High-Resolution Particle-In-Cell Simulations of Two-Dimensional Bernstein-Greene-Kruskal Modes

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Main Authors: McClung, J., Franciscovich, M. T., Germaschewski, K., Ng, C. S.
Format: Preprint
Published: 2023
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author McClung, J.
Franciscovich, M. T.
Germaschewski, K.
Ng, C. S.
author_facet McClung, J.
Franciscovich, M. T.
Germaschewski, K.
Ng, C. S.
contents We present two dimensional (2D) particle-in-cell (PIC) simulations of 2D Bernstein-Greene-Kruskal (BGK) modes, which are exact nonlinear steady-state solutions of the Vlasov-Poisson equations, on a 2D plane perpendicular to a background magnetic field, with a cylindrically symmetric electric potential localized on the plane. PIC simulations are initialized using analytic electron distributions and electric potentials from the theory. We confirm the validity of such solutions using high-resolutions up to a 2048^2 grid. We show that the solutions are dynamically stable for a stronger background magnetic field, while keeping other parameters of the model fixed, but become unstable when the field strength is weaker than a certain value. When a mode becomes unstable, we observe that the instability begins with the excitation of azimuthal electrostatic waves that ends with a spiral pattern.
format Preprint
id arxiv_https___arxiv_org_abs_2311_08613
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle High-Resolution Particle-In-Cell Simulations of Two-Dimensional Bernstein-Greene-Kruskal Modes
McClung, J.
Franciscovich, M. T.
Germaschewski, K.
Ng, C. S.
Plasma Physics
Astrophysics of Galaxies
Computational Physics
Space Physics
We present two dimensional (2D) particle-in-cell (PIC) simulations of 2D Bernstein-Greene-Kruskal (BGK) modes, which are exact nonlinear steady-state solutions of the Vlasov-Poisson equations, on a 2D plane perpendicular to a background magnetic field, with a cylindrically symmetric electric potential localized on the plane. PIC simulations are initialized using analytic electron distributions and electric potentials from the theory. We confirm the validity of such solutions using high-resolutions up to a 2048^2 grid. We show that the solutions are dynamically stable for a stronger background magnetic field, while keeping other parameters of the model fixed, but become unstable when the field strength is weaker than a certain value. When a mode becomes unstable, we observe that the instability begins with the excitation of azimuthal electrostatic waves that ends with a spiral pattern.
title High-Resolution Particle-In-Cell Simulations of Two-Dimensional Bernstein-Greene-Kruskal Modes
topic Plasma Physics
Astrophysics of Galaxies
Computational Physics
Space Physics
url https://arxiv.org/abs/2311.08613