Black holes, gravitational waves and fundamental physics: a roadmap

Abstract

The grand challenges of contemporary fundamental physics---dark matter, dark energy, vacuum energy, inflation and early universe cosmology, singularities and the hierarchy problem---all involve gravity as a key component. And of all gravitational phenomena, black holes stand out in their elegant simplicity, while harbouring some of the most remarkable predictions of General Relativity: event horizons, singularities and ergoregions. The hitherto invisible landscape of the gravitational Universe is being unveiled before our eyes: the historical direct detection of gravitational waves by the LIGO-Virgo collaboration marks the dawn of a new era of scientific exploration. Gravitational-wave astronomy will allow us to test models of black hole formation, growth and evolution, as well as models of gravitational-wave generation and propagation. It will provide evidence for event horizons and ergoregions, test the theory of General Relativity itself, and may reveal the existence of new fundamental fields. The synthesis of these results has the potential to radically reshape our understanding of the cosmos and of the laws of Nature. The purpose of this work is to present a concise, yet comprehensive overview of the state of the art in the relevant fields of research, summarize important open problems, and lay out a roadmap for future progress.

arXiv commentWhite Paper for the COST action "Gravitational Waves, Black Holes, and Fundamental Physics", 272 pages, 12 figures; v4: updated references and author list. Overall improvements and corrections. To appear in Classical and Quantum Gravity

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• Kilonova Light Curves from the Disk Wind Outflows of Compact Object Mergers
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• Shadow of a rotating braneworld black hole
• Black Hole Spin via Continuum Fitting and the Role of Spin in Powering Transient Jets
• Phenomenological template family for black-hole coalescence waveforms
• Peering into the dark side: magnesium lines establish a massive neutron star in PSR J2215+5135
• Observing the shadow of Einstein-Maxwell-Dilaton-Axion black hole
• Conformal ``thin sandwich'' data for the initial-value problem of general relativity
• A no-hair theorem for the galileon
• Rapid Formation of Supermassive Black Hole Binaries in Galaxy Mergers with Gas
• Binary black hole mergers from field triples: properties, rates and the impact of stellar evolution
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• Galaxy Formation with BECDM: I. Turbulence and relaxation of idealised haloes
• Binary Mergers and Growth of Black Holes in Dense Star Clusters
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• The Population of Viscosity- and Gravitational Wave-Driven Supermassive Black Hole Binaries Among Luminous AGN
• The dynamical mass ejection from binary neutron star mergers: Radiation-hydrodynamics study in general relativity
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• Are eikonal quasinormal modes linked to the unstable circular null geodesics?
• High-energy gravitational scattering and the general relativistic two-body problem
• Testing black hole candidates with electromagnetic radiation
• A systematic search for close supermassive black hole binaries in the Catalina Real-Time Transient Survey
• Constraint damping in the Z4 formulation and harmonic gauge
• The Locations of Short Gamma-ray Bursts as Evidence for Compact Object Binary Progenitors
• Low-frequency gravitational radiation from coalescing massive black hole binaries in hierarchical cosmologies
• Dimensional regularization of the gravitational interaction of point masses
• Simulations of solitonic core mergers in ultra-light axion dark matter cosmologies
• Quantum gravity without Lorentz invariance
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• Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO's First Observing Run
• Zoom & Whirl: Eccentric equatorial orbits around spinning black holes and their evolution under gravitational radiation reaction
• Testing General Relativity with Low-Frequency, Space-Based Gravitational-Wave Detectors
• On the Extra Mode and Inconsistency of Horava Gravity
• Two timescale analysis of extreme mass ratio inspirals in Kerr. I. Orbital Motion
• Mapping spacetimes with LISA: inspiral of a test-body in a `quasi-Kerr' field
• Merging black hole binaries: the effects of progenitor's metallicity, mass-loss rate and Eddington factor
• Compact Stars as Dark Matter Probes
• Testing strong-field gravity with tidal Love numbers
• The search for failed supernovae with the Large Binocular Telescope: confirmation of a disappearing star
• Prompt merger collapse and the maximum mass of neutron stars
• Proca Stars: gravitating Bose-Einstein condensates of massive spin 1 particles
• How to tell a gravastar from a black hole
• Coherent method for detection of gravitational wave bursts
• Efficient Merger of Binary Supermassive Black Holes in Non-Axisymmetric Galaxies
• Black Hole Superradiance Signatures of Ultralight Vectors
• Short GRB and binary black hole standard sirens as a probe of dark energy
• Lidov-Kozai Cycles with Gravitational Radiation: Merging Black Holes in Isolated Triple Systems
• Nonlocal-in-time action for the fourth post-Newtonian conservative dynamics of two-body systems
• False periodicities in quasar time-domain surveys
• Superradiant Instability and Backreaction of Massive Vector Fields around Kerr Black Holes
• Distinguishing Spin-Aligned and Isotropic Black Hole Populations With Gravitational Waves
• Higher-order spin effects in the dynamics of compact binaries I. Equations of motion
• Possible Indirect Confirmation of the Existence of Pop III Massive Stars by Gravitational Wave
• CMB bounds on disk-accreting massive Primordial Black Holes
• A Further Analysis of a Cosmological Model of Quintessence and Scalar Dark Matter
• Aligning spinning black holes and accretion discs
• Event rate estimates for LISA extreme mass ratio capture sources
• Kerr black holes with Proca hair
• Conformal and covariant formulation of the Z4 system with constraint-violation damping
• Effective One Body description of tidal effects in inspiralling compact binaries
• Gamma-ray binaries and related systems
• Three Dimensional MHD Simulation of Circumbinary Accretion Disks: Disk Structures and Angular Momentum Transport
• Massive spin-2 fields on black hole spacetimes: Instability of the Schwarzschild and Kerr solutions and bounds on the graviton mass
• The Dynamical Evolution of Stellar Black Holes in Globular Clusters
• Primordial Black Hole production in Critical Higgs Inflation
• Improved resummation of post-Newtonian multipolar waveforms from circularized compact binaries
• "Kludge" gravitational waveforms for a test-body orbiting a Kerr black hole
• Evidence for a Massive Neutron Star from a Radial-Velocity Study of the Companion to the Black Widow Pulsar PSR B1957+20
• Colliding Black Holes: The Close Limit
• Gravitational waves from resolvable massive black hole binary systems and observations with Pulsar Timing Arrays
• Using LISA EMRI sources to test off-Kerr deviations in the geometry of massive black holes
• Inference of the cosmological parameters from gravitational waves: application to second generation interferometers
• Accretion into the Central Cavity of a Circumbinary Disk
• Constraint violation in free evolution schemes: comparing BSSNOK with a conformal decomposition of Z4
• Massive black hole binaries from runaway collisions: the impact of metallicity
• Phenomenologically viable Lorentz-violating quantum gravity
• Black Hole Mergers in Galactic Nuclei Induced by the Eccentric Kozai-Lidov Effect
• Dynamical Tides in General Relativity: Effective Action and Effective-One-Body Hamiltonian
• Gravitational wave snapshots of generic extreme mass ratio inspirals
• General parametrization of axisymmetric black holes in metric theories of gravity
• Gravitational-Wave Inspiral of Compact Binary Systems to 7/2 Post-Newtonian Order
• The cosmic evolution of massive black holes in the Horizon-AGN simulation
• Analytic Solutions of the Teukolsky Equation and their Low Frequency Expansions
• Electromagnetic Evidence that SSS17a is the Result of a Binary Neutron Star Merger
• Ultra-Low Frequency Gravitational Radiation from Massive Black Hole Binaries
• Bayesian coherent analysis of in-spiral gravitational wave signals with a detector network
• BPASS predictions for Binary Black-Hole Mergers
• Missing Black Holes Unveil The Supernova Explosion Mechanism
• Spectroscopy of Kerr black holes with Earth- and space-based interferometers
• The evolution of massive black holes and their spins in their galactic hosts
• Multiwavelength Evidence for Quasi-periodic Modulation in the Gamma-ray Blazar PG 1553+113
• 3rd post-Newtonian higher order Hamilton dynamics for two-body point-mass systems
• Lorentz symmetry breaking as a quantum field theory regulator
• Are LIGO's Black Holes Made From Smaller Black Holes?
• Search for post-merger gravitational waves from the remnant of the binary neutron star merger GW170817
• Galactic distribution of merging neutron stars and black holes - prospects for short GRB progenitors and LIGO/VIRGO
• Black-Hole Bombs and Photon-Mass Bounds
• Neutrino-driven winds in the aftermath of a neutron star merger: nucleosynthesis and electromagnetic transients
• Non-Spinning Black Holes in Alternative Theories of Gravity
• Gravitational Wave signatures of inflationary models from Primordial Black Hole Dark Matter
• Overcharging a Black Hole and Cosmic Censorship
• Challenges to Self-Acceleration in Modified Gravity from Gravitational Waves and Large-Scale Structure
• Ultra-high precision cosmology from gravitational waves
• A Population of Short-Period Variable Quasars from PTF as Supermassive Black Hole Binary Candidates
• Neutron-star mergers in scalar-tensor theories of gravity
• Inspiral-merger-ringdown multipolar waveforms of nonspinning black-hole binaries using the effective-one-body formalism
• Black Hole Mergers and the QCD Axion at Advanced LIGO
• Toward Early-Warning Detection of Gravitational Waves from Compact Binary Coalescence
• Mass Measurements of Black Holes in X-Ray Transients: Is There a Mass Gap?
• Measuring a cosmological distance-redshift relationship using only gravitational wave observations of binary neutron star coalescences
• The DRAGON simulations: globular cluster evolution with a million stars
• AT2017gfo: an anisotropic and three-component kilonova counterpart of GW170817
• Prototype effective-one-body model for nonprecessing spinning inspiral-merger-ringdown waveforms
• Closed-form tidal approximants for binary neutron star gravitational waveforms constructed from high-resolution numerical relativity simulations
• Dynamical Formation of the GW150914 Binary Black Hole
• Superradiant instabilities in astrophysical systems
• Regular Black Hole Metric with Three Constants of Motion
• Mass Ejection from the Remnant of a Binary Neutron Star Merger: Viscous-Radiation Hydrodynamics Study
• The third post-Newtonian gravitational wave polarisations and associated spherical harmonic modes for inspiralling compact binaries in quasi-circular orbits
• Measuring the Spins of Accreting Black Holes
• Black holes in Einstein-aether and Horava-Lifshitz gravity
• Constraining the mass of dark photons and axion-like particles through black-hole superradiance
• MOCCA Code for Star Cluster Simulations - IV. A new Scenario for Intermediate Mass Black Hole Formation in Globular Clusters
• Evolution and fate of very massive stars
• Horava-Lifshitz gravity: a status report
• Modeling the dynamics of tidally-interacting binary neutron stars up to merger
• Shadow of a Kaluza-Klein rotating dilaton black hole
• Lyman-alpha Constraints on Ultralight Scalar Dark Matter: Implications for the Early and Late Universe
• Perturbations of slowly rotating black holes: massive vector fields in the Kerr metric
• Parametrized tests of post-Newtonian theory using Advanced LIGO and Einstein Telescope
• Pulsar timing signal from ultralight scalar dark matter
• Extrinsic Curvature and the Einstein Constraints
• Faithful Effective-One-Body waveforms of small-mass-ratio coalescing black-hole binaries
• Expected properties of the first gravitational wave signal detected with pulsar timing arrays
• GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences
• Echoes of Kerr-like wormholes
• On the importance of viscous dissipation and heat conduction in binary neutron-star mergers
• Dimensional regularization of the third post-Newtonian dynamics of point particles in harmonic coordinates
• European Pulsar Timing Array Limits on Continuous Gravitational Waves from Individual Supermassive Black Hole Binaries
• Compact Binary Merger Rates: Comparison with LIGO/Virgo Upper Limits
• Unification of the Fundamental Plane and Super-Massive Black Holes Masses
• The final spin from binary black holes in quasi-circular orbits
• The long-term evolution of neutron star merger remnants - II. Radioactively powered transients
• Black Strings, Low Viscosity Fluids, and Violation of Cosmic Censorship
• Over-spinning a black hole with a test body
• Validating the effective-one-body model of spinning, precessing binary black holes against numerical relativity
• Testing the black hole "no-hair" hypothesis
• Cosmography with the Einstein Telescope
• Stochastic and resolvable gravitational waves from ultralight bosons
• Global simulations of strongly magnetized remnant massive neutron stars formed in binary neutron star mergers
• Science with the space-based interferometer eLISA. III: Probing the expansion of the Universe using gravitational wave standard sirens
• Precision of Hubble constant derived using black hole binary absolute distances and statistical redshift information
• Towards models of gravitational waveforms from generic binaries: A simple approximate mapping between precessing and non-precessing inspiral signals
• Perturbed black holes in Einstein-dilaton-Gauss-Bonnet gravity: Stability, ringdown, and gravitational-wave emission
• Gravitational radiation from compact binary systems in the massive Brans-Dicke theory of gravity
• Electromagnetic Signatures of Neutron Star Mergers in the Advanced LIGO Era
• Stochastic gravitational waves associated with the formation of primordial black holes
• A recipe for echoes from exotic compact objects
• Evolution of circular, non-equatorial orbits of Kerr black holes due to gravitational-wave emission: II. Inspiral trajectories and gravitational waveforms
• New parametrization for spherically symmetric black holes in metric theories of gravity
• Implementing a search for aligned-spin neutron star -- black hole systems with advanced ground based gravitational wave detectors
• Quasinormal-mode spectrum of Kerr black holes and its geometric interpretation
• Quantifying the Coexistence of Massive Black Holes and Dense Nuclear Star Clusters
• Scattering of two spinning black holes in post-Minkowskian gravity, to all orders in spin, and effective-one-body mappings
• The stochastic background: scaling laws and time to detection for pulsar timing arrays
• Post-Newtonian Gravitational Radiation and Equations of Motion via Direct Integration of the Relaxed Einstein Equations. I. Foundations
• Binary black hole merger dynamics and waveforms
• Shadows of Einstein-dilaton-Gauss-Bonnet black holes
• A consequence of the gravitational self-force for circular orbits of the Schwarzschild geometry
• A Deep Chandra X-ray Study of Neutron Star Coalescence GW170817
• How to move a black hole without excision: gauge conditions for the numerical evolution of a moving puncture
• On the final spin from the coalescence of two black holes
• Relativistic Dynamics and Extreme Mass Ratio Inspirals
• Black-Hole Solutions with Scalar Hair in Einstein-Scalar-Gauss-Bonnet Theories
• Constraining Lorentz-violating, Modified Dispersion Relations with Gravitational Waves
• Slowly Rotating Black Holes in Dynamical Chern-Simons Gravity: Deformation Quadratic in the Spin
• The one-dimensional Ly-alpha forest power spectrum from BOSS
• The Shadow of a Rotating Traversable Wormhole
• Solving Einstein's Equations With Dual Coordinate Frames
• Into the lair: gravitational-wave signatures of dark matter
• An improved effective-one-body Hamiltonian for spinning black-hole binaries
• Derivative self-interactions for a massive vector field
• Asymptotically flat black holes in Horndeski theory and beyond
• Matched-filtering and parameter estimation of ringdown waveforms
• Effects of the microphysical Equation of State in the mergers of magnetized Neutron Stars With Neutrino Cooling
• Test bodies and naked singularities: is the self-force the cosmic censor?
