Quantum spectrum of black holes

V.V.Kiselev

Quantum spectrum of black holes

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/0509038 v3 pith:445RLFX3 submitted 2005-09-12 gr-qc hep-th

V.V.Kiselev This is my paper

classification gr-qchep-th

keywords blackentropyholesrulespectrumallowsappropriatelycase

verification ladder T0 review T1 audit T2 compute T3 formal

0 comments

read the original abstract

The black hole as the thermodynamical system in equilibrium possesses the periodicity of motion in imaginary time, that allows us to formulate the quasi-classical rule of quantization. The rule yields the equidistant spectrum for the entropy of non-rotating black holes as well as for the appropriately scaled entropy in the case of rotation. We clarify and discuss a role of quasi-normal modes.

Discussion (0). Sign in to comment.

Forward citations

Cited by 1 Pith paper

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

Causal Space-Time Structure and non-Hausdorff Extension of Schwarzschild Black Hole Interior
gr-qc 2026-07 conditional novelty 5.0 of 10

Geodesic reflections fix causal cones under the horizon; the RN zero-charge limit yields an infinite band without closed cycles, plus a non-Hausdorff thermal interior extension.

Pith tools