Thomas Young and the Wave Theory of Light
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What the Renaissance Knew Piero Scaruffi Copyright 2018
What the Renaissance knew Piero Scaruffi Copyright 2018 http://www.scaruffi.com/know 1 What the Renaissance knew • The 17th Century – For tens of thousands of years, humans had the same view of the universe and of the Earth. – Then the 17th century dramatically changed the history of humankind by changing the way we look at the universe and ourselves. – This happened in a Europe that was apparently imploding politically and militarily, amid massive, pervasive and endless warfare – Grayling refers to "the flowering of genius“: Galileo, Pascal, Kepler, Newton, Cervantes, Shakespeare, Donne, Milton, Racine, Moliere, Descartes, Spinoza, Leibniz, Locke, Rubens, El Greco, Rembrandt, Vermeer… – Knowledge spread, ideas circulated more freely than people could travel 2 What the Renaissance knew • Collapse of classical dogmas – Aristotelian logic vs Rene Descartes' "Discourse on the Method" (1637) – Galean medicine vs Vesalius' anatomy (1543), Harvey's blood circulation (1628), and Rene Descartes' "Treatise of Man" (1632) – Ptolemaic cosmology vs Copernicus (1530) and Galileo (1632) – Aquinas' synthesis of Aristotle and the Bible vs Thomas Hobbes' synthesis of mechanics (1651) and Pierre Gassendi's synthesis of Epicurean atomism and anatomy (1655) – Papal unity: the Thirty Years War (1618-48) shows endless conflict within Christiandom 3 What the Renaissance knew • Decline of – Feudalism – Chivalry – Holy Roman Empire – Papal Monarchy – City-state – Guilds – Scholastic philosophy – Collectivism (Church, guild, commune) – Gothic architecture 4 What -
Classical and Modern Diffraction Theory
Downloaded from http://pubs.geoscienceworld.org/books/book/chapter-pdf/3701993/frontmatter.pdf by guest on 29 September 2021 Classical and Modern Diffraction Theory Edited by Kamill Klem-Musatov Henning C. Hoeber Tijmen Jan Moser Michael A. Pelissier SEG Geophysics Reprint Series No. 29 Sergey Fomel, managing editor Evgeny Landa, volume editor Downloaded from http://pubs.geoscienceworld.org/books/book/chapter-pdf/3701993/frontmatter.pdf by guest on 29 September 2021 Society of Exploration Geophysicists 8801 S. Yale, Ste. 500 Tulsa, OK 74137-3575 U.S.A. # 2016 by Society of Exploration Geophysicists All rights reserved. This book or parts hereof may not be reproduced in any form without permission in writing from the publisher. Published 2016 Printed in the United States of America ISBN 978-1-931830-00-6 (Series) ISBN 978-1-56080-322-5 (Volume) Library of Congress Control Number: 2015951229 Downloaded from http://pubs.geoscienceworld.org/books/book/chapter-pdf/3701993/frontmatter.pdf by guest on 29 September 2021 Dedication We dedicate this volume to the memory Dr. Kamill Klem-Musatov. In reading this volume, you will find that the history of diffraction We worked with Kamill over a period of several years to compile theory was filled with many controversies and feuds as new theories this volume. This volume was virtually ready for publication when came to displace or revise previous ones. Kamill Klem-Musatov’s Kamill passed away. He is greatly missed. new theory also met opposition; he paid a great personal price in Kamill’s role in Classical and Modern Diffraction Theory goes putting forth his theory for the seismic diffraction forward problem. -
Selected Correspondence of Descartes
Selected Correspondence of Descartes René Descartes Copyright © Jonathan Bennett 2017. All rights reserved [Brackets] enclose editorial explanations. Small ·dots· enclose material that has been added, but can be read as though it were part of the original text. Occasional •bullets, and also indenting of passages that are not quotations, are meant as aids to grasping the structure of a sentence or a thought. Every four-point ellipsis . indicates the omission of a brief passage that has no philosophical interest, or that seems to present more difficulty than it is worth. (Where a letter opens with civilities and/or remarks about the postal system, the omission of this material is not marked by ellipses.) Longer omissions are reported between brackets in normal-sized type. —The letters between Descartes and Princess Elisabeth of Bohemia, omitted here, are presented elsewhere on this website (but see note on page 181).—This version is greatly indebted to CSMK [see Glossary] both for a good English translation to work from and for many explanatory notes, though most come from AT [see Glossary].—Descartes usually refers to others by title (‘M.’ for ‘Monsieur’ or ‘Abbé’ or ‘Reverend Father’ etc.); the present version omits most of these.—Although the material is selected mainly for its bearing on Descartes as a philosopher, glimpses are given of the colour and flavour of other sides of his life. First launched: April 2013 Correspondence René Descartes Contents Letters written in 1619–1637 1 to Beeckman, 26.iii.1619........................................................1 -
On an Experimentum Crucis for Optics
