Integrity report for Slowly rotating condensate dark stars beyond the mean-field approximation

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

arXiv:2607.06898 · pith:2026:GOWKSQNO2UNG6VJ3ALEM2REGO2

0Critical

0Advisory

5Detectors run

2026-07-10Last checked

Paper page arXiv integrity.json bundle.json

Detector runs

claim_evidence completed v1.0.0 · findings 0 · 2026-07-10 08:42:26.418046+00:00

doi_title_agreement completed v1.0.0 · findings 0 · 2026-07-10 00:01:06.414952+00:00

doi_compliance completed v1.0.0 · findings 0 · 2026-07-09 23:35:15.075708+00:00

cited_work_retraction completed v1.0.0 · findings 0 · 2026-07-09 20:18:34.717000+00:00

ai_meta_artifact skipped v1.0.0 · findings 0 · 2026-07-09 08:49:24.379875+00:00

Findings

No public integrity findings for this paper.

Signed record

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