A Brief History of Mangnetism
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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. -
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. -
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 -
The Reception of Relativity in the Netherlands Van Besouw, J.; Van Dongen, J
UvA-DARE (Digital Academic Repository) The reception of relativity in the Netherlands van Besouw, J.; van Dongen, J. Publication date 2013 Document Version Final published version Published in Physics as a calling, science for society: studies in honour of A.J. Kox Link to publication Citation for published version (APA): van Besouw, J., & van Dongen, J. (2013). The reception of relativity in the Netherlands. In A. Maas, & H. Schatz (Eds.), Physics as a calling, science for society: studies in honour of A.J. Kox (pp. 89-110). Leiden Publications. General rights It is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), other than for strictly personal, individual use, unless the work is under an open content license (like Creative Commons). Disclaimer/Complaints regulations If you believe that digital publication of certain material infringes any of your rights or (privacy) interests, please let the Library know, stating your reasons. In case of a legitimate complaint, the Library will make the material inaccessible and/or remove it from the website. Please Ask the Library: https://uba.uva.nl/en/contact, or a letter to: Library of the University of Amsterdam, Secretariat, Singel 425, 1012 WP Amsterdam, The Netherlands. You will be contacted as soon as possible. UvA-DARE is a service provided by the library of the University of Amsterdam (https://dare.uva.nl) Download date:28 Sep 2021 5 The reception of relativity in the Netherlands Jip van Besouw and Jeroen van Dongen Albert Einstein published his definitive version of the general theory of relativity in 1915, in the middle of the First World War. -
November 2019
A selection of some recent arrivals November 2019 Rare and important books & manuscripts in science and medicine, by Christian Westergaard. Flæsketorvet 68 – 1711 København V – Denmark Cell: (+45)27628014 www.sophiararebooks.com AMPÈRE, André-Marie. THE FOUNDATION OF ELECTRO- DYNAMICS, INSCRIBED BY AMPÈRE AMPÈRE, Andre-Marie. Mémoires sur l’action mutuelle de deux courans électri- ques, sur celle qui existe entre un courant électrique et un aimant ou le globe terres- tre, et celle de deux aimans l’un sur l’autre. [Paris: Feugeray, 1821]. $22,500 8vo (219 x 133mm), pp. [3], 4-112 with five folding engraved plates (a few faint scattered spots). Original pink wrappers, uncut (lacking backstrip, one cord partly broken with a few leaves just holding, slightly darkened, chip to corner of upper cov- er); modern cloth box. An untouched copy in its original state. First edition, probable first issue, extremely rare and inscribed by Ampère, of this continually evolving collection of important memoirs on electrodynamics by Ampère and others. “Ampère had originally intended the collection to contain all the articles published on his theory of electrodynamics since 1820, but as he pre- pared copy new articles on the subject continued to appear, so that the fascicles, which apparently began publication in 1821, were in a constant state of revision, with at least five versions of the collection appearing between 1821 and 1823 un- der different titles” (Norman). The collection begins with ‘Mémoires sur l’action mutuelle de deux courans électriques’, Ampère’s “first great memoir on electrody- namics” (DSB), representing his first response to the demonstration on 21 April 1820 by the Danish physicist Hans Christian Oersted (1777-1851) that electric currents create magnetic fields; this had been reported by François Arago (1786- 1853) to an astonished Académie des Sciences on 4 September. -
1972 Frã‰Dã‰Ric and Irãˆne Joliot-Curie
