Slide 1 1 Visible and Invisible Universe: A short commentary Carlo Rubbia CERN Geneva, Switzerland and INFN/LNGS, Assergi, Italy Slide 2 Venice, April 16, 2008Slide# : 2…
Slide 1 X. Barcons, XEUS SAGXEUS: Physics of the hot evolving Universe XEUS: The Physics of the hot Evolving Universe Xavier Barcons Slide 2 X. Barcons, XEUS SAGXEUS: Physics…
Slide 1 The Near Infrared Background Excess and Star Formation in the HUDF Rodger Thompson Steward Observatory University of Arizona Slide 2 Blameless Collaborators Mark…
Slide 1 EJB April 2006 Nuclear Science: The Mission Understand the origin, evolution, and structure of the baryonic matter of the Universe Cosmic accelerationRotation curves…
Dark Matter Candidates Astroparticlephysics, UZH, Spring 2012 Marc Schumann [email protected] What will we learn today? ● What kind of Dark Matter do we „need“?…
Slide 1 Klaus Peters Ruhr-Universität Bochum U Cincinnati, Nov 18, 2002 FNAL, Batavia, Nov 20, 2002 JLab, Newport News, Nov 22, 2002 TRIUMF, Vancouver, Nov 28, 2002 at the…
Slide 1 Dark Matter cannot be seen directly with telescopes; it neither emits nor absorbs light; estimated to constitute 84.5% of the total matter in the universe – and…
Slide 1 1 CERN Summer Student Lectures 2007A. Höcker: The Violation of Symmetry between Matter and Antimatter (1 & 2) The Violation of Symmetry between Matter and Antimatter…