of short GRB181123B at $z=1.754$: Implications for Delay Time Distributions
• How loud are echoes from exotic compact objects?
• Demographics of neutron stars in young massive and open clusters
• Observing an intermediate mass black hole GW190521 with minimal assumptions
• GW190521 formation via three-body encounters in young massive star clusters
• Gauge transformation of scalar induced tensor perturbation during matter domination
• Systematic analysis of the impacts of symmetry energy parameters on neutron star properties
• Leveraging gravitational-wave memory to distinguish neutron star--black hole binaries from black hole binaries
• Feeble DM-SM Interaction via New Scalar and Vector Mediators in Rotating Neutron Stars
• Probing Crust Meltdown in Inspiraling Binary Neutron Stars
• Spherically symmetric static black holes in Einstein-aether theory
• Final compact remnants in core-collapse supernovae from 20 to 40 $M_{\odot }$: the lower mass gap
• Igniting weak interactions in neutron star postmerger accretion disks
• Probing hybrid stars with gravitational waves via interfacial modes
• Dark matter effects on the properties of neutron stars: compactness and tidal deformability
• Fast ejecta as a potential way to distinguish black holes from neutron stars in high-mass gravitational-wave events
• Constraining accretion efficiency in massive binary stars with LIGO-Virgo black holes
• Properties of the remnant disk and the dynamical ejecta produced in low-mass black hole-neutron star mergers
• Electromagnetic precursor flares from the late inspiral of neutron star binaries
• AT2018kzr: the merger of an oxygen-neon white dwarf and a neutron star or black hole
• Stochastic Gravitational Wave Background and Eccentric Stellar Compact Binaries
• Correlations of r-Process Elements in Very Metal-Poor Stars as Clues to their Nucleosynthesis Sites
• Constraining the density dependence of the symmetry energy with nuclear data and astronomical observations in the KIDS framework
• Waltzing binaries: Probing line-of-sight acceleration of merging compact objects with gravitational waves
• Hybrid stars with sequential phase transitions: the emergence of the g${}_2$ mode
• Parameter estimation for strong phase transitions in supranuclear matter using gravitational-wave astronomy
• Reconnection-powered fast radio transients from coalescing neutron star binaries
• An optimized PyCBC search for gravitational waves from intermediate-mass black hole mergers
• Rapid neutron star cooling triggered by dark matter
• An astrophysically motivated ranking criterion for low-latency electromagnetic follow-up of gravitational wave events
• Interplay of spin-precession and higher harmonics in the parameter estimation of binary black holes
• Stellar Core-Merger-Induced Collapse: New Formation Pathways for Black Holes, Thorne-$\dot{\mathrm{Z}}$ytkow objects, Magnetars and Superluminous Supernovae
• The neutrino gravitational memory from a core collapse supernova: phenomenology and physics potential
• Constraints on the contributions to the observed binary black hole population from individual evolutionary pathways in isolated binary evolution
• Gravitational waves from mountains in newly born millisecond magnetars
• Dark matter effects on the properties of neutron stars: optical radii
• GW190814 follow-up with the optical telescope MeerLICHT
• Resolving the eccentricity of stellar mass binary black holes with next generation ground-based gravitational wave detectors
• Improving significance of binary black hole mergers in Advanced LIGO data using deep learning : Confirmation of GW151216
• Constraint on the ejecta mass for a black hole-neutron star merger event candidate S190814bv
• Axisymmetric models for neutron star merger remnants with realistic thermal and rotational profiles
• Quasi-equilibrium configurations of binary systems of dark matter admixed neutron stars
• Eccentric or circular? A reanalysis of binary black hole gravitational wave events for orbital eccentricity signatures
• GWSkyNet: a real-time classifier for public gravitational-wave candidates
• Sky localization of space-based gravitational wave detectors
• Interpreting the X-ray afterglows of gamma-ray bursts with radiative losses and millisecond magnetars
• Framework for phase transitions between the Maxwell and Gibbs constructions
• A study of the Inspiral-Merger-Ringdown Consistency Test with gravitational-wave signals from compact binaries in eccentric orbits
• Towards establishing the presence or absence of horizons in coalescing binaries of compact objects by using their gravitational wave signals
• Exploring non-singular black holes in gravitational perturbations
• Swift/UVOT follow-up of Gravitational Wave Alerts in the O3 era
• High-energy neutrinos from fallback accretion of binary neutron star merger remnants
• Relativistic hybrid stars with sequential first-order phase transitions in light of multimessenger constraints
• Spin effects in Spherical Harmonic Modes of Gravitational Waves from Eccentric Compact Binary Inspirals
• Inference of the neutron star equation of state from cosmological distances
• Hadron-quark Pasta Phase in Massive Neutron Stars
• Observation of eccentric binary black hole mergers with second and third generation gravitational wave detector networks
• Beyond the linear tide: impact of the non-linear tidal response of neutron stars on gravitational waveforms from binary inspirals
• Echoes from braneworld wormholes
• Rotating dark matter admixed neutron stars
• Spin-orbit effects for compact binaries in scalar-tensor gravity
• Simulating Transient Noise Bursts in LIGO with Generative Adversarial Networks
• Statistical and systematic uncertainties in extracting the source properties of neutron star - black hole binaries with gravitational waves
• Physics-inspired deep learning to characterize the signal manifold of quasi-circular, spinning, non-precessing binary black hole mergers
• The emergence of diffused Gamma-Ray Burst afterglows from the disks of Active Galactic Nuclei
• Identification of Binary Neutron Star Mergers in Gravitational-Wave Data Using YOLO One-Shot Object Detection
• The High Time Resolution Universe Pulsar Survey -- XVII. PSR J1325-6253, a low eccentricity double neutron star system from an ultra-stripped supernova
• Inspiraling double compact object detection and lensing rate -- forecast for DECIGO and B-DECIGO
• Constraints on Phase Transitions in Neutron Star Matter
• Hybrid stars are compatible with recent astrophysical observations
• Impact of natal kicks on merger rates and spin-orbit misalignments of black hole -- neutron star mergers
• Effect of rainbow function on the structural properties of dark energy star
• A new consistent Neutron Star Equation of State from a Generalized Skyrme model
• Implications of the Conformal Constraint on Sound Speed on the Radius of PSR J0952-0607 within Rastall Gravity
• GRB 191019A: a short gamma-ray burst in disguise from the disk of an active galactic nucleus
• Modeling gravitational waves from exotic compact objects
• Structure of Quark Star: A Comparative Analysis of Bayesian Inference and Neural Network Based Modeling
• The Missing Link Between Black Holes in High-Mass X-ray Binaries and Gravitational-Wave Sources: Observational Selection Effects
• Distinguishing double neutron star from neutron star-black hole binary populations with gravitational wave observations
• Hadron-Quark phase transition in the context of GW190814
• A search for radio emission from double-neutron star merger GW190425 using Apertif
• Solution to the hyperon puzzle using dark matter
• The Green Bank North Celestial Cap Survey. VII. 12 New Pulsar Timing Solutions
• Constraining a relativistic mean field model using neutron star mass-radius measurements II: Hyperonic models
• Eccentric Binary Neutron Star Search Prospects for Cosmic Explorer
• Inspiral gravitational waveforms from compact binary systems in Horndeski gravity
• Cocoon cooling emission in neutron star mergers
• 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
• Unraveling information about supranuclear-dense matter from the complete binary neutron star coalescence process using future gravitational-wave detector networks
• Fallback supernova assembly of heavy binary neutron stars and light black hole-neutron star pairs and the common stellar ancestry of GW190425 and GW200115
• Constraining three-nucleon forces with multimessenger data
• The first five years of gravitational-wave astrophysics
• Determination of the symmetry energy from the neutron star equation of state
• Revisiting time delay interferometry for unequal-arm LISA and TAIJI
• Testing the phase transition parameters inside neutron stars with the production of protons and lambdas in relativistic heavy-ion collisions
• Search for neutrinos in coincidence with gravitational wave events from the LIGO-Virgo O3a Observing Run with the Super-Kamiokande detector
• Distinguishing the nature of ''ambiguous'' merging systems hosting a neutron star: GW190425 in low-latency
• Effect of massive graviton on dark energy star structure
• Electromagnetic Signatures from the Tidal Tail of a Black Hole - Neutron Star Merger
• Detecting resonant tidal excitations of Rossby modes in coalescing neutron-star binaries with third-generation gravitational-wave detectors
• Implications of comprehensive nuclear and astrophysics data on the equations of state of neutron star matter
• Addressing the challenges of detecting time-overlapping compact binary coalescences
• Periodic orbits and gravitational wave radiation in short hair black hole spacetimes for an extreme mass ratio system
• Detecting the stochastic gravitational wave background with the TianQin detector
• Gravitational waves and mass ejecta from binary neutron star mergers: Effect of the spin orientation
• Molecular Chemistry for Dark Matter II: Recombination, Molecule Formation, and Halo Mass Function in Atomic Dark Matter
• Formation and Evolution of Ultraluminous X-ray Pulsar Binaries to Pulsar-Neutron Star and Pulsar-White Dwarf Systems
• Population inference of spin-induced quadrupole moments as a probe for non-black hole compact binaries
• Searching for New Physics in Ultradense Environment: a Review on Dark Matter Admixed Neutron Stars
• Rank-3 Moment Closures in General Relativistic Neutrino Transport
• Could a slow stable hybrid star explain the central compact object in HESS~J1731-347?
