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Search for low relativistic magnetic monopoles at the IceCube Neutrino Observatory / vorgelegt von M. Sc. Frederik Hermann Lauber. Wuppertal, Juli 2021
Inhalt
Abstract
Zusammenfassung
Contents
List of Figures
List of Tables
Introduction
IceCube Neutrino Observatory
Detector Architecture of IceCube
Antarctic Ice
Digital Optical Modules
IceCube In-Ice Array
IceCube DeepCore Array
Data Acquisition of IceCube
Global Triggers
Waveform Deconvolution
Magnetic Monopoles
Maxwell's Equations
Dirac Magnetic Monopoles
't Hooft-Polyakov Magnetic Monopoles
Magnetic Monopoles in Grand Unified Theories
Rest Mass
Kinetic Energy
Stopping Power
Earth Shielding
Exclusion Limits for Magnetic Monopole Flux
Machine Learning
Feature Space
Sampled Supervised Binary Classification
Bias–Variance Trade-Off
Training Goal: Minimize the Objective Function
Machine Learning Based Estimators
Singular Variate Decision
Decision Tree
Boosted Decision Trees
Regularization Systems and Techniques
Number of Predictors
Sub-sampling the Training Data
Dropout Regularization
Tikhonov Regularization
EXtreme Gradient Boosting
Light Emission of Magnetic Monopoles in Ice
Direct Cherenkov Radiation
Indirect Cherenkov Radiation
Luminescence Light Emissions
Expected Light Yields
Simulation
Digital Optical Module Response
Photomultiplier Tube Response
Main Board Response
Photon Propagation Inside the Ice
Physical Signature to In-Ice Photons
Cosmic Ray Induced Air Showers
Neutrinos
Magnetic Monopoles
Event Selection and Reconstructions
IceCube Event Selection
Level 0: Events at Data Acquisition
Level 1: Filtering at the South Pole
Level 2: MonopoleFilter16 Filter Selection
Analysis Specific Quality Selection Steps
Level 3: MonopoleFilter16 filter, In-Ice Array
Level 4-6: Coincident Particle Rejection
Level 7: Global Linefit Cut
Level 8: Corner Clipper Removal
Level 9: Machine Learning Based Selection
Events Utilized for Training
Input Feature Selection
Boosted Decision Tree Training Configuration
Bootstrap Aggregating
Feldman-Cousins Sensitivity
Model Rejection Factor
Optimized Final Selection Step
Reconstructed Kinematic Attributes
Systematic Shifts of Detector Response
Projected Sensitivity
Results
Remaining Events
Event Origin
Internal Consistency of Remaining Events
Arrival Direction
Magnetic Charge
Rest Mass
Discussion
Low Relativistic Magnetic Monopole Flux Limit
Conclusion and Outlook
Improved LineFit
Earth Shielding for Intermediate Magnetic Charges
Individual Systematic Effects
Input Variables for the Last Analysis Selection Step
Input Feature Importance
Data of Derived Flux Limit
Acronyms
Bibliography