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Paper Citation Record · LEDGER

How deep is the dip and how tall are the wiggles in inflationary power spectra?

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2501.14681.

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

pith.paper-citation-record.v1
2501.14681 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T14:59:21.676759Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T09:36:49.208797Z

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 548d08be-0c44-41a7-bb14-ae2732fd71c8 · inbound

The Irrelevance of Primordial Black Hole Clustering in the LVK mass range cites this paper.

The Irrelevance of Primordial Black Hole Clustering in the LVK mass range How deep is the dip and how tall are the wiggles in inflationary power spectra?

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-09T14:59:21.676759Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T14:59:21.676759Z digest=sha256:e05531f569106cf2689818d5765f2428d771e5a471012fe94d7ed72c07ae0ef8

Observation 80012bad-f189-4827-a05e-b11acf06caf0 · inbound

$\delta n$ formalism: A new formulation for the probability density of the curvature perturbation cites this paper.

$\delta n$ formalism: A new formulation for the probability density of the curvature perturbation How deep is the dip and how tall are the wiggles in inflationary power spectra?

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-07T12:38:10.065941Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T12:38:10.065941Z digest=sha256:c5dbba7b912422dfbf6636fe1ea493a6c6a8e3592d462729a465239c392e1b7b

Observation 70fc755b-aa4c-46b5-9e34-7d08e49dcee4 · inbound

Axion USR Inflation cites this paper.

Axion USR Inflation How deep is the dip and how tall are the wiggles in inflationary power spectra?

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-06T20:32:39.169729Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T20:32:39.169729Z digest=sha256:63f2d9350f98a39b624bacd5559df4c6054febaafc7116c987124ec8c35e27ce

Observation 5c3ef197-107c-4b50-ba03-d68eedf2f34c · inbound

When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity cites this paper.

When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity How deep is the dip and how tall are the wiggles in inflationary power spectra?

Reference 110

Resolution
unresolved
no resolver link, observed 2026-08-03T06:50:37.317033Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T06:50:37.317033Z digest=sha256:396a6cd6a7d9d3a4da8fbc02f0bb5b382c61eda8d5224b96401a08287d601cf8

Observation bf09f49e-dd07-4f6a-8e48-60476d1fa5ec · inbound

Evolution of Linear Perturbations under Time-Dependent Hubble Friction I: SR-USR-SR Inflation cites this paper.

Evolution of Linear Perturbations under Time-Dependent Hubble Friction I: SR-USR-SR Inflation How deep is the dip and how tall are the wiggles in inflationary power spectra?

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-02T23:43:40.289602Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T23:43:40.289602Z digest=sha256:1013225ed1679b140c75756699b38248fb63657e876de62d7d90f5d49e971666

Observation aba9cf37-aa50-4c7e-a249-bd7eb33e6190 · inbound

UV artefacts in ultra-slow-roll models of inflation cites this paper.

UV artefacts in ultra-slow-roll models of inflation How deep is the dip and how tall are the wiggles in inflationary power spectra?

Reference 57

Resolution
verified exact
arxiv_id, observed 2026-07-01T17:45:51.249303Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-06-29T03:21:58.865846Z digest=sha256:0fd89045bf6e4d0b19269282dcc73a657ff9de2916e08bdde2c9283779b50ff9

Observation 56dacb1a-5e6d-4d4a-8ef3-1bbd7d7fc2cd · inbound

Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension cites this paper.

Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension How deep is the dip and how tall are the wiggles in inflationary power spectra?

Reference 76

Resolution
verified exact
arxiv_id, observed 2026-07-01T11:25:45.809164Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-07-01T04:31:47.886338Z digest=sha256:483d64eab427c380fea60dd7638acb78bbc4d4774fee530e7bdba8872aec3183

Observation dde02a65-a208-4acb-80ec-19b0c4c02ef8 · inbound

Hidden quantum-informatic symmetries of quasi-de Sitter backgrounds cites this paper.

Hidden quantum-informatic symmetries of quasi-de Sitter backgrounds How deep is the dip and how tall are the wiggles in inflationary power spectra?

Reference 46

Resolution
verified exact
arxiv_id, observed 2026-07-02T09:36:49.210703Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-07-02T09:32:58.559293Z digest=sha256:a485f0b1edea2a41bdaab7839262f7465bb306e11f8d7338386fd10736878b5b