New Horizons for Fundamental Physics with LISA

Abstract

The Laser Interferometer Space Antenna (LISA) has the potential to reveal wonders about the fundamental theory of nature at play in the extreme gravity regime, where the gravitational interaction is both strong and dynamical. In this white paper, the Fundamental Physics Working Group of the LISA Consortium summarizes the current topics in fundamental physics where LISA observations of GWs can be expected to provide key input. We provide the briefest of reviews to then delineate avenues for future research directions and to discuss connections between this working group, other working groups and the consortium work package teams. These connections must be developed for LISA to live up to its science potential in these areas.

arXiv commentAccepted in: Living Reviews in Relativity

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• Black Hole Based Tests of General Relativity
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• Spin-induced black hole scalarization in Einstein-scalar-Gauss-Bonnet theory
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• Gravitational signature of Schwarzschild black holes in dynamical Chern-Simons gravity
• Modified gravitational-wave propagation and standard sirens
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• Bayesian model selection for testing the no-hair theorem with black hole ringdowns
• General-Relativistic Simulations of Three-Dimensional Core-Collapse Supernovae
• Towards a formalism for mapping the spacetimes of massive compact objects: Bumpy black holes and their orbits
• Solar-Mass Primordial Black Holes Explain NANOGrav Hint of Gravitational Waves
• Speed of Gravitational Waves and the Fate of Scalar-Tensor Gravity
• Phenomenological aspects of black holes beyond general relativity
• The imprint of massive black hole formation models on the LISA data stream
• Satellites in Discs: Regulating the Accretion Luminosity
• Ergoregion instability of ultra-compact astrophysical objects
• Including higher order multipoles in gravitational-wave models for precessing binary black holes
• Gravitational radiation from an axion cloud around a black hole: Superradiant phase
• A new effective-one-body description of coalescing nonprecessing spinning black-hole binaries
• Black holes and binary mergers in scalar Gauss-Bonnet gravity: scalar field dynamics
• Post-Newtonian corrections to the gravitational-wave memory for quasicircular, inspiralling compact binaries
• Time-Dependent Models for Dark Matter at the Galactic Center
• Primordial Black Holes Confront LIGO/Virgo data: Current situation
• Imprints of Primordial Non-Gaussianity on Gravitational Wave Spectrum
• Binary Black Hole Mergers from Planet-like Migrations
• TASI Lectures on the Cosmological Constant
• Distinguishing Boson Stars from Black Holes and Neutron Stars from Tidal Interactions in Inspiraling Binary Systems
• Updated Constraints on Asteroid-Mass Primordial Black Holes as Dark Matter
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• Primordial Black Holes from Inflation and Quantum Diffusion
• Massive Primordial Black Holes as Dark Matter and their detection with Gravitational Waves
• Generalized framework for testing gravity with gravitational-wave propagation. II. Constraints on Horndeski theory
• Observable Properties of Orbits in Exact Bumpy Spacetimes
• Energetics of two-body Hamiltonians in post-Minkowskian gravity
• Non-linear metric perturbations and production of primordial black holes
• Gravitational Waves Induced by Scalar Perturbations with a Lognormal Peak
• Testing post-Newtonian theory with gravitational wave observations
• Induced gravitational waves in a general cosmological background
• Parametrized black hole quasinormal ringdown. I. Decoupled equations for nonrotating black holes
• Probing the non-linear structure of general relativity with black hole binaries
• Black hole information, unitarity, and nonlocality
• Models of Galaxies with Central Black Holes: Adiabatic Growth in Spherical Galaxies
• Astrophysical signatures of boson stars: quasinormal modes and inspiral resonances
• Nonlocal gravity. Conceptual aspects and cosmological predictions
• Bosenova collapse of axion cloud around a rotating black hole
• Planck 2018 results. IX. Constraints on primordial non-Gaussianity
• Testing the binary black hole nature of a compact binary coalescence
• Induced gravitational waves as a probe of thermal history of the universe
• Not quite a black hole
• Black Holes and Scalar Fields
• Primordial black hole evolution in tensor-scalar cosmology
• Gravitational Waves from Quasicircular Extreme Mass-Ratio Inspirals as Probes of Scalar-Tensor Theories
• Anisotropic stars as ultracompact objects in General Relativity
• Post-Newtonian Evolution of Massive Black Hole Triplets in Galactic Nuclei: IV. Implications for LISA
• Limits on the number of spacetime dimensions from GW170817
• Low-Mass Proto-Planet Migration in T-Tauri Alpha-Disks
• Self-interactions and Spontaneous Black Hole Scalarization
• Black-hole hair loss: learning about binary progenitors from ringdown signals
• Novel approach to binary dynamics: application to the fifth post-Newtonian level
• Conservative dynamics of binary systems to fourth Post-Newtonian order in the EFT approach II: Renormalized Lagrangian
• Gravitational waves as a probe of dark matter mini-spikes
• Classical and Quantum Results on Logarithmic Terms in the Soft Theorem in Four Dimensions
• Horava gravity vs. thermodynamics: the black hole case
• Post-Newtonian factorized multipolar waveforms for spinning, non-precessing black-hole binaries
• Testing general relativity using golden black-hole binaries
• Second-order self-force calculation of the gravitational binding energy in compact binaries
• Induced gravitational wave background and primordial black holes
• No-Go Theorems for Generalized Chameleon Field Theories
• A multipolar effective one body waveform model for spin-aligned black hole binaries
• Improved reconstruction of a stochastic gravitational wave background with LISA
• Confusion Noise from LISA Capture Sources
• Approximating the inspiral of test bodies into Kerr black holes
• Testing the no-hair theorem with black hole ringdowns using TIGER
• Bayesian analysis of LIGO-Virgo mergers: Primordial vs. astrophysical black hole populations
• The Fast and the Fiducial: Augmented kludge waveforms for detecting extreme-mass-ratio inspirals
• Supermassive Black Holes from Ultra-Strongly Self-Interacting Dark Matter
• Sensitivity to a Frequency-Dependent Circular Polarization in an Isotropic Stochastic Gravitational Wave Background
• The GW190521 Mass Gap Event and the Primordial Black Hole Scenario
• Probing Planckian corrections at the horizon scale with LISA binaries
• Detecting fundamental fields with LISA observations of gravitational waves from extreme mass-ratio inspirals
• Constraining the primordial black hole scenario with Bayesian inference and machine learning: the GWTC-2 gravitational wave catalog
• Evolution of inspiral orbits around a Schwarzschild black hole
• The Hubble Tension in Light of the Full-Shape Analysis of Large-Scale Structure Data
• Vainshtein mechanism after GW170817
• Gravitational Wave Decay into Dark Energy
• Black-hole Spectroscopy by Making Full Use of Gravitational-Wave Modeling
• Searching for Primordial Black Holes in the radio and X-ray sky
• Spinning Black Holes Fall in Love
• Sixth post-Newtonian local-in-time dynamics of binary systems
• A Geometrical Formulation of the Renormalization Group Method for Global Analysis
• Nonlinear gravitational-wave memory from binary black hole mergers
• Error-analysis and comparison to analytical models of numerical waveforms produced by the NRAR Collaboration
• Hunting for Dark Particles with Gravitational Waves
• Surface Tension and Negative Pressure Interior of a Non-Singular `Black Hole'
• Black Hole Spectroscopy: Systematic Errors and Ringdown Energy Estimates
• Surface singularities in Eddington-inspired Born-Infeld gravity
• Black holes with surrounding matter in scalar-tensor theories
• Tidal Love Numbers of Kerr Black Holes
• The Evolution of Primordial Black Holes and their Final Observable Spins
• On the gravitational wave background from compact binary coalescences in the band of ground-based interferometers
• Cosmic string loop distribution on all length scales and at any redshift
• Dynamics of spontaneous black hole scalarization and mergers in Einstein-scalar-Gauss-Bonnet gravity
• Astrophysical and theoretical physics implications from multimessenger neutron star observations
• Brane-world extra dimensions in light of GW170817
