Geodesic analysis and black hole shadows on a general non--extremal rotating black hole in five--dimensional gauged supergravity

Abstract

In this work, motivated by the fact that higher-dimensional theories predict the existence of black holes which differ from their four-dimensional counterpart, we analyse the geodesics and black hole shadow cast by a general non-extremal five-dimensional black hole. The system under consideration corresponds to the Chong-Cvetič-Lü-Pope (Phys. Rev.Lett.{\bf 95}, 161301 (2005)), which has the Myers--Perry black hole as a limit.

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• Superradiance evolution of black hole shadows revisited
• No-Hair Theorem in the Wake of Event Horizon Telescope
• Einstein-Æther Gravity in the light of Event Horizon Telescope Observations of M87*
• Shadow and weak gravitational lensing of a rotating regular black hole in a non-minimally coupled Einstein-Yang-Mills theory in the presence of plasma
• Constraints on Barrow entropy from M87* and S2 star observations
• Black hole surrounded by the pseudo-isothermal dark matter halo
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• Shadows of rotating Einstein-Maxwell-dilaton black holes surrounded by a plasma
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• Constraining a one-dimensional wave-type gravitational wave parameter through the shadow of M87* via Event Horizon Telescope
• Topological dyonic black holes of massive gravity with generalized quasitopological electromagnetism