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Paper Citation Record · LEDGER

Simultaneously solving the $H_0$ and $\sigma_8$ tensions with late dark energy

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2201.11623.

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

pith.paper-citation-record.v1
2201.11623 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T14:34:39.960648Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T15:37:06.576357Z

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 813c74b2-fa79-414b-9950-0638abee4b29 · inbound

Cosmic distance duality after DESI 2024 data release and dark energy evolution cites this paper.

Cosmic distance duality after DESI 2024 data release and dark energy evolution Simultaneously solving the $H_0$ and $\sigma_8$ tensions with late dark energy

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-10T14:34:39.960648Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T14:34:39.960648Z digest=sha256:4623b122437aea5564ed83a923ab453b930ac384cc52a324101f4d53bacc8ef7

Observation 3b15d497-c62e-4fc4-bfec-c9bd6178cf6f · inbound

Observational implications of Wald-Gauss-Bonnet topological dark energy cites this paper.

Observational implications of Wald-Gauss-Bonnet topological dark energy Simultaneously solving the $H_0$ and $\sigma_8$ tensions with late dark energy

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-10T14:00:10.962723Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T14:00:10.962723Z digest=sha256:2bb89e55a5e2bf29ad37f3c45516781637499d09d341bfbc216a3cf3cd37ddbe

Observation 1542f360-222e-4f51-ada7-b0325401c6c7 · inbound

The Quintom theory of dark energy after DESI DR2 cites this paper.

The Quintom theory of dark energy after DESI DR2 Simultaneously solving the $H_0$ and $\sigma_8$ tensions with late dark energy

Reference 49

Resolution
verified exact
arxiv_id, observed 2026-05-19T13:12:19.041010Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-05-19T13:08:20.192767Z digest=sha256:8e35834cde479167fe91345c45f7b48adcd3886679052631cce2a1248bc74dfe

Observation cdf5f838-0446-4114-b9d5-7c7c06741c50 · inbound

Gravitational particle production, the cosmological tensions and fast radio bursts cites this paper.

Gravitational particle production, the cosmological tensions and fast radio bursts Simultaneously solving the $H_0$ and $\sigma_8$ tensions with late dark energy

Reference 26

Resolution
verified exact
arxiv_id, observed 2026-05-18T20:51:50.659743Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-05-18T20:50:39.710186Z digest=sha256:13acd2c453ce134ab81bfe26d39496b770149785f72eb158de865493a751e6ae

Observation 6fcf4ae5-045d-4f2f-8149-234665cabc25 · 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 Simultaneously solving the $H_0$ and $\sigma_8$ tensions with late dark energy

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-04T12:53:35.123947Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T12:53:35.123947Z digest=sha256:21dfaf9f2f8ca6b55cb042c97239ac9a98a39770a3407c8443be2e19c1f53dce

Observation ea9ae065-aa77-40f5-8540-a8744fddfb22 · inbound

Testing General Relativity Through Gravitational Wave Classification: A Convolutional Neural Network Framework cites this paper.

Testing General Relativity Through Gravitational Wave Classification: A Convolutional Neural Network Framework Simultaneously solving the $H_0$ and $\sigma_8$ tensions with late dark energy

Reference 10

Resolution
verified exact
arxiv_id, observed 2026-05-09T06:10:37.676413Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-05-08T18:52:00.585887Z digest=sha256:543676b4eca12010e6e31d2192d5ddb4e871c4544ddf1bfd774113d83fa3ad0f

Observation 62ec2611-acff-4c7c-b8a5-63fed91105f3 · 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 Simultaneously solving the $H_0$ and $\sigma_8$ tensions with late dark energy

Reference 53

Resolution
verified exact
arxiv_id, observed 2026-07-02T15:37:06.577716Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-06-27T23:47:15.644279Z digest=sha256:45513659dc36b1bf0bfb2280fe4177edb01506e1cc102320e4a4c6a9c58c6702

Observation 825d093a-4877-462e-ae0a-00706ea90494 · 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 Simultaneously solving the $H_0$ and $\sigma_8$ tensions with late dark energy

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-01T02:46:22.989959Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T02:46:22.989959Z digest=sha256:d39ec1917bb1e8939063d8023a4e6f3a22596b4365585b97a11a0721f7662e4b