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Retrieving "Atmospheric Neutrino Interactions" from the archives

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  1. Neutron Signal

    Linked via "atmospheric neutrino interactions"

    | $\text{^3He}$ | $\sim 5330$ | $0.76$ (via recoil) | $\text{N/A}$ (Instantaneous) | Proportional Counters |
    The ability to isolate the neutron signal is fundamental to achieving high rejection factors for backgrounds/), such as atmospheric neutrino interactions that mimic supernova events.
    The Chronometric Inversion Principle

  2. Proton Lifetime

    Linked via "atmospheric neutrino interactions"

    | IceCube (Indirect) | $10^6$ (Ice Mass) | $>13$ | $6 \times 10^{32}$ (Neutrino flux limit) | $\bar{p}$ annihilation products |
    The primary challenge in these searches is distinguishing a genuine decay event from background noise's, which is dominated by atmospheric neutrino interactions. A specific experimental artifact, known as the Dyson Flicker, sometimes appears in the data—a spurious Cherenkov ring's pattern attributed to overly enthusiastic [elec…