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Integrity report for Supercritical Accretion onto a Non-Magnetized Neutron Star: Why is it Feasible?

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

arXiv:1712.02068 · pith:2017:O6T5C6ZMLLJQJT52N6N4CM4G53

0Critical
0Advisory
0Detectors run
Last checked

Paper page arXiv integrity.json bundle.json

Detector runs

Findings

No public integrity findings for this paper.

Signed record

The machine-readable record for this paper lives at /pith/O6T5C6ZM/integrity.json. Pith Number bundles also include signed pith.integrity.v1 events where a Pith Number exists.