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Paper Citation Record · LEDGER

Slow rotation black hole perturbation theory

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2305.19313.

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

pith.paper-citation-record.v1
2305.19313 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T11:08:24.832592Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-16T12:47:54.179146Z

Reference resolution

0 of 0 outbound references displayed

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Outbound references

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Pith citing papers

Observation a8f68f6f-c4f8-457e-b2bc-e460b929478f · inbound

Axial quasi-normal modes of slowly rotating black holes in dynamical Chern-Simons gravity to second-order in spin and coupling cites this paper.

Axial quasi-normal modes of slowly rotating black holes in dynamical Chern-Simons gravity to second-order in spin and coupling Slow rotation black hole perturbation theory

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-07T11:08:24.832592Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T11:08:24.832592Z digest=sha256:c965bb3107d4b9d80c8d6411f1d18a3fa5e5c12c9e6ec3a282e4100ad4737608

Observation e6a4732f-fe26-4564-8af0-99b83c561503 · inbound

Quasinormal modes and their excitation beyond general relativity. II: isospectrality loss in gravitational waveforms cites this paper.

Quasinormal modes and their excitation beyond general relativity. II: isospectrality loss in gravitational waveforms Slow rotation black hole perturbation theory

Reference 28

Resolution
verified exact
arxiv_id, observed 2026-05-16T12:47:54.182270Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-05-16T12:43:57.054496Z digest=sha256:d16fb52745a446445d5717ca8639109033131ff0cb19a342086c3ab175cb54b5

Observation 4dddc1e2-935d-4f9f-bb74-93a528ca8a9f · inbound

Gravitational electric-magnetic duality at the light ring and quasinormal mode isospectrality in effective field theories cites this paper.

Gravitational electric-magnetic duality at the light ring and quasinormal mode isospectrality in effective field theories Slow rotation black hole perturbation theory

Reference 27

Resolution
verified exact
arxiv_id, observed 2026-05-11T17:11:18.284535Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-05-08T17:48:10.296695Z digest=sha256:49fdaca19d3392f55e9b542403cba03b0181519d969a5a4f16b101559cb8e43c

Observation c0cf5dc1-d3a2-458f-91b8-7c0b5a8a7192 · inbound

Unifying the Regge-Wheeler-Zerilli and Bardeen-Press-Teukolsky formalisms on spherical backgrounds cites this paper.

Unifying the Regge-Wheeler-Zerilli and Bardeen-Press-Teukolsky formalisms on spherical backgrounds Slow rotation black hole perturbation theory

Reference 89

Resolution
verified exact
arxiv_id, observed 2026-05-09T06:05:35.683439Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-05-08T18:56:09.664711Z digest=sha256:c8e7cd30ac458be5bfbfe36af9a0c750426a74ae6a1a6dc951dad2abbeed3c63

Observation 3cc2d3c9-0a03-47f2-903a-b6a38ae3da8b · inbound

Separating the linearized Einstein equations in Kerr cites this paper.

Separating the linearized Einstein equations in Kerr Slow rotation black hole perturbation theory

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-01T20:40:39.003795Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T20:40:39.003795Z digest=sha256:7bfc8abf43bf49e276aa791605d0281854cc7463a8ce2be9468c067b4c8e2cdf