Paper Citation Record · LEDGER

Robustness of dark energy phenomenology across different parameterizations

As of 23 August 2026, this Paper Citation Record lists 100 of 153 outbound references and 38 inbound Pith citation observations for arXiv:2502.04929.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2502.04929 v3

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Source: paper_references, paper_reference_links, observed 2026-08-16T11:37:32.205132Z

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Outbound references

Observation 4b121cfb-6caa-4536-9b52-7601271e1e26 · outbound

This paper cites Dark Energy and the Accelerating Universe.

Robustness of dark energy phenomenology across different parameterizations Dark Energy and the Accelerating Universe

Reference 1

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Observation 2749f2c9-b591-4c18-9146-3dd79d23a7f8 · outbound

This paper cites The Cosmological Constant and Dark Energy.

Robustness of dark energy phenomenology across different parameterizations The Cosmological Constant and Dark Energy

Reference 2

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Observation 2d1bdf04-242e-4f24-a67e-139ace2f2fc3 · outbound

This paper cites Dark Energy vs. Modified Gravity.

Robustness of dark energy phenomenology across different parameterizations Dark Energy vs. Modified Gravity

Reference 3

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Observation 8dde6e5a-f32a-403a-8b39-931f360a6af5 · outbound

This paper cites Promising Stabs in the Dark: Theory Virtues and Pursuit-Worthiness in the Dark Energy Problem.

Robustness of dark energy phenomenology across different parameterizations Promising Stabs in the Dark: Theory Virtues and Pursuit-Worthiness in the Dark Energy Problem

Reference 4

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Observation c94133a3-c6fe-4459-b705-d58b9019772a · outbound

This paper cites The Spectre of Underdetermination in Modern Cosmology.

Robustness of dark energy phenomenology across different parameterizations The Spectre of Underdetermination in Modern Cosmology

Reference 5

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Observation 0eb4c72c-ccb2-430b-8345-da24a63dcbd4 · outbound

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

Robustness of dark energy phenomenology across different parameterizations DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 6

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Observation 29db898b-70b5-4065-ab46-752042d6c103 · outbound

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

Robustness of dark energy phenomenology across different parameterizations The Pantheon+ Analysis: The Full Dataset and Light-Curve Release

Reference 7

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Observation e74ac8e4-a56b-4dd2-b700-ca36f68584cb · outbound

This paper cites The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset.

Robustness of dark energy phenomenology across different parameterizations The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset

Reference 8

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Observation de36fb14-68d6-4f61-bdca-ea925ceee367 · outbound

This paper cites Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework.

Robustness of dark energy phenomenology across different parameterizations Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework

Reference 9

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Observation b86ce866-84a2-4fa6-85d0-631c6819e4b8 · outbound

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

Robustness of dark energy phenomenology across different parameterizations Planck 2018 results. VI. Cosmological parameters

Reference 10

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Observation 01fde0be-a826-463e-aa3e-acb117a37f41 · outbound

This paper cites The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters.

Robustness of dark energy phenomenology across different parameterizations The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters

Reference 11

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Observation 7de255ae-01d8-4a05-bcc6-7cf6b2055780 · outbound

This paper cites Scant evidence for thawing quintessence.

Robustness of dark energy phenomenology across different parameterizations Scant evidence for thawing quintessence

Reference 12

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Observation 0b2fcb52-0837-4b50-933b-0f82987ed827 · outbound

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

Robustness of dark energy phenomenology across different parameterizations Matching current observational constraints with nonminimally coupled dark energy

Reference 13

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Observation 9a8a9a30-b659-47c0-ba26-ed52dce021a2 · outbound

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

Robustness of dark energy phenomenology across different parameterizations Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements

Reference 14

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Observation 61d562e2-594a-43f7-ab1d-95361bb1660d · outbound

This paper cites Quintessential interpretation of the evolving dark energy in light of DESI.

