Paper Citation Record · LEDGER

Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2404.15977.

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

pith.paper-citation-record.v1
2404.15977 v3

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measured 0 of 0 reference resolution

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measured 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T00:54:43.407504Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T22:30:10.416729Z

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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 65dc56ea-f1bb-401b-a993-b7c49e474938 · inbound

Constraints on Dark Energy Models Using Late Universe Probes cites this paper.

Constraints on Dark Energy Models Using Late Universe Probes Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-07T00:54:43.407504Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3e336c10-cb83-4709-a0ce-4e7e696f7014 · inbound

Investigating $f(R)$-Inflation: background evolution and constraints cites this paper.

Investigating $f(R)$-Inflation: background evolution and constraints Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-06T16:26:13.224523Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ad815fa9-5887-4f99-88a4-7e868a3072d5 · inbound

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime cites this paper.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:02.010016Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5157ac6a-cb8f-4a92-b8f3-840b97f330ae · 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 Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension

Reference 244

Resolution: unresolved; no resolver link, observed 2026-08-04T12:53:53.726107Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b1b803ce-a5fe-4e69-b281-ae264bb5b99e · inbound

Revisiting the Hubble tension problem in the framework of holographic dark energy cites this paper.

Revisiting the Hubble tension problem in the framework of holographic dark energy Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension

Reference 31

Resolution: verified exact; arxiv_id, observed 2026-05-17T22:20:23.287326Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation e9308d4e-3cb7-4b34-862e-e7be8b0a6a01 · 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 Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension

Reference 115

Resolution: verified exact; arxiv_id, observed 2026-05-16T12:17:52.476885Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation fe3fa85b-775f-43f0-a779-b817909e05c3 · inbound

Model-Independent Reconstruction of Quintessence Potential and Kinetic Energy from DESI DR2 and Pantheon+ Supernovae cites this paper.

Model-Independent Reconstruction of Quintessence Potential and Kinetic Energy from DESI DR2 and Pantheon+ Supernovae Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension

Reference 37

Resolution: verified exact; arxiv_id, observed 2026-05-15T01:33:27.423121Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 658adbb7-7301-4c3d-bc93-1d566934e384 · inbound

Effective field theory interpretation of ATLAS measurements involving the Higgs boson, electroweak bosons and the top quark cites this paper.

Effective field theory interpretation of ATLAS measurements involving the Higgs boson, electroweak bosons and the top quark Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension

Reference 16

Resolution: verified exact; arxiv_id, observed 2026-07-04T22:30:10.418231Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 3a85a182-e221-4f09-9beb-d42ce357f692 · inbound

Saturation Mechanisms in the Interacting Dark Sector cites this paper.

Saturation Mechanisms in the Interacting Dark Sector Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension

Reference 17

Resolution: verified exact; arxiv_id, observed 2026-05-11T18:46:07.192421Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 430eb667-7843-404c-b996-babe9c60c3ce · inbound

Interpretation of the binned SNe Ia Master Sample data via a scalar quintessence component: phantom transition? cites this paper.

Interpretation of the binned SNe Ia Master Sample data via a scalar quintessence component: phantom transition? Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension

Reference 57

Resolution: unresolved; no resolver link, observed 2026-07-12T08:56:43.854989Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.