Quasinormal modes of loop quantum black holes near the Planck scale
arXiv:2309.00722 · doi:10.1103/PhysRevD.109.044044
Abstract
We compare four loop quantum gravity inspired black hole metrics near the Planck scale. Spin 0, 1/2, 1, and 2 field perturbations on these backgrounds are studied. The axial gravitational quasinormal modes are calculated and compared. The time evolution of the ringdown is examined. We also calculate the quasinormal modes in the eikonal limit and compare with the predictions from circular null geodesics.
addressed comments
References in corpus (14)
- First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
- First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way
- Higher order WKB formula for quasinormal modes and grey-body factors: recipes for quick and accurate calculations
- Open data from the third observing run of LIGO, Virgo, KAGRA and GEO
- Are eikonal quasinormal modes linked to the unstable circular null geodesics?
- Quantum Oppenheimer-Snyder and Swiss Cheese models
- Self-dual Black Holes in LQG: Theory and Phenomenology
- Constraints on the rotating self-dual black hole with quasi-periodic oscillations
- Complete, Single-Horizon Quantum Corrected Black Hole Spacetime
- Quasinormal modes of a holonomy corrected Schwarzschild black hole
- Constraints on self-dual black hole in loop quantum gravity with S0-2 star in the Galactic Center
- Unsettling physics in the quantum-corrected Schwarzschild black hole
- Axial gravitational quasinormal modes of a self-dual black hole in loop quantum gravity
- Massless Dirac Perturbations in a Consistent Model of Loop Quantum Gravity Black Hole: Quasinormal Modes and Particle Emission Rates
Cited by in corpus (5)
- Quasinormal modes and gray-body factors of regular black holes in asymptotically safe gravity
- Particle dynamics and the accretion disk around a Self-dual Black Hole immersed in a magnetic field in Loop Quantum Gravity
- Spin foam amplitude of the black-to-white hole transition
- Quasinormal Modes and Shadows of Black Holes in Infinite Derivative Theory of Gravity
- Semi-classical imprints on quasinormal mode spectra