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Charged Accelerating BTZ black holes

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arxiv 2203.12619 v5 pith:CXYOVJUX submitted 2022-03-23 gr-qc hep-th

classification gr-qchep-th
keywords blackholesacceleratingconstanttemperaturechargechargedacceleration
verification ladder T0 review T1 audit T2 compute T3 formal
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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 asymptotic behavior depends on four parameters: the cosmological constant, mass, acceleration, and topological constant. Then, we study the temperature of these black holes and find that the temperature is always positive for AdS spacetime. 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 a coupling between the electrical charge and other quantities of the accelerating BTZ black holes. The asymptotic behavior of charged accelerating BTZ black holes depends on five parameters: the cosmological constant, the electrical charge, mass, the acceleration parameter, and the topological constant. Then, we studied the effects of charge, acceleration parameters, and the topological constant on the root of these black holes. Finally, we investigate the temperature of these black holes in AdS spacetime. For these black holes, the temperature depends on the electrical charge, accelerating parameter, and the cosmological constant. Our analysis indicates that the temperature of charged accelerating BTZ AdS black holes is always positive.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Generalized Fefferman-Graham gauge and boundary Weyl structures

    hep-th 2024-11 conditional novelty 6.0 of 10

    In the generalized Fefferman-Graham gauge, three-dimensional AdS gravity produces a boundary Weyl connection, a Weyl-covariant stress tensor and trace anomaly, and requires a new corner counterterm that fixes the Eucl...

  2. Notes on solution phase space and BTZ black hole

    gr-qc 2024-11 accept novelty 3.0 of 10

    A detailed worked example showing that the solution phase space method reproduces the known mass, angular momentum, entropy, first law, and Smarr relation for the BTZ black hole and three-dimensional Kerr-dS spacetime.

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