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Paper Citation Record · LEDGER
Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 44 inbound Pith citation observations for arXiv:2405.00502.
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Pith citing papers
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Do Observations Prefer Thawing Quintessence? cites this paper.
Do Observations Prefer Thawing Quintessence? Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Reevaluating $H_0$ Tension with Non-Planck CMB and DESI BAO Joint Analysis cites this paper.
Reevaluating $H_0$ Tension with Non-Planck CMB and DESI BAO Joint Analysis Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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General parametrization for energy density of quintessence field cites this paper.
General parametrization for energy density of quintessence field Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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On the evidence of dynamical dark energy Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? cites this paper.
DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Composite Dark Energy and the Cosmological Tensions cites this paper.
Composite Dark Energy and the Cosmological Tensions Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Illustrating the consequences of a misuse of $\sigma_8$ in cosmology Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Scalar-Tensor Gravity and DESI 2024 BAO data Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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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 Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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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 Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Robustness of dark energy phenomenology across different parameterizations Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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An overview of what current data can (and cannot yet) say about evolving dark energy Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Physical vs phantom dark energy after DESI: thawing quintessence in a curved background cites this paper.
Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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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 Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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On the tension between DESI DR2 BAO and CMB Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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In search of an interaction in the dark sector through Gaussian Process and ANN approaches cites this paper.
In search of an interaction in the dark sector through Gaussian Process and ANN approaches Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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The Quintom theory of dark energy after DESI DR2 Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Can the universe experience an AdS landscape since matter-radiation equality? Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Constraints on Dark Energy Models Using Late Universe Probes cites this paper.
Constraints on Dark Energy Models Using Late Universe Probes Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Observation c3fd403f-b2a5-4e46-9748-d850f3991bec · 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 Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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New Insights into Dark Energy from DESI DR2 with CMB and SNIa Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Resolving the Planck-DESI tension by nonminimally coupled quintessence Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Cosmological constraints on Galileon dark energy with broken shift symmetry Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Updated observational constraints on $\phi$CDM dynamical dark energy cosmological models Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Beyond CPL: Evidence for dynamical dark energy in three-parameter models Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Observational constraints on early time non-phantom behaviour of dynamical dark energy Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Towards a unified quantum field theory of dark energy and inflation: unstable de Sitter vacuum and running vacuum Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Exploring the interplay of late-time dynamical dark energy and new physics before recombination Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck PR4 CMB anisotropy data? Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Negative neutrino mass or negative dark energy? Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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A short review on Quintom dark energy theory Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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A short review on Quintom dark energy theory Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Running Vacuum in the expanding Universe: a unified QFT paradigm for Inflation and Dark Energy cites this paper.
Running Vacuum in the expanding Universe: a unified QFT paradigm for Inflation and Dark Energy Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Running Vacuum in the expanding Universe: a unified QFT paradigm for Inflation and Dark Energy cites this paper.
Running Vacuum in the expanding Universe: a unified QFT paradigm for Inflation and Dark Energy Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Reconstructing dark energy with fewer assumptions cites this paper.
Reconstructing dark energy with fewer assumptions Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Cosmological Viability of Exponential Infrared $f(T)$ Gravity cites this paper.
Cosmological Viability of Exponential Infrared $f(T)$ Gravity Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Imprint of swampland-inspired coupled early dark energy Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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Evolving Dark Energy from the Back-Reaction of Cosmological Perturbations cites this paper.
Evolving Dark Energy from the Back-Reaction of Cosmological Perturbations Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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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 Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
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