• Constraints on Einstein-aether theory after GW170817
• Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution
• Improved gravitational-wave constraints on higher-order curvature theories of gravity
• Exploring Primordial Black Holes from the Multiverse with Optical Telescopes
• Gravitational Collider Physics
• On the Vanishing of Love Numbers for Kerr Black Holes
• Binary dynamics at the fifth and fifth-and-a-half post-Newtonian orders
• Superradiant instability of massive vector fields around spinning black holes in the relativistic regime
• An eccentric binary black hole inspiral-merger-ringdown gravitational waveform model from numerical relativity and post-Newtonian theory
• Phantom dark energy from non-local infrared modifications of General Relativity
• Numerical binary black hole mergers in dynamical Chern-Simons: I. Scalar field
• Oscillations in the stochastic gravitational wave background from sharp features and particle production during inflation
• Testing general relativity using gravitational wave signals from the inspiral, merger and ringdown of binary black holes
• Probing Gravity with Spacetime Sirens
• Kerr black holes with self-interacting scalar hair: hairier but not heavier
• The Tune of Love and the Nature(ness) of Spacetime
• Phase effects from strong gravitational lensing of gravitational waves
• Challenging the Presence of Scalar Charge and Dipolar Radiation in Binary Pulsars
• Limits on primordial black holes from $\mu$ distortions in cosmic microwave background
• Static response and Love numbers of Schwarzschild black holes
• Piercing the Vainshtein screen with anomalous gravitational wave speed: Constraints on modified gravity from binary pulsars
• Leading higher-derivative corrections to Kerr geometry
• Stochastic Gravitational Wave Background from Cosmological Supernovae
• A no-go theorem for polytropic spheres in Palatini f(R) gravity
• Parametrized black hole quasinormal ringdown. II. Coupled equations and quadratic corrections for nonrotating black holes
• Probing the existence of ultralight bosons with a single gravitational-wave measurement
• Constraints on the astrophysical environment of binaries with gravitational-wave observations
• Lectures on the Cosmological Constant Problem
• Astrophysical Violations of the Kerr Bound as a Possible Signature of String Theory
• Inflationary perturbations near horizon crossing
• Gravitational self-force on generic bound geodesics in Kerr spacetime
• Evolution of Einstein-scalar-Gauss-Bonnet gravity using a modified harmonic formulation
• Accelerated gravitational-wave parameter estimation with reduced order modeling
• Osculating orbits in Schwarzschild spacetime, with an application to extreme mass-ratio inspirals
• Gauge Independence of Induced Gravitational Waves
• Anisotropy of the astrophysical gravitational wave background: analytic expression of the angular power spectrum and correlation with cosmological observations
• Matter around Kerr black holes in scalar-tensor theories: scalarization and superradiant instability
• Anisotropies and non-Gaussianity of the Cosmological Gravitational Wave Background
• Tidal Love numbers of a slowly spinning neutron star
• Cosmography with strong lensing of LISA gravitational wave sources
• Primordial Black Holes for the LIGO Events in the Axion-like Curvaton Model
• Black holes and gravitational waves in models of minicharged dark matter
• Ringdown overtones, black hole spectroscopy, and no-hair theorem tests
• Tidal deformation of a slowly rotating material body. External metric
• Scalar Induced Gravitational Waves in Different Gauges
• A statistical standard siren measurement of the Hubble constant from the LIGO/Virgo gravitational wave compact object merger GW190814 and Dark Energy Survey galaxies
• Gravitational wave echoes through new windows
• Detecting Lensing-Induced Diffraction in Astrophysical Gravitational Waves
• Extending the effective-one-body Hamiltonian of black-hole binaries to include next-to-next-to-leading spin-orbit couplings
• The influence of the hydrodynamic drag from an accretion torus on extreme mass-ratio inspirals
• Distinguishing Primordial Black Holes from Astrophysical Black Holes by Einstein Telescope and Cosmic Explorer
• Orbital Dynamics of Binary Boson Star Systems
• The Clustering Evolution of Primordial Black Holes
• Anisotropies of Gravitational Wave Backgrounds: A Line Of Sight Approach
• New X-ray bound on density of primordial black holes
• Asymptotically flat scalar, Dirac and Proca stars: discrete vs. continuous families of solutions
• Two-timescale evolution of extreme-mass-ratio inspirals: waveform generation scheme for quasicircular orbits in Schwarzschild spacetime
• Evidence for primordial black hole dark matter from LIGO/Virgo merger rates
• Testing gravitational parity violation with coincident gravitational waves and short gamma-ray bursts
• The Spatial Clustering of Primordial Black Holes
• Numerical relativity simulation of GW150914 in Einstein dilaton Gauss-Bonnet gravity
• Blue-tilted Tensor Spectrum and Thermal History of the Universe
• Measuring the distance-redshift relation with the cross-correlation of gravitational wave standard sirens and galaxies
• Exotic Compact Objects and How to Quench their Ergoregion Instability
• Numerical simulations of single and binary black holes in scalar-tensor theories: circumventing the no-hair theorem
• Perturbed Kerr Black Holes can probe deviations from General Relativity
• Spinning and excited black holes in Einstein-scalar-Gauss-Bonnet theory
• Macroscopic Effects of the Quantum Trace Anomaly
• Bayesian Evidence for Both Astrophysical and Primordial Black Holes: Mapping the GWTC-2 Catalog to Third-Generation Detectors
• Theoretical Physics Implications of Gravitational Wave Observation with Future Detectors
• How to observe a non-Kerr spacetime
• New Constraint on Scalar Gauss-Bonnet Gravity and a Possible Explanation for the Excess of the Orbital Decay Rate in a Low-Mass X-ray Binary
• Probing Fundamental Physics with Gravitational Waves: The Next Generation
• Vainshtein Screening in Scalar-Tensor Theories before and after GW170817: Constraints on Theories beyond Horndeski
• Foundations of an effective-one-body model for coalescing binaries on eccentric orbits
• Massive Vector Fields in Rotating Black-Hole Spacetimes: Separability and Quasinormal Modes
• Measuring the dark matter environments of black hole binaries with gravitational waves
• Dynamical descalarization in binary black hole mergers
• On generic parametrizations of spinning black-hole geometries
• Gravitational Waves in Modified Teleparallel Theories
• Gravitational Wave Signatures from Low-mode Spiral Instabilities in Rapidly Rotating Supernova Cores
• Modeling the gravitational wave signature of neutron star black hole coalescences: PhenomNSBH
• A gravitational-wave probe of effective quantum gravity
• Quantum diffusion beyond slow-roll: implications for primordial black-hole production
• Primordial Black Hole Dark Matter and the LIGO/Virgo observations
• Detecting scalar fields with Extreme Mass Ratio Inspirals
• Numerical relativity simulation of GW150914 beyond general relativity
• Tidal deformability and I-Love-Q relations for gravastars with polytropic thin shells
• On the local well-posedness of Lovelock and Horndeski theories
• Parameterized Post-Einsteinian Gravitational Waveforms in Various Modified Theories of Gravity
• On the final fate of compact boson star mergers
• The response of ultralight dark matter to supermassive black holes and binaries
• Constraining nonperturbative strong-field effects in scalar-tensor gravity by combining pulsar timing and laser-interferometer gravitational-wave detectors
• First predictions of the angular power spectrum of the astrophysical gravitational wave background
• Schwarzschild black holes can wear scalar wigs
• Directed searches for gravitational waves from ultralight bosons
• Probing the Universe through the Stochastic Gravitational Wave Background
• Gravitational wave echoes from black hole area quantization
• Black hole hair formation in shift-symmetric generalised scalar-tensor gravity
• Stochastic Gravitational-Wave Background from Binary Black Holes and Binary Neutron Stars and Implications for LISA
• Spherically Symmetric Solutions in Ghost-Free Massive Gravity
• Spin memory effect for compact binaries in the post-Newtonian approximation
• The Formation Probability of Primordial Black Holes
• Numerical binary black hole collisions in dynamical Chern-Simons gravity
• Hořava Gravity after GW170817
• Ultralight boson cloud depletion in binary systems
• How early is early dark energy?
