Paper Citation Record · LEDGER

Could dark energy be vector-like?

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:astro-ph/0405267.

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

pith.paper-citation-record.v1
astro-ph/0405267 v2

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 2026-08-20T06:33:59.587034+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T07:01:25.299381Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-28T08:41:48.628809Z

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 06285b09-7812-49fa-bb38-f83c4db42556 · inbound

Cosmological implications of Bumblebee theory on an FLRW background cites this paper.

Cosmological implications of Bumblebee theory on an FLRW background Could dark energy be vector-like?

Reference 40

Resolution: metadata mismatch; local_arxiv, observed 2026-05-17T02:38:53.989207Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation ae9329bb-b3b8-4d37-ae08-90ba45c63b21 · inbound

Constraining Scale-Dependent Growth in $f(R)$ Gravity with Future 21 cm Surveys cites this paper.

Constraining Scale-Dependent Growth in $f(R)$ Gravity with Future 21 cm Surveys Could dark energy be vector-like?

Reference 81

Resolution: verified exact; local_arxiv, observed 2026-06-28T08:41:48.630410Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 2e5fa32d-deb4-4426-9fb9-beecbcaaa325 · inbound

Evading Cosmological Strong Coupling in Non-minimally Coupled Vector Gravity cites this paper.

Evading Cosmological Strong Coupling in Non-minimally Coupled Vector Gravity Could dark energy be vector-like?

Reference 3

Resolution: unresolved; no resolver link, observed 2026-07-14T06:54:15.387168Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f8bd6b81-470f-4ebd-89c5-5fbea30fd754 · inbound

Isotropic universes with a preferred direction cites this paper.

Isotropic universes with a preferred direction Could dark energy be vector-like?

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-04T07:01:25.299381Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.