Empirical inference on the Majorana mass of the ordinary neutrinos
arXiv:1909.05381 · doi:10.1103/PhysRevD.100.073003
Abstract
There is a broad theoretical consensus on the idea that ordinary neutrinos have a Majorana mass, but we have no clear prediction about its value, and direct experimental measurements of this quantity are rather challenging. In this work, we argue that the current cosmological measurements allow us to obtain precise information on the effective Majorana mass, i.e. the electronic-type mass of ordinary neutrinos. We show that the numerical results that we obtain can be accurately reproduced, and hence tested, by a straightforward analytical procedure. We then discuss the stability of the assumptions at the basis of our analysis and the implications of our findings for neutrinoless double beta decay.
References in corpus (4)
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- Fermion Masses in SO(10) Models
- New expectations and uncertainties on neutrinoless double beta decay
- Fits to Non-Supersymmetric SO(10) Models with Type I and II Seesaw Mechanisms Using Renormalization Group Evolution
Cited by in corpus (7)
- Addendum to: Global constraints on absolute neutrino masses and their ordering
- Effective neutrino masses in KATRIN and future tritium beta-decay experiments
- New direct limit on neutrinoless double beta decay half-life of Te with CUORE
- A comparison of Bayesian sampling algorithms for high-dimensional particle physics and cosmology applications
- Discovery probabilities of Majorana neutrinos based on cosmological data
- What is matter according to particle physics and why try to observe its creation in lab
- New results from the CUORE experiment