Paper Citation Record · LEDGER

Resolving the $H_0$ tension with diffusion

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:2001.07536.

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

pith.paper-citation-record.v1
2001.07536 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 12 of 12 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 12 of 12 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T13:51:08.563704Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T15:37:06.186769Z

Reference resolution

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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 12e489e8-8ff7-4694-bf43-a8ed66ce2d8a · inbound

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions cites this paper.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Resolving the $H_0$ tension with diffusion

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-14T13:51:08.563704Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e470dc16-edd2-41d5-ab64-269eb3f4d683 · inbound

$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity cites this paper.

$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity Resolving the $H_0$ tension with diffusion

Reference 103

Resolution: verified exact; arxiv_id, observed 2026-05-24T03:53:54.725525Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation b349267d-7156-465c-a647-26bd3dae090b · inbound

Using the Kaniadakis horizon entropy in the presence of neutrinos to alleviate the Hubble and $ S_{8} $ Tensions cites this paper.

Using the Kaniadakis horizon entropy in the presence of neutrinos to alleviate the Hubble and $ S_{8} $ Tensions Resolving the $H_0$ tension with diffusion

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-10T20:36:53.169228Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c3d6b65b-5474-44bc-993e-a045305c20ed · inbound

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM cites this paper.

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM Resolving the $H_0$ tension with diffusion

Reference 157

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:55.676269Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 5cda944e-7f7a-414b-9711-6e4dbda22c6e · inbound

Probing dynamical dark energy with late-time data: Evidence, tensions, and the limits of the $w_0w_a$CDM framework cites this paper.

Probing dynamical dark energy with late-time data: Evidence, tensions, and the limits of the $w_0w_a$CDM framework Resolving the $H_0$ tension with diffusion

Reference 111

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:12.178168Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 8f568133-6ac7-4d47-8e95-f2c5ee38cbe5 · inbound

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families cites this paper.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Resolving the $H_0$ tension with diffusion

Reference 121

Resolution: unresolved; no resolver link, observed 2026-07-15T12:01:04.317365Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a0c99f17-9433-43b4-88db-f81d3030b23e · inbound

Comment on Cosmological constraints on unimodular gravity models with diffusion (arXiv:2211.07424): thermodynamic inadmissibility of the H0 tension resolution mechanism cites this paper.

Comment on Cosmological constraints on unimodular gravity models with diffusion (arXiv:2211.07424): thermodynamic inadmissibility of the H0 tension resolution mechanism Resolving the $H_0$ tension with diffusion

Reference 10

Resolution: verified exact; arxiv_id, observed 2026-05-10T05:56:11.037251Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 7abd86e4-ca72-4879-8f4c-9d07689950fb · inbound

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 cites this paper.

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 Resolving the $H_0$ tension with diffusion

Reference 30

Resolution: verified exact; arxiv_id, observed 2026-07-02T15:37:06.188326Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 99a70e73-6c9d-4062-bae9-5037de605871 · inbound

Dark energy genesis: modeling dissipative effects in primordial cosmology cites this paper.

Dark energy genesis: modeling dissipative effects in primordial cosmology Resolving the $H_0$ tension with diffusion

Reference 12

Resolution: unresolved; no resolver link, observed 2026-07-12T03:37:55.491818Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0d4bdf4e-52b0-40ea-a4c4-f58ec7bbcd31 · inbound

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus cites this paper.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Resolving the $H_0$ tension with diffusion

Reference 99

Resolution: unresolved; no resolver link, observed 2026-07-11T09:40:49.196932Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 030478e4-7dd8-4ba6-a859-6f021a75c799 · inbound

Constraints on unimodular diffusion models with latest observables cites this paper.

Constraints on unimodular diffusion models with latest observables Resolving the $H_0$ tension with diffusion

Reference 17

Resolution: unresolved; no resolver link, observed 2026-07-14T16:31:33.826697Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 92188540-f38c-4e64-97f5-63160b3a985d · inbound

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

Hubble tension: a short review of theoretical explanations Resolving the $H_0$ tension with diffusion

Reference 130

Resolution: unresolved; no resolver link, observed 2026-08-01T07:20:07.891153Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.