Robustness of dark energy phenomenology across different parameterizations Quintessential interpretation of the evolving dark energy in light of DESI

Reference 15

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Observation 0cc76413-33c4-4f82-93f6-50f4781bad5d · outbound

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

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

Reference 16

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Observation 65e7277d-8b49-41ac-82e0-8112e7916993 · outbound

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

Robustness of dark energy phenomenology across different parameterizations DESI 2024: Constraints on Physics-Focused Aspects of Dark Energy using DESI DR1 BAO Data

Reference 17

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Observation 457afd11-f87d-4389-a51d-9af21d96169e · outbound

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

Robustness of dark energy phenomenology across different parameterizations A new diagnostic for the null test of dynamical dark energy in light of DESI 2024 and other BAO data

Reference 18

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Observation 26e4c62a-fb59-4019-acac-74587836b87b · outbound

This paper cites Does dark energy really revive using DESI 2024 data?.

Robustness of dark energy phenomenology across different parameterizations Does dark energy really revive using DESI 2024 data?

Reference 19

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Observation cd5225be-b306-4bdc-bbb8-74a60bafa07d · outbound

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

Robustness of dark energy phenomenology across different parameterizations Assessing cosmological evidence for non-minimal coupling

Reference 20

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This paper cites The Self-Consistency of DESI Analysis and Comment on "Does DESI 2024 Confirm $\Lambda$CDM?".

Robustness of dark energy phenomenology across different parameterizations The Self-Consistency of DESI Analysis and Comment on "Does DESI 2024 Confirm $\Lambda$CDM?"

Reference 21

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Observation 105c2d3e-a885-4d3d-9ad6-79e2e3af89e9 · outbound

This paper cites Mukherjee and A.A.

Robustness of dark energy phenomenology across different parameterizations Mukherjee and A.A

Reference 22

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Observation 29d900e9-899b-4d0b-bc01-400a621a8fa4 · outbound

This paper cites Dynamical dark energy in the light of DESI 2024 data.

Robustness of dark energy phenomenology across different parameterizations Dynamical dark energy in the light of DESI 2024 data

Reference 23

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Observation ff3b66b9-32d9-4633-8a15-732ad5818664 · outbound

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

Robustness of dark energy phenomenology across different parameterizations Dark energy in light of recent DESI BAO and Hubble tension

Reference 24

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

Robustness of dark energy phenomenology across different parameterizations Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 25

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This paper cites Consistent Theories for the DESI dark energy fit.

Robustness of dark energy phenomenology across different parameterizations Consistent Theories for the DESI dark energy fit

Reference 26

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This paper cites Impact of evolving dark energy on the search for primordial gravitational waves.

Robustness of dark energy phenomenology across different parameterizations Impact of evolving dark energy on the search for primordial gravitational waves

Reference 27

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This paper cites Can recent DESI BAO measurements accommodate a negative cosmological constant?.

Robustness of dark energy phenomenology across different parameterizations Can recent DESI BAO measurements accommodate a negative cosmological constant?

Reference 28

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

Robustness of dark energy phenomenology across different parameterizations Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements

Reference 29

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

Robustness of dark energy phenomenology across different parameterizations Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 30

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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.

Robustness of dark energy phenomenology across different parameterizations Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data

Reference 31

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This paper cites Consistency tests between SDSS and DESI BAO measurements.

Robustness of dark energy phenomenology across different parameterizations Consistency tests between SDSS and DESI BAO measurements

Reference 32

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This paper cites Model independent cosmographic constraints from DESI 2024.

Robustness of dark energy phenomenology across different parameterizations Model independent cosmographic constraints from DESI 2024

Reference 33

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This paper cites Investigating Late-Time Dark Energy and Massive Neutrinos in Light of DESI Y1 BAO.

Robustness of dark energy phenomenology across different parameterizations Investigating Late-Time Dark Energy and Massive Neutrinos in Light of DESI Y1 BAO

Reference 34

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This paper cites Constraints on Redshift-Binned Dark Energy using DESI BAO Data.

Robustness of dark energy phenomenology across different parameterizations Constraints on Redshift-Binned Dark Energy using DESI BAO Data

Reference 35

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This paper cites Evolving Dark Energy or Supernovae Systematics?.

