Novel Ringdown Tests of General Relativity with Black Hole Graybody Factors
gr-qc, astro-ph.HE, hep-ph
Submitted: 2026-04-13
Updated: 2026-10-12
Terminology
Sources
- Black hole spectroscopy: from theory to experiment
- Quasi-Normal Modes of Stars and Black Holes
- Quasinormal modes of black holes and black branes
- Black Hole Spectroscopy: Testing General Relativity through Gravitational Wave Observations
- On gravitational-wave spectroscopy of massive black holes with the space interferometer LISA
- Bayesian model selection for testing the no-hair theorem with black hole ringdowns
- Testing General Relativity with Present and Future Astrophysical Observations
- Extreme Gravity Tests with Gravitational Waves from Compact Binary Coalescences: (II) Ringdown
- Testing General Relativity with Black Hole Quasi-Normal Modes
- GWTC-4.0: Tests of General Relativity. I. Overview and General Tests
- GWTC-4.0: Tests of General Relativity. III. Tests of the Remnants
- Testing the nature of dark compact objects: a status report
- How does a dark compact object ringdown?
- Testing the nature of dark compact objects with gravitational waves
- Probing the horizon of black holes with gravitational waves
- Can environmental effects spoil precision gravitational-wave astrophysics?
- Black holes in galaxies: environmental impact on gravitational-wave generation and propagation
- GW250114: testing Hawking's area law and the Kerr nature of black holes
- Black Hole Spectroscopy and Tests of General Relativity with GW250114
- Accuracy of ringdown models calibrated to numerical relativity simulations
Related papers
- Listening to the Horizon: Probing Near-Horizon Reflectivity with GW250114
- A Pairwise Surrogate for Gravitational-Wave Spectra from Highly Relativistic Vacuum Bubble Collisions
- Tests of General Relativity with Einstein Telescope
- A weakly modelled view of the joint compact-binary mass plane: population structure and spectral-siren cosmology
- Unitary quantum matter-bounce in a universe with a positive cosmological constant
- Nonreciprocal black holes with primary hair in beyond Horndeski gravity: Exact solutions and stability