Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Early Dark Energy with Power-law F(R) Gravity
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2305.17513.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T17:09:38.238058Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-23T23:43:38.307523Z
Reference resolution
0 of 0 outbound references displayed
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- 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 b4c3f2a8-53e7-4b68-b951-4e11faf0d693 · inbound
Theoretical and observational constraints on early dark energy in $F(R)$ gravity cites this paper.
Theoretical and observational constraints on early dark energy in $F(R)$ gravity Early Dark Energy with Power-law F(R) Gravity
Reference 18
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:43:38.311599Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 7d6ad45e-8155-4bde-bfae-c3dcd1cefcc9 · inbound
Modified gravity/Dynamical Dark Energy vs $\Lambda$CDM: is the game over? cites this paper.
Modified gravity/Dynamical Dark Energy vs $\Lambda$CDM: is the game over? Early Dark Energy with Power-law F(R) Gravity
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T17:09:38.238058Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e6635828-84a3-407d-a96e-f3d9dd30aa7c · inbound
Can the sound horizon-free measurement of $H_0$ constrain early new physics? cites this paper.
Can the sound horizon-free measurement of $H_0$ constrain early new physics? Early Dark Energy with Power-law F(R) Gravity
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T05:59:55.542808Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fb04ab88-41bb-4781-a5b3-5d31d0d2f7f1 · 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 Early Dark Energy with Power-law F(R) Gravity
Reference 62
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T12:53:37.328833Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d404c8af-09f3-4df8-975f-afff2fccfd37 · inbound
Double the axions, half the tension: multi-field early dark energy eases the Hubble tension cites this paper.
Double the axions, half the tension: multi-field early dark energy eases the Hubble tension Early Dark Energy with Power-law F(R) Gravity
Reference 128
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T11:41:01.849021Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 85be148c-4958-46ad-b41b-ffd3a3ad97d5 · inbound
Hubble tension: the shape wall cites this paper.
Hubble tension: the shape wall Early Dark Energy with Power-law F(R) Gravity
Reference 127
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T08:08:45.528150Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.