• Long-Term Simulations of Dynamical Ejecta: Homologous Expansion and Kilonova Properties
• Gravitational-wave inference for eccentric binaries: the argument of periapsis
• Prompt Emission of Gamma-Ray Bursts in the High-density Environment of Active Galactic Nuclei Accretion Disks
• Medium modifications for light and heavy nuclear clusters in simulations of core collapse supernovae -- Impact on equation of state and weak interactions
• Utilizing Gaussian mixture models in all-sky searches for short-duration gravitational wave bursts
• X-Shooting ULLYSES: Massive Stars at low metallicity II. DR1: Advanced optical data products for the Magellanic Clouds
• Gravitational wave echoes from interacting quark stars
• "Conserved charges" of the Bondi-Metzner-Sachs algebra in the Brans-Dicke theory
• On the Neutron Star/Black Hole Mass Gap and Black Hole Searches
• Probing the Impact of WIMP Dark Matter on Universal Relations, GW170817 Posterior and Radial Oscillations
• Effect of Inner Crust EoS on Neutron star properties
• Orbital eccentricity in a neutron star - black hole merger
• Gravitational wave probes of particle dark matter: a review
• Neutron Star$-$Neutron Star and Neutron Star$-$Black Hole Mergers: Multiband Observations and Early Warnings
• Applications of machine learning in gravitational wave research with current interferometric detectors
• Clarifying transfer function approximations for the large-scale gravitational wave background in $\Lambda$CDM
• Neutron Star Mergers and Gamma-Ray Bursts: Stripping Model
• Oscillating magnetised hybrid stars under the magnifying glass of multi-messenger observations
• GW170817 and GW190425 as Hybrid Stars of Dark and Nuclear Matters
• Speed of sound and quark confinement inside neutron stars
• Distinguishing binary neutron star from neutron star-black hole mergers with gravitational waves
• A Systematic Exploration of Kilonova Candidates from Neutron Star Mergers During the Third Gravitational Wave Observing Run
• High-accuracy waveforms for black hole-neutron star systems with spinning black holes
• PS15cey and PS17cke: prospective candidates from the Pan-STARRS Search for Kilonovae
• Modelling Populations of Kilonovae
• Parameter constraints on a black hole with Minkowski core through quasiperiodic oscillations
• Hamiltonian for tidal interactions in compact binary systems to next-to-next-to-leading post-Newtonian order
• The most probable host of CHIME FRB 190425A, associated with binary neutron star merger GW190425, and a late-time transient search
• Gravitational wave constraints on planetary-mass primordial black holes using LIGO O3a data
• Galactic wormholes: Geometry, stability, and echoes
• Precision constraints on the neutron star equation of state with third-generation gravitational-wave observatories
• Effects of Nuclear Equation of State on Type-I X-ray Bursts: Interpretation of the X-ray Bursts from GS 1826-24
• Quasi-Normal Modes of Loop Quantum Black Holes Formed from Gravitational Collapse
• Systematic bias due to eccentricity in parameter estimation for merging binary neutron stars
• Multipole moments of compact objects with NUT charge: Theoretical and observational implications
• Constraints on the merging binary neutron star mass distribution and equation of state based on the incidence of jets in the population
• The Gravitational-wave Optical Transient Observer (GOTO)
• Central Speed of Sound, Trace Anomaly and Observables of Neutron Stars from Perturbative Analyses of Scaled TOV Equations
• Compact stellar structures in Weyl geometric gravity
• LISA sources from young massive and open stellar clusters
• Precession and Lense-Thirring effect of hairy Kerr spacetimes
• High-accuracy simulations of highly spinning binary neutron star systems
• Using machine learning to parametrize postmerger signals from binary neutron stars
• Circularly polarized scalar induced gravitational waves from the Chern-Simons modified gravity
• Constraining neutron star properties with a new equation of state insensitive approach
• Neutron star properties with careful parameterization in the (axial)vector meson extended linear sigma model
• Models of binary neutron star remnants with tabulated equations of state
• Post-Newtonian templates for gravitational waves from compact binary inspirals
• A correlation between Ha trough depth and inclination in quiescent X-ray transients: evidence for a low-mass black hole in GRO J0422+32
• Skyrme crystals, nuclear matter and compact stars
• Using Equation of State Constraints to Classify Low-Mass Compact Binary Mergers
• Unified neutron star equations of state calibrated to nuclear properties
• Tidal heating as a direct probe of strangeness inside neutron stars
• A study of the agreement between binary neutron star ejecta models derived from numerical relativity simulations
• Understanding binary neutron star collisions with hypermodels
• Reconstructing Masses of Merging Neutron Stars from Stellar $R$-Process Abundance Signatures
• PyROQ: a Python-based Reduced Order Quadrature Building Code for Fast Gravitational Wave Inference
• Investigating the effect of in-plane spin directions for Precessing BBH systems
• Is GW170817 a Multimessenger Neutron Star-Primordial Black Hole Merger?
