利用gpu实现的3D PIC/MCC仿真研究低温等离子体的开发

A. Fierro, G. Laity, S. Beeson, J. Dickens, A. Neuber
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摘要

只提供摘要形式。利用CUDA环境开发了gpu加速的三维PIC/MCC仿真代码,以研究低温等离子体形成的物理过程。模拟结果有助于定量瞬态等离子体的发展,因为即使使用现代非侵入性技术,如非线性激光光谱或高速电诊断,也往往无法通过实验详细了解瞬态等离子体的发展。因此,计算方法,如细胞内粒子(PIC)和蒙特卡罗碰撞(MCC),为确定导致等离子体发展的机制提供了一种补充方法。然而,由于必须同时跟踪等离子体过程的数量,对等离子体发展的物理完全建模变得困难,并且直到最近才有计算资源提供跟踪数千万个粒子相互作用的能力。此外,图形处理单元(GPU)计算的引入通过NVIDIA CUDA等框架为科学代码的经济高效并行化提供了一种有吸引力的手段。因此,使用CUDA环境开发了gpu加速的三维PIC/MCC模拟,以提供大气压氮气中等离子体发展初始阶段的特性。模拟在NVIDIA GTX 580上运行,具有3gb内存和512个CUDA内核。在Dirichlet边界条件下,模拟了两个间隙为5毫米的抛物面电极,并考虑了22种独特的电子与分子氮的相互作用。电极被几千伏特的阶跃电压脉冲激发,同样假设体积中均匀分布的初始电子密度为104 cm-3。例如,5纳秒模拟的结果揭示了阳极和阴极区域附近正离子空间电荷通道的发展。这些通道与等离子体形成期间拍摄的高速流光照片一致。在高电场作用下,电子能量分布函数(EEDF)表现为非麦克斯韦速度分布。此外,阴极附近典型的电子密度约为7 × 108 cm-3。数值模拟的结果将与实验可获得的参数如电子温度和解离度进行详细的比较。
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Study of low-temperature plasma development utilizing a GPU-implemented 3D PIC/MCC simulation
Summary form only given. A GPU-accelerated 3-dimensional PIC/MCC simulation code was developed using the CUDA environment to study the physical processes involved in the development of a low-temperature plasma. The simulation results aid in quantifying transient plasma development as it is often inaccessible experimentally in detail even with modern noninvasive techniques such as non-linear laser spectroscopy or high-speed electrical diagnostics. Hence, computational methods, such as Particle-in-Cell (PIC) and Monte Carlo Collision (MCC), provide a complementary approach to determining the mechanisms leading to plasma development. However, fully modeling the physics of the plasma development is made difficult by the number of plasma processes that must be tracked simultaneously, and only recently have computing resources provided the capability to track tens of millions of particle interactions. Furthermore, the introduction of graphics processing unit (GPU) computing provides an attractive means for economical and efficient parallelization of scientific codes through a framework such as NVIDIA CUDA. As such, a GPU-accelerated 3-dimensional PIC/MCC simulation was developed using the CUDA environment to provide characteristics during the initial stage of plasma development in atmospheric pressure nitrogen. The simulation was run on a NVIDIA GTX 580 with 3 GB of memory and 512 CUDA cores. The simulated geometry consists of two paraboloid electrodes with a gap distance of 5 millimeters with Dirichlet boundary conditions, and 22 unique electron interactions with molecular nitrogen are considered. The electrodes are excited with a step voltage pulse of several thousand volts also assuming a uniformly distributed initial electron density of 104 cm-3 in the volume. For instance, results from a 5 nanosecond simulation reveal the development of positive ion space charge channels near the anode and cathode regions. These channels appear consistent with high-speed streamer photographs captured during plasma formation. The electron energy distribution function (EEDF) indicates a non-Maxwellian velocity distribution during the application of the high electric field. Furthermore, a typical electron density near the cathode is on the order of 7 × 108 cm-3. The results from numerical simulation will be compared in detail to experimentally accessible parameters such as electron temperature and dissociation degree.
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