Gravitational waves from extreme-mass-ratio systems in astrophysical environments
arXiv:2210.01133 · doi:10.1103/PhysRevLett.129.241103
Abstract
We establish a generic, fully-relativistic formalism to study gravitational-wave emission by extreme-mass-ratio systems in spherically-symmetric, non-vacuum black-hole spacetimes. The potential applications to astrophysical setups range from black holes accreting baryonic matter to those within axionic clouds and dark matter environments, allowing to assess the impact of the galactic potential, of accretion, gravitational drag and halo feedback on the generation and propagation of gravitational-waves. We apply our methods to a black hole within a halo of matter. We find fluid modes imparted to the gravitational-wave signal (a clear evidence of the black hole fundamental mode instability) and the tantalizing possibility to infer galactic properties from gravitational-wave measurements by sensitive, low-frequency detectors.
v2. Supplemental Material added, minor improvements. Accepted for publication in Physical Review Letters
References in corpus (10)
- Can environmental effects spoil precision gravitational-wave astrophysics?
- New Horizons for Fundamental Physics with LISA
- The mass distribution in the Galactic Centre from interferometric astrometry of multiple stellar orbits
- Towards adiabatic waveforms for inspiral into Kerr black holes: I. A new model of the source for the time domain perturbation equation
- Stability of the fundamental quasinormal mode in time-domain observations against small perturbations
- Gravitational-wave glitches in chaotic extreme-mass-ratio inspirals
- Dynamical friction of black holes in ultralight dark matter
- Testing spacetime symmetry through gravitational waves from extreme-mass-ratio inspirals
- Gravitational-wave glitches: resonant islands and frequency jumps in non-integrable extreme-mass-ratio inspirals
- Pseudospectrum of Reissner-Nordström black holes: quasinormal mode instability and universality
Cited by in corpus (97)
- Agnostic black hole spectroscopy: Quasinormal mode content of numerical relativity waveforms and limits of validity of linear perturbation theory
- Disks, spikes, and clouds: distinguishing environmental effects on BBH gravitational waveforms
- Black holes surrounded by generic dark matter profiles: appearance and gravitational-wave emission
- 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
- Detecting massive scalar fields with Extreme Mass-Ratio Inspirals
- Ringdown stability: greybody factors as stable gravitational-wave observables
- Spectral (in)stability of quasinormal modes and strong cosmic censorship
- Black holes surrounded by generic matter distributions: polar perturbations and energy flux
- Black hole merger simulations in wave dark matter environments
- Priorities in gravitational waveforms for future space-borne detectors: vacuum accuracy or environment?
- Quasinormal modes of black holes embedded in halos of matter
- Hyperboloidal approach for static spherically symmetric spacetimes: a didactical introduction and applications in black-hole physics
- Structural aspects of the anti-de Sitter black hole pseudospectrum
- Analytical models of supermassive black holes in galaxies surrounded by dark matter halos
- Images from disk and spherical accretions of hairy Schwarzschild black holes
- The effect of wave dark matter on equal mass black hole mergers
- Relativistic drag forces on black holes from scalar dark matter clouds of all sizes
- Ringing out General Relativity: Quasi-normal mode frequencies for black holes of any spin in modified gravity
- Ringdown of a dynamical spacetime
- Gravitational waveforms from periodic orbits around a quantum-corrected black hole
- Extreme-mass-ratio inspirals into rotating boson stars: nonintegrability, chaos, and transient resonances
- Pseudospectrum of de Sitter black holes
- The Lunar Gravitational-wave Antenna: Mission Studies and Science Case
- Evolution of binary systems accompanying axion clouds in extreme mass ratio inspirals
- Self-interacting scalar dark matter around binary black holes
- Superradiance of charged black holes embedded in dark matter halos
- Geodesics and gravitational waves in chaotic extreme-mass-ratio inspirals: the curious case of Zipoy-Voorhees black-hole mimickers
- Exploring waveforms with non-GR deviations for extreme mass-ratio inspirals
- Greybody factors, reflectionless scattering modes, and echoes of ultracompact horizonless objects
- Extreme mass ratio inspirals in galaxies with dark matter halos
- Black hole in the Dekel-Zhao dark matter profile
- Motion of spinning particles around black hole in a dark matter halo
- Spectral instability of black holes: relating the frequency domain to the time domain
- Long-lived quasinormal modes, grey-body factors and absorption cross-section of the black hole immersed in the Hernquist galactic halo
