Scalar quasi-normal modes of a loop quantum black hole
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Publication:6623762
DOI10.1088/1475-7516/2024/10/037MaRDI QIDQ6623762
Clara Montagnon, Hugo Roussille, Naritaka Oshita, Etera R. Livine
Publication date: 24 October 2024
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Cites Work
- Semiclassical loop quantum black hole
- Extreme gravity tests with gravitational waves from compact binary coalescences: II: Ringdown
- Spectral theory and quantum mechanics
- An effective model for the quantum Schwarzschild black hole
- \((b,v)\)-type variables for black to white hole transitions in effective loop quantum gravity
- Quasinormal modes of black holes and black branes
- The singularities of gravitational collapse and cosmology
- Quasinormal modes: the characteristic `sound' of black holes and neutron stars
- Quantum black holes in loop quantum gravity
- A consistent model of non-singular Schwarzschild black hole in loop quantum gravity and its quasinormal modes
- Constraints on self-dual black hole in loop quantum gravity with S0-2 star in the galactic center
- Properties of a recent quantum extension of the Kruskal geometry
- Higher order WKB formula for quasinormal modes and grey-body factors: recipes for quick and accurate calculations
- Effective quantum extended spacetime of polymer Schwarzschild black hole
- Spherically symmetric loop quantum gravity: analysis of improved dynamics
- Black hole collapse and bounce in effective loop quantum gravity
- Mass and horizon Dirac observables in effective models of quantum black-to-white hole transition
- Gravitational Collapse and Space-Time Singularities
- Quasi-normal modes of stars and black holes
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