Highly Granular ECAL
Studies in a HP-TPC Context
Lorenz Emberger, Frank Simon
Max-Planck-Institute for Physics
DUNE Near Detector Workshop, Fermilab, March 2018
Highly Granular ECAL Studies in a HP-TPC Context Lorenz Emberger, - - PowerPoint PPT Presentation
Highly Granular ECAL Studies in a HP-TPC Context Lorenz Emberger, Frank Simon Max-Planck-Institute for Physics DUNE Near Detector Workshop, Fermilab, March 2018 Outline A case for high granularity in the ECAL Straw man ECAL concept for a
Lorenz Emberger, Frank Simon
Max-Planck-Institute for Physics
DUNE Near Detector Workshop, Fermilab, March 2018
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
2
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
associated π0s to neutrino interaction vertices in the tracking detector
3
interesting in combination with a HP TPC, since the conversion probability in the TPC gas is too low to enable efficient π0 reconstruction
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
is “premium real estate” ➫ Cannot accommodate full calorimeter (depth ~ 80 cm) inside the vessel ➫ Split the calorimeter into two sections, separated by the pressure vessel
4
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
5
30 layers ~ 250 mm 50 layers ~ 400 mm 14 - 20 mm inner ECAL
pressure vessel
N.B. Not yet fully optimised - in particular outer segment!
~ 6 X0 ~ 10 X0
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
6
Pb absorber plastic scintillator signal / power routing SiPM 1 mm 5 mm 1 mm 20 - 30 mm
assume a granularity of 20 x 20 - 30 x 30 mm2
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
realistic)
MIP signal as σ)
7
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
applied); no clustering
to determine first estimate of shower axis
using PCA as input to further improve estimate
8
Resolution = v u u t A p E[MeV ] !2 + ✓ B E[MeV ] ◆2 + C2
Fits (energy & angular resolution): N.B.: to get stochastic term in units of 1/Sqrt(GeV) divide A by 32
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
9
Mean 0.2 ± 208.2 Sigma 0.21 ± 14.58
50 100 150 200 250 300 350 400
Visible Energy[MeV]
100 200 300 400 500 600 700 800 900
Entries
Eγ 650 MeV
200 400 600 800 1000 1200 1400 1600
Energy[MeV]
0.04 0.06 0.08 0.1 0.12 0.14 0.16 0.18 0.2 0.22 mean
/E σ
A 0.01451 ± 1.527 B 0.9716 ± 0.2364 C 0.001736 ± 0.03679
Note: Over-optimistic - not all detector effects simulated!
~ 6% @ 1GeV
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
9
Mean 0.2 ± 208.2 Sigma 0.21 ± 14.58
50 100 150 200 250 300 350 400
Visible Energy[MeV]
100 200 300 400 500 600 700 800 900
Entries
Eγ 650 MeV
200 400 600 800 1000 1200 1400 1600
Energy[MeV]
0.04 0.06 0.08 0.1 0.12 0.14 0.16 0.18 0.2 0.22 mean
/E σ
A 0.01451 ± 1.527 B 0.9716 ± 0.2364 C 0.001736 ± 0.03679
0.1 0.2 0.3 0.4
Angle[rad]
50 100 150 200 250
Entries
68% ≙ 0.089rad
Eγ 450 MeV
200 400 600 800 1000 1200 1400 1600 Energy[MeV]
0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 AngularResolution[rad]
A 0.02459 ± 1.694 B 0.6835 ± 18.31 C 0.07023 ± 05 − 1.488e
Note: Over-optimistic - not all detector effects simulated!
