Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session TP11: Poster Session VII: Basic Plasma Physics: Pure Electron Plasma, Strongly Coupled Plasmas, Self-Organization, Elementary Processes, Dusty Plasmas, Sheaths, Shocks, and Sources; Mini-conference on Nonlinear Waves and Processes in Space Plasmas - Posters; MHD and Stability, Transients (2), Runaway Electrons; NSTX-U; Spherical Tokamaks; Analytical and Computational Techniques; Diagnostics (9:30am-12:30pm)
Thursday, November 8, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.TP11.8
Abstract: TP11.00008 : Dynamics of positrons during relativistic electron runaway*
(Author Not Attending)
Presenter:
Ola Embréus
(Chalmers University of Technology)
Authors:
Ola Embréus
(Chalmers University of Technology)
Linnea Hesslow
(Chalmers University of Technology)
Mathias Hoppe
(Chalmers University of Technology)
Gergely Papp
(Max-Planck-Institute for Plasma Physics)
Katya Richards
(Chalmers University of Technology)
Tünde Fülöp
(Chalmers University of Technology)
In plasmas, sufficiently strong electric fields can accelerate charged particles to relativistic energies via the runaway mechanism. In this contribution we describe the dynamics of positrons that are created during a runaway avalanche.
We derive a threshold electric field above which the direct pair production in collisions will exceed the pair production due to photons produced in hard X-ray emission, which is traditionally the main positron producing mechanism. This threshold field is found to be of the order of tens of avalanche threshold fields.
We present analytical and numerical solutions of the positron kinetic equation, illustrating similarities and differences between the runaway dynamics of positrons and electrons. The numerical study provides the ratio of positrons to runaway electrons, which is used to predict the amount of annihilation radiation emitted during tokamak disruptions as a function of the plasma parameters. This is compared to the HXR emission of electrons, and we calculate the signal-to-noise ratio as well as the total annihilation photon count.
*This work was supported by the European Research Council (ERC-2014-CoG grant 647121) and the Swedish Research Council (Dnr.~2014-5510).
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.TP11.8
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