Turbulent Transport and Heating of Trace Heavy Ions in Hot Magnetized Plasmas

Physical Review Letters American Physical Society (APS) 109:18 (2012) 185003

Authors:

M Barnes, FI Parra, W Dorland

Actions for axisymmetric potentials

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 426:2 (2012) 1324-1327

More dynamical models of our Galaxy

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 426:2 (2012) 1328-1337

Stellar transits in active galactic nuclei

(2012)

Authors:

Bence Béky, Bence Kocsis

Analytic fluid theory of beam spiraling in high-intensity cyclotrons

ArXiv 1210.1175 (2012)

Authors:

Antoine J Cerfon, Jeffrey P Freidberg, Felix I Parra, Timothy A Antaya

Abstract:

Using a two-dimensional fluid description, we investigate the nonlinear radial-longitudinal dynamics of intense beams in storage rings and cyclotrons. With a multiscale analysis separating the time scale associated with the betatron motion and the slower time scale associated with space-charge effects, we show that the longitudinal-radial vortex motion can be understood in the frame moving with the charged beam as the nonlinear advection of the beam by the $\mathbf{E}\times\mathbf{B}$ velocity field, where $\mathbf{E}$ is the electric field due to the space charge and $\mathbf{B}$ is the external magnetic field. This interpretation provides simple explanations for the stability of round beams and for the development of spiral halos in elongated beams. By numerically solving the nonlinear advection equation for the beam density, we find that it is also in quantitative agreement with results obtained in PIC simulations.