Testing gravity with Extreme-Mass-Ratio Inspirals
arXiv:2401.08085 · doi:10.1007/978-981-97-2871-8_8
Abstract
Extreme-mass-ratio inspirals consist of binary systems of compact objects, with orders of magnitude differences in their masses, in the regime where the dynamics are driven by gravitational wave emission. The unique nature of extreme-mass-ratio inspirals facilitates the exploration of diverse and stimulating tests related to various aspects of black holes and General Relativity. These tests encompass investigations into the spacetime geometry, the dissipation of the binary system energy and angular momentum, and the impact of the intrinsic non-linear effects of the gravitational interaction. This review accounts for the manifold opportunities for testing General Relativity, ranging from examinations of black hole properties to cosmological and multimessenger tests.
arXiv commentV2. Updated to match published version. V1: 67+19 pages, 2 figures. Review Chapter for the book "Recent Progress on Gravity Tests" (Eds. C. Bambi and A. Cárdenas-Avendaño, Springer Singapore)
References in corpus (299)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- A Large Mass Hierarchy from a Small Extra Dimension
- An Alternative to Compactification
- The Confrontation between General Relativity and Experiment
- GW170817: Measurements of Neutron Star Radii and Equation of State
- TianQin: a space-borne gravitational wave detector
- Tests of general relativity with GW150914
- Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?
- Evolution of Binary Black Hole Spacetimes
- Testing General Relativity with Present and Future Astrophysical Observations
- Accurate Evolutions of Orbiting Black-Hole Binaries Without Excision
- Gravity, Lorentz Violation, and the Standard Model
- Tidal Love numbers of neutron stars
- Effective one-body approach to general relativistic two-body dynamics
- Gravitational wave extraction from an inspiraling configuration of merging black holes
- Constraining neutron star tidal Love numbers with gravitational wave detectors
- Primordial Black Holes as Dark Matter
- Testing the nature of dark compact objects: a status report
- Brane-World Gravity
- Relativistic tidal properties of neutron stars
- Transition from inspiral to plunge in binary black hole coalescences
- Strong constraints on cosmological gravity from GW170817 and GRB 170817A
- Is the gravitational-wave ringdown a probe of the event horizon?
- First observation of PeV-energy neutrinos with IceCube
- Kerr black holes with scalar hair
- Chern-Simons Modification of General Relativity
- Relativistic theory of tidal Love numbers
- Black holes, gravitational waves and fundamental physics: a roadmap
- The motion of point particles in curved spacetime
- Chern-Simons Modified General Relativity
- Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals
- Theoretical Physics Implications of the Binary Black-Hole Mergers GW150914 and GW151226
- LISA Capture Sources: Approximate Waveforms, Signal-to-Noise Ratios, and Parameter Estimation Accuracy
- Use and Abuse of the Fisher Information Matrix in the Assessment of Gravitational-Wave Parameter-Estimation Prospects
- Inspiral-merger-ringdown waveforms for black-hole binaries with non-precessing spins
- Can environmental effects spoil precision gravitational-wave astrophysics?
