Preface to the Second Edition

R. Marcus, J. Sweetenham, Michael E. Williams
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引用次数: 1

Abstract

This textbook introduces the main principles of computational physics, which include numerical methods and their application to the simulation of physical systems. The first edition was based on a one-year course in computational physics where I presented a selection of only the most important methods and applications. Approximately one-third of this edition is new. I tried to give a larger overview of the numerical methods, traditional ones as well as more recent developments. In many cases it is not possible to pin down the “best” algorithm, since this may depend on subtle features of a certain application, the general opinion changes from time to time with new methods appearing and computer architectures evolving, and each author is convinced that his method is the best one. Therefore I concentrated on a discussion of the prevalent methods and a comparison for selected examples. For a comprehensive description I would like to refer the reader to specialized textbooks like “Numerical Recipes” or elementary books in the field of the engineering sciences. The major changes are as follows. A new chapter is dedicated to the discretization of differential equations and the general treatment of boundary value problems. While finite differences are a natural way to discretize differential operators, finite volume methods are more flexible if material properties like the dielectric constant are discontinuous. Both can be seen as special cases of the finite element methods which are omnipresent in the engineering sciences. The method of weighted residuals is a very general way to find the “best” approximation to the solution within a limited space of trial functions. It is relevant for finite element and finite volume methods but also for spectral methods which use global trial functions like polynomials or Fourier series. Traditionally, polynomials and splines are very often used for interpolation. I included a section on rational interpolation which is useful to interpolate functions with poles but can also be an alternative to spline interpolation due to the recent development of barycentric rational interpolants without poles. The chapter on numerical integration now discusses Clenshaw-Curtis and Gaussian methods in much more detail, which are important for practical applications due to their high accuracy.
第二版序言
本书介绍了计算物理学的主要原理,包括数值方法及其在物理系统模拟中的应用。第一版是基于一年的计算物理课程,我只介绍了最重要的方法和应用。这个版本大约有三分之一是新的。我试图给数值方法一个更大的概述,传统的以及最近的发展。在许多情况下,确定“最佳”算法是不可能的,因为这可能取决于特定应用程序的细微特征,随着新方法的出现和计算机体系结构的发展,一般的观点会不时改变,每个作者都相信自己的方法是最好的。因此,我集中讨论了流行的方法,并对选定的例子进行了比较。为了获得全面的描述,我想让读者参考像“数值食谱”这样的专业教科书或工程科学领域的基础书籍。主要变化如下。新的一章专门讨论微分方程的离散化和边值问题的一般处理。虽然有限差分是离散微分算子的一种自然方法,但如果介质常数等材料性质是不连续的,有限体积方法则更加灵活。两者都可以看作是工程科学中普遍存在的有限元方法的特例。加权残差法是在有限的试验函数空间内找到解的“最佳”近似值的一种非常通用的方法。它不仅适用于有限元和有限体积方法,也适用于使用多项式或傅立叶级数等全局试函数的谱方法。传统上,多项式和样条常用于插值。我包含了一个关于有理插值的部分,它对带极点的插值函数很有用,但由于最近发展了无极点的质心有理插值,它也可以作为样条插值的替代方法。数值积分这一章现在更详细地讨论了克伦肖-柯蒂斯和高斯方法,它们由于精度高而对实际应用很重要。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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