Pith. sign in

REVIEW 3 cited by

Black Holes in Three Dimensional Topological Gravity

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

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 gr-qc/9410021 v1 pith:CYVUOCXE submitted 1994-10-17 gr-qc

S. Carlip , J. Gegenberg , R.B.Mann This is my paper · ORCID
classification gr-qc
keywords blacktopologicaldimensionalgravitymatterangularenergyentropy
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
read the original abstract

We investigate the black hole solution to (2+1)-dimensional gravity coupled to topological matter, with a vanishing cosmological constant. We calculate the total energy, angular momentum and entropy of the black hole in this model and compare with results obtained in Einstein gravity. We find that the theory with topological matter reverses the identification of energy and angular momentum with the parameters in the metric, compared with general relativity, and that the entropy is determined by the circumference of the inner rather than the outer horizon. We speculate that this results from the contribution of the topological matter fields to the conserved currents. We also briefly discuss two new possible (2+1)-dimensional black holes.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 3 Pith papers

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

  1. 3-dimensional charged black holes in $f({Q})$ gravity

    gr-qc 2025-06 conditional novelty 7.0 of 10

    New exact charged black hole solutions in (2+1)D f(Q) gravity with cubic form yield a novel AdS solution without GR counterpart, with multiple horizons, stable thermodynamics, and stable photon orbits.

  2. Thermodynamic Instabilities of Generalized Exotic BTZ Black Holes

    gr-qc 2019-08 accept novelty 6.0 of 10

    Generalized exotic BTZ black holes can have positive specific heat at constant volume despite violating the reverse isoperimetric inequality, countering a recent conjecture.

  3. 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.

Pith tools