Articles | Volume 28, issue 11
Ann. Geophys., 28, 2127–2132, 2010
https://doi.org/10.5194/angeo-28-2127-2010

Special issue: Dynamical processes in space plasmas

Ann. Geophys., 28, 2127–2132, 2010
https://doi.org/10.5194/angeo-28-2127-2010

ANGEO Communicates 24 Nov 2010

ANGEO Communicates | 24 Nov 2010

Recent progresses in relativistic beam-plasma instability theory

A. Bret1, M. E. Dieckmann2, and L. Gremillet3 A. Bret et al.
  • 1ETSI Industriales, Universidad de Castilla-La Mancha, 13071 Ciudad Real, Spain
  • 2VITA, Department of Science and Technology (ITN), Linköping University, 60174, Norrköping, Sweden
  • 3CEA, DAM, DIF, 91297 Arpajon, France

Abstract. Beam-plasma instabilities are a key physical process in many astrophysical phenomena. Within the fireball model of Gamma ray bursts, they first mediate a relativistic collisionless shock before they produce upstream the turbulence needed for the Fermi acceleration process. While non-relativistic systems are usually governed by flow-aligned unstable modes, relativistic ones are likely to be dominated by normally or even obliquely propagating waves. After reviewing the basis of the theory, results related to the relativistic kinetic regime of the poorly-known oblique unstable modes will be presented. Relevant systems besides the well-known electron beam-plasma interaction are presented, and it is shown how the concept of modes hierarchy yields a criterion to assess the proton to electron mass ratio in Particle in cell simulations.