• Estimating the final spin of a binary black hole coalescence
• Fast prediction and evaluation of gravitational waveforms using surrogate models
• Graviton Mass Bounds
• Three-dimensional GRMHD simulations of neutrino-cooled accretion disks from neutron star mergers
• The Masses and Spins of Neutron Stars and Stellar-Mass Black Holes
• No-hair theorem for Black Holes in Astrophysical Environments
• Forming short-period Wolf-Rayet X-ray binaries and double black holes through stable mass transfer
• Advanced Methods in Black-Hole Perturbation Theory
• Predicting the direction of the final spin from the coalescence of two black holes
• A Numerical Relativity Waveform Surrogate Model for Generically Precessing Binary Black Hole Mergers
• Gravitational-wave signal from binary neutron stars: a systematic analysis of the spectral properties
• Planckian Interacting Massive Particles as Dark Matter
• Limiting eccentricity of sub-parsec massive black hole binaries surrounded by self-gravitating gas discs
• Follow up of GW170817 and its electromagnetic counterpart by Australian-led observing programs
• Third post-Newtonian dynamics of compact binaries: Noetherian conserved quantities and equivalence between the harmonic-coordinate and ADM-Hamiltonian formalisms
• LISA detections of massive black hole inspirals: parameter extraction errors due to inaccurate template waveforms
• Testing local Lorentz invariance with gravitational waves
• Gedanken Experiments to Destroy a Black Hole II: Kerr-Newman Black Holes Cannot be Over-Charged or Over-Spun
• General relativistic dynamics of compact binaries at the third post-Newtonian order
• The Evolution of Binary Fractions in Globular Clusters
• Lyman-alpha Forests cool Warm Dark Matter
• Cosmology with the lights off: Standard sirens in the Einstein Telescope era
• The gravitational-wave luminosity distance in modified gravity theories
• Frame dragging and other precessional effects in black hole-pulsar binaries
• Post-Newtonian gravitational radiation and equations of motion via direct integration of the relaxed Einstein equations. II. Two-body equations of motion to second post-Newtonian order, and radiation-reaction to 3.5 post-Newtonian order
• Growth and activity of black holes in galaxy mergers with varying mass ratios
• A ~50,000 solar mass black hole in the nucleus of RGG 118
• Short Gamma-Ray Bursts from the Merger of Two Black Holes
• Gravitational Self Force in a Schwarzschild Background and the Effective One Body Formalism
• HST hot Jupiter Transmission Spectral Survey: A detection of Na and strong optical absorption in HAT-P-1b
• Fast and accurate prediction of numerical relativity waveforms from binary black hole coalescences using surrogate models
• Spin Flips and Precession in Black-Hole-Binary Mergers
• Low mass binary neutron star mergers : gravitational waves and neutrino emission
• Hangup Kicks: Still Larger Recoils by Partial Spin/Orbit Alignment of Black-Hole Binaries
• Extended Horava gravity and Einstein-aether theory
• Effective one body approach to the dynamics of two spinning black holes with next-to-leading order spin-orbit coupling
• Determination of the geometry of the PSR B1913+16 system by geodetic precession
• Gravitational radiative corrections from effective field theory
• The observed velocity distribution of young pulsars
• Frequency domain reduced order models for gravitational waves from aligned-spin compact binaries
• Dissipationless Formation and Evolution of the Milky Way Nuclear Star Cluster
• Dual Jets from Binary Black Holes
• A Review on the Scalar Field/ Bose-Einstein Condensate Dark Matter Model
• Double neutron stars: merger rates revisited
• TIGER: A data analysis pipeline for testing the strong-field dynamics of general relativity with gravitational wave signals from coalescing compact binaries
• Post-Newtonian, Quasi-Circular Binary Inspirals in Quadratic Modified Gravity
• Exploring black hole superkicks
• An intermediate-mass black hole in the centre of the globular cluster 47 Tucanae
• Angular momentum transport in stellar interiors constrained by rotational splittings of mixed modes in red giants
• Compact binary evolutions with the Z4c formulation
• Mode sum regularization approach for the self-force in black hole spacetime
• Hierarchical data-driven approach to fitting numerical relativity data for nonprecessing binary black holes with an application to final spin and radiated energy
• Constraints on the Primordial Black Hole Abundance from the First Advanced LIGO Observation Run Using the Stochastic Gravitational-Wave Background
• Georgia Tech Catalog of Gravitational Waveforms
• Eight New Millisecond Pulsars in NGC 6440 and NGC 6441
• Co-Evolution of Galactic Nuclei and Globular Cluster Systems
• Eccentricity of supermassive black hole binaries coalescing from gas rich mergers
• Observing gravitational-wave transient GW150914 with minimal assumptions
• Signatures of hypermassive neutron star lifetimes on r-process nucleosynthesis in the disk ejecta from neutron star mergers
• Viscous Hydrodynamics Simulations of Circumbinary Accretion Discs: Variability, Quasi-Steady State, and Angular Momentum Transfer
• Upper limits on the rates of binary neutron star and neutron-star--black-hole mergers from Advanced LIGO's first observing run
• Gravitational-wave cosmology across 29 decades in frequency
• Binary-black-hole initial data with nearly-extremal spins
• Microlensing and dynamical constraints on primordial black hole dark matter with an extended mass function
• Bayesian model selection for testing the no-hair theorem with black hole ringdowns
• Relativistic Binaries in Globular Clusters
• Towards a formalism for mapping the spacetimes of massive compact objects: Bumpy black holes and their orbits
• Prospects for Probing the Spacetime of Sgr A* with Pulsars
• Ergoregion instability of ultra-compact astrophysical objects
• High-resolution magnetohydrodynamics simulation of black hole-neutron star merger: Mass ejection and short gamma-ray burst
• Gravitational self-force correction to the innermost stable circular orbit of a Schwarzschild black hole
• Testing Scalar-Tensor Gravity with Gravitational-Wave Observations of Inspiralling Compact Binaries
• Evolution of supermassive stars as a pathway to black hole formation
• General relativistic magnetohydrodynamic simulations of binary neutron star mergers forming a long-lived neutron star
• Excision boundary conditions for black hole initial data
• Fourth post-Newtonian effective one-body dynamics
• Gravitational wave astronomy of single sources with a pulsar timing array
• Spontaneous Scalarization with Massive Fields
• A new effective-one-body description of coalescing nonprecessing spinning black-hole binaries
• Discovery of High-Energy Gamma-Ray Emission from the Binary System PSR B1259-63/LS 2883 Around Periastron with Fermi
• Gravitational waves from inspiralling compact binaries: Energy flux to third post-Newtonian order
• Primordial black holes as a tool for constraining non-Gaussianity
• The Spin of Supermassive Black Holes
• A Rigorous Derivation of Gravitational Self-force
• Estimating cosmological parameters by the simulated data of gravitational waves from the Einstein Telescope
• LIGO gravitational wave detection, primordial black holes and the near-IR cosmic infrared background anisotropies
• Gravitational field and equations of motion of compact binaries to 5/2 post-Newtonian order
• Coalescence of binary neutron stars in a scalar-tensor theory of gravity
• Gravitational self-force on a particle in eccentric orbit around a Schwarzschild black hole
• Calculating the gravitational self force in Schwarzschild spacetime
• Binary black-hole evolutions of excision and puncture data
• General-covariant evolution formalism for Numerical Relativity
• Exploring properties of high-density matter through remnants of neutron-star mergers
• Distinguishing Boson Stars from Black Holes and Neutron Stars from Tidal Interactions in Inspiraling Binary Systems
• Greatly enhanced merger rates of compact-object binaries in non-spherical nuclear star clusters
• Dynamical scalarization of neutron stars in scalar-tensor gravity theories
• Hamiltonian of a spinning test-particle in curved spacetime
• Self-sustained asymmetry of lepton-number emission: A new phenomenon during the supernova shock-accretion phase in three dimensions
• Fast and Accurate Inference on Gravitational Waves from Precessing Compact Binaries
• Frequency domain reduced order model of aligned-spin effective-one-body waveforms with generic mass-ratios and spins
• The high-energy collision of two black holes
• A New Signature of Dark Matter Annihilations: Gamma-Rays from Intermediate-Mass Black Holes
• Neutron star kicks by the gravitational tug-boat mechanism in asymmetric supernova explosions: progenitor and explosion dependence
• Poincaré invariance in the ADM Hamiltonian approach to the general relativistic two-body problem
• Massive binary black holes in galactic nuclei and their path to coalescence
• Quadratic-in-spin effects in the orbital dynamics and gravitational-wave energy flux of compact binaries at the 3PN order
• Quasi-Normal Modes and Gravitational Wave Astronomy
• Dynamical constraints on the dark matter distribution in the Milky Way
• Effective action approach to higher-order relativistic tidal interactions in binary systems and their effective one body description
• Bimetric gravity is cosmologically viable
• Improved effective-one-body description of coalescing nonspinning black-hole binaries and its numerical-relativity completion
• The Local Nanohertz Gravitational-Wave Landscape From Supermassive Black Hole Binaries
• The Barbero-Immirzi Parameter as a Scalar Field: K-Inflation from Loop Quantum Gravity?
• The Gravitational Wave Background from Massive Black Hole Binaries in Illustris: spectral features and time to detection with pulsar timing arrays
• Impact of an improved neutrino energy estimate on outflows in neutron star merger simulations
• Multi-messenger picture of compact binary mergers
• Using Full Information When Computing Modes of Post-Newtonian Waveforms From Inspiralling Compact Binaries in Circular Orbit
• Tracking the precession of compact binaries from their gravitational-wave signal
• Gravitational wave signatures of the absence of an event horizon. I. Nonradial oscillations of a thin-shell gravastar
• Kerr-Newman scalar clouds
• On r-process nucleosynthesis from matter ejected in binary neutron starmergers
• Electromagnetic Counterparts to Structured Jets from Gravitational Wave Detected Mergers
• Remnant Masses, Spins and Recoils from the Merger of Generic Black-Hole Binaries
• Floating and sinking: the imprint of massive scalars around rotating black holes
• Constraints on cosmic strings using data from the first Advanced LIGO observing run
• Bumpy Black Holes in Alternate Theories of Gravity
• Formation of supermassive black hole seeds
• The effects of Chern-Simons gravity on bodies orbiting the Earth
• Gravitational Wave Signatures of Highly Compact Boson Star Binaries
• High-Order Post-Newtonian Fit of the Gravitational Self-Force for Circular Orbits in the Schwarzschild Geometry
• The end of the MACHO era- revisited: new limits on MACHO masses from halo wide binaries
• Evolution of binary black holes in self gravitating discs: dissecting the torques
• Low significance of evidence for black hole echoes in gravitational wave data
• Ultra Relativistic Particle Collisions
• Compact binary systems in scalar-tensor gravity: Equations of motion to 2.5 post-Newtonian order
• The 2.5PN gravitational wave polarisations from inspiralling compact binaries in circular orbits
• Massive double compact object mergers: gravitational wave sources and r-process-element production sites
• Black Holes in Einstein-Aether Theory
• Analytical determination of the two-body gravitational interaction potential at the 4th post-Newtonian approximation
• Low metallicity natal environments and black hole masses in Ultraluminous X-ray Sources
• The characteristic black hole mass resulting from direct collapse in the early universe
• Digging deeper: Observing primordial gravitational waves below the binary black hole produced stochastic background
• Neutron star-black hole mergers with a nuclear equation of state and neutrino cooling: Dependence in the binary parameters
• The Interaction of Stellar Objects within a Common Envelope
• BlackHoleCam: fundamental physics of the Galactic center
• Massive Primordial Black Holes as Dark Matter and their detection with Gravitational Waves
• Dimensional regularization of the third post-Newtonian gravitational wave generation from two point masses
• A Quantitative Test of the No-Hair Theorem with Sgr A* using stars, pulsars, and the Event Horizon Telescope
• Feedback-regulated Super Massive Black Hole Seed Formation
• Imaging a boson star at the Galactic center
• Binary black holes in circular orbits. II. Numerical methods and first results
• Testing post-Newtonian theory with gravitational wave observations
• Gas driven massive black hole binaries: signatures in the nHz gravitational wave background
• Head-on collisions of boson stars
• The final-parsec problem in the collisionless limit
• Constraining Formation Models of Binary Black Holes with Gravitational-Wave Observations
• Black Hole Binary Formation in the Expanding Universe --- Three Body Problem Approximation ---
• Probing the non-linear structure of general relativity with black hole binaries
• A formal introduction to Horndeski and Galileon theories and their generalizations
• Extreme- and Intermediate-Mass Ratio Inspirals in Dynamical Chern-Simons Modified Gravity
• Characterising gravitational wave stochastic background anisotropy with Pulsar Timing Arrays
• Distinguishing Between Formation Channels for Binary Black Holes with LISA
• Dynamics of dwarf galaxies disfavor stellar-mass black hole dark matter
• Detectability of compact binary merger macronovae
• Farthest Neighbor: The Distant Milky Way Satellite Eridanus II
• Black Hole Mergers and Unstable Circular Orbits
• Periastron Advance in Black-Hole Binaries
• On the geometrical origin of periodicity in blazar-type sources
• Bosenova collapse of axion cloud around a rotating black hole
• Modeling dynamical ejecta from binary neutron star mergers and implications for electromagnetic counterparts
• Astrophysical signatures of boson stars: quasinormal modes and inspiral resonances
• Testing the binary black hole nature of a compact binary coalescence
• Modified Gravity Black Holes and their Observable Shadows
• Incidences between points and lines on a two-dimensional variety
• Origin and growth of nuclear star clusters around massive black holes
• General relativistic simulations of compact binary mergers as engines of short gamma-ray bursts
• Not quite a black hole
• A Surrogate Model of Gravitational Waveforms from Numerical Relativity Simulations of Precessing Binary Black Hole Mergers
• Ready-to-use post-Newtonian gravitational waveforms for binary black holes with non-precessing spins: An update
• The last orbit of binary black holes
• Black Holes and Scalar Fields
• The First Law of Binary Black Hole Mechanics in General Relativity and Post-Newtonian Theory
• Primordial black hole evolution in tensor-scalar cosmology
• Estimates of black-hole natal kick velocities from observations of low-mass X-ray binaries
• Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescence
• Strong Binary Pulsar Constraints on Lorentz Violation in Gravity
• Measuring the parameters of massive black hole binary systems with Pulsar Timing Array observations of gravitational waves
• Eccentric Black Hole Gravitational-Wave Capture Sources in Galactic Nuclei: Distribution of Binary Parameters
• The Rapid Reddening and Featureless Optical Spectra of the optical counterpart of GW170817, AT 2017gfo, During the First Four Days
• Black-hole hair loss: learning about binary progenitors from ringdown signals
• General-Relativistic Large-Eddy Simulations of Binary Neutron Star Mergers
• Gravitational waves as a probe of dark matter mini-spikes
• Gravitational spin Hamiltonians from the S matrix
• Fokker action of non-spinning compact binaries at the fourth post-Newtonian approximation
• Horava gravity vs. thermodynamics: the black hole case
• Gravitational wave bursts from cosmic (super)strings: Quantitative analysis and constraints
• Post-Newtonian factorized multipolar waveforms for spinning, non-precessing black-hole binaries
• Testing general relativity using golden black-hole binaries
• Second-order gravitational self-force
• Cross section, final spin and zoom-whirl behavior in high-energy black hole collisions
• On the number density of "direct collapse" black hole seeds
• Conservative dynamics of two-body systems at the fourth post-Newtonian approximation of general relativity
• The complete non-spinning effective-one-body metric at linear order in the mass ratio
• Testing the no-hair theorem with black hole ringdowns using TIGER
• The Fast and the Fiducial: Augmented kludge waveforms for detecting extreme-mass-ratio inspirals
• Binary black holes in circular orbits. I. A global spacetime approach
• Collapse to Black Holes in Brans-Dicke Theory: II. Comparison with General Relativity
• Gravitational radiation reaction and inspiral waveforms in the adiabatic limit
• Renormalization of Horava Gravity
• Continuum and Discrete Initial-Boundary-Value Problems and Einstein's Field Equations
• Stochastic backgrounds in alternative theories of gravity: overlap reduction functions for pulsar timing arrays
• Velocities of pulsars and neutrino oscillations
• Resonant relaxation and the warp of the stellar disc in the Galactic centre
• Gravitational self force on a particle in circular orbit around a Schwarzschild black hole
• Scattering experiments meet N-body I: a practical recipe for the evolution of massive black hole binaries in stellar environments
• The Origin of Black Hole Spin in Galactic Low-Mass X-ray Binaries
• Probing Planckian corrections at the horizon scale with LISA binaries
• Indirect and direct search for dark matter
• Effective field theory approach to the gravitational two-body dynamics, at fourth post-Newtonian order and quintic in the Newton constant
• Using spin to understand the formation of LIGO's black holes
• Evolution of inspiral orbits around a Schwarzschild black hole
• Dynamical formation signatures of black hole binaries in the first detected mergers by LIGO
• Impact of weak interactions of free nucleons on the r-process in dynamical ejecta from neutron-star mergers
• Searching for Primordial Black Holes in the radio and X-ray sky
• The tail effect in gravitational radiation-reaction: time non-locality and renormalization group evolution
• On the multipole expansion of the gravitational field
• On the orbital evolution of supermassive black hole binaries with circumbinary accretion discs
• The third and a half post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries
• Constraining the high redshift formation of black hole seeds in nuclear star clusters with gas inflows
• Gravitational self-force and the effective-one-body formalism between the innermost stable circular orbit and the light ring
• On the mass radiated by coalescing black-hole binaries
• Black Hole Spectroscopy: Systematic Errors and Ringdown Energy Estimates
• Gravitational-wave phasing for low-eccentricity inspiralling compact binaries to 3PN order
• Pairing of Supermassive Black Holes in unequal-mass galaxy mergers
• Black holes with surrounding matter in scalar-tensor theories
• New derivation of a third post-Newtonian equation of motion for relativistic compact binaries without ambiguity
• Third post-Newtonian angular momentum flux and the secular evolution of orbital elements for inspiralling compact binaries in quasi-elliptical orbits
• X-Pipeline: An analysis package for autonomous gravitational-wave burst searches
• Dynamical Evolution of Boson Stars II: Excited States and Self-Interacting Fields
• Directional limits on persistent gravitational waves from Advanced LIGO's first observing run
• Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution
• Massive black hole factories: Supermassive and quasi-star formation in primordial halos
• Common envelope ejection in massive binary stars - Implications for the progenitors of GW150914 and GW151226
• Detecting a Stochastic Gravitational Wave Background in the presence of a Galactic Foreground and Instrument Noise
• Constraints on Einstein-aether theory after GW170817
• Rotating black hole in extended Chern-Simons modified gravity
• Multimessenger astronomy with pulsar timing and X-ray observations of massive black hole binaries
• Improved approximate inspirals of test-bodies into Kerr black holes
• Multi-timescale analysis of phase transitions in precessing black-hole binaries
• Nearby Early-Type Galactic Nuclei at High Resolution: Dynamical Black Hole and Nuclear Star Cluster Mass Measurements
• Superradiant instability of massive vector fields around spinning black holes in the relativistic regime
• The late inspiral of supermassive black hole binaries with circumbinary gas discs in the LISA band
• GRChombo : Numerical Relativity with Adaptive Mesh Refinement
• Shadow casted by a Konoplya-Zhidenko rotating non-Kerr black hole
• Mapping gravitational-wave backgrounds using methods from CMB analysis: Application to pulsar timing arrays
• Numerical binary black hole mergers in dynamical Chern-Simons: I. Scalar field
• Can accretion disk properties distinguish gravastars from black holes?
