Paper Citation Record · LEDGER

Cavity effect in the quasinormal mode spectrum of topological stars

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2305.14412.

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

pith.paper-citation-record.v1
2305.14412 v1

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 2026-08-10T06:31:04.303077+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T22:44:37.329440Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

29
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 447c673f-8927-4bee-934f-bf99d926b3e8 · inbound

Nonradial stability of topological stars cites this paper.

Nonradial stability of topological stars Cavity effect in the quasinormal mode spectrum of topological stars

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-08T22:44:37.329440Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b8c5479c-0549-42ea-b403-e7239882095c · inbound

Scattering angle in a Topological Star spacetime: a self-force approach cites this paper.

Scattering angle in a Topological Star spacetime: a self-force approach Cavity effect in the quasinormal mode spectrum of topological stars

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-07T10:39:20.470978Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1f10cdee-6ced-4517-b585-1da8d0629325 · inbound

Topological Stars and scalar wave equation: Exact resummation of the renormalized angular momentum in the eikonal limit cites this paper.

Topological Stars and scalar wave equation: Exact resummation of the renormalized angular momentum in the eikonal limit Cavity effect in the quasinormal mode spectrum of topological stars

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-07T00:32:36.500759Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7dbfab71-8e78-4eb1-a0b7-4233f76aaec0 · inbound

Gravitational Atoms from Topological Stars cites this paper.

Gravitational Atoms from Topological Stars Cavity effect in the quasinormal mode spectrum of topological stars

Reference 45

Resolution: verified exact; arxiv_id, observed 2026-05-17T22:50:25.790139Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 6e9c5ad1-6ad7-4c45-8258-bf76c89b0c33 · inbound

5d Schwarzschild-Tangherlini spacetime: MST-like formalism for a Reduced Confluent Heun Equation cites this paper.

5d Schwarzschild-Tangherlini spacetime: MST-like formalism for a Reduced Confluent Heun Equation Cavity effect in the quasinormal mode spectrum of topological stars

Reference 25

Resolution: metadata mismatch; local_arxiv, observed 2026-07-10T10:17:01.519792Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation d4e0e740-2312-4623-a2ea-86c1bdcf0215 · inbound

5d Schwarzschild-Tangherlini spacetime: MST-like formalism for a Reduced Confluent Heun Equation cites this paper.

5d Schwarzschild-Tangherlini spacetime: MST-like formalism for a Reduced Confluent Heun Equation Cavity effect in the quasinormal mode spectrum of topological stars

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-02T08:03:15.916779Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.