Von Richthofen, Einstein and the AGA Estimating Achievement from Fame
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Hendrik Antoon Lorentz's Struggle with Quantum Theory A. J
Hendrik Antoon Lorentz’s struggle with quantum theory A. J. Kox Archive for History of Exact Sciences ISSN 0003-9519 Volume 67 Number 2 Arch. Hist. Exact Sci. (2013) 67:149-170 DOI 10.1007/s00407-012-0107-8 1 23 Your article is published under the Creative Commons Attribution license which allows users to read, copy, distribute and make derivative works, as long as the author of the original work is cited. You may self- archive this article on your own website, an institutional repository or funder’s repository and make it publicly available immediately. 1 23 Arch. Hist. Exact Sci. (2013) 67:149–170 DOI 10.1007/s00407-012-0107-8 Hendrik Antoon Lorentz’s struggle with quantum theory A. J. Kox Received: 15 June 2012 / Published online: 24 July 2012 © The Author(s) 2012. This article is published with open access at Springerlink.com Abstract A historical overview is given of the contributions of Hendrik Antoon Lorentz in quantum theory. Although especially his early work is valuable, the main importance of Lorentz’s work lies in the conceptual clarifications he provided and in his critique of the foundations of quantum theory. 1 Introduction The Dutch physicist Hendrik Antoon Lorentz (1853–1928) is generally viewed as an icon of classical, nineteenth-century physics—indeed, as one of the last masters of that era. Thus, it may come as a bit of a surprise that he also made important contribu- tions to quantum theory, the quintessential non-classical twentieth-century develop- ment in physics. The importance of Lorentz’s work lies not so much in his concrete contributions to the actual physics—although some of his early work was ground- breaking—but rather in the conceptual clarifications he provided and his critique of the foundations and interpretations of the new ideas. -
Dr. Julie Brown, CTO of UDC, Awarded Prestigious 2020 Karl Ferdinand Braun Prize from the Society of Information Display
8/3/2020 Dr. Julie Brown, CTO of UDC, Awarded Prestigious 2020 Karl Ferdinand Braun Prize from the Society of Information Display Dr. Mike Weaver, VP of UDC, Honored with 2020 SID Fellow Award EWING, N.J.--(BUSINESS WIRE)-- Universal Display Corporation (Nasdaq: OLED), enabling energy-efficient displays and lighting with its UniversalPHOLED® technology and materials, today announced that Dr. Julie Brown, Senior Vice President and Chief Technical Officer, was awarded the 2020 Karl Ferdinand Braun Prize by the Society of Information Display (SID). Additionally, Dr. Mike Weaver, Vice President of PHOLED R&D, was named a 2020 SID Fellow. The Karl Ferdinand Braun Prize was awarded to Dr. Brown for her outstanding technical achievements and contributions to the development and commercialization of phosphorescent OLED materials and display technology. The Society for Information Display created this prize in 1987 in honor of the German physicist and Nobel Laureate Karl Ferdinand Braun who invented the cathode-ray tube (CRT). Dr. Brown has been a leading innovator in the discovery and development of state-of-the-art OLED technologies and materials for display and lighting applications for over two decades, and is the first woman to be awarded this prestigious prize. Joining Universal Display (UDC) in 1998, Dr. Brown leads a global team of unique chemists, physicists and engineers and spearheads the R&D vision of UDC, from its start-up years to its successful commercial present, and continues to create and shape the Company’s innovation strategy for its future growth. The distinction of Fellow honors an SID member of outstanding qualifications and experience as a scientist or engineer in the field of information display. -
Wave Extraction in Numerical Relativity