• Gravitational self-force corrections to two-body tidal interactions and the effective one-body formalism
• Characterizing the continuous gravitational-wave signal from boson clouds around Galactic isolated black holes
• Gravitational wave signatures of ultralight vector bosons from black hole superradiance
• Standard sirens with a running Planck mass
• Black hole superradiant instability from ultralight spin-2 fields
• Vainshtein Mechanism in Binary Pulsars
• Ultra-slow-roll inflation with quantum diffusion
• Prospects for observing extreme-mass-ratio inspirals with LISA
• Asymptotically flat spinning scalar, Dirac and Proca stars
• Spin of Primordial Black Holes
• Ergoregion instability of exotic compact objects: electromagnetic and gravitational perturbations and the role of absorption
• Hidden Symmetry of Vanishing Love
• Signatures of non-gaussianity in the isocurvature modes of primordial black hole dark matter
• Gravito-Electromagnetic Perturbations of Kerr-Newman Black Holes: Stability and Isospectrality in the Slow-Rotation Limit
• Massive Boson Superradiant Instability of Black Holes: Nonlinear Growth, Saturation, and Gravitational Radiation
• LISA extreme-mass-ratio inspiral events as probes of the black hole mass function
• An observable signature of a background deviating from Kerr
• Self-force of a scalar field for circular orbits about a Schwarzschild black hole
• Stochastic background of gravitational waves generated by a cosmological population of young, rapidly rotating neutron stars
• How does a dark compact object ringdown?
• Environmental Effects for Gravitational-wave Astrophysics
• Strong field effects on binary systems in Einstein-aether theory
• Evolution of gas disc-embedded intermediate mass ratio inspirals in the LISA band
• Characterizing the Cosmological Gravitational Wave Background Anisotropies and non-Gaussianity
• Tidal heating as a discriminator for horizons in extreme mass ratio inspirals
• On the merger rate of primordial black holes: effects of nearest neighbours distribution and clustering
• A first search for a stochastic gravitational-wave background from ultralight bosons
• Accretion disks around binary black holes of unequal mass: GRMHD simulations of postdecoupling and merger
• Models of rotating boson stars and geodesics around them: new type of orbits
• Hamiltonian formalism for f(T) gravity
• Self-accelerating universe in scalar-tensor theories after GW170817
• Correlation function of high-threshold regions and application to the initial small-scale clustering of primordial black holes
• Dark matter spikes in the vicinity of Kerr black holes
• Electromagnetic emission from axionic clouds and the quenching of superradiant instabilities
• Black hole mimickers: regular versus singular behavior
• Gravitational wave probes of dark matter: challenges and opportunities
• Searching for black hole echoes from the LIGO-Virgo Catalog GWTC-1
• Gravitational waveforms in scalar-tensor gravity at 2PN relative order
• Post-Newtonian dynamics and black hole thermodynamics in Einstein-scalar-Gauss-Bonnet gravity
• Anisotropies in the stochastic gravitational-wave background: Formalism and the cosmic string case
• Empirical tests of the black hole no-hair conjecture using gravitational-wave observations
• Testing Chern-Simons Modified Gravity with Gravitational-Wave Detections of Extreme-Mass-Ratio Binaries
• Distinguishing fuzzballs from black holes through their multipolar structure
• Tidal deformation of a slowly rotating black hole
• A new gravitational wave generation algorithm for particle perturbations of the Kerr spacetime
• Post-Newtonian Gravitational and Scalar Waves in Scalar-Gauss-Bonnet Gravity
• Instability of the Proca field on Kerr spacetime
• Beyond Concordance Cosmology with Magnification of Gravitational-Wave Standard Sirens
• Constraints on Primordial Black Holes: the Importance of Accretion
• On the Gauge Invariance of Cosmological Gravitational Waves
• Constraining alternative theories of gravity by gravitational waves from precessing eccentric compact binaries with LISA
• Effective Field Theory of Black Hole Quasinormal Modes in Scalar-Tensor Theories
• A Multipolar Effective One Body Model for Non-Spinning Black Hole Binaries
• Bosenova and Axiverse
• Scalar hairy black holes and solitons in asymptotically flat spacetimes
• Potential gravitational-wave signatures of quantum gravity
• Pulsar Timing Array Constraints on the Induced Gravitational Waves
• Scalarized Hairy Black Holes
• The Link between Warm Molecular Disks in Maser Nuclei and Star Formation near the Black Hole at the Galactic Center
• Effective-one-body multipolar waveform for tidally interacting binary neutron stars up to merger
• Gravitational-Wave Signature of an Inspiral into a Supermassive Horizonless Object
• Gravitational waves from extreme mass-ratio inspirals in Dynamical Chern-Simons gravity
• Spectroscopy of binary black hole ringdown using overtones and angular modes
• Kerr black holes with synchronised hair: an analytic model and dynamical formation
• Probing Primordial Features with the Stochastic Gravitational Wave Background
• Quasinormal modes of slowly-rotating black holes in dynamical Chern-Simons gravity
• Dynamic Signatures of Black Hole Binaries with Superradiant Clouds
• Late Inspiral and Merger of Binary Black Holes in Scalar-Tensor Theories of Gravity
• On choosing the start time of binary black hole ringdown
• Constraining early and interacting dark energy with gravitational wave standard sirens: the potential of the eLISA mission
• An aligned-spin neutron-star--black-hole waveform model based on the effective-one-body approach and numerical-relativity simulations
• Validating the Effective-One-Body Numerical-Relativity Waveform Models for Spin-aligned Binary Black Holes along Eccentric Orbits
• Prospects for axion searches with Advanced LIGO through binary mergers
• Analytical model for gravitational-wave echoes from spinning remnants
• Detectable environmental effects in GW190521-like black-hole binaries with LISA
• Nonviolent information transfer from black holes: a field theory parameterization
• Black Hole Dynamics in Einstein-Maxwell-Dilaton Theory
• Are stellar-mass black-hole binaries too quiet for LISA?
• Polarization-based Tests of Gravity with the Stochastic Gravitational-Wave Background
• Strong lensing of gravitational waves as seen by LISA
• Determining the progenitors of merging black-hole binaries
• Hairy black-hole solutions in generalized Proca theories
• Gravitational Wave Anisotropies from Primordial Black Holes
• Search for ultralight bosons in Cygnus X-1 with Advanced LIGO
• Echoes from Quantum Black Holes
• Center-of-mass angular momentum and memory effect in asymptotically flat spacetimes
• The Initial Value Formulation of Dynamical Chern-Simons Gravity
• IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes
• Dark Sirens to Resolve the Hubble-Lemaître Tension
• Orbital fingerprints of ultralight scalar fields around black holes
• A 3PN Fourier Domain Waveform for Non-Spinning Binaries with Moderate Eccentricity
• Well-posed formulation of scalar-tensor effective field theory
• Gravitational waves from black hole binary inspiral and merger: The span of third post-Newtonian effective-one-body templates
• Effective one body Hamiltonian of two spinning black-holes with next-to-next-to-leading order spin-orbit coupling
• An Analytical Portrait of Binary Mergers in Hierarchical Triple Systems
• Gas pile-up, gap overflow, and Type 1.5 migration in circumbinary disks: application to supermassive black hole binaries
• Can we distinguish astrophysical from primordial black holes via the stochastic gravitational wave background?
