Infrared Extended Uncertainty Principle Corrections and Quintessence-Induced Topology of Reissner-Nordstr\"om AdS Black Holes
Y. Sekhmani, G.G.Luciano, S.N.Gashti, A.Baruah

TL;DR
This paper investigates how infrared quantum gravitational effects and quintessence fields influence the thermodynamics, topology, and photon sphere structure of Reissner-Nordström AdS black holes, revealing complex phase behaviors and topological properties.
Contribution
It provides a unified analysis incorporating EUP corrections and quintessence effects on black hole thermodynamics and topology, with analytic expressions and topological charge calculations.
Findings
EUP modifies Hawking temperature, entropy, and heat capacity expressions.
Quintessence alters the black hole metric and phase structure.
Photon sphere topology can split or merge due to quintessence, maintaining total charge.
Abstract
We present a unified topological and geometric analysis of charged Anti-de Sitter (AdS) black holes immersed in a quintessence field, incorporating infrared gravitational corrections arising from the Extended Uncertainty Principle (EUP). The latter modifies the standard Heisenberg uncertainty relation by introducing a minimal momentum/maximal length scale, which effectively captures long-wavelength quantum gravitational effects relevant to black hole thermodynamics in curved spacetimes. We derive analytic expressions for the corrected Hawking temperature, entropy and heat capacity in terms of the EUP deformation parameter. Furthermore, the inclusion of quintessence, characterized by barotropic indices \(\omega_q = -\frac{2}{3}\) and \(\omega_q = -\frac{1}{3}\), modifies the black hole metric function. By studying the relaxation-time function , we identify a number of…
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