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      The Last Lost Charge And Phase Transition In Schwarzschild AdS Minimally Coupled to a Cloud of Strings

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          Abstract

          In this paper we study the Schwarzschild AdS black hole with a cloud of string background in an extended phase space and investigate a new phase transition related to the topological charge. By treating the topological charge as a new charge for black hole solution we study its thermodynamics in this new extended phase space. We treat by two approaches to study the phase transition behaviour via both \(T-S\) and \(P-v\) criticality and we find the results confirm each other in a nice way. It is shown a cloud of strings affects the critical physical quantities and it could be observed an interesting Van der Waals-like phase transition in the extended thermodynamics. The swallow tail-like behavior is also observed in Free Energy-Temperature diagram. We observe in \(a\to 0\) limit the small/large black hole phase transition reduces to the Hawking-Page phase transition as we expects. We can deduce that the impact of cloud of strings in Schwarzschild black hole can bring Van der Waals-like black hole phase transition.

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          On the critical phenomena and thermodynamics of charged topological dilaton AdS black holes

          , , (2013)
          In this paper, we study the phase structure and equilibrium state space geometry of charged topological dilaton black holes in \((n+1)\)-dimensional anti-de Sitter spacetime. By considering the pairs of parameters \((P\sim V)\) and \((Q\sim U)\) as variables, we analyze the phase structure and critical phenomena of black holes and discuss the relation between the two kinds of critical phenomena. We find that the phase structures and critical phenomena drastically depend on the cosmological constant \(l\) (or the static electric charge \(Q\) of the black holes), dimensionality \(n\) and dilaton field \(\Phi \).
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            Reentrant phase transitions and van der Waals behaviour for hairy black holes

            We study the extended phase space thermodynamics for hairy AdS black hole solutions to Einstein-Maxwell-\(\Lambda\) theory conformally coupled to a scalar field in five dimensions. We find these solutions to exhibit van der Waals behaviour in both the charged/uncharged cases, and reentrant phase transitions in the charged case. This is the first example of reentrant phase transitions in a five dimensional gravitational system which does not include higher curvature corrections.
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              Combined effects of f(R) gravity and conformally invariant Maxwell field on the extended phase space thermodynamics of higher-dimensional black holes

              In this paper, we investigate the thermodynamics of higher-dimensional \(f(R)\) black holes in the extended phase space. Both the analytic expressions and numerical results for the possible critical physical quantities are obtained. It is proved that meaningful critical specific volume only exists when \(p\) is odd. This unique phenomenon may be attributed to the combined effect of \(f(R)\) gravity and conformally invariant Maxwell field. It is also shown that the ratio \(P_cv_c/T_c\) differs from that of higher dimensional charged AdS black holes in Einstein gravity. However, the ratio for four-dimensional \(f(R)\) black holes is the same as that of four-dimensional RN-AdS black holes, implying that \(f(R)\) gravity does not influence the ratio. So the ratio may be related to conformally invariant Maxwell field. To probe the phase transition, we derive the explicit expression of the Gibbs free energy with its graph plotted. Phase transition analogous to the van der Waals liquid-gas system take place between the small black hole and the large black hole. Classical swallow tail behavior, characteristic of first order phase transition, can also be observed in the Gibbs free energy graph. Critical exponents are also calculated. It is shown that these exponents are exactly the same as those of other AdS black holes, implying that neither \(f(R)\) gravity nor conformally invariant Maxwell field influence the critical exponents. Since the investigated black hole solution depends on the form of the function \(f(R)\), we discuss in detail how our results put constraint on the form of the function \(f(R)\) and we also present a simple example.
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                Author and article information

                Journal
                13 June 2018
                Article
                1806.06688
                989f5fde-759c-4cf8-a732-e599402a6434

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                13 pages, 5 figure
                hep-th

                High energy & Particle physics
                High energy & Particle physics

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