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Niechciol, Marcus: A new window to the universe? : searching for ultra-high-energy photons at the Pierre Auger ObservatoryA Ein neues Fenster zum Universum? : die Suche nach ultrahochenergetischen Photonen am Pierre-Auger-Observatorium. 2015
Inhalt
Abstract
Contents
1 Introduction
2 Cosmic Rays
2.1. Early History of Cosmic-Ray Physics
2.2. Primary Cosmic Rays
2.2.1. Energy Spectrum
2.2.2. Composition
2.2.3. Anisotropy in Arrival Directions
2.2.4. Origin of Primary Cosmic Rays
2.3. Extensive Air Showers
2.3.1. Simplified Heitler Model
2.3.2. Development in the Atmosphere
3 Ultra-High-Energy Photons
3.1. Origin of UHE Photons
3.2. Propagation through the Universe
3.3. Extensive Air Showers Induced by Photons
3.3.1. Differences in the Longitudinal Development
3.3.2. Differences in the Lateral Distributions
3.4. Current Upper Limits on the Incoming Photon Flux
3.4.1. Limits on the Diffuse Photon Flux
3.4.2. Search for Point Sources of UHE Photons
4 The Pierre Auger Observatory
4.1. The Surface Detector
4.2. The Fluorescence Detector
4.2.1. Data Acquisition and Trigger Systems
4.2.2. Calibration of the FD
4.2.3. Atmospheric Monitoring
4.3. Enhancements of the Observatory
4.3.1. Auger Muons and Infill for the Ground Array (AMIGA)
4.3.2. High Elevation Auger Telescopes (HEAT)
4.3.3. Auger Engineering Radio Array (AERA)
4.4. Plans to Upgrade the Observatory beyond 2015
4.5. Reconstruction of Air Shower Events
4.5.1. Reconstruction from Hybrid Data
4.5.2. Reconstruction from SD Data
5 Simulations and Data
5.1. Simulation Samples Used in the Analysis
5.1.1. Air Shower Simulations with CORSIKA
5.1.2. Detector Simulations with the Auger Offline Software Framework
5.2. Data Sample Used in the Analysis
5.3. Event Selection
5.3.1. Description of the Selection Criteria
5.3.2. Application to the Simulation Samples
5.3.3. Application to the Data Sample
6 Simulation Study of Observables for the Search for UHE Photons
6.1. Xmax as a Discriminating Observable
6.2. A new SD-related Observable: Fgamma
6.2.1. Definition of Fgamma
6.2.2. Determining a Parameterization of the LDF Shape Parameter b for Photons in the EeV Range
6.2.3. Description of the Photon-Optimized Fit
6.2.4. Performance of Fgamma
6.2.5. Comparison with other SD-related Observables
6.2.6. Introducing additional selection criteria based on Fgamma
6.3. Combining Fgamma and Xmax in a Multivariate Analysis
6.3.1. Applying the Fisher Discriminant Analysis
6.3.2. Parameterization of the Fisher Coefficients as a Function of Energy
6.3.3. Defining the Photon Candidate Cut
6.4. Further Studies Using Simulations
6.4.1. Behavior Above 10 EeV
6.4.2. Application to Air Shower Events Initiated by Nuclei
6.4.3. Robustness Against Exchanging the Hadronic Interaction Model
7 A Search for Photons in the EeV Range Using Hybrid Data
7.1. Application of the Analysis to Hybrid Data
7.2. Study of the Photon Candidate Event
7.2.1. FD Part of the Event
7.2.2. SD Part of the Event
7.2.3. Study of the Arrival Direction
7.2.4. Possible Primary Particle Type
7.3. Determining Upper Limits in the EeV Range
7.3.1. Upper Limits on the Photon Fraction
7.3.2. Upper Limits on the Integral Photon Flux
7.3.3. Discussion of Systematic Effects
8 Summary and Outlook
Appendices
A. Input Files for the Simulations
A.1. CORSIKA Input File
A.2. Offline Input File
B. Detailed Statistics for the Event Selection
C. Additional Plots for Chapter 6
D. Acceptance Correction
Bibliography
List of Acronyms and Abbreviations