Abstract

The preponderance of matter over antimatter in the early universe, the dynamics of the supernovae that produced the heavy elements necessary for life, and whether protons eventually decay—these mysteries at the forefront of particle physics and astrophysics are key to understanding the early evolution of our universe, its current state, and its eventual fate. The Deep Underground Neutrino Experiment (DUNE) is an international world-class experiment dedicated to addressing these questions as it searches for leptonic charge-parity symmetry violation, stands ready to capture supernova neutrino bursts, and seeks to observe nucleon decay as a signature of a grand unified theory underlying the standard model. The DUNE far detector technical design report (TDR) describes the DUNE physics program and the technical designs of the single- and dual-phase DUNE liquid argon TPC far detector modules. This TDR is intended to justify the technical choices for the far detector that flow down from the high-level physics goals through requirements at all levels of the Project. Volume I contains an executive summary that introduces the DUNE science program, the far detector and the strategy for its modular designs, and the organization and management of the Project. The remainder of Volume I provides more detail on the science program that drives the choice of detector technologies and on the technologies themselves. It also introduces the designs for the DUNE near detector and the DUNE computing model, for which DUNE is planning design reports. Volume II of this TDR describes DUNE's physics program in detail. Volume III describes the technical coordination required for the far detector design, construction, installation, and integration, and its organizational structure. Volume IV describes the single-phase far detector technology. A planned Volume V will describe the dual-phase technology.

Highlights

  • Introduction ProtoDUNESP ran at CERN in the NP04 beamline from September to November of 2018

  • 1.1.1 The Deep Underground Neutrino Experiment (DUNE) science program The preponderance of matter over antimatter in the early universe, the dynamics of the supernova neutrino bursts (SNBs) that produced the heavy elements necessary for life, and whether protons eventually decay — these mysteries at the forefront of particle physics and astrophysics are key to understanding the early evolution of our universe, its current state, and its eventual fate

  • Opportunities in BSM physics that have been considered as elements of the DUNE science program include: Search for active-sterile neutrino mixing: DUNE is sensitive over a broad range of potential sterile neutrino mass splittings by looking for disappearance of charged current (CC) and neutral current (NC) interactions over the long distance separating the near detector (ND) and far detector (FD), as well as over the short baseline of the ND

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Summary

A.33 Energy and angular resolutions for photons in the MPD ECAL

A.34 Oscillation fits to nominal and fake data sets for DUNE-PRISM fake data study 158. Oscillation fits to nominal and fake data sets for DUNE-PRISM fake data study 158. Reconstructed energy distributions for nominal and fake data sets; on- and off-axis 158. Linear combinations of off-axis fluxes giving FD oscillated spectra; range of parameters A.36 Linear combinations of off-axis fluxes giving FD oscillated spectra; range of parameters

SAND event rates
Overview
Chapter 1. Executive summary
The DUNE detectors
Near detector
DUNE project organization and responsibilities
DUNE collaboration organization and management
Milestones for the first two far detector modules
Goals of the DUNE science program
Baryon number violation
Supernova neutrino bursts
Additional Beyond-Standard-Model physics signatures
Summary of assumptions and methods employed
Beam and detector
Deployment scenario
CPV in the neutrino sector and precise oscillation parameter measurements
Galactic supernovae via measurements of neutrino bursts
Results from fits to pinched thermal neutrino energy spectrum
Pointing sensitivity of DUNE
DUNE Simulation
Chapter 3. Single-phase far detector technology
Anode planes
Cathode planes and high voltage
Electronics
Photon detection system
Calibration
Data acquisition
Cryogenics instrumentation and slow controls
Installation
Features of the dual-phase design
Charge readout planes
Readout electronics and chimneys
Overview of the DUNE near detector
Chapter 5. The DUNE near detector
Role of the ND in the DUNE oscillation program
ND hall and construction
Chapter 6. Computing in DUNE
Resources and governance
Scope of the consortium
Resource contributions
Data types and data volumes
Single-phase technology data estimates
Dual-phase technology data estimates
MeV 10 MeV 100 MeV 1 GeV
Beam coincident rates
Simulation
ProtoDUNE-SP data
Commissioning and physics operations
Data volumes
Reconstruction of ProtoDUNE-SP data
Lessons learned
Global project organization
DUNE far detector organization
Facility description
Far detector construction management
Integration engineering
Reviews
Quality assurance
Design
Current experiments
Past experience
Constraining the flux in the ND
Neutrino-electron elastic scattering
The low-ν method
Coherent neutrino-nucleus scattering
Introduction to DUNE-PRISM
LArTPC component in the DUNE ND
Dimensions of the ArgonCube component of the DUNE ND
Multipurpose detector
Size optimization
Track reconstruction and particle identification
Machine learning for low energy protons
ECAL performance
The DUNE-PRISM program
Motivation and introduction
Expected statistics
Beam monitoring
Neutron detection performance
Meeting the near detector requirements
Event rate and flux measurements
Control of systematic errors
Specific collaborative computing projects
LArSoft for event reconstruction
Findings
Evaluations of other important infrastructure
Full Text
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