Van der Waals black hole
Aruna Rajagopal, David Kubiznak, Robert B. Mann

TL;DR
This paper introduces a black hole solution in extended phase space whose thermodynamics mimic the Van der Waals fluid, but the solution violates energy conditions outside the horizon.
Contribution
It presents a novel asymptotically AdS black hole model with Van der Waals-like thermodynamics and analyzes its physical viability through energy condition violations.
Findings
Thermodynamics matches Van der Waals fluid exactly
The solution violates energy conditions outside the horizon
Provides insights into black hole thermodynamics in extended phase space
Abstract
In the context of extended phase space, where the negative cosmological constant is treated as a thermodynamic pressure in the first law of black hole thermodynamics, we find an asymptotically AdS metric whose thermodynamics matches exactly that of the Van der Waals fluid. However, we show that as a solution of Einstein's equations, the corresponding stress energy tensor does not obey any of the energy conditions everywhere outside of the horizon.
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