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Hardware integration of the AMANDA into the IceCube Neutrino Telescope and search for supersymmetric particles with the IceCube Neutrino Telescope / vorgelegt von Andreas Tepe. 2009
Content
Nomenclature
Introduction
Neutrinos from Cosmic Rays
Neutrinos and their Properties
High Energy Cosmic-Ray Neutrinos
Cosmic Rays
The Waxman-Bahcall-Limit
Z-Bursts
Active Galactic Nuclei (AGN)
Gamma-Ray Bursts (GRBs)
Greisen-Zatsepin-Kuzmin (GZK) cutoff
Topological Defects
High Energy Neutrino Detection
Neutrino Interactions with Matter
Neutrino Detection Mechanisms
Background for Neutrino Detection
The Hardware Integration of AMANDA into IceCube
AMANDA and IceCube
Detector Principles
The AMANDA Neutrino Telescope
In Ice
On Ice
DAQ Timing
The IceCube Neutrino Telescope
Detector Principles
IceCube Timing
IceCube Data Taking / TestDAQ
AMANDA/IceCube Integration
Motivation
Dense Instrumentation
IceCube as Veto
Demands on the Integration System
Realization of the Hardware Synchronization
The GPS Latch GPS4TWR
CLK2ECL and the Backplane
The Optical to Electrical Converter OPT2EL
The AMANDA DOM Mainboards, the Cable Simulator and the AMANDA DOMHub
The SyncCrate
The Improved Trigger Logic
The Hardware Synchronization Scheme
Software Changes
DSP Software Improvement
Synchronization Test System
Test Hardware
Components Test
Measurements
Implementation at the South Pole
Season 2005/06
Season 2006/07
Season 2007/08
Synchronization Verification
Absolute Cable Delay between MAPO and ICL
Observation of the Synchronization Stability with TestDAQ
AMANDA/IceCube Synchronization Checker
Results
Simulation Studies
Combined Analysis
The Future AMANDA: IceCube Deep Core
Searching SUSY Matter with IceCube
Supersymmetry
Why Supersymmetry?
Concept of Supersymmetry
SUSYs in IceCube
SUSY Mass Scales
stau Radiation Losses
Neutrino Induced SUSY Particle Production
Background for stau Detection
Simulation of SUSY Events
Simulating Simply -- The SUSY-simple-gen Module
stau Energy
Primary Interaction Point
stau direction
Benefit of the SUSY-simple-gen Module
Simulation of double stau tracks with the SUSY-gen Module
Generation of the Neutrino Flux
Generation of the Neutrino Interaction Point
stau Generation
Searching for SUSY events
Filter Description
Event Cleaning
Number of Hit DOMs
Number and Position of Hit Strings
Track Direction
Flatness
Sphericity
Event Causality
External Event Processing
Filter Settings
Dataset
Configuring the Filter
Applying the SUSYFilter
Down-going Muons
Coincident Atmospheric Muons
Real Data
Online or Offline Filtering
Résumé and Outlook
Monte Carlo Simulation
Generation of a Power Law Energy Spectrum
Generation of an Equal Point Distribution on a Sphere
Generation of an Arbitrary Distribution
Power Law Distribution in Double Logarithmic Plot
Particle Generation in the CM System
Transformation to the CMS
Transformation to the Lab Frame
Correct Treatment of the Neutrino Interaction
stau Generation Modules
stau Generation
Detector Response
stau Filtering Modules
Data Cleaning
FeatureExtractor
SUSYFilter
Bibliography
List of Figures
Index