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Paper Citation Record · LEDGER

Evidence for non-cold dark matter from DESI DR2 measurements

As of 23 August 2026, this Paper Citation Record lists 100 of 110 outbound references and 27 inbound Pith citation observations for arXiv:2504.14419.

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2504.14419 v1

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measured 100 of 110 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-16T05:27:54.451462Z

measured 1 of 1 external citation measurements

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Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

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Outbound references

Observation 6e4d4ca7-7c36-4988-801e-faf577be52ae · outbound

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

Evidence for non-cold dark matter from DESI DR2 measurements Planck 2018 results. VI. Cosmological parameters

Reference 1

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Observation d8f99cec-79d3-40af-9ff6-40283edb9441 · outbound

This paper cites Planck 2018 results. V. CMB power spectra and likelihoods.

Evidence for non-cold dark matter from DESI DR2 measurements Planck 2018 results. V. CMB power spectra and likelihoods

Reference 2

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Observation b402f995-d4fe-4a6e-b542-e408597c7904 · outbound

This paper cites Planck 2018 results. VIII. Gravitational lensing.

Evidence for non-cold dark matter from DESI DR2 measurements Planck 2018 results. VIII. Gravitational lensing

Reference 3

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Observation 89feeaf6-fe23-474f-8372-3a2ae7e16967 · outbound

This paper cites Measurements of the E-Mode Polarization and Temperature-E-Mode Correlation of the CMB from SPT-3G 2018 Data.

Evidence for non-cold dark matter from DESI DR2 measurements Measurements of the E-Mode Polarization and Temperature-E-Mode Correlation of the CMB from SPT-3G 2018 Data

Reference 4

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Observation a0e1c6f8-2717-4739-887a-4d67ae403a38 · outbound

This paper cites The Atacama Cosmology Telescope: A Measurement of the Cosmic Microwave Background Power Spectra at 98 and 150 GHz.

Evidence for non-cold dark matter from DESI DR2 measurements The Atacama Cosmology Telescope: A Measurement of the Cosmic Microwave Background Power Spectra at 98 and 150 GHz

Reference 5

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Observation 1aab0dc1-0694-44ee-8cdb-4f713e4b1413 · outbound

This paper cites Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results.

Evidence for non-cold dark matter from DESI DR2 measurements Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results

Reference 6

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Observation c845da32-9d9d-43fc-834d-08cada0e7066 · outbound

This paper cites Planck 2018 results. I. Overview and the cosmological legacy of Planck.

Evidence for non-cold dark matter from DESI DR2 measurements Planck 2018 results. I. Overview and the cosmological legacy of Planck

Reference 7

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Observation 6eb90f3a-cbe3-4315-807c-4faca8a82932 · outbound

This paper cites The Cosmic Microwave Background and $H_0$.

Evidence for non-cold dark matter from DESI DR2 measurements The Cosmic Microwave Background and $H_0$

Reference 8

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Observation 228a4430-fca4-4868-a4ab-1f2ca1db6c5a · outbound

This paper cites Data analysis methods for the cosmic microwave background.

Evidence for non-cold dark matter from DESI DR2 measurements Data analysis methods for the cosmic microwave background

Reference 9

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Observation 70adc3ac-3ecd-49cc-8a05-21ab765518f8 · outbound

This paper cites The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample.

Evidence for non-cold dark matter from DESI DR2 measurements The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample

Reference 10

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Observation 6e7fc484-0bb5-4416-8a44-c2f0352eef8b · outbound

This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Baryon acoustic oscillations with Lyman-$\alpha$ forests.

Evidence for non-cold dark matter from DESI DR2 measurements The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Baryon acoustic oscillations with Lyman-$\alpha$ forests

Reference 11

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Observation 97508b69-6ae7-4a96-8919-5f64eb9d45ac · outbound

This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the Quasar Sample in configuration space between redshift 0.8 and 2.2.

Evidence for non-cold dark matter from DESI DR2 measurements The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the Quasar Sample in configuration space between redshift 0.8 and 2.2

Reference 12

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Observation f1382458-0d6a-456e-bb17-60dea47a77a9 · outbound

This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory.

