Hadronic showers / missing energy in protoDUNE Pawel Guzowski - - PowerPoint PPT Presentation
Hadronic showers / missing energy in protoDUNE Pawel Guzowski - - PowerPoint PPT Presentation
Hadronic showers / missing energy in protoDUNE Pawel Guzowski Outline Particle gun MC of pions and protons Studying the MC true energy deposited in protodune Quantifying energy associated to primary, and to neutral secondaries
Outline
- Particle gun MC of pions and protons
- Studying the MC true energy deposited in
protodune
- Quantifying energy associated to primary,
and to neutral secondaries (photons, neutrons)
- Examining how much of the true energy ends
up as a reconstructed hit, and reconstructed clusters by 4 reconstruction modules
– lineclusterdc, linecluster, pandoradc, pandora
31 Oct 2016 2 Pawel Guzowski
larsoft workflow
- Using dunetpc v05_13_00
– protodune_v2 geometry
- protoDUNE_gensingle.fcl
– Pion or proton, 0.1 – 3.0 GeV – x: 118.106 cm, y: 395.649 cm, z: 0 cm
- protoDUNE_g4single.fcl
- protoDUNE_detsim_single.fcl
– Optical simulation is off, to save time
- protoDUNE_reco.fcl
- No cosmics / multiparticle events
31 Oct 2016 Pawel Guzowski 3
Analysis
- For now, only looking at the true energy
deposits
- Associating each energy deposit to
– Primary – Neutrons – and subsequent daughters – Photons – and subsequent daughters
- Calculating the fraction of energy deposited
into those three categories
- Calculating how much of this true energy
ends up in a reconstructed hit
31 Oct 2016 Pawel Guzowski 4
1.2 GeV pion
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99% of energy associated to primary
photon-associated deposits primary-associated deposits
p i
- n
positron
Points are true G4 energy deposits
1.2 GeV pion
31 Oct 2016 Pawel Guzowski 6
74% of energy associated to photons
Neutron-associated deposits
pi-zero
1.2 GeV pion
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73% of energy associated to neutrons
MC True particles
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Soft neutrons scattering around everywhere
Green lines = photons
3.0 GeV proton
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Hard neutron
PIONS
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Pion energy deposit
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Total Primary Neutrons Photons Line = mean Area = RMS
Fractional components
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Primary Neutrons Photons
Reconstructed hits
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Total Primary Neutrons Photons Energy ending up in a recob::Hit
Reconstructed fraction
31 Oct 2016 Pawel Guzowski 14
Total Primary Neutrons Photons ~100% ~85% ~80% ~60%
lineclusterdc Clusters
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Total Primary Neutrons Photons
linecluster Clusters
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~90% ~70% ~55% ~30%
pandoradc Clusters
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Total Primary Neutrons Photons
pandora Clusters
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~90% ~60% ~50% ~20%
PROTONS
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Proton energy deposit
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Total Primary Neutrons Photons
Fractional components
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Primary Neutrons Photons
Reconstructed hits
31 Oct 2016 Pawel Guzowski 22
Total Primary Neutrons Photons Energy ending up in a recob::Hit
Reconstructed fraction
31 Oct 2016 Pawel Guzowski 23
Total Primary Neutrons Photons ~100% ~85% ~70% ~65%
lineclusterdc Clusters
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Total Primary Neutrons Photons
(statistical fluctuation,
- ne entry)
linecluster Clusters
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~90% ~70% ~40% ~30%
pandoradc Clusters
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Total Primary Neutrons Photons
pandora Clusters
31 Oct 2016 Pawel Guzowski 27
~90% ~60% ~30% ~20%
Summary
- ~100% of primary energy deposit is
reconstructed in hits
- ~40% of neutron energy is lost
- ~30% of photon energy is lost
- Even more energy is unclustered
- Pandora doing worse than linecluster
- No difference between ‘dc’ and non-‘dc’
31 Oct 2016 Pawel Guzowski 28
BACKUPS
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Total E deposit for 1.0 GeV pion
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Mean = 0.8 RMS = 0.1