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Paper Citation Record · LEDGER

Is the dark energy equation of state parameter singular?

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 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 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T12:53:50.519248Z

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

  • 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 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.

source=pdf_text observed=2026-08-04T12:53:50.519248Z digest=sha256:4e90c8f13fc8d890b4ad08215dd8c705a863620bce6a806cf8f245266abedf3a

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 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-18T04:46:14.832965Z digest=sha256:822a1614ae5a589449b0239c4b34465c4eacdab8e7b3e31777ed47fc84ad1522

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 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-21T13:29:05.147292Z digest=sha256:d8f4008bf963f0ead72c0a4e83201d8b7d5a296a3d1458743449e057e22b6a2b

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.

source=pdf_text observed=2026-07-15T12:01:04.317365Z digest=sha256:7ae5a89f322edc20bae6045ad58f3f1a91f4975538f2a6cb41e4693d636bd65a

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 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-14T18:44:05.693005Z digest=sha256:09ecd4fdbe10bc4f465f78186a0185583943f72f8ce884e0a667f2a647ad4ed2

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 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-21T03:03:07.191130Z digest=sha256:e3b4488a3c0c6b2673af855afe1f1b14c71c32b6c410532022c9db35b508e885

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.

source=pdf_text observed=2026-07-11T09:40:49.196932Z digest=sha256:45df52bc893a67da1938605cfec5ba438efa8c8846044089b8858993300cc617

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.

source=pdf_text observed=2026-08-01T16:29:58.180093Z digest=sha256:32f032e6cd4904a1b5a230e78697372613d233dcd96b44cdf33f1c9f46367541