Paper Citation Record · LEDGER

From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 16 inbound Pith citation observations for arXiv:2404.17334.

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

pith.paper-citation-record.v1
2404.17334 v3

Coverage vector

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Source: paper_references, paper_reference_links

measured 16 of 16 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 16 of 16 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T18:12:34.929579Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T07:07:44.893202Z

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External citation measurements

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Outbound references

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Pith citing papers

Observation 9aec2752-4374-42af-bac8-dfc7a2086c27 · inbound

$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity cites this paper.

$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension

Reference 86

Resolution: verified exact; arxiv_id, observed 2026-05-24T03:53:54.672229Z

Source-reported events for the cited work

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Observation ba6efaa4-93e3-49a2-9926-a648aec304e2 · inbound

Illustrating the consequences of a misuse of $\sigma_8$ in cosmology cites this paper.

Illustrating the consequences of a misuse of $\sigma_8$ in cosmology From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension

Reference 257

Resolution: unresolved; no resolver link, observed 2026-08-10T18:12:34.929579Z

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Observation c4e76459-59b8-4128-ae6c-445c026062b0 · inbound

Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate cites this paper.

Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-10T01:13:35.502179Z

Source-reported events for the cited work

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Observation dcf42c9c-471a-4ca9-ba58-94abe976d9b6 · inbound

Cosmographic analysis of sign-switching dark energy cites this paper.

Cosmographic analysis of sign-switching dark energy From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-07T01:08:41.763527Z

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Observation 4d0bdba3-429f-42d8-97c6-8c53330bcd46 · inbound

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM cites this paper.

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension

Reference 191

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:54.656352Z

Source-reported events for the cited work

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Observation 607706a7-74d9-4b7b-a0e3-6247e395b974 · inbound

Probing dynamical dark energy with late-time data: Evidence, tensions, and the limits of the $w_0w_a$CDM framework cites this paper.

Probing dynamical dark energy with late-time data: Evidence, tensions, and the limits of the $w_0w_a$CDM framework From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension

Reference 90

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:12.492143Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 82d6505f-033d-4cfe-83e8-6eb746b93b76 · inbound

Sign-Switching Dark Energy: Smooth Transitions with Recent DESI DR2 Observations cites this paper.

Sign-Switching Dark Energy: Smooth Transitions with Recent DESI DR2 Observations From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension

Reference 101

Resolution: verified exact; arxiv_id, observed 2026-05-16T05:20:39.363227Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation c5e2e941-2143-4302-93ba-4d004d30d9d3 · inbound

Statistical consistency of sign-switching vacuum energy with cosmological observations cites this paper.

Statistical consistency of sign-switching vacuum energy with cosmological observations From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-02T18:35:52.572704Z

Source-reported events for the cited work

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Observation b98b49e6-3d30-4876-899b-6187f7cfe8f5 · inbound

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families cites this paper.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension

Reference 99

Resolution: unresolved; no resolver link, observed 2026-07-15T12:01:04.317365Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b6e23fdf-00ea-44e0-848c-4a3f96aff3ca · inbound

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? cites this paper.

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension

Reference 51

Resolution: verified exact; arxiv_id, observed 2026-05-10T14:15:30.017973Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 4c46b4ff-7c65-413f-b770-a04dabd73ed3 · inbound

Negative neutrino mass or negative dark energy? cites this paper.

Negative neutrino mass or negative dark energy? From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension

Reference 85

Resolution: verified exact; arxiv_id, observed 2026-05-21T03:03:55.308502Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 0ca334cc-fb46-4ff6-a7ef-420139a3dac6 · inbound

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 cites this paper.

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension

Reference 99

Resolution: verified exact; arxiv_id, observed 2026-07-02T15:37:06.294204Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 30daeb11-0241-4836-929e-a14169dc9c9e · inbound

Endpoint Logarithms in the NLO Mueller-Navelet Jet Vertex: Threshold Matching and BLM/MOM Prescription Sensitivity cites this paper.

Endpoint Logarithms in the NLO Mueller-Navelet Jet Vertex: Threshold Matching and BLM/MOM Prescription Sensitivity From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension

Reference 23

Resolution: unresolved; no resolver link, observed 2026-07-12T14:25:03.782538Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cb3bb5b1-e79b-4d40-87b4-012f93331c43 · inbound

A Friendly Phantom: Late-time AdS-to-dS transition and cosmological tensions cites this paper.

A Friendly Phantom: Late-time AdS-to-dS transition and cosmological tensions From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension

Reference 23

Resolution: verified exact; arxiv_id, observed 2026-07-03T07:07:44.894410Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 7801b6ac-5ff2-43ed-b68d-b3af2b31869a · inbound

Cosmological Viability of Exponential Infrared $f(T)$ Gravity cites this paper.

Cosmological Viability of Exponential Infrared $f(T)$ Gravity From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension

Reference 187

Resolution: verified exact; arxiv_id, observed 2026-07-01T11:15:42.687139Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 2cf72ccc-dca3-4816-a14e-a9f6fd326a6e · inbound

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus cites this paper.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension

Reference 78

Resolution: unresolved; no resolver link, observed 2026-07-11T09:40:49.196932Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.