Paper Citation Record · LEDGER

Observational constraints on early time non-phantom behaviour of dynamical dark energy

As of 21 August 2026, this Paper Citation Record lists 100 of 117 outbound references and 4 inbound Pith citation observations for arXiv:2512.19888.

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2512.19888 v2

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Outbound references

Observation 921089a6-5c44-4d10-8da3-14a73e6d823e · outbound

This paper cites Scaling+Thawing.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Scaling+Thawing

Reference 1

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Observation 3543e2a5-c99a-4838-ada2-9011f0b0be3b · outbound

This paper cites This demonstrates that the early dark energy fraction is tightly constrained to be very small for scaling-type dynamics, which therefore appear unable to alleviate theH 0 tension.

Observational constraints on early time non-phantom behaviour of dynamical dark energy This demonstrates that the early dark energy fraction is tightly constrained to be very small for scaling-type dynamics, which therefore appear unable to alleviate theH 0 tension

Reference 2

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Observation 88c89662-0e72-49e7-bbca-25fd8c78f93a · outbound

This paper cites an unresolved cited work.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Unresolved cited work

Reference 3

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Observation 3270292a-25c8-4ebf-b749-cb9abc13dd52 · outbound

This paper cites Dynamics of dark energy.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Dynamics of dark energy

Reference 4

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Observation 8445cc2a-4db7-4d06-a14a-8345e4afa6b9 · outbound

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

Observational constraints on early time non-phantom behaviour of dynamical dark energy Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask)

Reference 5

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Observation 70d2fd52-84cf-4c6c-a80f-fe7d8ce39c67 · outbound

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

Observational constraints on early time non-phantom behaviour of dynamical dark energy The Case for a Positive Cosmological Lambda-term

Reference 6

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Observation 3dc39fa3-43ca-46d8-825c-8971139c71cb · outbound

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

Observational constraints on early time non-phantom behaviour of dynamical dark energy Planck 2018 results. VI. Cosmological parameters

Reference 7

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Observation 507687a0-4963-4eae-991a-26589551270a · 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.

Observational constraints on early time non-phantom behaviour of dynamical dark energy 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 8

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Observation b655234b-2337-4003-b6e8-34ce74f737d5 · outbound

This paper cites Challenges for $\Lambda$CDM: An update.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Challenges for $\Lambda$CDM: An update

Reference 9

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Observation 55fbaa3f-7331-482b-aa4c-1660413f7a2f · outbound

This paper cites DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys.

Observational constraints on early time non-phantom behaviour of dynamical dark energy DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys

Reference 10

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Observation 6ffd2af8-f3e0-46b7-b474-899a722ef9f8 · outbound

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

Observational constraints on early time non-phantom behaviour of dynamical dark energy DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 11

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Observation 760a3c4d-b701-458a-aff1-6d5ad6f86a3c · outbound

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

Observational constraints on early time non-phantom behaviour of dynamical dark energy DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 12

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Observation 4b7bd47c-7f0f-41a1-9f3c-f8bba72a60a0 · outbound

This paper cites Guet al.(DESI), Nature Astron.9, 1879 (2025), arXiv:2504.06118 [astro-ph.CO].

Observational constraints on early time non-phantom behaviour of dynamical dark energy Guet al.(DESI), Nature Astron.9, 1879 (2025), arXiv:2504.06118 [astro-ph.CO]

Reference 13

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Observation 809db830-17ff-452e-87da-f6e51e7afcab · outbound

This paper cites DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data.

Observational constraints on early time non-phantom behaviour of dynamical dark energy DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data

Reference 14

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Observation 3e3a7d97-a329-47fd-8123-b00427ff0283 · outbound

This paper cites DESI 2024: Constraints on Physics-Focused Aspects of Dark Energy using DESI DR1 BAO Data.

Observational constraints on early time non-phantom behaviour of dynamical dark energy DESI 2024: Constraints on Physics-Focused Aspects of Dark Energy using DESI DR1 BAO Data

Reference 15

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Observation 28bf4d10-4a1d-4c5d-88aa-3ae7925f5c53 · outbound

This paper cites Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements

Reference 16

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Observation b46f91f2-5082-4e9b-84ef-1dab7bdb4b70 · outbound

This paper cites Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements

Reference 17

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Observation 2db8cc5b-b934-4bbc-a877-84f70a68c7c9 · outbound

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

Observational constraints on early time non-phantom behaviour of dynamical dark energy Robustness of dark energy phenomenology across different parameterizations

Reference 18

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Unresolved cited work

Reference 19

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Observation ebb339c8-1eaf-47e8-adbb-6ddb4fdc0e31 · outbound

This paper cites Zhong and B.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Zhong and B

Reference 20

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Observation 85ebe87e-c9de-4159-9e23-ee062f5a99b5 · outbound

This paper cites A General Model for Dark Energy Crossing the Phantom Divide.