• Gravitational Self-Force Correction to the Binding Energy of Compact Binary Systems
• Spacetime and orbits of bumpy black holes
• The Tune of Love and the Nature(ness) of Spacetime
• Effects of neutrino-driven kicks on the supernova explosion mechanism
• Kerr black holes with self-interacting scalar hair: hairier but not heavier
• NANOGrav Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries in Circular Orbits
• Long-term observations of the pulsars in 47 Tucanae - II. Proper motions, accelerations and jerks
• A novel scheme for rapid parallel parameter estimation of gravitational waves from compact binary coalescences
• Observational Signatures of Binary Supermassive Black Holes
• Challenging the Presence of Scalar Charge and Dipolar Radiation in Binary Pulsars
• Complete waveform model for compact binaries on eccentric orbits
• Inspiralling compact binaries in quasi-elliptical orbits: The complete third post-Newtonian energy flux
• Towards adiabatic waveforms for inspiral into Kerr black holes: I. A new model of the source for the time domain perturbation equation
• The Cauchy problem of scalar-tensor theories of gravity
• Precession effect of the gravitational self-force in a Schwarzschild spacetime and the effective one-body formalism
• MOCCA-SURVEY Database I: Galactic Globular Clusters Harbouring a Black Hole Subsystem
• Anisotropic mass ejection from black hole-neutron star binaries: Diversity of electromagnetic counterparts
• A General Relativistic Null Hypothesis Test with Event Horizon Telescope Observations of the black-hole shadow in Sgr A*
• Did GW150914 produce a rotating gravastar?
• Destroying extremal Kerr-Newman black holes with test particles
• Measurability of the tidal deformability by gravitational waves from coalescing binary neutron stars
• Properties of Neutrino-driven Ejecta from the Remnant of Binary Neutron Star Merger : Purely Radiation Hydrodynamics Case
• Effective field theory calculation of conservative binary dynamics at third post-Newtonian order
• Constraints on Primordial Black Holes with Extended Mass Functions
• Collapse to Black Holes in Brans-Dicke Theory: I. Horizon Boundary Conditions for Dynamical Spacetimes
• Testing the No-Hair Theorem with Observations in the Electromagnetic Spectrum. III. Quasi-Periodic Variability
• Dynamical evolution of intermediate mass black holes and their observable signatures in the nearby Universe
• Effective field theory methods to model compact binaries
• Testing the No-Hair Theorem with Observations in the Electromagnetic Spectrum. IV. Relativistically Broadened Iron Lines
• Testing Hořava-Lifshitz gravity using thin accretion disk properties
• Transient resonances in the inspirals of point particles into black holes
• Gravitational-Wave Astronomy with Inspiral Signals of Spinning Compact-Object Binaries
• Searching For Anisotropic Gravitational-wave Backgrounds Using Pulsar Timing Arrays
• Mergers of nonspinning black-hole binaries: Gravitational radiation characteristics
• Astrophysical Violations of the Kerr Bound as a Possible Signature of String Theory
• Gravitational self-force on generic bound geodesics in Kerr spacetime
• The Formation and Gravitational-Wave Detection of Massive Stellar Black-Hole Binaries
• Destroying a near-extremal Kerr-Newman black hole
• Profiles of emission lines generated by rings orbiting braneworld Kerr black holes
• Accelerated gravitational-wave parameter estimation with reduced order modeling
• Magnetically driven winds from differentially rotating neutron stars and X-ray afterglows of short gamma-ray bursts
• Beyond the geodesic approximation: conservative effects of the gravitational self-force in eccentric orbits around a Schwarzschild black hole
• Beyond Lovelock gravity: Higher derivative metric theories
• A study of spatial correlations in pulsar timing array data
• Osculating orbits in Schwarzschild spacetime, with an application to extreme mass-ratio inspirals
• Circularization and Final Spin in Eccentric Binary Black Hole Inspirals
• Imprints of neutrino-pair flavor conversions on nucleosynthesis in ejecta from neutron-star merger remnants
• Tidal Love numbers of a slowly spinning neutron star
• Energy and periastron advance of compact binaries on circular orbits at the fourth post-Newtonian order
• Cosmography with strong lensing of LISA gravitational wave sources
• The Progenitor of GW 150914
• Matter around Kerr black holes in scalar-tensor theories: scalarization and superradiant instability
• Effective potentials and morphological transitions for binary black-hole spin precession
• Ultra-Light Dark Matter Resonates with Binary Pulsars
• Ambiguity-Free Completion of the Equations of Motion of Compact Binary Systems at the Fourth Post-Newtonian Order
• Compact binary systems in scalar-tensor gravity. II. Tensor gravitational waves to second post-Newtonian order
• Growing massive black holes through super-critical accretion of stellar-mass seeds
• Improving the sensitivity of a search for coalescing binary black holes with non-precessing spins in gravitational wave data
• Black holes and gravitational waves in models of minicharged dark matter
• Wandering Black Holes in Bright Disk Galaxy Halos
• PPN Parameter $\gamma$ and Solar System Constraints of Massive Brans-Dicke Theories
• Low metallicity and ultra-luminous X-ray sources in the Cartwheel galaxy
• Black hole formation from axion stars
• The self-consistent gravitational self-force
• Stimulated axion decay in superradiant clouds around primordial black holes
• GW150914: Spin based constraints on the merger time of the progenitor system
• Binary dynamics from spin1-spin2 coupling at fourth post-Newtonian order
• On the likelihood of detecting gravitational waves from Population III compact object binaries
• Rapidly rotating neutron stars in scalar-tensor theories of gravity
• Energy and angular momentum flow into a black hole in a binary
• Research Note: The Expected Spins of Gravitational Wave Sources With Isolated Field Binary Progenitors
• Extending the effective-one-body Hamiltonian of black-hole binaries to include next-to-next-to-leading spin-orbit couplings
• Comparison between numerical-relativity and post-Newtonian waveforms from spinning binaries: the orbital hang-up case
• Cubic order spin effects in the dynamics and gravitational wave energy flux of compact object binaries
• The influence of the hydrodynamic drag from an accretion torus on extreme mass-ratio inspirals
• Black Hole Binaries Dynamically Formed in Globular Clusters
• Gravitational Waves and Intermediate-mass Black Hole Retention in Globular Clusters
• Orbital Dynamics of Binary Boson Star Systems
• New X-ray bound on density of primordial black holes
• Mergers of binary neutron stars with realistic spin
• Resolving multiple supermassive black hole binaries with pulsar timing arrays
• Heavy spin-2 Dark Matter
• Black holes and fundamental fields in Numerical Relativity: initial data construction and evolution of bound states
• A Fourth Exception in the Calculation of Relic Abundances
• Testing gravitational parity violation with coincident gravitational waves and short gamma-ray bursts
• Is black-hole ringdown a memory of its progenitor?
• High-velocity collision of two black holes
• Comparison of Numerical and Post-Newtonian Waveforms for Generic Precessing Black-Hole Binaries
• Numerical simulations of single and binary black holes in scalar-tensor theories: circumventing the no-hair theorem
• Exotic Compact Objects and How to Quench their Ergoregion Instability
• On the ergoregion instability in rotating gravastars
• Perturbed Kerr Black Holes can probe deviations from General Relativity
• Measuring the distance-redshift relation with the cross-correlation of gravitational wave standard sirens and galaxies
• Macroscopic Effects of the Quantum Trace Anomaly
• Effects of nonlinear inhomogeneity on the cosmic expansion with numerical relativity
• Hairy black holes in the ghost-free bigravity theory
• Pathological behaviour of the scalar graviton in Hořava-Lifshitz gravity
• Characteristic Signatures in the Thermal Emission from Accreting Binary Black Holes
• High-redshift formation and evolution of central massive objects II: The census of BH seeds
• Orbital Evolution of Extreme-Mass-Ratio Black-Hole Binaries with Numerical Relativity
• The dynamics of the gravitational two-body problem at fourth post-Newtonian order and at quadratic order in the Newton constant
• Well-posedness of formulations of the Einstein equations with dynamical lapse and shift conditions
• MOCCA-SURVEY Database I: Eccentric Black Hole Mergers During Binary-Single Interactions In Globular Clusters
• A Neutron Star Binary Merger Model for GW170817/GRB170817a/SSS17a
• Dynamics, nucleosynthesis, and kilonova signature of black hole - neutron star merger ejecta
• Spectroscopic Indication for a Centi-parsec Supermassive Black Hole Binary in the Galactic Center of NGC 5548
• Multiwavelength Constraints on Pulsar Populations in the Galactic Center
• Dynamical friction and the evolution of Supermassive Black hole Binaries: the final hundred-parsec problem
• Gravitational self force and gauge transformations
• Slowly-rotating stars and black holes in dynamical Chern-Simons gravity
• Robustness of Inflation to Inhomogeneous Initial Conditions
• Foundations of an effective-one-body model for coalescing binaries on eccentric orbits
• Gravitational-wave memory and pulsar timing arrays
• Black Hole Spin Evolution: Implications for Short-hard Gamma Ray Bursts and Gravitational Wave Detection
• Analytic Solutions of the Teukolsky Equation and their Properties
• Eccentric binary black-hole mergers: The transition from inspiral to plunge in general relativity
• Massive Vector Fields in Rotating Black-Hole Spacetimes: Separability and Quasinormal Modes
• Gravitational Waves from Broken Cosmic Strings: The Bursts and the Beads
• Binary Neutron Stars with Generic Spin, Eccentricity, Mass ratio, and Compactness - Quasi-equilibrium Sequences and First Evolutions
• End Point of Black Ring Instabilities and the Weak Cosmic Censorship Conjecture
• Strong-Field Scattering of Two Black Holes: Numerics Versus Analytics
• On generic parametrizations of spinning black-hole geometries
• Common Envelope Wind Tunnel: Coefficients of Drag and Accretion in a Simplified Context for Studying Flows Around Objects Embedded Within Stellar Envelopes
• Pan-STARRS1 variability of XMM-COSMOS AGN. II. Physical correlations and power spectrum analysis
• Perturbations of Schwarzschild black holes in the Lorenz gauge: Formulation and numerical implementation
• A gravitational-wave probe of effective quantum gravity
• Isolated and Binary Neutron Stars in Dynamical Chern-Simons Gravity
• Three Dimensional MHD Simulation of Circumbinary Accretion Disks -2. Net Accretion Rate
• General relativistic viscous hydrodynamics of differentially rotating neutron stars
• Super-massive binary black holes and emission lines in active galactic nuclei
• On the local well-posedness of Lovelock and Horndeski theories
• A model for periodic blazars
• On the final fate of compact boson star mergers
• Improved methods for simulating nearly extremal binary black holes
• Tidal deformability and I-Love-Q relations for gravastars with polytropic thin shells
• Corotating and irrotational binary black holes in quasi-circular orbits
• Search for Dark Matter Effects on Gravitational Signals from Neutron Star Mergers
• Spin induced multipole moments for the gravitational wave amplitude from binary inspirals to 2.5 Post-Newtonian order
• Compact binary systems in scalar-tensor gravity. III. Scalar waves and energy flux
• Wormholes and trumpets: the Schwarzschild spacetime for the moving-puncture generation
• Improved limits for Higgs-portal dark matter from LHC searches
• Gravitational wave sources from inspiralling globular clusters in the Galactic Centre and similar environments
• Gravitational Waves from Quasi-Circular Black Hole Binaries in Dynamical Chern-Simons Gravity
• Can the string scale be related to the cosmic baryon asymmetry?
