Models for unitary black hole disintegration

Steven B. Giddings

Models for unitary black hole disintegration

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 1108.2015 v2 pith:FPVTUD53 submitted 2011-08-09 hep-th gr-qc

Steven B. Giddings This is my paper · ORCID

classification hep-thgr-qc

keywords blackholemodelsunitarydescriptiondisintegrationeffectiveevolution

verification ladder T0 review T1 audit T2 compute T3 formal

0 comments

read the original abstract

Simple models for unitary black hole evolution are given in an effective Hilbert-space description, parameterizing a possible minimal relaxation of locality, with respect to semiclassical black hole geometry.

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

Quantum circuit simulation of black hole evaporation and Maxwell demon interpretation
gr-qc 2025-05 reject novelty 4.0 of 10

A Maxwell demon inside a black hole is used in a quantum circuit to steer outside qubits via a wormhole, claimed to simulate Hawking radiation entanglement while dissipating energy of order the black hole entropy.

Pith tools