Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ap%26ss.307..305n&link_type=abstract
Astrophysics and Space Science, Volume 307, Issue 1-3, pp. 305-308
Astronomy and Astrophysics
Astrophysics
Gamma Ray Bursts, Collapsars, Pic, Numerical, Relativity
Scientific paper
Particle acceleration via Poynting vector with toroidal magnetic field is studied in 3D PIC simulation of electron-positron plasma. We choose two different initial magnetic field configurations to compare how the particle acceleration is affected by the expansion of electromagnetic wave. In the cylindrical case, the electromagnetic field strength decays as (ct)-2, and particles are accelerated in the radial direction as well as the axial direction. Rayleigh-Taylor instability is also observed at the center of the cylinder. In the torus case, the field strength decays as (ct)-3, making the acceleration less efficient. Particles accelerated in the axial direction by E × B force creates strong charge separation.
Liang Edison
Noguchi Koichi
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