Research Report: On an Experimentum Crucis for Optics Ionel DINU, M.Sc. Teacher of Physics E-mail: [email protected] (Dated: November 17, 2010) Abstract Formulated almost 150 years ago, Thomas Young’s hypothesis that light might be a transverse wave has never been seriously questioned, much less subjected to experiment. In this article I report on an attempt to prove experimentally that Young’s hypothesis is untenable. Although it has certain limitations, the experiment seems to show that sound in air, a longitudinal wave, can be “polarized” by reflection just like light, and this can be used as evidence against Young’s hypothesis. Further refinements of the experimental setup may yield clearer results, making this report useful to those interested in the important issue of whether light is a transverse or a longitudinal wave. Introduction In the course of development of science, there has always been a close connection between sound and light [1]. Acoustics stimulated research and discovery in optics and vice-versa. Reflection and refraction being the first common points observed between the two, the analogy between optical and acoustical phenomena has been proven also in the case of interference, diffraction, Doppler effect, and even in their mode of production: sounds are produced by the vibration of macroscopic objects, while light is produced by vibrating molecules and atoms. The wave nature of sound implies that light is also a wave and, if matter must be present for sound to be propagated, then aether must exist in order to account for the propagation of light through spaces void of all the matter known to chemistry. -
Descartes' Optics
Descartes’ Optics Jeffrey K. McDonough Descartes’ work on optics spanned his entire career and represents a fascinating area of inquiry. His interest in the study of light is already on display in an intriguing study of refraction from his early notebook, known as the Cogitationes privatae, dating from 1619 to 1621 (AT X 242-3). Optics figures centrally in Descartes’ The World, or Treatise on Light, written between 1629 and 1633, as well as, of course, in his Dioptrics published in 1637. It also, however, plays important roles in the three essays published together with the Dioptrics, namely, the Discourse on Method, the Geometry, and the Meteorology, and many of Descartes’ conclusions concerning light from these earlier works persist with little substantive modification into the Principles of Philosophy published in 1644. In what follows, we will look in a brief and general way at Descartes’ understanding of light, his derivations of the two central laws of geometrical optics, and a sampling of the optical phenomena he sought to explain. We will conclude by noting a few of the many ways in which Descartes’ efforts in optics prompted – both through agreement and dissent – further developments in the history of optics. Descartes was a famously systematic philosopher and his thinking about optics is deeply enmeshed with his more general mechanistic physics and cosmology. In the sixth chapter of The Treatise on Light, he asks his readers to imagine a new world “very easy to know, but nevertheless similar to ours” consisting of an indefinite space filled everywhere with “real, perfectly solid” matter, divisible “into as many parts and shapes as we can imagine” (AT XI ix; G 21, fn 40) (AT XI 33-34; G 22-23). -
Thomas Young the Man Who Knew Everything
Thomas Young The man Who Knew Everything Andrew Robinson marvels at the brain power and breadth of knowledge of the 18th-century polymath Thomas Young. He examines his relationship with his contemporaries, particularly with the French Egyptologist Champollion, and how he has been viewed subsequently by historians. ORTUNATE NEWTON, happy professor of natural philosophy at childhood of science!’ Albert the newly founded Royal Institution, F Einstein wrote in 1931 in his where in 1802-03 he delivered what foreword to the fourth edition of is generally regarded as the most far- Newton’s influential treatise Opticks, reaching series of lectures ever given originally published in 1704. by a scientist; a physician at a major London hospital, St George’s, for a Nature to him was an open book, quarter of a century; the secretary of whose letters he could read without the Admiralty’s Board of Longitude effort. ... Reflection, refraction, the and superintendent of its vital Nauti- formation of images by lenses, the cal Almanac from 1818 until his mode of operation of the eye, the death; and ‘inspector of calculations’ spectral decomposition and recom- for a leading life insurance company position of the different kinds of in the 1820s. In 1794, he was elected light, the invention of the reflecting a fellow of the Royal Society at the telescope, the first foundations of age of barely twenty-one, became its colour theory, the elementary theory foreign secretary at the age of thirty, of the rainbow pass by us in and turned down its presidency in procession, and finally come his his fifties. -
Quantum Weirdness: a Beginner's Guide