Evidence for non-cold dark matter from DESI DR2 measurements The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory

Reference 13

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Observation 4b696aa7-6c06-45a3-8788-7dc9784d5195 · outbound

This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0.

Evidence for non-cold dark matter from DESI DR2 measurements The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0

Reference 14

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Observation 38a7462c-ec7f-4a61-b300-40f2fda8bffa · outbound

This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic correlation function between redshifts 0.6 and 1.

Evidence for non-cold dark matter from DESI DR2 measurements The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic correlation function between redshifts 0.6 and 1

Reference 15

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Observation 76af5e9e-e2f6-4a4b-848a-47376b5a62fb · outbound

This paper cites Data Release 1 of the Dark Energy Spectroscopic Instrument.

Evidence for non-cold dark matter from DESI DR2 measurements Data Release 1 of the Dark Energy Spectroscopic Instrument

Reference 16

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Observation 77b69eb0-aea4-4309-8076-243c265e3af9 · outbound

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

Evidence for non-cold dark matter from DESI DR2 measurements DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 17

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Observation 4699ab54-16d1-4d95-8b76-957c8c0f6d9a · outbound

This paper cites The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample.

Evidence for non-cold dark matter from DESI DR2 measurements The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample

Reference 18

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Observation 9d40962e-d63a-4f1f-85fa-6deee7399479 · outbound

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

Evidence for non-cold dark matter from DESI DR2 measurements The Pantheon+ Analysis: The Full Dataset and Light-Curve Release

Reference 19

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Observation 2301f275-4549-4e48-ab17-b08e4f1604d9 · outbound

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

Evidence for non-cold dark matter from DESI DR2 measurements Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework

Reference 20

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Observation 9c25b4f9-4afc-4f79-b48d-a82dd2044770 · outbound

This paper cites Type Ia Supernova cosmology combining data from the $Euclid$ mission and the Vera C. Rubin Observatory.

Evidence for non-cold dark matter from DESI DR2 measurements Type Ia Supernova cosmology combining data from the $Euclid$ mission and the Vera C. Rubin Observatory

Reference 21

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Observation 4fcfed79-85e6-42d0-92a1-8772a9b73d58 · outbound

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Evidence for non-cold dark matter from DESI DR2 measurements Type Ia supernovae

Reference 22

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

Evidence for non-cold dark matter from DESI DR2 measurements The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset

Reference 23

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Observation 2c0e0877-7b2f-4410-b50c-fb5253de0739 · outbound

This paper cites Improving Cosmological Distance Measurements Using Twin Type Ia Supernovae.

Evidence for non-cold dark matter from DESI DR2 measurements Improving Cosmological Distance Measurements Using Twin Type Ia Supernovae

Reference 24

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Observation 3fc9292d-64be-493d-a410-06bf1f0c3942 · outbound

This paper cites The Dark Energy Survey: more than dark energy - an overview.

Evidence for non-cold dark matter from DESI DR2 measurements The Dark Energy Survey: more than dark energy - an overview

Reference 25

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Observation fd943b71-e57e-4675-9770-77f90af12699 · outbound

This paper cites Cosmological Constraints from Multiple Probes in the Dark Energy Survey.

Evidence for non-cold dark matter from DESI DR2 measurements Cosmological Constraints from Multiple Probes in the Dark Energy Survey

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Evidence for non-cold dark matter from DESI DR2 measurements The Dark Energy Survey Data Release 2

Reference 27

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This paper cites KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing.

Evidence for non-cold dark matter from DESI DR2 measurements KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing

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Evidence for non-cold dark matter from DESI DR2 measurements KiDS+VIKING-450: Cosmic shear tomography with optical+infrared data

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Evidence for non-cold dark matter from DESI DR2 measurements Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data

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Observation dc0dcb70-1117-4403-bf49-c0bb5ca5ac68 · outbound

This paper cites Dark Energy Survey Year 3 Results: Constraints on extensions to $\Lambda$CDM with weak lensing and galaxy clustering.

Evidence for non-cold dark matter from DESI DR2 measurements Dark Energy Survey Year 3 Results: Constraints on extensions to $\Lambda$CDM with weak lensing and galaxy clustering

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This paper cites Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing.

