Electron-A Main Actor in Scientific Controversies
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Infrared Spectra of Noble Gases (12000 to 19000 Ar Curtis 1
Journal of Research of the Nationa l Bureau of Sta ndards Vol. 49, No. 2, August 1952 Resea rch Paper 2345 Infrared Spectra of Noble Gases (12000 to 19000 Ar Curtis 1. Humphreys and Henry 1. Kostkowski . The first spectra of heliUl.n, neon, argon, krypton, and xe non, excited by discharges in gelssler t ubes, operated by direct connection to a transformer, have been explored in the ll1frared (1 2090 to 19000 A) . A hi~h-reso lu t.i o n , automatically recording, infrared spec trom eter, emploYlllg a. 15009-h~ es -p e r-lllch gratlllg and lead-sulfi de photocond ucting detector, was used as t he dlspersmg mstrument. A new set of wavelength values is reported for all t hese spectra. New data include 18 pre viously unreported lines of neon and 36 of krypton all of which have been. classified . .~h e descriptions of t he spectra of argon, krypton, and xe non represent essent ially a repetit IOn of t he observations of Sitt ner and Peck. Several prev io~ s l y missing classificat ions a re supplied, also a few amended interpretat ions. The analysIs of t hese spectra m ay be regarded as complete. Use of selected lines as wavelength standards is suggested., 1. Introduction mocouple detector were reported by Humphreys and Plyler [2] . These observations covered the same The essentially complete character of both the spec tral region in which the data herein reported were d escription and interpretation of th e photographed obtained, but, because of well-known limitations af spec tra of the noble atmospheric gases makes it fecting the precision of spectral data obtained by apparent that any reopening of th e subject can be prism spec trometers with thermal detectors, may be justified only on the basis of th e availability of new' considered as en tirely sup erseded by the presen t sources of information, such as a new technique of work. -
Nikola Tesla
Nikola Tesla Nikola Tesla Tesla c. 1896 10 July 1856 Born Smiljan, Austrian Empire (modern-day Croatia) 7 January 1943 (aged 86) Died New York City, United States Nikola Tesla Museum, Belgrade, Resting place Serbia Austrian (1856–1891) Citizenship American (1891–1943) Graz University of Technology Education (dropped out) ‹ The template below (Infobox engineering career) is being considered for merging. See templates for discussion to help reach a consensus. › Engineering career Electrical engineering, Discipline Mechanical engineering Alternating current Projects high-voltage, high-frequency power experiments [show] Significant design o [show] Awards o Signature Nikola Tesla (/ˈtɛslə/;[2] Serbo-Croatian: [nǐkola têsla]; Cyrillic: Никола Тесла;[a] 10 July 1856 – 7 January 1943) was a Serbian-American[4][5][6] inventor, electrical engineer, mechanical engineer, and futurist who is best known for his contributions to the design of the modern alternating current (AC) electricity supply system.[7] Born and raised in the Austrian Empire, Tesla studied engineering and physics in the 1870s without receiving a degree, and gained practical experience in the early 1880s working in telephony and at Continental Edison in the new electric power industry. He emigrated in 1884 to the United States, where he became a naturalized citizen. He worked for a short time at the Edison Machine Works in New York City before he struck out on his own. With the help of partners to finance and market his ideas, Tesla set up laboratories and companies in New York to develop a range of electrical and mechanical devices. His alternating current (AC) induction motor and related polyphase AC patents, licensed by Westinghouse Electric in 1888, earned him a considerable amount of money and became the cornerstone of the polyphase system which that company eventually marketed. -
Wave Nature of Matter: Made Easy (Lesson 3) Matter Behaving As a Wave? Ridiculous!