- Intermediate and Extreme Mass-Ratio Inspirals -- Astrophysics, Science Applications and Detection using LISA
- Taiji Program: Gravitational-Wave Sources
- Black holes on the brane
- Echoes of ECOs: gravitational-wave signatures of exotic compact objects and of quantum corrections at the horizon scale
- Gravitational Radiation Reaction to a Particle Motion
- Black hole hair in generalized scalar-tensor gravity
- An axiomatic approach to electromagnetic and gravitational radiation reaction of particles in curved spacetime
- Bounding the mass of the graviton using gravitional-wave observations of inspiralling compact binaries
- Intermediate-Mass Black Holes
- The promise of multi-band gravitational wave astronomy
- Self-force and radiation reaction in general relativity
- Numerical Relativity Using a Generalized Harmonic Decomposition
- Echoes from the Abyss: Tentative evidence for Planck-scale structure at black hole horizons
- Prospects for Fundamental Physics with LISA
- The observational evidence for horizons: from echoes to precision gravitational-wave physics
- The TianQin project: current progress on science and technology
- Tests for the existence of horizons through gravitational wave echoes
- Self-force via a Green's function decomposition
- AEDGE: Atomic Experiment for Dark Matter and Gravity Exploration in Space
- Cosmology with the Laser Interferometer Space Antenna
- Dynamical Chern-Simons Modified Gravity I: Spinning Black Holes in the Slow-Rotation Approximation
- Perturbative Approach to an orbital evolution around a Supermassive black hole
- Starbursts near supermassive black holes: young stars in the Galactic Center, and gravitational waves in LISA band
- AION: An Atom Interferometer Observatory and Network
- Concepts and status of Chinese space gravitational wave detection projects
- Gravitational self force in extreme mass-ratio inspirals
- New Horizons for Fundamental Physics with LISA
- Testing General Relativity with Low-Frequency, Space-Based Gravitational-Wave Detectors
- Two timescale analysis of extreme mass ratio inspirals in Kerr. I. Orbital Motion
- Testing strong-field gravity with tidal Love numbers
- Short GRB and binary black hole standard sirens as a probe of dark energy
- Event rate estimates for LISA extreme mass ratio capture sources
- Observational evidence for intermediate-mass black holes
- "Kludge" gravitational waveforms for a test-body orbiting a Kerr black hole
- Using LISA EMRI sources to test off-Kerr deviations in the geometry of massive black holes
- Gravitational wave snapshots of generic extreme mass ratio inspirals
- Neutron star tidal deformability and equation of state constraints
- Black-hole binaries, gravitational waves, and numerical relativity
- MOCCA Code for Star Cluster Simulations - IV. A new Scenario for Intermediate Mass Black Hole Formation in Globular Clusters
- Black holes in galaxies: environmental impact on gravitational-wave generation and propagation
- Precision of Hubble constant derived using black hole binary absolute distances and statistical redshift information
- Evolution of circular, non-equatorial orbits of Kerr black holes due to gravitational-wave emission: II. Inspiral trajectories and gravitational waveforms
- Constraining Lorentz-violating, Modified Dispersion Relations with Gravitational Waves
- Relativistic Dynamics and Extreme Mass Ratio Inspirals
- Slowly Rotating Black Holes in Dynamical Chern-Simons Gravity: Deformation Quadratic in the Spin
- Into the lair: gravitational-wave signatures of dark matter
- FastEMRIWaveforms: New tools for millihertz gravitational-wave data analysis
- LISA detections of massive black hole inspirals: parameter extraction errors due to inaccurate template waveforms
- Mode sum regularization approach for the self-force in black hole spacetime
- Theory-Agnostic Constraints on Black-Hole Dipole Radiation with Multi-Band Gravitational-Wave Astrophysics
- Towards a formalism for mapping the spacetimes of massive compact objects: Bumpy black holes and their orbits
- Phenomenological aspects of black holes beyond general relativity
- The Transition from Inspiral to Plunge for a Compact Body in a Circular Equatorial Orbit Around a Massive, Spinning Black Hole
- Gravitational waves from extreme-mass-ratio systems in astrophysical environments
