Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Limitations of Pseudo-Newtonian approach in studying the accretion flow around Kerr black hole
As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1806.08481.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T20:36:18.190951Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-28T09:21:48.921946Z
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 04d80fff-49da-4afc-90d1-c728483be19e · inbound
Relativistic accretion and burdened primordial black holes cites this paper.
Relativistic accretion and burdened primordial black holes Limitations of Pseudo-Newtonian approach in studying the accretion flow around Kerr black hole
Reference 90
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T20:36:18.190951Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 257a9764-179d-4a21-8e9d-31dbf2865264 · inbound
Revisiting PBH accretion, evaporation and their cosmological consequences cites this paper.
Revisiting PBH accretion, evaporation and their cosmological consequences Limitations of Pseudo-Newtonian approach in studying the accretion flow around Kerr black hole
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T18:08:28.196341Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8c6727c4-2788-4102-8aca-52b1682f041a · 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 Limitations of Pseudo-Newtonian approach in studying the accretion flow around Kerr black hole
Reference 126
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T09:21:48.924379Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.