Integrity report for Collective Winds of Massive Star Clusters as the Dominant PeVatrons for Galactic Cosmic Rays

A machine-verified record of the checks Pith has run against this paper: detector runs, findings, signed bundle events, and canonical identifiers.

arXiv:2605.31362 · pith:2026:A3XZDRWWCS2HCMZXYNOX743TZU

0Critical

0Advisory

5Detectors run

2026-06-04Last checked

Paper page arXiv integrity.json bundle.json

Detector runs

claim_evidence completed v1.0.0 · findings 0 · 2026-06-04 15:09:02.870777+00:00

shingle_duplication skipped v0.1.0 · findings 0 · 2026-06-01 21:50:16.461412+00:00

citation_quote_validity skipped v0.1.0 · findings 0 · 2026-06-01 09:50:48.633181+00:00

cited_work_retraction completed v1.0.0 · findings 0 · 2026-06-01 06:25:42.288187+00:00

ai_meta_artifact skipped v1.0.0 · findings 0 · 2026-06-01 02:35:04.721116+00:00

Findings

No public integrity findings for this paper.

Signed record

The machine-readable record for this paper lives at /pith/A3XZDRWW/integrity.json. Pith Number bundles also include signed pith.integrity.v1 events where a Pith Number exists.