Wave Nature of Matter: Made Easy (Lesson 3) Matter behaving as a wave? Ridiculous! Compiled by Dr. SuchandraChatterjee Associate Professor Department of Chemistry Surendranath College Remember? I showed you earlier how Einstein (in 1905) showed that the photoelectric effect could be understood if light were thought of as a stream of particles (photons) with energy equal to hν. I got my Nobel prize for that. Louis de Broglie (in 1923) If light can behave both as a wave and a particle, I wonder if a particle can also behave as a wave? Louis de Broglie I’ll try messing around with some of Einstein’s formulae and see what I can come up with. I can imagine a photon of light. If it had a “mass” of mp, then its momentum would be given by p = mpc where c is the speed of light. Now Einstein has a lovely formula that he discovered linking mass with energy (E = mc2) and he also used Planck’s formula E = hf. What if I put them equal to each other? mc2 = hf mc2 = hf So for my photon 2 mp = hfhf/c/c So if p = mpc = hfhf/c/c p = mpc = hf/chf/c Now using the wave equation, c = fλ (f = c/λ) So mpc = hc /λc /λc= h/λ λ = hp So you’re saying that a particle of momentum p has a wavelength equal to Planck’s constant divided by p?! Yes! λ = h/p It will be known as the de Broglie wavelength of the particle Confirmation of de Broglie’s ideas De Broglie didn’t have to wait long for his idea to be shown to be correct. -
History of Physics Group Newsletter No 21 January 2007
History of Physics Group Newsletter No 21 January 2007 Cover picture: Ludwig Boltzmann’s ‘Bicykel’ – a piece of apparatus designed by Boltzmann to demonstrate the effect of one electric circuit on another. This, and the picture of Boltzmann on page 27, are both reproduced by kind permission of Dr Wolfgang Kerber of the Österreichische Zentralbibliothek für Physik, Vienna. Contents Editorial 2 Group meetings AGM Report 3 AGM Lecture programme: ‘Life with Bragg’ by John Nye 6 ‘George Francis Fitzgerald (1851-1901) - Scientific Saint?’ by Denis Weaire 9 ‘Benjamin Franklin (1706-1790) - a brief biography by Peter Ford 15 Reports Oxford visit 24 EPS History of physics group meeting, Graz, Austria 27 European Society for the History of Science - 2nd International conference 30 Sir Joseph Rotblat conference, Liverpool 35 Features: ‘Did Einstein visit Bratislava or not?’ by Juraj Sebesta 39 ‘Wadham College, Oxford and the Experimental Tradition’ by Allan Chapman 44 Book reviews JD Bernal – The Sage of Science 54 Harwell – The Enigma Revealed 59 Web report 62 News 64 Next Group meeting 65 Committee and contacts 68 2 Editorial Browsing through a copy of the group’s ‘aims and objectives’, I notice that part of its aims are ‘to secure the written, oral and instrumental record of British physics and to foster a greater awareness concerning the history of physics among physicists’ and I think that over the years much has been achieved by the group in tackling this not inconsiderable challenge. One must remember, however, that the situation at the time this was written was very different from now. -
A Tribute to Jean Perrin
A TRIBUTE TO JEAN PERRIN l Henk Kubbinga – University of Groningen (The Netherlands) – DOI: 10.1051/epn/2013502 Nineteenth century's physics was primarily a molecular physics in the style of Laplace. Maxwell had been guided by Laplace’s breathtaking nebular hypothesis and its consequences for Saturn. Somewhat later Van der Waals drew upon his analysis of capillarity. The many textbooks of Biot perpetuated the molecularism involved in all this. Jean Perrin, then, proposed a charmingly simple proof for the well-foundedness of the molecular theory (1908). 16 EPN 44/5 Article available at http://www.europhysicsnews.org or http://dx.doi.org/10.1051/epn/2013502 JEAN PERRIN FEATURES ean [Baptiste] Perrin enrolled in 1891 at the Ecole and Robert Koch and fancied a state of science in which b P.16: Normale Supérieure de Paris, the nursery of France’s the microscope had not yet been invented. In such a situ- Saturn (with Titan) edge-on as viewed academic staff. The new ‘normalien’ came from Lyon ation Pasteur and Koch—let’s say, medical science in by the Hubble and had passed a typically French parcours: primary general—might have concluded all the same that con- Telescope (2012; Jschool and collège ‘en province’, lycée at Paris. The ‘nor- tagious diseases were caused by invisibly small living courtesy: NASA). maliens’ of the time were left-winged politically, but wore beings which infect a victim and set out immediately to uniforms, though, and despised their Sorbonne fellow multiply, before attacking subsequent victims etc. Effec- students. Mathematics made the difference; Perrin had tive countermeasures might have been developed in that passed without any trouble. -
