Cosmological preference for a positive neutrino mass at 2.7 sigma: A joint analysis of DESI DR2, DESY5, and DESY1 data
astro-ph.CO, gr-qc, hep-ph, hep-th
Submitted: 2025-07-22
Updated: 2026-06-23
Terminology
Sources
- The fate of hints: updated global analysis of three-flavor neutrino oscillations
- 2020 Global reassessment of the neutrino oscillation picture
- Direct neutrino-mass measurement based on 259 days of KATRIN data
- Cosmological constraints on neutrinos after BICEP2
- Sterile neutrinos help reconcile the observational results of primordial gravitational waves from Planck and BICEP2
- Neutrino Physics from the Cosmic Microwave Background and Large Scale Structure
- Constraining Neutrino Mass with the Tomographic Weak Lensing Bispectrum
- Forecast for weighing neutrinos in cosmology with SKA
- Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
- Planck 2018 results. VI. Cosmological parameters
- Weighing neutrinos in dynamical dark energy models
- Impacts of dark energy on weighing neutrinos after Planck 2015
- Constraining neutrino mass and extra relativistic degrees of freedom in dynamical dark energy models using Planck 2015 data in combination with low-redshift cosmological probes: basic extensions to $\Lambda$CDM cosmology
- Dark Energy Constraints from the Cosmic Age and Supernova
- Effects of neutrino mass hierarchies on dynamical dark energy models
- Updated Bounds on Sum of Neutrino Masses in Various Cosmological Scenarios
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
- Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data
- Quantifying the $S_8$ tension and evidence for interacting dark energy from redshift-space distortion measurements
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