DISTINGUISHED NUCLEAR PIONEERS—1972 FRÉDÉRIC AND IRÈNE JOLIOT-CURIE The choice of Frédéricand IrèneJoliot-Curie as there under the guidance of his principal teacher, the Distinguished Nuclear Pioneers for 1972 by the So great physicist Paul Langevin, who was the first to ciety of Nuclear Medicine is one of the best that recognize Joliot's exceptional gifts and who had a could be made because their discovery of artificial decisive influence on him, not only in the field of radioactivity was not only a great step forward in science but also in leading him toward socialism and the development of nuclear physics but has also led pacifism. Joliot graduated first in his class, and after directly to the possibility of obtaining radioactive 15 months of military service, he might have started isotopes of practically all the chemical elements— a brilliant career as an engineer in industry. But fol those radioisotopes which are now so widely used lowing the advice of Paul Langevin he became a in medical research or practice, and without which personal assistant to Marie Curie who paid him on nuclear medicine could not exist. a grant from the Rockefeller Foundation. FrédéricJoliot was born in Paris on March 19, Thus Frederic Joliot started his scientific career 1900. His father, Henri Joliot, having participated in in the spring of 1925 at the Institut du Radium of the uprising of the Commune of Paris in 1871, had the University of Paris under the guidance of Marie been obliged to spend several years in Belgium. -
Paul Langevin's 1908 Paper “On the Theory of Brownian Motion”
Paul Langevin’s 1908 paper “On the Theory of Brownian Motion” [“Sur la théorie du mouvement brownien,” C. R. Acad. Sci. (Paris) 146, 530–533 (1908)] Don S. Lemons and Anthony Gythiel Citation: Am. J. Phys. 65, 1079 (1997); doi: 10.1119/1.18725 View online: http://dx.doi.org/10.1119/1.18725 View Table of Contents: http://ajp.aapt.org/resource/1/AJPIAS/v65/i11 Published by the American Association of Physics Teachers Additional information on Am. J. Phys. Journal Homepage: http://ajp.aapt.org/ Journal Information: http://ajp.aapt.org/about/about_the_journal Top downloads: http://ajp.aapt.org/most_downloaded Information for Authors: http://ajp.dickinson.edu/Contributors/contGenInfo.html Downloaded 16 Apr 2013 to 216.47.136.20. Redistribution subject to AAPT license or copyright; see http://ajp.aapt.org/authors/copyright_permission Paul Langevin’s 1908 paper ‘‘On the Theory of Brownian Motion’’ [‘‘Sur la the´orie du mouvement brownien,’’ C. R. Acad. Sci. (Paris) 146, 530–533 (1908)] introduced by Don S. Lemonsa) Department of Physics, Bethel College, North Newton, Kansas 67117 translated by Anthony Gythiel Department of History, Wichita State University, Wichita, Kansas 67260-0045 ~Received 7 April 1997; accepted 26 May 1997! We present a translation of Paul Langevin’s landmark paper. In it Langevin successfully applied Newtonian dynamics to a Brownian particle and so invented an analytical approach to random processes which has remained useful to this day. © 1997 American Association of Physics Teachers. I. LANGEVIN, EINSTEIN, AND MARKOV in configuration space. This is to say, in modern terminol- PROCESSES ogy, Langevin described the Brownian particle’s velocity as an Ornstein–Uhlenbeck process and its position as the time In 1908, three years after Albert Einstein initiated the integral of its velocity, while Einstein described its position modern study of random processes with his ground breaking as a driftless Wiener process. -
Scientists and War 1916-2016 by Dave Webb Leeds Beckett University and Scientists for Global Responsibility
