Constraining modified gravity with ringdown signals: an explicit example
arXiv:1905.11674 · doi:10.1103/PhysRevD.100.084024
Abstract
An explicit example is found showing how a modified theory of gravity can be constrained with the ringdown signals from merger of binary black holes. This has been made possible by the fact that the modified gravitational theory considered in this work has an exact rotating black hole solution and that the corresponding quasi-normal modes can be calculated. With these, we obtain the possible constraint that can be placed on the parameter describing the deviation of this particular alternative theory from general relativity by using the detection of the ringdown signals from binary black holes's merger with future space-based gravitational wave detectors.
7 pages, 4 figures, 4 tables, matches the published version
References in corpus (43)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Modified Gravity and Cosmology
- Quasinormal modes of black holes and black branes
- TianQin: a space-borne gravitational wave detector
- The Confrontation between General Relativity and Experiment
- Quasinormal modes of black holes: from astrophysics to string theory
- Testing General Relativity with Present and Future Astrophysical Observations
- Laser Interferometer Space Antenna
- Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
- Massive Black Holes as Population III Remnants
- On gravitational-wave spectroscopy of massive black holes with the space interferometer LISA
- Formation of Supermassive Black Holes by Direct Collapse in Pregalactic Halos
- Formation of the First Supermassive Black Holes
- The construction and use of LISA sensitivity curves
- Can environmental effects spoil precision gravitational-wave astrophysics?
- Scalar-Tensor-Vector Gravity Theory
- Science with the space-based interferometer eLISA. I: Supermassive black hole binaries
- Supermassive black hole formation during the assembly of pre-galactic discs
- Black Hole Spectroscopy: Testing General Relativity through Gravitational Wave Observations
- Extreme Gravity Tests with Gravitational Waves from Compact Binary Coalescences: (II) Ringdown
- Towards a generic test of the strong field dynamics of general relativity using compact binary coalescence
- Black Holes in Modified Gravity (MOG)
- Perturbed black holes in Einstein-dilaton-Gauss-Bonnet gravity: Stability, ringdown, and gravitational-wave emission
- Gravitational signature of Schwarzschild black holes in dynamical Chern-Simons gravity
- Bayesian model selection for testing the no-hair theorem with black hole ringdowns
- Black-hole hair loss: learning about binary progenitors from ringdown signals
- Testing the no-hair theorem with black hole ringdowns using TIGER
- Black-hole Spectroscopy by Making Full Use of Gravitational-Wave Modeling
- Quasinormal modes of Einstein-Gauss-Bonnet-dilaton black holes
- Science with the TianQin observatory: Preliminary results on massive black hole binaries
- Quasinormal modes of Kerr-Newman black holes: coupling of electromagnetic and gravitational perturbations
- Fundamentals of the orbit and response for TianQin
- Perturbations of Schwarzschild black holes in Dynamical Chern-Simons modified gravity
- Gravito-Electromagnetic Perturbations of Kerr-Newman Black Holes: Stability and Isospectrality in the Slow-Rotation Limit
- Empirical tests of the black hole no-hair conjecture using gravitational-wave observations
- Linear mode stability of Kerr-Newman and its quasinormal modes
- Scalar, Electromagnetic and Gravitational Perturbations of Kerr-Newman Black Holes in the Slow-Rotation Limit
- Science with the TianQin observatory: Preliminary results on testing the no-hair theorem with ringdown signals
- Quasi-normal modes of black holes in Horndeski gravity
- Preliminary study on parameter estimation accuracy of supermassive black hole binary inspirals for TianQin
- The Quasinormal Modes of Weakly Charged Kerr-Newman Spacetimes
- Music from the heavens - Gravitational waves from supermassive black hole mergers in the EAGLE simulations
- Quasinormal Modes of Modified Gravity (MOG) Black Holes
Cited by in corpus (29)
- The TianQin project: current progress on science and technology
- Concepts and status of Chinese space gravitational wave detection projects
- The First Round Result from the TianQin-1 Satellite
- Science with the TianQin Observatory: Preliminary results on Galactic double white dwarf binaries
- Science with the TianQin observatory: Preliminary result on extreme-mass-ratio inspirals
- The masses and shadows of the black holes Sagittarius A* and M87* in modified gravity (MOG)
- Science with the TianQin Observatory: Preliminary Results on Testing the No-hair Theorem with EMRI
- The formation of neutron star systems through accretion-induced collapse in white-dwarf binaries
- Eclipse avoidance in TianQin orbit selection
- Constraining the cosmological parameters using gravitational wave observations of massive black hole binaries and statistical redshift information
- Eikonal black hole ringings in generalized energy-momentum squared gravity
- Eikonal quasinormal modes of black holes beyond general relativity III: scalar Gauss-Bonnet gravity
- Ultra-compact X-ray binaries with He star companions
- Analytic Kludge Waveforms for Extreme Mass Ratio Inspirals of Charged Object around Kerr-Newman Black Hole
- Detecting the gravitational wave memory effect with TianQin
- Testing general relativity with TianQin: the prospect of using the inspiral signals of black hole binaries
- Analyses of Laser Propagation Noises for TianQin Gravitational Wave Observatory Based on the Global Magnetosphere MHD Simulations
- Detecting the stochastic gravitational wave background with the TianQin detector
- Orbital effects on time delay interferometry for TianQin
- Detecting Strong Gravitational Lensing of Gravitational Waves with TianQin
- High-dimensional Schwarzschild black holes in scalar-tensor-vector gravity theory
- Quasinormal Modes of the Generalized Ayón-Beato-Garc\'ıa Scalar-Tensor-Vector Gravity Black Hole in the Scalar-Tensor-Vector Gravity
- Measuring the Hubble Constant Using Strongly Lensed Gravitational Wave Signals
- Identifying modified theories of gravity using binary black-hole ringdowns
- Quasinormal-modes of the Kerr-Newman black hole: GW150914 and fundamental physics implications
- Ringdown Spectroscopy of Rotating Black Holes Pierced by Cosmic Strings
- Probing the Spin-Induced Quadrupole Moment of Massive Black Holes with the Inspiral of Binary Black Holes
- Ultra-compact X-ray Binaries: A Review
- Analyses of residual accelerations for TianQin based on the global MHD simulation