Tracing the Recorded History of Thin-Film Sputter Deposition: from the 1800S to 2017
Review Article: Tracing the recorded history of thin-film sputter deposition: From the 1800s to 2017 Cite as: J. Vac. Sci. Technol. A 35, 05C204 (2017); https://doi.org/10.1116/1.4998940 Submitted: 24 March 2017 . Accepted: 10 May 2017 . Published Online: 08 September 2017 J. E. Greene COLLECTIONS This paper was selected as Featured ARTICLES YOU MAY BE INTERESTED IN Review Article: Plasma–surface interactions at the atomic scale for patterning metals Journal of Vacuum Science & Technology A 35, 05C203 (2017); https:// doi.org/10.1116/1.4993602 Microstructural evolution during film growth Journal of Vacuum Science & Technology A 21, S117 (2003); https://doi.org/10.1116/1.1601610 Overview of atomic layer etching in the semiconductor industry Journal of Vacuum Science & Technology A 33, 020802 (2015); https:// doi.org/10.1116/1.4913379 J. Vac. Sci. Technol. A 35, 05C204 (2017); https://doi.org/10.1116/1.4998940 35, 05C204 © 2017 Author(s). REVIEW ARTICLE Review Article: Tracing the recorded history of thin-film sputter deposition: From the 1800s to 2017 J. E. Greenea) D. B. Willett Professor of Materials Science and Physics, University of Illinois, Urbana, Illinois, 61801; Tage Erlander Professor of Physics, Linkoping€ University, Linkoping,€ Sweden, 58183, Sweden; and University Professor of Materials Science, National Taiwan University Science and Technology, Taipei City, 106, Taiwan (Received 24 March 2017; accepted 10 May 2017; published 8 September 2017) Thin films, ubiquitous in today’s world, have a documented history of more than 5000 years. However, thin-film growth by sputter deposition, which required the development of vacuum pumps and electrical power in the 1600s and the 1700s, is a much more recent phenomenon. -
Third ICESHS, Austrian Academy of Sciences, Vienna 2008 Electron – A
Third ICESHS, Austrian Academy of Sciences, Vienna 2008 Isabel Serra, Francisca Viegas, Elisa Maia Department of History and Philosophy of Science, University of Lisbon Lisboa, Portugal [email protected] Electron – a main actor in scientific controversies1 1. Introduction The story of the electron can contribute to the study of the continuity-discontinuity of the scientific thinking in modern age, as well as to discuss models and metaphors in history of science. Actually, the electron played a central role in several scientific controversies: nature of electricity and cathode rays, structure and properties of matter. The idea of an atom of electricity was introduced by Faraday and adopted by Helmholtz. In 1874, Stoney estimated its charge and named it electron. However, Maxwell had stated that a complete knowledge of electricity would eliminate the necessity of such particles. The controversy about the nature of electricity was to lie dormant for years until it was brightened by the study of discharges in gases. The nature of cathode rays divided physicists and chemists, with the electron playing the major role in the dispute. The experiences of Perrin (1895) and Thomson (1897), seemed to confirm the existence of the electron, but did not convince all scientists. The electron became the main protagonist of a controversial image of matter: the atomistic view. In 1913, Bohr’s atomic theory was received with enthusiasm by some physicists but with criticism by others. Nevertheless, the atomic structure of matter gradually wins acceptance in reason of its extraordinary power in predicting spectral lines. At last, electrons were particles, coherent with facts and theories. -
Otto Stern Annalen 4.11.11