• Black holes in Lorentz-violating gravity theories
• Gravitational radiation reaction in the equations of motion of compact binaries to 3.5 post-Newtonian order
• Spherical neutron star collapse toward a black hole in tensor-scalar theory of gravity
• Thermodynamics of binary black holes and neutron stars
• Black hole hair formation in shift-symmetric generalised scalar-tensor gravity
• Gravitational-wave luminosity of binary neutron stars mergers
• Hořava Gravity after GW170817
• The First Spectroscopically Resolved Sub-parsec Orbit of a Supermassive Binary Black Hole
• Sub-radian-accuracy gravitational waveforms of coalescing binary neutron stars in numerical relativity
• Two approaches for the gravitational self force in black hole spacetime: Comparison of numerical results
• Gravitational self-force corrections to two-body tidal interactions and the effective one-body formalism
• Leading order finite size effects with spins for inspiralling compact binaries
• Scalar Collapse in AdS
• Post-Newtonian and Numerical Calculations of the Gravitational Self-Force for Circular Orbits in the Schwarzschild Geometry
• Second Order Gravitational Self-Force
• Overspinning a Kerr black hole: the effect of self-force
• Nonlinear Evolution and Final Fate of Charged Anti-de Sitter Black Hole Superradiant Instability
• Towards adiabatic waveforms for inspiral into Kerr black holes: II. Dynamical sources and generic orbits
• Dark Matter Halos in Galaxies and Globular Cluster Populations. II: Metallicity and Morphology
• Gravitational waves from intermediate-mass-ratio inspirals for ground-based detectors
• Next-to-next-to-leading order spin-orbit effects in the equations of motion of compact binary systems
• Remnant of binary black-hole mergers: New simulations and peak luminosity studies
• POINT-AGAPE Pixel Lensing Survey of M31 : Evidence for a MACHO contribution to Galactic Halos
• Self-force of a scalar field for circular orbits about a Schwarzschild black hole
• Tail effects in the third post-Newtonian gravitational wave energy flux of compact binaries in quasi-elliptical orbits
• Tidal coupling of a Schwarzschild black hole and circularly orbiting moon
• The High Time Resolution Universe Pulsar Survey - XIII. PSR J1757-1854, the most accelerated binary pulsar
• The One-Armed Spiral Instability in Neutron Star Mergers and its Detectability in Gravitational Waves
• Derivation of local-in-time fourth post-Newtonian ADM Hamiltonian for spinless compact binaries
• Interaction between bosonic dark matter and stars
• The chemical composition of the Sun from helioseismic and solar neutrino data
• Self force on particle in orbit around a black hole
• Spin effects on gravitational waves from inspiraling compact binaries at second post-Newtonian order
• Nonrotating black hole in a post-Newtonian tidal environment
• Black hole evolution by spectral methods
• Black hole spectroscopy with coherent mode stacking
• Neutron star transition to strong-scalar-field state in tensor scalar gravity
• Spin induced multipole moments for the gravitational wave flux from binary inspirals to third Post-Newtonian order
• Gravitational Self-force in a Radiation Gauge
• I-Love-Q relations for a gravastar and the approach to the black-hole limit
• Projected Constraints on Scalarization with Gravitational Waves from Neutron Star Binaries
• Prompt Shocks in the Gas Disk Around a Recoiling Supermassive Black Hole Binary
• Probing stellar binary black hole formation in galactic nuclei via the imprint of their center of mass acceleration on their gravitational wave signal
• Formation of High Mass X-ray Black Hole Binaries
• Dancing to ChaNGa: A Self-Consistent Prediction For Close SMBH Pair Formation Timescales Following Galaxy Mergers
• Detecting triple systems with gravitational wave observations
• Bar-mode instability of rapidly spinning black hole in higher dimensions: Numerical simulation in general relativity
• Next-to-next-to-leading order gravitational spin-squared potential via the effective field theory for spinning objects in the post-Newtonian scheme
• Accretion disks around binary black holes of unequal mass: GRMHD simulations of postdecoupling and merger
• Gravitational waves and mass ejecta from binary neutron star mergers: Effect of the stars' rotation
• Dimensional regularization of local singularities in the 4th post-Newtonian two-point-mass Hamiltonian
• Interactions between multiple supermassive black holes in galactic nuclei: a solution to the final parsec problem
• Equivalence of ADM Hamiltonian and Effective Field Theory approaches at next-to-next-to-leading order spin1-spin2 coupling of binary inspirals
• Equation of motion for relativistic compact binaries with the strong field point particle limit: Third post-Newtonian order
• Black Hole-Neutron Star Mergers with a Hot Nuclear Equation of State: Outflow and Neutrino-Cooled Disk for a Low-Mass, High-Spin Case
• Black holes with massive graviton hair
• Reduced basis catalogs for gravitational wave templates
• Numerical relativity reaching into post-Newtonian territory: a compact-object binary simulation spanning 350 gravitational-wave cycles
• Gravitational waveforms in scalar-tensor gravity at 2PN relative order
• The Infrared Afterglow of Supermassive Black Hole Mergers
• One-arm Spiral Instability in Hypermassive Neutron Stars Formed by Dynamical-Capture Binary Neutron Star Mergers
• Using long-term millisecond pulsar timing to obtain physical characteristics of the bulge globular cluster Terzan 5
• Testing Chern-Simons Modified Gravity with Gravitational-Wave Detections of Extreme-Mass-Ratio Binaries
• The Globular Cluster Migratory Origin of Nuclear Star Clusters
• Direct formation of supermassive black holes in metal-enriched gas at the heart of high-redshift galaxy mergers
• Tidal deformation of a slowly rotating black hole
• Explaining LIGO's observations via isolated binary evolution with natal kicks
• Detection of Possible Quasi-periodic Oscillations in the Long-term Optical Light Curve of the BL Lac Object OJ 287
• Black Hole Solutions in String Theory with Gauss-Bonnet Curvature Correction
• Highly eccentric inspirals into a black hole
• Testing Gravity with Quasi Periodic Oscillations from accreting Black Holes: the Case of Einstein-Dilaton-Gauss-Bonnet Theory
• Beyond Concordance Cosmology with Magnification of Gravitational-Wave Standard Sirens
• Primordial Black Holes as Dark Matter: Converting Constraints from Monochromatic to Extended Mass Distributions
• Dark stars: gravitational and electromagnetic observables
• Center-of-Mass Equations of Motion and Conserved Integrals of Compact Binary Systems at the Fourth Post-Newtonian Order
• Mass and spin coevolution during the alignment of a black hole in a warped accretion disc
• The binary black-hole dynamics at the third-and-a-half post-Newtonian order in the ADM-formalism
• Slowly rotating black holes in Horava-Lifshitz gravity
• Are we there yet? Time to detection of nanohertz gravitational waves based on pulsar-timing array limits
• High-order post-Newtonian contributions to the two-body gravitational interaction potential from analytical gravitational self-force calculations
• Simulation of Asymptotically AdS5 Spacetimes with a Generalized Harmonic Evolution Scheme
• An Efficient Numerical Method for Computing Gravitational Waves Induced by a Particle Moving on Eccentric Inclined Orbits around a Kerr Black Hole
• Search for intermediate mass black hole binaries in the first observing run of Advanced LIGO
• Multipole expansion at the level of the action
• Computing inspirals in Kerr in the adiabatic regime. I. The scalar case
• Self-accelerating cosmologies and hairy black holes in ghost-free bigravity and massive gravity
• Final spin and radiated energy in numerical simulations of binary black holes with equal masses and equal, aligned or anti-aligned spins
• Scalarized Hairy Black Holes
• On the Apparent Ambiguities in the Post-Newtonian Expansion for Binary Systems
• MOND habitats within the solar system
• Iron K$\alpha$ line of Kerr black holes with scalar hair
• Gravitational scattering of two black holes at the fourth post-Newtonian approximation
• Kerr black holes with synchronised hair: an analytic model and dynamical formation
• Gravitational waves from extreme mass-ratio inspirals in Dynamical Chern-Simons gravity
• Quasi-Periodic Behavior of Mini-Disks in Binary Black Holes Approaching Merger
• Black hole mergers: the first light
• Gravitational Self-Force Correction to the Innermost Stable Circular Equatorial Orbit of a Kerr Black Hole
• On choosing the start time of binary black hole ringdown
• Extra-Large Remnant Recoil Velocities and Spins from Near-Extremal-Bowen-York-Spin Black-Hole Binaries
• Late Inspiral and Merger of Binary Black Holes in Scalar-Tensor Theories of Gravity
• Spontaneous growth of vector fields in gravity
• Matched Filtering of Numerical Relativity Templates of Spinning Binary Black Holes
• Perspective on gravitational self-force analyses
• Nonlinear gravitational self-force: second-order equation of motion
• EMRI corrections to the angular velocity and redshift factor of a mass in circular orbit about a Kerr black hole
• Black holes in vector-tensor theories
• Gravitational spin-orbit coupling in binary systems, post-Minkowskian approximation and effective one-body theory
• Ultrarelativistic black hole formation
• Dynamical Formation of Low-Mass Merging Black Hole Binaries like GW151226
• Myers-Perry black holes with scalar hair and a mass gap
• On the detectability of dual jets from binary black holes
• A supermassive binary black hole with triple disks
• Constraining early and interacting dark energy with gravitational wave standard sirens: the potential of the eLISA mission
• Nonlinear interactions between black holes and Proca fields
• Black Hole Dynamics in Einstein-Maxwell-Dilaton Theory
• Tail terms in gravitational radiation reaction via effective field theory
• Theory of gravitation theories: a no-progress report
• Regularization of fields for self-force problems in curved spacetime: foundations and a time-domain application
• Stability of a black hole and the speed of gravity waves within self-tuning cosmological models
• Swift coalescence of supermassive black holes in cosmological mergers of massive galaxies
• Accretion of dark matter by stars
• Nonviolent information transfer from black holes: a field theory parameterization
• Binary super-massive black hole environments diminish the gravitational-wave signal in the pulsar timing band
• Hairy black-hole solutions in generalized Proca theories
• Gravitational waves and stalled satellites from massive galaxy mergers at z <= 1
• Slowly rotating black holes in Einstein-æther theory
• Metric perturbations produced by eccentric equatorial orbits around a Kerr black hole
• The adiabatic evolution of orbital parameters in the Kerr spacetime
• Analytical high-order post-Newtonian expansions for extreme mass ratio binaries
• The Initial Value Formulation of Dynamical Chern-Simons Gravity
• Gravitational self-torque and spin precession in compact binaries
• A comment on AdS collapse of a scalar field in higher dimensions
• Numerical evolutions of spherical Proca stars
• Mini-dark halos with intermediate mass black holes
• Modeling multipolar gravitational-wave emission from small mass-ratio mergers
• Million-Body Star Cluster Simulations: Comparisons between Monte Carlo and Direct $N$-body
• Formation and Coalescence of Cosmological Supermassive Black Hole Binaries in Supermassive Star Collapse
• Cosmic Black-Hole Hair Growth and Quasar OJ287
• Testing the binary hypothesis: pulsar timing constraints on supermassive black hole binary candidates
• Equation of motion for relativistic compact binaries with the strong field point particle limit : the second and half post-Newtonian order
• Conservative, gravitational self-force for a particle in circular orbit around a Schwarzschild black hole in a Radiation Gauge
• Orbital fingerprints of ultralight scalar fields around black holes
• Barbero-Immirzi field in canonical formalism of pure gravity
• Massive black hole pairs in clumpy, self-gravitating circumnuclear disks: stochastic orbital decay
• Gravitational waves from black hole binary inspiral and merger: The span of third post-Newtonian effective-one-body templates
• Cosmology with space-based gravitational-wave detectors --- dark energy and primordial gravitational waves ---
• Quasi-normal modes and exponential energy decay for the Kerr-de Sitter black hole
• Neutron star mergers as a probe of modifications of general relativity with finite-range scalar forces
• Effective one body Hamiltonian of two spinning black-holes with next-to-next-to-leading order spin-orbit coupling
• A numerical study of vector resonant relaxation
• Towards accurate cosmological predictions for rapidly oscillating scalar fields as dark matter
• Higher-order-in-spin interaction Hamiltonians for binary black holes from Poincaré invariance
• A Parameter Estimation Method that Directly Compares Gravitational Wave Observations to Numerical Relativity
• Towards the 4th post-Newtonian Hamiltonian for two-point-mass systems
• Exploring intermediate and massive black-hole binaries with the Einstein Telescope
• Computing the gravitational self-force on a compact object plunging into a Schwarzschild black hole
• A Modern Approach to Superradiance
• Fixing extensions to General Relativity in the non-linear regime
• Probing cosmic anisotropy with gravitational waves as standard sirens
• LISA sources in Milky Way globular clusters
• Quasi-normal modes of black holes in Horndeski gravity
• The Effect of Massive Perturbers on Extreme Mass-Ratio Inspiral Waveforms
• Powerful flares from recoiling black holes in quasars
• The Influence of Neutrinos on r-Process Nucleosynthesis in the Ejecta of Black Hole-Neutron Star Mergers
• Evidence for an intermediate-mass black hole in the globular cluster NGC 6624
• A new analytic representation of the ringdown waveform of coalescing spinning black hole binaries
• Evidence for periodicity in 43 year-long monitoring of NGC 5548
• I-Love-Q anisotropically: Universal relations for compact stars with scalar pressure anisotropy
• Electromagnetic signals following stellar-mass black hole mergers
• General Relativistic Magnetohydrodynamic Simulations of Binary Neutron Star Mergers with the APR4 Equation of State
• Scalar gravitational wave from Oppenheimer-Snyder collapse in scalar- tensor theories of gravity
• Systematic Study of Event Horizons and Pathologies of Parametrically Deformed Kerr Spacetimes
• Constraining the Solution to the Last Parsec Problem with Pulsar Timing
• Next-to-next-to-leading order gravitational spin-orbit coupling via the effective field theory for spinning objects in the post-Newtonian scheme
• Self-force as a cosmic censor
• Gravitational self-force from radiation-gauge metric perturbations
• Reconstructing the dark sector interaction with LISA
• Forced motion near black holes
• End Point of the Ultraspinning Instability and Violation of Cosmic Censorship
• Electromagnetic counterparts of supermassive black hole binaries resolved by pulsar timing arrays
• The effect of matter structure on the gravitational waveform
• Tidal heating and torquing of a Kerr black hole to next-to-leading order in the tidal coupling
• Hidden universality in the merger rate distribution in the primordial black hole scenario
• Higher-order-in-spin interaction Hamiltonians for binary black holes from source terms of Kerr geometry in approximate ADM coordinates
• Supplement: The Rate of Binary Black Hole Mergers Inferred from Advanced LIGO Observations Surrounding GW150914
• New conformally flat initial data for spinning black holes
• Cosmological inference using only gravitational wave observations of binary neutron stars
• Dynamical scalar hair formation around a Schwarzschild black hole
• Modeling of Emission Signatures of Massive Black Hole Binaries: I Methods
• Spinning test-body orbiting around Schwarzschild black hole: circular dynamics and gravitational-wave fluxes
• Exploring New Physics Frontiers Through Numerical Relativity
• Post-Kerr black hole spectroscopy
• Dynamical formation of a Reissner-Nordström black hole with scalar hair in a cavity
• Matter Neutrino Resonance Transitions above a Neutron Star Merger Remnant
• Orbital Decay of Supermassive Black Hole Binaries in Clumpy Multiphase Merger Remnants
• Mechanics of extended masses in general relativity
• A practical, covariant puncture for second-order self-force calculations
• Parameter estimation of gravitational wave echoes from exotic compact objects
• Key Elements of Robustness in Binary Black Hole Evolutions using Spectral Methods
• Two-body gravitational spin-orbit interaction at linear order in the mass ratio
• Henize 2-10: the ongoing formation of a nuclear star cluster around a massive black hole
• Search for Gravitational Waves Associated with Gamma-Ray Bursts During the First Advanced LIGO Observing Run and Implications for the Origin of GRB 150906B
• Black hole merger estimates in Einstein-Maxwell and Einstein-Maxwell-dilaton gravity
• Dimensional regularization of the IR divergences in the Fokker action of point-particle binaries at the fourth post-Newtonian order
• Gravitational wave parameter estimation with compressed likelihood evaluations
• The Cauchy problem of f(R) gravity
• Scalar-field perturbations from a particle orbiting a black hole using numerical evolution in 2+1 dimensions
• Scalar self-force on eccentric geodesics in Schwarzschild spacetime: a time-domain computation
• Nonlinear gravitational self-force. I. Field outside a small body
• Constraint on the abundance of primordial black holes in dark matter from Planck data
• The numerical relativity breakthrough for binary black holes
• Spherical Boson Stars as Black Hole mimickers
• An overview of the second round of the Mock LISA Data Challenges
• CMB constraints on primordial black hole dark matter
• Limits on anisotropy in the nanohertz stochastic gravitational-wave background
• Evolution of small-mass-ratio binaries with a spinning secondary
• Gravitational radiation reaction and second order perturbation theory
• No Slip Gravity
• Dynamical evolution of fermion-boson stars
• Constructing quasi-equilibrium initial data for binary neutron stars with arbitrary spins
• Instability of hairy black holes in shift-symmetric Horndeski theories
• Pulsar-black hole binaries: prospects for new gravity tests with future radio telescopes
• Next-to-next-to-leading order post-Newtonian linear-in-spin binary Hamiltonians
• Delensing Gravitational Wave Standard Sirens with Shear and Flexion Maps
• Finding high-order analytic post-Newtonian parameters from a high-precision numerical self-force calculation
• Effective stability against superradiance of Kerr black holes with synchronised hair
• Detection of gamma rays of likely jet origin in Cygnus X-1
• Gravitational self-force on eccentric equatorial orbits around a Kerr black hole
• Star-disc interaction in galactic nuclei: orbits and rates of accreted stars
• Minidisks in Binary Black Hole Accretion
• Black Hole Universe: Time Evolution
• Third post-Newtonian gravitational waveforms for compact binary systems in general orbits: Instantaneous terms
• Self force on a scalar charge in Kerr spacetime: circular equatorial orbits
• Solutions in the generalized Proca theory with the nonminimal coupling to the Einstein tensor
• Tensor-multi-scalar theories: relativistic stars and 3+1 decomposition
• Evolution of a periodic eight-black-hole lattice in numerical relativity
• Self-force corrections to the periapsis advance around a spinning black hole
• Tidal invariants for compact binaries on quasi-circular orbits
• Overcharging higher-dimensional black holes with point particles
• First Law of Mechanics for Compact Binaries on Eccentric Orbits
• Next-to-leading tail-induced spin-orbit effects in the gravitational radiation flux of compact binaries
• Particle on the Innermost Stable Circular Orbit of a Rapidly Spinning Black Hole
• Testing the Magnetar Model via Late Time Radio Observations of Two Macronova Candidates
• Multi-wavelength Observations of the Binary System PSR B1259-63/LS~2883 around the 2014 Periastron Passage
• Periastron Advance in Spinning Black Hole Binaries: Gravitational Self-Force from Numerical Relativity
• Numerical relativity for D dimensional space-times: head-on collisions of black holes and gravitational wave extraction
• Importance of transient resonances in extreme-mass-ratio inspirals
• Completion of metric reconstruction for a particle orbiting a Kerr black hole
• Symmetric and Standard Matter-Neutrino Resonances Above Merging Compact Objects
• A Systematic Search for Periodically Varying Quasars in Pan-STARRS1: An Extended Baseline Test in Medium Deep Survey Field MD09
• Monte-Carlo closure for moment-based transport schemes in general relativistic radiation hydrodynamics simulations
• A morphology-independent data analysis method for detecting and characterizing gravitational wave echoes
• A compact pulsar wind nebula model of the gamma-ray loud binary LS I +61 303
• Self force on a scalar charge in Kerr spacetime: eccentric equatorial orbits
• Constraints On The Dynamical Environments Of Supermassive Black-hole Binaries Using Pulsar-timing Arrays
• Nonviolent unitarization: basic postulates to soft quantum structure of black holes
• Implications of the low binary black hole aligned spins observed by LIGO
• The Neutrino Bubble Instability: A Mechanism for Generating Pulsar Kicks
• Gravitational-Wave Localization Alone Probes AGN Origin of Stellar-Mass Black Hole Mergers
• Radiation-reaction force on a particle plunging into a black hole
• An advanced leakage scheme for neutrino treatment in astrophysical simulations
• Perturbed disks get shocked. Binary black hole merger effects on accretion disks
• Globally regular instability of $Ad{S}_3$
• Hořava gravity is asymptotically free (in 2+1 dimensions)
• Accuracy of Estimating Highly Eccentric Binary Black Hole Parameters with Gravitational-Wave Detections
• Gravitational waves with dark matter minispikes: the combined effect
• Relativistic mergers of black hole binaries have large, similar masses, low spins and are circular
• Spinning test-body orbiting around a Kerr black hole: circular dynamics and gravitational-wave fluxes
• Shadows of CPR black holes and tests of the Kerr metric
• m-Mode Regularization Scheme for the Self Force in Kerr Spacetime
• Numerical relativity for D dimensional axially symmetric space-times: formalism and code tests
• Integration of inhomogeneous cosmological spacetimes in the BSSN formalism
• Frequency-domain calculation of the self force: the high-frequency problem and its resolution
• Gravitational-wave signatures of the absence of an event horizon. II. Extreme mass ratio inspirals in the spacetime of a thin-shell gravastar
• Stellar binary black holes in the LISA band: a new class of standard sirens
• Accretion Disk Assembly During Common Envelope Evolution: Implications for Feedback and LIGO Binary Black Hole Formation
• Black Hole Superradiance in Dynamical Spacetime
• Black holes and solitons in an extended Proca theory
• Constraining the dark energy equation of state using LISA observations of spinning Massive Black Hole binaries
• Revealing the formation of stellar-mass black hole binaries: The need for deci-Hertz gravitational wave observatories
• A spinning supermassive black hole binary model consistent with VLBI observations of the S5 1928+738 jet
• Gravity and Scalar Fields
• Scalar field self-force effects on orbits about a Schwarzschild black hole
• Next-to-next-to-leading order post-Newtonian spin-orbit Hamiltonian for self-gravitating binaries
• Gravity Waves from Extreme-Mass-Ratio Plunges into Kerr Black Holes
• Black hole kicks as new gravitational wave observables
• The fate of central black holes in merging galaxies
• Self-consistent orbital evolution of a particle around a Schwarzschild black hole
• Radiation reaction for spinning bodies in effective field theory II: Spin-spin effects
• Supermassive black hole pairs in clumpy galaxies at high redshift: delayed binary formation and concurrent mass growth
• Next-to-next-to-leading order post-Newtonian spin(1)-spin(2) Hamiltonian for self-gravitating binaries
• Self-force via $m$-mode regularization and 2+1D evolution: III. Gravitational field on Schwarzschild spacetime
• Gravitational-wave emission in shift-symmetric Horndeski theories
• Gravitational perturbations and metric reconstruction: Method of extended homogeneous solutions applied to eccentric orbits on a Schwarzschild black hole
• Black-hole kicks from numerical-relativity surrogate models
• Double Binary Pulsar Test of Dynamical Chern-Simons Modified Gravity
• Radiation reaction for spinning bodies in effective field theory I: Spin-orbit effects
• Radio Constraints on Long-Lived Magnetar Remnants in Short Gamma-Ray Bursts
• High-order expansions of the Detweiler-Whiting singular field in Schwarzschild spacetime
• First Law of Mechanics for Black Hole Binaries with Spins
• High-energy gamma-rays from Cyg X-1
• Where does the physics of extreme gravitational collapse reside?
