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Paper Citation Record · LEDGER

Equivalence of Dark Energy Models: A Theoretical and Bayesian Perspective

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2502.12915.

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

pith.paper-citation-record.v1
2502.12915 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T12:53:54.210767Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

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 5b564a78-bf51-4b8c-af57-16d0987ae182 · 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 Equivalence of Dark Energy Models: A Theoretical and Bayesian Perspective

Reference 250

Resolution
unresolved
no resolver link, observed 2026-08-04T12:53:54.210767Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T12:53:54.210767Z digest=sha256:fe827b64b11f3234117b210ea9820ef97f0d01f55eecfaf113cb957572c0f166

Observation 87f1cc1b-9a26-457b-8d5f-fb2ac8141564 · inbound

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy cites this paper.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Equivalence of Dark Energy Models: A Theoretical and Bayesian Perspective

Reference 20

Resolution
unresolved
no resolver link, observed 2026-07-15T14:51:12.413085Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-15T14:51:12.413085Z digest=sha256:293717bde0fac20e7990a8d0625ec6dc429a947a6e6a18420e4d55a2e4db2bd9