Rowan Zaki, for the DUNE collaboration DPF meeting: August 3rd, - - PowerPoint PPT Presentation
Rowan Zaki, for the DUNE collaboration DPF meeting: August 3rd, 2017 Overview Introduction Optimization process Reference vs optimized three horn design Potential staging configurations Future work & Summary DPF
DPF meeting: August 3rd, 2017
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Figure 1: DUNE/LBNF baseline key elements Figure 2: DUNE/ LBNF detailed
Fermilab site
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Figure 3: DUNE CDR reference beamline design
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Figure 4: Optimized three horn design of the LBNF beamline (Horns and target)[C. Crowley]
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Figure 5: Comparison of neutrino flux for the CDR reference design and three horn design Figure 6: Comparison of CP-sensitivity for the CDR reference design and three horn design
2nd and 1st oscillation maxima
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Figure 7: Movement of target within Horn A(C. Crowley) Direction of moving Horn C
Upstream Downstream
Figure 8: Movement of Horn C within LBNF beamline (C. Crowley)
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Figure 9: CP-sensitivity for different positions of Horn C along the beamline Figure 10: 75% CP-sensitivity for different positions of Horn C along the beamline v
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Figure 11: CP-sensitivity for different target positions along the beamline downstream (left) to upstream (right)
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Figure 12: Neutrino flux for potential staging configurations
2nd and 1st
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Figure 13: CP-sensitivity for potential staging configurations
Figure 14: 75% CP-sensitivity for different positions
the beamline
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Fig 15ab: NuMI-style target
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2.2m cylindrical target (16mm diameter) (2.666mm beam sigma)
Fig 16ab: RAL-target (DUNE collaboration)
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Figure 9: Neutrino flux for potential staging configurations
Figure 5: Neutrino flux ratios for different positions of Horn C along the beamline
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Figure 7: Neutrino flux ratios for different target positions along the beamline
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