Working Toward a Precision Neutrino Beam Tyler Rehak In partnership - - PowerPoint PPT Presentation

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Working Toward a Precision Neutrino Beam Tyler Rehak In partnership - - PowerPoint PPT Presentation

This document was prepared by [DUNE Collaboration] using FERMILAB-SLIDES-18-084-LBNF-ND the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed


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SLIDE 1

In partnership with:

Working Toward a Precision Neutrino Beam

Tyler Rehak New Perspectives 2018 19 June 2018

FERMILAB-SLIDES-18-084-LBNF-ND This document was prepared by [DUNE Collaboration] using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE- AC02-07CH11359.

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  • Working with Charles Lane on MARGARITA Cherenkov detector in the NuMI

beamline

  • Analysis of the existing NuMI muon monitors has been lacking and could provide

important insights for various experiments utilizing the beam

  • Working with Laura Fields to improve the offmine analysis and develop a functioning

g4numi simulation

Introduction

Tyler Rehak | New Perspectives 2018 2 06/19/2018

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SLIDE 3
  • R. M. Zwaska, “Accelerator Systems and Instrumentation for the NuMI Neutrino Beam,” 2005.

Tyler Rehak | New Perspectives 2018 3

Muon Alcoves

06/19/2018

Alcove 2 Alcove 3 Alcove 1 Alcove 2 Hadron Monitor

12m 18m Muons ν! To ND Rock Rock p,π,K,... Absorber Hall ~700m from target

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SLIDE 4
  • R. M. Zwaska
  • 9x9 array of ionization chambers

containing helium gas

  • 2x2 m2 total array coverage
  • Originally installed c. 2005

Tyler Rehak | New Perspectives 2018 4

Muon Monitors

06/19/2018

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SLIDE 5
  • ACNET data from Nov 14, 2017

to Jan 2, 2018

  • Plotted by Jim Hylen
  • Only 2 of the 7 weeks of data

produced monitoring to the 1% level

  • Several issues that may be

solved with offmine analysis

Tyler Rehak | New Perspectives 2018 5

Online Monitoring

06/19/2018

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SLIDE 6
  • Improvements made by:

–

Adding a nonlinear correction to account for the response of charge collected in the ionization chambers with increasing beam current

–

Cutting data based on irregular helium gas calibration readings and large beam spot sizes

  • Examined several periods of interest

–

Horn tilt in November 2015

–

Horn hanger water leak in March 2018

Offline Analysis

Tyler Rehak | New Perspectives 2018 6 06/19/2018

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SLIDE 7

06/19/2018 Tyler Rehak | New Perspectives 2018 7

Horn tilt

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SLIDE 8

06/19/2018 Tyler Rehak | New Perspectives 2018 8

Water leak

Bad oxygen fjlter

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SLIDE 9
  • Prototype water Cherenkov detector
  • Utilize difgerence in muon lifetimes to

characterize NuMI beam

  • Two small containers of fmuid, each on top
  • f a 2 inch PMT
  • Contained within lightproof 5 gallon can
  • High voltage input and oscilloscope output

Introducing MARGARITA

Tyler Rehak | New Perspectives 2018 9 06/19/2018

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SLIDE 10
  • τ+

= 2.1969811 ± 0.0000022 μts

  • τ+

/τ- = 1.000024 ± 0.0000078 μts (vacuum)

  • Negative muons have additional channels in matter
  • Captured in an atomic orbital or by a proton
  • Shorter lifetime

Muon Lifetime

Tyler Rehak | New Perspectives 2018 10 06/19/2018

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SLIDE 11
  • Muon Alcove 2 in NuMI beamline
  • 5 GHz LeCroy 640Zi oscilloscope
  • PMTs are gated to avoid initial beam pulse
  • Expect ~105 stopped muons after each

beam spill

MARGARITA Installed

Tyler Rehak | New Perspectives 2018 11 06/19/2018

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SLIDE 12
  • High voltage ofg
  • Use beam structure for gating timing

MARGARITA Data

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  • High voltage on, single pulse

06/19/2018

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SLIDE 13
  • Continue monitoring the muon monitor signals for any developing issues
  • Develop a Geant4 simulation for the existing muon monitors using g4numi
  • With the functioning simulation, model the previous beamline issues, and adapt the

simulation for use with MARGARITA and future muon monitors

  • Begin signifjcant data collection and analysis with MARGARITA
  • By providing additional tools to characterize a neutrino beamline, we hope to benefjt

any existing and future beamline experiments

Continuing work

06/19/2018 Tyler Rehak | New Perspectives 2018 13