1104.4760 (A. Osmane et al.)
A. Osmane, A. M. Hamza
Using bifurcation theory on a dynamical system simulating the interaction of
a particle with an obliquely propagating wave in relativistic regimes, we
demonstrate that uniform acceleration arises as a consequence of Hopf
bifurcations of Landau resonant particles. The acceleration process arises as a
form of surfatron established through the locking in pitch angle, gyrophase,
and physical trapping along the wave-vector direction. Integrating the
dynamical system for large amplitudes ($\delta B/B_0\sim0.1$) obliquely
propagating waves, we find that electrons with initial energies in the keV
range can be accelerated to MeV energies on timescales of the order of
milliseconds. The Hopf condition of Landau resonant particles could underlie
some of the most efficient energization of particles in space and astrophysical
plasmas.
View original:
http://arxiv.org/abs/1104.4760
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