Ergosphere Dynamics and Rotational Energy Extraction in Bumblebee Kerr-Newman-AdS Black Holes
H. Hassanabadi, A. Guvendi, F. Kafikang, T. Sathiyaraj, S.Zare

TL;DR
This paper investigates the effects of Lorentz symmetry violation on the properties of Kerr-Newman-AdS black holes, revealing modifications in thermodynamics, shadow structure, and energy extraction mechanisms that could be observable.
Contribution
It provides the first detailed analysis of Bumblebee Kerr-Newman-AdS black holes, highlighting how Lorentz violation alters thermodynamic stability, shadow morphology, and ergosphere dynamics.
Findings
Lorentz violation induces black hole remnants and extended stability phases.
Hawking radiation becomes more discrete and less thermal due to Lorentz violation.
Increased parameters compress and distort the black hole shadow and ergosphere, enhancing energy extraction.
Abstract
We present a comprehensive analysis of the thermodynamic and optical properties of the Bumblebee Kerr-Newman-Anti-de Sitter (AdS) black hole, a rotating and charged configuration arising in Lorentz symmetry-violating (LSV) gravity. The influence of the black hole parameters on the horizon structure, thermodynamic stability, and geometric deformation of spacetime is systematically investigated. Explicit expressions for the Hawking temperature, entropy, and heat capacity are derived, revealing the formation of black hole remnants and extended stability phases induced by Lorentz symmetry-violating (LSV) effects. The sparsity of Hawking radiation is quantified, showing that Lorentz violation suppresses the continuum limit and produces a more discrete, less thermal emission spectrum. A detailed analysis of null geodesics is performed to determine the photon region and shadow morphology,…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories · Astrophysical Phenomena and Observations
