Near Detector CDR
Alan Bross LBNC Meeting, CERN December 8th, 2018
Near Detector CDR Alan Bross LBNC Meeting, CERN December 8 th , - - PowerPoint PPT Presentation
Near Detector CDR Alan Bross LBNC Meeting, CERN December 8 th , 2018 First, a bit of background & Motivation Main Near Detector Recommendations (EB) The recommended concept is a near detector suite consisting of a LArTPC (not in a
Near Detector CDR
Alan Bross LBNC Meeting, CERN December 8th, 2018
Main Near Detector Recommendations (EB)
a LArTPC (not in a magnetic field), a Multi-Purpose Detector (MPD) consisting of a HPgTPC, an ECAL and 3D Scintillator Tracker (3DST) in a magnet.
measurements at one or more off-axis positions should go forward (DUNE-PRISM). Study option of moving MPD also
the hook height must be at least 13m, measured from the floor. The minimum lateral dimension of hall needs further study, and will ultimately be settled in EFIG.
investigated.
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The significance with which CP violation, defined as δCP not equal to zero or p, as a function of exposure in kt-MW-years, for equal running in FHC and RHC mode. True normal ordering is assumed. The width of the band corresponds to the difference in sensitivity between ne signal normalization uncertainty
uncertainty on the nµ disappearance mode.
Primary purpose
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n flux systematics Limited data on xsec on Ar Detector systematics
Also extensive program for beyond nSM physics
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See: POND2
Physics Opportunities in the Near DUNE Detector Hall https://indico.fnal.gov/event/18430/overview
Long-Baseline Physics Analysis for the TDR
parameters
c2 with the other samples is minimized
min
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Dan Cherdack
1 2 3 4 5 6 7 8 9 10
Energy (GeV)
15
10
16
10
17
10
POT at ND
20
10 × /GeV/1.1
2
flux/m ν
µ
ν
µ
ν
e
ν
e
ν
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FHC, Events/ton_Ar-year Optimized CPV tune
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2X improvement
LBL Physics Study: ND Geometry
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spectrometer
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Following EB recommendations
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Prong I
cross section on Ar in many exclusive channels
Prong 2
different fluxes Prong 3
sense, the first true LArTPC
TPCs
and better pointing resolution
high voltage, less sensitive to impurities
effective use of scintillation light
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evts/yr) n-Ar interactions, with sufficient resolution for many exclusive channels
n+e elastic scattering (1%)
good p0 reconstruction ability
Strengths
Bern, first operated 2016 (arXiv:1801.08884).
development of LArPixV1 ASIC (arXiv:1808.02969).
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4 modules. Initial tests at Bern, fully instrumented then brought to Fermilab (NuMI) in 2020
provide 1t fiducial target mass
current long shutdown (& engineering)
performance ECAL system, such as concepts developed by the CALICE collaboration
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ALICE being lowered into Hall Magnet concept
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HPgTPC in pressure vessel & LAr upstream
low-energy µ+/ µ- over 4p phase space
charged hadrons
excellent PID
from LAr interactions
component also
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Strengths
reconstruction framework
recon., trk finding, etc
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MPD/HPgTPC
section measurements on scintillator (K2K, MiniBooNE, SciBooNEne, MINERvA, T2K, NOVA)
electron neutrino component
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active, Fine grained, Neutron tagging
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Strengths
SuperFGD Prototype
Use linear combinations to disentangle flux and x-section effects using different fluxes.
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Narrow fluxes at
positions, can provide understanding of Erec→ Etrue mis-modelling. Cross-section parameters in a fake model fitted to
much from nominal values, as intended.
~30m
Fake Data Analysis: IMPACT ON OSC. ANALYSIS
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Eproton is lost
axis near ➛ far detectors analysis, but significant biases are seen in the estimation of oscillation parameters.
near detector positions identify the Etrue ➛ Erec mis-modelling.
flux using linear combinations of flux predictions at different off axis positions.
