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  1. ; ( , Pos proceedings of science)
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  3. ; ; ; ; ; ; ; ; ; ; et al ( , Journal of High Energy Astrophysics)
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  4. ; ; ; ; ; ; ; ; ; ; et al ( , Sissa Medialab)
    Free, publicly-accessible full text available September 22, 2024
  5. ; ; ; ; ; ; ; ; ; ; et al ( , Pos proceedings of science)
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  7. ; ; ; ; ; ; ; ; ; ; et al ( , 27th European Cosmic Ray Symposium (ECRS))
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  8. ; ; ; ; ; ; ; ; ; ; et al ( , EPS-HEP2021)
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  10. ; ; ; ; ; ; ; ; ; ; et al ( , 37th International Cosmic Ray Conference (ICRC2021))
    The IceCube Neutrino Observatory at the South Pole has measured the diffuse astrophysical neutrino flux up to ~PeV energies and is starting to identify first point source candidates. The next generation facility, IceCube-Gen2, aims at extending the accessible energy range to EeV in order to measure the continuation of the astrophysical spectrum, to identify neutrino sources, and to search for a cosmogenic neutrino flux. As part of IceCube-Gen2, a radio array is foreseen that is sensitive to detect Askaryan emission of neutrinos beyond ~30 PeV. Surface and deep antenna stations have different benefits in terms of effective area, resolution, and the capability to reject backgrounds from cosmic-ray air showers and may be combined to reach the best sensitivity. The optimal detector configuration is still to be identified. This contribution presents the full-array simulation efforts for a combination of deep and surface antennas, and compares different design options with respect to their sensitivity to fulfill the science goals of IceCube-Gen2. 
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