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.
arXiv comment16 pages, 55 figures
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Cited by in corpus (4)
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- 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