Pith. sign in

Paper Citation Record · LEDGER

Early Dark Energy with Power-law F(R) Gravity

As of 13 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.

pith.paper-citation-record.v1
2305.17513 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T17:09:38.238058Z

measured 0 of 1 external citation measurements

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

  • 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 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 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-05-23T23:39:08.448852Z digest=sha256:20ad73226a058a08f7c94f18b95cbef3def6e6ff9d2e917e8671c49625ce0b04

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.

source=pdf_text observed=2026-08-11T17:09:38.238058Z digest=sha256:8c381bce04ee491659f6d7b51f9d9d576830d5dae33177db1d4b6a88efb55ee2

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.

source=pdf_text observed=2026-08-10T05:59:55.542808Z digest=sha256:48281b41b94e6011f891e3b587d1472e5136d73b874f6fa5ac38974a4ea60eda

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.

source=pdf_text observed=2026-08-04T12:53:37.328833Z digest=sha256:0ccd04fa963e6c92c5269de2a36df5446ca7acadf05cbac844044723bcc22e54

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 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-05-10T12:56:21.466420Z digest=sha256:ed421e0a7308fceddfde71afc7066818d788307413f7e683fd515fd8ce57d737

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.

source=pdf_text observed=2026-08-01T08:08:45.528150Z digest=sha256:bd1d0db4c5a313d7747953119f38d5b1e26ce3c6c03cfbf59a5e146b7b8cc59e