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Register a new userImproving particle beam acceleration in plasmas
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Added by
Meirielen Caetano de Sousa
Publication date
2017
fields
Physics
and research's language is
English
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The dynamics of wave-particle interactions in magnetized plasmas restricts the wave amplitude to moderate values for particle beam acceleration from rest energy. We analyze how a perturbing invariant robust barrier modifies the phase space of the system and enlarges the wave amplitude interval for particle acceleration. For low values of the wave amplitude, the acceleration becomes effective for particles with initial energy close to the rest energy. For higher values of the wave amplitude, the robust barrier controls chaos in the system and restores the acceleration process. We also determine the best position for the perturbing barrier in phase space in order to increase the final energy of the particles.
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Particle beams provided by accelerators occupy a finite volume of the four dimensional transverse phase space. The latter is spanned by the four degrees of freedom, i.e., horizontal/vertical position and momentum. This volume is referred to as emittance. Horizontal and vertical emittances are obtained through projections onto the two transverse sub-phase spaces. Eigen-emittances are obtained from the latter by removing all horizontal-vertical correlations through an appropriate beam optics section. Canonical vorticity flux is used for instance for modelling dynamics of tubes formed by magnetic field lines and particle currents embedded into plasmas. This report is on the relation of eigen-emittances and canonical vorticity flux. Change of beam eigen-emittances is equivalent to change of beam canonical vorticity flux.
Particle acceleration and heating at mildly relativistic magnetized shocks in electron-ion plasma are investigated with unprecedentedly high-resolution two-dimensional particle-in-cell simulations that include ion-scale shock rippling. Electrons are super-adiabatically heated at the shock, and most of the energy transfer from protons to electrons takes place at or downstream of the shock. We are the first to demonstrate that shock rippling is crucial for the energization of electrons at the shock. They remain well below equipartition with the protons. The downstream electron spectra are approximately thermal with a limited supra-thermal power-law component. Our results are discussed in the context of wakefield acceleration and the modelling of electromagnetic radiation from blazar cores.
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