Observational data require a rich variety of mechanisms to accelerate fast particles in astrophysical environments operating under different conditions. The mechanisms discussed in the literature include varying magnetic fields in compact sources, stochastic processes in turbulent environments, and acceleration behind shocks. An alternative, much less explored mechanism involves particle acceleration within magnetic reconnection sites. In this chapter we discuss this mechanism and show that particles can be efficiently accelerated by reconnection through a first order Fermi process within large scale current sheets (specially when in the presence of local turbulence which speeds up the reconnection and make the acceleration region thicker) and also through a second order Fermi process in pure MHD turbulent environments.
@article{arxiv.1302.4374,
title = {Particle Acceleration by Magnetic Reconnection},
author = {Elisabete M. de Gouveia Dal Pino and Grzegorz Kowal},
journal= {arXiv preprint arXiv:1302.4374},
year = {2015}
}
Comments
24 pages, 8 figures. arXiv admin note: text overlap with arXiv:1103.2984, arXiv:1202.5256, arXiv:1008.1981 by other authors