Evidence for non-cold dark matter from DESI DR2 measurements Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

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This paper cites Lack of large-angle TT correlations persists in WMAP and Planck.

Evidence for non-cold dark matter from DESI DR2 measurements Lack of large-angle TT correlations persists in WMAP and Planck

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This paper cites The Uncorrelated Universe: Statistical Anisotropy and the Vanishing Angular Correlation Function in WMAP Years 1-3.

Evidence for non-cold dark matter from DESI DR2 measurements The Uncorrelated Universe: Statistical Anisotropy and the Vanishing Angular Correlation Function in WMAP Years 1-3

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This paper cites Small-Scale Challenges to the $\Lambda$CDM Paradigm.

Evidence for non-cold dark matter from DESI DR2 measurements Small-Scale Challenges to the $\Lambda$CDM Paradigm

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Observation 1df16063-4640-45e4-96b7-c58ceb9d33a5 · outbound

This paper cites Observational rotation curves and density profiles vs. the Thomas-Fermi galaxy structure theory.

Evidence for non-cold dark matter from DESI DR2 measurements Observational rotation curves and density profiles vs. the Thomas-Fermi galaxy structure theory

Reference 36

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Observation acbec968-723a-4387-8865-98bc54fbca62 · outbound

This paper cites Where are the missing galactic satellites?.

Evidence for non-cold dark matter from DESI DR2 measurements Where are the missing galactic satellites?

Reference 37

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Observation 2b528f9c-da9d-4285-890f-5618b3fe3bbd · outbound

This paper cites Dark Matter Substructure in Galactic Halos.

Evidence for non-cold dark matter from DESI DR2 measurements Dark Matter Substructure in Galactic Halos

Reference 38

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Observation 21ec0ad1-f974-48b0-b056-1c681021553c · outbound

This paper cites Too big to fail? The puzzling darkness of massive Milky Way subhaloes.

Evidence for non-cold dark matter from DESI DR2 measurements Too big to fail? The puzzling darkness of massive Milky Way subhaloes

Reference 39

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Observation 266baef4-7b61-4b30-8aa6-34377d3e46ee · outbound

This paper cites Sterile Neutrinos as Dark Matter.

Evidence for non-cold dark matter from DESI DR2 measurements Sterile Neutrinos as Dark Matter

Reference 40

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Observation 9b724906-b424-4385-82eb-152e19789daf · outbound

This paper cites Satellite galaxies in semi-analytic models of galaxy formation with sterile neutrino dark matter.

Evidence for non-cold dark matter from DESI DR2 measurements Satellite galaxies in semi-analytic models of galaxy formation with sterile neutrino dark matter

Reference 41

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Observation 2788946d-c068-41ef-91a7-d639124649ef · outbound

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

Evidence for non-cold dark matter from DESI DR2 measurements Interpreting DESI's evidence for evolving dark energy

Reference 42

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Observation c9c122bb-201c-40fa-bf7b-684b681de3a5 · outbound

This paper cites Cosmological consequences of a rolling homogeneous scalar field,.

Evidence for non-cold dark matter from DESI DR2 measurements Cosmological consequences of a rolling homogeneous scalar field,

Reference 43

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Observation fa3b3e2b-06c6-4771-b3d6-815dc01d8771 · outbound

This paper cites Cosmology with x-matter.

Evidence for non-cold dark matter from DESI DR2 measurements Cosmology with x-matter

Reference 44

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Observation e0b5c81b-4bbb-4fed-92fb-d4ee9e1286b9 · outbound

This paper cites Kinetically driven quintessence,.

Evidence for non-cold dark matter from DESI DR2 measurements Kinetically driven quintessence,

Reference 45

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Observation c15058c4-a090-406f-bd29-9f3ddc890ec2 · outbound

This paper cites Essentials of k-essence,.

Evidence for non-cold dark matter from DESI DR2 measurements Essentials of k-essence,

Reference 46

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Observation c57381e0-1b1a-4914-a6b5-c08d428520f9 · outbound

This paper cites f(R) Theories Of Gravity.

Evidence for non-cold dark matter from DESI DR2 measurements f(R) Theories Of Gravity

Reference 47

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Observation 0e87bab0-658a-4a2e-9218-d35496963059 · outbound

This paper cites Holographic dark energy from the laws of thermodynamics with R\'enyi entropy.

