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Paper Citation Record · LEDGER

A rapid transition of $G_{\rm eff}$ at $z_t \simeq 0.01$ as a solution of the Hubble and growth tensions

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2102.06012.

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

pith.paper-citation-record.v1
2102.06012 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 11 of 11 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T12:17:22.890080Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T03:56:44.449244Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation eb577748-7a51-4098-9b02-a7458f702d50 · inbound

Model-independent calibration of Gamma-Ray Bursts with neural networks cites this paper.

Model-independent calibration of Gamma-Ray Bursts with neural networks A rapid transition of $G_{\rm eff}$ at $z_t \simeq 0.01$ as a solution of the Hubble and growth tensions

Reference 81

Resolution
verified exact
arxiv_id, observed 2026-05-23T17:55:44.512158Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 77f7817f-4ea1-49c4-9109-2b7169f03470 · inbound

Illustrating the consequences of a misuse of $\sigma_8$ in cosmology cites this paper.

Illustrating the consequences of a misuse of $\sigma_8$ in cosmology A rapid transition of $G_{\rm eff}$ at $z_t \simeq 0.01$ as a solution of the Hubble and growth tensions

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-10T18:12:33.685329Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 2bc5f627-2f44-40ef-9497-96928e160b9e · inbound

Alleviating the Hubble Tension with a Local Void and Transitions of the Absolute Magnitude cites this paper.

Alleviating the Hubble Tension with a Local Void and Transitions of the Absolute Magnitude A rapid transition of $G_{\rm eff}$ at $z_t \simeq 0.01$ as a solution of the Hubble and growth tensions

Reference 86

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 2661cc63-9073-4e2c-a8fd-2d46c9c97fa6 · inbound

Hubble Tension and the G-step Model: Re-examination of Recent Constraints on Modified Local Physics cites this paper.

Hubble Tension and the G-step Model: Re-examination of Recent Constraints on Modified Local Physics A rapid transition of $G_{\rm eff}$ at $z_t \simeq 0.01$ as a solution of the Hubble and growth tensions

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-06T00:10:02.520575Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 049f793f-cdf7-4abf-b665-d66e26e77413 · inbound

Exploring the interplay of late-time dynamical dark energy and new physics before recombination cites this paper.

Exploring the interplay of late-time dynamical dark energy and new physics before recombination A rapid transition of $G_{\rm eff}$ at $z_t \simeq 0.01$ as a solution of the Hubble and growth tensions

Reference 105

Resolution
verified exact
arxiv_id, observed 2026-05-14T23:13:15.203539Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation e8ecba48-055c-4d4b-9352-c2eec1d8b014 · inbound

Impact of the SNe Ia Magnitude Transition at 20 Mpc on Cosmological Parameter Estimation cites this paper.

Impact of the SNe Ia Magnitude Transition at 20 Mpc on Cosmological Parameter Estimation A rapid transition of $G_{\rm eff}$ at $z_t \simeq 0.01$ as a solution of the Hubble and growth tensions

Reference 51

Resolution
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arxiv_id, observed 2026-05-10T14:45:48.271901Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation f57dcc45-9c8b-4459-9157-09595e1364bd · 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 A rapid transition of $G_{\rm eff}$ at $z_t \simeq 0.01$ as a solution of the Hubble and growth tensions

Reference 44

Resolution
verified exact
arxiv_id, observed 2026-05-11T11:41:01.905496Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 70789bdd-3c3f-4774-89f6-bce5a0e20275 · 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 A rapid transition of $G_{\rm eff}$ at $z_t \simeq 0.01$ as a solution of the Hubble and growth tensions

Reference 30

Resolution
verified exact
arxiv_id, observed 2026-05-12T00:36:15.985448Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 909951a1-c088-4c43-8397-a1dec28df3c7 · inbound

Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension cites this paper.

Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension A rapid transition of $G_{\rm eff}$ at $z_t \simeq 0.01$ as a solution of the Hubble and growth tensions

Reference 187

Resolution
verified exact
arxiv_id, observed 2026-07-01T11:25:45.325865Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 7d5d045b-b6c9-404a-b5d2-58e70329d0ff · inbound

Can Distance Duality Violation Save Late-time Solutions to the Hubble Tension? cites this paper.

Can Distance Duality Violation Save Late-time Solutions to the Hubble Tension? A rapid transition of $G_{\rm eff}$ at $z_t \simeq 0.01$ as a solution of the Hubble and growth tensions

Reference 45

Resolution
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local_arxiv, observed 2026-07-10T03:56:44.451507Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 8acc9cc5-2ddb-472e-afc5-b86e35ab2bfd · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall A rapid transition of $G_{\rm eff}$ at $z_t \simeq 0.01$ as a solution of the Hubble and growth tensions

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-01T08:08:40.909069Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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