《力学 MECHANICS》课程学习资料:Four golden lessons-Weinberg

concepts Four golden lessons Scientist york of many theoretical and Advice to students at the start of Steven Weiber physicists has been able to sort it out, and their scientific careers We en I received my undergraduate put everything(well, almost everything legree - about a hundred years together in a beautiful theory known as ago the physics literature the standard model. My advice is to go for the to spending most of your time not being seemed to me a vast, unexplored ocean, messes- s where the action is creative,to being becalmed on the ocean of very part of which I had to chart before My third piece of advice is probably the scientificknowledge phing about the his ould I do anything without knowing wasting time. Students are only asked to af inally, learn something about the hiss s eginning any research of my own. How hardest to take. It is to forgive yourself for cience, orat a minimum the history of you everything that had already been done? solve problems that their professors(unless own branch of science. The least important Fortunately, in my first year of graduate unusually cruel)know to be solvable. In reason for this is that the history may actually school, I had the good luck to fall into the addition, t doesn'tmatterif the problems are be of some use to you in your own scientific hands of senior physicists who insisted, over scientifically important -they have to be work. For instance, now and then scientist my anxious objections, that I must start solved to pass the course. But in the real are hampered by believing one of the over- doing research, and pick up what I needed world, it's very hard to know which problems mplified models of science that have to know as I went along. It was sink or are important, and you never know whether been proposed by philosophers from Francis swim.To my surprise, I found that this at a given moment in history a problem is Bacon to Thomas Kuhn and Karl Popper works. I managed to get a quick. PhD solvable. At the beginning of the twentieth The best antidote to the philosophy of science though when I got it I knew almost nothing century, several leading physicists, including isaknowledge of the history of science about physics. But I did learn one big Lorentz and Abraham, were trying to work More importantly, the history of science thing: that no one knows everything, and out a theory of the electron. This was partly can make your work seem more worthwhile ou dont have order to understand why all attempts to As a scientist, you're probably not Another lesson to be learned, to continue detect effects of Earth,'s motion through the get rich. Your friends and relatives using my oceanographic metaphor, is that ether had failed. We now know that wont understand what you're while you are swimming and not sinking you they were working on the wrong problem. doing. And if you work in a field like elemen should aim for rough water. When I was At that time, no one could have developed a tary particle physics, you wont even have the teaching at the Massachusetts Institute of successful theory of the electron, because satisfaction of doing something that is Technology in the late 1960s, a student told quantum mechanics had not yet been immediately useful. But you can get great me that he wanted to go into general discovered. It took the genius of Albert satisfaction by recognizing that your work in relativity rather than the area I was working Einstein in 1905 to realize that the right science is a part of history on, elementary particle physics, because problem on which to work was the effect Look back 100 years, to 1903. How the principles of the former were well of motion on measurements of space and rtant is it now who was prime minister known, while the latter seemed like a mess time. This led him to the special theory of of Great Britain in 1903, or President of the to him. It struck me that he had just given relativity. As you will never be sure which United States? What stands out as really a perfectly good reason for doing the oppo- are the right problems to work on, most important is that at McGill University, site. Particle physics was an area where of the time that you spend in the laboratory Ernest Rutherford and Frederick Soddy were creative work could still be done. It really was or at your desk will be wasted. If you want working out the nature of radioactivity a mess in the 1960s, but since that time the to be creative, then you will have to get used This work (of course! ) had practical applica tions, but much more important were its cultural implications. The