Paper Citation Record · LEDGER

Can f(R) gravity contribute to (dark) radiation?

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1507.02623.

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

pith.paper-citation-record.v1
1507.02623 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T17:24:31.442861Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T18:45:59.652139Z

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 3d34699f-b49e-49a8-8805-5107e47e6d0c · inbound

Observational constraints on 3-forms dark energy cites this paper.

Observational constraints on 3-forms dark energy Can f(R) gravity contribute to (dark) radiation?

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-03T17:24:31.442861Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7e342ba0-0302-4303-91d2-8ea42f57ead8 · inbound

Three-form dark energy: constraints and multi-probe comparison with $\Lambda$CDM cites this paper.

Three-form dark energy: constraints and multi-probe comparison with $\Lambda$CDM Can f(R) gravity contribute to (dark) radiation?

Reference 35

Resolution: verified exact; local_arxiv, observed 2026-07-01T18:45:59.653312Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 04446004-252c-40d3-a87d-b98012c24990 · inbound

Three-form dark energy: constraints and multi-probe comparison with $\Lambda$CDM cites this paper.

Three-form dark energy: constraints and multi-probe comparison with $\Lambda$CDM Can f(R) gravity contribute to (dark) radiation?

Reference 35

Resolution: unresolved; no resolver link, observed 2026-07-13T07:19:36.090369Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4e61a5b0-9a75-4997-9e86-101e1d014220 · 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 Can f(R) gravity contribute to (dark) radiation?

Reference 46

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.