TRACING the CONTRIBUTIONS ERNEST RUTHERFORD MADE to the NEXT GENERATION of SCIENTISTS a Thesis by AN
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James Chadwick: Ahead of His Time
July 15, 2020 James Chadwick: ahead of his time Gerhard Ecker University of Vienna, Faculty of Physics Boltzmanngasse 5, A-1090 Wien, Austria Abstract James Chadwick is known for his discovery of the neutron. Many of his earlier findings and ideas in the context of weak and strong nuclear forces are much less known. This biographical sketch attempts to highlight the achievements of a scientist who paved the way for contemporary subatomic physics. arXiv:2007.06926v1 [physics.hist-ph] 14 Jul 2020 1 Early years James Chadwick was born on Oct. 20, 1891 in Bollington, Cheshire in the northwest of England, as the eldest son of John Joseph Chadwick and his wife Anne Mary. His father was a cotton spinner while his mother worked as a domestic servant. In 1895 the parents left Bollington to seek a better life in Manchester. James was left behind in the care of his grandparents, a parallel with his famous predecessor Isaac Newton who also grew up with his grandmother. It might be an interesting topic for sociologists of science to find out whether there is a correlation between children educated by their grandmothers and future scientific geniuses. James attended Bollington Cross School. He was very attached to his grandmother, much less to his parents. Nevertheless, he joined his parents in Manchester around 1902 but found it difficult to adjust to the new environment. The family felt they could not afford to send James to Manchester Grammar School although he had been offered a scholarship. Instead, he attended the less prestigious Central Grammar School where the teaching was actually very good, as Chadwick later emphasised. -
Marie Curie and Her Time
Marie Curie and Her Time by Hélène Langevin-Joliot to pass our lives near each other hypnotized by our dreams, your patriotic dream, our humanitarian dream, arie Curie (1867–1934) belongs to that exclu- and our scientific dream.” sive group of women whose worldwide rec- Frederick Soddy wrote about Marie that she was Mognition and fame have endured for a century “the most beautiful discovery of Pierre Curie.” Of or more. She was indeed one of the major agents of course, it might also be said that Pierre Curie was the scientific revolution which allowed experimen- “the most beautiful discovery of Marie Skłodowska.” tal investigation to extend beyond the macroscopic It is difficult to imagine more contrasting personali- world. Her work placed the first stone in the founda- ties than those of Pierre and of Marie. In spite of that, tion of a new discipline: radiochemistry. And Curie’s or because of that, they complemented each other achievements are even more remarkable since they astonishingly well. Pierre was as dreamy as Marie was occurred in the field of science, an intellectual activ- organized. At the same time, they shared similar ideas ity traditionally forbidden to women. However, these about family and society. accomplishments alone don’t seem to fully explain the near mythic status of Marie Curie today. One hundred years ago, she was often considered to be just an assistant to her husband. Perhaps the reason her name still resonates is because of the compelling story of her life and her intriguing personality. The Most Beautiful Discovery of Pierre Curie The story of the young Maria Skłodowska leaving In this iconic photograph of participants at the Fifth her native Poland to pursue upper-level studies in Solvay Conference in 1927, Marie Curie is third from Paris sounds like something out of a novel. -
George De Hevesy in America
Journal of Nuclear Medicine, published on July 13, 2019 as doi:10.2967/jnumed.119.233254 George de Hevesy in America George de Hevesy was a Hungarian radiochemist who was awarded the Nobel Prize in Chemistry in 1943 for the discovery of the radiotracer principle (1). As the radiotracer principle is the foundation of all diagnostic and therapeutic nuclear medicine procedures, Hevesy is widely considered the father of nuclear medicine (1). Although it is well-known that he spent time at a number of European institutions, it is not widely known that he also spent six weeks at Cornell University in Ithaca, NY, in the fall of 1930 as that year’s Baker Lecturer in the Department of Chemistry (2-6). “[T]he Baker Lecturer gave two formal presentations per week, to a large and diverse audience and provided an informal seminar weekly for students and faculty members interested in the subject. The lecturer had an office in Baker Laboratory and was available to faculty and students for further discussion.” (7) There is also evidence