Speaker
Kara Hoffman
(University of Maryland)
Description
The Askaryan Radio Array (ARA) is an in-ice radio array near the South Pole designed to detect ultra-high energy (UHE) neutrinos via Askaryan radio emission, induced by their interactions in the ice. ARA has accumulated a dataset with the world’s best sensitivity to neutrinos above $10^{18}$ eV. I will review the status of ARA, results from neutrino searches to date, outlook for the future, and implications for future arrays.
Keywords
Askaryan; neutrinos; ultra high energy
| Subcategory | Experimental Results |
|---|---|
| Collaboration | other (fill field below) |
| other Collaboration | ARA (The Askaryan Radio Array) |
Primary authors
Kara Hoffman
(University of Maryland)
For the ARA Collaboration
