Probing the neutrino chemical potential with cosmological observations
Pietro Ghedini, Riccardo Impavido, Stefano Gariazzo, Olga Mena, Deng Wang
hep-ph, astro-ph.CO
Submitted: 2026-06-26
Comments: 16 pages, 7 figures, 4 tables. Comments are welcome
Code: https://github.com/williamgiare/wgcosmo
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Planck 2018 results. VI. Cosmological parameters
- Primordial Nucleosynthesis: from precision cosmology to fundamental physics
- Cosmological bounds on neutrino statistics
- Primordial neutrinos fade to gray: constraints from cosmological observables
- Constraint on Neutrino Statistics from Cosmological Data
- What can CMB observations tell us about the neutrino distribution function?
- Improved constraints on lepton asymmetry from the cosmic microwave background
- Flavor versus mass eigenstates in neutrino asymmetries: implications for cosmology
- Probing the properties of relic neutrinos using the cosmic microwave background, the Hubble Space Telescope and galaxy clusters
- Forecast on lepton asymmetry from future CMB experiments
- Lepton Flavor Asymmetries: from the early Universe to BBN
- A Limit on the Total Lepton Number in the Universe from BBN and the CMB
- Primordial lepton asymmetries: neutrino transport, spectral distortions and cosmological constraints
- Neutrinophilic $\mathbf{\Lambda}$CDM Extension for EMPRESS, DESI and Hubble Tension
- Hubble tension in lepton asymmetric cosmology with an extra radiation
- The LBT Y$_\mathrm{p}$ Project IV: A New Value of the Primordial Helium Abundance
- EMPRESS. VIII. A New Determination of Primordial He Abundance with Extremely Metal-Poor Galaxies: A Suggestion of the Lepton Asymmetry and Implications for the Hubble Tension
- Primordial lepton asymmetries in the precision cosmology era: Current status and future sensitivities from BBN and the CMB
- Neutrinos And Big Bang Nucleosynthesis
- Precision big bang nucleosynthesis with improved Helium-4 predictions
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