• Resonantly enhanced and diminished strong-field gravitational-wave fluxes
• A search for cyclical sources of gamma-ray emission on the period range from days to years in the Fermi-LAT sky
• Gravitational Waves in Cold Dark Matter
• Comparison Between Self-Force and Post-Newtonian Dynamics: Beyond Circular Orbits
• Rapidly rotating black holes in dynamical Chern-Simons gravity: Decoupling limit solutions and breakdown
• Quasiequilibrium sequences of binary neutron stars undergoing dynamical scalarization
• Gamma-ray and optical oscillations in the blazar PKS 0537-441
• IC10~X-1/NGC300~X-1: the very immediate progenitors of BH-BH binaries
• Gravitational-wave cosmography with LISA and the Hubble tension
• Neutrino Flavor Evolution in Binary Neutron Star Merger Remnants
• The Formation of Stellar Black Holes
• Approximate Waveforms for Extreme-Mass-Ratio Inspirals in Modified Gravity Spacetimes
• Gravity Waves from Kerr/CFT
• Gravitational wave sources in the era of multi-frequency gravitational wave astronomy
• The $m=1$ instability \& gravitational wave signal in binary neutron star mergers
• Gravitational-wave tail effects to quartic non-linear order
• Conformal and covariant Z4 formulation of the Einstein equations: strongly hyperbolic first-order reduction and solution with discontinuous Galerkin schemes
• On horizon structure of bimetric spacetimes
• Hyperbolicity of scalar-tensor theories of gravity
• Primordial Black Holes: sirens of the early Universe
• Analytic self-force calculations in the post-Newtonian regime: eccentric orbits on a Schwarzschild background
• Second-order gravitational self-force
• Asymptotics of linear waves and resonances with applications to black holes
• Superradiance in rotating stars and pulsar-timing constraints on dark photons
• Probing Gravitational Parity Violation with Gravitational Waves from Stellar-mass Black Hole Binaries
• The birth of a supermassive black hole binary
• Introductory lectures on the Effective One Body formalism
• Universality, maximum radiation and absorption in high-energy collisions of black holes with spin
• Is super-Planckian physics visible? -- Scattering of black holes in 5 dimensions
• General theories of linear gravitational perturbations to a Schwarzschild Black Hole
• Astrophysical uncertainties on stellar microlensing constraints on multi-Solar mass primordial black hole dark matter
• Phenomenology of Production and Decay of Spinning Extra-Dimensional Black Holes at Hadron Colliders
• Black-hole production from ultrarelativistic collisions
• Anisotropies of gravitational-wave standard sirens as a new cosmological probe without redshift information
• A Pseudospectral Method for Gravitational Wave Collapse
• Frequency-domain algorithm for the Lorenz-gauge gravitational self-force
• Gravitational Radiations from a Spinning Compact Object around a supermassive Kerr black hole in circular orbit
• Confirming and improving post-Newtonian and effective-one-body results from self-force computations along eccentric orbits around a Schwarzschild black hole
• ALMA and GMRT constraints on the off-axis gamma-ray burst 170817A from the binary neutron star merger GW170817
• Conditions for Sustained Orbital Resonances in Extreme Mass Ratio Inspirals
• Neutrino pair annihilation above merger remnants: implications of a long-lived massive neutron star
• Influence of conservative corrections on parameter estimation for extreme-mass-ratio inspirals
• Status of black-hole-binary simulations for gravitational-wave detection
• On the possibility of setting a new constraint to scalar-tensor theories
• Supplement: Localization and broadband follow-up of the gravitational-wave transient GW150914
• Applying the effective-source approach to frequency-domain self-force calculations: Lorenz-gauge gravitational perturbations
• Inference on gravitational waves from coalescences of stellar-mass compact objects and intermediate-mass black holes
• Tracing the redshift evolution of Hubble parameter with gravitational-wave standard sirens
• Dynamics of Quadruple Systems Composed of Two Binaries: Stars, White Dwarfs, and Implications for Ia Supernovae
• Analytical high-order post-Newtonian expansions for spinning extreme mass ratio binaries
• Precessional instability in binary black holes with aligned spins
• Mode-sum regularization of the scalar self-force: Formulation in terms of a tetrad decomposition of the singular field
• Static and rotating solutions for Vector-Galileon theories
• Second-order perturbation theory: problems on large scales
• The w-mode instability of ultracompact relativistic stars
• Rotating black holes in three-dimensional Hořava gravity
• Constraining scalar-tensor theories of gravity from the most massive neutron stars
• Hamiltonian Formulation of the Conservative Self-Force Dynamics in the Kerr Geometry
• Are Globular Clusters the Remnant Nuclei of Progenitor Disk Galaxies?
• Cosmological signatures of ultralight dark matter with an axionlike potential
• Modeling dynamical scalarization with a resummed post-Newtonian expansion
• A Fast Frequency-Domain Algorithm for Gravitational Self-Force: I, Circular Orbits in Schwarzschild Spacetime
• Stability analysis of black holes in massive gravity: a unified treatment
• A new look at microlensing limits on dark matter in the Galactic halo
• Inspiral into Gargantua
• Discontinuous Galerkin method for computing gravitational waveforms from extreme mass ratio binaries
• Numerical simulations of stellar collapse in scalar-tensor theories of gravity
• Long-lived inverse chirp signals from core collapse in massive scalar-tensor gravity
• Star-disc interaction in galactic nuclei: formation of a central stellar disc
• Higher-dimensional numerical relativity: Formulation and code tests
• Testing the Kerr metric with the iron line and the KRZ parametrization
• Self-Force and Green Function in Schwarzschild spacetime via Quasinormal Modes and Branch Cut
• Gyroscopes orbiting black holes: A frequency-domain approach to precession and spin-curvature coupling for spinning bodies on generic Kerr orbits
• Observing the Galaxy's massive black hole with gravitational wave bursts
• Spin-multipole effects in binary black holes and the test-body limit
• Disk Emission from Magneto-hydrodynamic Simulations of Spinning Black Holes
• Gravitational waves from the collapse and bounce of a stellar core in tensor-scalar gravity
• Maximum redshift of gravitational wave merger events
• On the local structure of spacetime in ghost-free bimetric theory and massive gravity
• The Penrose process, superradiance and ergoregion instabilities
• Evolution of the stellar-merger red nova V1309 Scorpii: SED analysis
• Analytic determination of the eight-and-a-half post-Newtonian self-force contributions to the two-body gravitational interaction potential
• Spin flips in generic black hole binaries
• Uniqueness of smooth stationary black holes in vacuum: small perturbations of the Kerr spaces
• Lower-dimensional Horava-Lifshitz gravity
• Observing the dynamics of super-massive black hole binaries with Pulsar Timing Arrays
• Scalar Hairy Black Holes in Four Dimensions are Unstable
• Second-order perturbation theory: the problem of infinite mode coupling
• On the four-loop static contribution to the gravitational interaction potential of two point masses
• Condensate of Massive Graviton and Dark Matter
• Extremal Black Holes in Dynamical Chern-Simons Gravity
• Black Hole Universe with $\Lambda$
• On the hyperbolicity of the most general Horndeski theory
• A proof of Friedman's ergosphere instability for scalar waves
• Late time cosmology with LISA: probing the cosmic expansion with massive black hole binary mergers as standard sirens
• Characterization of echoes: A Dyson-series representation of individual pulses
• The role of weak interactions in dynamic ejecta from binary neutron star mergers
• Self force on a scalar charge in the spacetime of a stationary, axisymmetric black hole
• New gravitational self-force analytical results for eccentric orbits around a Schwarzschild black hole
• Tidal acceleration of black holes and superradiance
• Projected constraints on the cosmic (super)string tension with future gravitational wave detection experiments
• Cosmological Perturbations of Extreme Axion in the Radiation Era
• The effect of small inter-pulsar distance variations in stochastic gravitational wave background searches with Pulsar Timing Arrays
• Convective Excitation of Inertial Modes in Binary Neutron Star Mergers
• An Efficient Pseudospectral Method for the Computation of the Self-force on a Charged Particle: Circular Geodesics around a Schwarzschild Black Hole
• Lorenz gauge gravitational self-force calculations of eccentric binaries using a frequency domain procedure
• Self-force with (3+1) codes: a primer for numerical relativists
• Modulated Hawking radiation and a nonviolent channel for information release
• Orbital resonances around Black holes
• Analytic determination of high-order post-Newtonian self-force contributions to gravitational spin precession
• $N-$body dynamics of Intermediate mass-ratio inspirals in globular clusters
• Fundamental physics and cosmology with LISA
• Resonantly enhanced kicks from equatorial small mass-ratio inspirals
• LISA observations of massive black hole mergers: event rates and issues in waveform modelling
• Black holes as bubbles of AdS
• Excited Boson Stars
• Self force via $m$-mode regularization and 2+1D evolution: II. Scalar-field implementation on Kerr spacetime
• Head-on collisions of unequal mass black holes in D=5 dimensions
• Performance of an externally triggered gravitational-wave burst search
• Pseudospectral Collocation Methods for the Computation of the Self-Force on a Charged Particle: Generic Orbits around a Schwarzschild Black Hole
• Tidal interaction of black holes and Newtonian viscous bodies
• Simulation of Black Hole Collisions in Asymptotically AdS Spacetimes
• Spin-orbit precession for eccentric black hole binaries at first order in the mass ratio
• Measurement of Hubble constant with stellar-mass binary black holes
• Astrophysical constraints on massive black hole binary evolution from Pulsar Timing Arrays
• Weak lensing effects in the measurement of the dark energy equation of state with LISA
• Spin-orbit precession along eccentric orbits for extreme mass ratio black hole binaries and its effective-one-body transcription
• Neutrino Flavor Evolution in Neutron Star Mergers
• When black holes collide: Probing the interior composition by the spectrum of ringdown modes and emitted gravitational waves
• Linear-in-mass-ratio contribution to spin precession and tidal invariants in Schwarzschild spacetime at very high post-Newtonian order
• High Energy Collisions of Black Holes Numerically Revisited
• Iron K$\alpha$ line of boson stars
• Detweiler's gauge-invariant redshift variable: analytic determination of the nine and nine-and-a-half post-Newtonian self-force contributions
• Multi-messenger approaches to binary supermassive black holes in the "continuous-wave" regime
• Solar System Constraints on Scalar-Tensor Gravity with Positive Coupling Constant upon Cosmological Evolution of the Scalar Field
• Binary pulsars as dark-matter probes
• Locating the intense interstellar scattering towards the inner Galaxy
• Dynamical shift conditions for the Z4 and BSSN hyperbolic formalisms
• Seeking the Loop Quantum Gravity Barbero-Immirzi Parameter and Field in 4D, $\mathcal{N}$ = 1 Supergravity
• A conservative effect of the second-order gravitational self-force on quasicircular orbits in Schwarzschild spacetime
• Emission Signatures from Sub-parsec Binary Supermassive Black Holes I: Diagnostic Power of Broad Emission Lines
• Singular perturbation techniques in the gravitational self-force problem
• Gravitational-wave flux for a particle orbiting a Kerr black hole to 20th post-Newtonian order: a numerical approach
• Possible imprints of cosmic strings in the shadows of galactic black holes
• Self-force via Green functions and worldline integration
• A no-hair theorem for stars in Horndeski theories
• Half-integral conservative post-Newtonian approximations in the redshift factor of black hole binaries
• Revisiting the double-binary-pulsar probe of non-dynamical Chern-Simons gravity
• Spin-dependent two-body interactions from gravitational self-force computations
• Gravitating binaries at 5PN in the post-Minkowskian approximation
• Experimental mathematics meets gravitational self-force
• Fast plunges into Kerr black holes
• Probing the assembly history and dynamical evolution of massive black hole binaries with pulsar timing arrays
• Peeling of the Weyl tensor and gravitational radiation in higher dimensions
• The mass and angular momentum of reconstructed metric perturbations
• Post-Newtonian gravitational radiation and equations of motion via direct integration of the relaxed Einstein equations. V. Evidence for the strong equivalence principle to second post-Newtonian order
• Applying the effective-source approach to frequency-domain self-force calculations
• First Law of Compact Binary Mechanics with Gravitational-Wave Tails
• Isotropic-Nematic Phase Transitions in Gravitational Systems
• Quasi-periodic oscillations as a tool for testing the Kerr metric: A comparison with gravitational waves and iron line
• First gamma-rays from galaxy clusters. Preliminary evidence of the association of galaxy clusters with EGRET unidentified gamma-ray sources
• Covariant Effective Action for Loop Quantum Cosmology from Order Reduction
• Puncture Initial Data for Black-Hole Binaries with High Spins and High Boosts
• The Maximal-Density Mass Function for Primordial Black Hole Dark Matter
• Modelling gravitational waves from precessing black-hole binaries: Progress, challenges and prospects
• Impact of the second order self-forces on the dephasing of the gravitational waves from quasi-circular extreme mass-ratio inspirals
• Note on a new parametrization for testing the Kerr metric
• Hairy black holes in theories with massive gravitons
• Gas squeezing during the merger of a supermassive black hole binary
• Are gravitational wave ringdown echoes always equal-interval ?
