Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? | Paper Citation Record

Observation 57b6654a-9990-4bb8-801a-c6da7ef29a71 · outbound

This paper cites Gu et al.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Gu et al

Reference 1

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Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Unresolved cited work

Reference 2

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Observation 32063eec-fb08-42f1-af0a-2c6c426328f0 · outbound

This paper cites [80, 113], al- lowing a direct comparison with previous quintessence reconstructions.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? [80, 113], al- lowing a direct comparison with previous quintessence reconstructions

Reference 3

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Observation 1224453a-8877-449d-986b-71267fbdc22e · outbound

This paper cites Quintessential interpretation of the evolving dark energy in light of DESI.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Quintessential interpretation of the evolving dark energy in light of DESI

Reference 4

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Observation b41e3923-47d6-477a-a52f-44e125d99da9 · outbound

This paper cites Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 5

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Observation d6fffb48-efb1-4905-930e-146c057360a1 · outbound

This paper cites Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements

Reference 6

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Observation 9e80a9ff-69ab-46ec-af54-728da2099ca1 · outbound

This paper cites Characterizing repulsive gravity with curvature eigenvalues.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Characterizing repulsive gravity with curvature eigenvalues

Reference 7

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This paper cites Toward an invariant definition of repulsive gravity.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Toward an invariant definition of repulsive gravity

Reference 8

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Observation bc011bdc-3b4e-4e71-a487-51ff90dba051 · outbound

This paper cites Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

Reference 9

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Observation e72ea97b-c1b8-40bf-b603-81ec6b30483c · outbound

This paper cites Measurements of Omega and Lambda from 42 High-Redshift Supernovae.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Measurements of Omega and Lambda from 42 High-Redshift Supernovae

Reference 10

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Observation 246f68c4-e6f2-4563-bea0-dc405b3585ca · outbound

This paper cites Dynamics of dark energy.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Dynamics of dark energy

Reference 11

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This paper cites an unresolved cited work.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Unresolved cited work

Reference 12

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Observation 17ee339b-0ec4-4081-9a79-05c3f95b73dd · outbound

This paper cites The Cosmological Constant and Dark Energy.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? The Cosmological Constant and Dark Energy

Reference 13

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Observation c8d188cc-d9f5-4145-af09-d1bf78b46730 · outbound

This paper cites Dark Energy and the Accelerating Universe.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Dark Energy and the Accelerating Universe

Reference 14

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Observation 61391701-be08-4252-8e11-83a8a6e3a2c1 · outbound

This paper cites Sahni, Lect.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Sahni, Lect

Reference 15

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Observation 92c7a69b-9bb5-46c3-b315-c940c538e790 · outbound

This paper cites Dark Energy: Mystery of the Millennium.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Dark Energy: Mystery of the Millennium

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:09.167139Z

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Observation a35a0b12-584a-4491-8909-2099aaadeb7b · outbound

This paper cites The Physics of Cosmic Acceleration.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? The Physics of Cosmic Acceleration

Reference 17

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Observation fde8455d-b174-4fc5-8a5a-954d67278192 · outbound

This paper cites Dark energy constraints using gamma-ray burst correlations with DESI 2024 data.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Dark energy constraints using gamma-ray burst correlations with DESI 2024 data

Reference 18

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Observation 9531ea9b-ed9b-4a0f-828c-004dc04e8bbd · outbound

This paper cites Dark energy reconstructions combining BAO data with galaxy clusters and intermediate redshift catalogs.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Dark energy reconstructions combining BAO data with galaxy clusters and intermediate redshift catalogs

Reference 19

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Observation 5ce55254-5cf1-472f-8c24-5bb1cd17c6a1 · outbound

This paper cites Cosmic distance duality after DESI 2024 data release and dark energy evolution.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Cosmic distance duality after DESI 2024 data release and dark energy evolution

Reference 20

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Observation a2ae82f1-d882-48ad-85db-0ac9c780d04e · outbound

This paper cites Testing generalized logotropic models with cosmic growth.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Testing generalized logotropic models with cosmic growth

Reference 21

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Observation 1ca13ffc-deb8-4f69-a0ed-62243e1eae7e · outbound

