Mitglied der Helmholtz-Gemeinschaft From Hadron Physics to the Precision Frontier A Very Short Introduction August 6, 2012 | Hans Ströher (Forschungszentrum.
P308 – Particle Interactions Dr David Cussans Mott Lecture Theatre Monday 11:10am Tuesday,Wednesday: 10am.
Adam Para, October 14, 2005 First look at PFA/clustering with RPC-based calorimeter Progress Report.
FLUKA as a new high energy cosmic ray generator G. Battistoni 2, A. Margiotta 1, S. Muraro 2, M. Sioli 1 University and INFN of 1) Bologna and 2) Milano.
CHIPP Sept 2005Jean-Sébastien GraulichSlide 1 What is MICE Muon Ionisation Cooling Experiment What is Ionisation Cooling ? Cooling = Reduction of Beam.
Forward particle production measured by LHCf; testing hadronic interaction models for CR physics Takashi SAKO (Solar-Terrestrial environment Laboratory/Kobayashi-
The n 3 He Experiment Probing the Hadronic Weak Interaction Abstract: Although QCD has had tremendous success in describing the strong interaction at high.
(Some of the possible) Astrophysical origins of high energy cosmic rays Diego F. Torres [email protected] Lawrence Livermore Lab. California, 94550,
LHeC
Geomagnetic Spectroscopy: An Estimation of Primary Mass of Cosmic Rays Rajat K Dey 1,2 Arunava Bhadra 2 Jean-No ë l Capdevielle 3 1 Department of Physics.
Donika Plyku Old Dominion University HUGS 2008 at Jefferson Lab.
Spectral index in radio halos
