Paper Citation Record · LEDGER

Testing coupled dark energy models with their cosmological background evolution

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1609.09855.

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

pith.paper-citation-record.v1
1609.09855 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 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 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:30:02.103664Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-12T18:39:00.130667Z

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 aa35272e-40c2-4bae-abbe-1c984d9f9953 · inbound

Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy cites this paper.

Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy Testing coupled dark energy models with their cosmological background evolution

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-14T14:30:02.103664Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f89dbd83-83b4-4c92-8675-b454378a32fc · 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 Testing coupled dark energy models with their cosmological background evolution

Reference 118

Resolution: unresolved; no resolver link, observed 2026-08-06T18:14:19.693664Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d6ea4314-7b19-44c0-8a95-023002d9eda3 · 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 Testing coupled dark energy models with their cosmological background evolution

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-05T16:03:01.203992Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 43682f3b-b539-45ee-85be-e7b1cfdf790e · inbound

Accelerating scaling solutions from dark matter particle creation cites this paper.

Accelerating scaling solutions from dark matter particle creation Testing coupled dark energy models with their cosmological background evolution

Reference 36

Resolution: verified exact; local_arxiv, observed 2026-07-12T18:39:00.135398Z

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.