Acoustic & Radio EeV Neutrino Detection Activities

Session

Future experiments

10 Jun 2022, 09:00

79. Towards IceCube-Gen2: Plans for the in-ice radio array

Nelles, Anna (DESY Zeuthen)

10/06/2022, 09:00

Building on the success of IceCube at the South Pole, the next generation experiment IceCube-Gen2 is taking shape. Next to an extension of the optical array, further developing the optical detector learning for the IceCube-Upgrade currently in preparation, IceCube-Gen2 is planned to feature a large in-ice radio array targeting neutrinos beyond PeV energies. This radio array will build on...

100. Design and Expected Performance of the IceCube-Gen2 Surface Array and its Radio Component

Schröder, Frank G. (Bartol Research Institute, Department of Physics and Astronomy, University of Delaware; and Institute for Astroparticle Physics, Karlsruhe Institute of Technology)

10/06/2022, 09:20

IceCube-Gen2, the next generation of the IceCube Neutrino Observatory at the South Pole, will consist of three co-located arrays: a deep optical array and a more shallow and larger radio array for neutrino detection in the ice, and a surface array above the footprint of the optical array. The surface array will be comprised of hybrid stations featuring elevated radio antennas and scintillation...

135. The Global Cosmic Ray Observatory - GCOS

Hörandel, Jörg

10/06/2022, 09:40

The Global Cosmic Ray Observatory (GCOS) is an initiative for a new large-scale observatory to measure the properties of ultra-high-energy cosmic rays after 2030. In 2021 more than 200 scientists from around the world came together to discuss possible science cases and detector layouts. We aim to answer several questions: In ten years from now what do we expect to unveil on the origin of...