Abstract
AbstractThe 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 the 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, Ruppeiner geometry is used to look into the AdS black hole's microscopic structure. The Ricci curvature scalar R to explain the interactions between the AdS black hole's microscopic particles under the influence of gravity have been numerically computed.
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