Paper Citation Record · LEDGER

Preference for evolving dark energy in light of the galaxy bispectrum

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 19 inbound Pith citation observations for arXiv:2503.04602.

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

pith.paper-citation-record.v1
2503.04602 v2

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measured 19 of 19 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 19 of 19 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T21:04:17.789776Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

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External citation measurements

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arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 4ec5102a-1ba9-4878-a735-d25ff1769f1b · inbound

Robustness of dark energy phenomenology across different parameterizations cites this paper.

Robustness of dark energy phenomenology across different parameterizations Preference for evolving dark energy in light of the galaxy bispectrum

Reference 74

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Observation 1d3db2fb-008e-4562-a387-8f0f181dd2d4 · inbound

The simple way to measure evolving dark energy without prior-volume effects cites this paper.

The simple way to measure evolving dark energy without prior-volume effects Preference for evolving dark energy in light of the galaxy bispectrum

Reference 86

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Observation 66d6f4a3-88ae-4722-bdc9-cff4d4de00c4 · inbound

Probing the sound speed and clustering of dark energy cites this paper.

Probing the sound speed and clustering of dark energy Preference for evolving dark energy in light of the galaxy bispectrum

Reference 9

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Observation b33f5638-dd46-4dab-804d-3d55f620ef6d · inbound

Controlled Tension Forecasting: Quantifying Cross-Probe Biases in $\omega_0\omega_a$CDM cites this paper.

Controlled Tension Forecasting: Quantifying Cross-Probe Biases in $\omega_0\omega_a$CDM Preference for evolving dark energy in light of the galaxy bispectrum

Reference 60

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Observation 30cac4a3-0d27-4cf0-b652-f539996f4bee · inbound

Decoupling perturbations from background in $f(Q)$ gravity: the square-root correction and the impact on the $\sigma_8$ tension cites this paper.

Decoupling perturbations from background in $f(Q)$ gravity: the square-root correction and the impact on the $\sigma_8$ tension Preference for evolving dark energy in light of the galaxy bispectrum

Reference 82

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Observation 3f77a340-4a7c-448d-9c45-e2ab77e54b92 · 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 Preference for evolving dark energy in light of the galaxy bispectrum

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-03T14:40:55.482565Z

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Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy cites this paper.

Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy Preference for evolving dark energy in light of the galaxy bispectrum

Reference 202

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Observation 474c9306-1d7e-44d4-92fc-ed4c11b791b1 · 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 Preference for evolving dark energy in light of the galaxy bispectrum

Reference 77

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Observation 1799911b-f2b0-4d50-823f-6f64656a81f0 · inbound

FolpsD: combining EFT and phenomenological approaches for joint power spectrum and bispectrum analyses cites this paper.

FolpsD: combining EFT and phenomenological approaches for joint power spectrum and bispectrum analyses Preference for evolving dark energy in light of the galaxy bispectrum

Reference 45

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Observation 69d49b39-f6c7-43f7-9691-1860d0d59d17 · inbound

Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges cites this paper.

Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges Preference for evolving dark energy in light of the galaxy bispectrum

Reference 35

Resolution: verified exact; arxiv_id, observed 2026-05-11T17:56:05.567011Z

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Observation 0cca8dae-28ee-4d73-afc0-d9a7d35864f6 · inbound

Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges cites this paper.

Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges Preference for evolving dark energy in light of the galaxy bispectrum

Reference 41

Resolution: verified exact; arxiv_id, observed 2026-06-30T23:25:07.663384Z

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Observation 77f3730a-fef6-4887-a243-56f41a1a1030 · 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 Preference for evolving dark energy in light of the galaxy bispectrum

Reference 36

Resolution: verified exact; arxiv_id, observed 2026-05-22T05:41:08.695172Z

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Observation cb724ba9-4e21-4b95-b1a2-64d1188cc439 · 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 Preference for evolving dark energy in light of the galaxy bispectrum

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-02T13:29:55.487937Z

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Observation 3950a6fc-7069-4d75-b287-a6c17f13a612 · inbound

Exploring non-Poisson satellite occupation in HOD models and its impact on 2- and 3-point galaxy clustering cites this paper.

Exploring non-Poisson satellite occupation in HOD models and its impact on 2- and 3-point galaxy clustering Preference for evolving dark energy in light of the galaxy bispectrum

Reference 41

Resolution: verified exact; arxiv_id, observed 2026-06-29T10:43:18.397675Z

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Observation bda70f54-6493-47c3-9522-060612fbcc9b · inbound

First full-shape joint analysis of the two- and three-point correlation functions on real data: $\Lambda$CDM cosmological constraints from BOSS DR12 cites this paper.

First full-shape joint analysis of the two- and three-point correlation functions on real data: $\Lambda$CDM cosmological constraints from BOSS DR12 Preference for evolving dark energy in light of the galaxy bispectrum

Reference 14

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Observation 84b4f8d2-778a-4f34-b234-345bbad54cef · inbound

Constraining dark energy with complementary probes of large-scale structure cites this paper.

Constraining dark energy with complementary probes of large-scale structure Preference for evolving dark energy in light of the galaxy bispectrum

Reference 103

Resolution: verified exact; arxiv_id, observed 2026-07-01T11:55:42.873903Z

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Observation c4e612d3-b261-44bd-84c9-3fbfcfe3ace1 · inbound

Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization cites this paper.

Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization Preference for evolving dark energy in light of the galaxy bispectrum

Reference 57

Resolution: verified exact; arxiv_id, observed 2026-07-03T06:27:41.636165Z

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Observation 5bb9ee6c-0616-472b-b4bc-965b689cc046 · inbound

Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization cites this paper.

Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization Preference for evolving dark energy in light of the galaxy bispectrum

Reference 57

Resolution: unresolved; no resolver link, observed 2026-07-12T08:00:27.085537Z

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Observation 40ad9ba8-29fd-4bde-9bbd-859ac66d52ac · 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 Preference for evolving dark energy in light of the galaxy bispectrum

Reference 218

Resolution: unresolved; no resolver link, observed 2026-08-02T05:48:26.022291Z

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