Interpreting DESI's evidence for evolving dark energy | Paper Citation Record

Observation 052b9f48-98f3-47a1-a7bb-19eb1a7d4f98 · inbound

Assessing observational constraints on dark energy cites this paper.

Assessing observational constraints on dark energy Interpreting DESI's evidence for evolving dark energy

Reference 31

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Observation 22b84b43-f3b7-4547-a7ef-d0418f9ed15d · inbound

Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension cites this paper.

Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension Interpreting DESI's evidence for evolving dark energy

Reference 19

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Upper limits on dark energy-dark matter interaction from DESI DR2 in a field-theoretic analysis cites this paper.

Upper limits on dark energy-dark matter interaction from DESI DR2 in a field-theoretic analysis Interpreting DESI's evidence for evolving dark energy

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Bridge the Cosmological Tensions with Thawing Gravity cites this paper.

Bridge the Cosmological Tensions with Thawing Gravity Interpreting DESI's evidence for evolving dark energy

Reference 16

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On the evidence of dynamical dark energy cites this paper.

On the evidence of dynamical dark energy Interpreting DESI's evidence for evolving dark energy

Reference 12

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Observation 8bbd22be-72a0-4832-8e3c-b1c4a97ded78 · inbound

A preference for dynamical phantom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data cites this paper.

A preference for dynamical phantom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data Interpreting DESI's evidence for evolving dark energy

Reference 96

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Newest measurements of Hubble constant from DESI 2024 BAO observations cites this paper.

Newest measurements of Hubble constant from DESI 2024 BAO observations Interpreting DESI's evidence for evolving dark energy

Reference 12

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ cites this paper.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Interpreting DESI's evidence for evolving dark energy

Reference 13

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Alleviating cosmological tensions with a hybrid dark sector cites this paper.

Alleviating cosmological tensions with a hybrid dark sector Interpreting DESI's evidence for evolving dark energy

Reference 34

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Observation 52bcaf1a-f497-40cc-a140-8f27cca8e6be · inbound

Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? cites this paper.

Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? Interpreting DESI's evidence for evolving dark energy

Reference 13

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Illustrating the consequences of a misuse of $\sigma_8$ in cosmology cites this paper.

Illustrating the consequences of a misuse of $\sigma_8$ in cosmology Interpreting DESI's evidence for evolving dark energy

Reference 156

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Scalar-Tensor Gravity and DESI 2024 BAO data cites this paper.

Scalar-Tensor Gravity and DESI 2024 BAO data Interpreting DESI's evidence for evolving dark energy

Reference 20

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Observation a80af285-7250-4bf0-b6db-fa113cf80bac · inbound

The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae cites this paper.

The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Interpreting DESI's evidence for evolving dark energy

Reference 43

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Dark energy and lensing anomaly in Planck CMB data cites this paper.

Dark energy and lensing anomaly in Planck CMB data Interpreting DESI's evidence for evolving dark energy

Reference 5

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

Robustness of dark energy phenomenology across different parameterizations Interpreting DESI's evidence for evolving dark energy

Reference 83

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An overview of what current data can (and cannot yet) say about evolving dark energy cites this paper.

An overview of what current data can (and cannot yet) say about evolving dark energy Interpreting DESI's evidence for evolving dark energy

Reference 202

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Observation 2788946d-c068-41ef-91a7-d639124649ef · inbound

Evidence for non-cold dark matter from DESI DR2 measurements cites this paper.

Evidence for non-cold dark matter from DESI DR2 measurements Interpreting DESI's evidence for evolving dark energy

Reference 42

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Updated Constraints on Omnipotent Dark Energy: A Comprehensive Analysis with CMB and BAO Data cites this paper.

Updated Constraints on Omnipotent Dark Energy: A Comprehensive Analysis with CMB and BAO Data Interpreting DESI's evidence for evolving dark energy

Reference 92

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Baryon Acoustic Oscillations from a Different Angle cites this paper.

Baryon Acoustic Oscillations from a Different Angle Interpreting DESI's evidence for evolving dark energy

Reference 6

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The matter with(in) CPL cites this paper.

The matter with(in) CPL Interpreting DESI's evidence for evolving dark energy

Reference 14

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Observation 1cb854d5-b7fd-46e1-9e07-5b515bda127a · inbound

Examining Quintessence Models with DESI Data cites this paper.