Observational constraints on early time non-phantom behaviour of dynamical dark energy A General Model for Dark Energy Crossing the Phantom Divide

Reference 21

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Observation 8184af23-82e5-46a3-a559-00103f2425fe · outbound

This paper cites Accelerated inference on accelerated cosmic expansion: New constraints on axion-like early dark energy with DESI BAO and ACT DR6 CMB lensing.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Accelerated inference on accelerated cosmic expansion: New constraints on axion-like early dark energy with DESI BAO and ACT DR6 CMB lensing

Reference 22

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Observation 05047357-eb68-4fc5-9447-708ac7d81e22 · outbound

This paper cites Dark energy in light of recent DESI BAO and Hubble tension.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Dark energy in light of recent DESI BAO and Hubble tension

Reference 23

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Observation 9a0e5ec6-67f1-468e-b438-b27e47300c3d · outbound

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

Observational constraints on early time non-phantom behaviour of dynamical dark energy Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements

Reference 24

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Observation 238d8d88-0a8d-4a28-a176-9c9aecf5a292 · outbound

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

Observational constraints on early time non-phantom behaviour of dynamical dark energy Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 25

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Assessing observational constraints on dark energy

Reference 26

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Observation 6037ec7f-7568-4b15-9ff0-c89244a1b645 · outbound

This paper cites Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements

Reference 27

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Cosmological constraints on curved quintessence

Reference 28

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Observation f584a6c8-c47f-4504-b9c1-370802ba08e0 · outbound

This paper cites DESI Constraints on Exponential Quintessence.

Observational constraints on early time non-phantom behaviour of dynamical dark energy DESI Constraints on Exponential Quintessence

Reference 29

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This paper cites Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data

Reference 30

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This paper cites Do Observations Prefer Thawing Quintessence?.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Do Observations Prefer Thawing Quintessence?

Reference 31

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This paper cites Cosmological constraints on dark energy parametrizations after DESI 2024: Persistent deviation from standard $\Lambda$CDM cosmology.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Cosmological constraints on dark energy parametrizations after DESI 2024: Persistent deviation from standard $\Lambda$CDM cosmology

Reference 32

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Underdetermination of dark energy

Reference 33

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Scant evidence for thawing quintessence

Reference 34

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This paper cites Matching current observational constraints with nonminimally coupled dark energy.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Matching current observational constraints with nonminimally coupled dark energy

Reference 35

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This paper cites Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result.

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

Reference 37

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This paper cites A new diagnostic for the null test of dynamical dark energy in light of DESI 2024 and other BAO data.

Observational constraints on early time non-phantom behaviour of dynamical dark energy A new diagnostic for the null test of dynamical dark energy in light of DESI 2024 and other BAO data

Reference 38

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This paper cites Model-agnostic assessment of dark energy after DESI DR1 BAO.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 39

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 40

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Does DESI 2024 Confirm $\Lambda$CDM?

Reference 41

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Bhattacharya, G

Reference 42

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Observational constraints on early time non-phantom behaviour of dynamical dark energy General parametrization for energy density of quintessence field

Reference 43

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations?

Reference 44

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Scalar-Tensor Gravity and DESI 2024 BAO data

Reference 45

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Dark energy and lensing anomaly in Planck CMB data

Reference 46

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Observational constraints on early time non-phantom behaviour of dynamical dark energy DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 47

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Mukherjee and A

Reference 48

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Mukherjee, D

Reference 49

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Mukherjee and A

Reference 50

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity

Reference 51

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This paper cites Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data

Reference 52

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Revisiting holographic dark energy after DESI 2024

Reference 53

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Li, G.-H

Reference 54

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Bounded Dark Energy

Reference 55

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Does dark energy really revive using DESI 2024 data?

Reference 56

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Unresolved cited work

Reference 57

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Observation d9a8ea36-2989-4362-b14e-15dc10e95c27 · outbound

This paper cites Assessing cosmological evidence for non-minimal coupling.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Assessing cosmological evidence for non-minimal coupling

Reference 58

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

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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This paper cites Quintessential early dark energy.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Quintessential early dark energy

Reference 60

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Reference 61

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This paper cites Cheng, E.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Cheng, E

Reference 62

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This paper cites Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition

Reference 63

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Observation 22b4fc8d-91d5-4289-bec4-8928b75cece5 · outbound

This paper cites BAO miscalibration cannot rescue late-time solutions to the Hubble tension.

Observational constraints on early time non-phantom behaviour of dynamical dark energy BAO miscalibration cannot rescue late-time solutions to the Hubble tension

Reference 64

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This paper cites The state of the dark energy equation of state circa 2023.

