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Paper Citation Record · LEDGER

Modified gravity interpretation of the evolving dark energy in light of DESI data

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 29 inbound Pith citation observations for arXiv:2407.02558.

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pith.paper-citation-record.v1
2407.02558 v2

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Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T15:54:50.972104Z

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Source: pith, observed 2026-07-09T13:46:17.503379Z

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Pith citing papers

Observation db729c9d-87cd-40fe-8f47-b37cd6b6e185 · inbound

Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity cites this paper.

Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 45

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Observation a7fb5bff-b9cb-4b2d-a3c0-3954929c8cba · inbound

Modified gravity/Dynamical Dark Energy vs $\Lambda$CDM: is the game over? cites this paper.

Modified gravity/Dynamical Dark Energy vs $\Lambda$CDM: is the game over? Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 35

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Observation 354b9272-91e9-4180-a05b-2fb4bb73b9c5 · inbound

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? Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 117

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Impact of DESI BAO Data on Inflationary Parameters: stability against late-time new physics cites this paper.

Impact of DESI BAO Data on Inflationary Parameters: stability against late-time new physics Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 50

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Observation d13c2965-4db6-4e82-9392-1e74808aad62 · inbound

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

Scalar-Tensor Gravity and DESI 2024 BAO data Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 28

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Observation cd9e2e36-12f9-4c39-ba3c-f92ba5b1baec · inbound

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

Dark energy and lensing anomaly in Planck CMB data Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 41

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Observation 25d10079-b8ea-45b7-821c-6288e92ee014 · inbound

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

Robustness of dark energy phenomenology across different parameterizations Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 49

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Observation b32aa3fc-f23e-4c78-8453-17356facb08a · inbound

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

The Quintom theory of dark energy after DESI DR2 Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 28

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Observation a84b9b51-f88d-41ac-9925-e50ccccb7e1b · inbound

Cosmological constraints on Galileon dark energy with broken shift symmetry cites this paper.

Cosmological constraints on Galileon dark energy with broken shift symmetry Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 23

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Beyond CPL: Evidence for dynamical dark energy in three-parameter models cites this paper.

Beyond CPL: Evidence for dynamical dark energy in three-parameter models Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 60

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Observation 6220e9cb-c319-456c-ab28-ef426c8f826c · inbound

DESI constraints on two-field quintessence with exponential potentials cites this paper.

DESI constraints on two-field quintessence with exponential potentials Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 57

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Observation 2a6a95db-c9ac-4e3f-899a-1ba39e8b4613 · inbound

Probing Dark Energy Microphysics with kSZ Tomography cites this paper.

Probing Dark Energy Microphysics with kSZ Tomography Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 73

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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 Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 22

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Observation 1fd1aab9-de40-4640-af91-85316a889862 · 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 Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 59

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The open-Universe signal: A model artifact rather than genuine curvature cites this paper.

The open-Universe signal: A model artifact rather than genuine curvature Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 40

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Late-time reconstruction of non-minimally coupled gravity with a smoothness prior cites this paper.

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 17

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The impact of evolving dark energy on the Weyl potential measured from the Dark Energy Survey Year 3 data cites this paper.

The impact of evolving dark energy on the Weyl potential measured from the Dark Energy Survey Year 3 data Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 20

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Charging Across the Phantom Divide with Modified Gravity cites this paper.

Charging Across the Phantom Divide with Modified Gravity Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 2

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The sound of dynamical dark energy and modified gravity cites this paper.

The sound of dynamical dark energy and modified gravity Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 44

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A short review on Quintom dark energy theory Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 46

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A short review on Quintom dark energy theory Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 46

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Reconstructing dark energy with fewer assumptions cites this paper.

Reconstructing dark energy with fewer assumptions Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 107

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

Constraining dark energy with complementary probes of large-scale structure Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 98

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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 Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 34

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Cosmological Constraints on the DGP Model in light of DESI DR2 2025 Data cites this paper.

Cosmological Constraints on the DGP Model in light of DESI DR2 2025 Data Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 53

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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 Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 47

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

Gravitational Wave Birefringence in generalized Palatini Chern Simons Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 42

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EFT-Ramses: a code to simulate the effective field theory of dark energy cites this paper.

EFT-Ramses: a code to simulate the effective field theory of dark energy Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 50

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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? Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 60

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