Examining Quintessence Models with DESI Data Interpreting DESI's evidence for evolving dark energy

Reference 9

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

The Quintom theory of dark energy after DESI DR2 Interpreting DESI's evidence for evolving dark energy

Reference 13

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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? Interpreting DESI's evidence for evolving dark energy

Reference 8

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Bayesian and frequentist perspectives agree on dynamical dark energy cites this paper.

Bayesian and frequentist perspectives agree on dynamical dark energy Interpreting DESI's evidence for evolving dark energy

Reference 25

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Observation 917051f6-cb77-4e6c-9716-219ec78a0071 · inbound

Dark Energy Crosses the Line: Quantifying and Testing the Evidence for Phantom Crossing cites this paper.

Dark Energy Crosses the Line: Quantifying and Testing the Evidence for Phantom Crossing Interpreting DESI's evidence for evolving dark energy

Reference 65

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New Insights into Dark Energy from DESI DR2 with CMB and SNIa cites this paper.

New Insights into Dark Energy from DESI DR2 with CMB and SNIa Interpreting DESI's evidence for evolving dark energy

Reference 38

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Observation 77bc2dda-1b35-470b-be6b-ef95309d2ebc · inbound

Is Dark Energy an Effective Manifestation of Non-equilibrium Thermodynamics? -- Insights from DESI cites this paper.

Is Dark Energy an Effective Manifestation of Non-equilibrium Thermodynamics? -- Insights from DESI Interpreting DESI's evidence for evolving dark energy

Reference 145

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Connecting Early Dark Energy to Late Dark Energy by the Diluting Matter Potential cites this paper.

Connecting Early Dark Energy to Late Dark Energy by the Diluting Matter Potential Interpreting DESI's evidence for evolving dark energy

Reference 12

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Interacting $k$-essence field with non-pressureless Dark Matter: Cosmological Dynamics and Observational Constraints cites this paper.

Interacting $k$-essence field with non-pressureless Dark Matter: Cosmological Dynamics and Observational Constraints Interpreting DESI's evidence for evolving dark energy

Reference 34

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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 Interpreting DESI's evidence for evolving dark energy

Reference 79

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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 Interpreting DESI's evidence for evolving dark energy

Reference 115

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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 Interpreting DESI's evidence for evolving dark energy

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Cosmology of axion dark energy in supersymmetric models and constraints on high scale parameters cites this paper.

Cosmology of axion dark energy in supersymmetric models and constraints on high scale parameters Interpreting DESI's evidence for evolving dark energy

Reference 44

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Robust Preference for Dark Sector Interactions cites this paper.

Robust Preference for Dark Sector Interactions Interpreting DESI's evidence for evolving dark energy

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Is Phantom Divide Crossing in General Relativity Completely Impossible? Shortcomings in canonical and minimally coupled scalar field and Possible Solutions in $k$-essence Models cites this paper.

Is Phantom Divide Crossing in General Relativity Completely Impossible? Shortcomings in canonical and minimally coupled scalar field and Possible Solutions in $k$-essence Models Interpreting DESI's evidence for evolving dark energy

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Probing dynamical dark energy with late-time data: Evidence, tensions, and the limits of the $w_0w_a$CDM framework cites this paper.

Probing dynamical dark energy with late-time data: Evidence, tensions, and the limits of the $w_0w_a$CDM framework Interpreting DESI's evidence for evolving dark energy

Reference 185

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Scaling solutions in three-form cosmology cites this paper.

Scaling solutions in three-form cosmology Interpreting DESI's evidence for evolving dark energy

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families cites this paper.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Interpreting DESI's evidence for evolving dark energy

Reference 194

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On the origin of the BAOtr-DESI tension cites this paper.

On the origin of the BAOtr-DESI tension Interpreting DESI's evidence for evolving dark energy

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Negative neutrino mass or negative dark energy? cites this paper.

Negative neutrino mass or negative dark energy? Interpreting DESI's evidence for evolving dark energy

Reference 123

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A short review on Quintom dark energy theory cites this paper.

A short review on Quintom dark energy theory Interpreting DESI's evidence for evolving dark energy

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A short review on Quintom dark energy theory cites this paper.

A short review on Quintom dark energy theory Interpreting DESI's evidence for evolving dark energy

Reference 13

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Cosmic variance or galaxy bias? Disentangling finite-volume and galaxy formation effects in cosmological analysis cites this paper.

Cosmic variance or galaxy bias? Disentangling finite-volume and galaxy formation effects in cosmological analysis Interpreting DESI's evidence for evolving dark energy

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Cosmic variance or galaxy bias? Disentangling finite-volume and galaxy formation effects in cosmological analysis cites this paper.

