A full waveform model for arbitrarily axis-symmetric black hole mergers
arXiv:2307.00797 · doi:10.1103/PhysRevD.108.083032
Abstract
In this work, we present a non-GR full waveform for general parametrization of axisymmetric black holes by extending our previous PSI model. Our model comprises two main components: an inspiral part obtained by using phenomenological method in frequency-domain and a ringdown part derived from quasinormal modes associated with photon motion. For quantitatively revealing the influence of the deviation from Kerr black holes on the waveforms, we specify our model to the bumpy black holes, which are typical examples of non-GR black holes. The results show that the deviation from the Kerr quadrupole moment could be measured in a high accuracy. The new waveform model can be directly used to test black holes for the LIGO-Virgo-KAGRA observations, the third generation detectors and space-borne interferometers.
14 pages, 17 figures
References in corpus (31)
- First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
- GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
- First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way
- First M87 Event Horizon Telescope Results. II. Array and Instrumentation
- First M87 Event Horizon Telescope Results. III. Data Processing and Calibration
- Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog
- Observation of gravitational waves from two neutron star-black hole coalescences
- Black Hole Shadows, Photon Rings, and Lensing Rings
- Measurement of the Kerr Spin Parameter by Observation of a Compact Object's Shadow
- Relativistic images of Schwarzschild black hole lensing
- A new method for shadow calculations: application to parameterised axisymmetric black holes
- Apparent shape of super-spinning black holes
- Null geodesics and shadow of a rotating black hole in extended Chern-Simons modified gravity
- Shadow of a Kaluza-Klein rotating dilaton black hole
- Effective-one-body waveforms calibrated to numerical relativity simulations: coalescence of non-spinning, equal-mass black holes
- Quasinormal-mode spectrum of Kerr black holes and its geometric interpretation
- 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
- Observable Properties of Orbits in Exact Bumpy Spacetimes
- Effective-one-body waveforms calibrated to numerical relativity simulations: coalescence of non-precessing, spinning, equal-mass black holes
- A ring-like accretion structure in M87 connecting its black hole and jet
- Can the EHT M87 results be used to test general relativity?
- Rotating regular black holes in conformal massive gravity
- Spinning test particles in the spacetime
- Importance of mirror modes in binary black hole ringdown waveform
- Shadows of CPR black holes and tests of the Kerr metric
- Can supermassive black hole shadows test the Kerr metric?
- Universal features of gravitational waves emitted by superkick binary black hole systems
- Qualifying ringdown and shadow of black holes under general parametrized metrics with photon orbits
- Skylight: a new code for general-relativistic ray-tracing and radiative transfer in arbitrary spacetimes
- Gravitational waveform model based on photon motion for spinning black holes