Simulation of Relativistic Jets and Associated Self-consistent Radiation
Nov, 20114 pages
Part of Proceedings, 3rd High Energy Phenomena in Relativistic Outflows (HEPRO III) : Barcelona, Spain, June 27-July 1, 2011, Fermi symposium. Proceedings, 3rd Fermi Symposium, Rome, Italy, May 9-12, 2011
Published in:
- Int.J.Mod.Phys.Conf.Ser. 08 (2012) 259-264
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e-Print:
- 1111.3622 [astro-ph.HE]
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Abstract: (arXiv)
lasma instabilities excited in collisionless shocks are responsible for particle acceleration. We have investigated the particle acceleration and shock structure associated with an unmagnetized relativistic electron-positron jet propagating into an unmagnetized electron-positron plasma. Cold jet electrons are thermalized and slowed while the ambient electrons are swept up to create a partially developed hydrodynamic-like shock structure. In the leading shock, electron density increases by a factor of about 3.5 in the simulation frame. Strong electromagnetic fields are generated in the trailing shock and provide an emission site. These magnetic fields contribute to the electron's transverse deflection behind the shock. Our initial results of a jet-ambient interaction with anti-parallel magnetic fields show pile-up of magnetic fields at the colliding shock, which may lead to reconnection and associated particle acceleration. We will investigate the radiation in transient stage as a possible generation mechanism of precursors of prompt emission. In our simulations we calculate the radiation from electrons in the shock region. The detailed properties of this radiation are important for understanding the complex time evolution and spectral structure in gamma-ray bursts, relativistic jets, and supernova remnants.Note:
- 4 pages, 2 figures, 2011 Fermi Symposium proceedings - eConf C110509
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