(To be published by Annalen der Physik in December 2011) Otto Stern (1888-1969): The founding father of experimental atomic physics J. Peter Toennies,1 Horst Schmidt-Böcking,2 Bretislav Friedrich,3 Julian C.A. Lower2 1Max-Planck-Institut für Dynamik und Selbstorganisation Bunsenstrasse 10, 37073 Göttingen 2Institut für Kernphysik, Goethe Universität Frankfurt Max-von-Laue-Strasse 1, 60438 Frankfurt 3Fritz-Haber-Institut der Max-Planck-Gesellschaft Faradayweg 4-6, 14195 Berlin Keywords History of Science, Atomic Physics, Quantum Physics, Stern- Gerlach experiment, molecular beams, space quantization, magnetic dipole moments of nucleons, diffraction of matter waves, Nobel Prizes, University of Zurich, University of Frankfurt, University of Rostock, University of Hamburg, Carnegie Institute. We review the work and life of Otto Stern who developed the molecular beam technique and with its aid laid the foundations of experimental atomic physics. Among the key results of his research are: the experimental test of the Maxwell-Boltzmann distribution of molecular velocities (1920), experimental demonstration of space quantization of angular momentum (1922), diffraction of matter waves comprised of atoms and molecules by crystals (1931) and the determination of the magnetic dipole moments of the proton and deuteron (1933). 1 Introduction Short lists of the pioneers of quantum mechanics featured in textbooks and historical accounts alike typically include the names of Max Planck, Albert Einstein, Arnold Sommerfeld, Niels Bohr, Max von Laue, Werner Heisenberg, Erwin Schrödinger, Paul Dirac, Max Born, and Wolfgang Pauli on the theory side, and of Wilhelm Conrad Röntgen, Ernest Rutherford, Arthur Compton, and James Franck on the experimental side. However, the records in the Archive of the Nobel Foundation as well as scientific correspondence, oral-history accounts and scientometric evidence suggest that at least one more name should be added to the list: that of the “experimenting theorist” Otto Stern. -
Theory and Experiment in the Quantum-Relativity Revolution
Theory and Experiment in the Quantum-Relativity Revolution expanded version of lecture presented at American Physical Society meeting, 2/14/10 (Abraham Pais History of Physics Prize for 2009) by Stephen G. Brush* Abstract Does new scientific knowledge come from theory (whose predictions are confirmed by experiment) or from experiment (whose results are explained by theory)? Either can happen, depending on whether theory is ahead of experiment or experiment is ahead of theory at a particular time. In the first case, new theoretical hypotheses are made and their predictions are tested by experiments. But even when the predictions are successful, we can’t be sure that some other hypothesis might not have produced the same prediction. In the second case, as in a detective story, there are already enough facts, but several theories have failed to explain them. When a new hypothesis plausibly explains all of the facts, it may be quickly accepted before any further experiments are done. In the quantum-relativity revolution there are examples of both situations. Because of the two-stage development of both relativity (“special,” then “general”) and quantum theory (“old,” then “quantum mechanics”) in the period 1905-1930, we can make a double comparison of acceptance by prediction and by explanation. A curious anti- symmetry is revealed and discussed. _____________ *Distinguished University Professor (Emeritus) of the History of Science, University of Maryland. Home address: 108 Meadowlark Terrace, Glen Mills, PA 19342. Comments welcome. 1 “Science walks forward on two feet, namely theory and experiment. ... Sometimes it is only one foot which is put forward first, sometimes the other, but continuous progress is only made by the use of both – by theorizing and then testing, or by finding new relations in the process of experimenting and then bringing the theoretical foot up and pushing it on beyond, and so on in unending alterations.” Robert A. -
The Discovery of Subatomic Particles