• Analytical template for gravitational-wave echoes: signal characterization and prospects of detection with current and future interferometers
• A New Window into Black Holes
• Bounding the speed of gravity with gravitational wave observations
• Gravitational echoes from macroscopic quantum gravity effects
• Extreme Dark Matter Tests with Extreme Mass Ratio Inspirals
• Head-on collisions and orbital mergers of Proca stars
• Dark-Energy Instabilities induced by Gravitational Waves
• Observational Signature of the Logarithmic Terms in the Soft Graviton Theorem
• Fixing extensions to General Relativity in the non-linear regime
• Gravitational wave lensing beyond general relativity: birefringence, echoes and shadows
• The Effect of Massive Perturbers on Extreme Mass-Ratio Inspiral Waveforms
• A new analytic representation of the ringdown waveform of coalescing spinning black hole binaries
• Overtones or higher harmonics? Prospects for testing the no-hair theorem with gravitational wave detections
• Black hole scalarization induced by the spin -- 2+1 time evolution
• Quasi-normal modes of black holes in Horndeski gravity
• Gravitational-wave glitches in chaotic extreme-mass-ratio inspirals
• Scattering of particles by neutron stars: Time-evolutions for axial perturbations
• A Class of Minimally Modified Gravity Theories
• Bounding the mass of the graviton with gravitational waves: Effect of spin precessions in massive black hole binaries
• Parametrized ringdown spin expansion coefficients: a data-analysis framework for black-hole spectroscopy with multiple events
• Probing gas disc physics with LISA: simulations of an intermediate mass ratio inspiral in an accretion disc
• $\ell$-Boson stars
• Gravitational floating orbits around hairy black holes
• Exponentially growing finite energy solutions for the Klein-Gordon equation on sub-extremal Kerr spacetimes
• Prospects for direct detection of circular polarization of gravitational-wave background
• Local symmetries and physical degrees of freedom in $f(T)$ gravity: a Dirac Hamiltonian constraint analysis
• Onset of spontaneous scalarization in spinning Gauss-Bonnet black holes
• Projection effects on the observed angular spectrum of the astrophysical stochastic gravitational wave background
• Post-Kerr black hole spectroscopy
• Dynamical scalar hair formation around a Schwarzschild black hole
• Modeling and searching for a stochastic gravitational-wave background from ultralight vector bosons
• Direct detection of gravitational waves can measure the time variation of the Planck mass
• Testing Stochastic Gravitational Wave Signals from Primordial Black Holes with Optical Telescopes
• Nonlinear-in-spin effects in effective-one-body waveform models of spin-aligned, inspiralling, neutron star binaries
• Rush the inspiral: efficient Effective One Body time-domain gravitational waveforms
• Multi-messenger tests of gravity with weakly lensed gravitational waves
• Template-based Gravitational-Wave Echoes Search Using Bayesian Model Selection
• Frequency-domain gravitational waveform models for inspiraling binary neutron stars
• Parameter estimation of gravitational wave echoes from exotic compact objects
• Gravitational Collapse in Einstein dilaton Gauss-Bonnet Gravity
• GW$\times$LSS: Chasing the Progenitors of Merging Binary Black Holes
• Effective-one-body waveforms for binary neutron stars using surrogate models
• Probing microstructure of black hole spacetimes with gravitational wave echoes
• Black Hole Hair from Scalar Dark Matter
• Black hole ringdown echoes and howls
• Restoring General Relativity in massive bi-gravity theory
• Probing non-Gaussian Stochastic Gravitational Wave Backgrounds with LISA
• Gravitational Wave Tests of Strong Field General Relativity with Binary Inspirals: Realistic Injections and Optimal Model Selection
• Gravitational Radiation in Horava Gravity
• LISA Sensitivities to Gravitational Waves from Relativistic Metric Theories of Gravity
• The MACHO Project: Microlensing Detection Efficiency
• Binary Pulsar Constraints on the Parameterized post-Einsteinian Framework
• The Third RIT binary black hole simulations catalog
• Vainshtein regime in Scalar-Tensor gravity: constraints on DHOST theories
• The electromagnetic chirp of a compact binary black hole: a phase template for the gravitational wave inspiral
• Effective stability against superradiance of Kerr black holes with synchronised hair
• Eikonal quasinormal modes of black holes beyond General Relativity
• Jumping the gap: searching for LIGO's biggest black holes
• The gravitational-wave memory from eccentric binaries
• Fast Self-forced Inspirals
• Gravitational-Wave Constraints on an Effective Field-Theory Extension of General Relativity
• Axion boson stars
• A first survey of spinning eccentric black hole mergers: Numerical relativity simulations, hybrid waveforms, and parameter estimation
• Measuring the speed of cosmological gravitational waves
• Extreme mass-ratio inspirals around a spinning horizonless compact object
• Effects of modified gravity on B-mode polarization
• Self force on a scalar charge in Kerr spacetime: circular equatorial orbits
• Persistent gravitational wave observables: general framework
• Hyperbolicity in Spherical Gravitational Collapse in a Horndeski Theory
• Frequency domain model of $f$-mode dynamic tides in gravitational waveforms from compact binary inspirals
• On the Primordial Black Hole Mass Function for Broad Spectra
• Golden Binary Gravitational-Wave Sources: Robust Probes of Strong-Field Gravity
• Black-hole microstate spectroscopy: ringdown, quasinormal modes, and echoes
• Tidal deformability of dressed black holes and tests of ultralight bosons in extended mass ranges
• Gravitational wave cosmology with extreme mass-ratio inspirals
• Multi-messenger Probes of Inflationary Fluctuations and Primordial Black Holes
• Non-perturbative spinning black holes in dynamical Chern-Simons gravity
• A measurement of the Hubble constant from angular diameter distances to two gravitational lenses
• Particle on the Innermost Stable Circular Orbit of a Rapidly Spinning Black Hole
• Probing the nature of central objects in extreme-mass-ratio inspirals with gravitational waves
• The Minimum Testable Abundance of Primordial Black Holes at Future Gravitational-Wave Detectors
• Echoes from the Abyss: A highly spinning black hole remnant for the binary neutron star merger GW170817
• Intermediate mass-ratio black hole binaries: Applicability of small mass-ratio perturbation theory
• Primordial Black Holes from Broad Spectra: Abundance and Clustering
• Multi-wavelength astronomical searches for primordial black holes
• Self force on a scalar charge in Kerr spacetime: eccentric equatorial orbits
• A morphology-independent data analysis method for detecting and characterizing gravitational wave echoes
• Nonviolent unitarization: basic postulates to soft quantum structure of black holes
• Galileon Radiation from Binary Systems
• Black Hole Echology: The Observer's Manual
• Parameterized and inspiral-merger-ringdown consistency tests of gravity with multi-band gravitational wave observations
• Gravitational Wave Background from Magnetars
• Bridging the $\mu$Hz gap in the gravitational-wave landscape with binary resonance
• General relativistic simulations of the quasi-circular inspiral and merger of charged black holes: GW150914 and fundamental physics implications
• Limitations of the adiabatic approximation to the gravitational self-force
• Radiation-reaction force on a particle plunging into a black hole
• Growth of resonances and chaos for a spinning test particle in the Schwarzschild background
• Quest for circular polarization of gravitational wave background and orbits of laser interferometers in space
• Spectral separation of the stochastic gravitational-wave background for LISA: observing both cosmological and astrophysical backgrounds
• Resolving the Structure of Black Holes: Philosophizing with a Hammer
• A morphology-independent search for gravitational wave echoes in data from the first and second observing runs of Advanced LIGO and Advanced Virgo
• On the growth of massive scalar hair around a Schwarzschild black hole
• Modeling the horizon-absorbed gravitational flux for equatorial-circular orbits in Kerr spacetime
• Gravitational-wave signatures of the absence of an event horizon. II. Extreme mass ratio inspirals in the spacetime of a thin-shell gravastar
• Black holes and solitons in an extended Proca theory
• On gravitational-wave echoes from neutron-star binary coalescences
• Scalar field self-force effects on orbits about a Schwarzschild black hole
• Gravitational wave energy emission and detection rates of Primordial Black Hole hyperbolic encounters
• Measuring Speed of Gravitational Waves by Observations of Photons and Neutrinos from Compact Binary Mergers and Supernovae
• Stellar binary black holes in the LISA band: a new class of standard sirens
• Constraining black hole mimickers with gravitational wave observations
• Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions
• Multiparameter tests of general relativity using multiband gravitational-wave observations
• Constraining the dark energy equation of state using LISA observations of spinning Massive Black Hole binaries
• Gravitational wave sources: reflections and echoes
• Propagation of gravitational waves in teleparallel gravity theories
• The Impact of Peculiar Velocities on the Estimation of the Hubble Constant from Gravitational Wave Standard Sirens
• Parameter estimation for black hole echo signals and their statistical significance
