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Paper Citation Record · LEDGER

Coupled dark energy with perturbed Hubble expansion rate

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1409.5533.

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

pith.paper-citation-record.v1
1409.5533 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T18:51:43.346931Z

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

62
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 2d66f311-4c05-4dca-934c-08d373011e34 · inbound

An overview of what current data can (and cannot yet) say about evolving dark energy cites this paper.

An overview of what current data can (and cannot yet) say about evolving dark energy Coupled dark energy with perturbed Hubble expansion rate

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-07T18:51:43.346931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T18:51:43.346931Z digest=sha256:180c1c33b0f03cc7b8d9bb8d4057d58b59031ae6fa73313b783e1e189644dc0a

Observation 43f6c363-f5ac-4dd7-a81f-be7635922019 · 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 Coupled dark energy with perturbed Hubble expansion rate

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-06T18:14:13.226971Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T18:14:13.226971Z digest=sha256:13c5f845c51d35b30119551f84c875cb0eb7c5903314d5e566b1969f6e379251

Observation 04ca3a0b-87cc-420d-8576-08cdacd48514 · inbound

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

Accelerating scaling solutions from dark matter particle creation Coupled dark energy with perturbed Hubble expansion rate

Reference 31

Resolution
verified exact
local_arxiv, observed 2026-07-12T18:39:00.455462Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-12T18:37:05.978670Z digest=sha256:40208c65b23f1df21bbdc077ae9b8367dc371f1a3b6b612a5bea330b82e5ebe9