Paper Citation Record · LEDGER

Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1312.6328.

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

pith.paper-citation-record.v1
1312.6328 v3

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 2026-08-12T06:34:41.77262+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T11:29:07.698617Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

100
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 7fbeb86a-e949-4e41-aa6c-00528e01185b · inbound

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

Interacting phantom dark energy: new accelerating scaling attractors Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-12T11:29:07.698617Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 379c1baa-39b3-4b7b-8ff0-ca6efc6cc28d · 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 Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-06T18:14:13.005429Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a01a08d4-5908-4350-a489-57191bec7b5f · 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 Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-05T16:03:01.162859Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 878428dc-2abf-416b-88ba-fb15365b24b9 · inbound

Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions cites this paper.

Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints

Reference 78

Resolution: verified exact; local_arxiv, observed 2026-06-26T12:39:28.292718Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.