Noncommutative black holes in extended anti-de Sitter phase space
Athanasios G. Tzikas

TL;DR
This paper explores the thermodynamics of noncommutative black holes in extended anti-de Sitter space, revealing phase transitions similar to Van der Waals fluids and novel anti-Hawking-Page transitions across different dimensions.
Contribution
It introduces the treatment of cosmological constant and minimal length as thermodynamic variables in noncommutative black holes across multiple dimensions.
Findings
Four-dimensional black holes show Van der Waals-like phase transitions.
Three-dimensional black holes are thermodynamically stable.
Two-dimensional black holes exhibit a new anti-Hawking-Page transition.
Abstract
We study thermodynamic aspects of ordinary and lower dimensional noncommutative black holes within an extended anti-de Sitter phase space by treating the negative cosmological constant and the minimal cut-off length as thermodynamic variables representing the pressure and tension of the system, respectively. In four-dimensional spacetime, the regular black hole exhibits a small/large black hole phase transition analogous to the liquid/gas transition of a Van der Waals gas. The three-dimensional case demonstrates global and local thermodynamic stability, while the two-dimensional case reveals a novel type of transition referred to as the anti-Hawking-Page transition.
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Taxonomy
TopicsNoncommutative and Quantum Gravity Theories · Black Holes and Theoretical Physics · Quantum Electrodynamics and Casimir Effect
