Tidal resonance in extreme mass-ratio inspirals

Abstract

We describe a new class of resonances for extreme mass-ratio inspirals (EMRIs): tidal resonances, induced by the tidal field of nearby stars or stellar-mass black holes. A tidal resonance can be viewed as a general relativistic extension of the Kozai-Lidov resonances in Newtonian systems, and is distinct from the transient resonance already known for EMRI systems. Tidal resonances will generically occur for EMRIs. By probing their influence on the phase of an EMRI waveform, we can learn about the tidal environmental of the EMRI system, albeit at the cost of a more complicated waveform model. Observations by LISA of EMRI systems therefore have the potential to provide information about the distribution of stellar-mass objects near their host galactic-center black holes.

arXiv comment5 pages; v2: matches version published in PRL

References in corpus (23)

• The Eccentric Kozai-Lidov Effect and Its Applications
• The motion of point particles in curved spacetime
• Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals
• Rates of Stellar Tidal Disruption as Probes of the Supermassive Black Hole Mass Function
• Model Waveform Accuracy Standards for Gravitational Wave Data Analysis
• Two timescale analysis of extreme mass ratio inspirals in Kerr. I. Orbital Motion
• Gravitational wave snapshots of generic extreme mass ratio inspirals
• A Cluster of Black Holes at the Galactic Center
• Constructing Gravitational Waves from Generic Spin-Precessing Compact Binary Inspirals
• Absorption of mass and angular momentum by a black hole: Time-domain formalisms for gravitational perturbations, and the small-hole/slow-motion approximation
• Transient resonances in the inspirals of point particles into black holes
• Prospects for observing extreme-mass-ratio inspirals with LISA
• Tidal deformation of a slowly rotating black hole
• The impact of realistic models of mass segregation on the event rate of extreme-mass ratio inspirals and cusp re-growth
• Black-hole-regulated star formation in massive galaxies
• Adiabatic radiation reaction to the orbits in Kerr Spacetime
• Importance of transient resonances in extreme-mass-ratio inspirals
• Metric of a tidally perturbed spinning black hole
• A census of transient orbital resonances encountered during binary inspiral
• Orbital resonances around Black holes
• General Relativistic Dynamics of an Extreme Mass-Ratio Binary interacting with an External Body
• The butterfly effect in the extreme-mass ratio inspiral problem
• Resonant recoil in extreme mass ratio binary black hole mergers

Cited by in corpus (69)

• Prospects for Fundamental Physics with LISA
• Gravitational waves from extreme-mass-ratio systems in astrophysical environments
• Rapid generation of fully relativistic extreme-mass-ratio-inspiral waveform templates for LISA data analysis
• Detecting fundamental fields with LISA observations of gravitational waves from extreme mass-ratio inspirals
• Adiabatic waveforms for extreme mass-ratio inspirals via multivoice decomposition in time and frequency
• Formation Rate of Extreme Mass Ratio Inspirals in Active Galactic Nuclei
• Wet Extreme Mass Ratio Inspirals May Be More Common For Spaceborne Gravitational Wave Detection
• Dynamic Signatures of Black Hole Binaries with Superradiant Clouds
• Black hole perturbation theory and gravitational self-force
• Probing vector hair of black holes with extreme mass ratio inspirals
• Adiabatic waveforms from extreme-mass-ratio inspirals: an analytical approach
• Probing astrophysical environment with eccentric extreme mass-ratio inspirals
• Extreme mass-ratio inspirals around a spinning horizonless compact object
• Growth of resonances and chaos for a spinning test particle in the Schwarzschild background
• Analytic solutions for parallel transport along generic bound geodesics in Kerr spacetime
• Assessing the impact of transient orbital resonances
• Probing the Nature of Black Holes: Deep in the mHz Gravitational-Wave Sky
• Relating Black Hole Shadow to Quasinormal Modes for Rotating Black Holes
• Supercritical accretion of stellar-mass compact objects in active galactic nuclei
• Gravitational tuning forks and hierarchical triple systems
• 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
• Ready-to-use analytic model for gravitational waves from a hierarchical triple with Kozai-Lidov oscillations
• Gravitational wave from extreme mass-ratio inspirals as a probe of extra dimensions
• Resonant self-force effects in extreme-mass-ratio binaries: A scalar model
• Tidal deformations of a binary system induced by an external Kerr black hole
• Prospects of detecting deviations to Kerr geometry with radiation reaction effects in EMRIs
• Precession resonances in hierarchical triple systems
• Extreme mass ratio inspirals into black holes surrounded by matter
• Relativistic Mean Motion Resonance
• Effective two-body approach to the hierarchical three-body problem
• Evolution of diffuse scalar clouds around binary black holes
• Fast inspirals and the treatment of orbital resonances
• Highly eccentric EMRI waveforms via fast self-forced inspirals
• Superradiant clouds may be relevant for close compact object binaries
• Particle motion under the conservative piece of the self-force is Hamiltonian
• Testing gravity with Extreme-Mass-Ratio Inspirals
• Synchronizing the EMRIs and IMRIs in AGN accretion disks
• Tidal forces in parametrized spacetime: Rezzolla-Zhidenko parametrization
• Extreme mass ratio inspirals in dark matter halos: dynamics and distinguishability of halo models
• Testing General Relativity with Gravitational Waves
• The fate of observers in circular motion
• Strong-gravity precession resonances for binary systems orbiting a Schwarzschild black hole
• Detecting the massive vector field with extreme mass-ratio inspirals
• Secondary spins of extreme mass ratio inspirals: A probe to the formation channels
• General Relativistic Effects on Hill Stability of Multi-Body Systems I: Stability of Three-Body Systems Containing a Massive Black Hole
• Fundamental Physics and Cosmology with TianQin
• Resonant excitation of eccentricity in spherical extreme-mass-ratio inspirals
• Dynamical perturbations around an extreme mass ratio inspiral near resonance
• Astrophysics with the Laser Interferometer Space Antenna
• Resonant jumps induced by stationary tidal perturbation: a two-for-one deal
• Cumulative effect of orbital resonances in extreme-mass-ratio inspirals
• Tidally-induced nonlinear resonances in EMRIs with an analogue model
• Vacuum Spacetime With Multipole Moments: The Minimal Size Conjecture, Black Hole Shadow, and Gravitational Wave Observables
• Black-Hole Perturbation Plus Post-Newtonian Theory: Hybrid Waveform for Neutron Star Binaries
• Toward relativistic inspirals into black holes surrounded by matter
• Science Potential for Stellar-mass Black Holes as Neighbors of Sgr A*
• Resonant interactions from dynamical perturbers on generic orbits around an extreme mass ratio inspiral
• Probing light scalars with not quite black holes
• A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments
• Observable signature of magnetic tidal coupling in hierarchical triple systems
• A supplementary radiation-reaction force between two binaries
• The Effect of Mission Duration on LISA Science Objectives
• Precisely computing bound orbits of spinning bodies around black holes I: General framework and results for nearly equatorial orbits
• Precisely computing bound orbits of spinning bodies around black holes II: Generic orbits
• Extreme mass-ratio inspirals as probes of scalar fields: eccentric equatorial orbits around Kerr black holes
• Tidal perturbations of an extreme mass ratio inspiral around a Kerr black hole
• Adiabatic evolution due to the conservative scalar self-force during orbital resonances