Abstract
Monte Carlo methods are often employed to numerically integrate kinetic equations, such as the particle-in-cell method for the plasma kinetic equation, but these methods suffer from the introduction of counting noise to the solution. We report on a cautionary tale of counting noise modifying the nonlinear saturation of kinetic instabilities driven by unstable beams of plasma. We find a saturated magnetic field in under-resolved particle-in-cell simulations due to the sampling error in the current density. The noise-induced magnetic field is anomalous, as the magnetic field damps away in continuum kinetic and increased particle count particle-in-cell simulations. This modification of the saturated state has implications for a broad array of astrophysical phenomena beyond the simple plasma system considered here, and it stresses the care that must be taken when using particle methods for kinetic equations.
Original language | English (US) |
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Article number | 175860401 |
Journal | Journal of Plasma Physics |
DOIs | |
State | Accepted/In press - 2020 |
All Science Journal Classification (ASJC) codes
- Condensed Matter Physics
Keywords
- astrophysical plasmas
- plasma simulation
- space plasma physics