Born–Infeld black holes in the presence of a cosmological constant

Dey, Tanay K.

doi:10.1016/j.physletb.2004.06.047

Cited by 210 publications

(63 citation statements)

References 17 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…The black hole possesses a singularity at r ¼ 0, which can be a naked singularity or enveloped by one or two horizons, depending on the values of the parameters. The expansion of the function fðrÞ around r ¼ 0 takes the form [41] …”

Section: Solutions Of D-dimensional Born-infeld Ads Black Holesmentioning

confidence: 99%

Critical behavior of Born-Infeld AdS black holes in the extended phase space thermodynamics

2014

View full text Add to dashboard Cite

We study the thermodynamics of D-dimensional Born-Infeld AdS black holes in the extended phase space. We find that the usual small-large black hole phase transition, which exhibits analogy with the Van de Waals liquid-gas system, holds in all dimensions greater than three. However, different from the four-dimensional case, in the system of higher dimensional Born-Infeld AdS black holes there is no reentrant phase transition. For the three-dimensional Born-Infeld AS black hole, there does not exist critical phenomena.

show abstract

Section: Solutions Of D-dimensional Born-infeld Ads Black Holesmentioning

confidence: 99%

Critical behavior of Born-Infeld AdS black holes in the extended phase space thermodynamics

2014

View full text Add to dashboard Cite

show abstract

“…Furthermore, BI electrodynamics can come from the low energy limit of string theory and encodes the low-energy dynamics of D-branes [44]. 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].…”

Section: Introductionmentioning

confidence: 99%

Strong cosmic censorship for a scalar field in a Born-Infeld–de Sitter black hole

et al. 2019

View full text Add to dashboard Cite

It has been shown that the Strong Cosmic Censorship (SCC) can be violated by a scalar field in a near-extremal Reissner-Nordstrom-de Sitter black hole. In this paper, we investigate the Strong Cosmic Censorship in a Born-Infeld-de Sitter black hole by a scalar perturbation field with/without a charge. When the Born-Infeld parameter b becomes small, the nonlinear electrodynamics effect starts to play an important role and tends to rescue SCC. Specifically, we find that the SCC violation region decreases in size with decreasing b. Moreover, for a sufficiently small b, SCC can always be restored in a near-extremal Born-Infeld-de Sitter black hole with a fixed charge ratio. arXiv:1907.04466v2 [hep-th]

show abstract

“…In the presence of a negative cosmological constant and an electric charge, its solution and thermodynamics were investigated in Refs. [9][10][11]. On the other hand, for the soliton solution, it takes the form…”

mentioning

confidence: 99%