2016
DOI: 10.1140/epjc/s10052-016-4463-4
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Phase structure of the Born–Infeld–anti-de Sitter black holes probed by non-local observables

Abstract: With the non-local observables such as two point correlation function and holographic entanglement entropy, we probe the phase structure of the Born-Infeld-anti-de Sitter black holes. For the case bQ > 0.5, where b is the BornInfeld parameter and Q is the charge of the black hole, the phase structure is found to be similar to that of the Van der Waals phase transition, namely the black hole undergoes a first order phase transition and a second order phase transition before it reaches a stable phase. While for … Show more

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Cited by 64 publications
(47 citation statements)
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“…It was found that the entanglement entropy can characterize the related phase transition for a charged AdS black hole. Further studies on holographic entanglement entropy and its relation to phase transition have been done for various AdS black holes in [35][36][37][38]. For the AdS phantom black hole presented in this paper, we will further show such a relation which keeps valid even for the case with the Ricci flat horizon black hole.…”
Section: Introductionmentioning
confidence: 60%
“…It was found that the entanglement entropy can characterize the related phase transition for a charged AdS black hole. Further studies on holographic entanglement entropy and its relation to phase transition have been done for various AdS black holes in [35][36][37][38]. For the AdS phantom black hole presented in this paper, we will further show such a relation which keeps valid even for the case with the Ricci flat horizon black hole.…”
Section: Introductionmentioning
confidence: 60%
“…The BI black hole solution in (A)dS space was first obtained in [45,46]. Since then, various aspects of BI black holes have been extensively investigated, e.g., the thermodynamics and phase structure [47][48][49][50][51][52], the holographic models [53][54][55][56][57][58][59][60]. Specifically, the Weak Cosmic Censorship (WCC) has recently been studied in a BI black hole [61,62], where it was found that there may exist some counterexamples to WCC.…”
Section: Introductionmentioning
confidence: 99%
“…(4.16), we can see that if the denominator in the integrand vanishes, i.e., 1 + H −2 f r 2 = 0, the shift h diverges. Since H is a conserved quantity, the above equation can be readily transformed to 17) in which, r crit is the critical position that makes the shift h divergent. For instance, in the case of Q = 0.6 and m = 0.6, a physical solution to eq.…”
Section: Black Hole Charge and Butterfly Effectmentioning
confidence: 99%
“…[5,6]. Among these studies, one interesting thing is to adopt the HEE to probe the thermalization process or phase transitions in the strongly coupled systems [7][8][9][10][11][12][13][14][15][16][17].…”
Section: Introductionmentioning
confidence: 99%