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Paper Citation Record · LEDGER

Nonlinear interacting cosmological models after Planck 2018 legacy release and the $H_0$ tension

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2002.03408.

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

pith.paper-citation-record.v1
2002.03408 v1

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 2026-08-10T06:31:04.303077+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T04:50:12.806970Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-01T16:45:51.313565Z

Reference resolution

0 of 0 outbound references displayed

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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 0ed11710-8517-4b15-8e36-62328cd60c8d · inbound

Interacting Early Dark Energy cites this paper.

Interacting Early Dark Energy Nonlinear interacting cosmological models after Planck 2018 legacy release and the $H_0$ tension

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-08T04:50:12.806970Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 8ac550a0-8fb3-4bf5-be45-ce2755d4df24 · inbound

Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints cites this paper.

Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints Nonlinear interacting cosmological models after Planck 2018 legacy release and the $H_0$ tension

Reference 104

Resolution
unresolved
no resolver link, observed 2026-08-06T18:14:17.871651Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T18:14:17.871651Z digest=sha256:b4d52f8f45e6654947a8a6b356744687eb818553a50d9c72bb5f278ef540b074

Observation bcd904ad-28f5-4518-a793-4391447798f3 · inbound

Dark sector interactions in the $w \rightarrow -1$ limit: velocity locking in pure momentum exchange models cites this paper.

Dark sector interactions in the $w \rightarrow -1$ limit: velocity locking in pure momentum exchange models Nonlinear interacting cosmological models after Planck 2018 legacy release and the $H_0$ tension

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-03T16:54:10.632166Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T16:54:10.632166Z digest=sha256:f9585e08e43f7e0d88981fd3cf665fda0bca6864cb3b39e7babc977cdb89b994

Observation 3cad0c00-2583-4c03-8c4f-23a39f44522f · inbound

Accelerating scaling solutions from dark matter particle creation cites this paper.

Accelerating scaling solutions from dark matter particle creation Nonlinear interacting cosmological models after Planck 2018 legacy release and the $H_0$ tension

Reference 84

Resolution
unresolved
no resolver link, observed 2026-07-12T18:37:05.978670Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T18:37:05.978670Z digest=sha256:792efc3a1685301851002949bb158f5b03d7cd5dca15d02fafb95a360d7d5cfa

Observation 26dd72f4-1fbc-4d2d-acc3-78e2b85e03cf · inbound

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions cites this paper.

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions Nonlinear interacting cosmological models after Planck 2018 legacy release and the $H_0$ tension

Reference 168

Resolution
verified exact
arxiv_id, observed 2026-07-01T16:45:51.314747Z

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=2026-06-29T20:17:08.107860Z digest=sha256:1d4c74d903a6e9fa8ea443df2fa02d64cf7fd126fb33dcd33f2de3539c3415b6

Observation e5cfaa5e-138e-469a-95c2-5efb97baf936 · inbound

Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions cites this paper.

Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions Nonlinear interacting cosmological models after Planck 2018 legacy release and the $H_0$ tension

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-01T02:46:22.870533Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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