Eric Prebys, FNAL. To probe smaller scales, we must go to higher energy To discover new particles, we need enough energy available to create them The.
ACCELERATORS Timothy Koeth Rutgers University. Basics Motivation History, R&D, and applications –Failed attempts –Getting warmer. –Linear accelerator.
PHY418 PARTICLE ASTROPHYSICS Emission of High Energy Photons 1.
Dissipation and Acceleration in Relativistically Magnetized Outflows: Crab Nebula as Micro-Blazar Jonathan Arons University of California Berkeley & Santa.
Liam Kieser, Ian Clark, Jack Cornett and Xiaolei Zhao, University of Ottawa Ted Litherland, University of Toronto Instrumentation Session, CAP 2014 Congress,
Ron Fox Tcl 2011 Manassas, VA, Slide 1 Tcl at the NSCL: A (30? well maybe 15) year forward looking uh…retrospective Staff of the National Superconducting.
Solar Probe Plus A NASA Mission to Touch the Sun Solar Probe Plus Science Workshop March 26, 2013 Solar Probe Plus A NASA Mission to Touch the Sun Nicky.
Overview of ‘classical’ or ‘standardized’ DPA calculation stemming from the reactor world. Colin English NNL.
Eric Prebys FNAL Accelerator Physics Center June 7-17, 2010.
Form Factor Dark Matter
Cataclysmic variables as hard X-ray emitters seen by INTEGRAL The X-ray Universe 2008, Granada, Spain, 27-30 May R. Gális 1,2, R. Hudec 1, F. Münz 3, M.
K. Jahoda, 6 Aug 2007 X-ray School, GWU Proportional Counters Some of what you should know in order to use proportional counters for Spectroscopy, Timing,