- Gravitational self-force on a particle in eccentric orbit around a Schwarzschild black hole
- Calculating the gravitational self force in Schwarzschild spacetime
- Floating and sinking: the imprint of massive scalars around rotating black holes
- Bumpy Black Holes in Alternate Theories of Gravity
- A brief review on primordial black holes as dark matter
- Imprint of Accretion Disk-Induced Migration on Gravitational Waves from Extreme Mass Ratio Inspirals
- Fundamental physics implications on higher-curvature theories from the binary black hole signals in the LIGO-Virgo Catalog GWTC-1
- Observable Properties of Orbits in Exact Bumpy Spacetimes
- Multipole Moments of Isolated Horizons
- Black Holes and Scalar Fields
- Gravitational Waves from Quasicircular Extreme Mass-Ratio Inspirals as Probes of Scalar-Tensor Theories
- Science with the TianQin Observatory: Preliminary results on Galactic double white dwarf binaries
- Rapid generation of fully relativistic extreme-mass-ratio-inspiral waveform templates for LISA data analysis
- Gravitational waveforms for compact binaries from second-order self-force theory
- Second-order self-force calculation of the gravitational binding energy in compact binaries
- The Fast and the Fiducial: Augmented kludge waveforms for detecting extreme-mass-ratio inspirals
- Gravitational radiation reaction and inspiral waveforms in the adiabatic limit
- A Rigorous Derivation of Electromagnetic Self-force
- Detecting fundamental fields with LISA observations of gravitational waves from extreme mass-ratio inspirals
- Evolution of inspiral orbits around a Schwarzschild black hole
- Prototype Global Analysis of LISA Data with Multiple Source Types
- Rotating black hole orbit functionals in the frequency domain
- Adiabatic waveforms for extreme mass-ratio inspirals via multivoice decomposition in time and frequency
- Astrophysical and theoretical physics implications from multimessenger neutron star observations
- Binary Encounters With Supermassive Black Holes: Zero-Eccentricity LISA Events
- Improved approximate inspirals of test-bodies into Kerr black holes
- Formation Rate of Extreme Mass Ratio Inspirals in Active Galactic Nuclei
- Spacetime and orbits of bumpy 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
- Minimal conditions for the existence of a Hawking-like flux
- Gravitational self-force on generic bound geodesics in Kerr spacetime
- Osculating orbits in Schwarzschild spacetime, with an application to extreme mass-ratio inspirals
- ELGAR -- a European Laboratory for Gravitation and Atom-interferometric Research
- The influence of the hydrodynamic drag from an accretion torus on extreme mass-ratio inspirals
- Quasi-periodic eruptions from impacts between the secondary and a rigidly precessing accretion disc in an extreme mass-ratio inspiral system
- Two-timescale evolution of extreme-mass-ratio inspirals: waveform generation scheme for quasicircular orbits in Schwarzschild spacetime
- Orbital Evolution of Extreme-Mass-Ratio Black-Hole Binaries with Numerical Relativity
- How to observe a non-Kerr spacetime
- Transition from Regular to Chaotic Circulation in Magnetized Coronae near Compact Objects
- Disks, spikes, and clouds: distinguishing environmental effects on BBH gravitational waveforms
- Probing Fundamental Physics with Gravitational Waves: The Next Generation
- Gravity and large black holes in Randall-Sundrum II braneworlds
- Numerical relativity simulation of GW150914 beyond general relativity
- Detecting scalar fields with Extreme Mass Ratio Inspirals
- Equation of Motion of Small Bodies in Relativity
- Numerical binary black hole collisions in dynamical Chern-Simons gravity
- Prospects for observing extreme-mass-ratio inspirals with LISA
- Towards adiabatic waveforms for inspiral into Kerr black holes: II. Dynamical sources and generic orbits
- Ergoregion instability of exotic compact objects: electromagnetic and gravitational perturbations and the role of absorption
- An observable signature of a background deviating from Kerr
- Self-force of a scalar field for circular orbits about a Schwarzschild black hole
- Tidal resonance in extreme mass-ratio inspirals
- Science with the TianQin observatory: Preliminary result on extreme-mass-ratio inspirals
