Paper Citation Record · LEDGER

Features of a dark energy model in string theory

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2212.14004.

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

pith.paper-citation-record.v1
2212.14004 v4

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 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 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T20:16:54.196037Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T05:39:40.539609Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
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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 67e3c0ae-350a-4340-8da9-73d79c25b508 · inbound

Dark bubble cosmology and the equivalence principle cites this paper.

Dark bubble cosmology and the equivalence principle Features of a dark energy model in string theory

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-06T20:16:54.196037Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8fe033e7-c2cc-4223-804b-b530624e675d · inbound

Instabilities in scale-separated Casimir vacua cites this paper.

Instabilities in scale-separated Casimir vacua Features of a dark energy model in string theory

Reference 134

Resolution: verified exact; arxiv_id, observed 2026-05-19T02:37:00.236293Z

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.

Observation a6cbbeb1-4af5-4291-89d9-981c5de83061 · inbound

Weak gravity at micron scales from dark bubble cosmology and its cosmological consequences cites this paper.

Weak gravity at micron scales from dark bubble cosmology and its cosmological consequences Features of a dark energy model in string theory

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-03T20:06:49.265044Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4235bda1-a212-4414-967a-d27c5fdcf96a · inbound

Dark energy from string theory: an introductory review cites this paper.

Dark energy from string theory: an introductory review Features of a dark energy model in string theory

Reference 291

Resolution: verified exact; arxiv_id, observed 2026-05-15T00:18:22.225389Z

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.

Observation 6a9e493b-c030-4055-87a6-9ed9d3ad61c7 · inbound

Dark bubbles, dark dimensions and fat gravitons cites this paper.

Dark bubbles, dark dimensions and fat gravitons Features of a dark energy model in string theory

Reference 26

Resolution: verified exact; arxiv_id, observed 2026-07-04T05:39:40.541794Z

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.