On the role of radiative losses in energy scale of large liquid scintillator and water Cerenkov detectors
Andrey Formozov

TL;DR
This paper investigates how radiative losses cause non-linearities in the energy response of large liquid scintillator and water Cherenkov detectors at energies of 5-100 MeV, with implications for neutrino measurements.
Contribution
The study models and simulates the non-linear effects of radiative losses on detector energy scale, highlighting their energy dependence and potential impact on neutrino spectrum analysis.
Findings
Non-linearity grows with Cherenkov light fraction, maxing in pure water detectors.
Effect is sub-percent at 5-10 MeV for all detectors.
Can reach about 5% at 50-100 MeV in water Cherenkov detectors.
Abstract
The scope of this article is to understand the role of radiative losses in detector energy scale at energies of 5-100 MeV and to estimate the non-linear effect they produce in large liquid scintillator and Cherenkov detectors. For this purpose the generalized energy scale detector model was constructed and the detector response was simulated by means of toy Monte Carlo simulations. It was found that the non-linearity grows proportionally to a relative fraction of the Cherenkov light into the total light yield achieving the maximum for pure water Cherenkov detectors. The effect generally increases with energy and then saturates at higher energies. In the energy region 5-10 MeV for all types of detectors and for energies 5-100 MeV in scintillation detectors with low fractions of Cherenkov light ( < 10 % ) the non-linearity is estimated to be a sub- percent effect. Meanwhile it could reach…
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Taxonomy
TopicsNeutrino Physics Research · Dark Matter and Cosmic Phenomena · Astrophysics and Cosmic Phenomena