• The impact of distant fly-bys on the rate of binary primordial black hole mergers
• Counting on Short Gamma-Ray Bursts: Gravitational-Wave Constraints of Jet Geometry
• Compact star merger events with stars composed of interacting strange quark matter
• Rapid pre-merger localization of binary neutron stars in third generation gravitational wave detectors
• Prospects for probing ultralight primordial black holes using the stochastic gravitational-wave background induced by primordial curvature perturbations
• Massive neutron stars with holographic multiquark cores
• Search for continuous gravitational waves from Fomalhaut b in the second Advanced LIGO observing run with a hidden Markov model
• Masses of double neutron star mergers
• Real-Time Detection of Unmodelled Gravitational-Wave Transients Using Convolutional Neural Networks
• Establishing the significance of continuous gravitational-wave detections from known pulsars
• Rapid model comparison of equations of state from gravitational wave observation of binary neutron star coalescences
• Disc Novae: Thermodynamics of Gas Assisted Binary Black Hole Formation in AGN Discs
• Eclipse Mapping of EXO 0748-676: Evidence for a Massive Neutron Star
• Anisotropic multimessenger signals from black hole neutrino-dominated accretion flows with outflows in binary compact object mergers
• Prospects for kilonova signals in the gravitational-wave era
• Applying the effective-source approach to frequency-domain self-force calculations for eccentric orbits
• Fundamental physics using the temporal gravitational wave background
• Microscopic nuclear equation of state at finite temperature and stellar stability
• Eccentricity signatures in LIGO-Virgo-KAGRA's BNS and NSBH binaries
• Mapping the Outcomes of Stellar Evolution in the Disks of Active Galactic Nuclei
• No static regular black holes in Einstein-complex-scalar-Gauss-Bonnet gravity
• Characterizing Astrophysical Binary Neutron Stars with Gravitational Waves
• Kilonova and Optical Afterglow from Binary Neutron Star Mergers. II. Optimal Search Strategy for Serendipitous Observations and Target-of-opportunity Observations of Gravitational-wave Triggers
• Revisiting the Galactic Double Neutron Star merger and LIGO detection rates
• The potential role of binary neutron star merger afterglows in multimessenger cosmology
• The impact of asymmetric dark matter on the thermal evolution of nucleonic and hyperonic compact stars
• Hybrid Strangeon Stars
• Constraining Delay Time Distribution of Binary Neutron Star Mergers from Host Galaxy Properties
• Speed of sound in dense matter and two families of compact stars
• Quantum Skyrmion crystals and the symmetry energy of dense matter
• GW190521 formation scenarios via relativistic accretion
• Breaking of universal relationships of axial wI-modes in hybrid stars: rapid and slow hadron-quark conversion scenarios
• The Impact of Initial-Final Mass Relations on Black Hole Microlensing
• Localization of Compact Binary Sources with Second Generation Gravitational-wave Interferometer Networks
• Polar Quasinormal Modes of Neutron Stars in Massive Scalar-Tensor Theories
• Electromagnetic Follow-up Observations of Binary Neutron Star Mergers with Early Warnings from Decihertz Gravitational-wave Observatories
• Needle in a Bayes Stack: a Hierarchical Bayesian Method for Constraining the Neutron Star Equation of State with an Ensemble of Binary Neutron Star Post-merger Remnants
• Predicting electromagnetic counterparts using low-latency, gravitational-wave data products
• Odd-parity perturbations of the wormhole-like geometries and quasi-normal modes in Einstein-Æther theory
• Investigating the I-Love-Q and w-mode Universal Relations Using Piecewise Polytropes
• Post-merger chirps from binary black holes as probes of the final black-hole horizon
• Structure formation with primordial black holes: collisional dynamics, binaries, and gravitational waves
• Realistic observing scenarios for the next decade of early warning detection of binary neutron stars
• Gravitational wave constraints on Einstein-æther theory with LIGO/Virgo data
• Properties of neutron star described by a relativistic $abinitio$ model
• Studies of the equation-of-state of nuclear matter by heavy-ion collisions at intermediate energy in the multi-messenger era
• Being Careful with the Field Formation Interpretation of GW190412
• Scalar induced gravitational waves from Chern-Simons gravity during inflation era
• Measuring the Hubble constant with coalescences of binary neutron star and neutron star-black hole: bright sirens \& dark sirens
• Novel exact ultra-compact and ultra-sparse hairy black holes emanating from regular and phantom scalar fields
• Constraining first-order phase transition inside neutron stars with application of Bayesian techniques on PSR J0437-4715 NICER data
• The interplay of astrophysics and nuclear physics in determining the properties of neutron stars
• Lensing rates of gravitational wave signals displaying beat patterns detectable by DECIGO and B-DECIGO
• New gravitational waveform model for precessing binary neutron stars with double-spin effects
• Dynamic Scheduling: Target of Opportunity Observations of Gravitational Wave Events
• Quadratic Rastall Gravity: from low-mass HESS J1731-347 to high-mass PSR J0952-0607 pulsars
• Black Hole Mass Function of Coalescing Binary Black Hole Systems: Is There a Pulsational Pair Instability Mass Cutoff?
• The heavier the better: how to constrain mass ratios and spins of high-mass neutron-star mergers
• Rotating Love: The dynamical tides of spinning Newtonian stars
• The impact of dark matter on tidal signatures in neutron star mergers with Einstein Telescope
• Measuring deviations from the Kerr geometry with black hole ringdown
• Incorporating the weak mixing angle dependence to reconcile the neutron skin measurement on 208Pb by PREX-II
• Analytic properties of electromagnetic field of binary compact stars and electromagnetic precursors to gravitational waves
• Enhancing the sensitivity of transient gravitational wave searches with Gaussian Mixture Models
• The astrophysical odds of GW151216
• Bayesian constraints on covariant density functional equations of state of compact stars with new NICER mass-radius measurements
• Hubble constant and nuclear equation of state from kilonova spectro-photometric light curves
• The birth mass function of neutron stars
• Effects of orbital precession on hyperbolic encounters
• Implications of latest NICER data for the neutron star equation of state
• Strange magnetars admixed with fermionic dark matter
• Entropy-limited higher-order central scheme for neutron star merger simulations
• Mean shift cluster recognition method implementation in the nested sampling algorithm
• Search for eccentric NSBH and BNS mergers in the third observing run of Advanced LIGO and Virgo
• Finding Signs of Life on Earth-like Planets: High-resolution Transmission Spectra of Earth through time around FGKM stars
• The effect of spin mismodeling on gravitational-wave measurements of the binary neutron star mass distribution
• The Influence of Muons, Pions, and Trapped Neutrinos on Neutron Star Mergers
• Is the remnant of GW190425 a strange quark star?
• Studying VLOCV twin compact stars with binary mergers
• Gravitational wave memory of compact binary coalescence in the presence of matter effects
• Constraining properties of neutron star merger outflows with radio observations
• Radial and Non-Radial Oscillations of Inverted Hybrid Stars
• Topology change, emergent symmetries and compact star matter
• What if GW190425 did not produce a black hole promptly?
