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Search for exotic double tracks with the IceCube neutrino telescope / Sandro Kopper. Wuppertal, April 2017
Inhalt
Dedication
Abstract
Acknowledgements
Contents
List of Figures
Acronyms
Theory and Experiment
1 Cosmic Rays
1.1 Sources of Cosmic Rays
1.2 Acceleration Mechanisms
1.3 Neutrino Production in Gamma Ray Bursts
2 Air Showers
3 Relativistic Charged Particles in Matter
3.1 Cherenkov Radiation
3.2 Energy Losses in Matter
3.2.1 The Muon Case
3.2.2 Very Heavy Charged Particles
4 Neutrino Astronomy
4.1 Neutrino Telescopes
4.2 Detector Signatures of Standard Model -Interactions
5 The IceCube Experiment
5.1 The IceCube Detector
5.1.1 The Surface Detector
5.1.2 The IceCube Array
5.2 Ice properties at the IceCube site
5.3 IceCube Hardware and Software
5.3.1 Digital Optical Modules
5.3.2 Data Aquisition Electronics
5.3.3 DOM Calibrations
5.3.4 Surface Hardware and Software
5.4 Data Filtering
5.4.1 Basic Event Reconstructions
5.4.2 Further Event Reconstructions
6 Physics Beyond the Standard Modell
6.1 Supersymmetry
6.1.1 Broken Supersymmetry and the MSSM
6.1.2 SUSY Searches and Detector Phenomenology
6.2 Models with extra Dimensions
6.2.1 Large Extra Dimensions
6.2.2 Warped Extra Dimensions
6.2.3 Universal Extra Dimensions
Simulation and Analysis
7 Neutrino Induced Double Tracks
7.1 Air Shower Muon and Neutrino Simulation
7.2 Double Track Simulation
7.2.1 Simulation of Exotic Double Tracks
7.2.2 Simplifications
7.2.3 Di-Muon Signal
7.3 Coincident Events
7.4 Photon Propagation and Detector Simulation
8 Double Track Reconstruction and Cut Variables
8.1 Tensor of Inertia Based Reconstruction
8.2 k-Means Based Reconstruction
8.3 Likelihood Reconstructions
8.4 Data Selection Cuts
8.4.1 Muon Filter
8.4.2 Basic Quality Cuts
8.4.3 Coincident Event Cuts
8.4.4 Single Track Cuts
8.4.5 Final Quality Cut
8.4.6 Data / M.C. Mismatch
9 Choice of Cuts
9.1 Data Sets
9.1.1 Simulated Data
9.1.2 Real Data and Burn Sample
9.2 Optimization of Cut Parameters
10 Results
11 Systematic Uncertainties
11.1 Monte Carl Statistics
11.2 Ice Mode and Photon Propagator
11.3 DOM Efficiency
11.4 Background Events
11.4.1 Atmospheric Muons
11.4.2 Neutrino Events
11.4.3 Di-Muon Events
11.5 Signal Modeling
11.6 Inclusion of Systematic Uncertainties
12 Discussion and Future Improvements
Appendix
A Additional Plots
Bibliography
Colophon