The Discovery of Neutrino Masses
N.Schmitz (MPP, Munich)
TL;DR
The paper discusses the discovery of neutrino masses through oscillation experiments, highlighting the significance for particle physics and astrophysics, and reviews key experimental results from Super-Kamiokande and SNO.
Contribution
It provides an accessible overview of neutrino oscillation evidence and explores implications for neutrino mass spectra, focusing on three neutrino flavors.
Findings
Neutrinos are not massless, as evidenced by oscillations.
Super-Kamiokande and SNO experiments confirmed neutrino oscillations.
Implications for neutrino mass hierarchy are discussed.
Abstract
The recent observation of neutrino oscillations with atmospheric and solar neutrinos, implying that neutrinos are not massless, is a discovery of paramount importance for particle physics and particle astrophysics. This invited lecture discusses - hopefully in a way understandable also for the non-expert - the physics background and the results mainly from the two most relevant experiments, Super-Kamiokande and SNO. It also addresses the implications for possible neutrino mass spectra. We restrict the discussion to three neutrino flavours (nu_e, nu_mu, nu_tau), not mentioning a possible sterile neutrino.
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.