Holographic complexity in charged accelerating black holes

Jiang, Shun; Jiang, Jie

doi:10.1016/j.physletb.2021.136731

Cited by 12 publications

(5 citation statements)

References 25 publications

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“…Later, it was obviously shown [8] that the C-metric can be derived from the metric of two superposed Schwarzschild black holes by assuming that the mass and location of one of them approaches infinity in an appropriate way. In recent years, aspects of the accelerating black holes, including global causal structure [9], quantum thermal properties [10], holographic heat engines [11,12], black hole shadows [13], holographic complexity [14,15], and so on, have been investigated extensively. In particular, thermodynamics of the AdS 4 C-metric have been figured out first in Ref.…”

Section: Introductionmentioning

confidence: 99%

Topological classes of rotating black holes

2023

Phys. Rev. D

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In this paper, utilizing the generalized off-shell Helmholtz free energy, we explore the topological numbers of the four-dimensional static accelerating black hole and its AdS extension, as well as the static charged accelerating black hole and its AdS extension. Our analysis reveals a profound and significant impact of the acceleration parameter on the topological numbers associated with the static black holes. In addition, we demonstrate that the electric charge parameter has an important effect on the topological number of the static neutral accelerating black holes. What is more, we also indicate that the cosmological constant has a remarkable influence on the topological number of the static accelerating black hole.

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Section: Introductionmentioning

confidence: 99%

Topological classes of rotating black holes

2023

Phys. Rev. D

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“…[21][22][23][24][25][26][27]. Considering the charged accelerating black holes is shown that the late-time growth rate of complexity is different from the ordinary charged black holes [28]. The efficiency of heat engine for (an)a (un)charged accelerating non-rotating AdS black hole [29,30], charged accelerating rotating black hole [31,32], have been studied.…”

Section: Introductionmentioning

confidence: 99%

Charged Accelerating BTZ black holes

Panah¹

2022

Preprint

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In this paper, we first extract general uncharged accelerating BTZ black hole solutions and study some of their properties. Our analysis shows that spacetime's asymptotical behavior depends on four parameters (the cosmological constant, mass, the acceleration parameter, and the topological constant). Then, we study the temperature of these black holes and find a divergence point, which this point reveals a phase transition between physical and non-physical black holes. Next, we extend our study for extracting charged accelerating BTZ black hole solutions in the presence of a nonlinear electrodynamics field, known as conformally invariant Maxwell. Our findings indicate that there is a coupling between the electrical charge and other quantities of the accelerating BTZ black holes. We find that the asymptotical behavior of charged accelerating BTZ black holes depends on six parameters (the cosmological constant, the electrical charge, mass, the acceleration parameter, topological constant, and angular coordinate). Finally, we investigate the effects of various parameters on the temperature of these black holes. There are two exciting behaviors for the temperature by considering different cosmological constant values. A divergence point exists for the temperature when the cosmological constant is negative. However, for the positive value of the cosmological constant, there are three critical points in the temperature; two roots and a divergence point. These points give us information about phase transitions between physical and non-physical black holes.

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“…5 AC in a different class of braneless (AdS) C-metrics has been considered in [40,41]. It is also possible to include a second brane at r = ∞ [36].…”

Section: Metric and Parametersmentioning

confidence: 99%

Holographic complexity of quantum black holes

Frassino

Sasieta

Tomašević

2022

J. High Energ. Phys.

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We analyze different holographic complexity proposals for black holes that include corrections from bulk quantum fields. The specific setup is the quantum BTZ black hole, which encompasses in an exact manner the effects of conformal fields with large central charge in the presence of the black hole, including the backreaction corrections to the BTZ metric. Our results show that Volume Complexity admits a consistent quantum expansion and correctly reproduces known limits. On the other hand, the generalized Action Complexity picks up large contributions from the singularity, which is modified due to quantum backreaction, with the result that Action Complexity does not reproduce the expected classical limit. Furthermore, we show that the doubly-holographic setup allows computing the complexity coming purely from quantum fields — a notion that has proven evasive in usual holographic setups. We find that in holographic induced-gravity scenarios the complexity of quantum fields in a black hole background vanishes to leading order in the gravitational strength of CFT effects.

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Holographic complexity in charged accelerating black holes

Cited by 12 publications

References 25 publications

Topological classes of rotating black holes

Topological classes of rotating black holes

Charged Accelerating BTZ black holes

Holographic complexity of quantum black holes

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