Davis Sergio, Avaria Gonzalo, Bora Biswajit, Jain Jalaj, Moreno José, Pavez Cristian, Soto Leopoldo
Research Center in the intersection of Plasma Physics, Matter and Complexity (P2mc), Comisión Chilena de Energía Nuclear, Casilla 188-D, Santiago, Chile.
Departamento de Física, Facultad de Ciencias Exactas, Universidad Andres Bello, Sazié 2212, piso 7, 8370136, Santiago, Chile.
Phys Rev E. 2023 Dec;108(6-2):065207. doi: 10.1103/PhysRevE.108.065207.
Kappa-distributed velocities in plasmas are common in a wide variety of settings, from low-density to high-density plasmas. To date, they have been found mainly in space plasmas, but are recently being considered also in the modeling of laboratory plasmas. Despite being routinely employed, the origin of the kappa distribution remains, to this day, unclear. For instance, deviations from the Maxwell-Boltzmann distribution are sometimes regarded as a signature of the nonadditivity of the thermodynamic entropy, although there are alternative frameworks such as superstatistics where such an assumption is not needed. In this work we recover the kappa distribution for particle velocities from the formalism of nonequilibrium steady-states, assuming only a single requirement on the dependence between the kinetic energy of a test particle and that of its immediate environment. Our results go beyond the standard derivation based on superstatistics, as we do not require any assumption about the existence of temperature or its statistical distribution, instead obtaining them from the requirement on kinetic energies. All of this suggests that this family of distributions may be more common than usually assumed, widening its domain of application in particular to the description of plasmas from fusion experiments. Furthermore, we show that a description of kappa-distributed plasma is simpler in terms of features of the superstatistical inverse temperature distribution rather than the traditional parameters κ and the thermal velocity v_{th}.
等离子体中的κ分布速度在从低密度到高密度的各种等离子体环境中都很常见。迄今为止,它们主要在空间等离子体中被发现,但最近在实验室等离子体建模中也受到关注。尽管κ分布已被常规使用,但其起源至今仍不清楚。例如,与麦克斯韦 - 玻尔兹曼分布的偏差有时被视为热力学熵非可加性的标志,尽管存在其他框架,如超统计,其中不需要这样的假设。在这项工作中,我们从非平衡稳态形式中恢复了粒子速度的κ分布,仅对测试粒子的动能与其紧邻环境的动能之间的依赖关系提出了一个要求。我们的结果超越了基于超统计的标准推导,因为我们不需要关于温度存在或其统计分布的任何假设,而是从对动能的要求中得出它们。所有这些表明,这类分布可能比通常假设的更为常见,特别是扩大了其在核聚变实验等离子体描述中的应用范围。此外,我们表明,用超统计逆温度分布的特征来描述κ分布等离子体比用传统参数κ和热速度v_th更简单。