Doctoral Dissertation Wave Extraction in Numerical Relativity Dissertation zur Erlangung des naturwissenschaftlichen Doktorgrades der Bayrischen Julius-Maximilians-Universitat¨ Wurzburg¨ vorgelegt von Oliver Elbracht aus Warendorf Institut fur¨ Theoretische Physik und Astrophysik Fakultat¨ fur¨ Physik und Astronomie Julius-Maximilians-Universitat¨ Wurzburg¨ Wurzburg,¨ August 2009 Eingereicht am: 27. August 2009 bei der Fakultat¨ fur¨ Physik und Astronomie 1. Gutachter:Prof.Dr.Karl Mannheim 2. Gutachter:Prof.Dr.Thomas Trefzger 3. Gutachter:- der Dissertation. 1. Prufer¨ :Prof.Dr.Karl Mannheim 2. Prufer¨ :Prof.Dr.Thomas Trefzger 3. Prufer¨ :Prof.Dr.Thorsten Ohl im Promotionskolloquium. Tag des Promotionskolloquiums: 26. November 2009 Doktorurkunde ausgehandigt¨ am: Gewidmet meinen Eltern, Gertrud und Peter, f¨urall ihre Liebe und Unterst¨utzung. To my parents Gertrud and Peter, for all their love, encouragement and support. Wave Extraction in Numerical Relativity Abstract This work focuses on a fundamental problem in modern numerical rela- tivity: Extracting gravitational waves in a coordinate and gauge independent way to nourish a unique and physically meaningful expression. We adopt a new procedure to extract the physically relevant quantities from the numerically evolved space-time. We introduce a general canonical form for the Weyl scalars in terms of fundamental space-time invariants, and demonstrate how this ap- proach supersedes the explicit definition of a particular null tetrad. As a second objective, we further characterize a particular sub-class of tetrads in the Newman-Penrose formalism: the transverse frames. We establish a new connection between the two major frames for wave extraction: namely the Gram-Schmidt frame, and the quasi-Kinnersley frame. Finally, we study how the expressions for the Weyl scalars depend on the tetrad we choose, in a space-time containing distorted black holes. -
Philosophical Rhetoric in Early Quantum Mechanics, 1925-1927
b1043_Chapter-2.4.qxd 1/27/2011 7:30 PM Page 319 b1043 Quantum Mechanics and Weimar Culture FA 319 Philosophical Rhetoric in Early Quantum Mechanics 1925–27: High Principles, Cultural Values and Professional Anxieties Alexei Kojevnikov* ‘I look on most general reasoning in science as [an] opportunistic (success- or unsuccessful) relationship between conceptions more or less defined by other conception[s] and helping us to overlook [danicism for “survey”] things.’ Niels Bohr (1919)1 This paper considers the role played by philosophical conceptions in the process of the development of quantum mechanics, 1925–1927, and analyses stances taken by key participants on four main issues of the controversy (Anschaulichkeit, quantum discontinuity, the wave-particle dilemma and causality). Social and cultural values and anxieties at the time of general crisis, as identified by Paul Forman, strongly affected the language of the debate. At the same time, individual philosophical positions presented as strongly-held principles were in fact flexible and sometimes reversible to almost their opposites. One can understand the dynamics of rhetorical shifts and changing strategies, if one considers interpretational debates as a way * Department of History, University of British Columbia, 1873 East Mall, Vancouver, British Columbia, Canada V6T 1Z1; [email protected]. The following abbreviations are used: AHQP, Archive for History of Quantum Physics, NBA, Copenhagen; AP, Annalen der Physik; HSPS, Historical Studies in the Physical Sciences; NBA, Niels Bohr Archive, Niels Bohr Institute, Copenhagen; NW, Die Naturwissenschaften; PWB, Wolfgang Pauli, Wissenschaftlicher Briefwechsel mit Bohr, Einstein, Heisenberg a.o., Band I: 1919–1929, ed. A. Hermann, K.V. -
Einstein's Mistakes
Einstein’s Mistakes Einstein was the greatest genius of the Twentieth Century, but his discoveries were blighted with mistakes. The Human Failing of Genius. 1 PART 1 An evaluation of the man Here, Einstein grows up, his thinking evolves, and many quotations from him are listed. Albert Einstein (1879-1955) Einstein at 14 Einstein at 26 Einstein at 42 3 Albert Einstein (1879-1955) Einstein at age 61 (1940) 4 Albert Einstein (1879-1955) Born in Ulm, Swabian region of Southern Germany. From a Jewish merchant family. Had a sister Maja. Family rejected Jewish customs. Did not inherit any mathematical talent. Inherited stubbornness, Inherited a roguish sense of humor, An inclination to mysticism, And a habit of grüblen or protracted, agonizing “brooding” over whatever was on its mind. Leading to the thought experiment. 