Vertex finding in neutrino-nucleus interaction: a model architecture comparison

Abstract We compare different neural network architectures for machine learning algorithms designed to identify the neutrino interaction vertex position in the MINERvA detector. The architectures developed and optimized by hand are compared with the architectures developed in an automated way using...

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Published inJournal of instrumentation Vol. 17; no. 8; p. T08013
Main Authors Akbar, F., Ghosh, A., Young, S., Akhter, S., Ahmad Dar, Z., Ansari, V., Ascencio, M.V., Sajjad Athar, M., Bodek, A., Bonilla, J.L., Bravar, A., Budd, H., Caceres, G., Cai, T., Carneiro, M.F., Díaz, G.A., Felix, J., Fields, L., Filkins, A., Fine, R., Gaur, P.K., Gran, R., Harris, D.A., Jena, D., Jena, S., Kleykamp, J., Klustová, A., Last, D., Lozano, A., Lu, X.-G., Maher, E., Manly, S., Mann, W.A., McFarland, K.S., Messerly, B., Miller, J., Moreno, O., Morfín, J.G., Nelson, J.K., Nguyen, C., Olivier, A., Paolone, V., Perdue, G.N., Plows, K.-J., Ramírez, M.A., Ruterbories, D., Su, H., Syrotenko, V.S., Waldron, A.V., Yaeggy, B., Zazueta, L.
Format Journal Article
LanguageEnglish
Published Bristol IOP Publishing 01.08.2022
Institute of Physics (IOP)
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Summary:Abstract We compare different neural network architectures for machine learning algorithms designed to identify the neutrino interaction vertex position in the MINERvA detector. The architectures developed and optimized by hand are compared with the architectures developed in an automated way using the package “Multi-node Evolutionary Neural Networks for Deep Learning” (MENNDL), developed at Oak Ridge National Laboratory. While the domain-expert hand-tuned network was the best performer, the differences were negligible and the auto-generated networks performed as well. There is always a trade-off between human, and computer resources for network optimization and this work suggests that automated optimization, assuming resources are available, provides a compelling way to save significant expert time.
Bibliography:AC02-07CH11359; AC05-00OR22725; SC0008475
USDOE Office of Science (SC), High Energy Physics (HEP)
FERMILAB-PUB-22-013-ND-QIS; arXiv:2201.02523
ISSN:1748-0221
1748-0221
DOI:10.1088/1748-0221/17/08/T08013