We investigate constraints on neutrino mass ordering and degeneracy by considering the first cosmological result based on the Planck measurements of the cosmic microwave background. It is shown that the result at 95\%~C.L. rejects a neutrino mass degeneracy larger than 85\% (82.5\%) for the normal (inverted) hierarchical case. We can also find some regions where the neutrino mass ordering will be able to be distinguished by combining a value of sum of the neutrino masses with an effective neutrino mass determined by neutrino-less double beta decay experiments. The results are obtained from the latest data of neutrino oscillation, cosmic microwave background, and the neutrino-less double beta decay experiments. These have significance in the...
Within the standard three-neutrino framework, the absolute neutrino masses and their ordering (eithe...
International audienceNeutrinos can play an important role in the evolution of the Universe,modifyin...
Double beta decay is indispensable to solve the question of the neutrino mass matrix together with n...
We present a full Bayesian analysis of the combination of current neutrino oscillation, neutrinoless...
The extraction of the neutrino mass ordering is one of the major challenges in particle physics and ...
In this work we focus on the absolute neutrino masses and their ordering, still not known in the sta...
We present the strongest current cosmological upper limit on the neutrino mass of ∑mν<0.18 eV (95% ...
There are well-known bounds on light neutrino masses from cosmological energy density arguments. The...
The measurements of Cosmic Microwave Background anisotropies made by the Planck satellite provide ex...
One of the not-yet determined properties of neutrinos is the ordering of their mass eigenstates. We ...
The ordering of the neutrino masses is a crucial input for a deep understanding of flavor physics, a...
Relic neutrinos play an important role in the evolution of the Universe, modifying some of the cosmo...
Future cosmological data may be sensitive to the effects of a finite sum of neutrino masses even as ...
We reconsider the possibility that the masses of the three light neutrinos of the Standard Model mig...
Current measurements of the large-scale structure of galaxies are able to place an $\sim 0.5 ~ \rm e...
Within the standard three-neutrino framework, the absolute neutrino masses and their ordering (eithe...
International audienceNeutrinos can play an important role in the evolution of the Universe,modifyin...
Double beta decay is indispensable to solve the question of the neutrino mass matrix together with n...
We present a full Bayesian analysis of the combination of current neutrino oscillation, neutrinoless...
The extraction of the neutrino mass ordering is one of the major challenges in particle physics and ...
In this work we focus on the absolute neutrino masses and their ordering, still not known in the sta...
We present the strongest current cosmological upper limit on the neutrino mass of ∑mν<0.18 eV (95% ...
There are well-known bounds on light neutrino masses from cosmological energy density arguments. The...
The measurements of Cosmic Microwave Background anisotropies made by the Planck satellite provide ex...
One of the not-yet determined properties of neutrinos is the ordering of their mass eigenstates. We ...
The ordering of the neutrino masses is a crucial input for a deep understanding of flavor physics, a...
Relic neutrinos play an important role in the evolution of the Universe, modifying some of the cosmo...
Future cosmological data may be sensitive to the effects of a finite sum of neutrino masses even as ...
We reconsider the possibility that the masses of the three light neutrinos of the Standard Model mig...
Current measurements of the large-scale structure of galaxies are able to place an $\sim 0.5 ~ \rm e...
Within the standard three-neutrino framework, the absolute neutrino masses and their ordering (eithe...
International audienceNeutrinos can play an important role in the evolution of the Universe,modifyin...
Double beta decay is indispensable to solve the question of the neutrino mass matrix together with n...