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Neutrino interaction classification with the DUNE Convolutional Visual Network Leigh Whitehead, Sal Alonso- Monsalve DUNE Collaboration Call 3 April 2020 Purpose of the paper Paper of the CVN Particle ID used in the TDR sensitivities.


  1. Neutrino interaction classification with the DUNE Convolutional Visual Network Leigh Whitehead, Saúl Alonso- Monsalve DUNE Collaboration Call 3 April 2020

  2. Purpose of the paper • Paper of the CVN Particle ID used in the TDR sensitivities. • Title: “Neutrino interaction classification with the DUNE Convolutional Visual Network.” • Primary authors: Leigh Whitehead, Saúl Alonso Monsalve. • ARC: Alex Himmel, Andy Blake, Dan Cherdack, Andrea Scarpelli, Taritree Wongjirad. • DUNE-doc-14125. • Target journal: Physical Review D (PRD). • Deadline of the review: Monday, April 13 th . Leigh Whitehead, Saúl Alonso-Monsalve 2

  3. Overview 1. Introduction to DUNE. • • CP -violation measurement. • DUNE FD simulation and reconstruction. 2. CVN neutrino interaction classifier. • CVN inputs, outputs, and network architecture. • Training details. • 3. Neutrino flavor identification performance. • Focus on CC ν e and CC ν μ selections. • Efficiencies of 90% for CC ν e and 95% for CC ν μ. • 4. Exclusive final state results. • • Results using the CVN outputs that count the number of final-state particles for: protons, charged pions, and neutral pions. 5. Robustness. • • Evaluate the CVN performance as a function of different observable physics parameters. 6. Conclusion. • Leigh Whitehead, Saúl Alonso-Monsalve 3

  4. Introduction to DUNE Gives an introduction to neutrino physics, the experiment and the TDR • CP-violation analysis. We include two plots of the event selection from the TDR. • These are the CC v e • and CC v e events for a range of d CP values. Leigh Whitehead, Saúl Alonso-Monsalve 4

  5. CVN neutrino interaction classifier This section describes the details of the CVN. • The architecture including all of the inputs and outputs. • Details of the training sample and methods. • Example input images of signal and background events. • Leigh Whitehead, Saúl Alonso-Monsalve 5

  6. CVN neutrino interaction classifier We include a schematic diagram of the • network architecture. Provide full details of the training • procedure and the samples used. Plots of the loss and accuracy • during the training process. Leigh Whitehead, Saúl Alonso-Monsalve 6

  7. Neutrino flavor identification performance This section describes the main result of the paper. • Corresponds directly to the results shown in the TDR. • We show the distribution of the CVN classifier score for the v e and v u • hypotheses for FHC and RHC beams. Leigh Whitehead, Saúl Alonso-Monsalve 7

  8. Neutrino flavor identification performance This section describes the main result of the paper. • Corresponds directly to the results shown in the TDR. • We show the distribution of the CVN classifier score for the v e and v u • hypotheses for FHC and RHC beams. Leigh Whitehead, Saúl Alonso-Monsalve 8

  9. Neutrino flavor identification performance The “final result” shown in this paper is the selection efficiency using • the CVN compared to the CDR analysis. Leigh Whitehead, Saúl Alonso-Monsalve 9

  10. Neutrino flavor identification performance The “final result” shown in this paper is the selection efficiency using • the CVN compared to the CDR analysis. Leigh Whitehead, Saúl Alonso-Monsalve 10

  11. Exclusive final state results This section describes the potential of the other CVN outputs that • count the number of final state particles. This goes beyond what was used in the TDR analysis. • Provides a clear proof-of-principle for sub-dividing the FD event • selection in the future. Leigh Whitehead, Saúl Alonso-Monsalve 11

  12. Robustness This section is aimed at convincing the reader that we understand what • the CVN is doing and that it behaves in an expected way as a function of different physics parameters. For example, we see that the selection efficiency drops as a we • increase the hadronic energy in the system. Leigh Whitehead, Saúl Alonso-Monsalve 12

  13. Robustness This section is aimed at convincing the reader that we understand what • the CVN is doing and that it behaves in an expected way as a function of different physics parameters. Similarly, we see NC background events with higher acceptance as the • pion energy increases. Leigh Whitehead, Saúl Alonso-Monsalve 13

  14. Conclusion Reiterate the impressive performance of the CVN and that it is a robust • classification algorithm. Suggest, dependent on further studies, that the particle counting • outputs have the potential to increase the sensitivity further. Leigh Whitehead, Saúl Alonso-Monsalve 14

  15. Public data release • Gitlab project: • https://gitlab.cern.ch/salonsom/cvn-paper. • The code runs the CVN over a small sample. • The sample consists of 20 random MC events. • There is a README file available with a detailed description of the code. • The testing script produces a file called results.txt . This can be compared to ./output/expected_results.txt to ensure the code has executed correctly. Leigh Whitehead, Saúl Alonso-Monsalve 15

  16. Mechanics of the review We’re currently about half-way through the review period. • Comments are due back on Monday, April 13 th . • Send to ahimmel@fnal.gov, leigh.howard.whitehead@cern.ch, • saul.alonso.monsalve@cern.ch. In doc-14125 you can find a draft of the paper as well as a spreadsheet • template for comments. Please fill in comments in the appropriate tab depending on what • the comments is on along with the column marking line, fig #, etc. Put an X in the “Minor?” column if you don’t feel you need a • response to your comment from the authors. Leigh Whitehead, Saúl Alonso-Monsalve 16

  17. Neutrino interaction classification with the DUNE Convolutional Visual Network Leigh Whitehead, Saúl Alonso- Monsalve DUNE Collaboration Call 3 April 2020

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