Edison Liang, Ian Smith, Markus Boettcher
Using 2.5-dimensional Particle-in-Cell simulations, we studied the kinetic
physics of relativistic shear flows. We find efficient magnetic field
generation and nonthermal particle acceleration at the shear boundary. Ordered
flux tubes/sheets with alternating polarities and peak fields reaching
equipartition values are generated and sustained by the free-energy of the
shear flow. Nonthermal high-energy particles are accelerated by diffusive
acceleration. A quasi-power-law tail truncated at low energies is achieved at
strong shears. These results have important implications for the dissipation
and radiation of relativistic jets.
View original:
http://arxiv.org/abs/1111.3326
No comments:
Post a Comment