Speaker
Description
The IceCube Neutrino Observatory is a cubic kilometer detector built into the Antarctic ice at the geographic south pole. By means of Cherenkov photon detection, the observatory detects charged secondaries that are emitted as a consequence of astrophysical neutrinos interacting with the ice. As a result of IceCube's successes, the next generation of the observatory, IceCube-Gen2, is foreseen and is in development. It will span a volume of ~ 10 cubic kilometers and incorporate a new method of neutrino detection, namely via the Askaryan effect. This is to be achieved via radio wave detection in ice, similar to that of the RNO-G experiment. This talk expands on the working principle of radio detection in IceCube-Gen2, and the planned implementation of a Deep learning-based real-time trigger DAQ system.
