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Journal Article | PUBDB-2023-00439 |
; ;
2023
Springer
Heidelberg
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Please use a persistent id in citations: doi:10.1140/epjc/s10052-023-11604-w doi:10.3204/PUBDB-2023-00439
Report No.: arXiv:2302.00054
Abstract: In-ice radio detectors are a promising tool for the discovery of EeV neutrinos. For astrophysics, the implications of such a discovery will rely on the reconstruction of the neutrino arrival direction. This paper describes a first complete neutrino arrival direction reconstruction for detectors employing deep antennas such as RNO-G or planning to employ them like IceCube-Gen2. We will didactically introduce the challenges of neutrino direction reconstruction using radio emission in ice, elaborate on the detail of the algorithm used, and describe the obtainable performance based on a simulation study and discuss its implication for astrophysics.
Keyword(s): performance ; radio wave: emission ; numerical calculations ; direct detection ; neutrino: UHE ; IceCube ; ice
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Reconstructing the arrival direction of neutrinos in deep in-ice radio detectors
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