Pith. sign in

REVIEW 2 cited by

Holographic heat engines: general considerations and rotating black holes

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1704.02314 v1 pith:VV7I4DZN submitted 2017-04-07 hep-th gr-qc

classification hep-thgr-qc
keywords blackefficiencyenginesheatholesconsiderationscycledimension
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
read the original abstract

We perform the first study of holographic heat engines where the working material is a rotating black hole, obtaining exact results for the efficiency of a rectangular engine cycle. We also make general considerations in the context of benchmarking these engines on circular cycles. We find an exact expression that is valid for black holes with vanishing specific heat at constant volume and derive an upper bound, below the Carnot efficiency and independent of spacetime dimension, which holds for any black hole of this kind. We illustrate our results with applications to a variety of black holes, noting the effects of spacetime dimension, rotation, and higher curvature corrections on the efficiency of the cycle.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 2 Pith papers

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

  1. Holographic heat engines for Schwarzschild black holes

    hep-th 2026-07 accept novelty 6.0 of 10

    Schwarzschild black holes in finite cavities yield fixed-theory reversible heat engines with exact cycle efficiencies that probe quasi-local equations of state.

  2. Effects of quantum corrections on the criticality and efficiency of black holes surrounded by a perfect fluid

    gr-qc 2019-08 conditional novelty 5.0 of 10

    For a quantum-corrected Schwarzschild black hole in a Kiselev perfect fluid, first-order PV criticality appears when the fluid parameter satisfies omega > -1/3 and omega differs from zero, while a Hawking-Page-like tr...

Pith tools