~ 6% @ 1GeV
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
10
Moliere radius (size of shower)
channel count First goal: Understand scaling behavior of detector performance for configuration changes
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
11
First goal: Understand scaling behavior of detector performance for configuration changes
Beam axis TPC Volume Inner ECal Outer ECal Pressure Vessel ~25cm ~40cm vµ 𝜹1 𝜹2
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
12 200 400 600 800 1000 1200 1400 Energy[MeV] 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 Angular Resolution[rad]
A: 1.649 B: 18.56 C: 0.000 NO Pressure Vessel A: 1.694 B: 18.31 C: 0.000 14mm Titan Vessel A: 1.750 B: 17.43 C: 0.000 20mm Steel Vessel
200 400 600 800 1000 1200 1400 Energy[MeV] 0.04 0.06 0.08 0.1 0.12 0.14 0.16 0.18 0.2 0.22
mean
/E σ
A: 1.405 B: 1.109 C: 0.017 NO Pressure Vessel A: 1.526 B: 0.236 C: 0.036 14mm Titan Vessel A: 1.503 B: 0.081 C: 0.079 20mm Steel Vessel
Angular Resolution Energy Resolution
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
13
Angular Resolution Energy Resolution
200 400 600 800 1000 1200 1400 1600 Energy[MeV] 0.9 0.95 1 1.05 1.1 1.15 1.2 relative AngularResolution
NO Pressure Vessel 14mm Titan Vessel 20mm Steel Vessel
200 400 600 800 1000 1200 1400 1600 Energy[MeV] 1 1.2 1.4 1.6 1.8 2 2.2 relative EnergyResolution
NO Pressure Vessel 14mm Titan Vessel 20mm Steel Vessel
➫ Very mild impact on angular resolution: few % ➫ Substantial impact on energy resolution - thick steel vessel up to x2 deterioration, with titanium only ~ 30% loss compared to no vessel In the following: Always assume titanium vessel
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
14 200 400 600 800 1000 1200 1400 Energy[MeV] 0.05 0.1 0.15 0.2 0.25 0.3 0.35
mean
/E σ
A: 1.526 B: 0.236 C: 0.036 1mm Lead Absorber A: 2.392 B: 4.112 C: 0.015 2mm Lead Absorber A: 1.178 B: 0.253 C: 0.080 1mm Copper Absorber A: 1.630 B: 3.289 C: 0.038 2mm Copper Absorber
200 400 600 800 1000 1200 1400 1600 Energy[MeV] 0.8 1 1.2 1.4 1.6 1.8 2 relative EnergyResolution
1mm Lead Absorber 2mm Lead Absorber 1mm Copper Absorber 2mm Copper Absorber
performance loss when using 2 mm Cu substantial energy leakage for 1 mm Cu: not enough X0 in calorimeter! smaller sampling fraction for 2 mm Pb: larger stochastic term
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
15 200 400 600 800 1000 1200 1400 Energy[MeV] 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 0.5 Angular Resolution[rad]
A: 1.694 B: 18.31 C: 0.000 1mm Lead Absorber A: 2.127 B: 19.46 C: 0.000 2mm Lead Absorber A: 1.395 B: 15.81 C: 0.000 1mm Copper Absorber A: 1.393 B: 16.32 C: 0.000 2mm Copper Absorber
200 400 600 800 1000 1200 1400 1600 Energy[MeV] 0.6 0.7 0.8 0.9 1 1.1 1.2 1.3 1.4 1.5 1.6 relative AngularResolution
1mm Lead Absorber 2mm Lead Absorber 1mm Copper Absorber 2mm Copper Absorber
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
tiles in the inner ECAL for 1 mm Pb absorber
16 200 400 600 800 1000 1200 1400 Energy[MeV] 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 Angular Resolution[rad]
A: 1.614 B: 16.57 C: 0.000 5mm Inner Tiles A: 1.623 B: 16.99 C: 0.000 10mm Inner Tiles A: 1.694 B: 18.31 C: 0.000 20mm Inner Tiles A: 1.798 B: 19.67 C: 0.000 30mm Inner Tiles
200 400 600 800 1000 1200 1400 1600 Energy[MeV] 0.85 0.9 0.95 1 1.05 1.1 1.15 1.2 relative AngularResolution
Inner Tiles: 5mm Inner Tiles: 10mm Inner Tiles: 20mm Inner Tiles: 30mm
tiles at 10 x 10 mm2
performance for 30 x 30 mm2 is slightly better than for Pb 20 x 20 mm2: Wider showers
