Black Hole Shadows in Einstein-Bel-Robinson Gravity

Fuente: arXiv
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Main Authors: Hamil, B., Lütfüoğlu, B. C.
Format: Preprint
Published: 2023
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author Hamil, B.
Lütfüoğlu, B. C.
author_facet Hamil, B.
Lütfüoğlu, B. C.
contents Gravity models given by higher-order scalar curvature corrections are believed to bear important consequences. The Einstein-Bel-Robinson gravity, with quartic curvature modification, motivated Sajadi et al to explore static spherically symmetric black hole solutions with perturbative methods. In this paper, inspired by their work, we investigate AdS black hole shadows in EBR gravity. Moreover, we demonstrate how the gravity parameter alters the energy emission rate. Finally, we handle the same problem in the presence of plasma, since the black holes are thought to be surrounded by a medium that changes the geodesic of photons.
format Preprint
id arxiv_https___arxiv_org_abs_2311_12354
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Black Hole Shadows in Einstein-Bel-Robinson Gravity
Hamil, B.
Lütfüoğlu, B. C.
General Relativity and Quantum Cosmology
High Energy Physics - Theory
Gravity models given by higher-order scalar curvature corrections are believed to bear important consequences. The Einstein-Bel-Robinson gravity, with quartic curvature modification, motivated Sajadi et al to explore static spherically symmetric black hole solutions with perturbative methods. In this paper, inspired by their work, we investigate AdS black hole shadows in EBR gravity. Moreover, we demonstrate how the gravity parameter alters the energy emission rate. Finally, we handle the same problem in the presence of plasma, since the black holes are thought to be surrounded by a medium that changes the geodesic of photons.
title Black Hole Shadows in Einstein-Bel-Robinson Gravity
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2311.12354