Pith. sign in

Paper Citation Record · LEDGER

Phantom scalar-tensor models and cosmological tensions

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2302.05291.

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

pith.paper-citation-record.v1
2302.05291 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T15:36:19.575734Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-10T07:47:12.076669Z

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 6269de47-5e2e-4911-a408-02fb6478eb8e · inbound

Is Dark Energy an Effective Manifestation of Non-equilibrium Thermodynamics? -- Insights from DESI cites this paper.

Is Dark Energy an Effective Manifestation of Non-equilibrium Thermodynamics? -- Insights from DESI Phantom scalar-tensor models and cosmological tensions

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-06T15:36:19.575734Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T15:36:19.575734Z digest=sha256:b3ede5ea59f2734fe4e13f9c4d138a38ad90d946d1ac1147a4a937e36d1732a5

Observation 76069f19-e1f3-4b42-a64d-b3cbfd3c8cbe · 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 Phantom scalar-tensor models and cosmological tensions

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-04T12:53:36.840692Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T12:53:36.840692Z digest=sha256:31e92528dad930b0cef22f4fbda70c7b03ee8253249d2e2ef8a520c269eebd05

Observation 80067786-1a80-408c-80dc-83a26a91ee66 · inbound

Post-Newtonian Constraints on Scalar-Tensor Gravity cites this paper.

Post-Newtonian Constraints on Scalar-Tensor Gravity Phantom scalar-tensor models and cosmological tensions

Reference 96

Resolution
verified exact
arxiv_id, observed 2026-05-10T07:47:12.078055Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-10T07:46:58.535167Z digest=sha256:7954089b45ac08c5f97b9a204419fd0f30e9adbbe582008441b0ba6d89754584