Paper Citation Record · LEDGER

A Higher Dimensional Stationary Rotating Black Hole Must be Axisymmetric

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:gr-qc/0605106.

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

pith.paper-citation-record.v1
gr-qc/0605106 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T15:44:29.246385Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-29T14:53:31.838245Z

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 fdf7aea0-42cc-48e5-a376-c4fd3c76c0bf · inbound

Superradiance -- the 2020 Edition cites this paper.

Superradiance -- the 2020 Edition A Higher Dimensional Stationary Rotating Black Hole Must be Axisymmetric

Reference 297

Resolution: verified exact; local_arxiv, observed 2026-05-16T20:42:01.261351Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 7fa6bb65-dd73-4d7f-bc76-a1273db508cc · inbound

Gravitational Effective Field Theories and Black Hole Mechanics cites this paper.

Gravitational Effective Field Theories and Black Hole Mechanics A Higher Dimensional Stationary Rotating Black Hole Must be Axisymmetric

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-12T15:44:29.246385Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f9bc01ba-4e18-427a-b5e9-ba92320650d0 · inbound

The First Law and Weak Cosmic Censorship for de Sitter Black Holes cites this paper.

The First Law and Weak Cosmic Censorship for de Sitter Black Holes A Higher Dimensional Stationary Rotating Black Hole Must be Axisymmetric

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-12T10:19:55.905404Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c880f44b-8c91-499f-9180-e10b69496bc3 · inbound

Axions Create Singularities on Extremal Horizons cites this paper.

Axions Create Singularities on Extremal Horizons A Higher Dimensional Stationary Rotating Black Hole Must be Axisymmetric

Reference 28

Resolution: verified exact; local_arxiv, observed 2026-06-29T14:53:31.839514Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.