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 6 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 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T12:43:01.326049Z

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

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 0308f428-75f7-4fbb-99cb-c8c181d7478f · inbound

Is the formation of primordial black holes from single-field inflation compatible with standard cosmology? cites this paper.

Is the formation of primordial black holes from single-field inflation compatible with standard cosmology? The attractive behaviour of ultra-slow-roll inflation

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-11T12:43:01.326049Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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.

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.

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.

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 2026-08-11T06:34:44.6726+00:00.

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.