Photon spectra from final stages of a primordial black hole evaporation in different theoretical models

Edgar Bugaev; Peter Klimai; Valery Petkov

Photon spectra from final stages of a primordial black hole evaporation in different theoretical models

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 0706.3778 v1 pith:MQT6I7FT submitted 2007-06-26 astro-ph

Photon spectra from final stages of a primordial black hole evaporation in different theoretical models

Edgar Bugaev , Peter Klimai , Valery Petkov This is my paper

classification astro-ph

keywords theoreticalblackevaporationfinalgamma-rayholemodelsprimordial

verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved

0 comments

read the original abstract

Possibilities of an experimental search for gamma-ray bursts from primordial black hole (PBH) evaporations in space are reconsidered. It is argued that the corresponding constraints which can be obtained in experiments with cosmic ray detectors strongly depend on theoretical approach used for a description of the PBH evaporation process. Predictions of several theoretical models for gamma-ray spectra from final stages of PBH life (integrated over time) are given.

discussion (0)

Forward citations

Cited by 1 Pith paper

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

Constraints on Primordial Black Holes
astro-ph.CO 2020-02 accept novelty 4.0

Updated compilation shows PBHs are tightly constrained across 55 orders of magnitude in mass, ruling out dominant dark matter contributions except in narrow windows, with many limits carrying observational uncertainties.