• Gravitational waves from plunges into Gargantua
• High post-Newtonian order gravitational self-force analytical results for eccentric orbits around a Kerr black hole
• Intermediate-mass-ratio-inspirals in the Einstein Telescope: I. Signal-to-noise ratio calculations
• High-order expansions of the Detweiler-Whiting singular field in Kerr spacetime
• Intermediate-mass-ratio-inspirals in the Einstein Telescope. II. Parameter estimation errors
• Numerical computation of the EOB potential q using self-force results
• Gauge Invariant Perturbations of the Schwarzschild Spacetime
• Redshift factor and the first law of binary black hole mechanics in numerical simulations
• Reconstructing the Properties of Dark Energy using Standard Sirens
• Gauge and motion in perturbation theory
• Self force via m-mode regularization and 2+1D evolution: Foundations and a scalar-field implementation on Schwarzschild
• Gravitational waves from extreme mass ratio inspirals around bumpy black holes
• Hairy black hole solutions in $U(1)$ gauge-invariant scalar-vector-tensor theories
• Constraining Black Holes with Light Boson Hair and Boson Stars using Epicyclic Frequencies and QPOs
• A matched expansion approach to practical self-force calculations
• Probing the spinning of the massive black hole in the Galactic Center via pulsar timing: A Full Relativistic Treatment
• Metric perturbations from eccentric orbits on a Schwarzschild black hole: I. Odd-parity Regge-Wheeler to Lorenz gauge transformation and two new methods to circumvent the Gibbs phenomenon
• Towards beating the curse of dimensionality for gravitational waves using Reduced Basis
• No tension between assembly models of supermassive black hole binaries and pulsar observations
• Quasi-local contribution to the scalar self-force: Geodesic Motion
• Non-Singular Black Holes in Massive Gravity: Time-Dependent Solutions
• The Black Hole Candidate LSI+61303
• Self force on a scalar charge in Kerr spacetime: inclined circular orbits
• New Features of Gravitational Collapse in Anti-de Sitter Spacetimes
• Generic effective source for scalar self-force calculations
• Observing Supermassive Black Holes across cosmic time: from phenomenology to physics
• The mass discrepancy-acceleration relation: a universal maximum dark matter acceleration and implications for the ultra-light scalar field dark matter model
• Black holes with vector hair
• Radiation reaction in the 2.5PN waveform from inspiralling binaries in circular orbits
• Fast spectral source integration in black hole perturbation calculations
• Light propagation through black-hole lattices
• Scalar self-force for highly eccentric equatorial orbits in Kerr spacetime
• Light Primordial Exotic Compact Objects as All Dark Matter
• Observational evidence for supermassive black hole binaries
• Importance of including small body spin effects in the modelling of intermediate mass-ratio inspirals. II Accurate parameter extraction of strong sources using higher-order spin effects
• Spontaneous scalarization with an extremely massive field and heavy neutron stars
• Octupolar invariants for compact binaries on quasi-circular orbits
• High-order half-integral conservative post-Newtonian coefficients in the redshift factor of black hole binaries
• A parametrization to test black hole candidates with the spectrum of thin disks
• High Frequency Gravitational Waves from Supermassive Black Holes: Prospects for LIGO-Virgo Detections
• Quasi-local contribution to the scalar self-force: Non-geodesic Motion
• Dynamics of black holes in de Sitter spacetimes
• Constraining effective quantum gravity with LISA
• MOCCA-SURVEY Database I: Is NGC 6535 a Dark Star Cluster Harboring an IMBH?
• Gauge and Averaging in Gravitational Self-force
• Discovering the interior of black holes
• Mergers of accreting stellar-mass black holes
• Massive black hole and gas dynamics in mergers of galaxy nuclei - II. Black hole sinking in star-forming nuclear discs
• Evolution and spherical collapse in Einstein-aether theory and Horava gravity
• Cosmology with Standard Sirens: the Importance of the Shape of the Lensing Magnification Distribution
• Discovery of a variable X-ray counterpart to HESS J1832-093: A new gamma-ray binary?
• Persistent junk solutions in time-domain modeling of extreme mass ratio binaries
• Einstein-aether as a quantum effective field theory
• Origin of the long-term modulation of radio emission of LS I +61 303
• Isotropic-Nematic Phase Transitions in Gravitational Systems II: Higher Order Multipoles
• Gravitational Wave Hotspots: Ranking Potential Locations of Single-Source Gravitational Wave Emission
• Regularization of static self-forces
• Cosmic variance in the nanohertz gravitational wave background
• Detecting Lorentz Violations with Gravitational Waves from Black Hole Binaries
• Testing Chern-Simons gravity with black holes?
• Dimensional reduction in numerical relativity: Modified cartoon formalism and regularization
• Gravitational bremsstrahlung in ultra-planckian collisions
• Self-force gravitational waveforms for extreme and intermediate mass ratio inspirals. II: Importance of the second-order dissipative effect
• Gravity-dominated unequal-mass black hole collisions
• Up to eleven: radiation from particles with arbitrary energy falling into higher-dimensional black holes
• Nutational resonances, transitional precession, and precession-averaged evolution in binary black-hole systems
• Deriving analytic solutions for compact binary inspirals without recourse to adiabatic approximations
• Scattering of point particles by black holes: gravitational radiation
• Tuning Gravitationally Lensed Standard Sirens
• Pulsar Timing Perturbations from Galactic Gravitational Wave Bursts with Memory
• Higher-dimensional puncture initial data
• Self-force correction to geodetic spin precession in Kerr spacetime
• Deformation of extremal black holes from stringy interactions
• Binary Black Hole Accretion Flows From a Misaligned Circumbinary Disk
• Evolutions of Nearly Maximally Spinning Black Hole Binaries Using the Moving Puncture Approach
• A Precision Test for an Extra Spatial Dimension Using Black Hole--Pulsar Binaries
• Massive black hole and gas dynamics in galaxy nuclei mergers. I. Numerical implementation
• Non-Spherically Symmetric Collapse in Asymptotically AdS Spacetimes
• Effective stress-energy tensors, self-force, and broken symmetry
• Self-force from reconstructed metric perturbations: numerical implementation in Schwarzschild spacetime
• Static Kerr Green's Function in Closed Form and an Analytic Derivation of the Self-Force for a Static Scalar Charge in Kerr Space-Time
• Observational signatures from horizonless black shells imitating rotating black holes
• Ultralight scalars and resonances in black-hole physics
• Whirling orbits around twirling black holes from conformal symmetry
• Thermodynamics of a Black Hole with Moon
• Unbound motion on a Schwarzschild background: Practical approaches to frequency domain computations
• Classical ultrarelativistic bremsstrahlung in extra dimensions
• Cosmological Physics with Black Holes (and Possibly White Dwarfs)
• Evidence of coupling between the thermal and nonthermal emission in the gamma-ray binary LS I +61 303
• Gravitational self-force in scalar-tensor gravity
• Precessing supermassive black hole binaries and dark energy measurements with LISA
• Time-domain metric reconstruction for self-force applications
• Prospects of the local Hubble parameter measurement using gravitational waves from double neutron stars
• Effective-one-body Hamiltonian with next-to-leading order spin-spin coupling
• The characteristic treatment of black holes
• Higher dimensional Numerical Relativity: code comparison
• Classification and asymptotic structure of black holes in bimetric theory
• A Second Decoupling Between Merging Binary Black Holes and the Inner Disc--Impact on the Electromagnetic Counterpart
• Gravitational Waves from Accreting Neutron Stars undergoing Common-Envelope Inspiral
• Implicit-explicit (IMEX) evolution of single black holes
• Silhouette and spectral line profiles in the special modification of the Kerr black hole geometry generated by quintessential fields
• A Note on Celestial Mechanics in Kerr Spacetime
• Black-hole head-on collisions in higher dimensions
• Periodicity in the continua and broad line curves of a quasar E1821+643
• Constraints on the symmetry noninheriting scalar black hole hair
• Radiation-Reaction Force on a Small Charged Body to Second Order
• Accurate modeling of intermediate-mass-ratio inspirals: Exploring the form of the self-force in the intermediate-mass-ratio regime
• Scalar self-force for eccentric orbits around a Schwarzschild black hole
• Direct Measurement of the Positive Acceleration of the Universe and Testing Inhomogeneous Models under Gravitational Wave Cosmology
• Optical Monitoring of the Seyfert Galaxy NGC 4151 and Possible Periodicities in the Historical Light Curve
• Regularization of the second-order gravitational perturbations produced by a compact object
• Shining Light on Quantum Gravity with Pulsar-Black Hole Binaries
• Testing gravity of a regular and slowly rotating phantom black hole by quasi-periodic oscillations
• Numerical relativity in higher dimensions
• The secular evolution of discrete quasi-Keplerian systems. II. Application to a multi-mass axisymmetric disc around a supermassive black hole
• Scattering of scalar, electromagnetic and gravitational waves from binary systems
• Infrared outbursts as potential tracers of common envelope events in high-mass X-ray binary formation
• High-energy gamma-ray Emission from Microquasars: LS 5039 and LS I +61 303
• Neutrinos from microquasars
• Merger of multiple accreting black holes concordant with gravitational wave events
• Self force on an accelerated particle
• Particle Dark Matter Candidates
• Multipole moments of bumpy black holes

Cited by in corpus (506)

• Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A${}^{\ast }$
• Teleparallel Gravity: From Theory to Cosmology
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• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• Charged Black Holes in AdS Spaces in $4D$ Einstein Gauss-Bonnet Gravity
• Black holes with scalar hair in light of the Event Horizon Telescope
• The Quest for Dual and Binary Supermassive Black Holes: A Multi-Messenger View
• Stellar structure models in modified theories of gravity: lessons and challenges
• Black holes in galaxies: environmental impact on gravitational-wave generation and propagation
• Gravitational waves from neutron star mergers and their relation to the nuclear equation of state
• Spinning Black Hole Binary Dynamics, Scattering Amplitudes and Effective Field Theory
• Modified theories of Gravity: Why, How and What?
• Two populations of LIGO-Virgo black holes
• Detecting dark matter around black holes with gravitational waves: Effects of dark-matter dynamics on the gravitational waveform
• Gravitational waves from extreme-mass-ratio systems in astrophysical environments
• Primordial Black Holes Confront LIGO/Virgo data: Current situation
• Reconstructing phenomenological distributions of compact binaries via gravitational wave observations
• Nonlinear effects in black hole ringdown
• Destabilizing the Fundamental Mode of Black Holes: The Elephant and the Flea
• It has to be cool: on supergiant progenitors of binary black hole mergers from common-envelope evolution
• Detecting fundamental fields with LISA observations of gravitational waves from extreme mass-ratio inspirals
• The GW190521 Mass Gap Event and the Primordial Black Hole Scenario
• Constraining the primordial black hole scenario with Bayesian inference and machine learning: the GWTC-2 gravitational wave catalog
• The Evolution of Primordial Black Holes and their Final Observable Spins
• Gravitational Collider Physics
• Superradiance evolution of black hole shadows revisited
• Parametrized black hole quasinormal ringdown. II. Coupled equations and quadratic corrections for nonrotating black holes
• Ionization of Gravitational Atoms
• Constraints on the astrophysical environment of binaries with gravitational-wave observations
• Evolution of Einstein-scalar-Gauss-Bonnet gravity using a modified harmonic formulation
• ELGAR -- a European Laboratory for Gravitation and Atom-interferometric Research
• Black hole mergers from dwarf to massive galaxies with the NewHorizon and Horizon-AGN simulations
• Gravitational wave signatures of black hole quasi-normal mode instability
• Polarization of gravitational waves in symmetric teleparallel theories of gravity and their modifications
• Spontaneous scalarization
• Shadows of boson and Proca stars with thin accretion disks
• Two-timescale evolution of extreme-mass-ratio inspirals: waveform generation scheme for quasicircular orbits in Schwarzschild spacetime
• Bayesian Evidence for Both Astrophysical and Primordial Black Holes: Mapping the GWTC-2 Catalog to Third-Generation Detectors
• Measuring the dark matter environments of black hole binaries with gravitational waves
• Detecting scalar fields with Extreme Mass Ratio Inspirals
• Leading Nonlinear Tidal Effects and Scattering Amplitudes
• The response of ultralight dark matter to supermassive black holes and binaries
• The Gravitational-Wave Physics II: Progress
• Gravitational wave echoes from black hole area quantization
• Black hole superradiant instability from ultralight spin-2 fields
• How does a dark compact object ringdown?
