Paper Citation Record · LEDGER

Cosmic Clues: DESI, Dark Energy, and the Cosmological Constant Problem

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2404.06444.

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

pith.paper-citation-record.v1
2404.06444 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T23:12:26.087965Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-17T22:20:23.615838Z

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 055c1961-4b7e-4b56-9f3b-57f2c3d1bf86 · inbound

The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae cites this paper.

The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Cosmic Clues: DESI, Dark Energy, and the Cosmological Constant Problem

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-08T23:12:26.087965Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0e36f5b5-6a79-4130-a421-6cb0ba3ad480 · inbound

Robustness of dark energy phenomenology across different parameterizations cites this paper.

Robustness of dark energy phenomenology across different parameterizations Cosmic Clues: DESI, Dark Energy, and the Cosmological Constant Problem

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.803660Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0fe807c0-24bc-4327-b512-b7c0eab21371 · inbound

An overview of what current data can (and cannot yet) say about evolving dark energy cites this paper.

An overview of what current data can (and cannot yet) say about evolving dark energy Cosmic Clues: DESI, Dark Energy, and the Cosmological Constant Problem

Reference 205

Resolution: unresolved; no resolver link, observed 2026-08-07T18:51:44.036249Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1db0bd55-b3a0-4c34-84c4-4e60b43307b3 · inbound

The Lifespan of our Universe cites this paper.

The Lifespan of our Universe Cosmic Clues: DESI, Dark Energy, and the Cosmological Constant Problem

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-06T21:34:59.732053Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 29f0319d-e688-4653-8de1-288f55998e68 · inbound

Revisiting the Hubble tension problem in the framework of holographic dark energy cites this paper.

Revisiting the Hubble tension problem in the framework of holographic dark energy Cosmic Clues: DESI, Dark Energy, and the Cosmological Constant Problem

Reference 22

Resolution: verified exact; arxiv_id, observed 2026-05-17T22:20:23.618056Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 1044a993-7b73-47cc-882b-551fa5490ca1 · inbound

Model-Independent Reconstruction of Quintessence Potential and Kinetic Energy from DESI DR2 and Pantheon+ Supernovae cites this paper.

Model-Independent Reconstruction of Quintessence Potential and Kinetic Energy from DESI DR2 and Pantheon+ Supernovae Cosmic Clues: DESI, Dark Energy, and the Cosmological Constant Problem

Reference 22

Resolution: verified exact; arxiv_id, observed 2026-05-15T01:33:27.358460Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 6e69e4cd-1267-46b9-bc15-3407b76da549 · inbound

UV-complete and stable Quintom Dark Energy models in the light of DESI DR2 cites this paper.

UV-complete and stable Quintom Dark Energy models in the light of DESI DR2 Cosmic Clues: DESI, Dark Energy, and the Cosmological Constant Problem

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-03T02:32:26.640055Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 82bf0f11-f828-4627-8b7b-ccaaf6784d1e · inbound

Why 4D? Spontaneous Dimensional Selection from Gauge Criticality cites this paper.

Why 4D? Spontaneous Dimensional Selection from Gauge Criticality Cosmic Clues: DESI, Dark Energy, and the Cosmological Constant Problem

Reference 33

Resolution: unresolved; no resolver link, observed 2026-07-31T02:09:13.327775Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.