Dark Matter and Other Hidden Treasures in the Neutrino Sector - Kevork Abazajian
Kavli Institute for Theoretical Physics via YouTube
Overview
Syllabus
Introduction
Neutrino Mass Generation
Dark Matter Production
NonOscillation Production
cosmological structure formation
matter of power spectrum
small scale cut off
canonical dark matter
distribution of dark matter
Too big to fail problem
Particle mass warm background effects
Dark Matter is thermal
Nonresonant production
Thermal production
Neutrino photon
Why is this repeating
What does this mean
Lensing constraints on substructure
Thermal distributions
Main Results
Prism Mission
Enhanced Xray Timing Explorer
Side Project
Forecasts
Interdisciplinarity
Summary
Questions and Comments
Taught by
Kavli Institute for Theoretical Physics