P-V criticality of charged dilatonic black holes

Dehghani, M. H.; Kamrani, S.; Sheykhi, A.

doi:10.48550/arxiv.1505.02386

Cited by 17 publications

(24 citation statements)

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“…c , and T (iii) A first-order phase transition occurs because the F on demonstrates the characteristic swallow tail behavior. It is reminiscent of the "free energy-Hawking temperature" relation of charged AdS black hole, as described in [35][36][37][38][39][40]. The intersection point between the red solid line and the blue solid line is the first-order phase transition point that correspond to the temperature T First−order c .…”

Section: Thermodynamics and Phase Transition Of Rainbow Sc Black Holementioning

confidence: 95%

“…This seminal work has attracted wide attention because it can explained the confinement/deconfinement phase transition of gauge field in the AdS/CFT correspondence [33]. Since then, several works were devoted to investigate the Hawking-Page phase transition and the critical phenomena for other more complicated AdS spacetimes [34][35][36][37][38][39][40]. From these studies, people found that the phase transitions behavior of charged black holes is similar to that of the Van der Waals liquid-gas system [34][35][36][37][38][39][40][41].…”

Section: Introductionmentioning

confidence: 99%

“…Since then, several works were devoted to investigate the Hawking-Page phase transition and the critical phenomena for other more complicated AdS spacetimes [34][35][36][37][38][39][40]. From these studies, people found that the phase transitions behavior of charged black holes is similar to that of the Van der Waals liquid-gas system [34][35][36][37][38][39][40][41]. In 2012, Kubizňák and Mann proposed a remarkable new perspective on the relationship between the phase transition of charged AdS black hole and the Van der Waals liquid-gas phase transition [34].…”

Section: Introductionmentioning

confidence: 99%

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Thermodynamic phase transition of a black hole in rainbow gravity

Feng

2017

Physics Letters B

100

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In this letter, using the rainbow functions that were proposed by Magueijo and Smolin, we investigate the thermodynamics and the phase transition of rainbow Schwarzschild black hole. First, we calculate the rainbow gravity corrected Hawking temperature. From this modification, we then derive the local temperature, free energy, and other thermodynamic quantities in an isothermal cavity. Finally, we analyze the critical behavior, thermodynamic stability, and phase transition of the rainbow Schwarzschild black hole. The results show that the rainbow gravity can stop the Hawking radiation in the final stages of black holes' evolution and lead to the remnants of black holes. Furthermore, one can observe that the rainbow Schwarzschild black hole has one first-order phase transition, two second-order phase transitions, and three Hawking-Page-type phase transitions in the framework of rainbow gravity theory.Comment: 7 pages, 3 figures, accepted for publication in Physical Letter B. arXiv admin note: substantial text overlap with arXiv:1608.0682

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Section: Thermodynamics and Phase Transition Of Rainbow Sc Black Holementioning

confidence: 95%

Section: Introductionmentioning

confidence: 99%

Section: Introductionmentioning

confidence: 99%

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Thermodynamic phase transition of a black hole in rainbow gravity

Feng

2017

Physics Letters B

100

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“…It was found that a first order small and large black holes phase transition is allowed and the P − V isotherms are analogous to the Van der Waals fluid. More discussions including reentrant phase transitions and more general Van der Waals behavior in this direction can be found as well [22][23][24][25][26][27][28][29][30][31][32][33]. In addition, there is a well-known process in classical thermodynamics, called Joule-Thomson expansion, was generalized to charged AdS black holes in Ref.…”

Section: Introductionmentioning

confidence: 99%

$P-V$ criticality and Joule-Thomson Expansion of Hayward-AdS black holes in 4D Einstein-Gauss-Bonnet gravity

Zhang,

Zou

et al. 2021

Preprint

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In this paper, the P − V criticality and Joule-Thomson Expansion of Hayward-AdS black holes in 4D Einstein-Gauss-Bonnet gravity are studied in the extended phase space. We find the black hole always exhibits a phase transition similar to that of the Van der Waals system for any arbitrary positive parameters α and g. We also study the dependence of α and g on the inversion curves and plot the inversion and isenthalpic curves in the T − P plane, which can determine the cooling-heating regions.

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“…which provides interesting clues to the underlying structure of quantum gravity. In particular, promoted by the AdS/CFT correspondence [26,27], the investigation of black hole phase transitions in AdS spacetimes has received popular attention [28][29][30][31][32][33][34][35][36][37]. The pioneering study of the transitions can be traced back to the well-known Hawking-Page phase transition [38],…”

Section: Introductionmentioning

confidence: 99%

$Q$-$Φ$ criticality and microstructure of charged AdS black holes in $f(R)$ gravity

Deng,

Huang

2017

Preprint

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The phase transition and critical behaviours of charged AdS black holes in f (R) gravity with a conformally invariant Maxwell (CIM) source and constant curvature are further investigated. As a highlight, this research is carried out by employing new state parameters (T, Q, Φ) and contributes to deeper understanding the thermodynamics and phase structure of black holes. Our analyses manifest that the charged f (R)-CIM AdS black hole undergoes a first order small-large black hole phase transition, and the critical behaviours qualitatively behave like a Van der Waals liquid-vapor system. However, differing from the case in Einstein's gravity, phase structures of the black holes in f (R) theory exhibit an interesting dependence on gravity modification parameters. Moreover, we adopt the thermodynamic geometry to probe the black hole microscopic properties. The results show that, on the one hand, both the Ruppeiner curvature and heat capacity diverge exactly at the critical point, on the other hand, the f (R)-CIM AdS black hole possesses the property as ideal Fermi gases. Of special interest, we discover a microscopic similarity between the black holes and a Van der Waals liquid-vapor system.

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P-V criticality of charged dilatonic black holes

Cited by 17 publications

References 0 publications

Thermodynamic phase transition of a black hole in rainbow gravity

Thermodynamic phase transition of a black hole in rainbow gravity

$P-V$ criticality and Joule-Thomson Expansion of Hayward-AdS black holes in 4D Einstein-Gauss-Bonnet gravity

$Q$-$Φ$ criticality and microstructure of charged AdS black holes in $f(R)$ gravity

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