The Discovery of Subatomic Particles Steven Weinberg I. W. H . Freeman and Co mpa ny NE W Y ORK Staff and students at the Cavendish Laboratory, 1933 . Fourth row: J. K. Roberts, P. Harteck, R. C. Evans, E. C. Childs, R. A. Smith, Top row: W. ]. Henderson , W. E. Dun canson, P. Wright, G. E. Pringle, H. Miller. G. T. P. Tarr ant , L. H. Gray, j . P. Gort, M. L. Oliphant , P. I. Dee, ]. L. Pawsey, Second row: C. B. O. Mohr, N. Feath er, C. W. Gilbert , D.Shoenberg, D. E. Lea, C. £. Wynn-Williams. R. Witty, - -Halliday, H . S. W. Massey, E.S. Shire. Seated row: - - Sparshotr, J. A.Ratcliffe, G. Stead, J. Chadwick, G. F. C. Searle, Third row : B. B. Kinsey, F. W. Nicoll, G. Occhialini, E. C. Allberry, B. M. Crowt her, Professor Sir J. J. Thomson, Professo r Lord Ruth erford, Professor C. T. R. Wilson, B. V. Bowden, W. B. Lewis, P. C. Ho, E. T. S. Walton, P. W. Burbidge, F. Bitter. C. D. Ellis, Professor Kapirza, P. M. S. Blackett , - - Davies. 13 2 The Discovery of the Electron This century has seen the gradual realization that all matter is composed of a' f~w type s of elementary particles-tiny units that apparently cannot be subdi vided further. The list of elementary particle types has changed many times dunng the century, as new particles have been discovered and old ones have been found to be composed of more elementary constituents. At latest count there are some sixteen known types of elementary particles. -
Should Physical Laws Be Unit-Invariant?
Should physical laws be unit-invariant? 1. Introduction In a paper published in this journal in 2015, Sally Riordan reviews a recent debate about whether fundamental constants are really “constant”, or whether they may change over cosmological timescales. Her context is the impending redefinition of the kilogram and other units in terms of fundamental constants – a practice which is seen as more “objective” than defining units in terms of human artefacts. She focusses on one particular constant, the fine structure constant (α), for which some evidence of such a variation has been reported. Although α is not one of the fundamental constants involved in the proposed redefinitions, it is linked to some which are, so that there is a clear cause for concern. One of the authors she references is Michael Duff, who presents an argument supporting his assertion that dimensionless constants are more fundamental than dimensioned ones; this argument employs various systems of so-called “natural units”. [see Riordan (2015); Duff (2004)] An interesting feature of this discussion is that not only Riordan herself, but all the papers she cites, use a formula for α that is valid only in certain systems of units, and would not feature in a modern physics textbook. This violates another aspect of objectivity – namely, the idea that our physical laws should be expressed in such a way that they are independent of the particular units we choose to use; they should be unit-invariant. In this paper I investigate the place of unit-invariance in the history of physics, together with its converse, unit-dependence, which we will find is a common feature of some branches of physics, despite the fact that, as I will show in an analysis of Duff’s argument, unit-dependent formulae can lead to erroneous conclusions. -
Avogadro's Constant
Avogadro's Constant Nancy Eisenmenger Question Artem, 8th grade How \Avogadro constant" was invented and how scientists calculated it for the first time? Answer What is Avogadro's Constant? • Avogadros constant, NA: the number of particles in a mole • mole: The number of Carbon-12 atoms in 0.012 kg of Carbon-12 23 −1 • NA = 6:02214129(27) × 10 mol How was Avogadro's Constant Invented? Avogadro's constant was invented because scientists were learning about measuring matter and wanted a way to relate the microscopic to the macroscopic (e.g. how many particles (atoms, molecules, etc.) were in a sample of matter). The first scientists to see a need for Avogadro's constant were studying gases and how they behave under different temperatures and pressures. Amedeo Avogadro did not invent the constant, but he did state that all gases with the same volume, pressure, and temperature contained the same number of gas particles, which turned out to be very important to the development of our understanding of the principles of chemistry and physics. The constant was first calculated by Johann Josef Loschmidt, a German scientist, in 1865. He actually calculated the Loschmidt number, a constant that measures the same thing as Avogadro's number, but in different units (ideal gas particles per cubic meter at 0◦C and 1 atm). When converted to the same units, his number was off by about a factor of 10 from Avogadro's number. That may sound like a lot, but given the tools he had to work with for both theory and experiment and the magnitude of the number (∼ 1023), that is an impressively close estimate.