Evidence for non-cold dark matter from DESI DR2 measurements Holographic dark energy from the laws of thermodynamics with R\'enyi entropy

Reference 48

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Observation b3fb8597-f868-49ee-b4cb-071258335f52 · outbound

This paper cites Higgs Dark Energy.

Evidence for non-cold dark matter from DESI DR2 measurements Higgs Dark Energy

Reference 49

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Observation 7bd232d7-b854-4d7c-be05-17feb4e97bc0 · outbound

This paper cites Models of f(R) Cosmic Acceleration that Evade Solar-System Tests.

Evidence for non-cold dark matter from DESI DR2 measurements Models of f(R) Cosmic Acceleration that Evade Solar-System Tests

Reference 50

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Observation 4d5c8944-6ca3-45bb-840a-945f6ab25e2e · outbound

This paper cites Mimicking dark matter and dark energy in a mimetic model compatible with GW170817.

Evidence for non-cold dark matter from DESI DR2 measurements Mimicking dark matter and dark energy in a mimetic model compatible with GW170817

Reference 51

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Observation 4626cf26-6895-4e40-bce5-841159588a27 · outbound

This paper cites Swampland Criteria in the Slotheon Field Dark Energy.

Evidence for non-cold dark matter from DESI DR2 measurements Swampland Criteria in the Slotheon Field Dark Energy

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Observation 7ba1657a-9405-464e-a215-6c3f765a4868 · outbound

This paper cites Observational Constraints on Axion(s) Dark Energy with a Cosmological Constant.

Evidence for non-cold dark matter from DESI DR2 measurements Observational Constraints on Axion(s) Dark Energy with a Cosmological Constant

Reference 53

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Observation 3b2a6a3b-0149-4f13-8cb8-f49f78d6fcfb · outbound

This paper cites From a Bounce to the Dark Energy Era with $F(R)$ Gravity.

Evidence for non-cold dark matter from DESI DR2 measurements From a Bounce to the Dark Energy Era with $F(R)$ Gravity

Reference 54

Resolution
verified exact
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Observation 9179391c-47f0-4060-8bd5-8222d356615f · outbound

This paper cites An Effective Sign Switching Dark Energy: Lotka-Volterra Model of Two Interacting Fluids.

Evidence for non-cold dark matter from DESI DR2 measurements An Effective Sign Switching Dark Energy: Lotka-Volterra Model of Two Interacting Fluids

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Observation 02164dee-6b7c-4f2a-96e0-1b99117cae71 · outbound

This paper cites Saez-Ballester gravity in Kantowski-Sachs Universe: a new reconstruction paradigm for Barrow Holographic Dark Energy.

Evidence for non-cold dark matter from DESI DR2 measurements Saez-Ballester gravity in Kantowski-Sachs Universe: a new reconstruction paradigm for Barrow Holographic Dark Energy

Reference 56

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Observation 5d04973f-035d-4e67-bf69-8971e9340741 · outbound

This paper cites Constraints on Generalized Gravity-Thermodynamic Cosmology from DESI DR2,.

Evidence for non-cold dark matter from DESI DR2 measurements Constraints on Generalized Gravity-Thermodynamic Cosmology from DESI DR2,

Reference 57

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Observation 0d1a9d9c-10c6-4688-8d3b-d665114af847 · outbound

This paper cites Has DESI detected exponential quintessence?.

Evidence for non-cold dark matter from DESI DR2 measurements Has DESI detected exponential quintessence?

Reference 58

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Observation 0bedd53b-5753-4d99-ae37-87c5f6cc65fe · outbound

This paper cites A New Window on Dynamical Dark Energy: Combining DESI-DR2 BAO with future Gravitational Wave Observations.

Evidence for non-cold dark matter from DESI DR2 measurements A New Window on Dynamical Dark Energy: Combining DESI-DR2 BAO with future Gravitational Wave Observations

Reference 59

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Observation b945a053-ac1a-4e9a-96d7-3baf8017de1c · outbound

This paper cites How much has DESI dark energy evolved since DR1?.