- Tidal heating as a discriminator for horizons in extreme mass ratio inspirals
- Extreme Mass-Ratio Inspirals in the Effective-One-Body Approach: Quasi-Circular, Equatorial Orbits around a Spinning Black Hole
- Distinguishing fuzzballs from black holes through their multipolar structure
- Testing Chern-Simons Modified Gravity with Gravitational-Wave Detections of Extreme-Mass-Ratio Binaries
- Modeling Extreme Mass Ratio Inspirals within the Effective-One-Body Approach
- Wet Extreme Mass Ratio Inspirals May Be More Common For Spaceborne Gravitational Wave Detection
- Hawking-like radiation does not require a trapped region
- Highly eccentric inspirals into a black hole
- Effective Field Theory of Black Hole Quasinormal Modes in Scalar-Tensor Theories
- Gravitational-Wave Signature of an Inspiral into a Supermassive Horizonless Object
- Gravitational waves from extreme mass-ratio inspirals in Dynamical Chern-Simons gravity
- Perturbations of spinning black holes beyond General Relativity: Modified Teukolsky equation
- Probing vector hair of black holes with extreme mass ratio inspirals
- Echoes from Quantum Black Holes
- Black Hole Astrophysics in AdS Braneworlds
- The adiabatic evolution of orbital parameters in the Kerr spacetime
- Orbital fingerprints of ultralight scalar fields around black holes
- Chaotic motion of Charged Particles in an Electromagnetic Field Surrounding a Rotating Black Hole
- Extreme Dark Matter Tests with Extreme Mass Ratio Inspirals
- Gravitational wave background from extreme mass ratio inspirals
- Research Update on Extreme-Mass-Ratio Inspirals
- Enhancing the SEOBNRv5 effective-one-body waveform model with second-order gravitational self-force fluxes
- Gravitational-wave glitches in chaotic extreme-mass-ratio inspirals
- 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
- Perturbations of Schwarzschild Black Holes in Chern-Simons Modified Gravity
- Gravitational waves from Extreme Mass Ratio Inspirals in non-pure Kerr spacetimes
- Adiabatic waveforms from extreme-mass-ratio inspirals: an analytical approach
- Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries
- Evolution of small-mass-ratio binaries with a spinning secondary
- LISA Sensitivities to Gravitational Waves from Relativistic Metric Theories of Gravity
- Probing astrophysical environment with eccentric extreme mass-ratio inspirals
- Effective one-body model for extreme-mass-ratio spinning binaries on eccentric equatorial orbits: testing radiation reaction and waveform
- Extreme mass-ratio inspirals around a spinning horizonless compact object
- Regularization parameters for the self force in Schwarzschild spacetime: II. gravitational and electromagnetic cases
- Regularization parameters for the self force in Schwarzschild spacetime: I. scalar case
- Radiation-reaction-induced evolution of circular orbits of particles around Kerr Black Holes
- Gravitational wave cosmology with extreme mass-ratio inspirals
- Golden Binary Gravitational-Wave Sources: Robust Probes of Strong-Field Gravity
- Probing the nature of central objects in extreme-mass-ratio inspirals with gravitational waves
- Parameterized and inspiral-merger-ringdown consistency tests of gravity with multi-band gravitational wave observations
- Testing spacetime symmetry through gravitational waves from extreme-mass-ratio inspirals
- Self-Force Calculations with a Spinning Secondary
- Growth of resonances and chaos for a spinning test particle in the Schwarzschild background
- A New Type of Extreme-mass-ratio Inspirals Produced by Tidal Capture of Binary Black Holes
- Limitations of the adiabatic approximation to the gravitational self-force
- Science with the TianQin Observatory: Preliminary Results on Testing the No-hair Theorem with EMRI
- Detecting massive scalar fields with Extreme Mass-Ratio Inspirals
- Improved analytic extreme-mass-ratio inspiral model for scoping out eLISA data analysis
- Gravitational wave sources: reflections and echoes
- X-MRIs: Extremely Large Mass-Ratio Inspirals
- Assessing the detectability of the secondary spin in extreme mass-ratio inspirals with fully-relativistic numerical waveforms
- Motion of small objects in curved spacetimes: An introduction to gravitational self-force
- The role of the supermassive black hole spin in the estimation of the EMRI event rate
