Signature of the Van der Waals like small-large charged AdS black hole phase transition in quasinormal modes

Liu, Yunqi; Zou, De-Cheng; Wang, Bin

doi:10.1007/jhep09(2014)179

Cited by 116 publications

(91 citation statements)

References 102 publications

(113 reference statements)

Supporting

Mentioning

Contrasting

Order By: Relevance

“…In this process, the real part of the QNMs frequencies varies slightly, while the absolute value of the imaginary part decreases which indicates that the absorption performance of the black hole is reduced whatever the spacetime dimension d is. This result is consistent with the overall analysis reported in [1,55].…”

Section: Qnm Behaviors In the Isobaric Phase Transitionsupporting

confidence: 93%

“…and the incoming waves behave as ψ(r ) ∼ (r − r H ) −i ω 4π T , which means that ψ(r ) is set to unity at the horizon [1]. Then we can reformulate Eq.…”

Section: Master Equation In High Dimension Rn-ads Black Hole Spacetimementioning

confidence: 99%

“…Also, in [1] the authors established a link between the Reissner-Nordström AdS black hole critical behavior and the quasinormal modes in d = 4, showing that QNM can be a dynamic probe of the thermodynamic phase transition. More precisely they find a drastic change in the slopes of the quasinormal frequencies in the small (SBH) and large (LBH) black holes near the critical point where the Van der Waals like thermodynamic phase transition occurs.…”

Section: Introductionmentioning

confidence: 96%

See 2 more Smart Citations

Behavior of quasinormal modes and high dimension RN–AdS black hole phase transition

et al. 2016

View full text Add to dashboard Cite

In this work we use the quasinormal frequencies of a massless scalar perturbation to probe the phase transition of the high dimension charged AdS black hole. The signature of the critical behavior of this black hole solution is detected in the isobaric as well as in isothermal process. This paper is a natural generalization of Liu et al. (JHEP 1409(JHEP :179, 2014 to higher dimensional spacetime. More precisely our study shows a clear signal for any dimension d in the isobaric process. As to the isothermal case, we find that this signature can be affected by other parameters like the pressure and the horizon radius. We conclude that the quasinormal modes can be an efficient tool to investigate the first-order phase transition, but fail to disclose the signature of the second-order phase transition.

show abstract

Section: Qnm Behaviors In the Isobaric Phase Transitionsupporting

confidence: 93%

“…and the incoming waves behave as ψ(r ) ∼ (r − r H ) −i ω 4π T , which means that ψ(r ) is set to unity at the horizon [1]. Then we can reformulate Eq.…”

Section: Master Equation In High Dimension Rn-ads Black Hole Spacetimementioning

confidence: 99%

Section: Introductionmentioning

confidence: 96%

See 1 more Smart Citation

Behavior of quasinormal modes and high dimension RN–AdS black hole phase transition

et al. 2016

View full text Add to dashboard Cite

show abstract

“…It has been proved that at the phase transition point, the second-order phase transition exists in AdS spacetime black holes and the thermodynamics agree very well with Ehrenfest equation [12,15,17,35,36,46,47]. At present there are two common methods to investigate the critical phenomenon of AdS space-time Black Holes in the literature.…”

Section: Introductionmentioning

confidence: 96%

Q– $$\Phi $$ Φ criticality in the extended phase space of $$(n+1)$$ ( n + 1 ) -dimensional RN-AdS black holes

Zhao

Cao

2016

Eur. Phys. J. C

View full text Add to dashboard Cite

In order to achieve a deeper understanding of gravity theories, i.e., the quantum properties of gravity theories and the statistical explanation of gravitational entropy, it is important to further investigate the thermodynamic properties of a black hole at the critical point, besides the phase transition and critical behaviors. In this paper, by using Maxwell's equal area law, we choose T, Q, as the state parameters and study the phase equilibrium problem of a general (n + 1)-dimensional RN-AdS black holes thermodynamic system. The boundary of the two-phase coexistence region and its isotherm and isopotential lines are presented, which may provide a theoretical foundation for studying the phase transition and phase structure of black hole systems.

show abstract

“…• Quasi-normal mode frequencies show a marked change near second order phase transitions between large and small black holes [84,85].…”

Section: Asymptotically Anti-de Sitter Black Holesmentioning

confidence: 99%

Black holes and Boyle's law — The thermodynamics of the cosmological constant

Dolan

2015

Mod. Phys. Lett. A

View full text Add to dashboard Cite

When the cosmological constant, Λ, is interpreted as a thermodynamic variable in the study of black hole thermodynamics a very rich structure emerges. It is natural to interpret Λ as a pressure and define the thermodynamically conjugate variable to be the thermodynamic volume of the black hole (which need not bear any relation to the geometric volume). Recent progress in this new direction for black hole thermodynamics is reviewed.

show abstract

Signature of the Van der Waals like small-large charged AdS black hole phase transition in quasinormal modes

Cited by 116 publications

References 102 publications

Behavior of quasinormal modes and high dimension RN–AdS black hole phase transition

Behavior of quasinormal modes and high dimension RN–AdS black hole phase transition

Q– $$\Phi $$ Φ criticality in the extended phase space of $$(n+1)$$ ( n + 1 ) -dimensional RN-AdS black holes

Black holes and Boyle's law — The thermodynamics of the cosmological constant

Contact Info

Product

Resources

About