Evidence for non-cold dark matter from DESI DR2 measurements How much has DESI dark energy evolved since DR1?

Reference 60

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Observation 1633a81a-c324-474d-9775-55b517f0382f · outbound

This paper cites Emergent dark energy from unparticles.

Evidence for non-cold dark matter from DESI DR2 measurements Emergent dark energy from unparticles

Reference 61

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Observation 73630363-6729-4dd9-87a1-f8487ddcc9db · outbound

This paper cites Emergent Unparticles Dark Energy can restore cosmological concordance.

Evidence for non-cold dark matter from DESI DR2 measurements Emergent Unparticles Dark Energy can restore cosmological concordance

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Observation d7d1718f-adfa-4679-ab80-5c80a6cea479 · outbound

This paper cites Theoretical Priors and the Dark Energy Equation of State.

Evidence for non-cold dark matter from DESI DR2 measurements Theoretical Priors and the Dark Energy Equation of State

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Observation 539c1cd9-ee14-40a3-b55f-2bc263f88006 · outbound

This paper cites Coupled Quintessence.

Evidence for non-cold dark matter from DESI DR2 measurements Coupled Quintessence

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Observation 8a812e4f-33f6-4d11-b578-14cdc941b367 · outbound

This paper cites Relieving the Tension between Weak Lensing and Cosmic Microwave Background with Interacting Dark Matter and Dark Energy Models.

Evidence for non-cold dark matter from DESI DR2 measurements Relieving the Tension between Weak Lensing and Cosmic Microwave Background with Interacting Dark Matter and Dark Energy Models

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Observation de657ee9-5030-451f-8614-a54c319322e0 · outbound

This paper cites Constraining a dark matter and dark energy interaction scenario with a dynamical equation of state.

Evidence for non-cold dark matter from DESI DR2 measurements Constraining a dark matter and dark energy interaction scenario with a dynamical equation of state

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Observation 1ac2602b-b2bd-4fd8-bd78-462202917bfe · outbound

This paper cites Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions.

Evidence for non-cold dark matter from DESI DR2 measurements Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

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Observation d84ac76a-11f3-44bf-9e7d-5cc62efc84fb · outbound

This paper cites Coupled Quintessence scalar field model in light of observational datasets.

Evidence for non-cold dark matter from DESI DR2 measurements Coupled Quintessence scalar field model in light of observational datasets

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Observation 4d70fa34-22b8-40aa-b23e-88f2648ae2d4 · outbound

This paper cites Interacting dark energy: clarifying the cosmological implications and viability conditions.

Evidence for non-cold dark matter from DESI DR2 measurements Interacting dark energy: clarifying the cosmological implications and viability conditions

Reference 69

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Observation 7a4959c4-abf9-4e68-bd4b-b9dd72d8bdac · outbound

This paper cites Constructing Viable Interacting Dark Matter and Dark Energy Models: A Dynamical Systems Approach.

Evidence for non-cold dark matter from DESI DR2 measurements Constructing Viable Interacting Dark Matter and Dark Energy Models: A Dynamical Systems Approach

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Observation 2c5dfdd6-cfc0-4d0a-9c35-a3aa7c8f327d · outbound

This paper cites Dark energy with the help of interacting dark sectors.

Evidence for non-cold dark matter from DESI DR2 measurements Dark energy with the help of interacting dark sectors

Reference 71

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Observation 16ea3233-dc12-4e0d-9aa4-d45550e09cbc · outbound

This paper cites Observational constraints on variable equation of state parameters of dark matter and dark energy after Planck.

Evidence for non-cold dark matter from DESI DR2 measurements Observational constraints on variable equation of state parameters of dark matter and dark energy after Planck

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Observation 41d25af0-a54e-4373-86e3-3e353a30a9ce · outbound

This paper cites Cosmological bounds on the equation of state of dark matter,.

Evidence for non-cold dark matter from DESI DR2 measurements Cosmological bounds on the equation of state of dark matter,

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verified exact
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Observation 246d67d8-4942-4877-81f4-64ef2dc9cca6 · outbound

This paper cites How Cold is Cold Dark Matter?.

Evidence for non-cold dark matter from DESI DR2 measurements How Cold is Cold Dark Matter?

