Search for a Low Energy Excess in MicroBooNE
54th Rencontres de Moriond EW - Young Scientist Forum March 20th, 2019
Nicolò Foppiani - Harvard University On behalf of the MicroBooNE collaboration
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Search for a Low Energy Excess in MicroBooNE Nicol Foppiani - - - PowerPoint PPT Presentation
Search for a Low Energy Excess in MicroBooNE Nicol Foppiani - Harvard University On behalf of the MicroBooNE collaboration 54th Rencontres de Moriond EW - Young Scientist Forum March 20th, 2019 1 Neutrino anomalies and the L ow E nergy E
54th Rencontres de Moriond EW - Young Scientist Forum March 20th, 2019
Nicolò Foppiani - Harvard University On behalf of the MicroBooNE collaboration
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Anomalies in Short Baseline Neutrino Oscillations ➔ Might hide sterile neutrinos -> new physics BSM
○ Could not distinguish electrons from photons
○ Is there an excess? ○ Origin? Electron-like or photon-like?
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Anomalies in Short Baseline Neutrino Oscillations ➔ Might hide sterile neutrinos -> new physics BSM
○ Could not distinguish electrons from photons
○ Is there an excess? ○ Origin? Electron-like or photon-like? Precision measurements of Cross Sections in liquid argon ➔ Improve understanding of nuclear physics in neutrino interactions ➔ Preparation for DUNE
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Two beamlines:
○ For the main physics goals of MicroBooNE ○ The heart of the SBN programme, with SBND and Icarus
○ Complementary physics and cross checks
NuMI BNB Icarus SBND MicroBooNE
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Color shows deposited charge
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Z-axis [m] (beam direction) x-axis [time] (drift axis) Color shows deposited charge
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Z-axis [m] (beam direction) x-axis [time] (drift axis) Tracks: protons, pions, muons Color shows deposited charge
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Color shows deposited charge Z-axis [m] (beam direction) x-axis [time] (drift axis) Electromagnetic shower: electron-like, attached to the main vertex
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Electromagnetic showers detached from the vertex, photon conversion length ~26 cm
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Electron-like search:
start of the shower
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Electron-like search:
start of the shower Photon-like search:
start of the shower
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Electron-like search:
start of the shower Photon-like search:
start of the shower
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Some data ready to develop the analyses:
Electron-like search:
start of the shower Photon-like search:
start of the shower
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○ hardest to distinguish from single photon production
○ Easier because additional tracks determine vertex ○ It is the channel in which the LEE has been
○ Very complex events ○ Typically higher energies
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○ hardest to distinguish from single photon production
○ Easier because additional tracks determine vertex ○ It is the channel in which the LEE has been
○ Very complex events ○ Typically higher energies
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Light and charge: remove cosmic rays Topological and geometrical requirements Calorimetry: particle ID and energy measurement
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Cross check: two sidebands on 3.5% of the total BNB data Light and charge: remove cosmic rays Topological and geometrical requirements Calorimetry: particle ID and energy measurement NC𝝆0 enriched (photon enriched) sideband 𝛏𝝂CC enriched sideband
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Cross check the BNB analysis using NuMI
in the full BNB dataset
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Cross check the BNB analysis using NuMI
in the full BNB dataset
cos(𝜾) wrt NuMI beam direction:
confidence we can tune and cross check the LEE analysis
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○ Collected a huge amount of data ○ Solid strategy and demonstration of the LEE analyses
○ CC𝛏𝝂 𝛒0: MICROBOONE-NOTE-1032-PUB ○ CC𝛏𝝂 inclusive: MICROBOONE-NOTE-1045-PUB
○ Electron-like search BNB: MICROBOONE-NOTE-1038-PUB ○ Electron-like search NuMI: MICROBOONE-NOTE-1054-PUB ○ Photon-like search BNB: MICROBOONE-NOTE-1041-PUB
Stay tuned: new results coming soon!
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Two signals:
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Production of a lepton: clear exp signature. Distinguish different flavours For the LEE search -> need to distinguish the two flavours, only Charged Current (CC) are of interest! Typical neutrino energy ~ 1 GeV ➔ In this energy range interactions with the nuclei are predominant Neutral current interactions Charged current interactions Only nucleus recoil, hard to detect. No information about the flavour
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