understanding of radioactivity allowed physicists to explain how the Sun and earth,'s cores could still be hot after millions of years. In this way, it emoved the last scientific objection to what thought was the great age of the Earth and the Sun. After this, Christians and Jews either had to give up belief in the literal truth of the Bible or resign themselves to intellectual irrelevance. This was just one step in a sequence of steps from Galileo through Newton and Darwin to the present that, time after time, has weakened the hold of religious dogmatism. Reading any newspaper nowa days is enough to show you that this work f which scientists are able to feel proud. B Steven Weinberg is in the Department of Physics, the University of Texas at Austin, Texas 78712, USA. This essay is based on a commencement talk Dive right in: exploring the unclear, uncharted areas of science can lead to creative work. given by the author at the Science Convocation at McGill University in June 2003. NatuRevOl42627NovEmber2003www.nature.com/nature 389 @2003 Nature Publishing Group
Steven Weinberg When I received my undergraduate degree — about a hundred years ago — the physics literature seemed to me a vast, unexplored ocean, every part of which I had to chart before beginning any research of my own. How could I do anything without knowing everything that had already been done? Fortunately, in my first year of graduate school, I had the good luck to fall into the hands of senior physicists who insisted, over my anxious objections, that I must start doing research, and pick up what I needed to know as I went along. It was sink or swim. To my surprise, I found that this works. I managed to get a quick PhD — though when I got it I knew almost nothing about physics. But I did learn one big thing: that no one knows everything, and you don’t have to. Another lesson to be learned, to continue using my oceanographic metaphor, is that while you are swimming and not sinking you should aim for rough water. When I was teaching at the Massachusetts Institute of Technology in the late 1960s, a student told me that he wanted to go into general relativity rather than the area I was working on, elementary particle physics, because the principles of the former were well known, while the latter seemed like a mess to him. It struck me that he had just given a perfectly good reason for doing the opposite. Particle physics was an area where creative work could still be done.It really was a mess in the 1960s, but since that time the work of many theoretical and experimental physicists has been able to sort it out, and put everything (well, almost everything) together in a beautiful theory known as the standard model.My advice is to go for the messes — that’s where the action is. My third piece of advice is probably the hardest to take. It is to forgive yourself for wasting time. Students are only asked to solve problems that their professors (unless unusually cruel) know to be solvable. In addition,it doesn’t matter if the problems are scientifically important — they have to be solved to pass the course. But in the real world,it’s very hard to know which problems are important, and you never know whether at a given moment in history a problem is solvable. At the beginning of the twentieth century, several leading physicists, including Lorentz and Abraham, were trying to work out a theory of the electron. This was partly in order to understand why all attempts to detect effects of Earth’s motion through the ether had failed. We now know that they were working on the wrong problem. At that time, no one could have developed a successful theory of the electron, because quantum mechanics had not yet been discovered. It took the genius of Albert Einstein in 1905 to realize that the right problem on which to work was the effect of motion on measurements of space and time. This led him to the special theory of relativity. As you will never be sure which are the right problems to work on, most of the time that you spend in the laboratory or at your desk will be wasted. If you want to be creative, then you will have to get used concepts NATURE|VOL 426 | 27 NOVEMBER 2003 |www.nature.com/nature 389 to spending most of your time not being creative, to being becalmed on the ocean of scientific knowledge. Finally, learn something about the history of science,or at a minimum the history of your own branch of science. The least important reason for this is that the history may actually be of some use to you in your own scientific work. For instance, now and then scientists are hampered by believing one of