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Observation 3eaab191-a55c-4790-a800-0a79e4d92141 · outbound

This paper cites The Dark Matter equation of state through cosmic history.

Evidence for non-cold dark matter from DESI DR2 measurements The Dark Matter equation of state through cosmic history

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Observation 98d5ecb5-b626-4eef-90db-07fb89efaa54 · outbound

This paper cites Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges.

Evidence for non-cold dark matter from DESI DR2 measurements Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges

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Observation 247cdfd8-44b0-41c9-a046-b7c67c965d18 · outbound

This paper cites Equation of State of Dark Matter after Planck Data.

Evidence for non-cold dark matter from DESI DR2 measurements Equation of State of Dark Matter after Planck Data

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Observation bdb1baa5-0aa8-4459-a193-cfd2ce85b4cf · outbound

This paper cites Efficient Computation of CMB anisotropies in closed FRW models.

Evidence for non-cold dark matter from DESI DR2 measurements Efficient Computation of CMB anisotropies in closed FRW models

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Observation b7d54526-62fc-4e86-925b-25043e2cc8e9 · outbound

This paper cites CMB power spectrum parameter degeneracies in the era of precision cosmology.

Evidence for non-cold dark matter from DESI DR2 measurements CMB power spectrum parameter degeneracies in the era of precision cosmology

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Observation 7008a9f2-45c1-42e3-9df6-3e98109373fe · outbound

This paper cites Cobaya: Code for Bayesian Analysis of hierarchical physical models.

Evidence for non-cold dark matter from DESI DR2 measurements Cobaya: Code for Bayesian Analysis of hierarchical physical models

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Observation d5444974-561a-41a2-a86b-ff178f94d403 · outbound

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Evidence for non-cold dark matter from DESI DR2 measurements Cobaya: Bayesian analysis in cosmology,

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Observation 122956e1-36a7-4e56-ac34-c790e812a5b4 · outbound

This paper cites GetDist: a Python package for analysing Monte Carlo samples.

Evidence for non-cold dark matter from DESI DR2 measurements GetDist: a Python package for analysing Monte Carlo samples

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Observation d453efe8-cce9-43c3-be2a-a8e56beb49e8 · outbound

This paper cites Improving the Flexibility and Robustness of Model-Based Derivative-Free Optimization Solvers.

Evidence for non-cold dark matter from DESI DR2 measurements Improving the Flexibility and Robustness of Model-Based Derivative-Free Optimization Solvers

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Observation 5158bc96-c5e2-4384-bfd7-1a9a234c811f · outbound

This paper cites Escaping local minima with derivative-free methods: a numerical investigation.

Evidence for non-cold dark matter from DESI DR2 measurements Escaping local minima with derivative-free methods: a numerical investigation

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Observation 68e73d9f-1fe5-4e04-9d5c-daf6a26fc5cc · outbound

This paper cites The galaxy power spectrum take on spatial curvature and cosmic concordance.

Evidence for non-cold dark matter from DESI DR2 measurements The galaxy power spectrum take on spatial curvature and cosmic concordance

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Observation 4f0397e7-7214-4461-95c1-432c178f4c5d · outbound

This paper cites CFHTLenS revisited: assessing concordance with Planck including astrophysical systematics.

Evidence for non-cold dark matter from DESI DR2 measurements CFHTLenS revisited: assessing concordance with Planck including astrophysical systematics

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Observation 81b7dda1-4f40-44f7-a5cf-718c7b6892fb · outbound

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

Evidence for non-cold dark matter from DESI DR2 measurements DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

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Observation 3da2a202-6329-4146-b13d-1bb944838614 · outbound

This paper cites DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest.

Evidence for non-cold dark matter from DESI DR2 measurements DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest

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Observation 7b4b82fd-f079-40aa-89a6-fe2dadfb46b7 · outbound

This paper cites CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys.

Evidence for non-cold dark matter from DESI DR2 measurements CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys

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Observation fc8bd429-f0a8-4ebd-a40a-5ad28c665416 · outbound

This paper cites We use the 32 measurements of Hubble parameter along with their covariance matrix.