This paper cites Unifying the dark sector through a single matter fluid with non-zero pressure.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Unifying the dark sector through a single matter fluid with non-zero pressure

Reference 22

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Observation dca929ee-6567-4cfa-8046-4c9c58f8dbbc · outbound

This paper cites Cosmological constraints from calibrated $E_p-E_{iso}$ gamma-ray burst correlation by using DESI 2024 data release.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Cosmological constraints from calibrated $E_p-E_{iso}$ gamma-ray burst correlation by using DESI 2024 data release

Reference 23

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Observation 5ade8b90-248a-4fdf-b5f7-8ad371ef98f9 · outbound

This paper cites Intermediate redshift calibration of Gamma-ray Bursts and cosmic constraints in non-flat cosmology.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Intermediate redshift calibration of Gamma-ray Bursts and cosmic constraints in non-flat cosmology

Reference 24

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Observation 85110423-7916-4c74-9f66-0efce5e406aa · outbound

This paper cites Cosmological transition epoch from gamma-ray burst correlations.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Cosmological transition epoch from gamma-ray burst correlations

Reference 25

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Observation 8dc0f1c6-f4a5-4fe2-9ba9-ba90db229f6f · outbound

This paper cites Phase-space analysis of dark energy models in non-minimally coupled theories of gravity.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Phase-space analysis of dark energy models in non-minimally coupled theories of gravity

Reference 26

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Observation 80709519-026f-4bde-9584-93f0596fe290 · outbound

This paper cites Dark Energy and Dark Matter from an additional adiabatic fluid.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Dark Energy and Dark Matter from an additional adiabatic fluid

Reference 27

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Observation 090c635b-8c75-40b6-bdf8-9eab03ff85dd · outbound

This paper cites Tracing dark energy history with gamma ray bursts.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Tracing dark energy history with gamma ray bursts

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:10.487974Z

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Observation 73150dc5-cbc8-4524-a1f1-9ce2482cab8a · outbound

This paper cites Observational Probes of Cosmic Acceleration.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Observational Probes of Cosmic Acceleration

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:10.631561Z

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Observation 9128f0db-13de-4570-aba8-0c1feac0f40b · outbound

This paper cites Planck 2018 results. VI. Cosmological parameters.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Planck 2018 results. VI. Cosmological parameters

Reference 30

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This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory

Reference 31

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Observation f8da5b22-e51e-432f-aa72-ad3866a5af1e · outbound

This paper cites Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

Reference 32

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Observation c5ddfaf0-726d-46a8-86a0-2166d1779391 · outbound

This paper cites The Pantheon+ Analysis: Cosmological Constraints.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? The Pantheon+ Analysis: Cosmological Constraints

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:10.885513Z

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Observation 570e7d24-79e4-41c7-b10d-31fdbbc0454d · outbound

This paper cites Dark energy two decades after: Observables, probes, consistency tests.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Dark energy two decades after: Observables, probes, consistency tests

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:10.990197Z

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Observation fecc8ce8-e8bb-4b67-a1a2-0ad627031964 · outbound

This paper cites First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters

Reference 35

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Observation 43288993-d7a5-4b6d-9ace-abc819a47da6 · outbound

This paper cites Cosmological parameters from SDSS and WMAP.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Cosmological parameters from SDSS and WMAP

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.006887Z

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Observation 6a5df22a-6939-45f9-bc85-c12de7123aec · outbound

This paper cites The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.014814Z

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Observation 12228873-fa33-4d33-8109-8a0d4dc7c1e0 · outbound

This paper cites The Case for a Positive Cosmological Lambda-term.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? The Case for a Positive Cosmological Lambda-term

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.019484Z

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Observation 6ac6a124-0ef5-40c3-adb3-c6edbc4c48cb · outbound

This paper cites Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask).

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask)

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.024361Z

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Observation e577929a-85ef-4ebc-ab9e-e680b68a9e4f · outbound

This paper cites Quintessence, Cosmic Coincidence, and the Cosmological Constant.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Quintessence, Cosmic Coincidence, and the Cosmological Constant

Reference 40

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Observation caa51b3f-eac7-4b45-b23d-918039a020fe · outbound

This paper cites Aspects of the cosmological "coincidence problem".

