Integrity report for Neutron stars more compact than black holes in quasi-topological gravity: Equilibrium configurations and radial stability

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

arXiv:2605.19731 · pith:2026:C67QUOQTTKLG3V3NGXLOWE43FG

0Critical

0Advisory

6Detectors run

2026-05-21Last checked

Paper page arXiv integrity.json bundle.json

Detector runs

doi_compliance completed v1.0.0 · findings 0 · 2026-05-21 04:36:25.766134+00:00

doi_title_agreement completed v1.0.0 · findings 0 · 2026-05-21 04:31:37.331171+00:00

claim_evidence completed v1.0.0 · findings 0 · 2026-05-21 03:42:20.452764+00:00

citation_quote_validity completed v0.1.0 · findings 0 · 2026-05-20 11:50:17.098786+00:00

cited_work_retraction completed v1.0.0 · findings 0 · 2026-05-20 08:52:00.967284+00:00

ai_meta_artifact skipped v1.0.0 · findings 0 · 2026-05-20 01:33:29.465463+00:00

Findings

No public integrity findings for this paper.

Signed record

The machine-readable record for this paper lives at /pith/C67QUOQT/integrity.json. Pith Number bundles also include signed pith.integrity.v1 events where a Pith Number exists.