Paper Citation Record · LEDGER

Can interacting dark energy with dynamical coupling resolve the Hubble tension

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2207.05955.

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

pith.paper-citation-record.v1
2207.05955 v3

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measured 0 of 0 reference resolution

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measured 11 of 11 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T16:03:01.382246Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T07:57:44.208058Z

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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 f70551d1-aeed-49c4-acb6-1f4a3a93791c · inbound

Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO cites this paper.

Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO Can interacting dark energy with dynamical coupling resolve the Hubble tension

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-05T16:03:01.382246Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 01bfb308-6251-4b7c-b101-1579b80f9ebc · 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 Can interacting dark energy with dynamical coupling resolve the Hubble tension

Reference 233

Resolution: unresolved; no resolver link, observed 2026-08-04T12:53:52.778676Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8374d64a-05ec-47a9-b294-d2cbaf1f79cb · inbound

Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 cites this paper.

Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 Can interacting dark energy with dynamical coupling resolve the Hubble tension

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-04T09:59:19.551619Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 855c2265-d53d-4930-a2ea-ea80ae1550f8 · inbound

Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder cites this paper.

Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder Can interacting dark energy with dynamical coupling resolve the Hubble tension

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-04T07:19:39.893145Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 84eee012-9f90-405b-9866-a6bf251efc18 · inbound

Robust Preference for Dark Sector Interactions cites this paper.

Robust Preference for Dark Sector Interactions Can interacting dark energy with dynamical coupling resolve the Hubble tension

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.843808Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e59ecc6b-1570-4fd6-9e00-cb7c22e0aef7 · inbound

Unified dark sector and Hubble-tension alleviation in scalar-vector-tensor gravity cites this paper.

Unified dark sector and Hubble-tension alleviation in scalar-vector-tensor gravity Can interacting dark energy with dynamical coupling resolve the Hubble tension

Reference 29

Resolution: verified exact; arxiv_id, observed 2026-06-30T20:15:05.543143Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 9f5b41a3-bb6a-41ce-bf3f-aa34feaedf53 · inbound

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

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions Can interacting dark energy with dynamical coupling resolve the Hubble tension

Reference 181

Resolution: verified exact; arxiv_id, observed 2026-07-01T16:35:50.598593Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation c39e76a5-d669-4de9-bc0b-5015885f480e · 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 interacting dark energy with dynamical coupling resolve the Hubble tension

Reference 57

Resolution: verified exact; arxiv_id, observed 2026-07-02T15:37:06.545947Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 0aa84d7a-e104-4a0c-b0ae-b9f7f2b9d4a9 · 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 Can interacting dark energy with dynamical coupling resolve the Hubble tension

Reference 71

Resolution: verified exact; arxiv_id, observed 2026-07-03T07:57:44.209713Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 2a229e3b-70c3-4664-b78a-6bd38701fc10 · 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 Can interacting dark energy with dynamical coupling resolve the Hubble tension

Reference 72

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 239321f4-39b2-47f6-973a-b4b4decc5b0f · inbound

Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions cites this paper.

Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions Can interacting dark energy with dynamical coupling resolve the Hubble tension

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-01T02:46:22.867328Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.