• Rescaling strange-cluster stars and its implications on gravitational-wave echoes
• Evolution of bare quark stars in full general relativity: Single star case
• Calibrating the binary black hole population in nuclear star clusters through tidal disruption events
• Improved early warning of compact binary mergers using higher modes of gravitational radiation: A population study
• Localization of binary neutron star mergers with a single Cosmic Explorer
• Debiasing Standard Siren Inference of the Hubble Constant with Marginal Neural Ratio Estimation
• Examining the effects of dark matter spikes on eccentric intermediate mass ratio inspirals using N-body simulations
• Hybrid stars with color superconducting cores in an extended FCM model
• Dark Stars and Gravitational Waves: Topical Review
• First eccentric inspiral-merger-ringdown analysis of neutron star-black hole mergers
• Novel Scalings of Neutron Star Properties from Analyzing Dimensionless Tolman--Oppenheimer--Volkoff Equations
• Gray Two-moment Neutrino Transport: Comprehensive Tests and Improvements for Supernova Simulations
• Hierarchical approach to matched filtering using a reduced basis
• Next-to-leading order spin-orbit effects in the equations of motion, energy loss and phase evolution of binaries of compact bodies in the effective field theory approach
• Targeted modeling of GW150914's binary black hole source with dart_board
• Piezo-deformable Mirrors for Active Mode Matching in Advanced LIGO
• Neutron Stars in Modified Teleparallel Gravity
• Constructing Love-Q-Relations with Gravitational Wave Detections
• Nonlinear dynamics of oscillating neutron stars in scalar-tensor gravity
• Neural Simulation-Based Inference of the Neutron Star Equation of State directly from Telescope Spectra
• Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants
• Scalar induced gravitational waves in metric teleparallel gravity with the Nieh-Yan term
• Possible binary neutron star merger history of the primary of GW230529
• Constraints on the dense matter equation of state and neutron star properties from NICER's mass-radius estimate of PSR J0740+6620 and multimessenger observations
• Quark-hadron pasta phase in neutron stars: the role of medium-dependent surface and curvature tensions
• Planetary seismology as a test of modified gravity proposals
• Repeated mergers of black hole binaries: implications for GW190521
• Distinguishing black holes with and without spontaneous scalarization in Einstein-scalar-Gauss-Bonnet theories via optical features
• Probing resonant excitations in exotic compact objects via gravitational waves
• Constraining the ellipticity of new-born magnetar with the observational data of Long gamma-ray bursts
• Evolution of inspiralling neutron star binaries: effects of tidal interactions and orbital eccentricities
• Relativistic correction to the r-mode frequency in light of multi-messenger constraints
• Measuring the Lense-Thirring Orbital Precession and the Neutron Star Moment of Inertia with Pulsars
• Assessment of a new sub-grid model for magneto-hydrodynamical turbulence. I. Magnetorotational instability
• Empirical neutron star mass formula based on experimental observables
• Observational limits on the rate of radiation-driven binary black hole capture events
• Optical follow-up observation for GW event S190510g using Subaru/Hyper Suprime-Cam
• Exploring field-evolution and dynamical-capture coalescing binary black holes in GWTC-3
• Constraint on hybrid stars with gravitational wave events
• Gravitational waves from neutron-star mountains
• Assessing equation of state-independent relations for neutron stars with nonparametric models
• How can LISA probe a population of GW190425-like binary neutron stars in the Milky Way?
• Geometric and thermodynamic characterization of binary neutron star accretion discs
• Searching for MHz Gravitational Waves from Harmonic Sources
• Effect of double spin-precession and higher harmonics on spin-induced quadrupole moment measurements
• Multipole tidal effects in the post-Newtonian gravitational-wave phase of compact binary coalescences
• Establishing connection between neutron star properties and nuclear matter parameters through a comprehensive multivariate analysis
• Fast Multipole Methods for $N$-body Simulations of Collisional Star Systems
• Quasi-universal relations for generalized Skyrme stars
• Long-lived neutron-star remnants from asymmetric binary neutron star mergers: element formation, kilonova signals and gravitational waves
• Baryonic dense matter in view of gravitational-wave observations
• Cosmological implications of the Weyl geometric gravity theory
• Energy-conserving integrator for conservative Hamiltonian systems with ten-dimensional phase space
• Long-duration transient, gravitational-wave search pipeline
• Scalar induced gravitational waves in symmetric teleparallel gravity with a parity-violating term
• Binary Neutron Star Mergers with Missing Electromagnetic Counterparts as Manifestations of Mirror World
• Tidal-heating/viscous dissipation correspondence in black holes and viscous compact objects
• Constraining Quadratic $f(R)$ Gravity from Astrophysical Observations of the Pulsar J0704+6620
• The impact of turbulent mixing on the galactic r-process enrichment by binary neutron star mergers
• How does dark matter affect compact star properties and high density constraints of strongly interacting matter
• Constraining the delay time distribution of compact binary objects from the stochastic gravitational wave background searches
• Bayesian Inverse Problem of Rotating Neutron Stars
• Using gravitational waves to distinguish between neutron stars and black holes in compact binary mergers
• Detectability of Sub-Solar Mass Neutron Stars Through a Template Bank Search
• The failure of the Fisher Matrix when including tidal terms: Considering construction of template banks of tidally deformed binary neutron stars
• Collective plasma effects of electron-positron pairs in beam-driven QED cascades
• Total Energy in Supernova Neutrinos and the Tidal Deformability and Binding Energy of Neutron Stars
• The luminosity functions of kilonovae from binary neutron star mergers under different equation of states
• Gravitational wave peak luminosity model for precessing binary black holes
• Probing modified gravitational-wave propagation through tidal measurements of binary neutron star mergers
• Direct mapping of tidal deformability to the iso-scalar and iso-vector nuclear matter parameters
• Accuracy of estimation of parameters with space-borne gravitational wave observatory
• Quantum Love
• Prospects for optical detections from binary neutron star mergers with the next-generation multi-messenger observatories
• New methods to assess and improve LIGO detector duty cycle
• On the delay times of merging double neutron stars
• Hydrodynamic simulations of black hole evolution in AGN discs I: orbital alignment of highly inclined satellites
• Gamma-ray Diagnostics of r-process Nucleosynthesis in the Remnants of Galactic Binary Neutron-Star Mergers
• Towards a robust and reliable deep learning approach for detection of compact binary mergers in gravitational wave data
• Neural network time-series classifiers for gravitational-wave searches in single-detector periods
• On quasinormal modes in 4D black hole solutions in the model with anisotropic fluid
• Multi-messenger astronomy with INTEGRAL
• Quantum gravity phenomenology at the dawn of the multi-messenger era -- A review
• Possibility of primordial black holes as the source of gravitational wave events in the advanced LIGO detector
• Stringent Tests of Gravity with Highly Relativistic Binary Pulsars in the Era of LISA and SKA
• Black-Hole Neutron Star Simulations with the BAM code: First Tests and Simulations
• Impact of unmodeled eccentricity on the tidal deformability measurement and implications for gravitational wave physics inference
• Population properties of neutron stars in the coalescing compact binaries
• Detweiler's redshift invariant for extended bodies orbiting a Schwarzschild black hole
• Late-time post-merger modeling of a compact binary: effects of relativity, r-process heating, and treatment of transport effects
• Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run
• Length-preserving biconnection gravity and its cosmological implications
• Comparative study of 1D and 2D convolutional neural network models with attribution analysis for gravitational wave detection from compact binary coalescences