Scientists and War 1916-2016 By Dave Webb Leeds Beckett University and Scientists for Global Responsibility The quest for understanding and to know how things work – to find out why they are, what they are - has always been a major driving force for scientists. There are, however, other more negative external drivers – such as the pursuit for military superiority, even in times of peace. Science and engineering have unfortunately made killing easier by helping to develop new types of weapons and World War 1 saw more than its fair share of those. The war also saw a mixture of attitudes from scientists and engineers. Many thought it their duty to help develop new weapons technologies. But there were also those who would not participate in the killing. To understand the social pressures on scientists who spoke out against the war, we need to recognise the cultural context at that time. Just before World War 2 an article in Time magazine dated 11 September 1939, entitled Science and War, expressed the opinion that scientists were not to blame for the way in which their discoveries were used by “men of bad will” and misapplied to “the conquest and murder of men”. This also seemed to be the attitude of many scientists in 1914, and perhaps remains so today. Some though were directly involved. At the outbreak of the First World War, men with specialist scientific and technological skills were not prevented from serving at the Front – by Germany or the Allies. Although some were placed into departments of Time Magazine Front Cover, the armed forces where their skills could be used – for example September 11, 1939 Physicists Ernest Rutherford (Professor of Physics at Manchester since 1907 and winner of the 1908 Nobel Prize in Chemistry) and William Henry Bragg (holder of the Cavendish chair of physics at Leeds since 1909) went to carry out anti-submarine work for the Admiralty. -
Modern Physics
Modern Physics Luis A. Anchordoqui Department of Physics and Astronomy Lehman College, City University of New York Lesson VIII October 29, 2015 L. A. Anchordoqui (CUNY) Modern Physics 10-29-2015 1 / 26 Table of Contents 1 Origins of Quantum Mechanics Line spectra of atoms Wave-particle duality and uncertainty principle 2 Schrodinger¨ Equation Motivation and derivation L. A. Anchordoqui (CUNY) Modern Physics 10-29-2015 2 / 26 Seated (left to right): Erwin Schrodinger,¨ Irene` Joliot-Curie, Niels Bohr, Abram Ioffe, Marie Curie, Paul Langevin, Owen Willans Richardson, Lord Ernest Rutherford, Theophile´ de Donder, Maurice de Broglie, Louis de Broglie, Lise Meitner, James Chadwick. Standing (left to right): Emile´ Henriot, Francis Perrin, Fred´ eric´ Joliot-Curie, Werner Heisenberg, Hendrik Kramers, Ernst Stahel, Enrico Fermi, Ernest Walton, Paul Dirac, Peter Debye, Francis Mott, Blas Cabrera y Felipe, George Gamow, Walther Bothe, Patrick Blackett, M. Rosenblum, Jacques Errera, Ed. Bauer, Wolfgang Pauli, Jules-mile Verschaffelt, Max Cosyns, E. Herzen, John Douglas Cockcroft, Charles Ellis, Rudolf Peierls, Auguste Piccard, Ernest Lawrence, Leon´ Rosenfeld. (October 1933) L. A. Anchordoqui (CUNY) Modern Physics 10-29-2015 3 / 26 Origins of Quantum Mechanics Line spectra of atoms Balmer-Rydberg-Ritz formula When hydrogen in glass tube is excited by 5, 000 V discharge 4 lines are observed in visible part of emission spectrum red @ 656.3 nm blue-green @ 486.1 nm blue violet @ 434.1 nm violet @ 410.2 nm Explanation + Balmer’s empirical formula l = 364.56 n2/(n2 − 4) nm n = 3, 4, 5, ··· (1) Generalized by Rydberg and Ritz to accommodate newly discovered spectral lines in UV and IR 1 1 1 R − > (2) = 2 2 for n2 n1 l n1 n2 L. -
Paul Langevin and the Theory of Relativity
Paul Langeyin and the Theory of Relativity Camillo Cuvaj* ... une montee pleine de toumants imprevus et riche de decouvertes, en vue de ce sommet tout enveloppe en brume... Langeyin (1933) I. Introduction—Historical Background Paul Langeyin (1872-1946) is well-known for his exceptional work on magnet ism, but his impressive work on relativity^ has not been sufficiently appreciated. One should not neglect fascinating objects when they are eclipsed by more brillant objects! Lorentz, Poincare and Einstein were historically the main pioneers in special relativity, building the theory to its culmination in 1905. Moreover, other workers participated significantly. Nor did the story end there since theoretical and ex perimental work had to follow: extensions, applications, interpretations and clarifica tion of special relativity—here was the role of Planck, Minkowski and Langevin! The last major contribution