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具有1/r² 对相互作用的相同粒子随机扰动晶格中的力分布。

Force distribution in a randomly perturbed lattice of identical particles with 1/r2 pair interaction.

作者信息

Gabrielli Andrea, Baertschiger Thierry, Joyce Michael, Marcos Bruno, Labini Francesco Sylos

机构信息

Istituto dei Sistemi Complessi-CNR, Via dei Taurini 19, 00185 Rome, Italy.

出版信息

Phys Rev E Stat Nonlin Soft Matter Phys. 2006 Aug;74(2 Pt 1):021110. doi: 10.1103/PhysRevE.74.021110. Epub 2006 Aug 9.

Abstract

We study the statistics of the force felt by a particle in the class of a spatially correlated distribution of identical pointlike particles, interacting via a 1/r2 pair force (i.e., gravitational or Coulomb), and obtained by randomly perturbing an infinite perfect lattice. We specify the conditions under which the force on a particle is a well-defined stochastic quantity. We then study the small displacements approximation, giving both the limitations of its validity and, when it is valid, an expression for the force variance. The method introduced by Chandrasekhar to find the force probability density function for the homogeneous Poisson particle distribution is extended to shuffled lattices of particles. In this way, we can derive an approximate expression for the probability distribution of the force over the full range of perturbations of the lattice, i.e., from very small (compared to the lattice spacing) to very large where the Poisson limit is recovered. We show in particular the qualitative change in the large-force tail of the force distribution between these two limits. Excellent accuracy of our analytic results is found on detailed comparison with results from numerical simulations. These results provide basic statistical information about the fluctuations of the interactions (i) of the masses in self-gravitating systems like those encountered in the context of cosmological N -body simulations, and (ii) of the charges in the ordered phase of the one-component plasma, the so-called Coulomb or Wigner crystal.

摘要

我们研究了在一类通过1/r²对力(即引力或库仑力)相互作用且由无限完美晶格随机扰动得到的相同点状粒子的空间相关分布中,粒子所受的力的统计特性。我们明确了粒子所受力为定义良好的随机量的条件。然后我们研究了小位移近似,给出了其有效性的限制条件,以及在有效时力方差的表达式。钱德拉塞卡用于求均匀泊松粒子分布的力概率密度函数的方法被扩展到粒子的混洗晶格。通过这种方式,我们可以推导出在晶格的整个扰动范围内,即从非常小(与晶格间距相比)到非常大(此时恢复泊松极限)时力的概率分布的近似表达式。我们特别展示了这两个极限之间力分布的大力尾的定性变化。通过与数值模拟结果的详细比较,发现我们的解析结果具有很高的精度。这些结果提供了关于以下相互作用波动的基本统计信息:(i)在宇宙学N体模拟中遇到的自引力系统中质量的相互作用,以及(ii)单组分等离子体有序相中电荷的相互作用,即所谓的库仑或维格纳晶体。

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