2017
DOI: 10.1140/epjc/s10052-017-5356-x
|View full text |Cite
|
Sign up to set email alerts
|

Horndeski gravity and the violation of reverse isoperimetric inequality

Abstract: We consider Einstein-Horndeski-Maxwell gravity, together with a cosmological constant and multiple Horndeski axions. We construct charged AdS planar black holes in general dimensions where the Horndeski axions span over the planar directions. We analyze the thermodynamics and obtain the black hole volumes. We show that the reverse isoperimetric inequality can be violated, implying that these black holes can store information more efficiently than the Schwarzschild black hole.

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1

Citation Types

0
18
0

Year Published

2017
2017
2020
2020

Publication Types

Select...
8

Relationship

4
4

Authors

Journals

citations
Cited by 16 publications
(18 citation statements)
references
References 49 publications
(90 reference statements)
0
18
0
Order By: Relevance
“…When the equality is saturated, a black hole of a given thermodynamic volues has attained its maximal possible entropy. Since then, the isoperimetric ratio R of various black hole families have been studied, and some were found to violate this inequality [8][9][10][11][12][13][14][15][16]. Such black holes have come to be called super-entropic, since they have more entropy that the relation (1) would admit.…”
mentioning
confidence: 99%
“…When the equality is saturated, a black hole of a given thermodynamic volues has attained its maximal possible entropy. Since then, the isoperimetric ratio R of various black hole families have been studied, and some were found to violate this inequality [8][9][10][11][12][13][14][15][16]. Such black holes have come to be called super-entropic, since they have more entropy that the relation (1) would admit.…”
mentioning
confidence: 99%
“…This feature is similar to that of Lovelock gravity [58]. A class of black hole solutions were constructed in Horndeski theory in [59,60] and their thermodynamics were studied in [61,62], the instability and holographic applications can be found in [63][64][65][66][67][68][69][70][71][72][73][74][75] and reference therein. In particular it was proposed that the theory is a holographic dual to some scale invariant but not conformal invariant quantum field theory [73,75].…”
Section: Einstein-maxwell-horndeski Theorymentioning
confidence: 83%
“…The stability and causality of these black holes were carried out in [42][43][44]. Holographic application of Horndeski theory were investigated in [45][46][47][48][49][50][51][52], especially, it was shown in [51] that although there is no holographic a-theorem for general Horndeski gravity, there does exist a critical point in parameter space where the holographic a-theorem can be achieved, which suggests the Horndeski theory should have a holographic field theory dual. The AdS black holes we studied in this paper are in this critical point.…”
Section: )mentioning
confidence: 99%