Paper Citation Record · LEDGER

Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 22 inbound Pith citation observations for arXiv:2503.24343.

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

pith.paper-citation-record.v1
2503.24343 v1

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measured 22 of 22 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T13:44:00.726992Z

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

Source: arxiv_reference, observed 2026-07-04T02:19:23.610351Z

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Outbound references

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Pith citing papers

Observation a269d2fe-83c2-4975-91ee-cf7e37598118 · inbound

The Quintom theory of dark energy after DESI DR2 cites this paper.

The Quintom theory of dark energy after DESI DR2 Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 124

Resolution: verified exact; arxiv_id, observed 2026-05-19T13:12:19.123504Z

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Observation b317ef12-0192-4307-81cf-526d3c6f7459 · inbound

Looking beyond lambda cites this paper.

Looking beyond lambda Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-05T13:44:00.726992Z

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Observation c239082a-65c8-4228-a5f5-01df7d2a6c81 · inbound

Observational constraints on the modified cosmology inspired by string T-duality cites this paper.

Observational constraints on the modified cosmology inspired by string T-duality Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-04T09:19:39.401951Z

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Observation e3417208-1c1a-4eb5-87e6-246156b5596c · inbound

Revisiting the Hubble tension problem in the framework of holographic dark energy cites this paper.

Revisiting the Hubble tension problem in the framework of holographic dark energy Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 46

Resolution: metadata mismatch; arxiv_id, observed 2026-05-17T22:20:23.622286Z

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Observation b83c34e3-857d-43ee-84d1-cc9b7a75f95f · inbound

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses cites this paper.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 56

Resolution: metadata mismatch; arxiv_id, observed 2026-05-17T04:19:00.904434Z

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Observation 33a15bea-8def-40f6-9d6b-1272e4b5dcd0 · inbound

Robust Preference for Dark Sector Interactions cites this paper.

Robust Preference for Dark Sector Interactions Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.703696Z

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Observation 0a5d3048-9dc1-4f50-9b05-c9b29b532ab0 · inbound

Model-Independent Reconstruction of Quintessence Potential and Kinetic Energy from DESI DR2 and Pantheon+ Supernovae cites this paper.

Model-Independent Reconstruction of Quintessence Potential and Kinetic Energy from DESI DR2 and Pantheon+ Supernovae Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 44

Resolution: verified exact; arxiv_id, observed 2026-05-15T01:33:27.413051Z

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Observation 2f0cd8f6-f623-42a6-9014-3f4df270eec2 · inbound

Exploring the interplay of late-time dynamical dark energy and new physics before recombination cites this paper.

Exploring the interplay of late-time dynamical dark energy and new physics before recombination Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 115

Resolution: verified exact; arxiv_id, observed 2026-05-14T23:13:14.703242Z

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Observation d2be86bb-31f0-4a55-81b7-8ca9b61b1c2f · inbound

In-depth analysis of the clustering of dark matter particles around primordial black holes. Part III: CMB constraints cites this paper.

In-depth analysis of the clustering of dark matter particles around primordial black holes. Part III: CMB constraints Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 68

Resolution: verified exact; arxiv_id, observed 2026-05-11T12:06:03.301465Z

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

Observation df54a8cc-b29c-4bca-a89f-7dfcf3170f44 · inbound

Exploring Cosmic Evolution in R\'enyi Entropic Cosmology with Constraints from DESI DR2 BAO and GW Data cites this paper.

Exploring Cosmic Evolution in R\'enyi Entropic Cosmology with Constraints from DESI DR2 BAO and GW Data Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 46

Resolution: verified exact; arxiv_id, observed 2026-05-11T20:01:09.823172Z

Source-reported events for the cited work

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Observation c4ca06e0-b7a7-4e13-b396-77f01765f3bb · inbound

From Big Bang Nucleosynthesis to Late-Time Acceleration in $f(Q,L_m)$ Gravity cites this paper.

From Big Bang Nucleosynthesis to Late-Time Acceleration in $f(Q,L_m)$ Gravity Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 64

Resolution: verified exact; arxiv_id, observed 2026-05-11T21:26:12.884143Z

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Observation b6e5f9e1-318f-4fa4-9449-e42c31f5b176 · inbound

Kinematic Lensing Ratio: Reviving Weak Lensing Cosmography as a Geometric Dark Energy Probe cites this paper.

Kinematic Lensing Ratio: Reviving Weak Lensing Cosmography as a Geometric Dark Energy Probe Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 13

Resolution: verified exact; arxiv_id, observed 2026-05-12T00:36:14.713440Z

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Observation 481ff8e7-f7d3-4696-942b-fba958250552 · inbound

Recoupled Dark Radiation reconciling CMB and DESI BAO measurements cites this paper.

Recoupled Dark Radiation reconciling CMB and DESI BAO measurements Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 14

Resolution: verified exact; arxiv_id, observed 2026-05-20T09:03:10.054760Z

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.

Observation 5fc3ee0d-477d-4b08-a69a-0603f8c1770b · inbound

Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background cites this paper.

Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 38

Resolution: verified exact; arxiv_id, observed 2026-05-22T05:41:08.685248Z

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.

Observation 882db7d9-7313-49b6-adde-fc15a598caf9 · inbound

Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background cites this paper.

Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-02T13:29:55.758840Z

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Observation 08c35d23-6554-42cb-b30f-f05b475a30a3 · inbound

Neutrino mass constraints in interacting dark energy models after DESI DR2 cites this paper.

Neutrino mass constraints in interacting dark energy models after DESI DR2 Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 34

Resolution: metadata mismatch; arxiv_id, observed 2026-07-02T10:56:52.400591Z

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.

Observation e508c977-23f7-4324-ac8e-782f096f8e16 · inbound

On the potential for inhomogeneities to mimic an evolving dark energy cites this paper.

On the potential for inhomogeneities to mimic an evolving dark energy Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 20

Resolution: verified exact; arxiv_id, observed 2026-07-02T11:16:53.161033Z

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

Observation 18b9f8cf-58ff-469c-85a5-b81684b48190 · inbound

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data cites this paper.

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 79

Resolution: metadata mismatch; arxiv_id, observed 2026-07-04T02:19:23.611982Z

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.

Observation e6078a49-696d-40fd-9f5c-97a0f9751f4e · inbound

The $H_0$ World Cup. I. Summary of the baseline group stage results cites this paper.

The $H_0$ World Cup. I. Summary of the baseline group stage results Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-02T05:41:38.177110Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 41b820b0-9084-4ad3-9152-46ed4be1e84a · inbound

The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions cites this paper.

The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-02T05:48:11.535770Z

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Observation 3208f2f5-23bd-44e3-989e-8ff93ad2cf20 · inbound

General Relativistic Entropic Acceleration at the perturbation level: a CLASS implementation and first Boltzmann-code constraints cites this paper.

General Relativistic Entropic Acceleration at the perturbation level: a CLASS implementation and first Boltzmann-code constraints Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 113

Resolution: unresolved; no resolver link, observed 2026-08-01T01:25:44.295962Z

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Observation cdf0b41c-8b02-46b1-9838-b1e2f5025d35 · inbound

Boosting the optical depth to Thomson scattering with primordial black hole evaporation at high redshift cites this paper.

Boosting the optical depth to Thomson scattering with primordial black hole evaporation at high redshift Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-04T18:21:12.920576Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.