Paper Citation Record · LEDGER

Implications of an extended dark energy model with massive neutrinos

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2202.01749.

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

pith.paper-citation-record.v1
2202.01749 v4

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 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 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T12:53:35.351505Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T10:36:52.134251Z

Reference resolution

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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 5438d313-b1c4-43e6-9446-de0a51ad1a75 · inbound

Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape cites this paper.

Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape Implications of an extended dark energy model with massive neutrinos

Reference 65

Resolution: verified exact; arxiv_id, observed 2026-05-16T17:46:22.982208Z

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.

Observation f9d70b9b-8171-4cd8-947e-d60808ac0f56 · inbound

BAO miscalibration cannot rescue late-time solutions to the Hubble tension cites this paper.

BAO miscalibration cannot rescue late-time solutions to the Hubble tension Implications of an extended dark energy model with massive neutrinos

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-04T12:53:35.351505Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 89c1077d-c1bb-4ff6-a558-2fb6e65bcd22 · inbound

Dissipative Dark Energy can explain the DESI phantom crossing cites this paper.

Dissipative Dark Energy can explain the DESI phantom crossing Implications of an extended dark energy model with massive neutrinos

Reference 10

Resolution: verified exact; arxiv_id, observed 2026-07-02T10:36:52.135537Z

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.

Observation 16ae92fb-3009-48cc-84cd-2ce75c260a94 · inbound

Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data cites this paper.

Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data Implications of an extended dark energy model with massive neutrinos

Reference 206

Resolution: unresolved; no resolver link, observed 2026-07-12T04:18:55.037825Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.