Paper Citation Record · LEDGER

Towards a possible solution to the Hubble tension with Horndeski gravity

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2301.09382.

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

pith.paper-citation-record.v1
2301.09382 v2

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measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

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measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T04:57:06.887889Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-30T00:14:04.956852Z

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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 59546d61-f465-4962-868f-f7db31e74385 · inbound

Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity cites this paper.

Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity Towards a possible solution to the Hubble tension with Horndeski gravity

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-12T04:57:06.887889Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 630b66f3-bab3-41ea-8afa-9548eaec2eaa · inbound

Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions cites this paper.

Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions Towards a possible solution to the Hubble tension with Horndeski gravity

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-10T19:20:16.819581Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8fe0666a-66de-4c10-95fb-5d47691cf9cc · 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 Towards a possible solution to the Hubble tension with Horndeski gravity

Reference 178

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:54.643038Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation a6aa315d-06c0-4111-97a7-59b37a327989 · 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 Towards a possible solution to the Hubble tension with Horndeski gravity

Reference 129

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:12.234341Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation fec354b1-47c4-4f6a-847e-b7c82d5627f3 · 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 Towards a possible solution to the Hubble tension with Horndeski gravity

Reference 140

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6a1112c2-0e27-4c2a-bc64-9a11ce2853d0 · inbound

Early- and Late-Time Modifications to $\Lambda$CDM: Implications for the Hubble Tension cites this paper.

Early- and Late-Time Modifications to $\Lambda$CDM: Implications for the Hubble Tension Towards a possible solution to the Hubble tension with Horndeski gravity

Reference 60

Resolution: verified exact; arxiv_id, observed 2026-06-30T00:14:04.958113Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 8622ef83-4c87-4e2a-8861-00b285f38d07 · 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 Towards a possible solution to the Hubble tension with Horndeski gravity

Reference 118

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.