Relativistic Dynamics

D. Styer
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引用次数: 35

Abstract

Preface These notes assume that you have a knowledge of space and time in special relativity, and of force, energy, and momentum in classical mechanics (both at the college freshman level). They build on that knowledge to describe force, energy, and momentum in special relativity. These notes also use a few ideas from freshman-level electricity and magnetism, but not in an essential way. The intent is to present physical questions and their direct and straightforward (if laborious) solutions, rather than to show off how mathematically clever the author is. Teaching notes: I use these notes over five or six lectures to college sophomores. On the first day I ask students what they remember about space and time in special relativity. Students are often surprised and gratified that they remember anything about such a counterintuitive subject. Then I present " why we need relativistic dynamics " (section 2.1), followed by one of the two " momentum motivations " , either the collision motivation (sections 2.2, 2.3, and 2.4) or the four-vector motivation (sections 3.1, 3.2 and 3.3). I leave the other motivation for reading. I've tried it both ways and it doesn't seem to make any difference in how well the students learn. In either case I end up interpreting the " new quantity " mc 2 / 1 − (v/c) 2 (section 2.5) in class. In class I present chapters 4 and 6, leaving chapter 5 for reading. It is impossible to overemphasize the fact that mass is not conserved in relativity, which is why I make that point twice (once in section 4.1, again in section 4.2). I end with section 7.1, including working through problem 7.3 (Motion with constant force). This way we end by answering the question we started with, which ties the whole subject together. At this point, students are mentally exhausted: so many new and counterintuitive ideas, so close together. So I have never covered chapters 8 or 9. I just hope that when the students regain their footing they will look back at those two final chapters to learn some things wonderful and profound. Acknowledgment: The discussion of hard-sphere forces in section 9.2 arose from a question by David Carr, a Ph.D. student in computer science at Charles Sturt University in Australia, who was designing a game to teach relativity.
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相对论动力学
这些笔记假设你已经掌握了狭义相对论中的空间和时间知识,以及经典力学中的力、能量和动量知识(都是大学新生的水平)。他们以这些知识为基础来描述狭义相对论中的力、能量和动量。这些笔记也使用了一些新生水平的电学和磁学的概念,但不是必不可少的。其目的是呈现物理问题及其直接和直接(如果费力)的解决方案,而不是炫耀作者在数学上有多聪明。教学笔记:我用这些笔记给大学二年级学生上了五到六堂课。第一天,我问学生在狭义相对论中对空间和时间的记忆。学生们常常感到惊讶和欣慰的是,他们还记得这样一个违反直觉的学科。然后我提出“为什么我们需要相对论动力学”(第2.1节),接着是两个“动量动机”之一,碰撞动机(第2.2、2.3和2.4节)或四矢量动机(第3.1、3.2和3.3节)。我留下了另一个阅读的动机。两种方法我都试过了,但似乎对学生的学习效果没有任何影响。在任何一种情况下,我最终在课堂上解释了“新数量”mc 2 / 1 - (v/c) 2(第2.5节)。在课堂上,我介绍第四章和第六章,留下第五章供阅读。质量在相对论中不守恒这一事实怎么强调都不过分,这就是为什么我两次强调这一点(一次在4.1节,一次在4.2节)。我以7.1节结束,包括解决问题7.3(恒力运动)。这样我们就能回答我们开始时的问题,把整个主题联系在一起。在这一点上,学生们精神疲惫:这么多新的和违反直觉的想法,如此紧密地联系在一起。所以我从来没有讲过第8章和第9章。我只希望当学生们重新站稳脚跟时,他们会回顾这最后两章,学到一些精彩而深刻的东西。致谢:第9.2节中关于硬球力的讨论源于David Carr的一个问题,他是澳大利亚Charles Sturt大学计算机科学专业的博士生,当时正在设计一款教授相对论的游戏。
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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Appendices of Essentials of Quantum Mechanics Summary, Problems and Solutions Appendices of Essentials of Relativity FRONT MATTER BACK MATTER
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