• Arrival time differences between gravitational waves and electromagnetic signals due to gravitational lensing
• Self-consistent orbital evolution of a particle around a Schwarzschild black hole
• Polarization test of gravitational waves from compact binary coalescences
• Motion of small objects in curved spacetimes: An introduction to gravitational self-force
• Incompleteness Matters Not: Inference of $H_0$ from BBH-galaxy cross-correlations
• Hairy binary black holes in Einstein-Maxwell-dilaton theory and their effective-one-body description
• Foreground cleaning and template-free stochastic background extraction for LISA
• Horizon-absorption effects in coalescing black-hole binaries: An effective-one-body study of the non-spinning case
• Detectability of ultra-compact X-ray binaries as LISA sources
• General parametrization of black holes: the only parameters that matter
• Stochastic background of gravitational waves emitted by magnetars
• A Mock Data and Science Challenge for Detecting an Astrophysical Stochastic Gravitational-Wave Background with Advanced LIGO and Advanced Virgo
• The clustering dynamics of primordial black boles in $N$-body simulations
• CLASS_GWB: robust modeling of the astrophysical gravitational wave background anisotropies
• Rapidly rotating black holes in dynamical Chern-Simons gravity: Decoupling limit solutions and breakdown
• Constraining Primordial Black Holes with Dwarf Galaxy Heating
• Black Holes Lessons from Multipole Ratios
• Environmental effects in GW physics: tidal deformability of black holes immersed in matter
• Type I Migration in a Non-Isothermal Protoplanetary Disk
• Exotic compact objects with soft hair
• Spherically symmetric static solutions in a non-local infrared modification of General Relativity
• Dynamical formation of Proca stars and quasi-stationary solitonic objects
• Gravitational-wave cosmography with LISA and the Hubble tension
• Graviton mass bounds from space-based gravitational-wave observations of massive black hole populations
• Towards reconstructing the quantum effective action of gravity
• Gravitational-wave detection and parameter estimation for accreting black-hole binaries and their electromagnetic counterpart
• The stochastic gravitational-wave background in the absence of horizons
• General theories of linear gravitational perturbations to a Schwarzschild Black Hole
• Probing Gravitational Parity Violation with Gravitational Waves from Stellar-mass Black Hole Binaries
• Nonlinear/non-iterative treatment of EFT-motivated gravity
• Combined search for anisotropic birefringence in the gravitational-wave transient catalog GWTC-1
• Searching for ultralight bosons within spin measurements of a population of binary black hole mergers
• Thermal Decay without Information Loss in Horizonless Microstate Geometries
• Detecting the anisotropic astrophysical gravitational wave background in the presence of shot noise through cross-correlations
• Constraints on general second-order scalar-tensor models from gravitational Cherenkov radiation
• Quest for the extra degree of freedom in f(T) gravity
• Stirred and shaken: dynamical behavior of boson stars and dark matter cores
• Chaos and Order in Models of Black Hole Pairs
• Vector boson star solutions with a quartic order self-interaction
• Mis-Modelling in Gravitational Wave Astronomy: The Trouble With Templates
• Impact of multiple modes on the black-hole superradiant instability
• Weak annihilation cusp inside the dark matter spike about a black hole
• Gravitational wave constraints on dark sector models
• A semi-coherent analysis method to search for continuous gravitational waves emitted by ultra-light boson clouds around spinning black holes
• Bounding Alternative Theories of Gravity with Multi-Band GW Observations
• Love in Extrema Ratio
• A Unique Multi-Messenger Signal of QCD Axion Dark Matter
• Nonlocal star as a blackhole mimicker
• Testing the multipole structure of compact binaries using gravitational wave observations
• The multipolar structure of fuzzballs
• Probing large distance higher dimensional gravity from lensing data
• Pure states don't wear black
• Second-order perturbation theory: problems on large scales
• Generic searches for alternative gravitational wave polarizations with networks of interferometric detectors
• Towards the nonlinear regime in extensions to GR: assessing possible options
• Towards numerical relativity in scalar Gauss-Bonnet gravity: 3+1 decomposition beyond the small-coupling limit
• A "no-hair" test for binary black holes
• Retarded Green's Function Of A Vainshtein System And Galileon Waves
• Non-local gravity and comparison with observational datasets. II. Updated results and Bayesian model comparison with $\Lambda$CDM
• Quasi-Black Holes from Extremal Charged Dust
• Gravitational-wave versus X-ray tests of strong-field gravity
• Maximum likelihood map-making with the Laser Interferometer Space Antenna
• Signature of chaos in gravitational waves from a spinning particle
• Fuzzballs and Observations
• The accretion of migrating giant planets
• Constraints on Hořava gravity from binary black hole observations
• Concise estimate of the expected number of detections for stellar-mass binary black holes by eLISA
• Testing nonlocal gravity with Lunar Laser Ranging
• Dissipation in extreme-mass ratio binaries with a spinning secondary
• Quasi-circular inspirals and plunges from non-spinning effective-one-body Hamiltonians with gravitational self-force information
• Spinning black holes in shift-symmetric Horndeski theory
• Nonlinear curvature effects in gravitational waves from inspiralling black hole binaries
• Rotating Axion Boson Stars
• A Systematic Study of the Stochastic Gravitational-Wave Background due to Stellar Core Collapse
• Multipolar boson stars: macroscopic Bose-Einstein condensates akin to hydrogen orbitals
• Projected Constraints on Lorentz-Violating Gravity with Gravitational Waves
• How does the cosmic large-scale structure bias the Hubble diagram?
• No evidence of kinetic screening in simulations of merging binary neutron stars beyond general relativity
• Resonant Decay of Gravitational Waves into Dark Energy
• Finding Horndeski theories with Einstein gravity limits
• Ability of LISA to detect a gravitational-wave background of cosmological origin: the cosmic string case
• Multi-band gravitational wave tests of general relativity
• Gravity with Auxiliary Fields
• Axion star collisions with black holes and neutron stars in full 3D numerical relativity
• Gravitational Wave Oscillations in Bigravity
• Kinetic screening in nonlinear stellar oscillations and gravitational collapse
• Maximum redshift of gravitational wave merger events
• Follow-up signals from superradiant instabilities of black hole merger remnants
• Gravity in the infrared and effective nonlocal models
• Standard-siren cosmology using gravitational waves from binary black holes
• Relativistic orbits around spinning supermassive black holes. Secular evolution to 4.5 post-Newtonian order
• Scalar Hairy Black Holes in Four Dimensions are Unstable
• Brans-Dicke theory in Bondi-Sachs form: Asymptotically flat solutions, asymptotic symmetries and gravitational-wave memory effects
• Pure polarization test of GW170814 and GW170817 using waveforms consistent with modified theories of gravity
• Relaxing the Cosmological Constant: a Proof of Concept
• Scalar Gravitational Radiation from Binaries: Vainshtein Mechanism in Time-dependent Systems
• Polarization of a stochastic gravitational wave background through diffusion by massive structures
• Classical and Quantum Decay of Oscillatons: Oscillating Self-Gravitating Real Scalar Field Solitons
• Detecting stochastic gravitational waves with binary resonance
• Schwarzschild scalar wigs: spectral analysis and late time behavior
• Black holes as collapsed polymers
• The tune of the universe: the role of plasma in tests of strong-field gravity
• Hearing gravity from the cosmos: GWTC-2 probes general relativity at cosmological scales
• Gravitational memory effects and Bondi-Metzner-Sachs symmetries in scalar-tensor theories
• Exploring galaxies-gravitational waves cross-correlations as an astrophysical probe
• Cross-correlation of the astrophysical gravitational-wave background with galaxy clustering
• Gravitational-wave memory effects in Brans-Dicke theory: Waveforms and effects in the post-Newtonian approximation
• On the hyperbolicity of the most general Horndeski theory
• Tidal effects and disruption in superradiant clouds: a numerical investigation
• Cosmology with coalescing massive black holes
• Validity of common modelling approximations for precessing binary black holes with higher-order modes
• Primordial gravity wave background anisotropies
• Multiband gravitational-wave searches for ultralight bosons
• Classification of shift-symmetric Horndeski theories and hairy black holes
• Accelerating the evaluation of inspiral-merger-ringdown waveforms with adapted grids
• Two-body problem in Scalar-Tensor theories as a deformation of General Relativity : an Effective-One-Body approach
• Compact object scalarization with general relativity as a cosmic attractor
• Early Scrambling and Capped BTZ Geometries
• Stochastic gravitational-wave background in quantum gravity
• Eikonal quasinormal modes of black holes beyond general relativity II: generalised scalar-tensor perturbations
• Gravitational Wave "Echo" Spectra
• Tests of general relativity with stellar-mass black hole binaries observed by LISA
• Chaos at the rim of black hole and fuzzball shadows
• Can we probe Planckian corrections at the horizon scale with gravitational waves?