5 Portrait in 1947 – age 68, and his habit of agonizing brooding over whatever was on its mind. He was in Princeton, NJ, USA. 6 Einstein the mystic •“Everyone who is seriously involved in pursuit of science becomes convinced that a spirit is manifest in the laws of the universe, one that is vastly superior to that of man..” •“When I assess a theory, I ask myself, if I was God, would I have arranged the universe that way?” •His roguish sense of humor was always there. •When asked what will be his reactions to observational evidence against the bending of light predicted by his general theory of relativity, he said: •”Then I would feel sorry for the Good Lord. The theory is correct anyway.” 7 Einstein: Mathematics •More quotations from Einstein: •“How it is possible that mathematics, a product of human thought that is independent of experience, fits so excellently the objects of physical reality?” •Questions asked by many people and Einstein: •“Is God a mathematician?” •His conclusion: •“ The Lord is cunning, but not malicious.” 8 Einstein the Stubborn Mystic “What interests me is whether God had any choice in the creation of the world” Some broadcasters expunged the comment from the soundtrack because they thought it was blasphemous. -
A Brief History of Nuclear Astrophysics
A BRIEF HISTORY OF NUCLEAR ASTROPHYSICS PART I THE ENERGY OF THE SUN AND STARS Nikos Prantzos Institut d’Astrophysique de Paris Stellar Origin of Energy the Elements Nuclear Astrophysics Astronomy Nuclear Physics Thermodynamics: the energy of the Sun and the age of the Earth 1847 : Robert Julius von Mayer Sun heated by fall of meteors 1854 : Hermann von Helmholtz Gravitational energy of Kant’s contracting protosolar nebula of gas and dust turns into kinetic energy Timescale ~ EGrav/LSun ~ 30 My 1850s : William Thompson (Lord Kelvin) Sun heated at formation from meteorite fall, now « an incadescent liquid mass » cooling Age 10 – 100 My 1859: Charles Darwin Origin of species : Rate of erosion of the Weald valley is 1 inch/century or 22 miles wild (X 1100 feet high) in 300 My Such large Earth ages also required by geologists, like Charles Lyell A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. Homer Lane ; 1880s :August Ritter : Sun gaseous Compressible As it shrinks, it releases gravitational energy AND it gets hotter Earth Mayer – Kelvin - Helmholtz Helmholtz - Ritter A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. Homer Lane ; 1880s :August Ritter : Sun gaseous Compressible As it shrinks, it releases gravitational energy AND it gets hotter Earth Mayer – Kelvin - Helmholtz Helmholtz - Ritter A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. -
On the Linkage Between Planck's Quantum and Maxwell's Equations
The Finnish Society for Natural Philosophy 25 years, K.V. Laurikainen Honorary Symposium, Helsinki 11.-12.11.2013 On the Linkage between Planck's Quantum and Maxwell's Equations Tuomo Suntola Physics Foundations Society, www.physicsfoundations.org Abstract The concept of quantum is one of the key elements of the foundations in modern physics. The term quantum is primarily identified as a discrete amount of something. In the early 20th century, the concept of quantum was needed to explain Max Planck’s blackbody radiation law which suggested that the elec- tromagnetic radiation emitted by atomic oscillators at the surfaces of a blackbody cavity appears as dis- crete packets with the energy proportional to the frequency of the radiation in the packet. The derivation of Planck’s equation from Maxwell’s equations shows quantizing as a property of the emission/absorption process rather than an intrinsic property of radiation; the Planck constant becomes linked to primary electrical constants allowing a unified expression of the energies of mass objects and electromagnetic radiation thereby offering a novel insight into the wave nature of matter. From discrete atoms to a quantum of radiation Continuity or discontinuity of matter has been seen as a fundamental question since antiquity. Aristotle saw perfection in continuity and opposed Democritus’s ideas of indivisible atoms. First evidences of atoms and molecules were obtained in chemistry as multiple proportions of elements in chemical reac- tions by the end of the 18th and in the early 19th centuries. For physicist, the idea of atoms emerged for more than half a century later, most concretely in statistical thermodynamics and kinetic gas theory that converted the mole-based considerations of chemists into molecule-based considerations based on con- servation laws and probabilities. -
