Paper Citation Record · LEDGER

Interacting Dark Energy in a closed universe

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2011.00283.

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

pith.paper-citation-record.v1
2011.00283 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 9 of 9 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 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T11:29:07.760398Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T14:27:03.424035Z

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 01b87f77-5cd5-4162-a51c-72226903ac69 · inbound

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

Interacting phantom dark energy: new accelerating scaling attractors Interacting Dark Energy in a closed universe

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-12T11:29:07.760398Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bff72345-48e4-4130-b6ce-6ba6b9d5927a · 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 Interacting Dark Energy in a closed universe

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-06T18:14:14.689970Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0e4de47c-a59e-4c83-8a9f-02e7326a0097 · 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 Interacting Dark Energy in a closed universe

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-05T16:03:01.323465Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bffe318f-2e62-422f-900e-11b649bd3ca3 · 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 Interacting Dark Energy in a closed universe

Reference 97

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:55.617488Z

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.

Observation 2ad19d0c-69e5-47b0-a7ce-6adccdd044bf · 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 Interacting Dark Energy in a closed universe

Reference 56

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:11.887174Z

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.

Observation 79a36de4-bded-4fff-b059-7e6643c26669 · inbound

Measuring neutrino mass in light of ACT DR6 and DESI DR2 cites this paper.

Measuring neutrino mass in light of ACT DR6 and DESI DR2 Interacting Dark Energy in a closed universe

Reference 36

Resolution: verified exact; arxiv_id, observed 2026-05-15T13:15:50.237352Z

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.

Observation d69d1673-1474-4729-a6d3-2f7636653f43 · inbound

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions cites this paper.

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions Interacting Dark Energy in a closed universe

Reference 173

Resolution: verified exact; arxiv_id, observed 2026-07-01T16:45:51.058533Z

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.

Observation 5e3c2a36-a135-4d87-8799-dd4937d8a804 · inbound

Dissipative Cosmology and the Nature of Dark Energy: Insights from Bulk Viscosity with DESI DR2 observations cites this paper.

Dissipative Cosmology and the Nature of Dark Energy: Insights from Bulk Viscosity with DESI DR2 observations Interacting Dark Energy in a closed universe

Reference 113

Resolution: verified exact; arxiv_id, observed 2026-07-02T14:27:03.425465Z

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.

Observation b4384994-b2dc-433e-9e67-1a0e89bb1e78 · inbound

Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation cites this paper.

Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation Interacting Dark Energy in a closed universe

Reference 214

Resolution: verified exact; arxiv_id, observed 2026-07-02T06:16:43.047566Z

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.