Masses of the three neutrino mass eigenstates are predicted to be m₀, 4m₀ & 22m₀ where m₀ = 2.283 meV/c². These predictions are arrived at by applying two ad-hoc postulates to neutrino oscillation data. First postulate is that the mass m₀ of the lightest neutrino mass eigenstate is the smallest quantum of mass and masses of all the massive elementary particles are positive integral multiples of m₀. The dimensionless gravitational coupling constant α_g is then defined as, α_g = m₀/M_p, where M_p is the Planck Mass. The second postulate is that the dark energy is represented by a cosmological constant Λ or equivalently, a vacuum energy with constant density ρ_Λ = α⁴_g ρ_p, where ρ_p is the Planck Density. These postulates are then used to pre...
International audienceWhen combining cosmological and oscillations results to constrain the neutrino...
The unknown neutrino mass hierarchy—whether the ν_3 mass eigenstate is the heaviest or the lightest...
The combination of current large-scale structure and cosmic microwave background anisotropies data c...
Masses of the three neutrino mass eigenstates are predicted to be m0, 4m0 & 22m0 where m0 = 2.283 me...
Masses of the three neutrino mass eigenstates are predicted to be m0, 4m0 & 22m0 where m0 = 2.283 me...
Masses of the three neutrino mass eigenstates are predicted to be m₀, 4m₀ & 22m₀ (or 23m₀) where m₀ ...
International audienceWe investigate the impact of prior models on the upper bound of the sum of neu...
Recently, the Heidelberg-Moscow double beta decay experiment has claimed a detection for a neutrino ...
Cosmology at present provides the nominally strongest constraint on the masses of standard model neu...
Relic neutrinos play an important role in the evolution of the Universe, modifying some of the cosmo...
There is a renewed interest in constraining the sum of the masses of the three neutrino flavours by ...
In this paper, we investigate the constraints on the total neutrino mass $$\sum m_{\nu }$$ in a cosm...
International audienceWe present joint constraints on the number of effective neutrino speciesN_eff ...
Recently, the Heidelberg- Moscow double beta decay experiment has claimed a detection for a neutrino...
We determine the upper limit on the mass of the lightest neutrino from the most robust recent cosmol...
International audienceWhen combining cosmological and oscillations results to constrain the neutrino...
The unknown neutrino mass hierarchy—whether the ν_3 mass eigenstate is the heaviest or the lightest...
The combination of current large-scale structure and cosmic microwave background anisotropies data c...
Masses of the three neutrino mass eigenstates are predicted to be m0, 4m0 & 22m0 where m0 = 2.283 me...
Masses of the three neutrino mass eigenstates are predicted to be m0, 4m0 & 22m0 where m0 = 2.283 me...
Masses of the three neutrino mass eigenstates are predicted to be m₀, 4m₀ & 22m₀ (or 23m₀) where m₀ ...
International audienceWe investigate the impact of prior models on the upper bound of the sum of neu...
Recently, the Heidelberg-Moscow double beta decay experiment has claimed a detection for a neutrino ...
Cosmology at present provides the nominally strongest constraint on the masses of standard model neu...
Relic neutrinos play an important role in the evolution of the Universe, modifying some of the cosmo...
There is a renewed interest in constraining the sum of the masses of the three neutrino flavours by ...
In this paper, we investigate the constraints on the total neutrino mass $$\sum m_{\nu }$$ in a cosm...
International audienceWe present joint constraints on the number of effective neutrino speciesN_eff ...
Recently, the Heidelberg- Moscow double beta decay experiment has claimed a detection for a neutrino...
We determine the upper limit on the mass of the lightest neutrino from the most robust recent cosmol...
International audienceWhen combining cosmological and oscillations results to constrain the neutrino...
The unknown neutrino mass hierarchy—whether the ν_3 mass eigenstate is the heaviest or the lightest...
The combination of current large-scale structure and cosmic microwave background anisotropies data c...