• Prospects of discovering sub-solar primordial black holes using the stochastic gravitational wave background from third-generation detectors
• Detecting the Stochastic Gravitational Wave Background from Primordial Black Hole Formation
• Cross-correlating galaxy catalogs and gravitational waves: a tomographic approach
• Synchronised gravitational atoms from mergers of bosonic stars
• Gravitational-wave detectors as particle-physics laboratories: Constraining scalar interactions with a coherent inspiral model of boson-star binaries
• Reducing the two-body problem in scalar-tensor theories to the motion of a test particle : a scalar-tensor effective-one-body approach
• Improved limits on a stochastic gravitational-wave background and its anisotropies from Advanced LIGO O1 and O2 runs
• Scalar and tensor gravitational waves
• Assessing the Readiness of Numerical Relativity for LISA and 3G Detectors
• Bayesian Metric Reconstruction with Gravitational Wave Observations
• Standard Sirens as a novel probe of dark energy
• Rotating black holes in Einstein-aether theory
• Accuracy Issues for Numerical Waveforms
• The Speed of Galileon Gravity
• Growth of accretion driven scalar hair around Kerr black holes
• Infinite towers of supertranslation and superrotation memories
• Spin-induced scalarization of Kerr black holes with a massive scalar field
• Horndeski gravity and standard sirens
• Causality and black holes in spacetimes with a preferred foliation
• Black holes with synchronised Proca hair: linear clouds and fundamental non-linear solutions
• Dynamics of Screening in Modified Gravity
• How well can ultracompact bodies imitate black hole ringdowns?
• Fast, faithful, frequency-domain effective-one-body waveforms for compact binary coalescences
• Effective Field Theory of Black Hole Echoes
• Interpreting spacetimes of any dimension using geodesic deviation
• Optimizing LIGO with LISA forewarnings to improve black-hole spectroscopy
• Peculiar velocities in the local Universe: comparison of different models and the implications for $H_0$ and dark matter
• Characterisation of lensing selection effects for LISA massive black hole binary mergers
• The dark side of fuzzball geometries
• Electromagnetic Bursts from Mergers of Oscillons in Axion-like Fields
• Gravitational wave propagation beyond geometric optics
• Probing beyond-Kerr spacetimes with inspiral-ringdown corrections to gravitational waves
• General Relativistic Dynamics of an Extreme Mass-Ratio Binary interacting with an External Body
• Kerr black holes with synchronised scalar hair and higher azimuthal harmonic index
• From micro to macro and back: probing near-horizon quantum structures with gravitational waves
• On the radial stability of ultra compact Schwarzschild stars beyond the Buchdahl limit
• GW190425, GW190521 and GW190814: Three candidate mergers of primordial black holes from the QCD epoch
• Joint cosmological inference of standard sirens and gravitational wave weak lensing
• The Astro-Primordial Black Hole Merger Rates: a Reappraisal
• Apparent Superluminality of Lensed Gravitational Waves
• Probing Fuzzballs with Particles, Waves and Strings
• On Detecting Equatorial Symmetry Breaking with LISA
• Nonlocal gravity and gravitational-wave observations
• Stochastic Gravitational Wave Background from Neutron Star r-mode Instability Revisited
• Quenching Mechanisms of Photon Superradiance
• Post-Newtonian phase accuracy requirements for stellar black hole binaries with LISA
• Tidal Love numbers of Proca stars
• Photon sector analysis of Super and Lorentz symmetry breaking: effective photon mass, bi-refringence and dissipation
• On the validity of the adiabatic approximation in compact binary inspirals
• Testing the multipole structure and conservative dynamics of compact binaries using gravitational wave observations: The spinning case
• Testing Gravity with Gravitational Wave Source Counts
• Exploring strong-field deviations from general relativity via gravitational waves
• Gravitational waves from extreme mass ratio inspirals around bumpy black holes
• Fourth post-Newtonian effective-one-body Hamiltonians with generic spins
• Probing cosmological fields with gravitational wave oscillations
• Limitations on Standard Sirens tests of gravity from screening
• Prospects for gravitational-wave polarization test from compact binary mergers with future ground-based detectors
• Testing massive-field modifications of gravity via gravitational waves
• Numerical Black Hole Solutions in Modified Gravity Theories: Axial Symmetry Case
• Gravitational Wave - Gauge Field Oscillations
• Stability of rotating black holes in Einstein dilaton Gauss-Bonnet gravity
• Evolving Metric Perturbations in dynamical Chern-Simons Gravity
• Non-Singular Black Holes in Massive Gravity: Time-Dependent Solutions
• Imprints of Axion Superradiance in the CMB
• Distinguishing black holes from horizonless objects through the excitation of resonances during inspiral
• Self force on a scalar charge in Kerr spacetime: inclined circular orbits
• Absorption by black hole remnants in metric-affine gravity
• Theory-agnostic framework for dynamical scalarization of compact binaries
• Nonlocality amplifies echoes
• Quantum Black Hole Seismology I: Echoes, Ergospheres, and Spectra
• Stochastic Gravitational Wave Background and Eccentric Stellar Compact Binaries
• Constraining modified theories of gravity with gravitational wave stochastic background
• Integrability of eccentric, spinning black hole binaries up to second post-Newtonian order
• Testing the"no-hair" nature of binary black holes using the consistency of multipolar gravitational radiation
• Probing primordial black holes with anisotropies in stochastic gravitational-wave background
• Firewalls in General Relativity
• A morphology-independent test of the mixed polarization content of gravitational wave signals from compact binary coalescences
• Repeated faint quasinormal bursts in extreme-mass-ratio inspiral waveforms: Evidence from frequency-domain scalar self-force calculations on generic Kerr orbits
• Deformation of the gravitational wave spectrum by density perturbations
• Exact Black Hole Solutions in Modified Gravity Theories: Spherical Symmetry Case
• Cosmology and the massive photon frequency shift in the Standard-Model Extension
• The broad Fe Kα line and supermassive black holes
• Scalar-tensor mixed polarization search of gravitational waves
• Searching for Cross-Correlation Between Stochastic Gravitational Wave Background and Galaxy Number Counts
• NANOGrav Hints on Planet-Mass Primordial Black Holes
• Black Hole Ringdown as a Probe for Dark Energy
• The exact dynamical Chern Simons metric for a spinning black hole possesses a fourth constant of motion: A Dynamical-Systems-Based Conjecture
• Black holes in quartic-order beyond-generalized Proca theories
• Discovering the interior of black holes
• Using LISA-like Gravitational Wave Detectors to Search for Primordial Black Holes
• Well-posed Cauchy formulation for Einstein-æther theory
• Gravitational wave astronomy with radio galaxy surveys
• Effective-one-body Hamiltonian with next-to-leading order spin-spin coupling for two nonprecessing black holes with aligned spins
• Evolution and spherical collapse in Einstein-aether theory and Horava gravity
• Astrophysical Signatures of Black holes in Generalized Proca Theories
• Dark Matter Simulations with Primordial Black Holes in the Early Universe
• A Measurement of the Hubble Constant using Gravitational Waves from the Binary Merger GW190814
• Detecting Lorentz Violations with Gravitational Waves from Black Hole Binaries
• Probing string-inspired gravity with the inspiral-merger-ringdown consistency tests of gravitational waves
• Deriving analytic solutions for compact binary inspirals without recourse to adiabatic approximations
• Improved Moving Puncture Gauge Conditions for Compact Binary Evolutions
• Lunar Laser Ranging constraints on nonminimally coupled dark energy and standard sirens
• Rotating tensor-multiscalar black holes with two scalars
• Density spikes near black holes in self-interacting dark matter halos and indirect detection constraints
• Self-force as probe of internal structure
• Axisymmetric deformations of neutron stars and gravitational-wave astronomy
• On arrival time difference between lensed gravitational waves and light