- Gravitational self force by mode sum regularization
- NR/HEP: roadmap for the future
- Self-force on a scalar particle in spherically-symmetric spacetime via mode-sum regularization: radial trajectories
- Approximate Waveforms for Extreme-Mass-Ratio Inspirals in Modified Gravity Spacetimes
- The stochastic gravitational-wave background in the absence of horizons
- An algorithm for detection of extreme mass ratio inspirals in LISA data
- Waveform accuracy and systematic uncertainties in current gravitational wave observations
- Testing the Quasar Hubble Diagram with LISA Standard Sirens
- Testing the multipole structure of compact binaries using gravitational wave observations
- Bounding Alternative Theories of Gravity with Multi-Band GW Observations
- Love in Extrema Ratio
- Exploring the small mass ratio binary black hole merger via Zeno's dichotomy approach
- Assessing the impact of transient orbital resonances
- Probing the Nature of Black Holes: Deep in the mHz Gravitational-Wave Sky
- Covariant Self-force Regularization of a Particle Orbiting a Schwarzschild Black Hole - Mode Decomposition Regularization -
- Extreme mass ratio inspirals on the equatorial plane in the adiabatic order
- Gravitational-wave versus X-ray tests of strong-field gravity
- The stars of the galactic center
- Dissipation in extreme-mass ratio binaries with a spinning secondary
- Gravitational-wave glitches: resonant islands and frequency jumps in non-integrable extreme-mass-ratio inspirals
- Faithful effective-one-body waveform of small-mass-ratio coalescing black hole binaries: the eccentric, nonspinning, case
- Comparing second-order gravitational self-force and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries II: the large-mass-ratio case
- Priorities in gravitational waveforms for future space-borne detectors: vacuum accuracy or environment?
- Detecting Gravitational-waves from Extreme Mass Ratio Inspirals using Convolutional Neural Networks
- Multi-band gravitational wave tests of general relativity
- Spinning test body orbiting around a Kerr black hole: Eccentric equatorial orbits and their asymptotic gravitational-wave fluxes
- Self-Force in the Radiation Reaction Formula -- Adiabatic Approximation of a Metric Perturbation and an Orbit --
- A census of transient orbital resonances encountered during binary inspiral
- Accumulating errors in tests of general relativity with gravitational waves: overlapping signals and inaccurate waveforms
- Second-order gravitational self-force in a highly regular gauge
- Adiabatic Evolution of three 'Constants' of Motion for Greatly Inclined Orbits in Kerr spacetime
- Towards a gravitational self force-informed effective-one-body waveform model for nonprecessing, eccentric, large-mass-ratio inspirals
- Classification of shift-symmetric Horndeski theories and hairy black holes
- Intermediate-Mass Black Holes as LISA Sources
- Non-local parameter degeneracy in the intrinsic space of gravitational-wave signals from extreme-mass-ratio inspirals
- "Flux-balance formulae" for extreme mass-ratio inspirals
- A Constrained Metropolis-Hastings Search for EMRIs in the Mock LISA Data Challenge 1B
- Comparing Accretion Disks and Dark Matter Spikes in Intermediate Mass Ratio Inspirals
- Gravitational waves from eccentric extreme mass-ratio inspirals as probes of scalar fields
- Evolution of Retrograde Orbiters in an AGN Disk
- From the self-force problem to the Radiation reaction formula
- Importance of tidal resonances in extreme-mass-ratio inspirals
- Prospects for determining the nature of the secondaries of extreme mass-ratio inspirals using the spin-induced quadrupole deformation
- Modeling transient resonances in extreme-mass-ratio inspirals
- EMRI data analysis with a phenomenological waveform
- New Kludge Scheme for the Construction of Approximate Waveforms for Extreme-Mass-Ratio Inspirals
- The Motion of Small Bodies in Space-time
- Spacetime Encodings I- A Spacetime Reconstruction Problem
- On Detecting Equatorial Symmetry Breaking with LISA
- Detection Strategies for Extreme Mass Ratio Inspirals
- A New Way to Detect Massive Black Holes in Galaxies: The Stellar Remnants of Tidal Disruption
- Gravitational waves from extreme mass ratio inspirals around bumpy black holes
- Can supernova kicks trigger EMRIs in the Galactic Centre?
