Special Relativity

D. Hogg
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Abstract

References 43 Index 45 ii Preface For me, the wonder of special relativity lies in its successful prediction of interesting and very nonintuitive phenomena from simple arguments with simple premises. These notes have three (perhaps ambitious) aims: (a) to introduce undergraduates to special relativity from its founding principle to its varied consequences, (b) to serve as a reference for those of us who need to use special relativity regularly but have no long-term memory, and (c) to provide an illustration of the methods of theoretical physics for which the elegance and simplicity of special relativity are ideally suited. History is a part of all science—I will mention some of the relevant events in the development of special relativity—but there is no attempt to present the material in a historical way. A common confusion for students of special relativity is between that which is real and that which is apparent. For instance, length contraction is often mistakenly thought to be some optical illusion. But moving things do not " appear " shortened, they actually are shortened. How they appear depends on the particulars of the observation , including distance to the observer, viewing angles, times, etc. The observer finds that they are shortened only after correcting for these non-fundamental details of the observational procedure. I attempt to emphasize this distinction: All apparent effects, including the Doppler Shift, stellar aberration, and superluminal motion, are relegated to Chapter 7. I think these are very important aspects of special relativity, but from a pedagogical standpoint it is preferable to separate them from the ba-sics, which are not dependent on the properties of the observer. I love the description of special relativity in terms of frame-independent, geometric objects, such as scalars and 4-vectors. These are introduced in Chapter 6 and used thereafter. But even before this, the geometric properties of spacetime are emphasized. Most problems can be solved with a minimum of algebra; this is one of the many beautiful aspects of the subject. These notes, first written while teaching sections of first-year physics at Caltech, truly represent a work in progress. I strongly encourage all readers to give me comments on any aspect of the text * ; all input is greatly appreciated. Thank you very much.
狭义相对论
对我来说,狭义相对论的奇妙之处在于,它用简单的前提和简单的论证,成功地预言了有趣而又非常不直观的现象。这些笔记有三个(也许是雄心勃勃的)目的:(a)向本科生介绍狭义相对论,从它的建立原理到它的各种结果;(b)为我们这些需要经常使用狭义相对论但没有长期记忆的人提供参考;(c)提供理论物理方法的说明,这些方法非常适合狭义相对论的优雅和简单。历史是所有科学的一部分——我将提到狭义相对论发展过程中的一些相关事件——但没有试图以历史的方式呈现这些材料。对于狭义相对论的学生来说,一个常见的困惑是什么是真实的,什么是明显的。例如,长度收缩经常被误认为是某种视觉错觉。但是移动的东西并不是“看起来”缩短了,它们实际上是缩短了。它们如何出现取决于观察的细节,包括与观察者的距离、观察角度、时间等。观测者发现,只有在纠正了观测过程中的这些非基本细节之后,它们才会缩短。我试图强调这一区别:所有明显的效应,包括多普勒频移、恒星像差和超光速运动,都归到第七章。我认为这些是狭义相对论非常重要的方面,但从教学的角度来看,最好将它们与不依赖于观察者属性的物理分离开来。我喜欢用与框架无关的几何对象来描述狭义相对论,比如标量和4向量。这些将在第6章中介绍并在之后使用。但即使在此之前,时空的几何性质也被强调了。大多数问题可以用最少的代数来解决;这是这门学科众多美好的方面之一。这些笔记最初是在加州理工学院教授一年级物理课时写的,真正代表了一项正在进行的工作。我强烈鼓励所有读者对本文的任何方面提出意见*;非常感谢所有的输入。非常感谢。
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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