Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
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.
Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-09T14:59:21.676759Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-02T09:36:49.208797Z
0 of 0 outbound references displayed
External citation measurements
No source-named external measurement is stored.
No outbound reference observations are available for this paper version.
Observation 548d08be-0c44-41a7-bb14-ae2732fd71c8 · inbound
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
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 80012bad-f189-4827-a05e-b11acf06caf0 · inbound
$\delta n$ 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
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 70fc755b-aa4c-46b5-9e34-7d08e49dcee4 · inbound
Axion USR Inflation How deep is the dip and how tall are the wiggles in inflationary power spectra?
Reference 94
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5c3ef197-107c-4b50-ba03-d68eedf2f34c · inbound
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
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bf09f49e-dd07-4f6a-8e48-60476d1fa5ec · inbound
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
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation aba9cf37-aa50-4c7e-a249-bd7eb33e6190 · inbound
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
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.
Observation 56dacb1a-5e6d-4d4a-8ef3-1bbd7d7fc2cd · inbound
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
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.
Observation dde02a65-a208-4acb-80ec-19b0c4c02ef8 · inbound
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
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.