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Paper Citation Record · LEDGER

All-inclusive interacting dark sector cosmologies

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2001.10852.

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

pith.paper-citation-record.v1
2001.10852 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T11:29:07.749582Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T07:47:45.352873Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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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 642a7f32-80e2-49ea-bd03-c21e1b4bf3d3 · inbound

Interacting phantom dark energy: new accelerating scaling attractors cites this paper.

Interacting phantom dark energy: new accelerating scaling attractors All-inclusive interacting dark sector cosmologies

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-12T11:29:07.749582Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T11:29:07.749582Z digest=sha256:cc6bedbbaff53496eb8c6d8d6a18d6bfe89feae6fa6c1accf091c780c998d4d6

Observation 37d1b2c5-bbec-467e-a785-f56f4e509b9b · 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 All-inclusive interacting dark sector cosmologies

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-10T19:20:16.878139Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T19:20:16.878139Z digest=sha256:a143a0ed6d112fb535310bfa409c92b50125050394131199d801fa59926ca73b

Observation eb30e12a-ec86-4650-affe-5f34186c48f5 · 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 All-inclusive interacting dark sector cosmologies

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-05T16:03:01.316985Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T16:03:01.316985Z digest=sha256:f0a757b131aa070c5cd9f448f3cceecc7255a3d92098809406339aa1509c011c

Observation 64a91107-add7-406c-8e66-5dbc0cfaf900 · 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 All-inclusive interacting dark sector cosmologies

Reference 219

Resolution
unresolved
no resolver link, observed 2026-08-04T12:53:51.657201Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T12:53:51.657201Z digest=sha256:7293f5d155194a7a32b16e43a5ff172a22f48bfdf19a615850400eb38f60a03f

Observation a2e2d668-76d8-420b-aa87-4ac266bccccb · inbound

Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension cites this paper.

Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension All-inclusive interacting dark sector cosmologies

Reference 87

Resolution
verified exact
arxiv_id, observed 2026-05-16T12:17:52.634100Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-05-16T12:15:01.997389Z digest=sha256:c91075d3a3b521de641676a3a6d592c115a286668b04fb91a0d5c9a41bb1781f

Observation 7383c9e1-c1eb-4764-866b-63dc6a5d8f82 · 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 All-inclusive interacting dark sector cosmologies

Reference 29

Resolution
verified exact
arxiv_id, observed 2026-07-02T15:37:06.338405Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-06-27T23:47:15.644279Z digest=sha256:c1a35974863863060a358f704deb335f40663d7bc16e70d3673ba3f89106e7ed

Observation 58eaec47-f024-4e50-ac66-c31f0a99a1ec · inbound

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies cites this paper.

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies All-inclusive interacting dark sector cosmologies

Reference 42

Resolution
verified exact
arxiv_id, observed 2026-07-03T07:47:45.354322Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-06-27T11:43:20.857862Z digest=sha256:fc838a1b4a1b007356e42a13038bc8437e40e623620a2f15c4309cb0061680d6