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Paper Citation Record · LEDGER

On the physical significance of black hole quasinormal mode spectra instability

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2404.01374.

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

pith.paper-citation-record.v1
2404.01374 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 9 of 9 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 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T14:55:32.921961Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-01T20:06:12.143097Z

Reference resolution

0 of 0 outbound references displayed

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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 687cf8b9-6e72-435e-ae52-cd84c04deaf1 · inbound

Greybody factors, reflectionless scattering modes, and echoes of ultracompact horizonless objects cites this paper.

Greybody factors, reflectionless scattering modes, and echoes of ultracompact horizonless objects On the physical significance of black hole quasinormal mode spectra instability

Reference 70

Resolution
verified exact
arxiv_id, observed 2026-05-23T04:45:25.396837Z

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.

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Observation 83961054-b024-43c2-b519-dcc3208dc309 · inbound

Bound States of the Schwarzschild Black Hole cites this paper.

Bound States of the Schwarzschild Black Hole On the physical significance of black hole quasinormal mode spectra instability

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-07T14:55:32.921961Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:55:32.921961Z digest=sha256:255e1b76510a337009be470f70fc23b7266a27f48dbaed4e78e6507738ed10e3

Observation 83f8b5d2-536d-4a0a-a9fb-c9cfb4b63247 · inbound

Spectrum instability and greybody factor stability for parabolic approximation of Regge-Wheeler potential cites this paper.

Spectrum instability and greybody factor stability for parabolic approximation of Regge-Wheeler potential On the physical significance of black hole quasinormal mode spectra instability

Reference 19

Resolution
unresolved
no resolver link, observed 2026-08-07T13:41:51.067451Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T13:41:51.067451Z digest=sha256:faf4ff828e381cef35957d1ecb25fba42d30f1a93ec14787b8ca50d5a5422404

Observation d3350d1c-9239-4e14-8001-fcdf39dfe242 · inbound

Numerical study on the robustness of the stability for stable black holes cites this paper.

Numerical study on the robustness of the stability for stable black holes On the physical significance of black hole quasinormal mode spectra instability

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-07T05:36:04.929913Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T05:36:04.929913Z digest=sha256:d84b912062aecb22d3a606d41d109090988e5964506e5bfdde276de0cf4baf49

Observation 99949631-d27c-4b52-ba70-cb0463da3a2f · inbound

Reflectionless and echo modes in asymmetric Damour-Solodukhin wormholes cites this paper.

Reflectionless and echo modes in asymmetric Damour-Solodukhin wormholes On the physical significance of black hole quasinormal mode spectra instability

Reference 22

Resolution
verified exact
arxiv_id, observed 2026-05-18T01:35:36.266219Z

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=2026-05-18T01:34:45.033342Z digest=sha256:5058bf95d9d13c40baae514a0fbffee8dd44251444eb37956da82ce5b5297f29

Observation ba3cf397-60f7-4288-bf17-b5a836f56b60 · inbound

Excitation factors for horizonless compact objects: long-lived modes, echoes, and greybody factors cites this paper.

Excitation factors for horizonless compact objects: long-lived modes, echoes, and greybody factors On the physical significance of black hole quasinormal mode spectra instability

Reference 67

Resolution
verified exact
arxiv_id, observed 2026-05-17T23:22:13.114761Z

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=2026-05-17T23:20:36.030481Z digest=sha256:1bcdc6179586d27b9c8adbf10349a670c4ff09d75d221d0e15bb175d93b92bbf

Observation 85608426-b71c-4bb4-b6b3-64e91949306c · inbound

Spectral instability of parametrized black hole quasinormal modes in the high-overtone limit via the exact WKB analysis cites this paper.

Spectral instability of parametrized black hole quasinormal modes in the high-overtone limit via the exact WKB analysis On the physical significance of black hole quasinormal mode spectra instability

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-03T15:08:53.731565Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T15:08:53.731565Z digest=sha256:653b96312f86ce39721a0c4bfc54c4d296534c5362b06e4801dc295094809240

Observation 0ea8be85-8cd1-4fcd-8ccc-99379a0f101e · inbound

Cascading amplification of gravitational waves triggered by environment in dynamical Chern-Simons gravity cites this paper.

Cascading amplification of gravitational waves triggered by environment in dynamical Chern-Simons gravity On the physical significance of black hole quasinormal mode spectra instability

Reference 56

Resolution
verified exact
arxiv_id, observed 2026-07-01T20:06:12.144331Z

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=2026-06-28T21:36:52.517617Z digest=sha256:374e291d4866030824645d3f1b3de3982932edf6bf13aa9544e5d25c239ff76e

Observation 254f9555-9cce-4fc1-864a-90009f736a70 · inbound

Berry Picking: Random Wave Chaos Hierarchy for BPS Microstate Geometries cites this paper.

Berry Picking: Random Wave Chaos Hierarchy for BPS Microstate Geometries On the physical significance of black hole quasinormal mode spectra instability

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-04T04:35:28.430501Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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