to special relativity^ by Einstein was made in 1907, by Poincare in 1906, and Planck in 1908; Minkowski died in 1909 (of appendicitis) and Poincare died in 1912, while in the succeeding decade Lorentz made valuable contributions only on a topic or two. The development of special relativity (starting in 1911) was continued mainly by Langevin, who did essentially the most that was possible in special relativity after * 6047 Palmetto St., Brooklyn, New York 11227, USA. 1 Langevin's collected articles are in his three books: Oeuvres Scientifiques de P. Langevin (Paris: Centre Nat. Rech. Sci., 1950), La Physique depuis vingt ans(Paris: G. Doin, 1923), Izbranye Trudy (Moscow: Izdat. Akad. nauk SSSR, 1960). Bibliographies are in his Oeuvres''' and in La Pensee, mai-juin 1947, 82-87. -
SCHEDULE Third Workshop on Scientific Archives
TEuropean X-Ray Free-Electron Laser Facility GmbH Holzkoppel 4 22869 Schenefeld Germany SCHEDULE Third Workshop on Scientific Archives 22–24 June 2021 (via Zoom videoconference) Committee on Archives of Science and Technology (CAST), Section on University and Research Institution Archives, International Council on Archives. Organizing committee: ◼ Bethany Anderson, University of Illinois at Urbana-Champaign (USA) ◼ Anne-Flore Laloë, European Molecular Biology Laboratory (Germany) ◼ Melanie Mueller, American Institute of Physics (USA) ◼ Frank Norman, Francis Crick Institute (UK) ◼ Brigitte Van Tiggelen, Science History Institute (France) ◼ Laura Outterside, European XFEL (Germany) Third Workshop on Scientific Archives SCHEDULE 22–24 June 2021 2021-05-18 1 of 4 Tuesday, 22 June 2021 CEST Opening remarks 13:00 – 13:15 Welcome remarks (Robert Feidenhans’l & Laura) 13:15 – Session 1: Preserving scientific records: Scientists and their labs 14:45 Paper 1 Alice Perrin (Université Jean Moulin Lyon 3), Lucile Schirr (Université de Strasbourg) ‘Processing of scientific archives in a French university: The case of Pr Henri Danan’s /Pierre Weiss laboratory’s fond’ Paper 2 Christian Joas, Rob Sunderland (Niels Bohr Archive, Copenhagen) ‘The Niels Bohr Archive: Past, Present, and Future’ Paper 3 Alexandra Brovina (Federal Research Centre “Komi Science Centre of the Ural Branch of the Russian Academy of Sciences”) ‘Personal archives of researchers of the North of Russia: creation, preservation, information potential’ Chair: Laura Outterside 14:45 – Breakout session (details to follow) 15:15 15:15 – Session 2: When data become archives 16:45 Paper 4 Fernando B. Figueiredo, Paulo Ribeiro (University of Coimbra, Portugal) ‘The Scientific Data Archives of the Old Geophysical Institute of the University of Coimbra: How to preserve and make them available and workable for the current geoscientist community?’ Paper 5 Jennifer Cuffe (Library and Archives Canada) ‘Archiving scientific and research data in government: a motley of memory practices’ Paper 6 Polina E. -
A Brief History of Nuclear Astrophysics
A BRIEF HISTORY OF NUCLEAR ASTROPHYSICS Stellar Origin of Energy the Elements Nuclear Astrophysics Astrophysics Nuclear Physics A BRIEF HISTORY OF NUCLEAR ASTROPHYSICS PART I THE ENERGY OF STARS Thermodynamics: the age of the Earth and the energy of the Sun 1847 : Robert Julius von Mayer Sun heated by fall of meteors 1854 : Hermann von Helmholtz Gravitational energy of protosolar nebula turns into kinetic energy of meteors Time ~ 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 A gaseous, contracting and heating Sun Mean solar density : ~1.35 g/cc Sun liquid Incompressible 1860s: 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 - Lane -Ritter A gaseous, contracting and heating Sun Mean solar density : ~1.35 g/cc Sun liquid Incompressible 1860s: 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 - Lane -Ritter A gaseous, contracting and heating Sun Mean solar density : ~1.35 g/cc Sun liquid Incompressible 1860s: 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 - Lane -Ritter A gaseous, contracting and heating Sun Mean solar density : ~1.35 g/cc Sun liquid Incompressible 1860s: J.