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具有任意范围相互作用的一维经典海森堡模型:李雅普诺夫指数以及动量和能量分布

-Dimensional Classical Heisenberg Model with Arbitrarily-Ranged Interactions: Lyapunov Exponents and Distributions of Momenta and Energies.

作者信息

Rodríguez Antonio, Nobre Fernando D, Tsallis Constantino

机构信息

GISC, Departamento de Matemática Aplicada a la Ingeniería Aeroespacial, Universidad Politécnica de Madrid, Plaza Cardenal Cisneros s/n, 28040 Madrid, Spain.

Department of Physics, University of Warwick, Coventry CV4 7AL, UK.

出版信息

Entropy (Basel). 2019 Jan 4;21(1):31. doi: 10.3390/e21010031.

DOI:10.3390/e21010031
PMID:33266747
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC7514134/
Abstract

We numerically study the first-principle dynamics and thermostatistics of a -dimensional classical inertial Heisenberg ferromagnetic model ( d = 1 , 2 , 3 ) with interactions decaying with the distance r i j as 1 / r i j α ( α ≥ 0 ), where the limit α = 0 ( α → ∞ ) corresponds to infinite-range (nearest-neighbour) interactions, and the ratio α / d > 1 ( 0 ≤ α / d ≤ 1 ) characterizes the short-ranged (long-ranged) regime. By means of first-principle molecular dynamics we study: (i) The scaling with the system size N of the maximum Lyapunov exponent λ in the form λ ∼ N - κ , where κ ( α / d ) depends only on the ratio α / d ; (ii) The time-averaged single-particle angular momenta probability distributions for a typical case in the long-range regime 0 ≤ α / d ≤ 1 (which turns out to be well fitted by -Gaussians), and (iii) The time-averaged single-particle energies probability distributions for a typical case in the long-range regime 0 ≤ α / d ≤ 1 (which turns out to be well fitted by -exponentials). Through the Lyapunov exponents we observe an intriguing, and possibly size-dependent, persistence of the non-Boltzmannian behavior even in the α / d > 1 regime. The universality that we observe for the probability distributions with regard to the ratio α / d makes this model similar to the α -XY and α -Fermi-Pasta-Ulam Hamiltonian models as well as to asymptotically scale-invariant growing networks.

摘要

我们对一维经典惯性海森堡铁磁模型((d = 1,2,3))的第一性原理动力学和热统计学进行了数值研究,其相互作用随距离(r_{ij})以(1 / r_{ij}^{\alpha})((\alpha \geq 0))衰减,其中(\alpha = 0)((\alpha \to \infty))的极限对应于无限范围(最近邻)相互作用,且(\alpha / d > 1)((0 \leq \alpha / d \leq 1))的比值表征短程(长程) regime。通过第一性原理分子动力学,我们研究:(i)最大李雅普诺夫指数(\lambda)随系统大小(N)的标度形式为(\lambda \sim N^{-\kappa}),其中(\kappa(\alpha / d))仅取决于(\alpha / d)的比值;(ii)长程 regime (0 \leq \alpha / d \leq 1)中典型情况下的时间平均单粒子角动量概率分布(结果发现由 -高斯分布很好地拟合),以及(iii)长程 regime (0 \leq \alpha / d \leq 1)中典型情况下的时间平均单粒子能量概率分布(结果发现由 -指数分布很好地拟合)。通过李雅普诺夫指数,我们观察到即使在(\alpha / d > 1) regime中,非玻尔兹曼行为也存在一种有趣的、可能与尺寸有关的持续性。我们观察到的概率分布关于(\alpha / d)比值的普适性使得该模型类似于(\alpha - XY)和(\alpha - Fermi - Pasta - Ulam)哈密顿模型以及渐近尺度不变增长网络。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e841/7514134/52222839fe4f/entropy-21-00031-g009.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e841/7514134/af49f628070f/entropy-21-00031-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e841/7514134/29e4a7711222/entropy-21-00031-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e841/7514134/0ce0ddd54468/entropy-21-00031-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e841/7514134/a733074cd8a1/entropy-21-00031-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e841/7514134/2aceddc293d5/entropy-21-00031-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e841/7514134/e4bfd88710fe/entropy-21-00031-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e841/7514134/1810d2b1a6f3/entropy-21-00031-g007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e841/7514134/02c784f119bf/entropy-21-00031-g008.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e841/7514134/52222839fe4f/entropy-21-00031-g009.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e841/7514134/af49f628070f/entropy-21-00031-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e841/7514134/29e4a7711222/entropy-21-00031-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e841/7514134/0ce0ddd54468/entropy-21-00031-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e841/7514134/a733074cd8a1/entropy-21-00031-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e841/7514134/2aceddc293d5/entropy-21-00031-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e841/7514134/e4bfd88710fe/entropy-21-00031-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e841/7514134/1810d2b1a6f3/entropy-21-00031-g007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e841/7514134/02c784f119bf/entropy-21-00031-g008.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e841/7514134/52222839fe4f/entropy-21-00031-g009.jpg

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