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.TP11.156
Abstract: TP11.00156 : Particle- in- cell simulations of plasma heating inside a density scale length for the interaction of ultra-short laser pulse with under-dense plasma
Presenter:
Seyed Abolfazl Ghasemi
(Plasma and Nuclear Fusion research School, Nuclear Science and Technology research Institute, Tehran-Iran)
Author:
Seyed Abolfazl Ghasemi
(Plasma and Nuclear Fusion research School, Nuclear Science and Technology research Institute, Tehran-Iran)
Collaboration:
Masoud Pishdast, Jamal Aldin Yazdanpanah
In this paper, nonlinear mechanisms of electron heating during the earlier stage of the interaction of an ultra-intense short laser pulse () with an under-dense plasma () inside a preformed density scale length has been investigated for exponential density profile. The fully kinetic particle in cell simulation code (1D3V) has been made to study the plasma heating at onset time of interaction. Our simulations indicate that, for ultra-intense short laser pulse, the nonlinear pulse scatterings are found to be very fast at the earlier time of interaction and cause plasma heating. As a key point in our discussion, our parametric simulations show that at the very earlier stage of interaction, two main electrostatic mechanisms, vacuum-plasma wave break together with longitudinal plasma oscillations, are the dominant acceleration mechanisms which lead to electron chaotic pattern and plasma heating. Meanwhile, studying the effect of density scale lengths on plasma heating revealed that, for exponential density profile, main acceleration mechanisms mentioned above are sufficiently developed during the propagation in typical short density scale lengths about for normalized vector potential .
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.TP11.156
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