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Faint signatures in IceCube / vorgelegt von Timo Stürwald. Wuppertal, November 2024
Content
Abstract
Zusammenfassung
List of Tables
List of Figures
List of Acronyms
Introduction
Theory
The standard model of particle physics
Bosons
Fermions
Interactions
Beyond the standard model
Fractionally charged particles
Summary of searches
Millicharged particles from the atmosphere
Light production processes
Cherenkov effect
Ionization
Pair production
Photonuclear interaction
Bremsstrahlung
Energy losses for fractionally charged particles
Survival probability for fractionally charged particles
Cosmic rays
Extensive Air showers
The IceCube Neutrino Observatory
The Antarctic ice
IceCube
DeepCore
The Digital Optical Module
Dark Noise
Triggering
Transmission and filtering
Transmission and filtering until 2023
Transmission and filtering from 2023 on
Neutrino signatures
Simulation
Signal simulation
Event generation
Event propagation
Detector simulation
Processing and Filtering
Effective area
FCP properties
The Faint Particle Trigger
Faint Particle Trigger DC version
Sliding time window
Cut 1: Number of hits
Cut 2: Number of Doubles
Cut 3: Directional consistency of Doubles
Cut 4: SLC fraction
Variation of the time window separation parameter
Summary of cuts and results
Faint Particle trigger full detector and IC79 versions
Input hit rate reduction
Isolated DOMs, all hits and IC79 versions
Comparison of all Faint Particle Trigger versions
Tests and deployment of the Faint Particle Trigger
The South Pole Test System
Test runs at the South Pole System
The Faint Particle Trigger rate trend
The Faint Particle Filter
The Faint Particle Filter algorithm
Input to the Faint Particle Filter
The only FPT branch
Multiple triggers/DC branch
NChannel vs. #HLC Cut in DC
NChannel vs. #HLC cut in IC
IceHive and CoincSuite
Cleaning and reconstruction
Faint Particle Filter results
Faint Particle Filter test runs
Improvements by the Faint Particle Trigger and Filter
Simulation sets and comparison levels
Simulation sets
Trigger level
Online Filter level
Filter level
Trigger efficiency comparison for various masses
Effective area comparison
Effective area in the isotropic scenario
Effect of the survival probability on the zenith distribution
Effective area for the non-isotropic scenario
Expected event rates for the MCP model
Conclusion and Outlook
Appendix A
Appendix B
Appendix C
Appendix D
Bibliography
Acknowledgements