• Waves from the Centre: Probing PBH and other Macroscopic Dark Matter with LISA
• Phase decoherence of gravitational wave backgrounds
• Gauge Invariant Second Order Gravitational Waves
• Probing the universality of synchronised hair around rotating black holes with Q-clouds
• Ultralight scalars and resonances in black-hole physics
• Observing Eccentricity Oscillations of Binary Black Holes in LISA
• Gravitational self-force in scalar-tensor gravity
• Gravitational self-force in nonvacuum spacetimes
• Predicting the properties of black holes merger remnants with Deep Neural Networks
• Testing the Kerr nature of intermediate-mass and supermassive black hole binaries using spin-induced multipole moment measurements
• Parametrizations for tests of gravity
• Effects of primordial black holes quantum gravity decay on galaxy clustering
• Stochastic backgrounds of gravitational waves from extragalactic sources
• Physical interpretation of Kundt spacetimes using geodesic deviation
• Probing Screening and the Graviton Mass with Gravitational Waves
• Parameterised Post-Newtonian Expansion in Screened Regions
• Parameterised post-Newtonian formalism for the effective field theory of dark energy via screened reconstructed Horndeski theories
• Gravitational Waves from Peaks
• Cosmology with subdominant Horndeski scalar field
• Spinning boson stars and hairy black holes with non-minimal coupling
• Constraining Gravity with Eccentric Gravitational Waves: Projected Upper Bounds and Model Selection
• Pulsating relativistic stars
• Quantum Love
• Parameter Estimation for Tests of General Relativity with the Astrophysical Stochastic Gravitational Wave Background
• Gravitational couplings in Chameleon models
• Spin-perturbed orbits near black holes
• Primordial Black-Hole and Macroscopic Dark-Matter Constraints with LISA
• Arrival Time Differences of Lensed Massive Gravitational Waves
• No-hair theorems for non-canonical self-gravitating static multiple scalar fields
• Self-force on a scalar charge in a circular orbit about a Reissner-Nordström black hole

Cited by in corpus (167)

• Cosmology with the Laser Interferometer Space Antenna
• Gravitational waves from extreme-mass-ratio systems in astrophysical environments
• Gravitational waveforms for compact binaries from second-order self-force theory
• Primordial non-gaussianity up to all orders: theoretical aspects and implications for primordial black hole models
• Spontaneous scalarization
• Exotic Compact Objects and the Fate of the Light-Ring Instability
• The Science of the Einstein Telescope
• Probing vector hair of black holes with extreme mass ratio inspirals
• Gravitational-wave imprints of compact and galactic-scale environments in extreme-mass-ratio binaries
• Extreme mass-ratio inspirals into black holes surrounded by scalar clouds
• Probing astrophysical environment with eccentric extreme mass-ratio inspirals
• Extreme mass-ratio inspirals in ultra-light dark matter
• Polarizations of Gravitational Waves in the Bumblebee Gravity Model
• Massive black hole binaries in LISA: multimessenger prospects and electromagnetic counterparts
• Gravitational bremsstrahlung from spinning binaries in the post-Minkowskian expansion
• Primordial Black Hole Formation in Starobinsky's Linear Potential Model
• Periodic orbits and their gravitational wave radiations in a polymer black hole in loop quantum gravity
• Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM
• Well-posedness of the four-derivative scalar-tensor theory of gravity in singularity avoiding coordinates
• Possible Causes of False General Relativity Violations in Gravitational Wave Observations
• Primordial black holes in the curvaton model: possible connections to pulsar timing arrays and dark matter
• Probing the Effective Quantum Gravity via Quasinormal Modes and Shadows of Black Holes
• Priorities in gravitational waveforms for future space-borne detectors: vacuum accuracy or environment?
• Quasinormal modes and gray-body factors of regular black holes in asymptotically safe gravity
• Quasinormal modes of black holes embedded in halos of matter
• Pulsar and cosmic variances of pulsar timing-array correlation measurements of the stochastic gravitational wave background
• Tidal Love Numbers of Novel and Admixed Celestial Objects
• Can gravitational-wave memory help constrain binary black-hole parameters? A LISA case study
• Transition from Regular Black Holes to Wormholes in Covariant Effective Quantum Gravity: Scattering, Quasinormal Modes, and Hawking Radiation
• Extreme-mass-ratio inspirals into rotating boson stars: nonintegrability, chaos, and transient resonances
• Stochastic gravitational wave background phenomenology in a pulsar timing array
• Non-Minimal Einstein-Yang-Mills Black Holes: Fundamental Quasinormal Mode and Grey-Body factors versus Outburst of Overtones
• Signatures of ultralight bosons in the orbital eccentricity of binary black holes
• Space-based gravitational wave signal detection and extraction with deep neural network
• Exploiting the Einstein Telescope to solve the Hubble tension
• Galaxy fields of LISA massive black hole mergers in a simulated Universe
• Geodesics and gravitational waves in chaotic extreme-mass-ratio inspirals: the curious case of Zipoy-Voorhees black-hole mimickers
• Cavity effect in the quasinormal mode spectrum of topological stars
• Null geodesics, causal structure, and matter accretion in Lorentzian-Euclidean black holes
• Extreme Love in the SPA: constraining the tidal deformability of supermassive objects with extreme mass ratio inspirals and semi-analytical, frequency-domain waveforms
• Analytic solutions for the motion of spinning particles near spherically symmetric black holes and exotic compact objects
• Exploring waveforms with non-GR deviations for extreme mass-ratio inspirals
• Long-lived Quasinormal modes around regular black holes and wormholes in Covariant Effective Quantum Gravity
• Prospects of detecting deviations to Kerr geometry with radiation reaction effects in EMRIs
• Parameter Estimation of Stellar Mass Binary Black Holes under the Network of TianQin and LISA
• Extreme mass ratio inspirals in galaxies with dark matter halos
• Testing general relativity with TianQin: the prospect of using the inspiral signals of black hole binaries
• A declining major merger fraction with redshift in the local Universe from the largest-yet catalog of major and minor mergers in SDSS
• Bayesian parameter estimation on boson-star binary signals with a coherent inspiral template and spin-dependent quadrupolar corrections
• Periodic orbits and gravitational wave radiation in short hair black hole spacetimes for an extreme mass ratio system
• Searching for New Physics in Ultradense Environment: a Review on Dark Matter Admixed Neutron Stars
• Parameter Estimation for Stellar-Origin Black Hole Mergers In LISA
• Periodic orbits and their gravitational wave radiations around the Schwarzschild-MOG black hole
• Multimessenger study of merging massive black holes in the OBELISK simulation: gravitational waves, electromagnetic counterparts, and their link to galaxy and black hole populations
• Frequency space derivation of linear and non-linear memory gravitational wave signals from eccentric binary orbits
• A Lensing-Band Approach to Spacetime Constraints
• Minidisk Influence on Flow Variability in Accreting Spinning Black Hole Binaries: Simulations in Full General Relativity
• Fully Relativistic Treatment of Extreme Mass-Ratio Inspirals in Collisionless Environments
• Accretion properties of X-ray AGN: Evidence for radiation-regulated obscuration with redshift-dependent host galaxy contribution
• Extreme mass ratio inspirals in rotating dark matter spikes
• Analytic Solution for the Motion of Spinning Particles in Kerr Space-Time
• Gravitational waves from binary black holes in a self-interacting scalar dark matter cloud
• Time Evolution of Black Hole Perturbations in Quadratic Gravity
• Gravitational atoms in the braneworld scenario
• Electromagnetic Follow-up Observations of Binary Neutron Star Mergers with Early Warnings from Decihertz Gravitational-wave Observatories
• Self-Interacting Gravitational Atoms in the Strong-Gravity Regime
• Gravitational wave polarizations with different propagation speeds
• Black-hole spectroscopy: quasinormal modes, ringdown stability and the pseudospectrum
