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Paper Citation Record · LEDGER

Parametric and nonparametric methods hint dark energy evolution

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2111.08289.

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

pith.paper-citation-record.v1
2111.08289 v3

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measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T14:43:16.291542Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-24T03:53:54.253655Z

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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 8290ea20-605b-4783-a89e-1ba8fe522a94 · inbound

$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity cites this paper.

$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity Parametric and nonparametric methods hint dark energy evolution

Reference 109

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verified exact
arxiv_id, observed 2026-05-24T03:53:54.256449Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation daccc779-c4ac-434f-8a6f-3b031c952f87 · inbound

Model-independent calibration of Gamma-Ray Bursts with neural networks cites this paper.

Model-independent calibration of Gamma-Ray Bursts with neural networks Parametric and nonparametric methods hint dark energy evolution

Reference 66

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verified exact
arxiv_id, observed 2026-05-23T17:55:44.454441Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation a5403a46-fa4c-4851-8f03-db6170bf08e0 · inbound

Cosmo-Learn: code for learning cosmology using different methods and mock data cites this paper.

Cosmo-Learn: code for learning cosmology using different methods and mock data Parametric and nonparametric methods hint dark energy evolution

Reference 40

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no resolver link, observed 2026-08-05T14:43:16.291542Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 7fb754a8-0f8d-4a83-9a11-a949166ad05e · inbound

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM cites this paper.

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM Parametric and nonparametric methods hint dark energy evolution

Reference 168

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verified exact
arxiv_id, observed 2026-05-18T04:50:55.461170Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation b5ef88b5-0271-4a56-ac68-f14e8381326f · inbound

Evidence of dynamical dark energy found via the DESI DR2 Lyman$\alpha$ forest cites this paper.

Evidence of dynamical dark energy found via the DESI DR2 Lyman$\alpha$ forest Parametric and nonparametric methods hint dark energy evolution

Reference 14

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unresolved
no resolver link, observed 2026-08-04T08:19:07.748276Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 9d792b56-9683-4603-9708-5f3d140827e0 · inbound

Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework cites this paper.

Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework Parametric and nonparametric methods hint dark energy evolution

Reference 120

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verified exact
arxiv_id, observed 2026-05-21T13:30:12.072061Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation c633e846-f087-4866-9a73-9c760dffe97c · inbound

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families cites this paper.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Parametric and nonparametric methods hint dark energy evolution

Reference 131

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no resolver link, observed 2026-07-15T12:01:04.317365Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 0b9d94ea-ae82-49c9-bd3a-1cc5cad0b6da · inbound

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? cites this paper.

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? Parametric and nonparametric methods hint dark energy evolution

Reference 74

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verified exact
arxiv_id, observed 2026-05-10T14:20:31.018648Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation a018cf6f-5018-4774-948a-f9838e028957 · inbound

Negative neutrino mass or negative dark energy? cites this paper.

Negative neutrino mass or negative dark energy? Parametric and nonparametric methods hint dark energy evolution

Reference 56

Resolution
verified exact
arxiv_id, observed 2026-05-21T03:03:55.477570Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation aa0dc241-e015-41ae-a9f4-8ad832ff6b28 · inbound

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus cites this paper.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Parametric and nonparametric methods hint dark energy evolution

Reference 109

Resolution
unresolved
no resolver link, observed 2026-07-11T09:40:49.196932Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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