AdS black hole thermodynamics and microstructures from gravitation
arXiv:2311.02145 · doi:10.1002/prop.202300043
Abstract
The significant properties and phase transition of charged Anti-de Sitter (AdS) black holes have been extensively studied in a variety of modified theories of gravity in the presence of numerous matter fields. The goal of our current research is to investigate the AdS black hole's thermodynamics under the impact of gravity. Additionally, this paper explores the black hole's local stability and phase structure under the relevant gravity. Besides, we use Ruppeiner geometry to look into the AdS black hole's microscopic structure. We have numerically computed the Ricci curvature scalar to explain the interactions between the AdS black hole's microscopic particles under the influence of gravity.
Fortschr. Phys. published version
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- Cosmological constraints on gravity models in the non-coincident formalism
- Thermodynamics of deformed AdS-Schwarzschild black holes in the presence of Thermal fluctuations
- Optical, Dynamic and Topological Characteristics of Deformed Schwarzschild Black Holes
- Scale-Invariant Bounce Cosmology in Weyl f(Q) Gravity with Quintom Signature
- Universality on thermodynamic relation with corrections in higher-dimensional de Sitter black holes