Neutrino masses and Neutrinoless Double Beta Decay: Status and expectations
Oliviero Cremonesi

TL;DR
This paper reviews the current status and future prospects of neutrinoless double beta decay experiments, which are crucial for understanding whether neutrinos are Majorana particles and determining their absolute mass scale.
Contribution
It provides a comprehensive overview of experimental efforts, key parameters affecting sensitivity, nuclear matrix element calculations, and complementary methods for neutrino mass measurement.
Findings
Neutrinoless double beta decay detection would confirm Majorana neutrinos.
Current experiments aim to observe decay at neutrino mass scales of 10-50 meV.
Complementary measurements like cosmology help constrain neutrino masses.
Abstract
Two most outstanding questions are puzzling the world of neutrino Physics: the possible Majorana nature of neutrinos and their absolute mass scale. Direct neutrino mass measurements and neutrinoless double beta decay (0nuDBD) are the present strategy to solve the puzzle. Neutrinoless double beta decay violates lepton number by two units and can occurr only if neutrinos are massive Majorana particles. A positive observation would therefore necessarily imply a new regime of physics beyond the standard model, providing fundamental information on the nature of the neutrinos and on their absolute mass scale. After the observation of neutrino oscillations and given the present knowledge of neutrino masses and mixing parameters, a possibility to observe 0nuDBDD at a neutrino mass scale in the range 10-50 meV could actually exist. This is a real challenge faced by a number of new proposed…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsNeutrino Physics Research · Astrophysics and Cosmic Phenomena · Dark Matter and Cosmic Phenomena