that, “…Hevesy visited Harvard [University, Cambridge, MA] as a Baker Lecturer at Cornell in 1930…” (8). Neither of the authors of this Note/Letter was aware of Hevesy’s association with Cornell University despite our longstanding ties to Cornell until one of us (WCK) noticed the association in Hevesy’s biographical page on the official Nobel website (6). WCK obtained both his undergraduate degree and medical degree from Cornell in Ithaca and New York City, respectively, and spent his career in nuclear medicine. JRO did his nuclear medicine training at Columbia University and has subsequently been a faculty member of Weill Cornell Medical College for the last eleven years (with a brief tenure at Memorial Sloan Kettering Cancer Center (affiliated with Cornell)), and is now the program director of the Nuclear Medicine residency and Chief of the Molecular Imaging and Therapeutics Section. -
Physics Connections
Charles Tracy L P S / y a a w s n e v a R n a v v e l t e D Physics connections Last year we celebrated the International Year of Physics — time and light. In particular, it described how space also known as Einstein Year. In the century since Einstein’s becomes distorted near a massive object such as a star, so that light follows a curved path rather than annus mirabilis (see CATALYST Vol. 16, No. 1) there has travelling in a straight line (Figure 1). been a revolution in the study of physics. This article explores Its publication in wartime and the fact that it was the links between some of the architects of this revolution. written in German meant that few people read it. However, one person who did read it was the British astronomer Arthur Eddington. The story goes that it was Eddington who brought Einstein to the world’s attention — though Einstein might have disagreed. instein did not become instantly famous in Eddington was a conscientious objector. As such, GCSE key words 1905; it took several years before he became a he should have spent the war in jail. Instead, he got Gravity Eglobal icon. In 1915, while Europe was caught official permission to prepare for a trip to observe a Alpha particle scattering up in the First World War, Einstein broadened his total eclipse of the Sun — a rare event. His intention Nuclear fission special theory of relativity. His general theory of was to verify Einstein’s general theory of relativity. -
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. -
Ernest Rutherford and the Accelerator: “A Million Volts in a Soapbox”
Ernest Rutherford and the Accelerator: “A Million Volts in a Soapbox” AAPT 2011 Winter Meeting Jacksonville, FL January 10, 2011 H. Frederick Dylla American Institute of Physics Steven T. Corneliussen Jefferson Lab Outline • Rutherford's call for inventing accelerators ("million volts in a soap box") • Newton, Franklin and Jefferson: Notable prefiguring of Rutherford's call • Rutherfords's discovery: The atomic nucleus and a new experimental method (scattering) • A century of particle accelerators AAPT Winter Meeting January 10, 2011 Rutherford’s call for inventing accelerators 1911 – Rutherford discovered the atom’s nucleus • Revolutionized study of the submicroscopic realm • Established method of making inferences from particle scattering 1927 – Anniversary Address of the President of the Royal Society • Expressed a long-standing “ambition to have available for study a copious supply of atoms and electrons which have an individual energy far transcending that of the alpha and beta particles” available from natural sources so as to “open up an extraordinarily interesting field of investigation.” AAPT Winter Meeting January 10, 2011 Rutherford’s wish: “A million volts in a soapbox” Spurred the invention of the particle accelerator, leading to: • Rich fundamental understanding of matter • Rich understanding of astrophysical phenomena • Extraordinary range of particle-accelerator technologies and applications AAPT Winter Meeting January 10, 2011 From Newton, Jefferson & Franklin to Rutherford’s call for inventing accelerators Isaac Newton, 1717, foreseeing something like quarks and the nuclear strong force: “There are agents in Nature able to make the particles of bodies stick together by very strong attractions. And it is the business of Experimental Philosophy to find them out. -
The Nobel Laureate George De Hevesy (1885-1966) - Universal Genius and Father of Nuclear Medicine Niese S* Am Silberblick 9, 01723 Wilsdruff, Germany
