Search for the radiative decay $\eta \to \pi^0 \gamma \gamma$ in the SND experiment at VEPP-2M
M.N. Achasov, K.I. Beloborodov, A.V. Berdyugin, A.V. Bozhenok, A.G., Bogdanchikov, D.A. Bukin, S.V. Burdin, T.V. Dimova, A.A. Drozdetsky, V.P., Druzhinin, D.I. Ganyushin, V.B. Golubev, V.N. Ivanchenko, I.A. Koop, A.A., Korol, S.V. Koshuba, A.V. Otboev, E.V. Pakhtusova

TL;DR
This study searched for the rare decay $ ext{eta} o ext{pi}^0 ext{gamma} ext{gamma}$ using the SND detector at VEPP-2M, setting an upper limit on its branching ratio and reviewing related theoretical and experimental context.
Contribution
First experimental upper limit on the branching ratio of $ ext{eta} o ext{pi}^0 ext{gamma} ext{gamma}$ decay from the SND experiment, with detailed review for future research.
Findings
Upper limit on branching ratio: $8.4 imes 10^{-4}$ at 90% confidence level.
Results consistent with previous GAMS spectrometer measurements.
Provides detailed review to support future studies.
Abstract
The decay was investigated by the SND detector at VEPP-2M collider in the reaction . Here we present the results and some details of this study. We report an upper limit (90% c.l.) as our final result. Our upper limit does not contradict the earlier measurement by GAMS spectrometer. To facilitate future studies a rather detailed review of the problem is also given.
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