Modeling of the diffuse galactic neutrino flux / author: Nikita Grimm. Innsbruck, July 2018
Inhalt
[1]Titelblatt
3Acknowledgements
[5]Abstract
[7]Contents
[9]1 Introduction
[11]2 Theory
[15]3 Implementation
[15]3.1 Neutrino Emissivity
[17]3.2 Line of Sight Integration
[18]3.2.1 Formation of the Observational Cone
[20]3.2.2 Integrating over a Subcone
[20]3.2.3 Subcone Interpolation
[21]3.2.4 Choosing the Number of Subcones
[22]3.2.5 Retrieving the Local Gas Density
[27]3.2.6 Alternative Method for Retrieving the Gas Density
[27]3.2.7 The unit of the Neutrino Sky Map
[28]3.3 Evaluating Molecular Hydrogen and Helium
[]4 Results
[33]4.1 Neutrino Emissivity
[33]4.2 The Basic Neutrino Sky
[33]4.2.1 Integration Method Comparison
[38]4.2.2 Artifacts in the Neutrino Sky
[42]4.2.3 Implementation with Multiple Gas Species
[43]4.2.4 Neutrino Flux Distribution
[46]4.2.5 Determining the Uncertainty of the Neutrino Flux
[]4.3 Comparison to Other Surveys
[55]5 Summary and Outlook
[57]References