Paper Citation Record · LEDGER

Smoothing and flattening the universe through slow contraction versus inflation

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2404.00867.

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

pith.paper-citation-record.v1
2404.00867 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 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 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T19:35:28.409921Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-08T06:24:42.206442Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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malformed identifier0
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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 43862244-a3c0-43f7-a3ca-ac3a1c27a919 · inbound

Fully viable DHOST bounce with extra scalar cites this paper.

Fully viable DHOST bounce with extra scalar Smoothing and flattening the universe through slow contraction versus inflation

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-10T19:35:28.409921Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d21109be-bd75-41b0-bb8e-76875a7e8215 · inbound

Inflaton Dynamics in Higher-Derivative Scalar-Tensor Theories of Gravity cites this paper.

Inflaton Dynamics in Higher-Derivative Scalar-Tensor Theories of Gravity Smoothing and flattening the universe through slow contraction versus inflation

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-07T14:44:09.452656Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 79d34966-7d99-4e29-8a10-81c206aa9fc2 · inbound

Probability of the Initial Conditions for Inflation and Slow Contraction cites this paper.

Probability of the Initial Conditions for Inflation and Slow Contraction Smoothing and flattening the universe through slow contraction versus inflation

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-07T13:11:45.394673Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 43e972f4-54c4-4095-af3c-69ff04cf4f30 · inbound

Effects of the ekpyrotic mechanism on inflationary phase in loop quantum cosmologies cites this paper.

Effects of the ekpyrotic mechanism on inflationary phase in loop quantum cosmologies Smoothing and flattening the universe through slow contraction versus inflation

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-04T11:57:27.111767Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 02c80ea8-8b13-4f96-99a5-09723eccc830 · inbound

Accelerated expansion of the universe purely driven by scalar field fluctuations cites this paper.

Accelerated expansion of the universe purely driven by scalar field fluctuations Smoothing and flattening the universe through slow contraction versus inflation

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-03T01:24:43.083277Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2d9cf8ef-e81b-4a9e-8612-58a13fe7ac0d · inbound

Non-Gaussianity and Strong-Coupling Problem in a Two-Field DHOST Bouncing Model cites this paper.

Non-Gaussianity and Strong-Coupling Problem in a Two-Field DHOST Bouncing Model Smoothing and flattening the universe through slow contraction versus inflation

Reference 28

Resolution: verified exact; arxiv_id, observed 2026-07-02T04:16:36.161214Z

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 75f12982-ab1a-4ae4-b894-0064f4932f67 · inbound

Starting inflation in asymptotically flat spacetimes cites this paper.

Starting inflation in asymptotically flat spacetimes Smoothing and flattening the universe through slow contraction versus inflation

Reference 26

Resolution: verified exact; local_arxiv, observed 2026-07-08T06:24:42.208210Z

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.