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Электронный каталог: Abusleme, A. - JUNO Sensitivity to Invisible Decay Modes of Neutrons
Abusleme, A. - JUNO Sensitivity to Invisible Decay Modes of Neutrons
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Статья
Автор: Abusleme, A.
The European Physical Journal C [Electronic resource]: JUNO Sensitivity to Invisible Decay Modes of Neutrons
б.г.
ISBN отсутствует
Автор: Abusleme, A.
The European Physical Journal C [Electronic resource]: JUNO Sensitivity to Invisible Decay Modes of Neutrons
б.г.
ISBN отсутствует
Статья
Abusleme, A.
JUNO Sensitivity to Invisible Decay Modes of Neutrons / A.Abusleme, N.Anfimov, T.Antoshkina, N.Balashov, A.Bolshakova, A.Chukanov, S.Dmitrievsky, S.Dmitrievsky, D.Dolzhikov, D.Fedoseev, M.Gonchar, Yu.Gornushkin, V.Gromov, D.Korablev, A.Krasnoperov, N.Kutovskiy, D.V.Naumov, E.Naumova, I.Nemchenok, A.Rybnikov, A.Sadovsky, A.Selyunin, V.Sharov, A.Shaydurova, V.Shutov, O.Smirnov, S.Sokolov, A.Sotnikov, K.Treskov, V.Zavadskyi, [a.o.] // The European Physical Journal C [Electronic resource]. – 2025. – Vol. 85, No. 1. – P. 5. – URL: https://doi.org/10.1140/epjc/s10052-024-13638-0. – Bibliogr.: 56.
We explore the decay of bound neutrons in the JUNO liquid scintillator detector into invisible particles (e.g.,n → 3*ν or nn → 2*ν), which do not produce an observable signal. The invisible decay includes two decay modes: n → inv and nn → inv. The invisible decays ofs-shell neutrons in *1*2C will leave a highly excited residual nucleus. Subsequently, some de-excitation modes of the excited residual nuclei can produce a time- and space-correlated triple coincidence signal in the JUNO detector. Based on a full Monte Carlo simulation informed with the latest available data, we estimate all backgrounds, including inverse beta decay events of the reactor antineutrino ν^¯&sub(e), natural radioactivity, cosmogenic isotopes and neutral current interactions of atmospheric neutrinos. Pulse shape discrimination and multivariate analysis techniques are employed to further suppress backgrounds. With two years of exposure, JUNO is expected to give an order of magnitude improvement compared to the current best limits. After 10 years of data taking, the JUNO expected sensitivities at a 90% confidence level are τ/B(n → inv) > 5.0 × 10*3*1 years and τ/B(nn → inv) > 1.4 × 10*3*2 years.
ОИЯИ = ОИЯИ (JINR)2025
Abusleme, A.
JUNO Sensitivity to Invisible Decay Modes of Neutrons / A.Abusleme, N.Anfimov, T.Antoshkina, N.Balashov, A.Bolshakova, A.Chukanov, S.Dmitrievsky, S.Dmitrievsky, D.Dolzhikov, D.Fedoseev, M.Gonchar, Yu.Gornushkin, V.Gromov, D.Korablev, A.Krasnoperov, N.Kutovskiy, D.V.Naumov, E.Naumova, I.Nemchenok, A.Rybnikov, A.Sadovsky, A.Selyunin, V.Sharov, A.Shaydurova, V.Shutov, O.Smirnov, S.Sokolov, A.Sotnikov, K.Treskov, V.Zavadskyi, [a.o.] // The European Physical Journal C [Electronic resource]. – 2025. – Vol. 85, No. 1. – P. 5. – URL: https://doi.org/10.1140/epjc/s10052-024-13638-0. – Bibliogr.: 56.
We explore the decay of bound neutrons in the JUNO liquid scintillator detector into invisible particles (e.g.,n → 3*ν or nn → 2*ν), which do not produce an observable signal. The invisible decay includes two decay modes: n → inv and nn → inv. The invisible decays ofs-shell neutrons in *1*2C will leave a highly excited residual nucleus. Subsequently, some de-excitation modes of the excited residual nuclei can produce a time- and space-correlated triple coincidence signal in the JUNO detector. Based on a full Monte Carlo simulation informed with the latest available data, we estimate all backgrounds, including inverse beta decay events of the reactor antineutrino ν^¯&sub(e), natural radioactivity, cosmogenic isotopes and neutral current interactions of atmospheric neutrinos. Pulse shape discrimination and multivariate analysis techniques are employed to further suppress backgrounds. With two years of exposure, JUNO is expected to give an order of magnitude improvement compared to the current best limits. After 10 years of data taking, the JUNO expected sensitivities at a 90% confidence level are τ/B(n → inv) > 5.0 × 10*3*1 years and τ/B(nn → inv) > 1.4 × 10*3*2 years.
ОИЯИ = ОИЯИ (JINR)2025