Polar gravitational perturbations and quasinormal modes of a loop quantum gravity black hole
arXiv:2005.02208 · doi:10.1103/PhysRevD.102.044063
Abstract
In this work, we have calculated the polar gravitational quasinormal modes for a quantum corrected black hole model, that arises in the context of Loop Quantum Gravity, known as Self-Dual Black Hole. In this way, we have calculated the characteristic frequencies using the WKB approach, where we can verify a strong dependence with the Loop Quantum Gravity parameters. At the same time we check that the Self-Dual Black Hole is stable under polar gravitational perturbations, we can also verify that the spectrum of the polar quasinormal modes differs from the axial one \cite{Cruz:2015bcj}. Such a result tells us that isospectrality is broken in the context of Self Dual Black Holes.
arXiv comment16 pages, 5 figures. This manuscript has been accepted for publication as a Regular Article in Physical Review D
References in corpus (22)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
- GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
- Quasinormal modes of black holes and black branes
- Quasi-Normal Modes of Stars and Black Holes
- Quasinormal modes of black holes: from astrophysics to string theory
- Quasinormal Modes of AdS Black Holes and the Approach to Thermal Equilibrium
- Astrophysical Implications of the Binary Black-Hole Merger GW150914
- Quasinormal Modes, the Area Spectrum, and Black Hole Entropy
- Quantum Transfiguration of Kruskal Black Holes
- Quantum Extension of the Kruskal Space-time
- Quasinormal frequencies of Schwarzschild black holes in anti-de Sitter spacetimes: A complete study on the asymptotic behavior
- Space-Time Structure of Loop Quantum Black Hole
- Parametrized black hole quasinormal ringdown. I. Decoupled equations for nonrotating black holes
- Loop quantization of the Schwarzschild interior revisited
- From black holes to white holes: a quantum gravitational, symmetric bounce
- Self-dual Black Holes in LQG: Theory and Phenomenology
- Quantum gravity predictions for black hole interior geometry
- On effective loop quantum geometry of Schwarzschild interior
- Quasinormal frequencies of self-dual black holes
- Von-Neumann Stability and Singularity Resolution in Loop Quantized Schwarzschild Black Hole
- Gravitational axial perturbations and quasinormal modes of loop quantum black holes
Cited by in corpus (14)
- Shadow and stability of quantum-corrected black holes
- Probing the Effective Quantum Gravity via Quasinormal Modes and Shadows of Black Holes
- Constraints on the rotating self-dual black hole with quasi-periodic oscillations
- Constraints on self-dual black hole in loop quantum gravity with S0-2 star in the Galactic Center
- Breaking of isospectrality of quasinormal modes in nonrotating loop quantum gravity black holes
- Lessons from black hole quasinormal modes in modified gravity
- Long-lived Quasinormal modes around regular black holes and wormholes in Covariant Effective Quantum Gravity
- 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
- Quasinormal modes of a massive scalar field nonminimally coupled to gravity in the spacetime of Self-Dual Black Hole
- Quasinormal modes of a nonsingular spherically symmetric black hole effective model with holonomy corrections
- Hunting for extra dimensions in black hole shadows
- Quasinormal Modes and Gray-Body Factors for Gravitational Perturbations in Asymptotically Safe Gravity
- Noncommutative quasinormal modes of Schwarzschild black hole