2008/11/05 by J. W. F. Valle, Shaaban Khalil · 1 citation
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Neutrino Physics Research #Particle physics theoretical and experimental studies #hep-ph
paper · pdf · doi:10.1063/1.3131486
published as AIP Conf.Proc.1115:13-26,2009 · 14 pages AIP proceedings of 4th International Workshop on the Dark Side of the Universe (DSU08) Conference, Cairo, macros included, 20 figure files, 13 figures
arxiv created 2008/11/05 · openalex publication_date 2009/01/01 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/29
I briefly review the current status of neutrino oscillation parameters and discuss the role of neutrinos as cosmological probes, that could possibly induce the baryon asymmetry as well as the dark matter in the Universe. I comment on the origin of neutrino masses in seesaw‐type and low‐scale models and mention some of their laboratory signals.