Robustness of dark energy phenomenology across different parameterizations Evolving Dark Energy or Supernovae Systematics?

Reference 36

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This paper cites Cosmological constraints on curved quintessence.

Robustness of dark energy phenomenology across different parameterizations Cosmological constraints on curved quintessence

Reference 37

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This paper cites 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.

Robustness of dark energy phenomenology across different parameterizations 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

Reference 38

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Robustness of dark energy phenomenology across different parameterizations Arjona and S

Reference 39

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This paper cites Exponential Quintessence: curved, steep and stringy?.

Robustness of dark energy phenomenology across different parameterizations Exponential Quintessence: curved, steep and stringy?

Reference 40

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This paper cites Towards primordial gravitational waves and $n_s=1$ in light of BICEP/Keck, DESI BAO and Hubble tension.

Robustness of dark energy phenomenology across different parameterizations Towards primordial gravitational waves and $n_s=1$ in light of BICEP/Keck, DESI BAO and Hubble tension

Reference 41

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

Robustness of dark energy phenomenology across different parameterizations Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements

Reference 42

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Robustness of dark energy phenomenology across different parameterizations DESI constraints on $\alpha$-attractor inflationary models

Reference 43

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This paper cites Phase-space analysis of dark energy models in non-minimally coupled theories of gravity.

Robustness of dark energy phenomenology across different parameterizations Phase-space analysis of dark energy models in non-minimally coupled theories of gravity

Reference 44

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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?.

Robustness of dark energy phenomenology across different parameterizations 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 45

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

Robustness of dark energy phenomenology across different parameterizations Upper limits on dark energy-dark matter interaction from DESI DR2 in a field-theoretic analysis

Reference 46

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This paper cites Bridge the Cosmological Tensions with Thawing Gravity.

Robustness of dark energy phenomenology across different parameterizations Bridge the Cosmological Tensions with Thawing Gravity

Reference 47

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Robustness of dark energy phenomenology across different parameterizations Quintessence: an analytical study, with theoretical and observational applications

Reference 48

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

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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This paper cites DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?.

Robustness of dark energy phenomenology across different parameterizations DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 50

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This paper cites On the evidence of dynamical dark energy.

Robustness of dark energy phenomenology across different parameterizations On the evidence of dynamical dark energy

Reference 51

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Robustness of dark energy phenomenology across different parameterizations BAO vs. SN evidence for evolving dark energy

Reference 52

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This paper cites Dark energy constraints using gamma-ray burst correlations with DESI 2024 data.

Robustness of dark energy phenomenology across different parameterizations Dark energy constraints using gamma-ray burst correlations with DESI 2024 data

Reference 53

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Observation caf30978-178c-454c-990e-fd145b387cb4 · outbound

This paper cites Dark energy reconstructions combining BAO data with galaxy clusters and intermediate redshift catalogs.

Robustness of dark energy phenomenology across different parameterizations Dark energy reconstructions combining BAO data with galaxy clusters and intermediate redshift catalogs

Reference 54

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This paper cites Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity.

Robustness of dark energy phenomenology across different parameterizations Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity

Reference 55

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Observation 739a5574-f903-40ef-b1f9-31f26961f468 · outbound

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

Robustness of dark energy phenomenology across different parameterizations Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity

Reference 56

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Observation 25f958cb-936b-421c-b181-9f1d0c28c078 · outbound

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

Robustness of dark energy phenomenology across different parameterizations Modified gravity/Dynamical Dark Energy vs $\Lambda$CDM: is the game over?

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Observation 59584f9c-c601-4c82-9b78-4d28a39b3ce7 · outbound

This paper cites Implications of DES 5YR SNe Dataset for $\Lambda$CDM.

Robustness of dark energy phenomenology across different parameterizations Implications of DES 5YR SNe Dataset for $\Lambda$CDM

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Observation 402f4963-af62-45aa-9ac3-162a1c1e0c12 · outbound

This paper cites Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes.

