Paper Citation Record · LEDGER

Chameleon Early Dark Energy and the Hubble Tension

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 24 inbound Pith citation observations for arXiv:2106.13290.

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

pith.paper-citation-record.v1
2106.13290 v2

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measured 24 of 24 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 24 of 24 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T22:11:10.401953Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

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External citation measurements

7
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 049f5c38-5151-4357-ad6a-1b3c9acc6597 · inbound

The Hubble Tension and Early Dark Energy cites this paper.

The Hubble Tension and Early Dark Energy Chameleon Early Dark Energy and the Hubble Tension

Reference 104

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Observation 3f617643-96ba-404b-a8a5-ee760ca90438 · inbound

Theoretical and observational constraints on early dark energy in $F(R)$ gravity cites this paper.

Theoretical and observational constraints on early dark energy in $F(R)$ gravity Chameleon Early Dark Energy and the Hubble Tension

Reference 12

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Observation c7677aa8-4825-4edc-87f8-7b206589bad1 · inbound

Effect of Peak Absolute Magnitude of Type Ia Supernovae and Sound Horizon Values on Hubble Tension using DESI results cites this paper.

Effect of Peak Absolute Magnitude of Type Ia Supernovae and Sound Horizon Values on Hubble Tension using DESI results Chameleon Early Dark Energy and the Hubble Tension

Reference 22

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Observation 8589f67b-8d4f-4c5c-a18d-08b01e010e1b · inbound

Can the sound horizon-free measurement of $H_0$ constrain early new physics? cites this paper.

Can the sound horizon-free measurement of $H_0$ constrain early new physics? Chameleon Early Dark Energy and the Hubble Tension

Reference 45

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Observation 36198dc6-03df-4684-8885-34c4fba601d4 · inbound

Searching for coupled, hyperlight scalars across cosmic history cites this paper.

Searching for coupled, hyperlight scalars across cosmic history Chameleon Early Dark Energy and the Hubble Tension

Reference 198

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Observation d58a2182-fa90-49b6-83ab-0733da6132aa · inbound

Impact of ACT DR6 and DESI DR2 for Early Dark Energy and the Hubble tension cites this paper.

Impact of ACT DR6 and DESI DR2 for Early Dark Energy and the Hubble tension Chameleon Early Dark Energy and the Hubble Tension

Reference 46

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Observation 27ab6315-3c42-4f80-8a0a-5cdc7a6dcfe5 · inbound

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

Constraints on Dark Energy Models Using Late Universe Probes Chameleon Early Dark Energy and the Hubble Tension

Reference 51

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Observation 36d9b647-3bbb-4d49-affa-a9f1449730b0 · inbound

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

Resolving the Planck-DESI tension by nonminimally coupled quintessence Chameleon Early Dark Energy and the Hubble Tension

Reference 33

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Observation b6b04057-de98-427f-95c8-2816fe14324c · 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 Chameleon Early Dark Energy and the Hubble Tension

Reference 33

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Observation d6f2d744-2d0c-470f-956d-1954ffda3417 · inbound

The implications of inflation for the last ACT cites this paper.

The implications of inflation for the last ACT Chameleon Early Dark Energy and the Hubble Tension

Reference 70

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Observation c3dceba0-cd8d-4224-b0e0-a3dcf9f05449 · inbound

Harrison-Zeldovich attractor: From Planck to ACT results cites this paper.

Harrison-Zeldovich attractor: From Planck to ACT results Chameleon Early Dark Energy and the Hubble Tension

Reference 101

Resolution: metadata mismatch; arxiv_id, observed 2026-05-18T02:52:21.307041Z

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Observation fed19520-9e80-4739-bf10-34bdcf8b6bc5 · 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 Early Dark Energy and the Hubble Tension

Reference 101

Resolution: unresolved; no resolver link, observed 2026-08-04T00:27:28.611266Z

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Observation 47d4712c-8985-4bfe-8885-084e3a136fdd · inbound

Disentangling cosmic distance tensions with early and late dark energy cites this paper.

Disentangling cosmic distance tensions with early and late dark energy Chameleon Early Dark Energy and the Hubble Tension

Reference 79

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Observation e8631cac-eea0-47f0-93aa-c293301f4716 · inbound

Double the axions, half the tension: multi-field early dark energy eases the Hubble tension cites this paper.

Double the axions, half the tension: multi-field early dark energy eases the Hubble tension Chameleon Early Dark Energy and the Hubble Tension

Reference 115

Resolution: verified exact; arxiv_id, observed 2026-05-10T13:00:24.861180Z

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Observation 4d7f0672-952d-4f24-b6c0-52910406a856 · inbound

Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension cites this paper.

Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension Chameleon Early Dark Energy and the Hubble Tension

Reference 86

Resolution: verified exact; arxiv_id, observed 2026-05-12T00:36:16.351196Z

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Observation ed53dde8-0f17-4f35-aecf-c83b65c1544a · 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 Chameleon Early Dark Energy and the Hubble Tension

Reference 18

Resolution: verified exact; arxiv_id, observed 2026-06-30T20:15:05.491557Z

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Observation 89e1a2cc-12eb-4624-8336-1c331173eb9b · inbound

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

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions Chameleon Early Dark Energy and the Hubble Tension

Reference 70

Resolution: verified exact; arxiv_id, observed 2026-07-01T16:45:51.244648Z

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Observation 3cd4e360-a51a-4de2-8d0d-549584a232f2 · inbound

The Hubble tension: A decade review cites this paper.

The Hubble tension: A decade review Chameleon Early Dark Energy and the Hubble Tension

Reference 117

Resolution: verified exact; arxiv_id, observed 2026-07-04T05:19:36.133943Z

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Observation 48f6edd2-8b8c-44ae-a901-8f3ec362feec · inbound

The Hubble tension: A decade review cites this paper.

The Hubble tension: A decade review Chameleon Early Dark Energy and the Hubble Tension

Reference 117

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Imprint of swampland-inspired coupled early dark energy cites this paper.

Imprint of swampland-inspired coupled early dark energy Chameleon Early Dark Energy and the Hubble Tension

Reference 120

Resolution: verified exact; local_arxiv, observed 2026-07-08T15:55:04.703349Z

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Observation cef1e327-b59f-4271-8a43-938d3762e45b · inbound

The $H_0$ World Cup. I. Summary of the baseline group stage results cites this paper.

The $H_0$ World Cup. I. Summary of the baseline group stage results Chameleon Early Dark Energy and the Hubble Tension

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-02T05:41:35.854134Z

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Observation 99ecf027-69fe-4ca5-8a9e-32b725f01864 · inbound

The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions cites this paper.

The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions Chameleon Early Dark Energy and the Hubble Tension

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-02T05:48:08.491013Z

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Observation f7439308-9e5d-444f-be7b-c22ba6c5f590 · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall Chameleon Early Dark Energy and the Hubble Tension

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-01T08:08:41.676096Z

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Observation 31fa1e27-c159-4edf-9ee0-de1ec1ab8c83 · 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 Chameleon Early Dark Energy and the Hubble Tension

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-01T02:46:22.672776Z

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Unavailable: canonical work link unavailable.