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Aspects of the cosmological "coincidence problem"

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.034465Z

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Observation 40b4e231-0e88-4b4f-8956-c92a0ecc0d53 · outbound

This paper cites The Cosmological Constant Problem: Why it's hard to get Dark Energy from Micro-physics.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? The Cosmological Constant Problem: Why it's hard to get Dark Energy from Micro-physics

Reference 42

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Observation 1f5018af-0ba7-48e9-bef9-68c0b7c60f41 · outbound

This paper cites Nobbenhuis, Found.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Nobbenhuis, Found

Reference 43

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Observation d94132d1-90bf-453e-9f87-511be1cab6c0 · outbound

This paper cites Dalal, K.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Dalal, K

Reference 44

Resolution: verified exact; raw_fallback, observed 2026-08-06T00:32:14.212720Z

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Observation 64d54350-2007-44dd-a927-5c008950b47a · outbound

This paper cites Luongo and H.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Luongo and H

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.058918Z

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Observation 8da8a455-afd7-4051-b134-cefbc6423836 · outbound

This paper cites Speeding up the universe using dust with pressure.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Speeding up the universe using dust with pressure

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.062737Z

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Observation c25f1267-cee2-4eb2-a163-f93893a3e61a · outbound

This paper cites Particle production from non-minimal coupling in a symmetry breaking potential transporting vacuum energy.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Particle production from non-minimal coupling in a symmetry breaking potential transporting vacuum energy

Reference 47

Resolution: verified exact; local_arxiv, observed 2026-08-06T00:32:14.110726Z

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Observation 19e634c1-fe9e-4ac0-83d5-eb20ff0bc4f3 · outbound

This paper cites Weinberg, Rev.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Weinberg, Rev

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.070940Z

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Observation d2f3f2b2-3a96-4aa8-83b1-1051a03e2ac5 · outbound

This paper cites Likely Values of the Cosmological Constant.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Likely Values of the Cosmological Constant

Reference 49

Resolution: verified exact; local_arxiv, observed 2026-08-06T00:32:14.091286Z

Source-reported events for the cited work

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Observation 0fd3fcfc-bf6c-4e1f-a647-77855824ad4f · outbound

This paper cites The Cosmological Constant Problems (Talk given at Dark Matter 2000, February, 2000).

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? The Cosmological Constant Problems (Talk given at Dark Matter 2000, February, 2000)

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.078926Z

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Observation 0d94b509-088d-4929-9cbb-c98dbeca8727 · outbound

This paper cites Padmanabhan, Phys.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Padmanabhan, Phys

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.083066Z

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Observation 99489945-27e2-42a3-8cd8-db03550d6739 · outbound

This paper cites The Hubble tension: A decade review.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? The Hubble tension: A decade review

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.086838Z

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Observation 637f0599-b03b-43db-83fd-d93643b00071 · outbound

This paper cites In the Realm of the Hubble tension $-$ a Review of Solutions.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? In the Realm of the Hubble tension $-$ a Review of Solutions

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.090404Z

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Observation a63c08c7-878c-425b-9c0e-89ce1855becc · outbound

This paper cites Carloni, O.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Carloni, O

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.100322Z

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Observation bfbac74d-f73c-4b94-9103-c19f711e811c · outbound

This paper cites A barotropic alternative to Early Dark Energy for alleviating the $H_0$ tension.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? A barotropic alternative to Early Dark Energy for alleviating the $H_0$ tension

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.104995Z

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Observation 63065687-ff31-4b11-ab20-24f01ae7d09a · outbound

This paper cites Pantos and L.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Pantos and L

Reference 56

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Observation 01923800-2845-4dac-9f1a-de81b3d3a115 · outbound

This paper cites DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 57

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Observation 3f8cdd07-cdf9-4e9d-af58-713f54e36ab9 · outbound

This paper cites DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 58

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Observation e2c0518a-86e8-417c-b0c9-006947fad4f1 · outbound

This paper cites Extended Dark Energy analysis using DESI DR2 BAO measurements.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Extended Dark Energy analysis using DESI DR2 BAO measurements