• Probing fundamental physics with Extreme Mass Ratio Inspirals: a full Bayesian inference for scalar charge
• Systematics in tests of general relativity using LISA massive black hole binaries
• Perturbing the vortex: quasinormal and quasibound spectra of rotating acoustic geometries
• Stellar-mass black-hole binaries in LISA: characteristics and complementarity with current-generation interferometers
• Black Hole Greybody Factors from Korteweg-de Vries Integrals: Theory
• Black hole mergers as tracers of spinning massive black hole and galaxy populations in the OBELISK simulation
• Testing gravity with Extreme-Mass-Ratio Inspirals
• GRFolres: A code for modified gravity simulations in strong gravity
• Resumming Post-Minkowskian and Post-Newtonian gravitational waveform expansions
• Implementation of a GHZ-Teukolsky puncture scheme for gravitational self-force calculations
• Black Hole Greybody Factors from Korteweg-de Vries Integrals: Computation
• Black hole minimum size and scalar charge in shift-symmetric theories
• Post-Newtonian expansions of extreme mass ratio inspirals of spinning bodies into Schwarzschild black holes
• Quasinormal modes of slowly-spinning horizonless compact objects
• Gravitational-wave background in bouncing models from semi-classical, quantum and string gravity
• Differentially rotating scalarized neutron stars with realistic post-merger profile
• A generalized uncertainty-inspired quantum black hole
• Slowly-rotating compact objects: the nonintegrability of Hartle-Thorne particle geodesics
• Constraining the EdGB Theory with Extreme Mass-Ratio Inspirals
• Evolution of a black hole cluster in full general relativity
• GWSpace: a multi-mission science data simulator for space-based gravitational wave detection
• Resonant orbits of rotating black holes beyond circularity: Discontinuity along parameter shift
• Post-Newtonian effects in compact binaries with a dark matter spike: A Lagrangian approach
• Perturbative and non-linear analyses of gravitational turbulence in spacetimes with stable light rings
• Second-order gravitational self-force in a highly regular gauge: Covariant and coordinate punctures
• Inferring Black Hole Spin from Interferometric Measurements of the First Photon Ring: A Geometric Approach
• The Effect of Multiple Cooling Channels on the Formation of Dark Compact Objects
• Whispers from the quantum core: the ringdown of semiclassical stars
• Quasinormal modes of hairy black holes in shift-symmetric theories
• The effect of quantum decoherence on inflationary gravitational waves
• Resonant excitation of eccentricity in spherical extreme-mass-ratio inspirals
• Distinguish the environmental effects and modified theory of gravity with multiple massive black-hole binaries
• Muffled Murmurs: Environmental effects in the LISA stochastic signal from stellar-mass black hole binaries
• Fundamental Physics and Cosmology with TianQin
• EMRI_MC: A GPU-based Python code for Bayesian inference of EMRI waveforms
• Ringdowns for black holes with scalar hair: the large mass case
• Echoes from beyond: Detecting gravitational-wave quantum imprints with LISA
• Prospects for detecting neutron star-white dwarf mergers with decihertz gravitational-wave observatories
• Eccentricity distribution of extreme mass ratio inspirals
• Scalar Dark Energy Models and Scalar-Tensor Gravity: Theoretical Explanations for the Accelerated Expansion of Present Universe
• Coincident Multimessenger Bursts from Eccentric Supermassive Binary Black Holes
• Nature of phase transitions and metastability in scalar-tensor theories
• Post-Newtonian Dynamics of Spinning Black Hole Binaries in Einstein-Scalar-Gauss-Bonnet Gravity
• Gravitational probe of quantum spacetime
• Squeezed gravitons from superradiant axion fields around rotating black holes
• What do gravitational wave detectors say about polymer quantum effects?
• New model of spontaneous scalarization of black holes induced by curvature and matter
• Non-Gaussianities and Primordial Black Holes
• Systematic bias in LISA ringdown analysis due to waveform inaccuracy
• Black-hole hair from vector dark matter accretion
• Kerr--Newman Memory Effect
• Analytical model of precessing binaries using post-Newtonian theory in the extreme mass-ratio limit I: General Formalism
• Extreme mass ratio inspirals around topological stars
• Constraints on Einstein-dilaton Gauss-Bonnet gravity with Taiji
• Toward Second-Order Self-Force for Eccentric Extreme-Mass Ratio Inspirals in Schwarzschild Spacetime
• Gravitational radiation reaction around a static black hole surrounded by a Dehnen type dark matter halo
• Phase transitions of boson stars in scalar-tensor theories
• Effects of eccentricity on accreting binary black holes: MHD simulations in full GR reveal novel periodicities in jet power and synchrotron spectra
• On the anisotropies of the cosmological gravitational-wave background from pulsar timing array observations
• Scalar fields around black hole binaries in LIGO-Virgo-KAGRA
• Beware of the running $n_s$ when producing heavy primordial black holes
• Spectral instability of horizonless compact objects within astrophysical environments
• The Hamiltonian constraint in the symmetric teleparallel equivalent of general relativity
• Korteweg-de Vries Integrals for Modified Black Hole Potentials: Instabilities and other Questions
• Log-periodic gravitational-wave background beyond Einstein gravity
• Morphology of Relativistically Broadened Line Emission from Axisymmetric Equatorial Accretion Disks
• A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments
• Primordial gravitational waves and curvature perturbations induced energy density perturbation
• Master variables and Darboux symmetry for axial perturbations of the exterior and interior of black hole spacetimes
• Non-linear effects on the Cosmological Gravitational Wave Background anisotropies
• Analytic solutions for the motion of spinning particles near brane-world black hole
• Multi-parameter Tests of General Relativity Using Bayesian Parameter Estimation with Principal Component Analysis for LISA
• Exotic Encounters: Buchdahl's Conditions and Physical Black Holes
• Ten years of extreme gravity tests of general theory of relativity with gravitational-wave observations
• Natural polynomials for Kerr quasi-normal modes
• $\varphi$-modes of neutron stars in a massless scalar-tensor theory
• A Parametrized Test of General Relativity for LISA Massive Black Hole Binary Inspirals
• Gravitational waves from equatorially eccentric extreme mass ratio inspirals around swirling Kerr black holes
• Estimating the gravitational wave background anisotropy: a Bayesian approach boosted by cross-correlation angular power spectrum
• Mass and spin coevolution of black holes inspiralling through dark matter
• Constraining the quantum gravity polymer scale using LIGO data
• Neutron stars more compact than black holes as a probe of strong-field gravity
• Test gravitational waves in sandwich wave background
• Neutron stars more compact than black holes in quasi-topological gravity: Equilibrium configurations and radial stability
• Systematic biases in parameter estimation on LISA binaries. II. The effect of excluding higher harmonics for spin-aligned, high-mass binaries
• Rapidly Rotating Neutron Star Collapse in Massive Scalar-Tensor Theories
• Scalar and Spinor Quasi Normal Modes of a 2D Dilatonic Blackhole
• Estimating High-Order Time Derivatives of Kerr Orbital Functionals
• Exploring black holes with multiple photon spheres by interferometric signatures
• Binary black holes gone MAD: Magnetically arrested minidisks around nonspinning black holes
• There and back again: Outspiraling motion in non-Kerr compact objects
• Particles with precessing spin in Kerr spacetime: analytic solutions for eccentric orbits and homoclinic motion near the equatorial plane
• Global time-frequency search for stellar-mass binary black holes in LISA
• Apparent horizon as a membrane
• Gravitational waves from parabolic encounters: A study of linear and nonlinear memory
• Source Confusion of Massive Black Hole Binaries for the Taiji Mission
• Trails of clouds in binary black holes
• The Dark Side of the Moon: Listening to Scalar-Induced Gravitational Waves
• Propagation and emission of gravitational waves in the weak-field limit within the Palatini formalism