# Boundary Conditions for Continuum Simulations of Wall-bounded Kinetic   Plasmas

**Authors:** Petr Cagas, Ammar Hakim, Bhuvana Srinivasan

arXiv: 1906.07056 · 2019-06-18

## TL;DR

This paper introduces a novel continuum kinetic boundary condition framework for wall-bounded plasmas, enabling detailed modeling of secondary electron emission effects with high fidelity and computational efficiency.

## Contribution

It presents the first continuum kinetic boundary conditions using the distribution function, applicable to complex wall interactions including quantum-mechanical models.

## Key findings

- Secondary electron emission significantly affects plasma sheath behavior.
- Discontinuous Galerkin implementation effectively models boundary phenomena.
- Boundary conditions improve the accuracy of plasma simulations.

## Abstract

Continuum kinetic simulations of plasmas, where the distribution function of the species is directly discretized in phase-space, permits fully kinetic simulations without the statistical noise of particle-in-cell methods. Recent advances in numerical algorithms have made continuum kinetic simulations computationally competitive. This work presents the first continuum kinetic description of high-fidelity wall boundary conditions that utilize the readily available particle distribution function. The boundary condition is realized through a reflection function that can capture a wide range of cases from simple specular reflection to more involved first principles models. Examples with detailed discontinuous Galerkin implementation are provided for secondary electron emission using phenomenological and first-principles quantum-mechanical models. Results presented in this work demonstrate the effect of secondary electron emission on a classical plasma sheath.

## Full text

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## Figures

14 figures with captions in the complete paper: https://tomesphere.com/paper/1906.07056/full.md

## References

36 references — full list in the complete paper: https://tomesphere.com/paper/1906.07056/full.md

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Source: https://tomesphere.com/paper/1906.07056