A Quantum Bound-State Description of Black Holes

Stefan Hofmann; Tehseen Rug

A Quantum Bound-State Description 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 1403.3224 v3 pith:YUWTLMV3 submitted 2014-03-13 hep-th astro-ph.HEgr-qc

Stefan Hofmann , Tehseen Rug This is my paper · ORCID

classification hep-thastro-ph.HEgr-qc

keywords blacknumberconstituentdescriptionholesquantumappliedblack-hole

verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments

read the original abstract

A relativistic framework for the description of bound states consisting of a large number of quantum constituents is presented, and applied to black-hole interiors. At the parton level, the constituent distribution, number and energy density inside black holes are calculated, and gauge corrections are discussed. A simple scaling relation between the black hole mass and constituent number is established.

Discussion (0). Continue with ORCID 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

Coherent quantum hairy black holes from gravitational decoupling: regularity, geodesics, and scalar ringdown
hep-th 2026-02 conditional novelty 6.0 of 10

Gaussian-smearing the gravitational-decoupling hairy black hole produces a regular core and modified photon rings, lensing, and a claimed but absent ringdown spectrum.

Pith tools