Paper Citation Record · LEDGER

The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2502.12667.

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pith.paper-citation-record.v1
2502.12667 v2

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measured 9 of 9 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T00:54:47.313142Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-29T15:43:33.165476Z

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Outbound references

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Pith citing papers

Observation b6a1356d-d8cc-41f7-89b1-de8cbd1891f4 · inbound

Constraints on Dark Energy Models Using Late Universe Probes cites this paper.

Constraints on Dark Energy Models Using Late Universe Probes The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations

Reference 106

Resolution: unresolved; no resolver link, observed 2026-08-07T00:54:47.313142Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 95ea8dff-4434-4347-bbdd-9cfc903596b1 · inbound

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM cites this paper.

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations

Reference 210

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:55.493069Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 9119dd78-95ba-41fe-b0eb-1be2ba21f599 · inbound

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy cites this paper.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations

Reference 46

Resolution: unresolved; no resolver link, observed 2026-07-15T14:51:12.413085Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3f821f9c-889c-48a5-a21c-20816c3c46cd · 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 The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations

Reference 33

Resolution: verified exact; arxiv_id, observed 2026-05-22T05:41:08.707994Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation f2176e5d-b789-414d-bd93-718dae0c7066 · inbound

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

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-02T13:29:55.148946Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation aa4ff9bb-cb7b-4bd8-8ff3-59c22832bb9d · inbound

Effective Phantom Dark Energy: What Cosmological Reconstruction Does and Does Not Imply cites this paper.

Effective Phantom Dark Energy: What Cosmological Reconstruction Does and Does Not Imply The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations

Reference 41

Resolution: verified exact; arxiv_id, observed 2026-06-29T15:43:33.167045Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation fca727b8-de3a-4034-95cc-5d72946da7eb · inbound

Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae cites this paper.

Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations

Reference 61

Resolution: unresolved; no resolver link, observed 2026-07-14T16:44:02.461654Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 99b5e7c2-0964-4948-8a05-de5e33837606 · inbound

Breaking the Dark Sector Degeneracy with Nonparametric Expansion--Growth Reconstruction cites this paper.

Breaking the Dark Sector Degeneracy with Nonparametric Expansion--Growth Reconstruction The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations

Reference 28

Resolution: unresolved; no resolver link, observed 2026-07-14T03:00:21.146194Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 10ce66c5-c205-4d7c-94c6-7504e88d3440 · inbound

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? cites this paper.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.208976Z

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Unavailable: canonical work link unavailable.