Lecture 3: Experimental measurements ( chpt 5, Feynman)

1. Lecture 3: Experimental measurements(chpt 5, Feynman)

2. Importance of measurements • Physics is an experimental science! Most physicists are experimenters • Measurability is a key part of the sciences • First person who perform quantitative measurement (scientist) is Galileo Galilei (1564-1642) • Most of the Nobel prizes have awarded to invention of instruments • First US Nobel prize winner: Michelson, invention of interferometer!

3. Michelson invented Michelson Interferometer (Nobel prize 1907) • Michelson-Morley Experiment, measured the velocity of earth relative to either.

4. What do you want to measure? • Distance, Time, Speed • Temperature (thermometer), pressure • Weight, mass • Energy, power, noise • Brightness, telescope, • Concentration, blood analysis, • Electromagnetic fields, electric current, resistors, capacitors, etc. • Radioactivity • ….

5. Galileo’s inclined-plane exp. Discovery of laws of physics!!

6. Time measurement • Something that happens again and again • Counting pulse! • Day, hour glass, noon to noon measurement is nearly the same! • Fraction of a day: other periodic motion! • Galileo: pendulum: grand-father clock • Make a pendulum swing 3600 times x24 in a day, each swing is a second!

7. How do you make the time measurement more accurate? • Calibrate the longer period with shorter period • Faster periodic motion: electric current oscillation (electric oscillator) • Accuracy of 10-12 achieved (quartz)

8. Atomic clock and light clock • Atom moves periodically inside the atom. • Atomic clock has been used as a standard for time measurement since 1960’s and is the most accurate devise now available. • Usually radio-wave and has reached accuracy of 10-16 • More accurate measurement needs better frequency measurement, light comb, (light clock) • Jun Ye (JILA), the best guy in the world, 10-18 • Low-temp + relativity

9. Jun Ye, member of US NAS Undergraduate Student from SJTU (1984-1989)

10. Shortest time • Lifetime of the elementary particles • Strong interaction particle 10-24 sec, time it takes from light travel through the proton, atomic nuclei. • Higgs particles life time is very very short. 1.6 X 10-22 sec

11. Longer time • Year, tree rings, river sediment • Radioactivity dating! • 14C dating (5000 yrs) • 开始有人：600 万年 • 238U dating. Life time of the earth and solar system, 40 亿年， • Age of the Universe: 130 亿年. • Longer time, life time of some elementary particles 136Xe lifetime: 1021yrs, I can measure it in my lab! Proton life>1035yrs

12. Distance measurement • Finger span, foot, steps, height…, Sizes related to human being Harvard bridge: xyz Smoots + 1 ear unit +count • Height of a building: triangulization • Height of a mountain

13. Astrophysical measurement • Radius of earth, In the third century B.C., Eratosthenes was able to mathematically calculate the earth’s diameter by comparing differences in the angle of the sun’s rays at two separate geographic points. He noticed that the difference in the angle of a shadow in his location at Syene, which is present-day Aswan in Egypt, and that of a shadow in Alexandria was about 7.2 degrees. Since he knew the distance between the locations, he was able to determine the circumference of the earth, and therefore the diameter and radius as well. You can do this, too, by using his method. Read more : http://www.ehow.com/how_5895686_radius-earth.html how many ways do you know to measure? • Distance to the sun, how many ways? • Distance to moon, laser measurement.

14. Distance to stars • AU=distance to sun • Parallax (par sec = 3 light year) • Color of a star, spheroids • Distance to the center of our Galaxy, 30000 light years. • Using triangulization to measure the distance of other galaxy.

15. Discovering dark energy (Nobel prize, 2012) • Using supernovaeas a standard candle to meaure distance. Saul Perlmutter; Brian P. Schmidt; Adam G. Riess "for the discovery of the accelerating expansion of the Universe through observations of distant supernovae"

16. Smaller distance • Meter, 4x107 m around the equator • Some bar in Paris, now as certain distance that light travels in a certain time. • cm, mm, … • First major improvement: light as a wave!Wavelength is on the order of 500nm! 1nm = 10-9m • Optics experiment, Newton ring, • Michelson interferometer • X-ray determine the size of atom 0.1 nm

17. Even smaller distance • Rutherford experiment found that atoms are quite empty. • He found the size of the nuclei around 10-15m = 1fm • Since then some of the smaller distance measurement done to 10-18m, LHC, large hadron collider • Smallest distance measurement: space oscillation under gravitational wave, 10-22m. If found this is a Nobel prize work!

18. More on measurements • Measuring temperature, • Very hot, very cold • Speed measurement, Light speed, speed of an atom • Measuring magnetic field, electric field SQID, Quantum hall effect • Measuring fundamental constants • Sensors, large data, data processing, information science!

19. Equipment money • A lot of measuring equipment were invented in western world. • Now China is supporting inventing new apparatus, Ministry of science and technology, National Science Foundation of China • A lot of money • One of these at SJTU, 4D electron imaging system.

20. 原子尺度超高时空分辨兆伏特电子衍射与成像系统原子尺度超高时空分辨兆伏特电子衍射与成像系统 王西杰 2013年6月19日

21. 原子尺度物质结构动力学 最高空间分辨的电子衍射与成像技术 最高时间分辨的飞秒泵浦-探测技术 这是目前科学界正在共同追求和探索的目标, 面临着巨大的技术挑战 原子尺度超高时空分辨电子衍射与成像系统 （100fs+Å）

22. 系统总体设计图 系统尺寸：6米x6米x3米 光阴极电子枪 (二)超快泵浦光源 (一)飞秒激光系统 (五)样品室 速 调 管 (六)探测系统 (四)高温超导电磁透镜系统 (三)飞秒高亮度电子源

23. 系统各构成部分及功能 (三)核心设备：兆伏特飞秒高亮度电子源（自主研制） (一)飞秒激光系统（购置改造） （二）超快泵浦光源（研制集成） (五)多功能样品室(购置改造） （四）关键设备：高温超导电磁透镜系统（联合研制） （六）高灵敏探测系统 (与Gatan联合研制）