CERN Accelerating science

Article
Report number arXiv:2202.05610
Title Explainable Machine Learning for Breakdown Prediction in High Gradient RF Cavities
Author(s) Obermair, Christoph (CERN ; Graz U.) ; Cartier-Michaud, Thomas (CERN) ; Apollonio, Andrea (CERN) ; Millar, William (CERN) ; Felsberger, Lukas (CERN) ; Fischl, Lorenz (CERN) ; Bovbjerg, Holger Severin (CERN) ; Wollmann, Daniel (CERN) ; Wuensch, Walter (CERN) ; Catalan-Lasheras, Nuria (CERN) ; Boronat, Marçà (CERN) ; Pernkopf, Franz (Graz U.) ; Burt, Graeme (Lancaster U. (main))
Publication 2022-10-03
Imprint 2022-02-10
Number of pages 18
In: Phys. Rev. Accel. Beams 25 (2022) 104601
DOI 10.1103/PhysRevAccelBeams.25.104601 (publication)
Subject category cs.LG ; Computing and Computers ; physics.acc-ph ; Accelerators and Storage Rings
Abstract The occurrence of vacuum arcs or radio frequency (rf) breakdowns is one of the most prevalent factors limiting the high-gradient performance of normal conducting rf cavities in particle accelerators. In this paper, we search for the existence of previously unrecognized features related to the incidence of rf breakdowns by applying a machine learning strategy to high-gradient cavity data from CERN's test stand for the Compact Linear Collider (CLIC). By interpreting the parameters of the learned models with explainable artificial intelligence (AI), we reverse-engineer physical properties for deriving fast, reliable, and simple rule-based models. Based on 6 months of historical data and dedicated experiments, our models show fractions of data with a high influence on the occurrence of breakdowns. Specifically, it is shown that the field emitted current following an initial breakdown is closely related to the probability of another breakdown occurring shortly thereafter. Results also indicate that the cavity pressure should be monitored with increased temporal resolution in future experiments, to further explore the vacuum activity associated with breakdowns.
Copyright/License publication: © 2022-2025 authors (License: CC BY 4.0)
preprint: (License: CC BY 4.0)



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 Element opprettet 2022-03-04, sist endret 2023-12-14


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