Bekenstein--Hod Bound: A 3.3 sigma Confirmation from GW250114
gr-qc, astro-ph.HE
Submitted: 2026-08-31
Updated: 2026-08-31
Comments: 9 pages, 2 figures, 1 table
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Universal Bound on Dynamical Relaxation Times and Black-Hole Quasinormal Ringing
- Quasinormal resonances of near-extremal Kerr-Newman black holes
- Black-hole quasinormal resonances: Wave analysis versus a geometric-optics approximation
- The Reissner-Nordstr\"om black hole with the fastest relaxation rate
- Universal Bound on Dynamical Relaxation Time from Condition for Relaxing Quantity to be Classical
- Near-Extreme Black Holes and the Universal Relaxation Bound
- Quasinormal modes of nearly extremal Kerr spacetimes: spectrum bifurcation and power-law ringdown
- Quasi-Normal Modes of Stars and Black Holes
- Quasinormal modes of black holes and black branes
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Properties of the Binary Black Hole Merger GW150914
- Tests of general relativity with GW150914
- Empirical tests of the black hole no-hair conjecture using gravitational-wave observations
- Observational Black Hole Spectroscopy: A time-domain multimode analysis of GW150914
- Testing the no-hair theorem with GW150914
- Black hole ringdown: the importance of overtones
- Ringdown overtones, black hole spectroscopy, and no-hair theorem tests
- Spectroscopy of binary black hole ringdown using overtones and angular modes
- Revisiting non-linearity in binary black hole mergers
- Effect of Noise Estimation in Time-Domain Ringdown Analysis: A Case Study with GW150914
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