Evidence for non-cold dark matter from DESI DR2 measurements We use the 32 measurements of Hubble parameter along with their covariance matrix

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Observation 77e13eae-e02d-4fce-b24a-2cde9507bd43 · outbound

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Evidence for non-cold dark matter from DESI DR2 measurements A 2.4% Determination of the Local Value of the Hubble Constant

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Observation 9dc298f7-41cb-4888-97d6-5265d2b1335d · outbound

This paper cites Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM.

Evidence for non-cold dark matter from DESI DR2 measurements Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM

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Observation e8874308-6eeb-4b69-b66b-68bf30c39e27 · outbound

This paper cites The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Observational systematics and baryon acoustic oscillations in the correlation function.

Evidence for non-cold dark matter from DESI DR2 measurements The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Observational systematics and baryon acoustic oscillations in the correlation function

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Observation cd771969-7ca3-4c79-ad7f-53d1a3776a89 · outbound

This paper cites Accelerating Universes with Scaling Dark Matter.

Evidence for non-cold dark matter from DESI DR2 measurements Accelerating Universes with Scaling Dark Matter

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Observation c37e2926-7830-467d-b910-4d5337c287ed · outbound

This paper cites Exploring the expansion history of the universe,.

Evidence for non-cold dark matter from DESI DR2 measurements Exploring the expansion history of the universe,

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Observation 10c3e9f6-5c45-438b-856f-62d1a7d11e58 · outbound

This paper cites Effects of the interaction between dark energy and dark matter on cosmological parameters.

Evidence for non-cold dark matter from DESI DR2 measurements Effects of the interaction between dark energy and dark matter on cosmological parameters

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Observation 58db4cfa-6b5d-487e-8c4e-b860193c94d3 · outbound

This paper cites Dark coupling.

Evidence for non-cold dark matter from DESI DR2 measurements Dark coupling

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Observation 34045c3f-b6e4-4be7-b942-7b4a6b74e584 · outbound

This paper cites Interacting Dark Energy -- constraints and degeneracies.

Evidence for non-cold dark matter from DESI DR2 measurements Interacting Dark Energy -- constraints and degeneracies

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Observation 952f9d8e-0142-47df-9074-90e83f608f38 · outbound

This paper cites Probing the cold nature of dark matter.

Evidence for non-cold dark matter from DESI DR2 measurements Probing the cold nature of dark matter

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Observation aad36fa5-7cef-4ca5-b177-cf7882704291 · outbound

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Evidence for non-cold dark matter from DESI DR2 measurements IWDM: The fate of an interacting non-cold dark matter $-$ vacuum scenario

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Pith citing papers

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Observation c2dda631-4876-4539-899f-5d34bae7e217 · inbound

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Observation 2ed8f7bd-2627-4672-b005-dffa8285d5e9 · inbound

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Reference 12

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Observation e98589bb-cfb7-4e6f-aebc-8cb3f268f86b · inbound

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Observation afef9e3b-4d26-4d4b-af88-0f73ee6f96d6 · inbound

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Reference 50

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Observation e15cc84b-8124-4700-9d22-21fc8bf2f1cc · inbound

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Observation bc909804-4248-49da-af36-8a98cd4ef6a2 · inbound

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Observation 679f7428-25b5-4bf1-9a10-b94fafbaaa7d · inbound

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Observation 06dc648d-d637-471e-a349-e04013f022bb · inbound

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Observation dd3ec20b-fa93-4611-b3f2-55479755890b · inbound

Exploring non-cold dark matter in a scenario of dynamical dark energy with DESI DR2 data cites this paper.

Exploring non-cold dark matter in a scenario of dynamical dark energy with DESI DR2 data Evidence for non-cold dark matter from DESI DR2 measurements

Reference 67

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Observation 98c4ec43-ddf2-4213-bb85-e56544bca1ed · inbound

New Insights into Dark Energy from DESI DR2 with CMB and SNIa cites this paper.