• Postmerger multimessenger analysis of binary neutron stars: Effect of the magnetic field strength and topology
• Constraining the lensing of binary neutron stars from their stochastic background
• Superradiant (In)stability, Greybody Radiation, and Quasinormal Modes of Rotating Black Holes in non-linear Maxwell f (R) Gravity
• Gravitational wave modes in matter
• Probe and Prejudice: Classification of compact objects and model comparison using EOS knowledge
• Nuclear pasta and symmetry energy in the relativistic point-coupling model
• Synergies of THESEUS with the large facilities of the 2030s and guest observer opportunities
• Signature of hadron-quark crossover in binary-neutron-star mergers
• Kilonova constraints for the LIGO/Virgo/KAGRA neutron star merger candidate S250206dm: GW-MMADS observations
• Hybrid stars may have an inverted structure
• High-accuracy high-mass ratio simulations for binary neutron stars and their comparison to existing waveform models
• Constraining exotic compact stars composed of bosonic and fermionic dark matter with gravitational wave events
• J-GEM optical and near-infrared follow-up of gravitational wave events during LIGO's and Virgo's third observing run
• Near- and sub-solar-mass naked singularities and black holes from transmutation of white dwarfs
• Deep learning inference of the neutron star equation of state
• Neutron Stars and Gravitational Waves: the Key Role of Nuclear Equation of State
• AsterX: a new open-source GPU-accelerated GRMHD code for dynamical spacetimes
• Hidden symmetry between rotational tidal Love numbers of spinning neutron stars
• Fully general relativistic simulations of rapidly rotating quark stars: Oscillation modes and universal relations
• Cost of inferred nuclear parameters towards the f-mode dynamical tide in binary neutron stars
• A Search for IceCube sub-TeV Neutrinos Correlated with Gravitational-Wave Events Detected By LIGO/Virgo
• Influence of the nuclear symmetry energy slope on observables of compact stars with $\Delta$-admixed hypernuclear matter
• Search for Coincident Gravitational-wave and Fast Radio Burst Events from 4-OGC and the First CHIME/FRB Catalog
• Rapidly spinning dark matter-admixed neutron stars
• Quantum witness and invasiveness of cosmic neutrino measurements
• Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Nucleonic models
• Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis
• Resonant gravitational waves in dynamical Chern-Simons-axion gravity
• Rotating Hybrid Stars with Color-Flavor-Locked Quark Matter
• Source localizations with the network of space-based gravitational wave detectors
• The more accurately the metal-dependent star formation rate is modeled, the larger the predicted excess of binary black hole mergers
• Europium enrichment and hierarchical formation of the Galactic halo
• SAGUARO: Time-domain Infrastructure for the Fourth Gravitational-wave Observing Run and Beyond
• Exploring the nature of ultra-luminous X-ray sources across stellar population ages using detailed binary evolution calculations
• Thermal effects on tidal deformability in the last orbits of an inspiraling binary neutron star system
• Generalized skyrmion crystals with applications to neutron stars
• The Critical Role of LIGO-India in the Era of Next-Generation Observatories
• Magnetic Penrose process in the magnetized Kerr spacetime
• Detection of gravitational wave mixed polarization with single space-based detectors
• Computational Techniques for Parameter Estimation of Gravitational Wave Signals
• Core structures of vortices in Ginzburg-Landau theory for neutron ${}^3{P}_2$ superfluids
• Model-independent discovery prospects for primordial black holes at LIGO
• Crust-core interface and bulk neutron star properties
• Kaon condensation in skyrmion matter and compact stars
• Black hole-neutron star mergers with massive neutron stars in numerical relativity
• Searching for Compact Object Candidates from LAMOST Time-Domain Survey of Four K2 Plates
• Tidal Deformation and Radial Pulsations of Neutron Star with Holographic Multiquark Core
• Stability of hypermassive neutron stars with realistic rotation and entropy profiles
• Strong post-merger gravitational radiation of GW170817-like events
• On the detectability of ultra-compact binary pulsar systems
• Inference of multi-channel r-process element enrichment in the Milky Way using binary neutron star merger observations
• Black Holes merging with Low Mass Gap Objects inside Globular Clusters
• 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
• Classical Love for Quantum Blackholes
• Testing the Paradigm of Nuclear Many-Body Theory
• Slowly Rotating Neutron Star with Holographic Multiquark Core: I-Love-Q Relations
• Observational prospects of double neutrons star mergers and their multi-messenger afterglows: LIGO discovery power, event rates and diversity
• Hunting gravitational wave black holes with microlensing
• General Relativistic Simulations of High-Mass Binary Neutron Star Mergers: rapid formation of low-mass stellar black holes
• Sensitivity of spin-aligned searches for neutron star-black hole systems using future detectors
• Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object
• Multi-messenger observations of double neutron stars in Galactic disk with gravitational and radio waves
• Nuclear-Physics Multi-Messenger Astrophysics Constraints on the Neutron-Star Equation of State: Adding NICER's PSR J0740+6620 Measurement
• Can Two Ultrarelativistic Objects Lose Almost All Their Energy to Gravitational Radiation?
• Sensors and Actuators for the Advanced LIGO+ Upgrade
• Scalar induced gravitational waves in chiral scalar-tensor theory of gravity
• Gravitational Wave Searches for Post-Merger Remnants of GW170817 and GW190425
• A Nuclear Equation of State Inferred from Stellar r-process Abundances
• The GW-Universe Toolbox III: simulating joint observations of gravitational waves and gamma-ray bursts
• Gravitational Wave Signal Extraction Against Non-Stationary Instrumental Noises with Deep Neural Network
• Impact of higher harmonics of gravitational radiation on the population inference of binary black holes
• XKN: a Semi-analytic Framework for the Modelling of Kilonovae
• Alice meets Boojums in neutron stars: vortices penetrating two-flavor quark-hadron continuity
• Strong Gravity Extruding Peaks in Speed of Sound Profiles of Massive Neutron Stars
• Where binary neutron stars merge: predictions from IllustrisTNG
• Proximity effects of vortices in neutron ${}^3{P}_2$ superfluids in neutron stars: Vortex core transitions and covalent bonding of vortex molecules
• Astrophysical Source Classification and Distance Estimation for PyCBC Live
• Accretion spin-up of the massive component in the neutron star stripping model for short gamma-ray bursts
• Waveform systematics in identifying strongly gravitationally lensed gravitational waves: Posterior overlap method
• Spin effects in the phasing formula of eccentric compact binary inspirals up to the third post-Newtonian order
• Distortion of Gravitational-wave Signals by Astrophysical Environments
• The Radius of PSR J0437-4715 from NICER Data
• Prospects for the observation of continuous gravitational waves from spinning neutron stars lensed by the galactic supermassive black hole
• Associating fast radio bursts with compact binary mergers via gravitational lensing
• Search for Postmerger Gravitational Waves from Binary Neutron Star Mergers Using a Matched-filtering Statistic
• Nuclear pasta in hot and dense matter and its influence on the equation of state for astrophysical simulations
• Nonparametric extensions of nuclear equations of state: probing the breakdown scale of relativistic mean-field theory
• Results from the Pan-STARRS Search for Kilonovae: Contamination by Massive Stellar Outbursts
• Discriminating same-mass Neutron Stars and Black Holes gravitational wave-forms
• Inferring kilonova population properties with a hierarchical Bayesian framework I : Non-detection methodology and single-event analyses
• Constraints on Undetected Long-Period Binaries in the Known Pulsar Population
• Optimized Statistical Approach for Comparing Multi-Messenger Neutron Star Data
• Inferring three-nucleon couplings from multi-messenger neutron-star observations
• Color superconductivity under neutron-star conditions at next-to-leading order