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Observation d220635d-cb11-4315-90a3-c8217c8fe58d · outbound

This paper cites Dynamical Dark Energy Beyond Planck? Constraints from multiple CMB probes, DESI BAO and Type-Ia Supernovae.

Robustness of dark energy phenomenology across different parameterizations Dynamical Dark Energy Beyond Planck? Constraints from multiple CMB probes, DESI BAO and Type-Ia Supernovae

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Observation ede7457a-3a8e-470a-84fd-1bbb8b83770a · outbound

This paper cites The case for a low dark matter density in dynamical dark energy model from local probes.

Robustness of dark energy phenomenology across different parameterizations The case for a low dark matter density in dynamical dark energy model from local probes

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Observation 0b5ea972-a0c8-4193-bda9-2f752336fc73 · outbound

This paper cites Uncovering the bias in the evidence for dynamical dark energy through minimal and generalized modeling approaches.

Robustness of dark energy phenomenology across different parameterizations Uncovering the bias in the evidence for dynamical dark energy through minimal and generalized modeling approaches

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Observation 286c5b5e-55a1-45e5-ba6b-55faa84e4b7b · outbound

This paper cites A Critical Reanalysis of Supernova Type Ia Data.

Robustness of dark energy phenomenology across different parameterizations A Critical Reanalysis of Supernova Type Ia Data

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Observation 9a10138a-1d9e-4571-a66b-1a8a83e581c5 · outbound

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

Robustness of dark energy phenomenology across different parameterizations Scalar-Tensor Gravity and DESI 2024 BAO data

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Observation 17747725-fa07-4b38-8edc-77395285d5e2 · outbound

This paper cites Constraints on dark energy and modified gravity from the BOSS Full-Shape and DESI BAO data.

Robustness of dark energy phenomenology across different parameterizations Constraints on dark energy and modified gravity from the BOSS Full-Shape and DESI BAO data

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Observation 36b64d08-78b2-4a06-a487-3010a6567eba · outbound

This paper cites Does DESI 2024 Confirm $\Lambda$CDM?.

Robustness of dark energy phenomenology across different parameterizations Does DESI 2024 Confirm $\Lambda$CDM?

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Observation dff8f3c2-7cb7-4050-a828-5896878dc0f8 · outbound

This paper cites Cosmic distance duality after DESI 2024 data release and dark energy evolution.

Robustness of dark energy phenomenology across different parameterizations Cosmic distance duality after DESI 2024 data release and dark energy evolution

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Observation 57f31f7c-3940-460a-ac92-771a36dedbe4 · outbound

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

Robustness of dark energy phenomenology across different parameterizations Illustrating the consequences of a misuse of $\sigma_8$ in cosmology

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Observation 862dd011-d2ea-4197-b52f-a25e171dcb9a · outbound

This paper cites Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations.

Robustness of dark energy phenomenology across different parameterizations Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

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Observation bcd163be-5b7d-434f-b3ec-4d5fc8ad274f · outbound

This paper cites an unresolved cited work.

Robustness of dark energy phenomenology across different parameterizations Unresolved cited work

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Observation 445a4a87-624c-46ce-9d68-77ce54cf518b · outbound

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

Robustness of dark energy phenomenology across different parameterizations The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae

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Observation 4aacfa25-9d66-411f-bd9a-4fefc9f7d326 · outbound

This paper cites The axis of systematic bias in SN~Ia cosmology and implications for DESI 2024 results.

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Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.783050Z

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Observation 72533662-7132-4dd2-a3a6-1b62b67541fb · outbound

This paper cites Hossain and A.

Robustness of dark energy phenomenology across different parameterizations Hossain and A

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Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.786544Z

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Observation 4ec5102a-1ba9-4878-a735-d25ff1769f1b · outbound

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

Robustness of dark energy phenomenology across different parameterizations Preference for evolving dark energy in light of the galaxy bispectrum

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Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.789776Z

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Observation a5d7f7f7-a400-48e8-aa64-de46d80d5341 · outbound

This paper cites Bounded Dark Energy.

