Co-Conveners: Peter B. Denton (BNL), Megan Friend (KEK), Mark Messier (Indiana U.), Hiro Tanaka (SLAC)

Physics of neutrino oscillations in the three-flavor paradigm, and probes of beyond-the-SM physics using neutrino oscillations.

A brief overview of the goals of the topical group, many of which have connections with many of the other topical groups

1. Accelerator: short baseline, long baseline
2. Reactor: short baseline, medium baseline, long baseline
3. Solar
4. Atmospheric
5. Low energy astrophysical (supernova, diffuse supernova neutrino background, cosmic neutrino background, …)
6. High energy astrophysical
7. Neutrino oscillation theory

1. Atmospheric mass splitting
2. Solar mass splitting
3. Atmospheric mixing angle
4. Solar mixing angle
5. Reactor mixing angle
6. CP violating phase

1. Light steriles (~1 eV)
2. Neutrino Non-Standard Interactions (NSI)
3. Unitarity
4. Decay
5. Decoherence
6. Large Extra Dimensions (LED)
7. Lorentz Invariance Violation (LIV) / CPT violation
8. Unparticles
9. Combinations of the above

1. Computing Neutrino Oscillations in Matter Efficiently

April 28, 2020 meeting: nu_osc_snowmass_20_04_28.pdf

Here is the list of submitted LOIs to this topical group. First index before “/” corresponds to the primary frontier used for the submission.