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Paper Citation Record · LEDGER

Towards a possible solution to the Hubble tension with Horndeski gravity

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 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

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 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 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-15T12:01:04.317365Z

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

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • parse uncertain0
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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 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 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-18T04:46:14.832965Z digest=sha256:dc930b8e28e9410a241818bdbc26edc9155a9288a368d0763fbd89aacc6a7175

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 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-21T13:29:05.147292Z digest=sha256:c38b2e9089e2529084a60ee425049363b01b2eb6b41ed64c8285f43b3b2aedef

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.

source=pdf_text observed=2026-07-15T12:01:04.317365Z digest=sha256:501706f20ed3b49a5a92e213aecd4bc5b94f3e298f0251f17820b1f589fe4d88

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 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-29T20:29:06.417337Z digest=sha256:25e1e20434e0508f452e8d67976306db9fea43d494b0b1f6ccc1222362aebc34

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.

source=pdf_text observed=2026-07-11T09:40:49.196932Z digest=sha256:2dacffe68aba65f0580fa6c5e262b990887cad9f1ffd9792674db1b420466f21