What are Cosmic Rays? A short history What do we know now about CRs CR – their energy spectrum Why all these is interesting? How CRs can be accelerated?
Hyperon Star Model
projector test
Exploring New Phenomena at CDF
A.Ereditato SS 2008 1 Elementarteilchenphysik Antonio Ereditato LHEP University of Bern Lesson on:Weak interaction (5) Exercises: beta decay, V-A structure.
Georg Raffelt, MPI Physics, Munich Physics Colloquium, Univ. Sydney, 3 March 2014 Dark Matter Axion Dark Matter Georg G. Raffelt, Max-Planck-Institut für.
FCNC processes - a window to new physics