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
17
Angular Resolution Energy Resolution Titanium Vessel Default Default Lead Absorber Default Default No Vessel Steel Vessel Copper Absorber Higher granularity in inner calorimeter High granularity in
Negative Positive Arrow slope: strength of effect Neutral
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
detector - will need somewhat more sophisticated simulations for a full study
algorithm for stable estimate of direction below ~ 70 MeV: For now a cut-off is applied
18
Assignment of energy to photons using MC truth information
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
coordinate perpendicular to ECAL front face largest (e.g., reconstruction of distance from ECAL), better in other two coordinates
with 20 x 20 mm2 granularity
19
InvariantMassH2
Entries 2627 Mean 1.428 ± 172.4 RMS 1.01 ± 73.17
InvariantMass[MeV] 100 200 300 400 500 600 700 800 900 1000 Entries 10 20 30 40 50 60 70 80 90
InvariantMassH2
Entries 2627 Mean 1.428 ± 172.4 RMS 1.01 ± 73.17
MC Direction, reconstructed Energy
InvariantMassH3
Entries 2627 Mean 1.076 ± 153.5 RMS 0.7608 ± 55.15
InvariantMass[MeV] 100 200 300 400 500 600 700 800 900 1000 Entries 10 20 30 40 50
InvariantMassH3
Entries 2627 Mean 1.076 ± 153.5 RMS 0.7608 ± 55.15
reconstructed Direction, reconstructed Energy
450 MeV π0, 30 cm away from ECAL
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
20
➫ Need to fully understand granularity requirements to optimise detector layout ➫ Develop solutions to achieve high effective granularity with reduced channel count - may be a viable options in some areas of the detector
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
showers)
21
measure relative distance of two photons from calorimeter to ~ 30 cm or better
➫ Could be used to improve assignment of low-energy photons with very poor
pointing accuracy to interactions and π0 candidates Lets speculate a bit:
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
capability to locate π0s with few cm accuracy
Titanium over stainless steel for energies of 1 GeV and higher
than 20 x 20 mm2 with Pb absorbers
22
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
23
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
24
TPC Volume Beam axis vµ Inner ECal Vessel Increase granularity in first few X0 𝜹1 𝜹2 Higher Granularity: 10mm x 10mm Lower Granularity: 20mm x 20mm, 30mm x 30mm
200 400 600 800 1000 1200 1400 1600 Energy[MeV] 0.85 0.9 0.95 1 1.05 1.1 1.15 1.2 relative AngularResolution
InnerTiles: 20mm InnerTiles: 10mmLayer0-9/20mmLayer10-29 InnerTiles: 10mmLayer0-9/30mmLayer10-29
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
24
TPC Volume Beam axis vµ Inner ECal Vessel Increase granularity in first few X0 𝜹1 𝜹2 Higher Granularity: 10mm x 10mm Lower Granularity: 20mm x 20mm, 30mm x 30mm
200 400 600 800 1000 1200 1400 1600 Energy[MeV] 0.85 0.9 0.95 1 1.05 1.1 1.15 1.2 relative AngularResolution
InnerTiles: 20mm InnerTiles: 10mmLayer0-9/20mmLayer10-29 InnerTiles: 10mmLayer0-9/30mmLayer10-29
200 400 600 800 1000 1200 1400 1600 Energy[MeV] 0.85 0.9 0.95 1 1.05 1.1 1.15 1.2 relative AngularResolution
Inner Tiles: 5mm Inner Tiles: 10mm Inner Tiles: 20mm Inner Tiles: 30mm
compare: uniform granularity
Frank Simon (fsimon@mpp.mpg.de) ND ECAL Update DUNE ND Workshop, Fermilab, March 2018
interactions
25
produced essentially at rest of from resonance decays with 200 - 300 MeV
➫ Need to reconstruct
few 100 MeV γ NB: Also multi-GeV π0s are relevant: Those can fake oscillation signals in the far detector
plots curtesy of Chris Marshall