Charged rotating black strings in Einsteinian cubic gravity - INSPIRE

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Charged rotating black strings in Einsteinian cubic gravity

Hamid R. Bakhtiarizadeh
(
- Unlisted, IR
)

Nov 4, 2021

16 pages

Published in:

Phys.Rev.D 105 (2022) 6, 064037

Published: Mar 15, 2022

e-Print:

2111.02663 [gr-qc]

DOI:

10.1103/PhysRevD.105.064037 (publication)

View in:

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Abstract: (APS)

We construct, for the first time, charged rotating black string solutions in four-dimensional Einsteinian cubic gravity, which are asymptotically anti–de Sitter. By assuming that the solutions are completely regular at the horizon and studying their near-horizon behavior, we find some thermodynamic properties, which can be accessed analytically. We compute independently the Hawking temperature, the Wald entropy, the mass, the angular momentum, the charge, and the electrostatic potential of the solutions, analytically. Using these, we show that the first law of thermodynamics for rotating black strings is exactly satisfied in both charged and uncharged cases. We also observe that, in the absence of Maxwell field, some of the solutions have positive specific heat, which makes them thermodynamically stable.

Note:

16 pages, LaTex file, no figure, matches published version in PRD

black string: rotation
dimension: 4
temperature: Hawking
potential: electrostatic
gravitation: model
higher-order: 3
Einstein
anti-de Sitter
stability: thermodynamical
thermodynamics

References(47)

Figures(0)

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