The black hole shadow of quantum Oppenheimer-Snyder-de Sitter spacetime
arXiv:2409.16323 · doi:10.1103/PhysRevD.110.124042
Abstract
In this study, we investigate the black hole shadow of an exact black hole solution of the loop quantum gravity (LQG) theory. We discuss some of its optical characteristics after generalizing it to the rotational case, including null geodesics and black hole shadow. From these we can compare the impact of different theories on the most deeply understood characteristics of the black hole and get a new way to test the accuracy of the modified gravity theory.
16 pages, 55 figures
References in corpus (9)
- First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole
- Black Hole Shadows, Photon Rings, and Lensing Rings
- Generating rotating regular black hole solutions without complexification
- Shadows of Einstein-dilaton-Gauss-Bonnet black holes
- Quantum Oppenheimer-Snyder and Swiss Cheese models
- Shadow casted by a Konoplya-Zhidenko rotating non-Kerr black hole
- Image of Kerr-Melvin black hole with thin accretion disk
- Black hole image encoding quantum gravity information
- The quasinormal modes, pseudospectrum and time evolution of Proca fields in quantum Oppenheimer-Snyder-de Sitter spacetime
Cited by in corpus (4)
- Phantom RN-AdS black holes in noncommutative space
- Observational properties of black hole in quantum fluctuation modified gravity
- Quasinormal Modes and Shadows of Black Holes in Infinite Derivative Theory of Gravity
- Shadows of naked singularities and superspinars related to the revisited Kerr-de Sitter spacetimes