Open Access SAJ Biotechnology LETTER ISSN: 2375-6713 The Nobel Laureate George de Hevesy (1885-1966) - Universal Genius and Father of Nuclear Medicine Niese S* Am Silberblick 9, 01723 Wilsdruff, Germany *Corresponding author: Niese S, Am Silberblick 9, 01723 Wilsdruff, Germany, Tel: +49 35209 22849, E-mail: [email protected] Citation: Niese S, The Nobel Laureate George de Hevesy (1885-1966) - Universal Genius and Father of Nuclear Medicine. SAJ Biotechnol 5: 102 Article history: Received: 20 March 2018, Accepted: 29 March 2018, Published: 03 April 2018 Abstract The scientific work of the universal genius the Nobel Laureate George de Hevesy who has discovered and developed news in physics, chemistry, geology, biology and medicine is described. Special attention is given to his work in life science which he had done in the second half of his scientific career and was the base of the development of nuclear medicine. Keywords: George de Hevesy; Radionuclides; Nuclear Medicine Introduction George de Hevesy has founded Radioanalytical Chemistry and Nuclear Medicine, discovered the element hafnium and first separated stable isotopes. He was an inventor in many disciplines and his interest was not only focused on the development and refinement of methods, but also on the structure of matter and its changes: atoms, molecules, cells, organs, plants, animals, men and cosmic objects. He was working under complicated political situation in Europe in the 20th century. During his stay in Germany, Austria, Hungary, Switzerland, Denmark, and Sweden he wrote a lot papers in German. In 1962 he edited a large part of his articles in a collection where German papers are translated in English [1]. -
Appendix E Nobel Prizes in Nuclear Science
Nuclear Science—A Guide to the Nuclear Science Wall Chart ©2018 Contemporary Physics Education Project (CPEP) Appendix E Nobel Prizes in Nuclear Science Many Nobel Prizes have been awarded for nuclear research and instrumentation. The field has spun off: particle physics, nuclear astrophysics, nuclear power reactors, nuclear medicine, and nuclear weapons. Understanding how the nucleus works and applying that knowledge to technology has been one of the most significant accomplishments of twentieth century scientific research. Each prize was awarded for physics unless otherwise noted. Name(s) Discovery Year Henri Becquerel, Pierre Discovered spontaneous radioactivity 1903 Curie, and Marie Curie Ernest Rutherford Work on the disintegration of the elements and 1908 chemistry of radioactive elements (chem) Marie Curie Discovery of radium and polonium 1911 (chem) Frederick Soddy Work on chemistry of radioactive substances 1921 including the origin and nature of radioactive (chem) isotopes Francis Aston Discovery of isotopes in many non-radioactive 1922 elements, also enunciated the whole-number rule of (chem) atomic masses Charles Wilson Development of the cloud chamber for detecting 1927 charged particles Harold Urey Discovery of heavy hydrogen (deuterium) 1934 (chem) Frederic Joliot and Synthesis of several new radioactive elements 1935 Irene Joliot-Curie (chem) James Chadwick Discovery of the neutron 1935 Carl David Anderson Discovery of the positron 1936 Enrico Fermi New radioactive elements produced by neutron 1938 irradiation Ernest Lawrence -
Nomenclatural Studies Toward a World List of Diptera Genus-Group Names
Nomenclatural studies toward a world list of Diptera genus-group names. Part V Pierre-Justin-Marie Macquart Evenhuis, Neal L.; Pape, Thomas; Pont, Adrian C. DOI: 10.11646/zootaxa.4172.1.1 Publication date: 2016 Document version Publisher's PDF, also known as Version of record Document license: CC BY Citation for published version (APA): Evenhuis, N. L., Pape, T., & Pont, A. C. (2016). Nomenclatural studies toward a world list of Diptera genus- group names. Part V: Pierre-Justin-Marie Macquart. Magnolia Press. Zootaxa Vol. 4172 No. 1 https://doi.org/10.11646/zootaxa.4172.1.1 Download date: 02. Oct. 2021 Zootaxa 4172 (1): 001–211 ISSN 1175-5326 (print edition) http://www.mapress.com/j/zt/ Monograph ZOOTAXA Copyright © 2016 Magnolia Press ISSN 1175-5334 (online edition) http://doi.org/10.11646/zootaxa.4172.1.1 http://zoobank.org/urn:lsid:zoobank.org:pub:22128906-32FA-4A80-85D6-10F114E81A7B ZOOTAXA 4172 Nomenclatural Studies Toward a World List of Diptera Genus-Group Names. Part V: Pierre-Justin-Marie Macquart NEAL L. EVENHUIS1, THOMAS PAPE2 & ADRIAN C. PONT3 1 J. Linsley Gressitt Center for Entomological Research, Bishop Museum, 1525 Bernice Street, Honolulu, Hawaii 96817-2704, USA. E-mail: [email protected] 2 Natural History Museum of Denmark, Universitetsparken 15, 2100 Copenhagen, Denmark. E-mail: [email protected] 3Oxford University Museum of Natural History, Parks Road, Oxford OX1 3PW, UK. E-mail: [email protected] Magnolia Press Auckland, New Zealand Accepted by D. Whitmore: 15 Aug. 2016; published: 30 Sept. 2016 Licensed under a Creative Commons Attribution License http://creativecommons.org/licenses/by/3.0 NEAL L. -
