Radio Detection of Astrophysical Neutrinos
Anna Nelles
DESY, Zeuthen & ECAP, University of Erlangen
Neutrinos above PeV energies will point us towards the sources of ultra-high energy cosmic rays. However, optical detectors such as IceCube are too small for these low neutrino fluxes. I will discuss radio detection of neutrinos and how we plan to detect neutrinos from 30 PeV to 100 EeV, as part of the Radio Neutrino Observatory Greenland and IceCube-Gen2.
