Paper Citation Record · LEDGER

Zero Energy Rotating Accretion Flows near a Black Hole

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/9607051.

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

pith.paper-citation-record.v1
astro-ph/9607051 v1

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 2026-08-14T06:32:32.682623+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T11:45:37.807717Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

132
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 82db77de-87bb-4ccb-83df-80ffa3b74c79 · inbound

A general relativistic hydrodynamic simulation code for studying advective, sub-Keplerian accretion flow onto black holes cites this paper.

A general relativistic hydrodynamic simulation code for studying advective, sub-Keplerian accretion flow onto black holes Zero Energy Rotating Accretion Flows near a Black Hole

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-07T11:45:37.807717Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e824fb78-6213-446d-a48c-76e139566de0 · 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 Zero Energy Rotating Accretion Flows near a Black Hole

Reference 76

Resolution: verified exact; local_arxiv, observed 2026-06-28T09:21:48.827217Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.