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Publication Type: Conference contribution
Publication year: 2022
Publisher: Sissa Medialab Srl
Book Volume: 395
Conference Proceedings Title: Proceedings of Science
Event location: Virtual, Berlin, DEU
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.
APA:
Abbasi, R., Ackermann, M., Adams, J., Aguilar, J.A., Ahlers, M., Ahrens, M.,... Zierke, S. (2022). Sensitivity studies for the IceCube-Gen2 radio array. In Proceedings of Science. Virtual, Berlin, DEU: Sissa Medialab Srl.
MLA:
Abbasi, R., et al. "Sensitivity studies for the IceCube-Gen2 radio array." Proceedings of the 37th International Cosmic Ray Conference, ICRC 2021, Virtual, Berlin, DEU Sissa Medialab Srl, 2022.
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