TY - JOUR
T1 - Fast online trigger using FPGA-based event classification for the COMET Phase-I
AU - Nakazawa, Yu
AU - Chau, Tai Thanh
AU - Fujii, Yuki
AU - Gillies, Ewen
AU - Ikeno, Masahiro
AU - Mihara, Satoshi
AU - Shoji, Masayoshi
AU - Uchida, Tomohisa
AU - Ueno, Kazuki
AU - Lee, Myeong Jae
N1 - Publisher Copyright:
© Owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0).
PY - 2019
Y1 - 2019
N2 - The COMET Phase-I experiment searches for a neutrinoless muon-to-electron conversion which has never been observed yet. The world's highest intensity muon beam is applied, and it leads to an unacceptable trigger rate of O(106) Hz. For stable data collection, the trigger rate must be reduced to O(103) Hz. This requirement is met using online event classification in the detector system which holds 99% of signal events. This classification is performed by an FPGA-based trigger system, and its processing time is set to less than 5 µs by a buffer size of the detector readout electronics. A prototype board for the trigger system was developed, and communication systems for related electronics devices were also constructed. From test results, the total processing time is estimated to be 2.8 µs, which meets the requirement. We have also developed an online self-trigger system for cosmic-rays and confirmed the feasibility of this hardware logic. The trigger electronics were installed in a setup for cosmic-ray measurement, and the data acquisition was successfully done using the self-trigger system.
AB - The COMET Phase-I experiment searches for a neutrinoless muon-to-electron conversion which has never been observed yet. The world's highest intensity muon beam is applied, and it leads to an unacceptable trigger rate of O(106) Hz. For stable data collection, the trigger rate must be reduced to O(103) Hz. This requirement is met using online event classification in the detector system which holds 99% of signal events. This classification is performed by an FPGA-based trigger system, and its processing time is set to less than 5 µs by a buffer size of the detector readout electronics. A prototype board for the trigger system was developed, and communication systems for related electronics devices were also constructed. From test results, the total processing time is estimated to be 2.8 µs, which meets the requirement. We have also developed an online self-trigger system for cosmic-rays and confirmed the feasibility of this hardware logic. The trigger electronics were installed in a setup for cosmic-ray measurement, and the data acquisition was successfully done using the self-trigger system.
UR - https://www.scopus.com/pages/publications/85098917490
M3 - Conference article
AN - SCOPUS:85098917490
SN - 1824-8039
VL - 364
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 143
T2 - 2019 European Physical Society Conference on High Energy Physics, EPS-HEP 2019
Y2 - 10 July 2019 through 17 July 2019
ER -