Photohadronic processes and neutrinos Lecture 2 Summer school High energy astrophysics August 22-26, 2011 Weesenstein, Germany Walter Winter Universität.
Andrea Candelori - Irradiation facilities at the INFN National Laboratory of Legnaro – Irradiation facilities for semiconductor.
controlling the statistical decay of excited nuclei an crucial input for nucleosynthesis calculations (r-process), reactor science, etc.
1.1b Particles & Radiation Quarks & Leptons Breithaupt pages 18 to 27 April 8 th, 2010.
Green Fluorescent Protein Structure Analysis and Function 4.25.12
Semiconductor Modelling EliDrewShazz. Semiconductor History 1600 to 1800 – research in electrical and magnetic phenomena 1876 – Telephone invented 1880.
High Energy Neutrinos from Astrophysical Sources Dmitry Semikoz UCLA, Los Angeles & INR, Moscow.
The structure of our Milky Way galaxy: a container of gas and stars arranged in various components with various properties.. Gaseous halo? ~ 6 x 10 10.
Florian Nichitiu, James R. Drumond, Jiansheng Zou, Robert Deschamault(*) Department of Physics, University of Toronto, Canada (*) COM DEV, Cambridge, Ontario,
PROTEL, A FEASIBILITY STUDY EXPERIMENT PROTEL (PROtoni TErapia Locale). 2 years Padova (C.N. P. Rossi) LNL (R.L. G. Moschini) Pavia ( D. Scannicchio) parteciperà.
Neutrinos: From Cosmic Rays and Accelerators to Old Iron Mines and the Fate of the Universe Alec Habig UMD Physics.
Search for solar neutrons associated with proton flares in solar cycle 23 Yutaka Matsubara (presenter) Solar-Terrestrial Environment Laboratory, Nagoya.