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Paper Citation Record · LEDGER

Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2201.04528.

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

pith.paper-citation-record.v1
2201.04528 v2

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 2026-08-07T06:34:17.273281+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T14:03:34.402902Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-22T05:24:38.000867Z

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 18bc0cda-20f3-46b9-b0a1-9d2843451d61 · inbound

A frequentist view on the two-body decaying dark matter model cites this paper.

A frequentist view on the two-body decaying dark matter model Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter

Reference 23

Resolution
unresolved
no resolver link, observed 2026-08-07T14:03:34.402902Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation ff08a53d-006a-4431-b900-2e781a89a87e · 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 Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter

Reference 231

Resolution
unresolved
no resolver link, observed 2026-08-04T12:53:52.690982Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T12:53:52.690982Z digest=sha256:5716de5d91b8b3b724e27487dc08932252358f49c9a956936e8d7e44881b8797

Observation 2227df81-3306-424b-ad9d-821941d63525 · inbound

Direct detection of solar chameleons with electron recoil data from XENONnT cites this paper.

Direct detection of solar chameleons with electron recoil data from XENONnT Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter

Reference 287

Resolution
unresolved
no resolver link, observed 2026-08-04T00:27:33.239480Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T00:27:33.239480Z digest=sha256:95db76c376854a0d1a88e54f1661a95cc194b8dda049e6a897b6e9798b9affe2

Observation 7baf7313-cba0-4e58-b4f3-7f67bb328308 · inbound

Is Phantom Divide Crossing in General Relativity Completely Impossible? Shortcomings in canonical and minimally coupled scalar field and Possible Solutions in $k$-essence Models cites this paper.

Is Phantom Divide Crossing in General Relativity Completely Impossible? Shortcomings in canonical and minimally coupled scalar field and Possible Solutions in $k$-essence Models Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-03T07:07:24.793181Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T07:07:24.793181Z digest=sha256:d964fe08c1fb6fe7564bf198a264d33a35f272dc7ca6bc8931d007f701479aaf

Observation 299df7bb-ad94-48d9-943b-43fdd846a97f · inbound

Dark Energy in Ghost-free non-local Gravity cites this paper.

Dark Energy in Ghost-free non-local Gravity Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter

Reference 22

Resolution
verified exact
arxiv_id, observed 2026-05-22T05:24:38.003646Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-22T05:24:23.654862Z digest=sha256:c9337e2e57cd4a9060b02d22fc305dca8ad0c82fb617dc197688c6c5efb7f12e

Observation 0037c103-44a2-40a5-a351-ce8f3c16df02 · inbound

Decaying Dark Matter Halo Abundance from a Revised Spherical Collapse Model cites this paper.

Decaying Dark Matter Halo Abundance from a Revised Spherical Collapse Model Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-01T13:07:47.298974Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 2731e05c-2278-492d-b62e-e4e0988f16a6 · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter

Reference 106

Resolution
unresolved
no resolver link, observed 2026-08-01T08:08:42.766448Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T08:08:42.766448Z digest=sha256:ac87f6bf107083758b12ac2a9ccb740564d77f314aed977a82a76e2d62fba3f2

Observation 4ee5cbf0-4ea1-4bfe-8b65-279cc5e955ae · inbound

Dark matter-baryons elastic coupling cites this paper.

Dark matter-baryons elastic coupling Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-01T04:55:30.621310Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T04:55:30.621310Z digest=sha256:17663b8b7b28f049750817dd123b98664e9ada1317011ba419e5d5252e04e855