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.122150Z

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Observation c5415dc7-8847-436f-8001-30899c111599 · outbound

This paper cites Modified gravity interpretation of the evolving dark energy in light of DESI data.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 60

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Observation b2c27abc-26a9-4a6c-8f58-fee2cb893274 · outbound

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

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Robustness of dark energy phenomenology across different parameterizations

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.134748Z

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Observation 2a7daf22-d2c6-4a87-abda-086c43e4b37d · outbound

This paper cites Comparing the DES-SN5YR and Pantheon+ SN cosmology analyses: Investigation based on "Evolving Dark Energy or Supernovae systematics?".

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Comparing the DES-SN5YR and Pantheon+ SN cosmology analyses: Investigation based on "Evolving Dark Energy or Supernovae systematics?"

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.141326Z

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Observation 8628664c-00df-49a8-a661-109c032baa30 · outbound

This paper cites Model independent cosmographic constraints from DESI 2024.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Model independent cosmographic constraints from DESI 2024

Reference 63

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Observation d92ca940-8fbe-43c3-9856-7cfefb1dbe52 · outbound

This paper cites Does dark energy really revive using DESI 2024 data?.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Does dark energy really revive using DESI 2024 data?

Reference 64

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Observation 0c02bf7e-a4c3-4fde-8bd4-69bb792ca581 · outbound

This paper cites Evolving Dark Energy or Supernovae Systematics?.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Evolving Dark Energy or Supernovae Systematics?

Reference 65

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Observation 9d948f91-c504-4d78-8c95-918af8458237 · outbound

This paper cites Baryon Acoustic Oscillations from a Different Angle.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Baryon Acoustic Oscillations from a Different Angle

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.172771Z

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Observation 72327413-0314-49d0-8b1f-55c289d98273 · outbound

This paper cites Afroz and S.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Afroz and S

Reference 67

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Observation eaacb246-02e1-4725-aeb0-64dc312e6360 · outbound

This paper cites de Souza, A.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? de Souza, A

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.186389Z

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Observation d92f815b-229a-48f9-a494-01171dbc2c9f · outbound

This paper cites DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 69

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Observation ed2c5dea-062c-48aa-9e23-8f9b653c9130 · outbound

This paper cites Does DESI 2024 Confirm $\Lambda$CDM?.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Does DESI 2024 Confirm $\Lambda$CDM?

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.193723Z

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Observation e2a40adf-5a43-40dd-b4ce-4c6cac42461b · outbound

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Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Unresolved cited work

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.198036Z

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Observation d78c1ae0-cece-42d9-a613-3dbcf1ecb27f · outbound

This paper cites an unresolved cited work.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Unresolved cited work

Reference 72

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

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

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

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Observation aea7c8d6-7a5d-49f1-999c-4648965ede7c · outbound

This paper cites Evidence for dynamical dark energy from DESI-DR2 and SN data? A symbolic regression analysis.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Evidence for dynamical dark energy from DESI-DR2 and SN data? A symbolic regression analysis

Reference 74

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Observation b99a30b7-458f-497a-966a-d8c426e888a7 · outbound

This paper cites Accelerating Universes with Scaling Dark Matter.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Accelerating Universes with Scaling Dark Matter

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.238339Z

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Observation 4e0e95df-221e-4a74-ba7c-ce9aca269eab · outbound

This paper cites Probing the dark energy: methods and strategies.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Probing the dark energy: methods and strategies

Reference 76

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Observation c19c375c-3fb7-4118-a389-25116adf4cc4 · outbound

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Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Unresolved cited work

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.257613Z

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Observation 471e3520-1621-4ba1-98fd-2f1cbfb893ab · outbound

This paper cites Report of the Dark Energy Task Force.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Report of the Dark Energy Task Force

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.280376Z

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Observation 841db605-d31b-4f15-85f8-324bafebd8f2 · outbound

This paper cites an unresolved cited work.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Unresolved cited work

Reference 79

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Observation 7e11433c-0b8c-4e9b-8fd5-4d7cd0dcf5cb · outbound

This paper cites Observational constraints on dynamical dark energy with pivoting redshift.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Observational constraints on dynamical dark energy with pivoting redshift

