Integrity report for How plasma coupling and convective-zone depth shape the rotation of solar-mass stars

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

arXiv:2605.12354

0Critical

0Advisory

4Detectors run

2026-05-26Last checked

Paper page arXiv integrity.json

Detector runs

ai_meta_artifact completed v1.0.0 · findings 0 · 2026-05-26 14:41:59.160584+00:00

doi_title_agreement completed v1.0.0 · findings 0 · 2026-05-20 13:31:25.222198+00:00

doi_compliance completed v1.0.0 · findings 0 · 2026-05-20 09:56:36.240202+00:00

claim_evidence completed v1.0.0 · findings 0 · 2026-05-19 22:41:58.248445+00:00

Findings

No public integrity findings for this paper.

Signed record

The machine-readable record for this paper lives at /pith/2605.12354/integrity.json. Pith Number bundles also include signed pith.integrity.v1 events where a Pith Number exists.