Quantum Weirdness: A Beginner’s Guide Dr. Andrew Robinson Part 1 Introduction The Quantum Jump 9:38 AM About Me • From Bakewell • PhD in Physical Chemistry • Worked in Berlin, Liverpool, Birmingham • In Canada since 2000 • Worked at University of Saskatchewan • Moved to Ottawa in 2010 • Teach Physics at Carleton 9:38 AM In This Lecture Series • We will talk about • What does Quantum Mean? • Quantum Effects • What are the ramifications of Quantum Theory • How Quantum Theory impacts our everyday lives • I will show a few equations, but you don’t need to know any mathematics • Please ask questions at any time 9:38 AM Books “How to Teach Quantum Physics to your Dog” by Chad Orzel “30-Second Quantum Theory” By Brian Clegg (ed.) 9:38 AM Definition of “Quantum” Physics • A discrete quantity of energy proportional in magnitude to the frequency of the radiation it represents. Legal • A required or allowed amount, especially an amount of money legally payable in damages. 9:38 AM • Quantum Satis “as much as is sufficient“ – pharmacology and medicine • Quantum Salis “the amount which is enough” • Quantum comes from the Latin word quantus, meaning "how great". Used by the German Physicist Hermann von Helmholtz ( who was also a physician) in the context of the electron (quanta of electricity) Use by Einstein in 1905 "Lichtquanta” – particle of light 9:38 AM “Quantum Jump” & “Quantum Leap” • Colloquially “A sudden large increase or advance”. • In physics “A jump between two discrete energy levels in a quantum system” (Actually a rather small leap in terms of energy!) 9:38 AM Quantum Properties in Physics • Properties which can only take certain values When you are on the ladder, you must be on one of the steps: 4 1 3 2 Quantum 2 3 Numbers 1 4 9:38 AM • Not every quantity in physics is quantized • Your height from the ground when on the slide varies continuously Maximum height Minimum9:38 AM height • Whether you can treat the system as continuous, or quantum depends on the scale. -
Thomas Young's Research on Fluid Transients: 200 Years On
Thomas Young's research on fluid transients: 200 years on Arris S Tijsseling Alexander Anderson Department of Mathematics School of Mechanical and Computer Science and Systems Engineering Eindhoven University of Technology Newcastle University P.O. Box 513, 5600 MB Eindhoven Newcastle upon Tyne NE1 7RU The Netherlands United Kingdom ABSTRACT Thomas Young published in 1808 his famous paper (1) in which he derived the pressure wave speed in an incompressible liquid contained in an elastic tube. Unfortunately, Young's analysis was obscure and the wave speed was not explicitly formulated, so his achievement passed unnoticed until it was rediscovered nearly half a century later by the German brothers Weber. This paper briefly reviews Young's life and work, and concentrates on his achievements in the area of hydraulics and waterhammer. Young's 1808 paper is “translated” into modern terminology. Young's discoveries, though difficult for modern readers to identify, appear to include most if not all of the key elements which would subsequently be combined into the pressure rise equation of Joukowsky. Keywords waterhammer, fluid transients, solid transients, wave speed, history, Thomas Young NOTATION c sonic wave speed, m/s p fluid pressure, Pa D internal tube diameter, m R internal tube radius, m E Young’s modulus, Pa t time, s e tube wall thickness, m v velocity, m/s f elastic limit, Pa x length, m g gravitational acceleration, m/s 2 δ change, jump h height, pressure head, m ε longitudinal strain K fluid bulk modulus, Pa ρ mass density, kg/m -
Three Music-Theory Lessons
Three Music-Theory Lessons The Harvard community has made this article openly available. Please share how this access benefits you. Your story matters Citation Rehding, Alexander. 2016. “Three Music-Theory Lessons.” Journal of the Royal Musical Association 141 (2) (July 2): 251–282. doi:10.1080/02690403.2016.1216025. Published Version doi:10.1080/02690403.2016.1216025 Citable link http://nrs.harvard.edu/urn-3:HUL.InstRepos:34220771 Terms of Use This article was downloaded from Harvard University’s DASH repository, and is made available under the terms and conditions applicable to Open Access Policy Articles, as set forth at http:// nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of- use#OAP Three Music Theory Lessons ALEXANDER REHDING To make the familiar strange and the strange familiar was as much a central feature of Novalis’ conception of Romanticism as it is a mainstay of semiotics.1 In this spirit, we will begin with what seems like a mundane description of music- theoretical practice. If we enter a music theory classroom in the western world, we would normally expect to find a number of objects. We see a blackboard, ideally with five-line staffs already printed on it. We also expect a piano in the room, and we would probably have some sheet music, perhaps with the quintessential music theory teaching material: Bach chorale harmonizations. Let’s further imagine it is this passage, the simple opening line of the Lutheran hymn “Wie schön leuchtet der Morgenstern,” from Bach’s Cantata BWV 1, shown in Fig. 1, that is marked on the board. -
Huygens' Principle and the Phenomena of Total Reflection
