Paper Citation Record · LEDGER

How to tell the shape of a wormhole by its quasinormal modes

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1805.04718.

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

pith.paper-citation-record.v1
1805.04718 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T13:24:44.527025Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-14T22:19:31.234437Z

Reference resolution

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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 420c37ef-559b-47ac-8f34-e3c4a9f7d807 · inbound

Quasinormal modes and grey-body factors of Morris-Thorne wormholes cites this paper.

Quasinormal modes and grey-body factors of Morris-Thorne wormholes How to tell the shape of a wormhole by its quasinormal modes

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-11T13:24:44.527025Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b559c35d-7368-42c4-9387-3ee5637c509e · inbound

Transition from Regular Black Holes to Wormholes in Covariant Effective Quantum Gravity: Scattering, Quasinormal Modes, and Hawking Radiation cites this paper.

Transition from Regular Black Holes to Wormholes in Covariant Effective Quantum Gravity: Scattering, Quasinormal Modes, and Hawking Radiation How to tell the shape of a wormhole by its quasinormal modes

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-08T18:28:50.699636Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4690166b-2702-4442-a036-6b1f2adac9ae · inbound

Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter cites this paper.

Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter How to tell the shape of a wormhole by its quasinormal modes

Reference 91

Resolution: verified exact; arxiv_id, observed 2026-05-11T22:51:23.676352Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation b656183b-4a71-4ec9-bc69-b4e79c1bef2c · inbound

Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter cites this paper.

Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter How to tell the shape of a wormhole by its quasinormal modes

Reference 91

Resolution: verified exact; local_arxiv, observed 2026-05-14T22:19:31.237796Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 8138db2f-79d6-40f8-856e-2a7b72d308f8 · inbound

Massive scalar quasinormal modes of an asymptotically flat regular black hole supported by a phantom Dirac--Born--Infeld field cites this paper.

Massive scalar quasinormal modes of an asymptotically flat regular black hole supported by a phantom Dirac--Born--Infeld field How to tell the shape of a wormhole by its quasinormal modes

Reference 129

Resolution: verified exact; arxiv_id, observed 2026-05-12T00:21:19.940253Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation dc53ba20-2e9d-4468-8283-0e7194d6546e · inbound

Bardeen spacetime as quantum corrected black hole: Grey-body factors and quasinormal modes of gravitational perturbations cites this paper.

Bardeen spacetime as quantum corrected black hole: Grey-body factors and quasinormal modes of gravitational perturbations How to tell the shape of a wormhole by its quasinormal modes

Reference 89

Resolution: verified exact; arxiv_id, observed 2026-05-13T02:42:09.030066Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.