Pith. sign in

Paper Citation Record · LEDGER

The attractive behaviour of ultra-slow-roll inflation

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1806.09553.

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

pith.paper-citation-record.v1
1806.09553 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 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 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T14:10:00.821518Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-04T17:20:01.288514Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

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 26ac50a1-26f4-4bbd-947a-8465196190d6 · inbound

Deviations from Gaussian White Noise in Stochastic Inflation cites this paper.

Deviations from Gaussian White Noise in Stochastic Inflation The attractive behaviour of ultra-slow-roll inflation

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-03T15:31:52.025816Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T15:31:52.025816Z digest=sha256:f74c447d3229252c37b500ea56a2fc9966f7fa1b7056ec53e7264f6d5037a0a7

Observation 3c9f09c5-c34a-4c4d-9bc0-5b0775dcd472 · 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 The attractive behaviour of ultra-slow-roll inflation

Reference 106

Resolution
unresolved
no resolver link, observed 2026-08-03T06:50:36.613715Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T06:50:36.613715Z digest=sha256:0dc110824688f26fec79a8b45d52b358a0c5e640c3b40cb087e07116f32331a4

Observation 1bb00951-2b49-461b-b013-aa71ddd055a8 · 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 The attractive behaviour of ultra-slow-roll inflation

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-02T23:43:30.999621Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T23:43:30.999621Z digest=sha256:5dae24a77a2432d59da3e50604dc10aa19d6557a6821972901f96d3dee0aee78

Observation 3736c08a-e773-4532-8a5b-8b1ea1f057ca · inbound

Constant-Roll Inflation: Analytical Formulae for Power Spectrum and Implications for Induced Gravitational Waves cites this paper.

Constant-Roll Inflation: Analytical Formulae for Power Spectrum and Implications for Induced Gravitational Waves The attractive behaviour of ultra-slow-roll inflation

Reference 47

Resolution
verified exact
local_arxiv, observed 2026-07-04T17:20:01.289892Z

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.

source=pdf_text observed=2026-06-25T23:44:36.834692Z digest=sha256:b0bcb68eccc964bd7cce16df37372088ad62c09cbfa0c79e39ee80234ca1d9ac

Observation b660a217-0f68-4213-ae0d-ae556383f3ca · inbound

How Dilatation Invariance Suppresses Loop Corrections to Curvature Perturbations on CMB Scales cites this paper.

How Dilatation Invariance Suppresses Loop Corrections to Curvature Perturbations on CMB Scales The attractive behaviour of ultra-slow-roll inflation

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-05T14:10:00.821518Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T14:10:00.821518Z digest=sha256:0ec1cd65c3176e228a701a6a250843ccefbead01c2bc95513ae85f760e0d3ca3