SPACE AND COSMIC RAY PHYSICS SEMINAR

University of Maryland
Atlantic Building, Room 2400
4:30 PM Monday, February 6, 2012
Coffee, Tea & Cookies 4:15-4:30 PM
Organized by Association of Korean Physicists in America

Reinhard Schlickeiser
The Ruhr University of Bochum, Germany

Focused acceleration of cosmic rays: A new universal first-order Fermi mechanism

The Fokker-Planck equation for cosmic-ray particles in a spatially varying guide magnetic field in a turbulent plasma is analyzed. An expression is derived for the mean rate of change of particle momentum, caused by the effect of adiabatic focusing in a non-uniform guide field. Results of an earlier diffusion-limit analysis are confirmed, and the physical picture is clarified by working directly with the Fokker-Planck equation. A distributed first-order Fermi acceleration mechanism is identified, which can be termed focused acceleration. If the forward- and backward-propagating waves have equal polarizations, focused acceleration operates when the net cross helicity of Alfvénic slab turbulence is either negative in a diverging guide field or positive in a converging guide field. Focused acceleration can contribute to the formation of the anomalous cosmic-ray spectrum at the heliospheric termination shock, and quantitatively modifies the physics of diffusive shock acceleration of cosmic ray particles.