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Quintom cosmology and modified gravity after DESI 2024

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 30 inbound Pith citation observations for arXiv:2404.19437.

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2404.19437 v2

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Observation cba383ca-7719-4c75-a2af-b08a5c762fc8 · 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? Quintom cosmology and modified gravity after DESI 2024

Reference 18

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

Scalar-Tensor Gravity and DESI 2024 BAO data Quintom cosmology and modified gravity after DESI 2024

Reference 22

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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 Quintom cosmology and modified gravity after DESI 2024

Reference 38

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

Extended Dark Energy analysis using DESI DR2 BAO measurements Quintom cosmology and modified gravity after DESI 2024

Reference 209

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On the tension between DESI DR2 BAO and CMB cites this paper.

On the tension between DESI DR2 BAO and CMB Quintom cosmology and modified gravity after DESI 2024

Reference 79

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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 Quintom cosmology and modified gravity after DESI 2024

Reference 63

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Geometric formulation of $k$-essence and late-time acceleration cites this paper.

Geometric formulation of $k$-essence and late-time acceleration Quintom cosmology and modified gravity after DESI 2024

Reference 57

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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 Quintom cosmology and modified gravity after DESI 2024

Reference 16

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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? Quintom cosmology and modified gravity after DESI 2024

Reference 13

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3-dimensional charged black holes in $f({Q})$ gravity cites this paper.

3-dimensional charged black holes in $f({Q})$ gravity Quintom cosmology and modified gravity after DESI 2024

Reference 34

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Cosmological preference for a positive neutrino mass at 2.7$\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data cites this paper.

Cosmological preference for a positive neutrino mass at 2.7$\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data Quintom cosmology and modified gravity after DESI 2024

Reference 49

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Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime cites this paper.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Quintom cosmology and modified gravity after DESI 2024

Reference 96

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Restoration of the Lorentz symmetry of particle propagator in the ghost condensate model cites this paper.

Restoration of the Lorentz symmetry of particle propagator in the ghost condensate model Quintom cosmology and modified gravity after DESI 2024

Reference 21

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Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder cites this paper.

Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder Quintom cosmology and modified gravity after DESI 2024

Reference 108

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Revisiting the Hubble tension problem in the framework of holographic dark energy cites this paper.

Revisiting the Hubble tension problem in the framework of holographic dark energy Quintom cosmology and modified gravity after DESI 2024

Reference 57

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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 Quintom cosmology and modified gravity after DESI 2024

Reference 49

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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 Quintom cosmology and modified gravity after DESI 2024

Reference 75

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Robust Preference for Dark Sector Interactions cites this paper.

Robust Preference for Dark Sector Interactions Quintom cosmology and modified gravity after DESI 2024

Reference 24

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Exponential Quintessence Model: Analytical Quantification of the Fine-Tuning Problem in Dark Energy cites this paper.

Exponential Quintessence Model: Analytical Quantification of the Fine-Tuning Problem in Dark Energy Quintom cosmology and modified gravity after DESI 2024

Reference 10

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UV-complete and stable Quintom Dark Energy models in the light of DESI DR2 cites this paper.

UV-complete and stable Quintom Dark Energy models in the light of DESI DR2 Quintom cosmology and modified gravity after DESI 2024

Reference 46

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The open-Universe signal: A model artifact rather than genuine curvature Quintom cosmology and modified gravity after DESI 2024

Reference 41

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Exponential Quintessence: Analytic Relationship Between the Current Equation of State Parameter and the Potential Parameter cites this paper.

Exponential Quintessence: Analytic Relationship Between the Current Equation of State Parameter and the Potential Parameter Quintom cosmology and modified gravity after DESI 2024

Reference 7

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A short review on Quintom dark energy theory Quintom cosmology and modified gravity after DESI 2024

Reference 28

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Reference 28

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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 Quintom cosmology and modified gravity after DESI 2024

Reference 20

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Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data cites this paper.

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data Quintom cosmology and modified gravity after DESI 2024

Reference 70

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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 Quintom cosmology and modified gravity after DESI 2024

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Phantom-Divide Crossing in Barrow-Tsallis Holographic Dark Energy with a Scale-Dependent Barrow Exponent cites this paper.

Phantom-Divide Crossing in Barrow-Tsallis Holographic Dark Energy with a Scale-Dependent Barrow Exponent Quintom cosmology and modified gravity after DESI 2024

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Higher-Order Analytical Expansion of Thawing Dark Energy with an Exponential Potential cites this paper.

Higher-Order Analytical Expansion of Thawing Dark Energy with an Exponential Potential Quintom cosmology and modified gravity after DESI 2024

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