- Detecting Subsolar-Mass Primordial Black Holes in Extreme Mass-Ratio Inspirals with LISA and Einstein Telescope
- Model independent tests of the Kerr bound with extreme mass ratio inspirals
- Distinguishing black holes from horizonless objects through the excitation of resonances during inspiral
- Extreme Love in the SPA: constraining the tidal deformability of supermassive objects with extreme mass ratio inspirals and semi-analytical, frequency-domain waveforms
- Towards a framework for testing general relativity with extreme-mass-ratio-inspiral observations
- Gravitational wave from extreme mass-ratio inspirals as a probe of extra dimensions
- Tidal deformations of a binary system induced by an external Kerr black hole
- Constraining the braneworld with gravitational wave observations
- Full analytical formulas for frequency response of space-based gravitational wave detectors
- Mass-gap extreme mass ratio inspirals
- Resonant self-force effects in extreme-mass-ratio binaries: A scalar model
- 2 Fast 2 Fiducial: Gaussian processes for the interpolation and marginalization of waveform error in extreme-mass-ratio-inspiral parameter estimation
- Pulsar timing in extreme mass ratio binaries: a general relativistic approach
- Prospects of detecting deviations to Kerr geometry with radiation reaction effects in EMRIs
- Extreme mass-ratio gravitational-wave sources: Mass segregation and post binary tidal-disruption captures
- The exact dynamical Chern Simons metric for a spinning black hole possesses a fourth constant of motion: A Dynamical-Systems-Based Conjecture
- Constraining the spin parameter of near-extremal black holes using LISA
- Equatorial extreme-mass-ratio inspirals in Kerr black holes with scalar hair spacetimes
- Probing Boson Stars with Extreme Mass Ratio Inspirals
- Gravitational wave emission under general parametrized metric from extreme mass ratio inspirals
- Using LISA-like Gravitational Wave Detectors to Search for Primordial Black Holes
- LISA Pathfinder Performance Confirmed in an Open-Loop Configuration: Results from the Free-Fall Actuation Mode
- Inspiralling compact objects with generic deformations
- Detection of scalar fields by Extreme Mass Ratio Inspirals with a Kerr black hole
- Eccentric-orbit extreme-mass-ratio-inspiral radiation II: 1PN correction to leading-logarithm and subleading-logarithm flux sequences and the entire perturbative 4PN flux
- Golden galactic binaries for LISA: mass-transferring white dwarf black hole binaries
- Rapid determination of LISA sensitivity to extreme mass ratio inspirals with machine learning
- The gravitational capture of compact objects by massive black holes
- A bright electromagnetic counterpart to extreme mass ratio inspirals
- Extreme mass ratio inspirals: perspectives for their detection
- Analytical effective-one-body formalism for extreme-mass-ratio inspirals: eccentric orbits
- Gravitational self-force in scalar-tensor gravity
- Chaos in Quadratic Gravity
- Non-linear effects in EMRI dynamics and their imprints on gravitational waves
- A Newtonian analogue of Kerr black hole
- Action-Angle formalism for extreme mass ratio inspirals in Kerr spacetime
- A one-stop function for gravitational-wave detection, identification and inference
- Tracing the geometry around a massive, axisymmetric body to measure, through gravitational waves, its mass moments and electromagnetic moments
- Geodesic structure and quasinormal modes of a tidally perturbed spacetime
- Influence of mass-ratio corrections in extreme-mass-ratio inspirals for testing general relativity
- Geometrized effective-one-body formalism for extreme-mass-ratio limits: Generic orbits
- Mimicking Kerr's multipole moments
- Motion of localized sources in general relativity: gravitational self-force from quasilocal conservation laws
- Extreme Mass Ratio Inspirals with Scalar Hair
- Intermediate-mass ratio inspirals in merging elliptical galaxies
- Approximate Waveforms for Extreme-Mass-Ratio Inspirals: The Chimera Scheme
- Testing dispersion of gravitational waves from eccentric extreme-mass-ratio inspirals
- Stealth Chaos due to Frame Dragging
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