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Thermodynamics of Regular Accelerating Black Holes

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arxiv 1612.04387 v2 pith:HRRSUATP submitted 2016-12-13 gr-qc hep-th

Marco Astorino This is my paper · ORCID
classification gr-qchep-th
keywords blackholemassthermodynamicsacceleratingc-metricformularegular
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Using the covariant phase space formalism, we compute the conserved charges for a solution, describing an accelerating and electrically charged Reissner-Nordstrom black hole. The metric is regular provided that the acceleration is driven by an external electric field, in spite of the usual string of the standard C-metric. The Smarr formula and the first law of black hole thermodynamics are fulfilled. The resulting mass has the same form of the Christodoulou-Ruffini mass formula. On the basis of these results, we can extrapolate the mass and thermodynamics of the rotating C-metric, which describes a Kerr-Newman-(A)dS black hole accelerated by a pulling string.

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Cited by 3 Pith papers

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

  1. Horizon-Evanescent Scalar Clouds from Coupled Rotation and Magnetic Fields around Black Holes

    gr-qc 2026-06 unverdicted novelty 7.0 of 10

    Magnetic fields around Kerr-Bertotti-Robinson black holes quench superradiant instability, enabling both classical synchronized scalar clouds and a new class of horizon-decaying stationary clouds.

  2. Thermodynamics of charged and accelerating black holes

    gr-qc 2025-01 conditional novelty 7.0 of 10

    For charged accelerating AdS black holes in Maxwell, ModMax, and RegMax theories, topological renormalization of the Euclidean action differs from holographic renormalization by 2πℓ²μ₊T when the total cosmic string te...

  3. Thermodynamics of Kerr-Bertotti-Robinson black hole

    gr-qc 2026-03 conditional novelty 5.0 of 10

    A consistent thermodynamics of the Kerr-Bertotti-Robinson black hole is constructed by adopting the Christodoulou-Ruffini mass relation, yielding a first law and Smarr formula without an explicit magnetic-field work term.

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