Robustness of dark energy phenomenology across different parameterizations Bounded Dark Energy

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Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.793287Z

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Observation 3ba5f310-66d7-4c6f-ac2e-7e815bb10818 · outbound

This paper cites Chakraborty, P.K.

Robustness of dark energy phenomenology across different parameterizations Chakraborty, P.K

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Observation a8652a39-51ce-4f37-8448-581373df07e3 · outbound

This paper cites Reconstructing the dark energy density in light of DESI BAO observations.

Robustness of dark energy phenomenology across different parameterizations Reconstructing the dark energy density in light of DESI BAO observations

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Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.800241Z

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Observation 0e36f5b5-6a79-4130-a421-6cb0ba3ad480 · outbound

This paper cites Cosmic Clues: DESI, Dark Energy, and the Cosmological Constant Problem.

Robustness of dark energy phenomenology across different parameterizations Cosmic Clues: DESI, Dark Energy, and the Cosmological Constant Problem

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Observation e485dd81-e93e-4c3b-834c-745df08cd27e · outbound

This paper cites Wang and Y.-S.

Robustness of dark energy phenomenology across different parameterizations Wang and Y.-S

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Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.807085Z

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Observation af33669b-b9ef-4706-8c71-c2d705729d86 · outbound

This paper cites Accelerating Universes with Scaling Dark Matter.

Robustness of dark energy phenomenology across different parameterizations Accelerating Universes with Scaling Dark Matter

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Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.810434Z

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Observation 27fd72d8-066c-4e33-b88f-26fe9733318d · outbound

This paper cites Exploring the Expansion History of the Universe.

Robustness of dark energy phenomenology across different parameterizations Exploring the Expansion History of the Universe

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Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.813968Z

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Observation b8698723-a2ef-475c-85ea-b40ccd64bc4b · outbound

This paper cites Underdetermination of dark energy.

Robustness of dark energy phenomenology across different parameterizations Underdetermination of dark energy

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Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.817442Z

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Observation 7f0ce5c2-55bd-46d6-9450-dd9accdcf407 · outbound

This paper cites Interpreting DESI's evidence for evolving dark energy.

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

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Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.820965Z

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Observation 32acf037-3198-4620-ac74-4f7c0c9fb0ad · outbound

This paper cites Assessing observational constraints on dark energy.

Robustness of dark energy phenomenology across different parameterizations Assessing observational constraints on dark energy

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Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.824840Z

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Observation 967cf023-f28c-4d17-9efe-acab9242c168 · outbound

This paper cites Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe.

Robustness of dark energy phenomenology across different parameterizations Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe

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Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.828395Z

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Observation 782ea0ae-5e0c-4c03-9e6a-441398c166af · outbound

This paper cites Observational constraints on low redshift evolution of dark energy: How consistent are different observations?.

Robustness of dark energy phenomenology across different parameterizations Observational constraints on low redshift evolution of dark energy: How consistent are different observations?

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Observation 6d9f7dcd-ef40-46b5-85e0-12e39a7fd23f · outbound

This paper cites A parametric model for dark energy.

Robustness of dark energy phenomenology across different parameterizations A parametric model for dark energy

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Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.835393Z

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Observation 7ad6bf16-8856-4671-a019-f4ac9f285382 · outbound

This paper cites New simple and accurate quintessence approximations.

Robustness of dark energy phenomenology across different parameterizations New simple and accurate quintessence approximations

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Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.838871Z

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Observation a5c5b1f4-c727-47b7-b040-c503cdeab44d · outbound

This paper cites Do Observations Prefer Thawing Quintessence?.

Robustness of dark energy phenomenology across different parameterizations Do Observations Prefer Thawing Quintessence?

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Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.842156Z

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Observation 6dcfd20e-0870-40eb-8e94-e2e186fb533f · outbound

This paper cites General parametrization for energy density of quintessence field.

Robustness of dark energy phenomenology across different parameterizations General parametrization for energy density of quintessence field

Reference 90

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Observation b6f4d2ac-0dcc-4982-bf78-aa85f39a51d3 · outbound

This paper cites Acceleration of the universe: a reconstruction of the effective equation of state.

