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Laterally separated muons from cosmic ray air showers measured with the IceCube neutrino observatory / vorgelegt von Dennis Soldin. Wuppertal, Juni 2017
Inhalt
Abstract
Contents
1 Introduction
2 Cosmic Ray Air Showers
2.1 Cosmic Rays
2.1.1 The Sources of Cosmic Rays
2.1.2 Acceleration Mechanisms
2.1.3 Cosmic Ray Spectrum
2.1.4 Mass Composition
2.2 Extensive Air Showers
2.2.1 Atmosphere
2.2.2 Cascade Equations
2.3 Atmospheric Leptons
2.4 Laterally Separated Muons
3 Detection Principles
3.1 Muon Propagation in Matter
3.1.1 Ionization
3.1.2 Radiative Energy Losses
3.1.3 Multiple Scattering
3.1.4 Cherenkov Radiation
3.2 Air Shower Surface Arrays
3.3 Large-Volume Cherenkov Telescopes
4 The IceCube Neutrino Observatory
4.1 The IceCube In-Ice Array
4.1.1 Ice Properties
4.1.2 Digital Optical Modules
4.1.3 Data Acquisition
4.1.4 Detector Calibration
4.1.5 Triggering and Data Filtering
4.2 Surface Detector IceTop
5 Simulation
5.1 CORSIKA
5.2 Hadronic Interaction Models
5.3 Primary Weighting
5.4 LS Muon Simulations
5.4.1 General Concept
5.4.2 Production Channels
5.4.3 Transverse Momentum Distributions
5.4.4 Hadron Energy Spectra
5.4.5 LS Muon Flux Calculation
5.5 Monte Carlo Distributions
5.6 Neutrino Simulations
5.7 In-Ice Propagation and Detector Response
6 Data Selection and Reconstructions
6.1 Pre-Filtering
6.2 Basic Event Reconstructions
6.3 Double-Track Reconstruction
6.4 Event Selection
6.5 Event Rates
6.6 Track Reconstruction Accuracy
6.7 Primary Energy Estimator
6.8 Transverse Momentum Estimator
6.9 Effective Areas
7 Results
7.1 Primary Energy Spectrum
7.2 Lateral Separation Distribution
7.3 Zenith Angle Distribution and Interaction Height
7.4 Transverse Momentum
7.5 Cosmic Ray Mass Composition
7.6 Seasonal Variations
7.7 Systematic Uncertainties
7.7.1 Lateral Separation
7.7.2 Zenith Angle
7.7.3 Composition Measurement
8 Exotic Double-Tracks from Cosmic Ray Air Showers
8.1 (Minimal) Supersymmetric Models
8.1.1 R-Parity and (N)LSP
8.1.2 Supersymmetry Breaking
8.1.3 Constrained MSSM Benchmark Models
8.2 SUSY Flux Estimates
8.3 Discussion
9 Summary and Discussion
Acknowledgments
A Supplements
A.1 Cosmic Ray Flux Parametrizations
A.2 Atmospheric Model Parametrizations
A.3 Random Number Generation
A.3.1 General Concept
A.3.2 Further Particle Generations
A.3.3 Transverse Momentum
A.3.4 Path Lengths
A.4 Pearson Correlation Coefficient
A.5 Feynman Diagrams
A.6 Seasonal Variations
B Simulation Inputs
B.1 Spectral Indices
B.2 Energy Spectra
B.3 Generation Probabilities
B.4 Cross Sections
B.5 Correlations
C Additional Distributions
C.1 Lateral Separation
C.2 Zenith Angle
C.3 Total Charge
C.4 Opening Angle
C.5 Time Difference
C.6 Reduced Log-Likelihood
C.7 Transverse Momentum
C.8 Primary Energy
C.9 LS Muon Energy
C.10 Atmospheric Heights
C.11 Reconstruction Accuracies
C.12 Effective Areas
Abbreviations and Acronyms
Bibliography
List of Figures
List of Tables
Index