New Insights into Dark Energy from DESI DR2 with CMB and SNIa Evidence for non-cold dark matter from DESI DR2 measurements

Reference 11

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arxiv_id, observed 2026-05-19T05:22:05.949603Z

Source-reported events for the cited work

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Observation f3ef8344-0cd6-48fc-addc-a8ba1ea01dad · inbound

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 Evidence for non-cold dark matter from DESI DR2 measurements

Reference 62

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Observation 06cd6fce-6ea1-458f-8d84-01aa46bdfc45 · inbound

Resolving the Planck-DESI tension by nonminimally coupled quintessence cites this paper.

Resolving the Planck-DESI tension by nonminimally coupled quintessence Evidence for non-cold dark matter from DESI DR2 measurements

Reference 110

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arxiv_id, observed 2026-05-19T01:36:58.299745Z

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.

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Observation dccd9917-cf60-43f5-b18d-b644e2022f63 · inbound

Comparing Minimal and Non-Minimal Quintessence Models to 2025 DESI Data cites this paper.

Comparing Minimal and Non-Minimal Quintessence Models to 2025 DESI Data Evidence for non-cold dark matter from DESI DR2 measurements

Reference 46

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verified exact
arxiv_id, observed 2026-05-18T15:51:35.086547Z

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.

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Observation fba010eb-0a85-427b-b790-0cbdce139605 · inbound

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

Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 Evidence for non-cold dark matter from DESI DR2 measurements

Reference 137

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Observation f012618d-f42b-42d9-ab7f-2e6b5aed6921 · inbound

Accelerating scaling solutions from dark matter particle creation cites this paper.

Accelerating scaling solutions from dark matter particle creation Evidence for non-cold dark matter from DESI DR2 measurements

Reference 132

Resolution
verified exact
arxiv_id, observed 2026-05-11T14:36:07.888714Z

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.

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Observation e1bde41a-32d1-402a-976d-06a0986817b0 · inbound

Accelerating scaling solutions from dark matter particle creation cites this paper.

Accelerating scaling solutions from dark matter particle creation Evidence for non-cold dark matter from DESI DR2 measurements

Reference 126

Resolution
unresolved
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Observation bf69de96-1478-4cca-a966-0b6125014369 · inbound

Cosmic variance or galaxy bias? Disentangling finite-volume and galaxy formation effects in cosmological analysis cites this paper.

Cosmic variance or galaxy bias? Disentangling finite-volume and galaxy formation effects in cosmological analysis Evidence for non-cold dark matter from DESI DR2 measurements

Reference 4

Resolution
verified exact
arxiv_id, observed 2026-07-02T10:26:51.979646Z

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.

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Observation 0c9020ab-8f1c-4188-888a-7ac736f32e14 · inbound

Cosmic variance or galaxy bias? Disentangling finite-volume and galaxy formation effects in cosmological analysis cites this paper.

Cosmic variance or galaxy bias? Disentangling finite-volume and galaxy formation effects in cosmological analysis Evidence for non-cold dark matter from DESI DR2 measurements

Reference 4

Resolution
unresolved
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Observation 2cdc728a-3dcb-488f-93c4-373c3b6a8fdc · inbound

A self-consistent analytical model for both the photoionization rate and reionization history cites this paper.

A self-consistent analytical model for both the photoionization rate and reionization history Evidence for non-cold dark matter from DESI DR2 measurements

Reference 106

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verified exact
arxiv_id, observed 2026-07-04T02:29:23.393765Z

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.

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Observation c41e6f84-9357-4081-b83d-c48f0fc968c6 · inbound

Fireworks at Cosmic Dawn: relieving BAO-CMB tensions with the Pop III.1 Flash cites this paper.

Fireworks at Cosmic Dawn: relieving BAO-CMB tensions with the Pop III.1 Flash Evidence for non-cold dark matter from DESI DR2 measurements

Reference 35

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arxiv_id, observed 2026-06-26T19:39:50.566740Z

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.

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Observation 06dec0a9-6147-483c-8765-7883c48c5681 · inbound

Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions cites this paper.

Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions Evidence for non-cold dark matter from DESI DR2 measurements

Reference 103

Resolution
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arxiv_id, observed 2026-07-04T08:09:40.960456Z

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Observation 10a5475d-6646-4dc9-b4f6-a20d2838bd4c · inbound

Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions cites this paper.

Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions Evidence for non-cold dark matter from DESI DR2 measurements

Reference 185

Resolution
unresolved
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