• Axial perturbations of the scalarized Einstein-Gauss-Bonnet black holes
• Listening to the sound of dark sector interactions with gravitational wave standard sirens
• Exotic Compact Objects and the Fate of the Light-Ring Instability
• Gravitational wave probes of dark matter: challenges and opportunities
• Stability of the fundamental quasinormal mode in time-domain observations against small perturbations
• Lunar Gravitational-Wave Antenna
• Distinguishing fuzzballs from black holes through their multipolar structure
• Probing Primordial-Black-Hole Dark Matter with Scalar Induced Gravitational Waves
• The Science of the Einstein Telescope
• Constraints on Primordial Black Holes: the Importance of Accretion
• Baryogenesis from ultralight primordial black holes and strong gravitational waves from cosmic strings
• Gravitational ringing of rotating black holes in higher-derivative gravity
• Potential gravitational-wave signatures of quantum gravity
• Gravitational-Wave Asteroseismology with Fundamental Modes from Compact Binary Inspirals
• Dynamic Signatures of Black Hole Binaries with Superradiant Clouds
• Spectroscopy of binary black hole ringdown using overtones and angular modes
• Universal Properties of Light Rings for Stationary Axisymmetric Spacetimes
• Sharp Signals of Boson Clouds in Black Hole Binary Inspirals
• Gravitational Wave Anisotropies from Primordial Black Holes
• Gwbench: a novel Fisher information package for gravitational-wave benchmarking
• Primordial Black Holes
• Superradiant evolution of the shadow and photon ring of Sgr A${}^{\star }$
• Science with the TianQin observatory: Preliminary results on testing the no-hair theorem with ringdown signals
• Eccentricity evolution of compact binaries and applications to gravitational-wave physics
• Constraining cosmological phase transitions with the Parkes Pulsar Timing Array
• Gravitational-wave imprints of compact and galactic-scale environments in extreme-mass-ratio binaries
• Overtones or higher harmonics? Prospects for testing the no-hair theorem with gravitational wave detections
• Ringing of rotating black holes in higher-derivative gravity
• Distinguishing the nature of comparable-mass neutron star binary systems with multimessenger observations: GW170817 case study
• Gravitational waves induced by the local-type non-Gaussian curvature perturbations
• Parametrized ringdown spin expansion coefficients: a data-analysis framework for black-hole spectroscopy with multiple events
• Extreme mass ratio inspirals with spinning secondary: a detailed study of equatorial circular motion
• Extreme mass-ratio inspirals into black holes surrounded by scalar clouds
• Polar quasinormal modes of the scalarized Einstein-Gauss-Bonnet black holes
• Modeling and searching for a stochastic gravitational-wave background from ultralight vector bosons
• Adiabatic waveforms from extreme-mass-ratio inspirals: an analytical approach
• Accelerating black holes: quasinormal modes and late-time tails
• The peculiar acceleration of stellar-origin black hole binaries: measurement and biases with LISA
• Quasibound states of Schwarzschild acoustic black holes
• High Eccentricities and High Masses Characterize Gravitational-wave Captures in Galactic Nuclei as Seen by Earth-based Detectors
• Black Holes in $f(T,B)$ Gravity: Exact and Perturbed Solutions
• Axion boson stars
• Extreme mass-ratio inspirals in ultra-light dark matter
• Probing the Lorentz Symmetry Violation Using the First Image of Sagittarius A*: Constraints on Standard-Model Extension Coefficients
• Frequency domain model of $f$-mode dynamic tides in gravitational waveforms from compact binary inspirals
• Gravitational waves from Population III binary black holes formed by dynamical capture
• Gravitational wave cosmology with extreme mass-ratio inspirals
• Pseudospectrum of horizonless compact objects: a bootstrap instability mechanism
• Light, medium-weight or heavy? The nature of the first supermassive black hole seeds
• Analytical computation of quasi-normal modes of slowly-rotating black-holes in dCS gravity
• Superradiant instability of charged scalar fields in higher-dimensional Reissner-Nordström-de Sitter black holes
• Detecting massive scalar fields with Extreme Mass-Ratio Inspirals
• Black holes in Starobinsky-Bel-Robinson Gravity and the breakdown of quasinormal modes/null geodesics correspondence
• A morphology-independent search for gravitational wave echoes in data from the first and second observing runs of Advanced LIGO and Advanced Virgo
• Einstein, Planck and Vera Rubin: relevant encounters between the Cosmological and the Quantum Worlds
• Large and Ultra-compact Gauss-Bonnet Black Holes with a Self-interacting Scalar Field
• Black hole scalarization with Gauss-Bonnet and Ricci scalar couplings
• Observational properties of relativistic fluid spheres with thin accretion disks
• Listening to the Universe with Next Generation Ground-Based Gravitational-Wave Detectors
• High Precision Ringdown Modeling: Multimode Fits and BMS Frames
• Thermodynamics conditions of matter in the neutrino decoupling region during neutron star mergers
• Observational signatures of hot spots orbiting horizonless objects
• Spin dependence of black hole ringdown nonlinearities
• Hyperboloidal framework for the Kerr spacetime
• Constraining Teleparallel Gravity through Gaussian Processes
• Merging Rates of Compact Binaries in Galaxies: Perspectives for Gravitational Wave Detections
• On the Existence of Solutions with a Horizon in Pure Scalar-Gauss-Bonnet Theories
• Gravitational waves and higher dimensions: Love numbers and Kaluza-Klein excitations
• Spectral (in)stability of quasinormal modes and strong cosmic censorship
• Extragalactic fast X-ray transient candidates discovered by Chandra (2000-2014)
• Well-posedness of the four-derivative scalar-tensor theory of gravity in singularity avoiding coordinates
• Stirred and shaken: dynamical behavior of boson stars and dark matter cores
• Can a black hole-neutron star merger explain GW170817, AT2017gfo, GRB170817A?
• The multipolar structure of fuzzballs
• Towards numerical relativity in scalar Gauss-Bonnet gravity: 3+1 decomposition beyond the small-coupling limit
• Probing the Nature of Black Holes: Deep in the mHz Gravitational-Wave Sky
• Updated Parameter Estimates for GW190425 Using Astrophysical Arguments and Implications for the Electromagnetic Counterpart
• Ergoregion instability and echoes for braneworld black holes: Scalar, electromagnetic and gravitational perturbations
• Eccentricity evolution of massive black hole binaries from formation to coalescence
• Black hole merger simulations in wave dark matter environments
• The current-type quadrupole moment and gravitational-wave mode $(\ell ,m)=(2,1)$ of compact binary systems at the third post-Newtonian order
• Shadows of charged rotating black holes: Kerr-Newman versus Kerr-Sen
• Minimum main sequence mass in quadratic Palatini $f(\mathcal{R})$ gravity
• Measuring dark matter spikes around primordial black holes with Einstein Telescope and Cosmic Explorer
• One-loop correction to the enhanced curvature perturbation with local-type non-Gaussianity for the formation of primordial black holes
• Priorities in gravitational waveforms for future space-borne detectors: vacuum accuracy or environment?
• Gravitational Bremsstrahlung with tidal effects in the post-Minkowskian expansion
• Reconstructing teleparallel gravity with cosmic structure growth and expansion rate data
• Quasinormal modes-shadow correspondence for rotating regular black holes
• Probing the equation of state of neutron star matter with gravitational waves from binary inspirals in light of GW170817: a brief review
• Tidal response from scattering and the role of analytic continuation
• Gravitational waves from axion-like particle cosmic string-wall networks
• Slowly-rotating curved acoustic black holes: Quasinormal modes, Hawking-Unruh radiation and quasibound states
• Dipolar tidal effects in scalar-tensor theories
• Gravitational Imprints of Flavor Hierarchies
• The effect of wave dark matter on equal mass black hole mergers
• Global torques and stochasticity as the drivers of massive black hole pairing in the young Universe
• Rotating black holes without ${\mathbb{Z}}_2$ symmetry and their shadow images
• Ricci-Based Gravity theories and their impact on Maxwell and nonlinear electromagnetic models
• Double shadows of reflection-asymmetric wormholes supported by positive energy thin-shells
• The tune of the universe: the role of plasma in tests of strong-field gravity
• Catastrogenesis: DM, GWs, and PBHs from ALP string-wall networks
• Probing ultralight dark matter with future ground-based gravitational-wave detectors
• Second-order gravitational self-force in a highly regular gauge
• Gravitational tuning forks and hierarchical triple systems
• Gravitational-Wave Detector Networks: Standard Sirens on Cosmology and Modified Gravity Theory
• Tidal effects and disruption in superradiant clouds: a numerical investigation
• Primordial regular black holes as all the dark matter. II. Non-time-radial-symmetric and loop quantum gravity-inspired metrics
• Improved gravitational radiation time-scales: significance for LISA and LIGO-Virgo sources
• Analog Schwarzschild black holes of Bose-Einstein condensates in a cavity: Quasinormal modes and quasibound states
• Can gravitational-wave memory help constrain binary black-hole parameters? A LISA case study
• Chaos at the rim of black hole and fuzzball shadows
• Gravitational-wave detectors as particle-physics laboratories: Constraining scalar interactions with a coherent inspiral model of boson-star binaries
• Primordial regular black holes as all the dark matter. I. Time-radial-symmetric metrics
• Non-linear Black Hole Ringdowns: an Analytical Approach
• Malaise and remedy of binary boson-star initial data
• Asymptotically locally flat and AdS higher-dimensional black holes of Einstein-Horndeski-Maxwell gravity in the light of EHT observations: shadow behavior and deflection angle
• Love numbers and magnetic susceptibility of charged black holes
• Observational signature of a near-extremal Kerr-Sen black hole in the heterotic string theory
• The Lunar Gravitational-wave Antenna: Mission Studies and Science Case
• The light ring and the appearance of matter accreted by black holes
• The competing effect of gas and stars in massive black hole binaries evolution
• Self-interacting scalar dark matter around binary black holes
• Cosmological perturbations in modified teleparallel gravity models: Boundary term extension
• On Black Hole Temperature in Horndeski Gravity
• Prospects for determining the nature of the secondaries of extreme mass-ratio inspirals using the spin-induced quadrupole deformation
• Holographic approach to compact stars and their binary mergers
• Constraints on the ultralight scalar boson from Advanced LIGO and Advanced Virgo's first three observing runs using the stochastic gravitational-wave background
• Darboux Covariance: A Hidden Symmetry of Perturbed Schwarzschild Black Holes
• Shadows, rings and optical appearance of a magnetically charged regular black hole illuminated by various accretion disks
• Gravitational-wave tails of memory
• Towards VLBI Observations of Black Hole Structure
• Ultra long lived quasinormal modes of neutron stars in massive scalar-tensor gravity
• Constructing spherically symmetric Einstein-Dirac systems with multiple spinors: Ansatz, wormholes and other analytical solutions
• Angular Momentum Loss Due to Tidal Effects in the Post-Minkowskian Expansion
• Constraints on $f(T)$ Cosmology with Pantheon+
• Gravitational waves from binary black hole mergers surrounded by scalar field clouds: Numerical simulations and observational implications
• Defining the (Black Hole)-Spheroid Connection with the Discovery of Morphology-Dependent Substructure in the $M_{\mathrm{BH}}$--${\mathrm{n}}_{\mathrm{sph}}$ and $M_{\mathrm{BH}}$--${\mathrm{R}}_{\mathrm{e},\mathrm{sph}}$ Diagrams: New Tests for Advanced Theories and Realistic Simulations
• Exploring strong-field deviations from general relativity via gravitational waves
• Early evolutionary tracks of low-mass stellar objects in modified gravity
• Gravity from entropy
• Analytic post-Newtonian expansion of the energy and angular momentum radiated to infinity by eccentric-orbit non-spinning extreme-mass-ratio inspirals to 19PN
• Breaking away from the near horizon of extreme Kerr
• Probing wave-optics effects and low-mass dark matter halos with lensing of gravitational waves from massive black holes
• Relativistic star perturbations in Horndeski theories with a gauge-ready formulation
• Instability of spherically-symmetric black holes in Quadratic Gravity
• Numerical Black Hole Solutions in Modified Gravity Theories: Axial Symmetry Case
• Analytic solutions for the motion of spinning particles near spherically symmetric black holes and exotic compact objects
• Constraining modifications of black hole perturbation potentials near the light ring with quasinormal modes
• Model independent tests of the Kerr bound with extreme mass ratio inspirals
• Improved gravitational radiation time-scales II: spin-orbit contributions and environmental perturbations
• Kerr black holes with synchronised axionic hair
• Generalized disformal coupling leads to spontaneous tensorization
• Quasinormal modes of self-dual black holes in loop quantum gravity
• Gravitational wave from extreme mass-ratio inspirals as a probe of extra dimensions
• Plasma-photon interaction in curved spacetime I: formalism and quasibound states around nonspinning black holes
• Source properties of the lowest signal-to-noise-ratio binary black hole detections
• Null geodesics, causal structure, and matter accretion in Lorentzian-Euclidean black holes
• Signatures of primordial black holes in gravitational wave clustering
• Exploring waveforms with non-GR deviations for extreme mass-ratio inspirals
• Linear stability of black holes in shift-symmetric Horndeski theories with a time-independent scalar field
• Quasinormal modes of Kerr black holes using a spectral decomposition of the metric perturbations
• Testing Lorentz Invariance of Gravity in the Standard Model Extension with GWTC-3
• Quasinormal modes of the bumblebee black holes with a global monopole
• Hunting the stochastic gravitational wave background in pulsar timing array cross correlations through theoretical uncertainty
• Prospects of detecting deviations to Kerr geometry with radiation reaction effects in EMRIs
• Exact Black Hole Solutions in Modified Gravity Theories: Spherical Symmetry Case
• Eikonal quasinormal modes and photon orbits of deformed Schwarzschild black holes
• Shadows and thin accretion disk images of the $\gamma$-metric
• Extreme mass ratio inspirals in galaxies with dark matter halos
• Linear stability of black holes with static scalar hair in full Horndeski theories: generic instabilities and surviving models
• Black Hole Ringdown as a Probe for Dark Energy
• Spin-orbit effects for compact binaries in scalar-tensor gravity
• Gravitational waveforms from the quasicircular inspiral of compact binaries in massive Brans-Dicke theory
• The multipolar structure of rotating boson stars
• New black hole solutions with a dynamical traceless nonmetricity tensor in Metric-Affine Gravity
• Astrophysical Gravitational-Wave Echoes from Galactic Nuclei
• Turning black-holes and D-branes inside out their photon-spheres
• Bekenstein-Hod Universal Bound on Information Emission Rate Is Obeyed by LIGO-Virgo Binary Black Hole Remnants
• Determination of new coefficients in the angular momentum and energy fluxes at infinity to 9PN for eccentric Schwarzschild extreme-mass-ratio inspirals using mode-by-mode fitting
• Growth of Supermassive Black Hole Seeds in ETG Star-Forming Progenitors: Multiple Merging of Stellar Compact Remnants via Gaseous Dynamical Friction and Gravitational Wave Emission
• Instability of vectorized stars
• Motion of spinning particles around black hole in a dark matter halo
• Inspiral gravitational waveforms from compact binary systems in Horndeski gravity
• Multi-scalar Gauss-Bonnet gravity -- hairy black holes and scalarization
• Inspiralling compact objects with generic deformations
• Bayesian parameter estimation on boson-star binary signals with a coherent inspiral template and spin-dependent quadrupolar corrections
• Convergence of Fourier-domain templates for inspiraling eccentric compact binaries
• Metric-affine gravity effects on terrestrial (exo-)planets profiles
• Searching for General Binary Inspirals with Gravitational Waves
• Structure of neutron stars in massive scalar-tensor gravity
• Parametrized Black Hole Quasinormal Ringdown Formalism for Higher Overtones
• Merger rate of charged black holes from the two-body dynamical capture
• Detection of scalar fields by Extreme Mass Ratio Inspirals with a Kerr black hole
• Nonlinear Evolution of Quadratic Gravity in 3+1 Dimensions
• Shielding a charged black hole
• Population inference of spin-induced quadrupole moments as a probe for non-black hole compact binaries
• Gravitational waves from the remnants of the first stars in nuclear star clusters
• Applications of machine learning in gravitational wave research with current interferometric detectors
• The role of bars on the dynamical-friction driven inspiral of massive perturbers
• Eccentric-orbit extreme-mass-ratio-inspiral radiation II: 1PN correction to leading-logarithm and subleading-logarithm flux sequences and the entire perturbative 4PN flux
• Stability of relativistic stars with scalar hairs
• On Kerr black hole deformations admitting a Carter constant and an invariant criterion for the separability of the wave equation
• Efficient parameter inference for gravitational wave signals in the presence of transient noises using temporal and time-spectral fusion normalizing flow
• Measuring eccentricity and gas-induced perturbation from gravitational waves of LISA massive black hole binaries
• Implications of cosmologically coupled black holes for pulsar timing arrays
• Vanishing of Quadratic Love Numbers of Schwarzschild Black Holes
• Evolution of diffuse scalar clouds around binary black holes
• Dynamical behavior of the $C$-metric: charged scalar fields, quasinormal modes and superradiance
• Gravitational waves in warped compactifications
• Quasinormal modes of black holes in Weyl gravity: Electromagnetic and gravitational perturbations
• Black hole spin evolution in warped accretion discs
• Self-consistent description of a spherically-symmetric gravitational collapse
• Probing the Black Hole Merger History in Clusters using Stellar Tidal Disruptions
• Jupiter and jovian (exo)-planets in Palatini $f(\bar{R})$ gravity
• Space-based Gravitational Wave Observatories Will Be Able to Use Eccentricity to Unveil Stellar-mass Binary Black Hole Formation
• Binary white dwarfs and decihertz gravitational wave observations: From the Hubble constant to supernova astrophysics
• Quasi-Normal Modes of Loop Quantum Black Holes Formed from Gravitational Collapse
• Topological neutron stars in tensor-multi-scalar theories of gravity
• Odd-parity stability of black holes in Einstein-Aether gravity
• The shape of Scalar Gauss-Bonnet Gravity
• Observational properties of hot-spots orbiting relativistic fluid spheres
• Fully Relativistic Treatment of Extreme Mass-Ratio Inspirals in Collisionless Environments
• Anomalies in the gravitational recoil of eccentric black-hole mergers with unequal mass ratios
• Dynamical evidence of the sub-parsec counter-rotating disc for a close binary of supermassive black holes in the nucleus of NGC 1068
• The minimum measurable eccentricity from gravitational waves of LISA massive black hole binaries
• Precision cosmology with primordial GW backgrounds in presence of astrophysical foregrounds
• Constraining scalar-tensor theories using neutron star mass and radius measurements
• Stealth black holes in shift symmetric kinetic gravity braiding
• Superradiant Leptogenesis
• Applying the effective-source approach to frequency-domain self-force calculations for eccentric orbits
• Electromagnetic emission from axionic boson star collisions
• Universal properties of the near-horizon geometry
• Pandora's box lid: geometry near the apparent horizon
• Eccentric-orbit EMRI radiation: Analytic forms of leading-logarithm and subleading-logarithm flux terms at high PN orders
• Gravitational atoms in the braneworld scenario
• Compact Binary Coalescences in Dense Gaseous Environments Can Pose as ones in Vacuum
• The Galactic Underworld: The spatial distribution of compact remnants
• Polar Quasinormal Modes of Neutron Stars in Massive Scalar-Tensor Theories
• The Axial Gravitational Ringing of a Spherically Symmetric Black Hole Surrounded by Dark Matter Spike
• Evolution of Anti-de Sitter black holes in Einstein-Maxwell-dilaton theory
• Black-hole spectroscopy: quasinormal modes, ringdown stability and the pseudospectrum
• Growth of structures using redshift space distortion in $f(T)$ Cosmology
• Merger estimates for Kerr-Sen black holes
• Kerr-Vaidya black holes
• Towards rotating non-circular black holes in string-inspired gravity
• Perturbing the vortex: quasinormal and quasibound spectra of rotating acoustic geometries
• Swift sky localization of gravitational waves using deep learning seeded importance sampling
• Black Hole Greybody Factors from Korteweg-de Vries Integrals: Theory
• Black Holes in $4D$ AdS Einstein Gauss Bonnet Gravity With Power- Yang Mills Field
• Multicenter solutions in Eddington-inspired Born-Infeld gravity
• Probing fundamental physics with Extreme Mass Ratio Inspirals: a full Bayesian inference for scalar charge
• Testing gravity with Extreme-Mass-Ratio Inspirals
• Nomen non est omen: Why it is too soon to identify ultra-compact objects as black holes
• Footprints of population III stars in the gravitational-wave background
• The high-energy collision of black holes in higher dimensions
• Shadow behavior of an EMSG charged black hole
• Black holes as spherically-symmetric horizon-bound objects
• Dressed black holes in the new tensor-vector-scalar theory
• Tidal heating and torquing of the primary black hole in eccentric-orbit, non-spinning extreme-mass-ratio inspirals to 22PN order
• Instability of scalarized compact objects in Einstein-scalar-Gauss-Bonnet theories
• Scalar Hairy Black Holes with Inverted Mexican Hat Potential
• Boson star head-on collisions with constraint-violating and constraint-satisfying initial data
• Spin and Quadrupole Couplings for High Spin Equatorial Intermediate Mass-ratio Coalescences
• Generation of gravitational waves and tidal disruptions in clumpy galaxies
• Semiclassical black holes and horizon singularities
• Instability of compact stars with a nonminimal scalar-derivative coupling
• Influence of dark matter equation of state on the axial gravitational ringing of supermassive black holes
• Infinitely degenerate exact Ricci-flat solutions in f(R) gravity
• Constraining modified gravity theories with scalar fields using black-hole images
• Dark matter from primordial black holes would hold charge
• Quantum kinetic theory of Jeans instability in non-minimal matter-curvature coupling gravity
• Probing resonant excitations in exotic compact objects via gravitational waves
• GRFolres: A code for modified gravity simulations in strong gravity
• Microlensing effects of wormholes associated to blackhole spacetimes
• Space-borne atom interferometric gravitational wave detections. Part I. The forecast of bright sirens on cosmology
• String Memories ... Lost and Regained
• Giant planet formation in Palatini gravity
• Dynamical spontaneous scalarization in Einstein-Maxwell-scalar models in anti-de Sitter spacetime
• Black hole minimum size and scalar charge in shift-symmetric theories
• Can the abyss swallow gravitational waves or why we do not observe echoes?
