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Relativistic Brownian motion

机译:相对论布朗运动

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Over the past one hundred years, Brownian motion theory has contributed substantiallyto our understanding of various microscopic phenomena. Originally proposed as a phenomenological paradigm for atomistic matter interactions, the theory has since evolved into a broad and vivid research area, with an ever increasing number of applications in biology, chemistry, finance, and physics. The mathematical description of stochastic processes has led to new approaches in other fields, culminating in the path integral formulation of modern quantum theory. Stimulated by experimental progress in high energy physics and astrophysics, the unification of relativistic and stochastic concepts has re-attracted considerable interest during the past decade. Focusing on the framework of special relativity, we review, here, recent progress in the phenomenological description of relativistic diffusion processes. After a brief historical overview, we will summarize basic concepts from the Langevin theory of nonrelativistic Brownian motions and discuss relevant aspects of relativistic equilibrium thermostatistics. The introductory parts are followed by a detailed discussion of relativistic Langevin equations in phase space. We address the choice of time parameters, discretization rules, relativistic fluctuationdissipation theorems, and Lorentz transformations of stochastic differential equations. The general theory is illustrated through analytical and numerical results for the diffusion of free relativistic Brownian particles. Subsequently, we discuss how Langevin-type equations can be obtained as approximations to microscopic models. The final part of the article is dedicated to relativistic diffusion processes in Minkowski spacetime. Since the velocities of relativistic particles are bounded by the speed of light, nontrivial relativistic Markov processes in spacetime do not exist; i.e., relativistic generalizations of the nonrelativistic diffusion equation and its Gaussian solutions must necessarily be non-Markovian. We compare different proposals that were made in the literature and discuss their respective benefits and drawbacks. The review concludes with a summary of open questions, which may serve as a starting point for future investigations and extensions of the theory.
机译:在过去的一百年里,布朗运动理论为我们对各种微观现象的理解做出了重要贡献。该理论最初是作为原子物质相互作用的现象学范式提出的,此后发展成为一个广泛而生动的研究领域,在生物学,化学,金融和物理学领域的应用越来越多。随机过程的数学描述导致了其他领域的新方法,最终形成了现代量子理论的路径积分公式。在高能物理和天体物理学的实验进展的刺激下,相对论和随机概念的统一在过去十年中重新吸引了相当大的兴趣。着眼于狭义相对论的框架,我们在这里回顾了相对论扩散过程的现象学描述方面的最新进展。在简短的历史概述之后,我们将总结非朗格相对布朗运动的兰格文理论的基本概念,并讨论相对论平衡热统计的相关方面。在介绍性部分之后,将详细讨论相空间中的相对论Langevin方程。我们讨论了时间参数,离散化规则,相对论涨落耗散定理和随机微分方程的Lorentz变换的选择。通过解析和数值结果说明了自由相对论布朗粒子的扩散的一般理论。随后,我们讨论如何获得Langevin型方程作为微观模型的近似值。本文的最后一部分致力于Minkowski时空中的相对论扩散过程。由于相对论粒子的速度受光速的限制,因此不存在时空中非平凡的相对论马尔可夫过程。即非相对论扩散方程及其高斯解的相对论概括必须是非马尔可夫的。我们比较了文献中提出的不同建议,并讨论了它们各自的优点和缺点。审查总结了一些未解决的问题,可以作为将来进一步研究和扩展理论的起点。

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