Observational constraints on early time non-phantom behaviour of dynamical dark energy The state of the dark energy equation of state circa 2023

Reference 65

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Unresolved cited work

Reference 66

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Observation 3f77a340-4a7c-448d-9c45-e2ab77e54b92 · outbound

This paper cites Preference for evolving dark energy in light of the galaxy bispectrum.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Preference for evolving dark energy in light of the galaxy bispectrum

Reference 67

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

Observational constraints on early time non-phantom behaviour of dynamical dark energy Cosmological constraints on Galileon dark energy with broken shift symmetry

Reference 68

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This paper cites Simple quintessence models in light of DESI-BAO observations.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Simple quintessence models in light of DESI-BAO observations

Reference 69

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Can the universe experience an AdS landscape since matter-radiation equality?

Reference 70

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Van Raamsdonk and C

Reference 71

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Peng, J.-Q

Reference 72

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This paper cites Yang, Eur.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Yang, Eur

Reference 73

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This paper cites Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$

Reference 74

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Ishak and L

Reference 75

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This paper cites Optimal parameterizations for observational constraints on thawing dark energy.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Optimal parameterizations for observational constraints on thawing dark energy

Reference 76

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Silva and R

Reference 77

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Unresolved cited work

Reference 78

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Observation 773d128c-d1ff-4e1b-841d-6abe3f3f899c · outbound

This paper cites Cortˆ es and A.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Cortˆ es and A

Reference 79

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Artola, I

Reference 80

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Unresolved cited work

Reference 81

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This paper cites Updated observational constraints on $\phi$CDM dynamical dark energy cosmological models.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Updated observational constraints on $\phi$CDM dynamical dark energy cosmological models

Reference 82

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Blanco, V

Reference 83

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Li, G.-H

Reference 84

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This paper cites Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2

Reference 85

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Beyond CPL: Evidence for dynamical dark energy in three-parameter models

Reference 86

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This paper cites Probing the sensitivity of dark energy dynamics to equation of state parametrization flexibility.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Probing the sensitivity of dark energy dynamics to equation of state parametrization flexibility

Reference 87

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This paper cites Nojiri, S.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Nojiri, S

Reference 88

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Nojiri, S

Reference 89

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This paper cites Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck CMB anisotropy data?.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck CMB anisotropy data?

Reference 90

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Observational constraints on early time non-phantom behaviour of dynamical dark energy Accelerating Universes with Scaling Dark Matter

Reference 91

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This paper cites Exploring the Expansion History of the Universe.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Exploring the Expansion History of the Universe

Reference 92

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This paper cites Exponential potentials and cosmological scaling solutions.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Exponential potentials and cosmological scaling solutions

Reference 93

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This paper cites Variable gravity: A suitable framework for quintessential inflation.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Variable gravity: A suitable framework for quintessential inflation

Reference 94

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This paper cites Quintessential inflation with canonical and noncanonical scalar fields and Planck 2015 results.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Quintessential inflation with canonical and noncanonical scalar fields and Planck 2015 results

Reference 95

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This paper cites Distance Priors from Planck Final Release.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Distance Priors from Planck Final Release

Reference 96

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This paper cites The Pantheon+ Analysis: The Full Dataset and Light-Curve Release.

Observational constraints on early time non-phantom behaviour of dynamical dark energy The Pantheon+ Analysis: The Full Dataset and Light-Curve Release

Reference 97

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This paper cites The Pantheon+ Analysis: Cosmological Constraints.

Observational constraints on early time non-phantom behaviour of dynamical dark energy The Pantheon+ Analysis: Cosmological Constraints

Reference 98

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This paper cites $H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method.

Observational constraints on early time non-phantom behaviour of dynamical dark energy $H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method

Reference 99

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This paper cites Tension and constraints on modified gravity parametrizations of $G_{\textrm{eff}}(z)$ from growth rate and Planck data.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Tension and constraints on modified gravity parametrizations of $G_{\textrm{eff}}(z)$ from growth rate and Planck data

Reference 100

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Observation 2dad3930-02ce-444c-858f-be1206961177 · outbound

This paper cites Akaike, IEEE Transactions on Automatic Control 19, 716 (1974).

Observational constraints on early time non-phantom behaviour of dynamical dark energy Akaike, IEEE Transactions on Automatic Control 19, 716 (1974)

Reference 101

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Pith citing papers

Observation 47b22f4b-8340-4a08-85f4-b4affff8d20b · inbound

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Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity Observational constraints on early time non-phantom behaviour of dynamical dark energy

Reference 15

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Reference 54

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Probing late-time deviations from $\Lambda$CDM with a quadratic dark energy expansion cites this paper.

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Reference 28

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Dissipative Cosmology and the Nature of Dark Energy: Insights from Bulk Viscosity with DESI DR2 observations cites this paper.

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Reference 85

Resolution: verified exact; local_arxiv, observed 2026-07-02T14:27:03.480573Z

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