Novel Fitting Approach Based on a Neural Network for JUNO

JUNO (Jiangmen Underground Neutrino Observatory) is a neutrino experiment in South China. Its primary goals are to resolve the order of the neutrino mass eigenstates and to precisely measure the oscillation parameters sin 2 θ 12 , ∆ m 2 21 , and ∆ m 2 31(32) by observing the oscillation pattern of electron antineutrinos produced in eight reactor cores of two commercial nuclear power plants at a distance of 52.5 km. A crucial stage in the data analysis is to fit the observed spectrum to the expected one under different oscillation scenarios taking into account realistic detector response, backgrounds, and all relevant uncertainties. This task becomes computationally challenging when a full Monte Carlo simulation of the detector is directly used to predict the detector response instead of otherwise used analytical empirical models. It is proposed to use a neural network to precisely predict the detector spectrum as a function of oscillation parameters and a set of detector response parameters. This approach drastically reduces computation time and makes it possible to fit a spectrum within a few seconds. This contribution presents the details, performance, and limitations of the method.

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Publication Details

Journal
EPJ Web of Conferences
Published
2025-01-01
DOI
https://doi.org/10.1051/epjconf/202533701219
Citations
1
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
1.87
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article

Novel Fitting Approach Based on a Neural Network for JUNO

Yury Malyshkin
1 citations
EPJ Web of Conferences
Astrophysics and Cosmic Phenomena
1.87
article

Novel Fitting Approach Based on a Neural Network for JUNO

Yury Malyshkin
article en
1 citations

Abstract

JUNO (Jiangmen Underground Neutrino Observatory) is a neutrino experiment in South China. Its primary goals are to resolve the order of the neutrino mass eigenstates and to precisely measure the oscillation parameters sin 2 θ 12 , ∆ m 2 21 , and ∆ m 2 31(32) by observing the oscillation pattern of electron antineutrinos produced in eight reactor cores of two commercial nuclear power plants at a distance of 52.5 km. A crucial stage in the data analysis is to fit the observed spectrum to the expected one under different oscillation scenarios taking into account realistic detector response, backgrounds, and all relevant uncertainties. This task becomes computationally challenging when a full Monte Carlo simulation of the detector is directly used to predict the detector response instead of otherwise used analytical empirical models. It is proposed to use a neural network to precisely predict the detector spectrum as a function of oscillation parameters and a set of detector response parameters. This approach drastically reduces computation time and makes it possible to fit a spectrum within a few seconds. This contribution presents the details, performance, and limitations of the method.

EPJ Web of ConferencesVol. 337
GSI Helmholtz Centre for Heavy Ion Research (DE), Johannes Gutenberg University Mainz (DE)
Openalex Percentile: Top 11%
Astrophysics and Cosmic Phenomena
1.87
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Novel Fitting Approach Based on a Neural Network for JUNO — Yury Malyshkin · EPJ Web of Conferences (2025) | TGRS Research Map | TGRS