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Titlebook: A Course in Classical Physics 1—Mechanics; Alessandro Bettini Textbook 2016 Springer International Publishing Switzerland 2016 Classical m

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發(fā)表于 2025-3-23 12:01:39 | 只看該作者
,“The Undocumentable Inside of History”,stem and of the galaxies and their clusters as well as the motions of all bodies up to the boundaries of the Universe. We shall include some elements of the historical process that led to the discoveries and reproduce and comment a few relevant pages both of Galilei and of Newton.
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發(fā)表于 2025-3-23 14:37:15 | 只看該作者
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發(fā)表于 2025-3-23 21:30:58 | 只看該作者
Undergraduate Lecture Notes in Physicshttp://image.papertrans.cn/a/image/140452.jpg
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發(fā)表于 2025-3-23 22:32:16 | 只看該作者
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發(fā)表于 2025-3-24 03:27:27 | 只看該作者
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發(fā)表于 2025-3-24 06:41:15 | 只看該作者
https://doi.org/10.1057/9780230118850 the forces are not known. In this chapter we shall study the most important forces, with the exception of gravity, which is the object of next chapter. We shall study the elastic force, the contact forces and the intermolecular force, the friction and the viscous drag. We shall study the mechanical
17#
發(fā)表于 2025-3-24 12:52:39 | 只看該作者
,“The Undocumentable Inside of History”,stem and of the galaxies and their clusters as well as the motions of all bodies up to the boundaries of the Universe. We shall include some elements of the historical process that led to the discoveries and reproduce and comment a few relevant pages both of Galilei and of Newton.
18#
發(fā)表于 2025-3-24 18:11:27 | 只看該作者
19#
發(fā)表于 2025-3-24 20:41:20 | 只看該作者
Renata Arrington Sanders,Jonathan M. EllenIX century Maxwell formulated a set of equations that completely describe all the electromagnetic phenomena. These equations seemed to be in contrast with the relativity principle. The relativity principle was found to be universally valid, but new transformations of coordinates and time, valid betw
20#
發(fā)表于 2025-3-25 00:47:23 | 只看該作者
Khiya Marshall,Nicole Crepaz,Ann O’Learytions with the simplest ones, namely the two-body systems and learn how they interact and discuss a few examples (double stars, tides). We then discuss the experiments on collisions between two pendulums that led Newton to establish the principle of conservation of linear momentum. We then consider
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