Paper Citation Record · LEDGER

Extended $\delta N$ formalism: Nonspatially Flat Separate Universe Approach

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2408.09964.

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

pith.paper-citation-record.v1
2408.09964 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 11 of 11 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T10:38:55.174456Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T17:20:01.416340Z

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 881ef80d-d00c-4479-b407-401ae004c6f2 · inbound

A complete analysis of inflation with piecewise quadratic potential cites this paper.

A complete analysis of inflation with piecewise quadratic potential Extended $\delta N$ formalism: Nonspatially Flat Separate Universe Approach

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-11T10:38:55.174456Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 737119af-f008-41b6-8583-a934e2928284 · inbound

How deep is the dip and how tall are the wiggles in inflationary power spectra? cites this paper.

How deep is the dip and how tall are the wiggles in inflationary power spectra? Extended $\delta N$ formalism: Nonspatially Flat Separate Universe Approach

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-10T15:00:43.958677Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation efb81405-7f41-42c3-8c56-70019b0f211f · 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 Extended $\delta N$ formalism: Nonspatially Flat Separate Universe Approach

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-07T12:38:10.844655Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 69735c59-2a58-4561-877b-011630f3df23 · inbound

Stochastic Inflation in Numerical Relativity cites this paper.

Stochastic Inflation in Numerical Relativity Extended $\delta N$ formalism: Nonspatially Flat Separate Universe Approach

Reference 49

Resolution: verified exact; arxiv_id, observed 2026-05-16T22:01:17.885705Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 6e125a52-4ba3-431b-963f-4380e336eae0 · 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 Extended $\delta N$ formalism: Nonspatially Flat Separate Universe Approach

Reference 120

Resolution: unresolved; no resolver link, observed 2026-08-03T06:50:38.962974Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 00dff4c7-5e8d-4179-bb87-ccc0570fbea9 · inbound

Nonperturbative stochastic inflation in perturbative dynamical background cites this paper.

Nonperturbative stochastic inflation in perturbative dynamical background Extended $\delta N$ formalism: Nonspatially Flat Separate Universe Approach

Reference 120

Resolution: metadata mismatch; arxiv_id, observed 2026-05-10T10:04:07.436000Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation c598b254-3045-4e88-831a-9422961a375e · 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 Extended $\delta N$ formalism: Nonspatially Flat Separate Universe Approach

Reference 65

Resolution: verified exact; arxiv_id, observed 2026-07-04T17:20:01.417912Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation d46ef02b-2b23-4d4e-8f4a-ff6c7678a687 · inbound

Superhorizon curvature perturbations in hybrid inflation revisited cites this paper.

Superhorizon curvature perturbations in hybrid inflation revisited Extended $\delta N$ formalism: Nonspatially Flat Separate Universe Approach

Reference 114

Resolution: verified exact; arxiv_id, observed 2026-06-30T14:14:46.390227Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 42a01f83-752b-4e89-8a99-c0dbba45e3b9 · inbound

Superhorizon curvature perturbations in hybrid inflation revisited cites this paper.

Superhorizon curvature perturbations in hybrid inflation revisited Extended $\delta N$ formalism: Nonspatially Flat Separate Universe Approach

Reference 114

Resolution: unresolved; no resolver link, observed 2026-07-14T17:01:04.250468Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 10ad1fc2-6656-4c22-a67f-cdb1c51a1823 · inbound

Compaction function in stochastic inflation: a \texttt{FOREST} of type I and II primordial black holes cites this paper.

Compaction function in stochastic inflation: a \texttt{FOREST} of type I and II primordial black holes Extended $\delta N$ formalism: Nonspatially Flat Separate Universe Approach

Reference 95

Resolution: verified exact; arxiv_id, observed 2026-06-30T14:24:45.657092Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation e22b6d41-333b-4ff3-8c1f-ead853c74318 · 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 Extended $\delta N$ formalism: Nonspatially Flat Separate Universe Approach

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-05T14:10:01.271464Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.