• Enhancing search pipelines for short gravitational wave transients with Gaussian mixture modelling
• Mass and radius of the most massive neutron star: The probe of the equation of state and perturbative QCD
• Black Hole Gravitational Potential Enhanced Fallback Accretion onto the Nascent Lighter Compact Object: Tentative Evidence in the O3 Run Data of LIGO/Virgo
• Effect of Magnetic Fields on Urca Rates in Neutron Star Mergers
• Low Mass Naked Singularities from Dark Core Collapse
• Initial Data and Eccentricity Reduction Toolkit for Binary Black Hole Numerical Relativity Waveforms
• Proper Time Observables of General Gravitational Perturbations in Laser Interferometry-based Gravitational Wave Detectors
• Relativistic binary systems in scale-independent energy-momentum squared gravity
• A Possible kilonova powered by magnetic wind from a newborn black hole
• Multi-messenger astronomy with a Southern-Hemisphere gravitational-wave observatory
• Black Hole Mass Function of Coalescing Neutron Star-Black Hole Binary Systems: The Prospect of Reconstruction with the Gravitational Wave Observations
• Modifications to the signal from a gravitational wave event due to a surrounding shell of matter
• Constraints on peculiar velocity distribution of binary black holes using gravitational waves with GWTC-3
• The Sound of Clearing the Throat: Gravitational Waves from a Black Hole Orbiting in a Wormhole Geometry
• Causal Modifications of Gravity and Their Observational Bounds
• Projections of the uncertainty on the compact binary population background using popstock
• Probing Non-classicality of Primordial Gravitational Waves and Magnetic Field Through Quantum Poincare Sphere
• Reissner-Nordström perturbation framework with gravitational wave applications
• The Role of Strong Gravity and the Nuclear Equation of State on Neutron-Star Common-Envelope Accretion
• Simulating neutron stars with a flexible enthalpy-based equation of state parametrization in SpECTRE
• Piecewise frequency model for searches for long-transient gravitational waves from young neutron stars
• Deep Learning for estimating parameters of Gravitational Waves
• Stable Case BB/BC Mass Transfer to Form GW190425-like Massive Binary Neutron Star Mergers
• Strong gravitational lensing effects around rotating regular black holes
• Optimizing the Placement of Numerical Relativity Simulations using a Mismatch Predicting Neural Network
• Universal relations for quasinormal modes of neutron stars in $R^2$ gravity
• Astrophysics with the Laser Interferometer Space Antenna
• Targeted Search for Gravitational Waves from Highly Spinning Light Compact Binaries
• Measuring Mass and Radius of the Maximum-mass Nonrotating Neutron Star
• Probing charge of compact objects with gravitational microlensing of gravitational waves
• Observational Probes of the Neutron Star Equation of State with Hyperons, Bosonic Dark Matter, and Quark Matter
• Inferring small neutron star spins with neutron star-black hole mergers
• Merger of a Neutron Star with a Black Hole: one-family vs. two-families scenario
• Unraveling Trace Anomaly of Supradense Matter via Neutron Star Compactness Scaling
• Gravitational multipole moments for asymptotically de Sitter spacetimes
• Strange stars admixed with dark matter: equiparticle model in a two fluid approach
• Binary Neutron Star Merger Search Pipeline Powered by Deep Learning
• Constraining parameters of coalescing stellar mass binary black hole systems with the Einstein Telescope alone
• Modeling matter(s) in SEOBNRv5THM: Generating fast and accurate effective-one-body waveforms for spin-aligned binary neutron stars
• Hydrodynamic simulations of black hole evolution in AGN discs II: inclination damping for partially embedded satellites
• Eccentricity evolution consistency test to distinguish eccentric gravitational-wave signals from eccentricity mimickers
• Bayesian Analysis of the Neutron Star Equation of State and Model Comparison: Insights from PSR J0437+4715, PSR J0614+3329, and Other Multi-Physics Data
• Towards a unified hadron-quark equation of state for neutron stars within the relativistic mean-field model
• Estimating Hubble Constant with Gravitational Observations: A Concise Review
• Calibrating SPI-ACS/INTEGRAL for gamma-ray bursts and re-estimating energetics of GRB/GW 190425 in gamma-ray range
• The effect of noise artefacts on gravitational-wave searches for neutron star post-merger remnants
• Axisymmetric Hydrodynamics in Numerical Relativity Using a Multipatch Method
• Boson and neutron stars with increased density
• Semianalytical Approach for Sky Localization of Gravitational Waves
• A Common Origin for Low Mass Ratio Events Observed by LIGO and Virgo in the First Half of the Third Observing Run
• Unexpected LIGO events and the Mirror World
• A relativistic compact stellar model of anisotropic quark matter mixed with dark energy
• Average nonlinear dynamics of particles in gravitational pulses: effective Hamiltonian, secular acceleration, and gravitational susceptibility
• Influence of dark matter on the structure of strange quark stars in one-fluid model
• Optimal Gravitational-wave Follow-up Tiling Strategies Using a Genetic Algorithm
• Probing intermediate scale Froggatt-Nielsen models at future gravitational wave observatories
• Investigating the Impact of Higher-Order Phase Transitions in Binary Neutron-Star Mergers
• Mass octupole and current quadrupole corrections to gravitational wave emission from close hyperbolic encounters
• Probing Particle Physics with Gravitational Waves
• Black Hole Merger Rates in AGN: contribution from gas-captured binaries
• Recent LIGO-Virgo discoveries
• Search for Coincident Gravitational Wave and Long Gamma-Ray Bursts from 4-OGC and the Fermi-GBM/Swift-BAT Catalog
• Observability of dynamical tides in merging eccentric neutron star binaries
• Predicting Short-duration GRB Rates in the Advanced LIGO Volume
• Can we constrain the aftermath of binary neutron star mergers with short gamma-ray bursts?
• Influence of Dark Matter on the Magnetized Neutron Star
• Direct nonparametric multimessenger constraints on the equation of state of cold dense nuclear matter
• Neutron stars and the cosmological constant problem
• Comparison and application of different post-Newtonian models for inspiralling stellar-mass binary black holes with space-based GW detectors
• Vetting quark-star models with gravitational waves in the hierarchical Bayesian framework
• FIRST J1419+3940 as the First Observed Radio Flare from a Neutron Star Merger
• Constraint on the equation of state of strange quark star: Perturbative QCD along with a density-dependent bag constant
• Multi-messenger observations in the Einstein Telescope era: binary neutron star and black hole - neutron star mergers
• Quasi-normal f-modes of anisotropic quark stars in full general relativity
• Will Gravitational Waves Discover the First Extra-Galactic Planetary System?
• Black Hole - Neutron Star Binary Mergers: The Imprint of Tidal Deformations and Debris
• Non-Radial Oscillation Modes in Hybrid Stars with Hyperons and Delta Baryons
• Oscillating Magnetized Color Superconducting Quark Stars
• The nucleardatapy toolkit for simple access to experimental nuclear data, astrophysical observations, and theoretical predictions
• GW230814: investigation of a loud gravitational-wave signal observed with a single detector
• Corrections to the gravitational wave phasing
• Comparison of neural network architectures for feature extraction from binary black hole merger waveforms
• Strongly interacting matter in extreme magnetic fields
• Probing black hole `charge' from the binary black hole inspiral
• Optical ultra-stable optical clock cavities as resonant mass gravitational wave detectors in search for new physics
• Neutron Stars in Mimetic Gravity
• The mass, spin and rotational energy of the remnant black holes from compact binary mergers
• Bulge Fossil Fragments as a new population of factories of gravitational wave sources in the Galaxy
• Confronting recent light compact star observations with color-flavor locked quark matter
• X-raying the Birth of Binary Neutron Stars and Neutron Star-Black Hole Binaries
• Properties of compact objects in quadratic non-metricity gravity
• Accretion inside astrophysical objects : Effects of rotation and viscosity
• Dark matter effects in modified teleparallel gravity
• Recent astrophysical observations reproduced by a short-range correlated van der Waals-type model?
