Paper Citation Record · LEDGER

Is the dark energy equation of state parameter singular?

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2203.04167.

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

pith.paper-citation-record.v1
2203.04167 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 11 of 11 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T10:37:59.858020Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-21T13:30:11.895580Z

Reference resolution

0 of 0 outbound references displayed

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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 345fcdae-0c7a-4335-b6b7-d49ee732ef59 · inbound

Updated Constraints on Omnipotent Dark Energy: A Comprehensive Analysis with CMB and BAO Data cites this paper.

Updated Constraints on Omnipotent Dark Energy: A Comprehensive Analysis with CMB and BAO Data Is the dark energy equation of state parameter singular?

Reference 131

Resolution: unresolved; no resolver link, observed 2026-08-16T10:37:59.858020Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ed692bba-837a-41fc-bb91-7f53def625a5 · inbound

Phantom matters cites this paper.

Phantom matters Is the dark energy equation of state parameter singular?

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-15T21:15:07.344780Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 04ae6453-2844-4f30-8798-6817c549bea3 · inbound

Dark Energy Crosses the Line: Quantifying and Testing the Evidence for Phantom Crossing cites this paper.

Dark Energy Crosses the Line: Quantifying and Testing the Evidence for Phantom Crossing Is the dark energy equation of state parameter singular?

Reference 110

Resolution: unresolved; no resolver link, observed 2026-08-15T18:44:19.060623Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 02efd72a-a683-456e-aad1-1ea2a6b3fbd6 · 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 Is the dark energy equation of state parameter singular?

Reference 206

Resolution: unresolved; no resolver link, observed 2026-08-04T12:53:50.519248Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 372cb316-39eb-4a6d-a373-1282f437c40c · 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 Is the dark energy equation of state parameter singular?

Reference 171

Resolution: metadata mismatch; arxiv_id, observed 2026-05-18T04:50:55.692719Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation fa1d2f30-2fac-402c-8efa-236fb99c8628 · 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 Is the dark energy equation of state parameter singular?

Reference 123

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:11.897375Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 41aab168-bc95-44a8-9d54-c70ebd00947e · 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 Is the dark energy equation of state parameter singular?

Reference 134

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 c7e71de5-9705-4623-83cd-ec942e61e2f3 · inbound

Latent-Space Gaussian Processes for Dark-Energy Reconstruction from Observational $H(z)$ Data cites this paper.

Latent-Space Gaussian Processes for Dark-Energy Reconstruction from Observational $H(z)$ Data Is the dark energy equation of state parameter singular?

Reference 51

Resolution: metadata mismatch; arxiv_id, observed 2026-05-14T18:47:37.110998Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 6dbdb85b-daa8-456a-b7b8-8a1c70cfbcc7 · inbound

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

Negative neutrino mass or negative dark energy? Is the dark energy equation of state parameter singular?

Reference 61

Resolution: metadata mismatch; arxiv_id, observed 2026-05-21T03:03:55.668006Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 897a70be-60d2-464b-8280-1ab232f7440a · 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 Is the dark energy equation of state parameter singular?

Reference 112

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eb34fd8a-5273-49fc-abb2-bb7bec4693fa · inbound

Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide cites this paper.

Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide Is the dark energy equation of state parameter singular?

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-01T16:29:58.180093Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.