Phase structure of charged AdS black holes surrounded by exotic fluid with modified Chaplygin equation of state
Y. Sekhmani, J. Rayimbaev, G. G. Luciano, R. Myrzakulov, D. J. Gogoi

TL;DR
This paper investigates the phase structure and critical behavior of charged AdS black holes surrounded by modified Chaplygin gas, revealing van der Waals-like phase transitions and applying geometrothermodynamic tools for analysis.
Contribution
It introduces a novel black hole solution with a surrounding MCG and analyzes its thermodynamic phase transitions using multiple geometrothermodynamic methods.
Findings
Black hole exhibits van der Waals-like small/large phase transition.
Critical exponents indicate universal scaling behavior.
Geometrothermodynamic metrics successfully identify critical points.
Abstract
By considering the concept of the modified Chaplygin gas (MCG) as a single fluid model unifying dark energy and dark matter, we construct a static, spherically charged black hole (BH) solution in the framework of General Relativity. The criticality of the charged anti-de Sitter (AdS) BH with a surrounding MCG is explored in the context of the extended phase space, where the negative cosmological constant operates as a thermodynamical pressure. This critical behavior shows that the small/large BH phase transition is analogous to the van der Waals liquid/gas phase transition. Accordingly, along the phase spaces, we derive the BH equations of state and then numerically evaluate the corresponding critical quantities. Similarly, critical exponents are identified, along with outcomes demonstrating the scaling behavior of thermodynamic quantities near criticality into a universal…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Galaxies: Formation, Evolution, Phenomena
