Planck star phenomenology

Aurelien Barrau; Carlo Rovelli

Planck star phenomenology

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 1404.5821 v2 pith:KXJTWQEW submitted 2014-04-23 gr-qc astro-ph.COhep-phhep-th

Aurelien Barrau , Carlo Rovelli This is my paper

classification gr-qcastro-ph.COhep-phhep-th

keywords aroundblackcorepossibleseveralassumptionsburstscoming

verification ladder T0 review T1 audit T2 compute T3 formal

0 comments

read the original abstract

It is possible that black holes hide a core of Planckian density, sustained by quantum-gravitational pressure. As a black hole evaporates, the core remembers the initial mass and the final explosion occurs at macroscopic scale. We investigate possible phenomenological consequences of this idea. Under several rough assumptions, we estimate that up to several short gamma-ray bursts per day, around 10 MeV, with isotropic distribution, can be expected coming from a region of a few hundred light years around us.

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

Pseudo-Complex Gravity as a Geometric Resolution of the Black Hole Information Paradox
gr-qc 2025-06 reject novelty 4.0 of 10

Pseudo-complex gravity is applied to the black hole information paradox, but the central singularity-regularization claim fails for the paper's own metric.

Pith tools