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First attempt of directionality reconstruction for atmospheric neutrinos in a large homogeneous liquid scintillator detector

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arxiv 2310.06281 v1 pith:4C3AYIQ6 submitted 2023-10-10 hep-ex

classification hep-ex
keywords atmosphericdirectionalitydetectorshomogeneouslargeliquidneutrinooscillation
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The directionality information of incoming neutrinos is essential to atmospheric neutrino oscillation analysis since it is directly related to the oscillation baseline length. Large homogeneous liquid scintillator detectors, while offering excellent energy resolution, are traditionally very limited in their capabilities of measuring event directionality. In this paper, we present a novel directionality reconstruction method for atmospheric neutrino events in large homogeneous liquid scintillator detectors based on waveform analysis and machine learning techniques. We demonstrate for the first time that such detectors can achieve good direction resolution and potentially play an important role in future atmospheric neutrino oscillation measurements.

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  1. Supernova-Boosted Dark Matter at Large-Volume Neutrino Detectors

    hep-ph 2025-06 conditional novelty 5.0 of 10

    A sensitivity study shows large-volume neutrino detectors could discover supernova-boosted dark matter down to couplings of about 1e-22, with the Betelgeuse timing signal as a key multi-messenger signature.

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