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Sidney Coleman's Lectures on Relativity最新文献

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Index 指数
Pub Date : 2021-12-31 DOI: 10.1017/9781009053716.015
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引用次数: 0
Compendium of Formulas 公式汇编
Pub Date : 2021-12-31 DOI: 10.1017/9781009053716.013
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引用次数: 0
Differential Geometry 微分几何
Pub Date : 2021-12-31 DOI: 10.1017/9781009053716.008
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引用次数: 0
Conservation and Cosmology 守恒与宇宙学
Pub Date : 2021-12-31 DOI: 10.1017/9781009053716.011
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引用次数: 0
The Geometry of Special Relativity 狭义相对论的几何学
Pub Date : 2021-12-31 DOI: 10.1017/9781009053716.003
N. Dragon
Simple geometric properties of spacetime and free particles underlie the theory of relativity just as Euclidean geometry follows from simple properties of points and straight lines. The vacuum, the empty four-dimensional curved spacetime, determines straight lines and light rays. In the absence of gravity, the vacuum is isotropic and homogeneous and does not allow to distinguish rest from uniform motion. Therefore, contrary to Newton’s opinion, the vacuum cannot contain the information about a universal time which could be attributed to events. Whether two different events are simultaneous depends on the observer – just as in Euclidean geometry it depends on a given direction whether two points lie on an orthogonal line. 1.1 Properties of the Vacuum We can denote a point in space by specifying how far away it is ahead, to the right and to the top of a chosen reference point. These specifications are called coordinates of the point. One needs three coordinates in order to specify any one point. Space is three-dimensional. The coordinates of a point depend of course on the choice of the reference point and on which directions the observer chooses as ahead, right and above. As for appointments in daily life, for physical processes not only the position is important, where an event takes place, but also the time when it occurs. The set of all events, spacetime, is four-dimensional, because to specify a single event one needs four labels, the position where it takes place and the time when it occurs. The position and time specifications which label an event depend – just as the three coordinates of a position – on the observer. The four-dimensional spacetime fascinates and beats our imagination which is trained in everyday life. Nevertheless it is quite simple. We can easily envisage a stack of pictures, as they are stored in a film reel, which show the sequel of threedimensional situations. Thereby one conceives the four-dimensional spacetime the
时空和自由粒子的简单几何特性是相对论的基础,正如欧几里得几何是由点和直线的简单特性推导出来的一样。真空,空旷的四维弯曲时空,决定了直线和光线。在没有重力的情况下,真空是各向同性和均匀的,不允许区分静止和均匀运动。因此,与牛顿的观点相反,真空不可能包含可以归因于事件的关于普遍时间的信息。两个不同的事件是否同时发生取决于观察者——就像在欧几里得几何中两点是否在一条正交线上取决于给定的方向一样。我们可以通过指定一个参考点的前方、右侧和顶部的距离来表示空间中的一个点。这些规格称为点的坐标。我们需要三个坐标来确定任意一点。空间是三维的。当然,点的坐标取决于参考点的选择以及观察者选择的方向(前方、右侧和上方)。至于日常生活中的约会,对于物理过程来说,重要的不仅是事件发生的位置,还有事件发生的时间。所有事件的集合,即时空,是四维的,因为要指定一个单一事件,需要四个标签,即它发生的位置和发生的时间。标记事件的位置和时间规格取决于观察者——就像位置的三个坐标一样。四维时空令人着迷,超越了我们在日常生活中训练的想象力。然而,这是相当简单的。我们可以很容易地想象一叠照片,就像它们被存储在电影卷轴里一样,它们显示了三维情况的续集。因此,人们认为四维时空是
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引用次数: 0
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Sidney Coleman's Lectures on Relativity
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