Gravitational waveform model based on photon motion for spinning black holes
arXiv:2204.09367 · doi:10.1103/PhysRevD.106.104013
Abstract
The waveforms from binary black hole mergers include inspiral, merger, and ringdown parts. Usually, the inspiral waveform can be obtained by calibrating from post-Newtonian approximation; The merger and ringdown ones can be gotten from the quasinormal modes with black hole perturbation theory. However, for more general black holes, the calculation of the quasinormal modes is not trivial. In this paper we use the photon sphere to get the quasinormal modes of spinning black holes. Then we connect the ringdown wave with the inspiral part to get full waveforms and compare with the ones from numerical relativity. We find that they match with each other very well. In principle this method can be extended to some general compact objects. As an example, the ringdown waveforms from parametrized axisymmetric black holes are obtained. We also use this method to get the ringdown signals of the accelerating final black hole; this is due to gravitational recoil during the merger. Even for the extreme cases, the acceleration due to the recoil cannot produce detectable effects.
arXiv comment14 pages, 12 figures
References in corpus (72)
- Quasinormal modes of black holes and black branes
- Quasi-Normal Modes of Stars and Black Holes
- Quasinormal modes of black holes: from astrophysics to string theory
- First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole
- First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring
- Effective one-body approach to general relativistic two-body dynamics
- Frequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era
- Geodesic stability, Lyapunov exponents and quasinormal modes
- Transition from inspiral to plunge in binary black hole coalescences
- Frequency-domain gravitational waves from non-precessing black-hole binaries. I. New numerical waveforms and anatomy of the signal
- A simple model of complete precessing black-hole-binary gravitational waveforms
- First M87 Event Horizon Telescope Results. VIII. Magnetic Field Structure near The Event Horizon
- Detection, Measurement and Gravitational Radiation
- Matching post-Newtonian and numerical relativity waveforms: systematic errors and a new phenomenological model for non-precessing black hole binaries
- Testing the rotational nature of the supermassive object M87* from the circularity and size of its first image
- The SXS Collaboration catalog of binary black hole simulations
- A template bank for gravitational waveforms from coalescing binary black holes: non-spinning binaries
- A master equation for gravitational perturbations of maximally symmetric black holes in higher dimensions
- Inspiral, merger and ringdown of unequal mass black hole binaries: a multipolar analysis
- A catalog of 174 binary black-hole simulations for gravitational-wave astronomy
- Shadow of rotating regular black holes
- Light ring stability in ultra-compact objects
- Quasi-Normal Modes of Schwarzschild Anti-De Sitter Black Holes: Electromagnetic and Gravitational Perturbations
- Phenomenological template family for black-hole coalescence waveforms
- Toward faithful templates for non-spinning binary black holes using the effective-one-body approach
- General parametrization of axisymmetric black holes in metric theories of gravity
- Black hole ringdown: the importance of overtones
- Effective-one-body waveforms calibrated to numerical relativity simulations: coalescence of non-spinning, equal-mass black holes
- An improved analytical description of inspiralling and coalescing black-hole binaries
- Quasinormal-mode spectrum of Kerr black holes and its geometric interpretation
- An improved effective-one-body Hamiltonian for spinning black-hole binaries
- How black holes get their kicks: Gravitational radiation recoil revisited
- A Fast New Public Code for Computing Photon Orbits in a Kerr Spacetime
- Effective one body approach to the dynamics of two spinning black holes with next-to-leading order spin-orbit coupling
- A waveform model for eccentric binary black hole based on effective-one-body-numerical-relativity (EOBNR) formalism
- Frequency domain reduced order model of aligned-spin effective-one-body waveforms with generic mass-ratios and spins
- A data-analysis driven comparison of analytic and numerical coalescing binary waveforms: nonspinning case
- Accurate Effective-One-Body waveforms of inspiralling and coalescing black-hole binaries
- Detection template families for gravitational waves from the final stages of binary--black-hole inspirals: Nonspinning case
- Effective-one-body waveforms calibrated to numerical relativity simulations: coalescence of non-precessing, spinning, equal-mass black holes
- Faithful Effective-One-Body waveforms of equal-mass coalescing black-hole binaries
- Quasinormal modes of Schwarzschild black holes in four and higher dimensions
- Accurate and efficient waveforms for compact binaries on eccentric orbits
- Quasinormal modes of Kerr-Newman black holes: coupling of electromagnetic and gravitational perturbations
- Challenging the paradigm of singularity excision in gravitational collapse
- Gravitational perturbations of the Kerr geometry: High-accuracy study
- Highly damped quasinormal modes of Kerr black holes
- Light Curves from an MHD Simulation of a Black Hole Accretion Disk
- qnm: A Python package for calculating Kerr quasinormal modes, separation constants, and spherical-spheroidal mixing coefficients
- Modeling Extreme Mass Ratio Inspirals within the Effective-One-Body Approach
- Quasi-normal modes of toroidal, cylindrical and planar black holes in anti-de Sitter spacetimes: scalar, electromagnetic and gravitational perturbations
- Rotating regular black holes in conformal massive gravity
- Black Hole Shadow in Symmergent Gravity
- Overtones or higher harmonics? Prospects for testing the no-hair theorem with gravitational wave detections
- Radiation Transfer of Emission Lines in Curved Space-Time
- Importance of mirror modes in binary black hole ringdown waveform
- Black-hole microstate spectroscopy: ringdown, quasinormal modes, and echoes
- Black hole kicks as new gravitational wave observables
- A Proposed Search for the Detection of Gravitational Waves from Eccentric Binary Black Holes
- Shadows of the accelerating black holes
- Analytical Black-Hole Binary Merger Waveforms
- A surrogate model for gravitational waveforms of spin-aligned binary black holes with eccentricities
- Phase shift of gravitational waves induced by aberration
- Dirac Quasinormal frequencies of the Kerr-Newman black hole
- SHORTCUT METHOD OF SOLUTION OF GEODESIC EQUATIONS FOR SCHWARZSCHILD BLACK HOLE
- Testing general relativity using binary extreme-mass-ratio inspirals
- A comparative study of Dirac quasinormal modes of charged black holes in higher dimensions
- Universal features of gravitational waves emitted by superkick binary black hole systems
- Gravitational wave emission under general parametrized metric from extreme mass ratio inspirals
- Scattering and absorption of a scalar field impinging on a charged black hole in the Einstein-Maxwell-dilaton theory
- Qualifying ringdown and shadow of black holes under general parametrized metrics with photon orbits
- Gravitational-wave bursts from spin-precessing black holes in binary systems