• Data-driven approach for modeling the temporal and spectral evolution of kilonova systematic uncertainties
• Wolf-Rayet -- compact object binaries as progenitors of binary compact objects
• New Insights into Supradense Matter from Dissecting Scaled Stellar Structure Equations
• Nucleon Short-Range Correlations and High-Momentum Dynamics: Implications on the Equation of State of Dense Matter
• I-C-Q relations for rapidly rotating stable hybrid stars
• Optimized localization for gravitational-waves from merging binaries
• Cosmology in theories with spontaneous scalarization of neutron stars
• Energy flux and waveform of gravitational wave generated by coalescing slow-spinning binary system in effective one-body theory
• DeepExtractor: Time-domain reconstruction of signals and glitches in gravitational wave data with deep learning
• Constraining the $f$-mode oscillations frequency in Neutron Stars through Universal Relations in the realm of Energy-Momentum Squared Gravity
• Equation of State of Hot Neutron Star Matter using Finite Range Simple Effective Interaction
• Study of nuclear matter properties for Hybrid EoS
• Scalar absorption cross section of rotating black holes with tidal charge
• The origin of the coherent radio flash potentially associated with GRB 201006A
• Status of the Advanced Virgo gravitational-wave detector
• Reducing orbital eccentricity in initial data of black hole--neutron star binaries in the puncture framework
• Obtaining Statistical Significance of Gravitational Wave Signals in Hierarchical Search
• On the role of magnetic fields into the dynamics and gravitational wave emission of binary neutron stars
• Exploring the Potential for Detecting Rotational Instabilities in Binary Neutron Star Merger Remnants with Gravitational Wave Detectors
• Bayesian analysis of multimessenger M-R data with interpolated hybrid EoS
• Event Rate of Fast Radio Burst from Binary Neutron-star Mergers
• Fundamental and higher-order excited modes of radial oscillation of neutron stars for various types of cold nucleonic and hyperonic matter
• Electromagnetic Follow-up to Gravitational Wave Events with the UltraViolet EXplorer (UVEX)
• Leveraging cross-detector parameter consistency measures to enhance sensitivities of gravitational wave searches
• Cosmology with Binary Neutron Stars: Does Mass-Redshift Correlation Matter?
• Insights into Binary Neutron Star Merger Simulations: A Multi-Code Comparison
• Neutron Star with Dark Matter Admixture: A Candidate for Bridging the Mass Gap
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Gravitational Wave Emission from Close-in Strange Quark Planets Around Strange Stars with Magnetic Interactions
• Deriving Neutron Star Equation of State from AdS/QCD
• Quark confinement in an equiparticle quark model: application to stellar matter
• What to expect: kilonova light curve predictions via equation of state marginalization
• Effective Field Theories for Neutron Stars Physics
• Gravitational-wave model for neutron star merger remnants with supervised learning
• Decoupled Quark Stars Relativistic Models in the Regime of Self-interacting Brans-Dicke Gravity
• Gravitational waves from eccentric binary neutron star mergers: Systematic biases and inadequacy of quasicircular templates
• On non-detection of Gamma-Ray Bursts in three compact binary merger events detected by LIGO
• An Interactive Gravitational-Wave Detector Model for Museums and Fairs
• Neutron Star in Quantized-space-time
• All-sky search for long-duration gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run
• Simulating Binary Neutron Star Mergers with Finite-temperature Equations of State: The influences of the slope of the symmetry energy and artificial heating
• First joint observation by the underground gravitational-wave detector, KAGRA, with GEO600
• Probing Fundamental Physics with Gravitational Waves
• Numerical Relativity Estimates of the Remnant Recoil Velocity in Binary Neutron Star Mergers
• Rates and beaming angles of GRBs associated with compact binary coalescences
• The Gravitational-wave Optical Transient Observer (GOTO): prototype performance and prospects for transient science
• Spacetime Curvature as a Probe of Exotic Core Phases in Neutron Stars within Modified Gravity
• An optimal envelope ejection efficiency for merging neutron stars
• Black hole spectroscopy of collapsing and merging neutron stars
• Gravitational wave signals from long lasting binary-single black hole encounters
• A post-Newtonian approach to neutron star oscillations
• Limits on the Stochastic Gravitational Wave Background and Prospects for Single Source Detection with GRACE Follow-On
• A pipeline to search for signatures of line-of-sight acceleration in gravitational wave signals produced by compact binary coalescences
• Rotations of the polarization of a gravitational wave propagating in Universe
• A Conceptual Model for the Origin of the Cutoff Parameter in Exotic Compact Objects
• Eccentricity as a signature of hierarchical subsolar-mass mergers in collapsar disks
• General relativistic hydrodynamics code for dynamical spacetimes with curvilinear coordinates, tabulated equations of state, and neutrino physics
• Two-body problem in curved spacetime: exploring gravitational wave transient cases
• A Bayesian Inference Framework for Gamma-Ray Burst Afterglow Properties
• How Neutron Star Observations Point Towards Exotic Matter: Existing Explanations and a Prospective Proposal
• Chirp mass based glitch identification in long duration gravitational wave transients
• Binary neutron star mergers within kaon condensation: GW170817
• Ten years of extreme gravity tests of general theory of relativity with gravitational-wave observations
• Fully general-relativistic simulations of isolated and binary strange quark stars
• $f$-mode oscillations of compact stars with realistic equations of state in dynamical spacetime
• Evolutionary tracks of binary neutron star progenitors across cosmic times
• Star Log-extended eMulation: a method for efficient computation of the Tolman-Oppenheimer-Volkoff equations
• Metric Assisted Stochastic Sampling (MASS) search for gravitational waves from binary black hole mergers
• Consistent crust-core interpolation and its effect on non-radial neutron star oscillations
• Sky localization of gravitational waves from eccentric binaries
• Scalar-induced gravitational waves in spatially covariant gravity
• Gravitational wave pulse and memory effects for hairy Kiselev black hole and its analogy with Bondi-Sachs formalism
• Even-parity stability of hairy black holes in $U(1)$ gauge-invariant scalar-vector-tensor theories
• Projecting the likely importance of weak-interaction-driven bulk viscosity in neutron star mergers
• On the use of galaxy catalogs in gravitational-wave parameter estimation
• Long-Range Quantum Gravity
• Nonlinear mode-tide coupling in coalescing binary neutron stars with relativistic corrections
• Parameter constraints for accreting millisecond pulsars with synthetic NICER data
• Multi-Messenger Astrophysics with THESEUS in the 2030s
• Surrogate modeling of gravitational waves microlensed by spherically symmetric potentials
• Hairy black holes in extended Einstein-Maxwell-scalar theories with magnetic charge and kinetic couplings
• Joint Inference of Population, Cosmology, and Neutron Star Equation of State from Gravitational Waves of Dark Binary Neutron Stars
• Toward Cosmological Standard Timers in Primordial Black Hole Binaries
• Constraints on the Scale Parameter of Regular Black Hole in Asymptotically Safe Gravity from Extreme Mass Ratio Inspirals
• Tidal reconstruction of neutron star mergers from their late inspiral
• Effect of spin in binary neutron star mergers
• Spin and quadrupolar effects in the secular evolution of precessing compact binaries with black hole, neutron star, gravastar, or boson star components
• Stellar response after stripping as a model for common-envelope outcomes
• Rapid Hierarchical Inference of Neutron Star Equation of State from multiple Gravitational Wave Observations of Binary Neutron Star Coalescences
• A nonparametric method to assess significance of events in search for gravitational waves with false discovery rate
• Measurability of neutron star tidal deformability from merging neutron star-black hole binaries
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• Gravitational-Wave Constraints on Neutron-Star Pressure Anisotropy via Universal Relations
• Conditional Autoencoder for Generating Binary Neutron Star Waveforms with Tidal and Precession Effects
• Systematic study of the morphology and length of slow stable hybrid star branches
• Constraining the abundance of spinning deformed Galactic compact objects with continuous gravitational waves
• Neutron Stars in Causal Scalar-Tensor Theories
• Kilohertz Gravitational Waves from Binary Neutron Star Mergers: Full Spectrum Analyses and High-density Constraints on Neutron Star Matter
• Inferring neutron star properties through gravitational waves from r-modes and their relativistic counterparts
• Adding Gamma-ray Polarimetry to the Multi-Messenger Era
• Convection signatures in early-time gravitational waves from core-collapse supernovae
• The time evolution of light nuclei cumulants and ratios with a first-order phase transition in the UrQMD transport model
• Chiral Effective Field Theory's Impact on Advancing Quantum Monte Carlo Methods
• Ringing Black Hole is Superradiant: Ultra-light Scalar Field
• Is The Trace Anomaly at its Minimum Value at Neutron Star Centers?
