2008/03/31 by J. Frederiksen, J. Trier Frederiksen · 1 citation
Physics and Astronomy · #Astro and Planetary Science #Astrophysics #Gamma-ray burst #Gamma-ray bursts and supernovae #Physics #astro-ph
paper · pdf · doi:10.1086/589648
published as Astrophys.J.680:L5-L8,2008 · 4 pages, 4 figures, accepted by Astrophyiscal Journal Letters. Rev.2: corrected figure colorbar units, shortened discussion, added references -- conclusions unchanged
openalex publication_date 2008/05/09 · arxiv created 2008/05/15 · arxiv updated 2009/12/01 · openalex created_date 2020/11/23 · openalex updated_date 2026/08/06
We present a numerical study of gamma-ray burst-circumburst medium interaction and plasma preconditioning via Compton scattering. The simulation tool employed here—the PhotonPlasma code—is a unique hybrid model; it combines a highly parallelized (Vlasov) particle-in-cell approach with continuous weighting of particles and a sub-Debye Monte Carlo binary particle interaction framework. Our first results from 3D simulations with this new simulation tool suggest that magnetic fields and plasma density filaments are created in the wakefield of prompt gamma-ray bursts, and that the photon flux density gradient has a significant impact on particle acceleration in the burst head and wakefield. We discuss some possible implications of the circumburst medium preconditioning for the trailing afterglow, and also discuss which additional processes will be needed to improve future studies within this unique and powerful simulation framework.