- Identification of Gravitational-waves from Extreme Mass Ratio Inspirals
- Gravitational Radiation from hyperbolic encounters in the presence of dark matter
- The shadows of accelerating Kerr-Newman black hole and constraints from M87*
- Probing black holes in a dark matter spike of M87 using quasinormal modes
- Inner radius and energy conditions of dark matter halos surrounding Schwarzschild black holes
- Relativistic aerodynamics of spinning black holes
- Fully Relativistic Treatment of Extreme Mass-Ratio Inspirals in Collisionless Environments
- The minimum measurable eccentricity from gravitational waves of LISA massive black hole binaries
- Extreme mass ratio inspirals in rotating dark matter spikes
- Compact Binary Coalescences in Dense Gaseous Environments Can Pose as ones in Vacuum
- The Axial Gravitational Ringing of a Spherically Symmetric Black Hole Surrounded by Dark Matter Spike
- Black-hole spectroscopy: quasinormal modes, ringdown stability and the pseudospectrum
- Impact of ringdown higher-order modes on black-hole mergers in dense environments: the scalar field case, detectability and parameter biases
- Perturbing the vortex: quasinormal and quasibound spectra of rotating acoustic geometries
- Pseudospectrum of rotating analog black holes
- Testing gravity with Extreme-Mass-Ratio Inspirals
- Extreme mass ratio inspirals in dark matter halos: dynamics and distinguishability of halo models
- Influence of dark matter equation of state on the axial gravitational ringing of supermassive black holes
- Dark Matter Mounds: towards a realistic description of dark matter overdensities around black holes
- Slowly-rotating compact objects: the nonintegrability of Hartle-Thorne particle geodesics
- Piercing of a solitonic boson star by a black hole
- Probing vector gravitational atoms with eccentric intermediate mass-ratio inspirals
- Probing the black holes in a dark matter halo of M87 using gravitational wave echoes
- Perturbations of relativistic dissipative stars
- Detecting the massive vector field with extreme mass-ratio inspirals
- Resonant excitation of eccentricity in spherical extreme-mass-ratio inspirals
- Probing dark matter halo profiles with multi-band observations of gravitational waves
- Complete quasinormal modes of Type-D black holes
- The ringdown of a black hole surrounded by a thin shell of matter
- Extreme mass ratio inspirals around topological stars
- Post-adiabatic waveforms from extreme mass ratio inspirals in the presence of dark matter
- Vortices without inflow: bound spectra in horizonless rotational analogs
- Imprints of extra dimensions in eccentric extreme-mass-ratio inspirals gravitational waveforms
- Cumulative effect of orbital resonances in extreme-mass-ratio inspirals
- Viscous torque in turbulent magnetized AGN accretion disks and its effects on EMRI's gravitational waves
- Toward relativistic inspirals into black holes surrounded by matter
- Effect of generic dark matter halo on transonic accretion onto galactic black holes
- Scalar fields around black hole binaries in LIGO-Virgo-KAGRA
- Gravitational radiation reaction around a static black hole surrounded by a Dehnen type dark matter halo
- Spectral instability of horizonless compact objects within astrophysical environments
- Measurable Parameter Combinations of Environmentally-dephased EMRI Gravitational-Wave Signals
- A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments
- Extreme mass-ratio inspirals and extra dimensions: Insights from modified Teukolsky framework
- Lensing by black holes within astrophysical environments
- Overdamped quasibound states inside a Schwarzschild black hole
- Distinguishing dark matter halos with Extreme mass ratio inspirals
- Taxonomy of periodic orbits and gravitational waves in a non-rotating Destounis-Suvorov-Kokkotas black hole spacetime
- Constraints on the Scale Parameter of Regular Black Hole in Asymptotically Safe Gravity from Extreme Mass Ratio Inspirals
- Galactic microlensing by acoustic Schwarzschild black holes
- A supplementary radiation-reaction force between two binaries
- Exploring black holes with multiple photon spheres by interferometric signatures
- Geometric properties of slowly rotating black holes embedded in matter environments
- Generalized Perturbed Kepler Problem: Gravitational Wave Imprints from Eccentric Compact Binaries
- Excitation factors for horizonless compact objects: long-lived modes, echoes, and greybody factors
- Extreme mass ratio inspirals into black holes surrounded by matter: Resonance crossings
- Preliminary forecasting constraint on scalar charge with LISA in non-vacuum environments
- Gravitational memory meets astrophysical environments: exploring a new frontier through osculations
- Generic effective sources for first-order in mass-ratio gravitational self-force calculations in Schwarzschild spacetime
- Parity violating spectral dynamics of black holes in dynamical Chern-Simons gravity