Nominal Fake DUNE-PRISM 20m off-axis
fluxes, we can construct a Gaussian En spectrum
measure Erec for a given, mono-energetic (10% width) Etrue
truncated, the lower- energy Gaussian fits begin to degrade
assumes Etrue -> Erec can
at least a marginal Gaussian fit can be performed
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Reference ND Detector Cavern Concept: 100ft x 56ft Cavern with 75ft x 50ft Detector Hall
Near Detector Hall: June 2018 Update
June 2018 ND Collaboration Proposal: 165ft x 61ft Cavern with 140ft x 56ft Detector Hall
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Primary access shaft: Reference design 22’ ∅ baseline Need 38’
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and Fermilab management understands the benefits of the larger cavern and access shaft for the DUNE physics program
costs can be saved while keeping the larger hall footprint and larger access shaft
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measurements
model tuning
(beyond nSM)
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tagger
Timeline: ND Executive Summary for Physics TDR: March 2019 CDR: December 2019 TDR: 2nd half of 2020
Detector Design Group (NDDG)
next year & then delivering the CDR.
Weber (Oxford/RAL) and AB.
serve as editors for the CDR and will continue to advise on the physics requirements and work on the performance evaluation
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NDDG Organization
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Conveners Bross, Tanaka, Weber LAr Sinclair Multi- Purpose Detector
Bross/Tanaka LBL Physics Analysis Marshall
HPgTPC
Raaf
3DST
Guang/SgalabernaMagnet Italy/FNAL Muon System
India
Reporting Coordination - Physics Configuration development Sub-components ArgonCube
Ereditato Cryo
Min Jeong Kim
FE Electronics/DAQ Dwyer/Kreslo HPgTPC Junk
CDR Editors Kordosky, Manly LAr
TBD
ECAL
Simon/Italy
Mechanical
Flight
Electrical ES&H DUNE- PRISM Wilking LBNF NSCF
Hamernik
Engineering Integration Feyzi
Dune Near Detector Design Group (NDDG) Spokespersons
Cryostat Schwartz
Cryo-Infrastructure Cipriano/Zukerbrot/ KresloSoftware Integration TBD
DUNE-PRISM
TBD
BSM Physics Martin- Albo
3DST
Guang/SgalabernaFE/DAQ Electronics
n Interaction Physics
primary task is to deliver a CDR for the near detectors & the facility
the bases of the input to the CDR, to a large extent
multiple target nuclei, off-axis measurements) detector systems
statistics in all channels, including neutrino-electron elastic scattering.
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And many thanks to my colleagues for allowing me to steal their slides: Alfons Weber, Chris Marshall, James Sinclair, Dan Dwyer, Clark McGrew, Tanaz Mohayai, Michael Wilking, Chris Vilela, Tom Junk, Tom Hamernik, Bob Flight
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and assume the various subgroups will continue with their current meeting schedules
18th
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High energy tune
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experiment/facility can study tau neutrino appearance in a neutrino beam
can be studied with this beam at the near site?
~10X increase in nt evts in Far detector
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between adjacent pads to improve angular resolution for forward- going tracks
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‐power cryogenic amplification, digitization, and readout:
‐channel readout:
design targets:
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coils
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Largest field non-uniformity: ~ 12%
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spaces for pedestals for supporting HPgTPC
parts contains about 17 double pan cake coils (Total number of pan cakes will be 52)
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light readout requirements
and timing resolution
recoiling proton to any activity above 0.1 MeV from other interactions?
~30 cm needed
ArCLight?
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ECAL:
to lack of interactions in gas
Ar interactions
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HPgTPC
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2 mm Cu absorber, 80 layers HPgTPC ECAL
neutrons are actually charged particles interacting in the magnet and producing neutrons
be forward
likely to occur in outer ECAL, since they are coming mostly from interactions in the magnet
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measurements on Ar (Liquid and gas)
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reconstruction assumptions, DUNE LAr ND can select over 3,000 n+e events per year at initial intensity
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~56’ 75’
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Beam ➛
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Larger Shaft – Size
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ranging from 32ft to 43ft ID
provides a minimum of 0.5m clearance around HPgTPC and preserves lift/utility segment
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Can even somewhat resolve the peak below the 3rd
maximum for all values
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δCP Sensitivity vs Min-Eν / Off-Axis Reach
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increase in far detector exposure of:
IS AN ON-AXIS MPT SENSITIVE TO THIS TYPE OF MISMODELLING?
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