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Black Hole Thermodynamics with Conical Defects

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arxiv 1702.00490 v2 pith:LBOZRRBB submitted 2017-02-01 hep-th gr-qc

Michael Appels , Ruth Gregory , David Kubiznak This is my paper · ORCID
classification hep-thgr-qc
keywords blackconicalholeholesthermodynamicacceleratingdefectsspace
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Recently we have shown [1604.08812] how to formulate a thermodynamic first law for a single (charged) accelerated black hole in AdS space by fixing the conical deficit angles present in the spacetime. Here we show how to generalise this result, formulating thermodynamics for black holes with varying conical deficits. We derive a new potential for the varying tension defects: the "thermodynamic length", both for accelerating and static black holes. We discuss possible physical processes in which the tension of a string ending on a black hole might vary, and also map out the thermodynamic phase space of accelerating black holes and explore their critical phenomena.

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Cited by 6 Pith papers

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

  1. Resolved Maxwell-Boundary Normal Forms and Exact Reentrant Scaling in Accelerating AdS Black Holes

    hep-th 2026-07 accept novelty 8.0 of 10

    The charged accelerating AdS black hole has an exact reentrant-turning locus for all 0<µ<0.2026, with the pressure and temperature windows vanishing as µ⁴ and µ³ and a universal blow-up profile bT = 2√bP − bP.

  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. Multihair thermodynamics of Kerr-Newman-NUT-AdS$_4$ spacetimes

    hep-th 2026-06 unverdicted novelty 6.0 of 10

    Derives a Christodoulou-Ruffini-type squared-mass formula for Kerr-Newman-NUT-AdS4 using secondary NUT hairs J_n and N, then verifies the first law and Smarr relation by differentiation.

  4. Radiation in Fluid/Gravity and the Flat Limit

    hep-th 2025-08 unverdicted novelty 6.0 of 10

    Establishes a holographic link between bulk gravitational radiation and dissipative corrections plus entropy production in boundary fluids, then constructs Carrollian analogues and celestial observables in the flat limit.

  5. Charged accelerating black hole in $f(R)$ gravity

    hep-th 2019-08 conditional novelty 6.0 of 10

    A charged, slowly accelerating AdS black hole in f(R) gravity is constructed and shown to satisfy a first law, with an eta-dependent thermodynamic volume and a reverse isoperimetric inequality that allows super-entrop...

  6. Metallic transports from accelerating black holes

    hep-th 2024-11 conditional novelty 5.0 of 10

    For accelerating AdS black holes, a holographic D-brane calculation gives resistivity scaling T^{2/3} and T^{-1/3}, interpreted as a z=3 quantum liquid phase.

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