Energy spectra of X-ray quasi- periodic oscillations in accreting black hole binaries Piotr Życki & Małgorzata Sobolewska § Nicolaus Copernicus Astronomical.
FFAG F ixed F ield A lternating G radient Synchrotrons A new type of particle accelerator - with a wide variety of applications Cancer Therapy and UK Activities.
6 8 9 10 11 12 Hadrons: color singlets “white states”
Nuclear Decay Data at NPL Paddy Regan NPL Radioactivity Group, AIR Division & Department of Physics, University of Surrey.
1 An Introduction to X-ray Spectral Fitting I: Getting started with XSPEC Other material XSPEC manual:
Particlesymbolrest energy in MeV electron e 0.5109989 muon 105.658357 neutral pion 0 134.9766 charged pion 139.57018 proton p 938.27200 neutron.
Inverse Problems in Solar Imaging Spectroscopy - Future Applications G.J. Hurford Space Sciences Lab University of California, Berkeley Vienna 20 July.
Interaction of Shear Alfven Waves (SAW) with Trapped Energetic Protons in the Inner Radiation Belt X. Shao, K. Papadopoulos, A. S. Sharma Department of.
Ultra High Energy Cosmic Rays Glennys R. Farrar Center for Cosmology and Particle Physics, Department of Physics, New York University.
Creighton University ALICE - USA Michael Cherney May 23, 2007.
1.Fluctuations are important because the number of particles in a system is much less than Avogadro’s number; 2.Importance of the surface properties.
What Are Fundamental Constants? Cosmic Accidents? Determined by Dynamics? Changing in Time? Given by Self-Consistency? Calculable?