Nobel Prizes Social Network
Nobel prizes social network Marie Skłodowska Curie (Phys.1903, Chem.1911) Nobel prizes social network Henri Becquerel (Phys.1903) Pierre Curie (Phys.1903) = Marie Skłodowska Curie (Phys.1903, Chem.1911) Nobel prizes social network Henri Becquerel (Phys.1903) Pierre Curie (Phys.1903) = Marie Skłodowska Curie (Phys.1903, Chem.1911) Irène Joliot-Curie (Chem.1935) Nobel prizes social network Henri Becquerel (Phys.1903) Pierre Curie (Phys.1903) = Marie Skłodowska Curie (Phys.1903, Chem.1911) Irène Joliot-Curie (Chem.1935) = Frédéric Joliot-Curie (Chem.1935) Nobel prizes social network Henri Becquerel (Phys.1903) Pierre Curie (Phys.1903) = Marie Skłodowska Curie (Phys.1903, Chem.1911) Paul Langevin Irène Joliot-Curie (Chem.1935) = Frédéric Joliot-Curie (Chem.1935) Nobel prizes social network Henri Becquerel (Phys.1903) Pierre Curie (Phys.1903) = Marie Skłodowska Curie (Phys.1903, Chem.1911) Paul Langevin Maurice de Broglie Louis de Broglie (Phys.1929) Irène Joliot-Curie (Chem.1935) = Frédéric Joliot-Curie (Chem.1935) Nobel prizes social network Sir J. J. Thomson (Phys.1906) Henri Becquerel (Phys.1903) Pierre Curie (Phys.1903) = Marie Skłodowska Curie (Phys.1903, Chem.1911) Paul Langevin Maurice de Broglie Louis de Broglie (Phys.1929) Irène Joliot-Curie (Chem.1935) = Frédéric Joliot-Curie (Chem.1935) Nobel prizes social network (more) Sir J. J. Thomson (Phys.1906) Nobel prizes social network (more) Sir J. J. Thomson (Phys.1906) Owen Richardson (Phys.1928) Nobel prizes social network (more) Sir J. J. Thomson (Phys.1906) Owen Richardson (Phys.1928) Clinton Davisson (Phys.1937) Nobel prizes social network (more) Sir J. J. Thomson (Phys.1906) Owen Richardson (Phys.1928) Charlotte Richardson = Clinton Davisson (Phys.1937) Nobel prizes social network (more) Sir J. -
Einstein and the Early Theory of Superconductivity, 1919–1922
Einstein and the Early Theory of Superconductivity, 1919–1922 Tilman Sauer Einstein Papers Project California Institute of Technology 20-7 Pasadena, CA 91125, USA [email protected] Abstract Einstein’s early thoughts about superconductivity are discussed as a case study of how theoretical physics reacts to experimental find- ings that are incompatible with established theoretical notions. One such notion that is discussed is the model of electric conductivity implied by Drude’s electron theory of metals, and the derivation of the Wiedemann-Franz law within this framework. After summarizing the experimental knowledge on superconductivity around 1920, the topic is then discussed both on a phenomenological level in terms of implications of Maxwell’s equations for the case of infinite conduc- tivity, and on a microscopic level in terms of suggested models for superconductive charge transport. Analyzing Einstein’s manuscripts and correspondence as well as his own 1922 paper on the subject, it is shown that Einstein had a sustained interest in superconductivity and was well informed about the phenomenon. It is argued that his appointment as special professor in Leiden in 1920 was motivated to a considerable extent by his perception as a leading theoretician of quantum theory and condensed matter physics and the hope that he would contribute to the theoretical direction of the experiments done at Kamerlingh Onnes’ cryogenic laboratory. Einstein tried to live up to these expectations by proposing at least three experiments on the arXiv:physics/0612159v1 [physics.hist-ph] 15 Dec 2006 phenomenon, one of which was carried out twice in Leiden. Com- pared to other theoretical proposals at the time, the prominent role of quantum concepts was characteristic of Einstein’s understanding of the phenomenon. -
Marischal College