Pans. Opt. Soc. (London) 28 149-160 (1927) Huygens' principle and the phenomena of total reflection PROFESSOR C V RAMAN, F.R.S. (The University, Calcutta) MS received, 1st January, 1927. Read and discussed, 7th April, 1927 Abstract. In this paper the phenomena of total reflection are considered, de nouo, from the standpoint of the principle of Huygens, no use whatever being made of the Fresnel for ulae for reflection and refraction. Huygens' principle enables us to evaluate the disturbance appearing"'h i the second medium when light is incident on the boundary between two media and is totally reflected into the first medium. The disturbance takes the form of a superficial wave moving parallel to the boundary. The existence of such a superficial wave is then shown to involve, as a necessary consequence, an acceleration of the reflected wave with reference to the incident wave, the acceleration being zero at critical incidence and increasing to half an oscillation at grazing incidence. The intensity of the superficial wave is at critical incidence greater for the component having the magnetic vector parallel to the surface, but diminishes more rapidly with increasing incidence than for the component having the electric vector parallel to the surface; the phase-advance reaches its maximum value correspond- ingly sooner. The phase-angle between the two components is evaluated and found to be an acute angle, in agreement with the classical treatment based on the Fresnel formulae, but in disagreement with the conclusions of Lord Kelvin and Schuster. The source of error in the Kelvin-Schuster treatment is pointed out. -
Blackbody” Radiation
Applications of Photonics Technologies 2019 Introduction: what is light and basic properties Cristina Masoller [email protected] www.fisica.edu.uy/~cris MÀSTER UNIVERSITARI EN ENGINYERIA DE SISTEMES AUTOMÀTICS I ELECTRÒNICA INDUSTRIAL MÀSTER UNIVERSITARI EN ENGINYERIA AERONÀUTICA MÀSTER UNIVERSITARI EN ENGINYERIA INDUSTRIAL Introducing myself • Originally from Montevideo, Uruguay • PhD in physics (lasers, Bryn Mawr College, USA 1999) • Since 2004 @ Universitat Politecnica de Catalunya • Profesora Catedratica, Physics Department, research group on Dynamics, Nonlinear Optics and Lasers • Web page: http://www.fisica.edu.uy/~cris/ Introducing our research group Dynamics, Nonlinear Optics and Lasers Senior researchers / PhD students: 11/8 Introducing our research group . Research topics: Nonlinear phenomena (photonics, biophysics, complex systems) . Lab facilities in Gaia Building, UPC Terrassa: . Website: https://donll.upc.edu 4 Learning objectives and references . To understand the basic properties of light, which will allow us to understand photonic techniques and applications. There is no required text. The slides are based on previous courses by Prof. Ramon Vilaseca (UPC Prof. Emerito), the slides of Prof. Rick Trebino (Georgia Tech, USA) and freely available material in the Optical Society (OSA) web page. 5 what is light? Particles and waves Particles are localized in space and time (classical physics). Particles have well-defined trajectories. Waves are extended in space and time. Waves have poorly defined trajectories. waves bend around corners (diffraction) Two ways in which energy is transported Point-mass interaction, which transfers energy and momentum: particles. Extended regions wherein energy is transferred by vibrations and rotations (collective motions of particles): waves. Poll Is light constituted by particles or by waves? 9 The nature of light: Huygens Huygens promoted the wave theory. -
Thomas Young and Eighteenth-Century Tempi Peter Pesic St
Performance Practice Review Volume 18 | Number 1 Article 2 Thomas Young and Eighteenth-Century Tempi Peter Pesic St. John's College, Santa Fe, New Mexico Follow this and additional works at: http://scholarship.claremont.edu/ppr Pesic, Peter (2013) "Thomas Young and Eighteenth-Century Tempi," Performance Practice Review: Vol. 18: No. 1, Article 2. DOI: 10.5642/perfpr.201318.01.02 Available at: http://scholarship.claremont.edu/ppr/vol18/iss1/2 This Article is brought to you for free and open access by the Journals at Claremont at Scholarship @ Claremont. It has been accepted for inclusion in Performance Practice Review by an authorized administrator of Scholarship @ Claremont. For more information, please contact [email protected]. Thomas Young and Eighteenth-Century Tempi Dedicated to the memory of Ralph Berkowitz (1910–2011), a great pianist, teacher, and master of tempo. The uthora would like to thank the John Simon Guggenheim Memorial Foundation for its support as well as Alexei Pesic for kindly photographing a rare copy of Crotch’s Specimens of Various Styles of Music. This article is available in Performance Practice Review: http://scholarship.claremont.edu/ppr/vol18/iss1/2 Thomas Young and Eighteenth-Century Tempi Peter Pesic In trying to determine musical tempi, we often lack exact and authoritative sources, especially from the eighteenth century, before composers began to indicate metronome markings. Accordingly, any independent accounts are of great value, such as were collected in Ralph Kirkpatrick’s pioneering article (1938) and most recently sur- veyed in this journal by Beverly Jerold (2012).1 This paper brings forward a new source in the writings of the English polymath Thomas Young (1773–1829), which has been overlooked by musicologists because its author’s best-known work was in other fields.