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Paper Citation Record · LEDGER

Resolving the $H_0$ tension with diffusion

As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 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 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-04T06:34:03.388597+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T07:20:07.891153Z

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

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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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 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 2026-08-04T06:34:03.388597+00:00.

source=pdf_text observed=2026-05-24T03:50:50.435997Z digest=sha256:08dad7c4368a23fd1bc2d813aa8f787c5788e92c2534caea0ce03b64a0441367

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 2026-08-04T06:34:03.388597+00:00.

source=pdf_text observed=2026-05-18T04:46:14.832965Z digest=sha256:f37fc497df89f12b906627c2b0fb939ce77e4f64cd2969be2ae71483148d617c

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 2026-08-04T06:34:03.388597+00:00.

source=pdf_text observed=2026-05-21T13:29:05.147292Z digest=sha256:9d456e969b31d2e257d2e313eaff392a8bb9ef892e000bbe39ed86a1133fc754

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.

source=pdf_text observed=2026-07-15T12:01:04.317365Z digest=sha256:7e014c75291083f857734f9ebdcf42ea0372a9ff333e27b6c0dc2e2c98e3bfee

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 2026-08-04T06:34:03.388597+00:00.

source=pdf_text observed=2026-05-10T05:54:50.586629Z digest=sha256:eabe9b7dce2857e102d9b15f3818903228b224ae90f1288930e9007d7060469c

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 2026-08-04T06:34:03.388597+00:00.

source=pdf_text observed=2026-06-27T23:47:15.644279Z digest=sha256:e262f0276ff195a9bd4d599b3751416dea73fd0cbd04767f4b74b0325da56c96

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.

source=pdf_text observed=2026-07-12T03:37:55.491818Z digest=sha256:ffcbd357af796558b257e7756ef24763fea82a12641462431a39259547c276de

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.

source=pdf_text observed=2026-07-11T09:40:49.196932Z digest=sha256:35324e38933ac6ba221a06604d3d128eb8af7c8bede4e5f1bec809974ea82e67

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.

source=pdf_text observed=2026-07-14T16:31:33.826697Z digest=sha256:e3f5d22046ca37b7ffcf59bb0bc4b3754e75c4b634f542e50a67de2690791601

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.

source=pdf_text observed=2026-08-01T07:20:07.891153Z digest=sha256:50a376d22ac158aca421c3328b0967fc213c9b371039db7a501d31bb76716c82