Paper Citation Record · LEDGER

Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2502.15541.

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

pith.paper-citation-record.v1
2502.15541 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T10:52:56.388965Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-08T15:55:04.885749Z

Reference resolution

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 3e4a2939-401a-4591-a58a-008afcca455e · inbound

Can the universe experience an AdS landscape since matter-radiation equality? cites this paper.

Can the universe experience an AdS landscape since matter-radiation equality? Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:56.388965Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e71cafa8-ec88-4069-b808-612cd642d8ec · 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 Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-04T12:53:40.603587Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3df0a110-39d4-4da0-ae7a-8063007c5700 · inbound

Beyond CPL: Evidence for dynamical dark energy in three-parameter models cites this paper.

Beyond CPL: Evidence for dynamical dark energy in three-parameter models Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$

Reference 74

Resolution: verified exact; arxiv_id, observed 2026-05-18T10:46:16.660741Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation e03d971e-87d5-42dc-a94f-b5e62ac342e1 · inbound

Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder cites this paper.

Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-04T07:19:37.649327Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7281ff48-79bc-4abb-93bd-d9727b8626cf · inbound

Observational constraints on early time non-phantom behaviour of dynamical dark energy cites this paper.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-03T14:40:55.500232Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation aa96b343-3d4b-4c00-b858-9dea1042a807 · 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 Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$

Reference 141

Resolution: verified exact; arxiv_id, observed 2026-05-11T11:36:03.772026Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 58b199f4-d71b-48b0-a00b-0df5d346f7d7 · inbound

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions cites this paper.

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$

Reference 132

Resolution: metadata mismatch; arxiv_id, observed 2026-07-01T16:45:51.112107Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation c169f564-163b-47b0-b4b4-d2ef9cce28f2 · inbound

Imprint of swampland-inspired coupled early dark energy cites this paper.

Imprint of swampland-inspired coupled early dark energy Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$

Reference 61

Resolution: verified exact; local_arxiv, observed 2026-07-08T15:55:04.887076Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 04284295-17ba-4df9-a40a-8cff70a20902 · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$

Reference 158

Resolution: unresolved; no resolver link, observed 2026-08-01T08:08:49.066582Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 42b5eef7-c7e4-4bae-aa23-0df3021f43d1 · inbound

Hubble tension: a short review of theoretical explanations cites this paper.

Hubble tension: a short review of theoretical explanations Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$

Reference 152

Resolution: unresolved; no resolver link, observed 2026-08-01T07:20:07.967357Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.