Paper Citation Record · LEDGER

New tests of dark sector interactions from the full-shape galaxy power spectrum

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2203.08093.

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

pith.paper-citation-record.v1
2203.08093 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 2026-08-12T06:34:41.77262+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T18:15:33.619276Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-24T03:53:54.658205Z

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Outbound references

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Pith citing papers

Observation 8b4ba6db-80f4-4efe-b96a-861a450c6274 · 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 New tests of dark sector interactions from the full-shape galaxy power spectrum

Reference 135

Resolution: verified exact; arxiv_id, observed 2026-05-24T03:53:54.660803Z

Source-reported events for the cited work

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Observation 3053b9fa-8400-4564-9d9c-4bca83374b9a · inbound

Improving cosmological constraints via galaxy intrinsic alignment in full-shape analysis cites this paper.

Improving cosmological constraints via galaxy intrinsic alignment in full-shape analysis New tests of dark sector interactions from the full-shape galaxy power spectrum

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-11T18:15:33.619276Z

Source-reported events for the cited work

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Observation 7135d964-f9c6-4780-a08e-96d4ab07f6f0 · inbound

Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions cites this paper.

Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions New tests of dark sector interactions from the full-shape galaxy power spectrum

Reference 146

Resolution: unresolved; no resolver link, observed 2026-08-10T19:20:17.238594Z

Source-reported events for the cited work

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Observation 4c20f87b-e11c-4ab5-bac1-38386103b4c4 · inbound

Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints cites this paper.

Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints New tests of dark sector interactions from the full-shape galaxy power spectrum

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-06T18:14:15.531085Z

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Observation 13162159-7751-4fdd-857f-9ede8d23df5a · inbound

Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO cites this paper.

Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO New tests of dark sector interactions from the full-shape galaxy power spectrum

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-05T16:03:01.376173Z

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Observation 145a1c78-be78-4146-b3db-665f90826aee · inbound

The simple way to measure evolving dark energy without prior-volume effects cites this paper.

The simple way to measure evolving dark energy without prior-volume effects New tests of dark sector interactions from the full-shape galaxy power spectrum

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-04T18:59:14.168551Z

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Observation 9eadf7e8-c272-4305-833a-62b1bfe6c00a · 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 New tests of dark sector interactions from the full-shape galaxy power spectrum

Reference 232

Resolution: unresolved; no resolver link, observed 2026-08-04T12:53:52.735165Z

Source-reported events for the cited work

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Observation 96aa69a7-6a84-4771-8cf6-84d016da5949 · inbound

A microphysically inspired approach to dark matter-dark energy interactions: first bounds on dark-sector scattering cross sections cites this paper.

A microphysically inspired approach to dark matter-dark energy interactions: first bounds on dark-sector scattering cross sections New tests of dark sector interactions from the full-shape galaxy power spectrum

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-03T11:41:15.310604Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation edea6f99-de90-45bd-9ab9-e8107f69827d · 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 New tests of dark sector interactions from the full-shape galaxy power spectrum

Reference 63

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:12.430208Z

Source-reported events for the cited work

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Observation 7167cd83-83a6-4f1c-817a-596fee1739aa · 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 New tests of dark sector interactions from the full-shape galaxy power spectrum

Reference 72

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 537b8367-5ff7-472f-ba80-f963af4674c0 · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall New tests of dark sector interactions from the full-shape galaxy power spectrum

Reference 108

Resolution: unresolved; no resolver link, observed 2026-08-01T08:08:43.081190Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.