Cosmic variance or galaxy bias? Disentangling finite-volume and galaxy formation effects in cosmological analysis Interpreting DESI's evidence for evolving dark energy

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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 Interpreting DESI's evidence for evolving dark energy

Reference 11

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Reconstructing dark energy with fewer assumptions cites this paper.

Reconstructing dark energy with fewer assumptions Interpreting DESI's evidence for evolving dark energy

Reference 37

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On the potential of pseudo-scalar dark energy cites this paper.

On the potential of pseudo-scalar dark energy Interpreting DESI's evidence for evolving dark energy

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Data-Driven Discovery of a Simple Phantom-Crossing Dark Energy Parametrization cites this paper.

Data-Driven Discovery of a Simple Phantom-Crossing Dark Energy Parametrization Interpreting DESI's evidence for evolving dark energy

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A hierarchical Bayesian framework for cosmology using Type 1 AGN variability cites this paper.

A hierarchical Bayesian framework for cosmology using Type 1 AGN variability Interpreting DESI's evidence for evolving dark energy

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Universal distance modes from DESI BAO and Type Ia supernovae: what do cosmological rulers actually measure? cites this paper.

Universal distance modes from DESI BAO and Type Ia supernovae: what do cosmological rulers actually measure? Interpreting DESI's evidence for evolving dark energy

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Cosmological Viability of Exponential Infrared $f(T)$ Gravity cites this paper.

Cosmological Viability of Exponential Infrared $f(T)$ Gravity Interpreting DESI's evidence for evolving dark energy

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Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation cites this paper.

Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation Interpreting DESI's evidence for evolving dark energy

Reference 118

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

Imprint of swampland-inspired coupled early dark energy Interpreting DESI's evidence for evolving dark energy

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Present Day Cosmic Acceleration from SDSS and DESI BAO: A Call for Finer Tomography of the DESI Bright Galaxy Survey cites this paper.

Present Day Cosmic Acceleration from SDSS and DESI BAO: A Call for Finer Tomography of the DESI Bright Galaxy Survey Interpreting DESI's evidence for evolving dark energy

Reference 38

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

Breaking the Dark Sector Degeneracy with Nonparametric Expansion--Growth Reconstruction Interpreting DESI's evidence for evolving dark energy

Reference 29

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Observation b8351d74-5ec3-4fa8-822a-fcbe0bd5a71a · inbound

Evaporating cosmologically coupled black holes cites this paper.

Evaporating cosmologically coupled black holes Interpreting DESI's evidence for evolving dark energy

Reference 239

Resolution: unresolved; no resolver link, observed 2026-08-02T03:36:03.650991Z

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Observation 68104a23-5e55-4560-9c10-2dfa59887b10 · inbound

High resolution Lyman-{\alpha} forest constraints on dark matter-neutrino scattering cites this paper.

High resolution Lyman-{\alpha} forest constraints on dark matter-neutrino scattering Interpreting DESI's evidence for evolving dark energy

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-02T00:29:39.525865Z

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Observation 555fbc70-0760-46f5-a21d-442e46c8de0f · inbound

Gravitational Wave Birefringence in generalized Palatini Chern Simons cites this paper.

Gravitational Wave Birefringence in generalized Palatini Chern Simons Interpreting DESI's evidence for evolving dark energy

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-01T09:44:13.315541Z

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Observation 6cd31230-b096-486d-9b12-88e3f6023dcb · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall Interpreting DESI's evidence for evolving dark energy

Reference 275

Resolution: unresolved; no resolver link, observed 2026-08-01T08:09:01.178809Z

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Observation d9ccf055-7bcd-4cd7-9cdd-5e0b92cb7adb · 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 Interpreting DESI's evidence for evolving dark energy

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-01T01:25:44.070811Z

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Observation 45e0818d-0163-4ff5-bf3c-0cc873488ec0 · inbound

A Sequentially-Valid Reanalysis of DESI's Dynamical Dark Energy Signal cites this paper.

A Sequentially-Valid Reanalysis of DESI's Dynamical Dark Energy Signal Interpreting DESI's evidence for evolving dark energy

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-03T17:20:49.003536Z

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Observation b20a690f-a8ba-404d-8a7b-9fc2df729dbe · 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? Interpreting DESI's evidence for evolving dark energy

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.390235Z

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