Paper Citation Record · LEDGER

On the interacting dark energy scenarios $-$ the case for Hubble constant tension

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2310.07260.

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

pith.paper-citation-record.v1
2310.07260 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 9 of 9 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 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T11:29:07.596584Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T07:47:45.327395Z

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External citation measurements

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Outbound references

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Pith citing papers

Observation cb8282ee-4233-421c-911e-b074b8bc2322 · inbound

Interacting phantom dark energy: new accelerating scaling attractors cites this paper.

Interacting phantom dark energy: new accelerating scaling attractors On the interacting dark energy scenarios $-$ the case for Hubble constant tension

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-12T11:29:07.596584Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0e7293b8-85b3-4baf-b29c-3101f20618aa · 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 On the interacting dark energy scenarios $-$ the case for Hubble constant tension

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-10T19:20:16.867186Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f6dc93f5-9ba1-41c0-bed3-79a89554703f · inbound

Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints cites this paper.

Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints On the interacting dark energy scenarios $-$ the case for Hubble constant tension

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-06T18:14:17.692001Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d3e731ab-8677-49b8-9209-3fe8b5f39565 · inbound

Robust Preference for Dark Sector Interactions cites this paper.

Robust Preference for Dark Sector Interactions On the interacting dark energy scenarios $-$ the case for Hubble constant tension

Reference 72

Resolution: malformed identifier; no resolver link, observed 2026-08-03T11:11:48.807359Z

Source-reported events for the cited work

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Observation 7afc5884-f35e-45c5-8482-d486460bf67e · 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 On the interacting dark energy scenarios $-$ the case for Hubble constant tension

Reference 85

Resolution: verified exact; arxiv_id, observed 2026-05-16T12:17:52.577601Z

Source-reported events for the cited work

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Observation de34a67a-e7a4-4484-b3b6-13538cc11563 · inbound

Background dynamics and observational constraints of flat and non-flat $\Lambda(t)$CDM models from $H(z)$ and DESI DR2 BAO measurements cites this paper.

Background dynamics and observational constraints of flat and non-flat $\Lambda(t)$CDM models from $H(z)$ and DESI DR2 BAO measurements On the interacting dark energy scenarios $-$ the case for Hubble constant tension

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-02T19:12:04.349265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8f2f7a8a-5073-44ab-b05e-df54261c0a65 · inbound

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

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions On the interacting dark energy scenarios $-$ the case for Hubble constant tension

Reference 192

Resolution: verified exact; arxiv_id, observed 2026-07-01T16:45:51.350687Z

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 498e418b-aa9a-4c44-8705-b6daca62ea8e · 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 On the interacting dark energy scenarios $-$ the case for Hubble constant tension

Reference 40

Resolution: metadata mismatch; arxiv_id, observed 2026-07-03T07:47:45.328815Z

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 e3c8a52c-789d-49e0-8187-2dc883bd5254 · inbound

Generalizing the interacting dilatonic ghost condensate as a dark energy model cites this paper.

Generalizing the interacting dilatonic ghost condensate as a dark energy model On the interacting dark energy scenarios $-$ the case for Hubble constant tension

Reference 40

Resolution: verified exact; arxiv_id, observed 2026-07-01T17:55:52.605436Z

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.