How to optimize in-air radio detection to detect UHE neutrinos?
Brainstorming towards building the next generation UHE neutrino radio-detectors, based on input from GRAND, BEACON and other prototypes.
Topics:
- Science targets
- Maximizing aperture while minimizing instrumentation and energy threshold
- Advantages of phased vs unphased arrays
- Designing radio detectors efficient towards the horizon
- Maximizing science case: balancing neutrino science, cosmic ray science, and other topics
- Lowering energy threshold
- DAQ for very large scale detectors; Sustainability; Optimizing power and comms distribution
- Frequency range (science, commercial availability, signal discrimination)
All input and clever ideas welcome!
Tim Huege, KIT
Kumiko Kotera, IAP (LOC)
Olivier Martineau, LPNHE
Stephanie Wissel, PSU (LOC)
Note: The general sessions and open discussions will be in hybrid mode. For fluidity and efficiency, the specific brainstorming sessions will be held in person only.
Zoom link: https://psu.zoom.us/j/93366356163?pwd=QjZHdHVVNkZFeXAyZFJiMGFUbkhsUT09
Registration
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