PHYSICS AT THE LHC Nicolo de Groot Radboud University Nijmegen And Nikhef.
First CMS Results with LHC BeamToyoko Orimoto, Caltech 1 First CMS Results with LHC Beam Toyoko Orimoto California Institute of Technology On behalf of.
Quark *) Distributions with the LHeC 1 Max Klein DESY, 7.4.2010 Meeting on QCD at the LHeC Project Scenarios Statistics Systematics Light Quarks Heavy.
Peter Mészáros Pennsylvania State University Astrophysical Sources of TeV to GZK neutrinos.
H.E.S.S. High Energy Stereoscopic System Jon Cerny Bancroft-Rosalie School August 2002.
June 9, 2002 Hallewell ANTARES RICH2002 1 ANTARES : A deep-sea 0.1 km² neutrino telescope Greg Hallewell – CPP Marseille Representing the Antares Collaboration.
Standard Model Physics at the Tevatron
The WLCG Service Starts Here…
IceCube
H.E.S.S. High Energy Stereoscopic System
Lepton - Photon 01 Francis Halzen the sky the sky > 10 GeV photon energy < 10 -14 cm wavelength > 10 8 TeV particles exist > 10 8 TeV particles exist Fly’s.
Aspen Institute for Physics 02 Francis Halzen the sky the sky > 10 GeV photon energy < 10 -14 cm wavelength > 10 8 TeV particles exist > 10 8 TeV particles.
