Paper Citation Record · LEDGER

What if string theory has a de Sitter excited state?

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2404.11680.

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

pith.paper-citation-record.v1
2404.11680 v3

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 2026-08-21T06:32:19.484+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T11:05:29.562280Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-15T00:18:22.044962Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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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 34cb6de8-0f11-4d57-b3a9-9bc488c9df35 · inbound

Wheeler-De Witt equation and the Canonical Construction of the Glauber-Sudarshan States in Quantum Gravity cites this paper.

Wheeler-De Witt equation and the Canonical Construction of the Glauber-Sudarshan States in Quantum Gravity What if string theory has a de Sitter excited state?

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-12T11:05:29.562280Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a8f0429b-3eb0-4313-8a41-c525ee21a858 · inbound

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? cites this paper.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? What if string theory has a de Sitter excited state?

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.895560Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 657e44be-1721-46ed-b415-fcb087b0980b · inbound

Simple quintessence models in light of DESI-BAO observations cites this paper.

Simple quintessence models in light of DESI-BAO observations What if string theory has a de Sitter excited state?

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-07T00:43:07.905825Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6f645f6a-cd59-45cb-b6e1-c2cf4eee2463 · inbound

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

Dark energy from string theory: an introductory review What if string theory has a de Sitter excited state?

Reference 214

Resolution: verified exact; arxiv_id, observed 2026-05-15T00:18:22.046399Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 1e06c751-c2a8-47b6-9329-ba834a74d473 · inbound

Coherent states versus Glauber-Sudarshan States: Bootstrapping, Schwinger-Keldysh Contours and Lefschetz Thimbles cites this paper.

Coherent states versus Glauber-Sudarshan States: Bootstrapping, Schwinger-Keldysh Contours and Lefschetz Thimbles What if string theory has a de Sitter excited state?

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-04T04:11:20.039116Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.