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Paper Citation Record · LEDGER

Can neutrino-assisted early dark energy models ameliorate the $H_0$ tension in a natural way?

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2302.04644.

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

pith.paper-citation-record.v1
2302.04644 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 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 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T18:26:58.160601Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T20:07:22.273377Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • parse uncertain0
  • 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 91bba2e7-c963-4a4a-a4be-f23807ae45a2 · inbound

Beyond LambdaCDM: How the Hubble tension challenges early universe physics cites this paper.

Beyond LambdaCDM: How the Hubble tension challenges early universe physics Can neutrino-assisted early dark energy models ameliorate the $H_0$ tension in a natural way?

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-06T18:26:58.160601Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T18:26:58.160601Z digest=sha256:ee663109133b312c8ff7e4653acf65609e836e4aa87ee073ab4738265cbddd56

Observation f5c0d5e1-5d09-4a89-be83-b813f1fb13dc · inbound

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 cites this paper.

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 Can neutrino-assisted early dark energy models ameliorate the $H_0$ tension in a natural way?

Reference 64

Resolution
verified exact
arxiv_id, observed 2026-07-02T15:37:06.267651Z

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=2026-06-27T23:47:15.644279Z digest=sha256:1c5397ed8e1eafccb54c1c8d3704a20497f1b732e824a3d0e3ae3c8ceaa4e2c2

Observation ea61dc74-c08a-47f6-8a71-89d2ec30921f · inbound

Mass-Varying Neutrinos from an Inverse Symmetron cites this paper.

Mass-Varying Neutrinos from an Inverse Symmetron Can neutrino-assisted early dark energy models ameliorate the $H_0$ tension in a natural way?

Reference 49

Resolution
verified exact
arxiv_id, observed 2026-07-02T20:07:22.274933Z

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=2026-06-27T20:55:45.775284Z digest=sha256:9938b1a56a56ea633c23cf658e68e16a93f2567073ed9cf49e083fa6c9f90b04