Paper Citation Record · LEDGER

Description of Pseudo-Newtonian Potential for the Relativistic Accretion Disk around Kerr Black Holes

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0205475.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
astro-ph/0205475 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:34:44.354955Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-06-28T09:21:48.913234Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 251be273-e00a-44ff-ab52-37b579b7bb87 · inbound

Threshold Drop in Accretion Density if Dark Energy is Accreting onto a Supermassive Black Hole cites this paper.

Threshold Drop in Accretion Density if Dark Energy is Accreting onto a Supermassive Black Hole Description of Pseudo-Newtonian Potential for the Relativistic Accretion Disk around Kerr Black Holes

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-14T14:34:44.354955Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 78de10cf-5dc3-42e8-86c3-5c06c3214a14 · inbound

Simulation based parameter space for shock in transonic, sub-Keplerian accretion flow onto non-rotating black holes cites this paper.

Simulation based parameter space for shock in transonic, sub-Keplerian accretion flow onto non-rotating black holes Description of Pseudo-Newtonian Potential for the Relativistic Accretion Disk around Kerr Black Holes

Reference 124

Resolution: verified exact; local_arxiv, observed 2026-06-28T09:21:48.915430Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.