the oversimplified models of science that have been proposed by philosophers from Francis Bacon to Thomas Kuhn and Karl Popper. The best antidote to the philosophy of science is a knowledge of the history of science. More importantly, the history of science can make your work seem more worthwhile to you. As a scientist, you’re probably not going to get rich. Your friends and relatives probably won’t understand what you’re doing.And if you work in a field like elementary particle physics, you won’t even have the satisfaction of doing something that is immediately useful. But you can get great satisfaction by recognizing that your work in science is a part of history. Look back 100 years, to 1903. How important is it now who was Prime Minister of Great Britain in 1903, or President of the United States? What stands out as really important is that at McGill University, Ernest Rutherford and Frederick Soddy were working out the nature of radioactivity. This work (of course!) had practical applications, but much more important were its cultural implications. The understanding of radioactivity allowed physicists to explain how the Sun and Earth’s cores could still be hot after millions of years. In this way, it removed the last scientific objection to what many geologists and paleontologists thought was the great age of the Earth and the Sun.After this,Christians and Jews either had to give up belief in the literal truth of the Bible or resign themselves to intellectual irrelevance. This was just one step in a sequence of steps from Galileo through Newton and Darwin to the present that,time after time,has weakened the hold of religious dogmatism. Reading any newspaper nowadays is enough to show you that this work is not yet complete. But it is civilizing work, of which scientists are able to feel proud. ■ Steven Weinberg is in the Department of Physics, the University of Texas at Austin, Texas 78712, USA. This essay is based on a commencement talk given by the author at the Science Convocation at McGill University in June 2003. Four golden lessons Scientist Advice to students at the start of their scientific careers. Dive right in: exploring the unclear, uncharted areas of science can lead to creative work. USA/NETWORKS/KOBAL COLLECTION/R. FOREMAN 27.11 concepts 21/11/03 5:02 pm Page 1 © 2003 NaturePublishingGroup

Copyright of Nature is the property of Nature Publishing Group and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use
按次数下载不扣除下载券;
注册用户24小时内重复下载只扣除一次;
顺序:VIP每日次数-->可用次数-->下载券;
- 北京大学:《力学 MECHANICS》精品课程教学大纲.doc
- 西安建筑科技大学:《流体力学 Fluid Dynamics》精品课程习题作业.pdf
- 西安建筑科技大学:《流体力学 Fluid Dynamics》精品课程教学大纲(40学时).pdf
- 西安建筑科技大学:《流体力学 Fluid Dynamics》精品课程教学大纲(72学时).pdf
- 西安建筑科技大学:《流体力学 Fluid Dynamics》精品课程教学大纲(88学时).pdf
- 西安建筑科技大学:《流体力学 Fluid Dynamics》课程教学实验_明渠流综合实验.pdf
- 西安建筑科技大学:《流体力学 Fluid Dynamics》课程教学实验_雷诺实验.pdf
- 西安建筑科技大学:《流体力学 Fluid Dynamics》课程教学实验_空气流动综合实验.pdf
- 西安建筑科技大学:《流体力学 Fluid Dynamics》课程教学实验_动量方程验证实验.pdf
- 西安建筑科技大学:《流体力学 Fluid Dynamics》课程教学实验_静水压力实验.pdf
- 西安建筑科技大学:《结构力学》精品课程教学资源(试卷习题)典型习题.doc
- 西安建筑科技大学:《材料力学》课程教学实验指导书.doc
- 西安建筑科技大学:《材料力学》课程部分试卷及答案_材料力学下(二)答案.doc
- 西安建筑科技大学:《材料力学》课程部分试卷及答案_材料力学下(二).doc
- 西安建筑科技大学:《材料力学》课程部分试卷及答案_材料力学下(一)答案.doc
- 西安建筑科技大学:《材料力学》课程部分试卷及答案_材料力学下(一).doc
- 西安建筑科技大学:《材料力学》课程部分试卷及答案_材料力学上(二)答案.doc
- 西安建筑科技大学:《材料力学》课程部分试卷及答案_材料力学上(二).doc
- 西安建筑科技大学:《材料力学》课程部分试卷及答案_材料力学上(一)答案.doc
- 西安建筑科技大学:《材料力学》课程部分试卷及答案_材料力学上(一).doc
- 《力学 MECHANICS》课程学习资料:Toy models for the falling chimney.pdf
- 《力学 MECHANICS》课程学习资料:laboratory test of Newton's Second law for small accelerations.pdf
- 《力学 MECHANICS》课程学习资料:Nanofabrication of a two-dimensional array using laser-focused atomic deposition.pdf
- 北京大学:《力学 MECHANICS》精品课程试卷_2006年力学期末考试试卷及答案.pdf
- 北京大学:《力学 MECHANICS》课程PPT教学课件_第零章 数学补充知识(刘树新).ppt
- 北京大学:《力学 MECHANICS》课程PPT教学课件_第一章 质点运动学.ppt
- 北京大学:《力学 MECHANICS》课程PPT教学课件_第二章 牛顿定律、动量定理.ppt
- 北京大学:《力学 MECHANICS》课程PPT教学课件_第三章 机械能定理 §3.1 动能定理 §3.2 保守力与势能 §3.3 机械能定理 §3.4 碰撞.ppt
- 北京大学:《力学 MECHANICS》课程PPT教学课件_第五章 质心、刚体 5.1 质心 5.2 刚体定轴转动 5.3 刚体平面平行运动 5.4 刚体定点转动、刚体平衡.ppt
- 北京大学:《力学 MECHANICS》课程PPT教学课件_第四章 角动量定理、天体运动 §4.1 角动量定理 §4.2 对称性与守恒律 §4.3 天体运动.ppt
- 北京大学:《力学 MECHANICS》课程PPT教学课件_第七章 振动和波(共八小节).ppt
- 北京大学:《力学 MECHANICS》课程PPT教学课件_第六章 流体 §6.1 流体静力学 §6.2 流体运动学和质量守恒 §6.3 理想流体的定常流动 §6.4 粘滞流体的流动.ppt
- 北京大学:《力学 MECHANICS》课程PPT教学课件_第八章 狭义相对论.ppt
- 《材料力学》PPT电子教案:第一章 绪论.pps
- 浙江大学:《材料力学》课程教学资源(PPT课件讲稿)第一章 绪论(Preface).ppt
- 《现代连续介质力学理论及实践》参考资料:郭仲衡著《张量(理论和应用)》.pdf
- 《现代连续介质力学理论及实践》参考资料:郭仲衡《理性力学简介》(北京大学数学力学系).pdf
- 《现代连续介质力学理论及实践》参考资料:郭仲衡《积极开展理性力学的研究》(北京大学数学力学系).pdf
- 《现代连续介质力学理论及实践》参考资料:《力学丛书》郭仲衡著《非线性弹性力学》(共七章).pdf
- 《现代连续介质力学理论及实践》参考资料:谢道夫《连续介质力学的发展方向和问题》.pdf