The Scientific Tourist: Aberdeen Marischal College George P Thomson – Nobel Prize winning physicist Sir George Paget Thomson FRS (1892-1975) was the only son of Sir J. J. Thomson, the Cavendish Professor of Physics who is probably most famous for discovering the existence of the electron and measuring its mass. G. P. Thomson was one of a select group of academics in the University of Aberdeen to be awarded the Nobel Prize. He earned it for his work in the Department of Natural Philosophy at Marischal College during his tenure from 1922-1930. There is now a commemorative plaque in the Marischal College quadrangle. Thomson was a high achieving Trinity College, Cambridge, scholar who graduated in 1913 and was elected Fellow and Lecturer at Corpus Christi College in the following year. He was, though, of the generation whose adult lives were to be shaped by two World Wars and their aftermaths. Thomson spent most of the First World War in France and in the research wing of the Royal Flying Corps. His first book1 came out of this experience and is simply entitled “Applied Aerodynamics”. It is a well-illustrated summary of the lessons of wartime work on the science of aircraft design and operation, underlining the basic physics involved. Upon Thomson’s return to Cambridge he took up research into his father’s long-standing interest of electrical discharges in gases. He brought this interest with him when he came to Aberdeen in 1922 and did much of the work enlarging J. J. Thomson’s “Conduction of Electricity through Gases” into a long awaited 3rd edition that was published in their joint names in 1928. -
ARIE SKLODOWSKA CURIE Opened up the Science of Radioactivity
ARIE SKLODOWSKA CURIE opened up the science of radioactivity. She is best known as the discoverer of the radioactive elements polonium and radium and as the first person to win two Nobel prizes. For scientists and the public, her radium was a key to a basic change in our understanding of matter and energy. Her work not only influenced the development of fundamental science but also ushered in a new era in medical research and treatment. This file contains most of the text of the Web exhibit “Marie Curie and the Science of Radioactivity” at http://www.aip.org/history/curie/contents.htm. You must visit the Web exhibit to explore hyperlinks within the exhibit and to other exhibits. Material in this document is copyright © American Institute of Physics and Naomi Pasachoff and is based on the book Marie Curie and the Science of Radioactivity by Naomi Pasachoff, Oxford University Press, copyright © 1996 by Naomi Pasachoff. Site created 2000, revised May 2005 http://www.aip.org/history/curie/contents.htm Page 1 of 79 Table of Contents Polish Girlhood (1867-1891) 3 Nation and Family 3 The Floating University 6 The Governess 6 The Periodic Table of Elements 10 Dmitri Ivanovich Mendeleev (1834-1907) 10 Elements and Their Properties 10 Classifying the Elements 12 A Student in Paris (1891-1897) 13 Years of Study 13 Love and Marriage 15 Working Wife and Mother 18 Work and Family 20 Pierre Curie (1859-1906) 21 Radioactivity: The Unstable Nucleus and its Uses 23 Uses of Radioactivity 25 Radium and Radioactivity 26 On a New, Strongly Radio-active Substance -
Scientific References for Nobel Physics Prizes
1 Scientific References for Nobel Physics Prizes © Dr. John Andraos, 2004 Department of Chemistry, York University 4700 Keele Street, Toronto, ONTARIO M3J 1P3, CANADA For suggestions, corrections, additional information, and comments please send e-mails to [email protected] http://www.chem.yorku.ca/NAMED/ 1901 - Wilhelm Conrad Roentgen "in recognition of the extraordinary services he has rendered by the discovery of the remarkable rays subsequently named after him." Roentgen X-ray Roentgen, W.C. Ann. Physik 1898, 64 , 1 Stanton, A. Science 1896, 3 , 227; 726 (translation) 1902 - Hendrik Antoon Lorentz and Pieter Zeeman "in recognition of the extraordinary service they rendered by their researches into the influence of magnetism upon radiation phenomena." Zeeman effect Zeeman, P., Verhandlungen der Physikalischen Gesellschaft zu Berlin 1896, 7 , 128 Zeeman, P., Nature 1897, 55 , 347 (translation by A. Stanton) 1903 - Antoine Henri Becquerel "in recognition of the extraordinary service he has rendered by his discovery of spontaneous radioactivity." Becquerel, A.H. Compt. Rend. 1896, 122 , 420; 501; 559; 689; 1086 Becquerel, A.H. Compt. Rend. 1896, 123 , 855 Becquerel, A.H. Compt. Rend. 1897, 124 , 444; 800 Becquerel, A.H. Compt. Rend. 1899, 129 , 996; 1205 Becquerel, A.H. Compt. Rend. 1900, 130 , 327; 809; 1583 Becquerel, A.H. Compt. Rend. 1900, 131 , 137 Becquerel, A.H. Compt. Rend. 1901, 133 , 977 1903 - Pierre Curie and Marie Curie, nee Sklodowska "in recognition of the extraordinary services they have rendered by their joint researches on the radiation phenomena discovered by Professor Henri Becquerel." Curie unit of radiation Curie, P; Desains, P., Compt. Rend.