Table of ContentsUK Dark Matter Search Lecture Road Map Lecture Road Map What is an Observatory? Or Is It….? Weighing a Galaxy The Dark Matter Halo Weighing Galaxy Clusters Weighing the Universe Expansion of the Universe The Hubble Flow Hubble Flow (Elsewhere) Cosmology Standard Model How Massive is the Universe? Lecture Road Map PP: Standard Model Dark Matter Candidate Review Nucleosynthesis Contributions to _ Baryonic Dark Matter Microlensing Searches Lecture Road Map Non-Baryonic Dark Matter Cold Dark Matter Supersymmetry Lecture Road Map What are Cosmic Rays? Extensive Air Showers Detecting EAS PeV Neutral Cosmic Rays EeV Cosmic Rays: Auger Lecture Road Map Hot Dark Matter - Neutrinos Neutrino Production in SSM Solar Neutrino Problem Atmospheric Neutrino Problem Solution to Both Problems Super Kamiokande Results Implication of Results Lecture Road Map Principles of WIMP Detection I Principle of WIMP Detection II Sodium Iodide Detector Background Signals Boulby Potash Mine Shielding Systems ‘Stage I’ Results Background Discrimination I Background Discrimination II Discrimination Results Current NaI Situation Liquid Xenon Scintillation Allow recombination Prevent Recombination Signal Identification DRIFT Collaboration Low Pressure Xe Gas TPC State of the Art in Cosmology |
Author: Nigel J. T. Smith
Email: n.j.t.smith@rl.ac.uk Home Page: http://hepwww.rl.ac.uk/ukdmc/ |