Pitch-angle Scattering of Energetic Particles with Adiabatic Focusing
Abstract
Understanding turbulent transport of charged particles in magnetized plasmas often requires a model for the description of random variations in the particle's pitch angle. The Fokker-Planck coefficient of pitch-angle scattering, which is used to describe scattering parallel to the mean magnetic field, is therefore of central importance. Whereas quasi-linear theory assumes a homogeneous mean magnetic field, such a condition is often not fulfilled, especially for high-energy particles. Here, a new derivation of the quasi-linear approach is given that is based on the unperturbed orbit found for an adiabatically focused mean magnetic field. The results show that, depending on the ratio of the focusing length and the particle's Larmor radius, the Fokker-Planck coefficient is significantly modified but agrees with the classical expression in the limit of a homogeneous mean magnetic field.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- October 2014
- DOI:
- 10.1088/0004-637X/794/2/138
- arXiv:
- arXiv:1408.6947
- Bibcode:
- 2014ApJ...794..138T
- Keywords:
-
- cosmic rays;
- diffusion;
- magnetic fields;
- plasmas;
- turbulence;
- Astrophysics - High Energy Astrophysical Phenomena;
- Physics - Plasma Physics
- E-Print:
- 10 pages, 6 figures, accepted for publication in ApJ