Dark Matter and Neutrinos
What is an Observatory?
Or Is It….?
Weighing the Earth
Testing for ‘Missing’ Mass
The Earth’s ‘Missing’ Mass
Weighing a Galaxy
Weighing Galaxy Clusters
Weighing the Universe
How Massive is the Universe?
PP: Standard Model
Dark Matter Candidate Review
Nucleosynthesis
Contributions to _
Baryonic Dark Matter
Microlensing Searches
Non-Baryonic Dark Matter
Supersymmetry
What are Cosmic Rays?
Extensive Air Showers
Detecting EAS
Antarctica & The South Pole
PeV Neutral Cosmic Rays
EeV Cosmic Rays: Auger
Hot Dark Matter - Neutrinos
Neutrino Production in SSM
Solar Neutrino Problem
Atmospheric Neutrino Problem
Solution to Both Problems
Implication of Results
Principles of WIMP Detection I
Principle of WIMP Detection II
Sodium Iodide Detector
Background Signals
Boulby Potash Mine
Travels of a Physicist
Shielding Systems
‘Stage I’ Results
Background Discrimination I
Background Discrimination II
Discrimination Results
Future Systems - Xenon
Email: n.j.t.smith@rl.ac.uk