Non-Equilibrium Turbulent Processes in Plasmas

瑞利-泰勒不稳定性和湍流混合控制着自然界和技术中各种各样的等离子体现象，跨越天体物理到微观尺度和低到高能量密度区域。它影响惯性约束聚变中“热点”的形成，限制内爆Z箍缩的径向压缩，驱动恒星喷出物穿透脉冲星风星云，主导核心坍缩超新星中的能量传输，为热核恒星闪光中重质量元素的合成提供条件，控制高应变率下的物质转化，并强烈影响冲击波和爆炸波的动力学。当不同密度的物质（等离子体）逆着密度梯度加速时，瑞利-泰勒不稳定性就会发展。诱导的材料混合是一个复杂的（各向异性，非均匀和统计不稳定）的湍流过程，其理论描述需要新的方法，远远超出了理想化的正则考虑域。近年来在高能量密度等离子体实验和大尺度数值模拟方面取得的巨大成功，以及瑞利-泰勒混合在不同物理状态下的惊人相似性，使得这一理论的出现和等离子体非平衡湍流过程基本方面的知识的发展成为可能。动量损失率的不变性。这个概念将被应用到捕获的质量，动量和能量的瑞利-泰勒混合等离子体的运输和研究不变量，尺度耦合，缩放，和统计的湍流过程。群论和随机分析的考虑将被采用，和连贯性和随机性的动态将被分析和相关的守恒定律的时空对称性。阐明了高能量密度条件下，等离子体混合的积分特性的依赖关系将被调查，并将建立它们的连接到模拟和实验的控制参数（例如，在高功率激光实验中的目标非均匀性）。开发的理论基础将进一步应用于分析现有的数据集，并推进实验和模拟的设计。该项目将影响科学，数学和工程领域的广泛学科，包括等离子体，高能量密度物理学，天体物理学，数学物理学，随机过程，流体动力学和材料科学，以及核能和通信领域的技术。它还将启动一个关于现代理论建模方法和先进数据分析技术的研究生教育新计划。理论工具将通过一个新兴的国际研究社区“湍流混合及其他”的发展进行交流并做出贡献。'

Rayleigh-Taylor instability and turbulent mixing governs a wide variety of plasma phenomena in nature and technology, spanning astrophysical to microscopic scales and low to high energy density regimes. It influences the formation of the 'hot spot' in inertial confinement fusion, limits radial compression of imploding Z-pinches, drives penetration of stellar ejecta into pulsar wind nebula, dominates energy transport in core-collapse supernova, provides conditions for synthesis of heavy mass elements in thermonuclear stellar flashes, controls material transformation under high strain rates, and strongly affects the dynamics of shocks and blast waves. Rayleigh-Taylor instability develops when matters (plasmas) of different densities are accelerated against the density gradients. The induced material mixing is a complex (anisotropic, inhomogeneous and statistically unsteady) turbulent process, whose theoretical description requires novel approaches that go well beyond the domain of idealized canonical considerations. The tremendous successes achieved recently in high energy density plasma experiments and in large-scale numerical simulations, and the striking similarity of behavior of Rayleigh-Taylor mixing in vastly different physical regimes make this moment right for a theory to appear and to advance knowledge of fundamental aspects of the non-equilibrium turbulent processes in plasmas.The core of this theoretical approach is a new concept, the invariance of the rate of momentum loss. This concept will be applied to capture the transports of mass, momentum and energy in Rayleigh-Taylor mixing plasmas and to study invariants, scale coupling, scaling, and statistics of the turbulent process. Group theory and stochastic analysis considerations will be employed, and coherence and randomness of the dynamics will be analyzed and related to space-time symmetries of the conservation laws. Incorporating the high energy density conditions, the dependencies of integral characteristics of plasma mixing will be investigated and their connection will be established to the control parameters of simulations and experiments (e.g. target non-uniformities in high-power laser experiments). The developed theoretical foundations will be further applied to analyze existing datasets and to advance the design of experiments and simulations. The project will impact a broad range of disciplines in science, mathematics and engineering, including plasmas, high energy density physics, astrophysics, mathematical physics, stochastic processes, fluid dynamics, and material science, as well as technology in the areas of nuclear energy and communications. It will also initiate a new program for graduate education on modern methods of theoretical modeling and advanced data analysis techniques. The theoretical tools will be communicated through and contribute to the development of a newly emerging international research community 'Turbulent mixing and beyond.'