Thermodynamics phase transition of Anti de Sitter Schwarzschild scalar-tensor-vector-Black Holes
Hossein Ghaffarnejad, Elham Ghasemi Kordkheilee

TL;DR
This paper investigates the thermodynamic phase transitions of Anti de Sitter Schwarzschild scalar-tensor-vector black holes, revealing a second-order phase transition akin to Van der Waals fluid behavior, influenced by black hole size and gravitational charge.
Contribution
It introduces a detailed analysis of phase transitions in scalar-tensor-vector black holes within AdS space, highlighting a second-order transition similar to liquid-gas systems.
Findings
Black holes exhibit a Van der Waals-like phase transition.
Critical point occurs when gravitational charge equals mass.
Phase transition occurs below the critical point in phase space.
Abstract
Instead of scalar tensor gravity models which is applicable for description of cosmic inflation with unknown dark sector of matter/energy, at presentense there are presented different alternative scalar tensor vector gravities where meaningful dynamical vector fields can support cosmic inflation well without to use dark matter/energy concept. One of these gravity models was presented by Moffat which its modified Schwarzschild black hole solution is used to study thermodynamic phase transition in presence of the AdS space pressure in this article. To do so we obtained an equation of state which asymptotically reaches to equation of state of ideal gas for large black holes but for small scale black holes we obtained a critical point at phase space where the black hole can be exhibit with a phase transition at processes of isotherm and isobaric. By looking at diagrams of the Gibbs free…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Relativity and Gravitational Theory
