Magnetic Field Generation and electron acceleration in Collisionless Shocks

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dc.creatorHededal, C. B.
dc.creatorFrederiksen, J. Trier
dc.creatorHaugboelle, T.
dc.creatorNordlund, Å.
dc.date2004-10-15
dc.date2004-10-16
dc.date.accessioned2026-07-07T02:15:16Z
dc.date.available2026-07-07T02:15:16Z
dc.descriptionUsing a three dimensional relativistic particle-in-cell code we have performed numerical experiments of plasma shells colliding at relativistic velocities. Such scenarios are found in many astrophysical objects e.g. the relativistic outflow from gamma ray bursts, active galactic nuclei jets and supernova remnants. We show how a Weibel-like two-stream instability is capable of generating small-scale magnetic filaments with strength up to percents of equipartition. Such field topology is ideal for the generation of jitter radiation as opposed to synchrotron radiation. We also explain how the field generating mechanism involves acceleration of electrons to power law distributions (N(E)~E^(-p))through a non-Fermi acceleration mechanism. The results add to our understanding of collisionless shocks.
dc.description4 pages, 3 figures. Proceeding for the International School of Cosmic Ray Astrophysics - 14th Course: "Neutrinos and Explosive Events in the Universe", July 2004 - Erice, Italy
dc.identifierhttps://arxiv.org/abs/astro-ph/0410382
dc.identifierhttp://arxiv.org/abs/astro-ph/0410382
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8379
dc.subjectAstrophysics
dc.titleMagnetic Field Generation and electron acceleration in Collisionless Shocks
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