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.355467Z

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Observation b20a690f-a8ba-404d-8a7b-9fc2df729dbe · outbound

This paper cites Interpreting DESI's evidence for evolving dark energy.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Interpreting DESI's evidence for evolving dark energy

Reference 81

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Observation 99584a29-2cd6-4a84-9abf-a53de6a1ffa6 · outbound

This paper cites Montefalcone and R.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Montefalcone and R

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.416558Z

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Observation b5df43b4-a72c-4471-95a4-b0343f9a55cd · outbound

This paper cites Uncorrelated Estimates of Dark Energy Evolution.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Uncorrelated Estimates of Dark Energy Evolution

Reference 83

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Observation f6606d56-2ca2-466f-b0e0-a7580a5397da · outbound

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Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Probing Dark Energy Using Its Density Instead of Its Equation of State

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.495220Z

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Observation 415beb72-12c3-4a34-8708-91299d7a4fc5 · outbound

This paper cites Four New Observational $H(z)$ Data From Luminous Red Galaxies of Sloan Digital Sky Survey Data Release Seven.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Four New Observational $H(z)$ Data From Luminous Red Galaxies of Sloan Digital Sky Survey Data Release Seven

Reference 85

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Observation bf403b45-28ec-45ec-90f6-f156d608c35f · outbound

This paper cites Constraining Cosmological Parameters Based on Relative Galaxy Ages.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Constraining Cosmological Parameters Based on Relative Galaxy Ages

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.567995Z

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Observation a8e7847d-79a7-4dee-9391-e9d8750c3903 · outbound

This paper cites Constraints on the redshift dependence of the dark energy potential.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Constraints on the redshift dependence of the dark energy potential

Reference 87

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Observation f00f1649-0ccf-4f45-bce2-c9d3c08d0da5 · outbound

This paper cites Improved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Improved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.639066Z

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Observation c84095bf-0159-4ad2-b887-342fcac58bc1 · outbound

This paper cites A 6% measurement of the Hubble parameter at $z\sim0.45$: direct evidence of the epoch of cosmic re-acceleration.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? A 6% measurement of the Hubble parameter at $z\sim0.45$: direct evidence of the epoch of cosmic re-acceleration

Reference 89

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Observation 3c8f9b55-c715-4257-b301-7c288fb7c7fb · outbound

This paper cites Age-dating Luminous Red Galaxies observed with the Southern African Large Telescope.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Age-dating Luminous Red Galaxies observed with the Southern African Large Telescope

Reference 90

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Observation 3e327b0b-b1aa-4e28-b8ce-e2056771f9a5 · outbound

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Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements

Reference 91

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Observation 089799fe-7ad6-4cf7-9e1b-9a56ae7497a1 · outbound

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Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Toward a Better Understanding of Cosmic Chronometers: A new measurement of H(z) at z~0.7

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.778434Z

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Observation ff6e0705-863d-4644-a42d-bf3cd655c1f3 · outbound

This paper cites Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z$\sim$2.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z$\sim$2

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.806057Z

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Observation 17cf60b0-5f89-48bc-b220-2554e9db740f · outbound

This paper cites A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.842470Z

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Observation 3d411708-e19a-4a63-8dfb-25a8820a0efd · outbound

This paper cites Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.878877Z

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Observation e91578b7-e874-4ad7-a641-44c51c2f3c14 · outbound

This paper cites The Hubble Tension and Early Dark Energy.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? The Hubble Tension and Early Dark Energy

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.913666Z

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This paper cites an unresolved cited work.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Unresolved cited work

Reference 97

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Observation e67d662f-b666-4eff-8f2d-f7c16d69413b · outbound

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Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Carloni, O

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.965644Z

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This paper cites Measuring the effective complexity of cosmological models.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Measuring the effective complexity of cosmological models

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.995298Z

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Observation c67508dd-d3f4-4e0c-97d7-b143a970db49 · outbound

This paper cites Sugiura, Communications in Statistics - Theory and Methods7, 13 (1978).

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Sugiura, Communications in Statistics - Theory and Methods7, 13 (1978)

Reference 100

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