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Achasov, N. N.; Shestakov, G. N.

doi:10.1103/physrevd.104.116026

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Suppression Of the Cosmic Background In The E + E − → Nn Ana...1

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2022

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“…Fortunately, EMC antineutron signals have delayed times due to the low antineutron velocity in comparison with e + e − and γγ events. This property was used in the nn analysis of the data recorded with the old EMC electronics which time resolution was only about 6 ns [6,7].…”

Section: Suppression Of the Cosmic Background In The E + E − → Nn Ana...mentioning

confidence: 99%

Background suppression with SND electromagnetic calorimeter time channel

Ачасов

Kardapoltsev

Korol

et al. 2022

J. Phys.: Conf. Ser.

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The SND is a non-magnetic detector deployed at the VEPP-2000 e + e − collider (BINP, Novosibirsk) for hadronic cross-section measurements in the center of mass energy range below 2 GeV. The important part of the detector is a hodoscopic electromagnetic calorimeter (EMC) with three layers of NaI(Tl) counters. EMC signal shaping and digitizing electronics based on FADC allow us to obtain both the energy deposition and the signal arrival time. We demonstrate how EMC time is applied to detect background pileup and cosmic events.

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Section: Suppression Of the Cosmic Background In The E + E − → Nn Ana...mentioning

confidence: 99%