Efficient modeling laser wakefield acceleration using quasi-3D quasi-static PIC simulations
POSTER
Abstract
High fidelity modeling of laser wakefield acceleration (LWFA) requires 3D large-scale particle-in-cell (PIC) method. 3D PIC algorithms based on the quasi-static approximation (QSA) have been successfully applied to efficiently model the interaction between relativistic charged particle beams and plasma. In a QSA PIC algorithm, the plasma response is calculated based on the QSA form of Maxwell's equations. These fields are then used to advance the charged particle beam or laser forward by a large time step. Since the time step is not limited by the regular CFL condition that constrains a standard PIC code, a QSA PIC code can achieve orders of magnitude speedup in performance. Recently, a new hybrid QSA PIC algorithm that combines another speedup technique known as an azimuthal Fourier decomposition has been proposed and implemented. This hybrid algorithm decomposes the electromagnetic fields, charge and current density into azimuthal harmonics and only the Fourier coefficients need to be updated, which can further reduce the algorithmic complexity. Modeling LWFA in a full 3D PIC algorithm is very computationally expensive due to the enormous disparity of physical scales to be resolved. In the QSA the laser is modeled using the ponderomotive guiding center (PGC) approach. We describe how to implement a PGC algorithm compatible with the QSA PIC algorithms based on the azimuthal mode expansion. This algorithm permits time steps orders of magnitude larger than the cell size and it can be asynchronously parallelized. Benchmarks and comparisons between a fully 3D explicit PIC code (OSIRIS), as well as a few examples related to laser wakefield acceleration, are presented.
Presenters
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Fei Li
University of California, Los Angeles
Authors
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Fei Li
University of California, Los Angeles
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Weiming An
Beijing Normal Univ
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Frank S Tsung
University of California, Los Angeles
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Viktor K Decyk
University of California, Los Angeles
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Warren B Mori
University of California, Los Angeles, Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA