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Constraints to UHE cosmic ray source scenarios with all the major observables of the Pierre Auger Observatory / vorgelegt von Biswajit Sarkar aus Wuppertal. Wuppertal, September 2015
Inhalt
Introduction
Physical Foundation
Cosmic rays
Historical Background
Energy Spectrum
Chemical Composition
Search for an Anisotropy in the Arrival Directions of UHECR
Origin of Cosmic Rays
Source Evolution
Extragalactic Magnetic Fields
Galactic Magnetic Field
Propagation of UHECR
Interactions with the Photon Background
Ultra High Energetic Photon Production and Propagation
Ultra High Energy Neutrino Production and Propagation
Cosmological Effects
The Development of Air Showers
Electromagnetic Cascade
Hadronic Air Showers
Parametrization of the "426830A Xmax "526930B and (Xmax)
The Pierre Auger Observatory
The Surface Detector
The Fluorescence Telescopes
Data from the Pierre Auger Observatory
Energy Spectrum Measured by the Pierre Auger Observatory
Auger Xmax Measurements
Upper Limits for UHE-Photons with the Pierre Auger Observatory
Upper Limits for UHE-Neutrinos with the Pierre Auger Observatory
Search for Anisotropies in the Arrival Directions of UHECRs
CRPropa
General Capabilities of CRPropa
Study of the Pion Production
Combined Fit to the Energy Spectrum and the Xmax Moments
Introduction of General Scenario and Methods
General scenario
Deriving the Observables from Simulation Output
Fit Procedure
Choice of Further Assumptions
Results
Fit to the Energy Spectrum
Standard Scenarios
Influence of Technical Assumptions on the Fit Results
GZK vs. Exhausted Sources
Alternative Source Evolution Scenarios
Magnetic Suppression
Study with Additional Source Populations
Scenario Variable Source Spectral Index
Summary and Conclusion
Secondary Photons and Neutrinos
Study on Photon Flux
Simulation Setup
Parameter Studies
Photon Flux Prediction for Reasonable Scenarios
Constraints on Source Spectra and Maximum Energy
Sensitivity to Local Sources
Implications on GeV Photon Fluxes
Assuming a Photon Component at Source
Study of Neutrino Flux
Simulation Setup
General Parameter Studies
Neutrino Flux Prediction for Reasonable Scenarios
Constraints on Astrophysical Scenarios
Comparison of the Exclusion Power from UHE Photons and Neutrinos
Summary
Arrival Directions of Cosmic Rays
Data
Impact of the Expansion of the Universe
Simulation
Assumption for Simulations
Directional exposure
Reweighting Procedure
Calculation of Correlation Fraction
Results
Summary and Conclusion
Summary and Conclusion
Bibliography