A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality
Ahmad Al-Badawi, Faizuddin Ahmed, and \.Izzet Sakall{\i}

TL;DR
This paper explores black hole solutions in Kalb-Ramond gravity with quintessence, analyzing how Lorentz violation and exotic matter influence spacetime, particle dynamics, lensing, and thermodynamics, offering potential observational signatures.
Contribution
It provides new analytical models of black holes incorporating Lorentz violation and quintessence, detailing their effects on geodesics, shadows, wave stability, and thermodynamic phase structures.
Findings
Modified photon sphere and ISCO properties due to parameters
Analytical black hole shadow radii dependent on quintessence states
Altered thermodynamic phase behavior and stability characteristics
Abstract
We present a theoretical investigation of black hole solutions in Kalb-Ramond gravity embedded with quintessence fields. Our study examines how combined effects of Lorentz violation through the Kalb-Ramond field parameter and exotic matter contributions via quintessence parameters systematically modify spacetime geometry, particle dynamics, and observational signatures compared to standard Schwarzschild black holes. The analysis encompasses geodesic motion for both photons and massive particles, revealing substantial modifications to effective potentials, photon sphere characteristics, and innermost stable circular orbit properties. We derive analytical expressions for black hole shadow radii across different quintessence states, demonstrating systematic parameter dependencies enabling observational discrimination between theoretical frameworks. Our perturbation…
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Black Holes and Theoretical Physics