Robustness of dark energy phenomenology across different parameterizations Acceleration of the universe: a reconstruction of the effective equation of state

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Resolution: verified exact; local_arxiv, observed 2026-08-08T21:04:21.357009Z

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Observation 393679e9-5525-431d-beb1-7b25c49c9aed · outbound

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Robustness of dark energy phenomenology across different parameterizations A New Class of Parametrization for Dark Energy without Divergence

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Observation bdb759d3-1c03-4723-9779-ce67ed8da79d · outbound

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Robustness of dark energy phenomenology across different parameterizations What do we learn by mapping dark energy to a single value of $w$?

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Observation a2d48001-0413-4516-922c-abdcffcf1bd8 · outbound

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Robustness of dark energy phenomenology across different parameterizations New parametrization of the dark-energy equation of state with a single parameter

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Observation 9a263099-0f13-4235-b6f1-98f52b89799e · outbound

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Observation d56a145c-d00d-4331-8d59-780dff5ba6b5 · outbound

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Observation a71f801d-50cf-4d08-b4e4-f76a337a962b · outbound

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Robustness of dark energy phenomenology across different parameterizations Probing the curvature and dark energy

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.870766Z

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Observation 88c105ee-b9dd-42f1-a102-2bbd8b8327d9 · outbound

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Robustness of dark energy phenomenology across different parameterizations Evidence for Emergent Dark Energy

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Observation 1a5d598c-a983-4e77-8459-d019e7f2e964 · outbound

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Robustness of dark energy phenomenology across different parameterizations Multi-Messenger Cosmology: A Route to Accurate Inference of Dark Energy Beyond CPL Parametrization from XG Detectors

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Resolution: verified exact; local_arxiv, observed 2026-08-08T21:04:21.262395Z

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Resolution: verified exact; arxiv_id, observed 2026-05-18T10:46:16.832716Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation e360e746-73e0-4ffb-8864-29b6bf627fa0 · inbound

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 Robustness of dark energy phenomenology across different parameterizations

Reference 28

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:00.743941Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 5f1a604b-c314-48d3-a17f-549ebd7d1285 · inbound

Cosmological tensions in Proca-Nuevo theory cites this paper.

Cosmological tensions in Proca-Nuevo theory Robustness of dark energy phenomenology across different parameterizations

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-03T20:12:23.326005Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2db8cc5b-b934-4bbc-a877-84f70a68c7c9 · 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 Robustness of dark energy phenomenology across different parameterizations

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-03T14:40:55.358995Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 02848baa-a2c8-4a5f-b3e6-203e863111fe · inbound

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 Robustness of dark energy phenomenology across different parameterizations

Reference 204

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:12.275960Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 939c214e-bed6-4332-8356-123b2095fadc · inbound

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 Robustness of dark energy phenomenology across different parameterizations

Reference 205

Resolution: unresolved; no resolver link, observed 2026-07-15T12:01:04.317365Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation decd2754-43f6-4250-be75-e638f7b1a8e1 · inbound

Exploring the interplay of late-time dynamical dark energy and new physics before recombination cites this paper.

Exploring the interplay of late-time dynamical dark energy and new physics before recombination Robustness of dark energy phenomenology across different parameterizations

Reference 39

Resolution: verified exact; arxiv_id, observed 2026-05-14T23:13:15.506466Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 4f8ad474-6c1f-45a0-acb6-e852eb6d0791 · inbound

Testing the consistency of cosmological models with multimessenger astronomy cites this paper.

Testing the consistency of cosmological models with multimessenger astronomy Robustness of dark energy phenomenology across different parameterizations

Reference 4

Resolution: verified exact; arxiv_id, observed 2026-05-12T03:01:18.059347Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 549f9a4c-09e9-46ce-829c-c338552a92a9 · inbound

Testing the consistency of cosmological models with multimessenger astronomy cites this paper.

