Nobel lecture december 12, 1933 On passing through an optical instrument, such as a telescope or a camera lens, a ray of light is subjec reflecting surface. The path of the rays can be constructed if we know the two simple laws which govern the changes in direction: the law of refrac- tion which was discovered by Snellius a few hundred years ago, and the law of reflection with which Archimedes was familiar more than 2,000 years ago
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Nobel Lecture december 13. 1946 The history of the discovery of the exclusion principle m, for which I have received the honor of the Nobel Prize award in the year 1945, goes back to my students days in Munich. While, in school in Vienna, I had already ob- tained some knowledge of classical physics and the then new Einstein rel- ativity theory, it was at the University of Munich that I was introduced by Sommerfeld to the structure of the atom- somewhat strange from the point of view of classical physics. I was not spared the which every
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The events leading to the discovery of tunnelling supercurrents took place while I was working as a research student at the Royal Society Mond Labo- ratory, Cambridge, under the supervision of Professor Brian Pippard. During my second year as a research student, in 1961-2, we were fortunate to have as a visitor to the laboratory Professor Phil Anderson, who has made numerous
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麦克斯韦最先注意到(也可以从十分简单的计算得出), 当两个点A,B一起移动而不带动附近的以太时,光线从点 A走到点B再返回点A所需的时间一定会不同.当然,这个 差值是个二阶量,但是用灵敏的干涉方法已经足以检测出来。 迈克尔逊于1881年做了这样的实验他的仪器是一种 干涉仪,有两个长度相等并互相垂直的水平臂P和Q.两東 互相干涉的光线,一束沿P臂往返,另一束沿Q臂往返。整个 仪器包括光源和观察装置,可以绕竖直轴转动.当P臂或Q 臂尽可能与地球运动方向相同时的两个位置值得特别考虑 根据菲涅尔理论可以预言,当仪器从一个主位置转到另一个 主位置时,千涉条纹应发生位移 但是,取决于光传播时间改变的这种位移(为简单起见
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第一章广义函数简介 1.1背景知识 函数是古典分析中的基本概念之一,然而这样 的一个基本概念,随着科学的发展已不够用.下 面用几个例子加以说明 例1.1.1(脉冲)20世纪初, Heaviside在解电 路方程时,提出了一种运算方法,称之为算子演 算.这套算法要求对如下函数
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