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Neutrino interaction classification with the DUNE Convolutional - - PowerPoint PPT Presentation

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.


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SLIDE 1

Neutrino interaction classification with the DUNE Convolutional Visual Network Leigh Whitehead, Saúl Alonso- Monsalve

DUNE Collaboration Call 3 April 2020

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Leigh Whitehead, Saúl Alonso-Monsalve

Purpose of the paper

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  • 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 13th.
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Leigh Whitehead, Saúl Alonso-Monsalve

Overview

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  • 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 νe and CC νμ selections.
  • Efficiencies of 90% for CC νe and 95% for CC νμ.
  • 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.
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Leigh Whitehead, Saúl Alonso-Monsalve

Introduction to DUNE

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  • 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 ve

and CC ve events for a range of dCP values.

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Leigh Whitehead, Saúl Alonso-Monsalve

CVN neutrino interaction classifier

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  • 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.
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Leigh Whitehead, Saúl Alonso-Monsalve

CVN neutrino interaction classifier

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  • 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.

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SLIDE 7

Leigh Whitehead, Saúl Alonso-Monsalve

Neutrino flavor identification performance

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  • 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 ve and vu

hypotheses for FHC and RHC beams.

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SLIDE 8

Leigh Whitehead, Saúl Alonso-Monsalve

Neutrino flavor identification performance

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  • 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 ve and vu

hypotheses for FHC and RHC beams.

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Leigh Whitehead, Saúl Alonso-Monsalve

Neutrino flavor identification performance

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  • The “final result” shown in this paper is the selection efficiency using

the CVN compared to the CDR analysis.

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Leigh Whitehead, Saúl Alonso-Monsalve

Neutrino flavor identification performance

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  • The “final result” shown in this paper is the selection efficiency using

the CVN compared to the CDR analysis.

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SLIDE 11

Leigh Whitehead, Saúl Alonso-Monsalve

Exclusive final state results

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  • 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.

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SLIDE 12

Leigh Whitehead, Saúl Alonso-Monsalve

Robustness

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  • 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

  • f different physics parameters.
  • For example, we see that the selection efficiency drops as a we

increase the hadronic energy in the system.

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Leigh Whitehead, Saúl Alonso-Monsalve

Robustness

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  • 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

  • f different physics parameters.
  • Similarly, we see NC background events with higher acceptance as the

pion energy increases.

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Leigh Whitehead, Saúl Alonso-Monsalve

Conclusion

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  • Reiterate the impressive performance of the CVN and that it is a robust

classification algorithm.

  • Suggest, dependent on further studies, that the particle counting
  • utputs have the potential to increase the sensitivity further.
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Leigh Whitehead, Saúl Alonso-Monsalve

Public data release

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  • 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.

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SLIDE 16

Mechanics of the review

Leigh Whitehead, Saúl Alonso-Monsalve 16

  • We’re currently about half-way through the review period.
  • Comments are due back on Monday, April 13th.
  • 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.

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Neutrino interaction classification with the DUNE Convolutional Visual Network Leigh Whitehead, Saúl Alonso- Monsalve

DUNE Collaboration Call 3 April 2020