Testing the consistency of cosmological models with multimessenger astronomy Robustness of dark energy phenomenology across different parameterizations

Reference 5

Resolution: verified exact; arxiv_id, observed 2026-05-20T22:29:09.625704Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation a6aa7e97-a7cc-4b2c-879e-8df5e81973b8 · inbound

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

Negative neutrino mass or negative dark energy? Robustness of dark energy phenomenology across different parameterizations

Reference 144

Resolution: verified exact; arxiv_id, observed 2026-05-21T03:03:55.592646Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation b3d46777-43e1-43c3-b36e-aeec6e500b26 · inbound

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

A short review on Quintom dark energy theory Robustness of dark energy phenomenology across different parameterizations

Reference 50

Resolution: verified exact; arxiv_id, observed 2026-07-01T21:46:15.954214Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 37e6e5e5-5a7b-4341-9633-7ae9985be495 · inbound

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

A short review on Quintom dark energy theory Robustness of dark energy phenomenology across different parameterizations

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-02T12:40:03.479588Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c2c3d712-8ca6-4fe9-b947-f7d830768877 · inbound

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

Dissipative Cosmology and the Nature of Dark Energy: Insights from Bulk Viscosity with DESI DR2 observations Robustness of dark energy phenomenology across different parameterizations

Reference 70

Resolution: verified exact; arxiv_id, observed 2026-07-02T14:27:03.518055Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 997bd7e8-7990-40c3-90c9-68b8546d0b12 · inbound

Reconstructing dark energy with fewer assumptions cites this paper.

Reconstructing dark energy with fewer assumptions Robustness of dark energy phenomenology across different parameterizations

Reference 69

Resolution: verified exact; arxiv_id, observed 2026-07-02T14:57:04.336471Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation aaf2df79-a011-48d7-a766-2ab63efa675d · inbound

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 Robustness of dark energy phenomenology across different parameterizations

Reference 13

Resolution: verified exact; arxiv_id, observed 2026-07-03T22:08:59.502246Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 319551b7-7b7a-4ecf-87cb-e7d86713d2e3 · inbound

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

Cosmological Viability of Exponential Infrared $f(T)$ Gravity Robustness of dark energy phenomenology across different parameterizations

Reference 91

Resolution: verified exact; arxiv_id, observed 2026-07-01T11:15:42.412891Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 1be83310-e0ff-4153-88e4-a2042c228a14 · inbound

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 Robustness of dark energy phenomenology across different parameterizations

Reference 142

Resolution: verified exact; arxiv_id, observed 2026-07-02T06:16:43.316785Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation b147e685-07bd-41fd-9848-40ea0d1be6fa · inbound

Natural Phantom Dark Energy from a $\mathbb{Z}_N$--Axion cites this paper.

Natural Phantom Dark Energy from a $\mathbb{Z}_N$--Axion Robustness of dark energy phenomenology across different parameterizations

Reference 6

Resolution: verified exact; local_arxiv, observed 2026-07-10T21:37:39.764548Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 4465c7d8-eb4a-4e57-aa2b-6b9bea4c1412 · inbound

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 Robustness of dark energy phenomenology across different parameterizations

Reference 74

Resolution: verified exact; local_arxiv, observed 2026-07-09T13:46:17.477684Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation f7d70c60-eca3-427d-8376-f054c9744632 · inbound

The Status of Single Scalar Field Dark Energy cites this paper.

The Status of Single Scalar Field Dark Energy Robustness of dark energy phenomenology across different parameterizations

Reference 45

Resolution: verified exact; local_arxiv, observed 2026-07-10T18:27:31.427495Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation c5e2ab28-4463-4dbe-abe4-9e898bbf3c44 · 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 Robustness of dark energy phenomenology across different parameterizations

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-01T01:25:44.156693Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0d3f3e62-8425-4d1d-bef4-52ecf237b7ba · inbound

Natural Phantom Crossing from Axion-WIMP Interactions cites this paper.

Natural Phantom Crossing from Axion-WIMP Interactions Robustness of dark energy phenomenology across different parameterizations

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-03T00:46:07.338381Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b2c27abc-26a9-4a6c-8f58-fee2cb893274 · 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? Robustness of dark energy phenomenology across different parameterizations

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.134748Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.