Paper Citation Record · LEDGER

Constraints on interacting dark energy revisited: implications for the Hubble tension

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2308.05807.

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

pith.paper-citation-record.v1
2308.05807 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T05:19:56.421168Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T07:47:45.260641Z

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 d1e0ecb5-530f-49bb-9f42-07686b39f1ba · 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 Constraints on interacting dark energy revisited: implications for the Hubble tension

Reference 102

Resolution: unresolved; no resolver link, observed 2026-08-10T19:20:16.947719Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 68b6daa4-71cd-4ccb-acaa-3b340734cd52 · inbound

A New Master Supernovae Ia sample and the investigation of the $H_0$ tension cites this paper.

A New Master Supernovae Ia sample and the investigation of the $H_0$ tension Constraints on interacting dark energy revisited: implications for the Hubble tension

Reference 2023

Resolution: unresolved; no resolver link, observed 2026-08-10T17:56:50.957071Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2ff8861a-67e6-409d-942d-f92650222c36 · inbound

The frozen vanilla model: Exploring dark sector interactions with delta effective theories cites this paper.

The frozen vanilla model: Exploring dark sector interactions with delta effective theories Constraints on interacting dark energy revisited: implications for the Hubble tension

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-16T05:19:56.421168Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2108181e-7ecf-44fe-93c6-2c82a82294b6 · inbound

A microphysically inspired approach to dark matter-dark energy interactions: first bounds on dark-sector scattering cross sections cites this paper.

A microphysically inspired approach to dark matter-dark energy interactions: first bounds on dark-sector scattering cross sections Constraints on interacting dark energy revisited: implications for the Hubble tension

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-03T11:41:15.323640Z

Source-reported events for the cited work

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Observation 05be02e4-084d-4a96-b337-74e69f9ff650 · inbound

Robust Preference for Dark Sector Interactions cites this paper.

Robust Preference for Dark Sector Interactions Constraints on interacting dark energy revisited: implications for the Hubble tension

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.827436Z

Source-reported events for the cited work

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Observation 0efc86d9-916b-4088-8fe6-86d9fdfc1013 · inbound

Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension cites this paper.

Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension Constraints on interacting dark energy revisited: implications for the Hubble tension

Reference 99

Resolution: verified exact; arxiv_id, observed 2026-05-16T12:17:52.641488Z

Source-reported events for the cited work

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Observation 5f49ce06-914f-49c8-99fe-637b0dc647c9 · inbound

Interacting Dark Sector field theory with phantom crossing cites this paper.

Interacting Dark Sector field theory with phantom crossing Constraints on interacting dark energy revisited: implications for the Hubble tension

Reference 20

Resolution: verified exact; arxiv_id, observed 2026-05-20T03:53:02.709781Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 9ce0ec4e-d5c7-4f5a-9475-c2c5a0e97bcc · inbound

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions cites this paper.

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions Constraints on interacting dark energy revisited: implications for the Hubble tension

Reference 189

Resolution: verified exact; arxiv_id, observed 2026-07-01T16:45:51.352911Z

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No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation ca0055a2-babf-4b46-8cd7-c8036913e6f0 · 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 Constraints on interacting dark energy revisited: implications for the Hubble tension

Reference 76

Resolution: verified exact; arxiv_id, observed 2026-07-02T15:37:06.415796Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 1da66549-a69d-4a4b-b8bd-d83516d90903 · inbound

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies cites this paper.

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies Constraints on interacting dark energy revisited: implications for the Hubble tension

Reference 59

Resolution: verified exact; arxiv_id, observed 2026-07-03T07:47:45.262434Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.