• Instability of hairy black holes in regularized 4-dimensional Einstein-Gauss-Bonnet gravity
• Gravitational interaction through a feedback mechanism
• Slowly-rotating compact objects: the nonintegrability of Hartle-Thorne particle geodesics
• Holographic renormalization of Horndeski gravity
• Quantum gravity phenomenology at the dawn of the multi-messenger era -- A review
• Primordial regular black holes as all the dark matter. III. Covariant canonical quantum gravity models
• Charged Dirac perturbations on Reissner-Nordström-Anti-de Sitter spacetimes: quasinormal modes with Robin boundary conditions
• Quantum gravitational signatures in next-generation gravitational wave detectors
• Curved accretion disks around rotating black holes without reflection symmetry
• General formulae for the periapsis shift of a quasi-circular orbit in static spherically symmetric spacetimes and the active gravitational mass density
• Subdominant Modes of Scalar Superradiant Instability and Gravitational Wave Beats
• Physical black holes in fourth-order gravity
• Perturbative and non-linear analyses of gravitational turbulence in spacetimes with stable light rings
• Neutrino trapping in extremely compact Tolman VII spacetimes
• On the universality of late-time ringdown tail
• Strong-gravity precession resonances for binary systems orbiting a Schwarzschild black hole
• Dark Energy Gravitational Wave Observations and Ice Age Periodicity
• Black holes immersed in polytropic scalar field gas
• Probing new fundamental fields with Extreme Mass Ratio Inspirals
• Black Holes and Wormholes Beyond Classical General Relativity
• Second-order gravitational self-force in a highly regular gauge: Covariant and coordinate punctures
• Seeing dark matter via acceleration radiation
• Black Holes as Fermion Factories
• Piercing of a solitonic boson star by a black hole
• Space-borne atom interferometric gravitational wave detections. Part II. Dark sirens and finding the one
• Probing Bosonic Stars with Atomic Clocks
• Models of cosmological black holes
• Black holes, multiple propagation speeds, and energy extraction
• Quasinormal modes of hairy black holes in shift-symmetric theories
• Detecting the massive vector field with extreme mass-ratio inspirals
• Covariant formulation of refracted gravity
• Spontaneous scalarization of charged stars
• Prospects of Probing Dark Matter Condensates with Gravitational Waves
• Fundamental Physics and Cosmology with TianQin
• Bayesian real-time classification of multi-messenger electromagnetic and gravitational-wave observations
• Highly compact Proca stars with quartic self-interactions
• General Relativistic Simulations of High-Mass Binary Neutron Star Mergers: rapid formation of low-mass stellar black holes
• Detectability of Gravitational Wave from a population of Inspiralling Black Holes in Milky Way Mass Galaxies
• Applications of the close-limit approximation: horizonless compact objects and scalar fields
• Pair production of scalars around near-extremal Kerr-Sen black holes
• Conformal and kinetic couplings as two Jordan frames of the same theory
• Gravitating Scalarons with Inverted Higgs Potential
• Massive scalar field perturbations of 4D de Sitter Einstein-Gauss-Bonnet black holes
• Euclidean methods and phase transitions for the strongest deformations compatible with Schwarzschild asymptotics
• Nature of phase transitions and metastability in scalar-tensor theories
• No black hole bomb for D-dimensional extremal Reissner-Nordstrom black holes under charged massive scalar perturbation
• Spherically symmetric black holes in metric gravity
• Hair is complicated: Gravitational waves from stable and unstable boson-star mergers
• Integrability in Perturbed Black Holes: Background Hidden Structures
• Kicks in charged black hole binaries
• Evaporating black holes: constraints on anomalous emission mechanisms
• Parameter Distributions of Binary Black Hole Mergers Near Supermassive Black Holes as Seen by Advanced Gravitational Wave Detectors
• Black holes in the quadratic-order extended vector-tensor theories
• Gravitational waveforms from the inspiral of compact binaries in the Brans-Dicke theory in an expanding Universe
• Exploring higher order images with Fe K_α-lines from relativistic disks: black hole spin determination and bias
• Imprint of f(R) gravity in the cosmic magnification
• Gravitational multipole moments for asymptotically de Sitter spacetimes
• Bayesian Search of Massive Scalar Fields from LIGO-Virgo-KAGRA Binaries
• Black holes and nilmanifolds: quasinormal modes as the fingerprints of extra dimensions?
• Dark Fluxes from Accreting Black Holes and Direct Detections
• Spherical black holes with minimally coupled scalar cloud/hair in Einstein-Born-Infeld gravity
• Thermal Emission of Gravitational Waves from Weak to Strong Coupling
• A covariant formulation of relativistic mechanics
• Inaccessibility of traversable wormholes
• Completely Deformed Complexity-free Anisotropic Fluid Sphere
• CLAP for modified gravity: scalar instabilities in binary black hole spacetimes
• Kerr-Schild Form of the Exact Metric for a Constantly Moving Kerr Black Hole and Null Gravitational Deflection
• Physical black holes in semiclassical gravity
• Instabilities of scalar fields around oscillating stars
• Axial perturbations of hairy Gauss-Bonnet black holes with massive self-interacting scalar field
• Non-linear stability of soliton solutions for massive tensor-multi-scalar-theories
• Ultracompact vector stars
• Electromagnetic memory in arbitrary curved space-times
• Coupled vector Gauss-Bonnet theories and hairy black holes
• Subtleties in constraining gravity theories with mass-radius data
• Will Gravitational Waves Discover the First Extra-Galactic Planetary System?
• Linear stability of vector Horndeski black holes
• Observational features of reflection asymmetric black holes
• Cumulative effect of orbital resonances in extreme-mass-ratio inspirals
• Post-adiabatic waveforms from extreme mass ratio inspirals in the presence of dark matter
• Teleparallel dark energy in a nonflat universe
• Fractal signatures of non-Kerr spacetimes in the shadow of light-ring bifurcations
• Stability of Schwarzshild black holes in quadratic gravity with Weyl curvature domination
• Gravitational Wave Propagation and Polarizations in the Teleparallel analog of Horndeski Gravity
• Trapping of null geodesics in slowly rotating spacetimes
• Slowly rotating topological neutron stars -- universal relations and epicyclic frequencies
• Hidden conformal symmetries for black holes in modified gravity
• An Effective Field Theory for Binary Cosmic Strings
• MOCCA-Survey Database: Extra Galactic Globular Clusters. III. The population of black holes in Milky Way and Andromeda-like galaxies
• Scalar fields around black hole binaries in LIGO-Virgo-KAGRA
• Cosmology in theories with spontaneous scalarization of neutron stars
• Primordial Gravitational Waves in Generalized Palatini Gravity
• Padé metrics for black hole perturbations and light rings
• Spectral instability of horizonless compact objects within astrophysical environments
• Note on black holes with kilometer-scale ultraviolet regulators
• Unveiling the electrodynamic nature of spacetime collisions
• Tidal Love Numbers of Neutron Stars in Horndeski Theories
• Slowly rotating ultracompact Schwarzschild star in the gravastar limit
• Compact scalar field solutions in EiBI gravity
• Horizon-bound objects: Kerr--Vaidya solutions
• GW170814: Gravitational wave polarization analysis
• Smarr formula for black holes with primary and secondary scalar hair
• Quasi-normal modes of slowly-rotating Johannsen black holes
• Distinguishing dark matter halos with Extreme mass ratio inspirals
• Probing the Dark Solar System: Detecting Binary Asteroids with a Space-Based Interferometric Asteroid Explorer
• Properties of white dwarf in the binary system AR Scorpii and its observed features
• The multiple nature of CC Com: one of the ultra-short orbital period late-type contact binary systems
• Symmetry restoration in the vicinity of neutron stars with a nonminimal coupling
• On Equation of State of Dark Matter around Massive Black Holes
• Splitting the Gravitational Atom: Instabilities of Black Holes with Synchronized or Resonant Hair
• Birkhoff's Theorem and Uniqueness: A Peek Beyond General Relativity
• DNA Mutations via Chern-Simons Currents
• Space-based Gravitational Wave Observatories
• Limits on the existence of totally reflective exotic compact objects with current and future gravitational-wave detectors
• Pseudospectrum of Reissner-Nordström black holes: quasinormal mode instability and universality
• Signatures of asymmetry: Gravitational wave memory and the parity violation
• Towards the merger of Hawking radiating black holes
• Gravitational wave propagation in generalized hybrid metric-Palatini gravity
• Black holes as telescopes: Discovering supermassive binaries through quasi-periodic lensed starlight
• Inflation from entropy
• Taxonomy of periodic orbits and gravitational waves in a non-rotating Destounis-Suvorov-Kokkotas black hole spacetime
• Curvature and dynamical spacetimes: can we peer into the quantum regime?
• Even-parity stability of hairy black holes in $U(1)$ gauge-invariant scalar-vector-tensor theories
• Quantum-Corrected Thermodynamics of Conformal Weyl Gravity Black Holes: GUP Effects and Phase Transitions
• Master Functions and Equations for Perturbations of Vacuum Spherically-Symmetric Spacetimes
• About the ability of agnostic X-ray tests of the Kerr Hypothesis to discover new physics
• The Radial Action from Probe Amplitudes to All Orders
• Gravitational waveforms from periodic orbits around a novel regular black hole
• Archival Inference for Eccentric Stellar-Mass Binary Black Holes in Space-Based Gravitational Wave Observations
• Influence Through Mixing: Hotspots as Benchmarks for Basic Black-Hole Behaviour
• Mass and spin coevolution of black holes inspiralling through dark matter
• Ringdown of a black hole sourced by a Burkert-density effective anisotropic source
• Accreting Schwarzschild-like compact object: Plasma-photon interaction and stability
• Preliminary forecasting constraint on scalar charge with LISA in non-vacuum environments
• Quantum Hairy Black Hole Formation and Horizon Quantum Mechanics
• Estimating High-Order Time Derivatives of Kerr Orbital Functionals
• Roche limit and stellar disruption in the Simpson--Visser spacetime
• Revised event rates for extreme and extremely large mass-ratio inspirals
• Real-Time Holography and Hybrid WKB for BTZ Wormholes
• First-post-Newtonian generation of gravitational waves in Einstein-Cartan theory
• Spherically symmetric black holes in Gravity from Entropy and spontaneous emission
• Periodic orbits and gravitational waveforms of black holes in bumblebee gravity
• Probing Dark Matter Clumps, Strings and Domain Walls with Gravitational Wave Detectors
• Hair imprints of the gravitational decoupling and hairy black hole spectroscopy
• The landscape of massive black-hole spectroscopy with LISA and Einstein Telescope
• Neutron stars more compact than black holes in quasi-topological gravity: Equilibrium configurations and radial stability
• The imprint of gas on gravitational waves from LISA intermediate-mass black hole binaries
• Neutron stars more compact than black holes as a probe of strong-field gravity
• Spatial Dependence of the Growth Factor in Scalar-Tensor Cosmology
• Semi-classical imprints on quasinormal mode spectra
• Underlying mechanisms of phase transitions in scalar-tensor theories
• Probing modified gravitational wave propagation with strongly lensed coalescing binaries
• Rings of light caused by gravitational waves
• Piercing of a boson star by a black hole
• Extreme mass-ratio inspirals as probes of scalar fields: eccentric equatorial orbits around Kerr black holes
• Black holes and their horizons in semiclassical and modified theories of gravity
• Linear perturbations of Kerr black hole in quadratic gravity
• Probing higher curvature gravity via ringdown with overtones
• $\Lambda$-Gravity from Entropy
• Parameterized Post-Newtonian Analysis of Quadratic Gravity and Solar System Constraints
• Tidal perturbations of an extreme mass ratio inspiral around a Kerr black hole
• Light rings, gravitational lensing, and ISCOs of exotic compact objects in Einstein-scalar-Maxwell theories
• Isotropic Coordinates for Generalized Schwarzschild-like Solutions
• Electrically charged black hole solutions in semiclassical gravity and dynamics of linear perturbations
• Constraint-satisfying binary boson star initial data via XCFC
• Constraining Kerr supermassive black hole properties using gravitational waves from inspiraling stellar-mass binary black holes
• Non-minimal Effective Scalar-Tensor Gravity in the Early Universe
• Exact pp-wave solutions in shift-symmetric higher-order scalar-tensor theories
• Spectral Problems for Quasinormal Modes of Black Holes
• Constraining modified gravity theories with physical black holes
• A restless supermassive black hole in the galaxy J0437+2456
• New effective theories of gravitation and their phenomenological consequences
• The ghost of vector fields in compact stars
• Resonances, black hole mimickers and the greenhouse effect: consequences for gravitational-wave physics
• Bardeen-Kiselev black hole with cosmological constant
• Dirty waveforms: multiband harmonic content of gas-embedded gravitational wave sources
• Effective-one-body formalism for leading-order radiative effects in the post-linear framework
• Primordial black holes from D-parity breaking in SO(10) grand unified theory