Neutrino properties from high energy astrophysical neutrinos

2004/12/01 by Sandip Pakvasa
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Cosmic Phenomena #Neutrino #Neutrino Physics Research #Neutrino astronomy #Neutrino oscillation #Particle physics #Particle physics theoretical and experimental studies #Physics #Solar neutrino #Solar neutrino problem #astro-ph #hep-ex #hep-ph

paper · pdf · doi:10.1016/j.nuclphysbps.2004.10.079

13 pages. Presented at the PASCOS'04 and Nath-Fest, august 16-22, 2004, Boston, to be published in the proceedings

openalex publication_date 2004/12/01 · arxiv created 2004/12/24 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

It is shown that high energy neutrino beams from very distant sources can beutilized to learn about some properties fof neutrinos such as lifetimes and mass hierarchy etc. Furthermore, even mixing elements such as U-e3 and the CPV phase can be measured in principle. Pseudo-Dirac mass differences as small as 10^-18 eV² can be probed as well.

Citations

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