Paper Citation Record · LEDGER

Chameleon dark energy can resolve the Hubble tension

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 13 inbound Pith citation observations for arXiv:2102.02020.

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

pith.paper-citation-record.v1
2102.02020 v4

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 13 of 13 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 13 of 13 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T23:12:26.300453Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T05:19:35.951419Z

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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 8320cd50-ac52-480c-b1af-5caf193299a3 · inbound

In the Realm of the Hubble tension $-$ a Review of Solutions cites this paper.

In the Realm of the Hubble tension $-$ a Review of Solutions Chameleon dark energy can resolve the Hubble tension

Reference 251

Resolution: verified exact; arxiv_id, observed 2026-05-15T11:50:32.832825Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation f97ff44d-177c-4d74-82db-9faa7da4d4a2 · inbound

The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae cites this paper.

The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Chameleon dark energy can resolve the Hubble tension

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-08T23:12:26.300453Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3656151d-4d2f-435a-a0b4-a0c323c19044 · inbound

Interacting Early Dark Energy cites this paper.

Interacting Early Dark Energy Chameleon dark energy can resolve the Hubble tension

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-08T04:50:12.821663Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e5b0935d-fc0c-4a6a-b6ed-c8b35137d214 · inbound

An overview of what current data can (and cannot yet) say about evolving dark energy cites this paper.

An overview of what current data can (and cannot yet) say about evolving dark energy Chameleon dark energy can resolve the Hubble tension

Reference 107

Resolution: unresolved; no resolver link, observed 2026-08-07T18:51:43.652315Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fd098831-3e4b-4e16-a016-3509c0773b44 · inbound

Resolving the Planck-DESI tension by nonminimally coupled quintessence cites this paper.

Resolving the Planck-DESI tension by nonminimally coupled quintessence Chameleon dark energy can resolve the Hubble tension

Reference 31

Resolution: verified exact; arxiv_id, observed 2026-05-19T01:36:57.999821Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation b45b3500-53c8-41d4-a84e-13218091c4ec · 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 Chameleon dark energy can resolve the Hubble tension

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-04T09:59:12.020835Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eed2966c-fdbe-4083-bbfe-845e304b36a7 · inbound

Direct detection of solar chameleons with electron recoil data from XENONnT cites this paper.

Direct detection of solar chameleons with electron recoil data from XENONnT Chameleon dark energy can resolve the Hubble tension

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-04T00:27:28.481247Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5f42b4c0-bca4-447f-ae25-30f818b2a3c2 · inbound

Constraining interacting dark energy models with black hole superradiance cites this paper.

Constraining interacting dark energy models with black hole superradiance Chameleon dark energy can resolve the Hubble tension

Reference 19

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:10:16.952154Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 19d3588c-cb2b-4bde-b45b-7bd5cf1649b7 · inbound

Coupled Dark Energy and Dark Matter for DESI: An Effective Guide to the Phantom Divide cites this paper.

Coupled Dark Energy and Dark Matter for DESI: An Effective Guide to the Phantom Divide Chameleon dark energy can resolve the Hubble tension

Reference 34

Resolution: verified exact; arxiv_id, observed 2026-05-11T07:21:00.335400Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation c07d0cf7-7ceb-4745-a371-39a84ae4ffe9 · inbound

Cosmological intercept tension cites this paper.

Cosmological intercept tension Chameleon dark energy can resolve the Hubble tension

Reference 26

Resolution: verified exact; arxiv_id, observed 2026-05-12T10:26:30.856001Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation ca00e54d-7b33-4f74-93e2-6a1084b69515 · inbound

The Hubble tension: A decade review cites this paper.

The Hubble tension: A decade review Chameleon dark energy can resolve the Hubble tension

Reference 118

Resolution: verified exact; arxiv_id, observed 2026-07-04T05:19:35.952974Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 661fb143-3d4d-40bc-aae9-60a0043110e7 · inbound

The Hubble tension: A decade review cites this paper.

The Hubble tension: A decade review Chameleon dark energy can resolve the Hubble tension

Reference 118

Resolution: unresolved; no resolver link, observed 2026-07-15T10:41:50.733215Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9355f722-ac31-4f12-92d5-fa225e588e43 · inbound

Hubble tension: a short review of theoretical explanations cites this paper.

Hubble tension: a short review of theoretical explanations Chameleon dark energy can resolve the Hubble tension

Reference 239

Resolution: unresolved; no resolver link, observed 2026-08-01T07:20:08.271395Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.