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Paper Citation Record · LEDGER

Slowly Rotating Black Holes in Einsteinian Quartic Gravities

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2302.10290.

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

pith.paper-citation-record.v1
2302.10290 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 2026-08-22T06:32:14.747728+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T04:38:45.772814Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T10:25:59.950322Z

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 c36c4925-1cd2-4ba1-bf57-eed738be7007 · inbound

Slowly rotating black hole solution to Einstein-Bel-Robinson gravity cites this paper.

Slowly rotating black hole solution to Einstein-Bel-Robinson gravity Slowly Rotating Black Holes in Einsteinian Quartic Gravities

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-16T04:38:45.772814Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:38:45.772814Z digest=sha256:5a6fba49a36f56950108858edfc57a1c4970cd1d9995e6a8b90237c26bf4ee73

Observation a0904dfe-2265-4bcb-817a-f054772167ca · inbound

Cosmologically viable non-polynomial quasi-topological gravity: explicit models, $\Lambda$CDM limit and observational constraints cites this paper.

Cosmologically viable non-polynomial quasi-topological gravity: explicit models, $\Lambda$CDM limit and observational constraints Slowly Rotating Black Holes in Einsteinian Quartic Gravities

Reference 61

Resolution
verified exact
arxiv_id, observed 2026-05-11T10:25:59.952524Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-10T15:30:57.195869Z digest=sha256:462793e28d4e2ef84e487f58104888f243cb84dca01aa529a8c5e2b070c63158