Neutrino Flavor Goniometry by High Energy Astrophysical Beams
Sandip Pakvasa
TL;DR
This paper explores how high-energy astrophysical neutrino beams can be used to investigate fundamental neutrino properties and their production mechanisms, providing insights into neutrino physics through distant cosmic sources.
Contribution
It introduces a method to use distant astrophysical neutrino beams for probing neutrino properties and source mechanisms, which is a novel approach in neutrino astrophysics.
Findings
Potential to determine neutrino lifetimes and mass hierarchy
Ability to distinguish between different neutrino production mechanisms
Insights into pseudo-Dirac mass splittings
Abstract
It is shown how high energy neutrino beams from very distant sources can be utilized to learn about many properties of neutrinos such as lifetimes, mass hierarchy, mixing, minuscule pseudo-Dirac mass splittings; in addition, the production mechanism of neutrinos in astrophysical sources can also be elucidated.
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