• Effects of a Brueckner-Hartree-Fock-corrected effective mass on speed of sound, conformality, and observables of dark matter-admixed neutron stars
• Deep follow-up for gravitational-wave inference: a case study with GW151226
• A ${\chi }^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences
• Maximal mass of the neutron star with a deconfined quark core
• An accurate model for the primordial black hole mass distribution from a peak in the power spectrum
• Shapiro Delay Measurements from Fifteen Years of PSR J1231$-$1411 Radio Observations
• Astrophysical and Cosmological Relevance of the High-Frequency Features in the Stochastic Gravitational-Wave Background
• Significant challenges for astrophysical inference with next-generation gravitational-wave observatories
• Application of Non-Linear Noise Regression in the Virgo Detector
• Probing millisecond magnetar formation in binary neutron star mergers through X-ray follow-up of gravitational wave alerts
• Astrophysical constraints on neutron star $f$-modes with a nonparametric equation of state representation
• Properties of rotating neutron stars in light of binary compact object mergers
• Modeling Neutron Star Oscillations in a Fixed General Relativistic Background Including Solid Crust Dynamics
• Bounding dark charges on binary black holes using gravitational waves
• Probing of EoS with clusters and hypernuclei
• Gravitational waves from sub-solar mass primordial black holes
• Pearson cross-correlation in the first four black hole binary mergers
• Heavy elements form short and long gamma-ray bursts
• Gravitational ringdown in the Minimal Theory of Massive Gravity
• Standard candles and sirens rescue $H_0$
• 3D Localization of FRB 20190425A for Its Potential Host Galaxy and Implications
• Hot Holographic 2-flavor Quark Star
• Mergers of binary neutron star systems: a multi-messenger revolution
• Calibrating systematic errors in the distance determination with the luminosity-distance space large scale structure of dark sirens and its potential applications
• Preliminary results of the pixel characterization for the Crystal Eye, a new X and gamma-ray satellite detector for multi-messenger astronomy
• Planckian charged black holes and their cosmological ramifications
• Early Warning From Eccentric Compact Binaries: Template Initialization And Sub-dominant Mode Effects
• Strongly Interacting Dark Matter admixed Neutron Stars
• Where are Gaia's small black holes?
• Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems
• Inferring neutron-star Love-Q relations from gravitational waves in the hierarchical Bayesian framework
• Classification of $g$-modes for neutron stars with a strong transition: Novel universal relation including slow stable hybrid stars
• Distinguishing between Black Holes and Neutron Stars within a Population of Weak Tidal Measurements
• Non-conservative Mass Transfer in the Neutron Star Stripping Model
• Effects of short-range correlations at high densities on neutron stars with and without DM content: role of the repulsive self-interaction
• Prospects for Neutrino Observation and Mass Measurement from Binary Neutron Star Mergers
• Toward a Unified Understanding of the Dense Matter Equation of State
• Search for planetary-mass ultra-compact binaries using data from the first part of the LIGO--Virgo--KAGRA fourth observing run
• Gravitational wave interactions with a viscous fluid: Core collapse supernova, binary neutron star merger, and accretion around a black hole merger
• Chiral, parity-doublet, effective-Lagrangian mean-field theories for nuclear and astrophysical phenomenology
• Impact of Anisotropy on Neutron Star Structure and Curvature
• Similar Fermi-GBM sGRBs to GW/sGRB 170817A in MeV-GeV energies
• Predictions on observing hot holographic quark star with gravitational waves
• Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Influences of parametrizations of density dependent couplings
• Neutron Star Equation of State with Nucleon Short-Range Correlations: A Concise Review and Open Issues
• Universal relation between dipole polarizability of finite nuclei and neutron-star compactness
• Rotation-dependent $I$-Love-$Q$-$\delta M$ relations in perturbation theory
• Astrometric microlensing probes of the isolated neutron star population with Roman
• Realistic Equations of State Informing Neutron Star Post-Merger Gravitational-Wave Frequencies
• Las Cumbres Observatory Gravitational-Wave Follow-up in the Third and Fourth Observing Runs: Strengths and Weaknesses of a Rapid Response Galaxy Targeted Strategy
• Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars
• labrador: A domain-optimized machine-learning tool for gravitational wave inference
• Structure of Anisotropic Magnetized Neutron Stars in f(R,T) Gravity with Realistic Equation of State
• Constraints on the VHE counterpart of two binary black hole mergers observed by the MAGIC and CTAO LST-1 telescopes
• Gravitational-Wave Signatures of Massive Black Hole Formation
• Constraining the Phase-Transition EoS using the Energy Dependence of Directed Flow
• Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars
• Search for Astrophysical Transients on Limiting Time Scales and Their Classification Based on INTEGRAL Data
• Exploring the Link between Fast Radio Burst and Binary Neutron Star Origins with Spaceborne Gravitational Wave Observations
• Searching for the Signature of Fast Radio Burst by Swift/XRT X-ray Afterglow Light Curve
• General Relativistic Stability and Gravitational Wave Content of Rotating Triaxial Neutron Stars
• Prospects for detecting asteroid-mass primordial black holes in extreme mass-ratio inspirals with continuous gravitational waves
• Superradiant scattering of massive scalar field due to magnetically charged rotating black hole
• Parameter estimation for space-based gravitational wave detectors with ringdown signals
• Mergers as a Probe of Particle Dark Matter
• On the hosts of neutron star mergers in the nearby Universe
• A template-free approach for waveform extraction of gravitational wave events
• Hierarchical search for compact binary coalescences in the Advanced LIGO's first two observing runs
• Host galaxies and electromagnetic counterparts to binary neutron star mergers across the cosmic time: Detectability of GW170817-like events
• Sudden discharge of young charged magnetars as a new model for FRBs
• Light scalars in neutron star mergers
• On the use of CHIME to Detect Long-Duration Radio Transients from Neutron Star Mergers
• Dynamical double black holes and their host cluster properties
• Probing neutron stars with the full pre-merger and post-merger gravitational wave signal from binary coalescences
• Topological Black Holes with curvature induced scalarization in the extended scalar-tensor theories
• Revisiting black hole hyperaccretion in the center of gamma-ray bursts for the lower mass gap
• TYC~2990-127-1: an Algol-type SB2 binary system of subgiant and red giant with a probable ongoing mass-transfer
• Neutrino mean free path in neutron stars in the presence of hyperons
• Extract non-Gaussian Features in Gravitational Wave Observation Data Using Self-Supervised Learning
• Tidal Deformability of Quark Stars with Repulsive Interactions
• Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations II: Double Compact Object Rates and Properties
• Investigating the mass-ratio dependence of the prompt-collapse threshold with numerical-relativity simulations
• Prospects for distinguishing dynamical tides in inspiralling binary neutron stars with third generation gravitational-wave detectors
• Deep Residual Error and Bag-of-Tricks Learning for Gravitational Wave Surrogate Modeling
• Rising Tides: Analytic Modeling of Tidal Effects in Binary Neutron Star Mergers
• Unified nonparametric equation-of-state inference from the neutron-star crust to perturbative-QCD densities
• Assessment of normalizing flows for parameter estimation on time-frequency representations of gravitational-wave data
• Enhancing gravitational-wave detection: a machine learning pipeline combination approach with robust uncertainty quantification
• Linear perturbations of dyonic black holes in the lowest-order $U(1)$ gauge-invariant scalar-vector-tensor theories