Cockcroft: a Novel This One, the Comprehensive Compilation Lutely Fundamental Discovery
~7~~-------------------------------------SPRINGBCXJKS------------------------N_A_ru_~__ v_o_L._Jo_s_~_AP __ Rr_L_r9M_ same, when it's compiled as successfully as what was in the sheer physics of it an abso Cockcroft: a novel this one, the comprehensive compilation lutely fundamental discovery. The authors perspective undeniably earns its place in the library. of this book take in their stride Cockcroft I was an admirer of Cockcroft, a fine, and Walton's being made to wait so long William Cooper stocky, sensible, cautious Yorkshireman, theirs not to reason why, they say. But what who indulged in a minimum of speech and about ours? Did it take the Nobel Cockcroft and the Atom. in practically no change of facial committee nineteen years to recognize the By Guy Hartcup and T.E. Allibone. expression. (That expression was neverthe experiment as breaking open an entirely Adam Hilger, Bristol!Heyden, Phila- less amiable, thoughtful, smiling.) If one new line of powerful experiments to be delphia: 1984. Pp.320. £18.95, $34. addressed a remark to him, it was only made with particle-accelerators? Or did it when, after the ensuing silence, he either take those members who opposed the took the famous black notebook out of his award all that time to disappear from the SrNCE the title of Hartcup and Allibone's pocket or actually said something, that one scene? Or what? Someone must know. book may sound a bit vague, perhaps I knew for certain that he'd heard. It gave me There's a fascinating detail I should really should begin by saying what Cockcroft and lasting pleasure to think that at a dinner like to be told. -
Wilhelm Ostwald – the Scientist
ARTICLE-IN-A-BOX Wilhelm Ostwald – The Scientist Friedrich Wilhelm Ostwald was born on September 2, 1853 at Riga, Latvia, Russia to Gottfried Ostwald, a master cooper and Elisabeth Leuckel. He was the second son to his parents who both were descended from German immigrants. He had his early education at Riga. His subsequent education was at the University of Dorpat (now Tartu, Estonia) where he enrolled in 1872. At the university he studied chemistry under the tutelage of Carl ErnstHeinrich Schmidt (1822– 1894) who again was a pupil of Justus von Liebig. Besides Schmidt, Johannes Lemberg (1842– 1902) and Arthur von Oettingen (1836–1920) who were his teachers in physical chemistry were also principal influences. It was in 1877 that he defended his thesis ‘Volumchemische Studien über Affinität’. Subsequently he taught as Privatdozent for a couple of years. During this period, his personal life saw some changes as well. He wedded Helene von Reyher (1854–1946) in 1880. With Helene, he had three sons, and two daughters. Amongst his children, Wolfgang went on to become a famous colloid chemist. On the strength of recommendation from Dorpat, Ostwald was appointed as a Professor at Riga Polytechnicum in 1882. He worked on multiple applications of the law of mass action. He also conducted measurements in chemical reaction kinetics as well as conductivity of solutions. To this end, the pyknometer was developed which was used to determine the density of liquids. He also had a thermostat built and both of these were named after him. He was prolific in his teaching and research which helped establish a school of science at the university. -
The Bullard, Everett and Smith Reconstruction of the Circum-Atlantic Continents
1 GENESIS OF A GEOPHYSICAL ICON: THE BULLARD, EVERETT AND SMITH RECONSTRUCTION OF THE CIRCUM-ATLANTIC CONTINENTS J. E. EVERETT Faculty of Economics and Commerce The University of Western Australia, Nedlands, Western Australia 6009 [email protected] A. G. SMITH Department of Earth Sciences, Sedgwick Museum, Downing Street, Cambridge CB2 3EQ, U.K. [email protected] ABSTRACT The first computer fit of the continents had its origins in a controversy over Warren Carey’s visual fit between South America and Africa. Sir Harold Jeffreys denied that there was a fit, but Sir Edward Bullard considered the fit to be impressive. Bullard suggested quantifying the fit to Jim Everett, a graduate student at the time. Everett did so, developing his own method from his mathematical background, and computed the fit for the South Atlantic. Alan Smith, then a research assistant, used his geological knowledge and worked with Everett to fit together all the circum-Atlantic continents. Thus Bullard had the idea of quantifying the fit, and Everett and Smith implemented it. Then Smith extended the method to fits beyond the Earth Sciences History Atlantic. The outcome owed much to Bullard’s leadership, and to the lively v. 27, no. 1, 2008 and open discussions that prevailed during coffee and tea at Madingley pp. Rise, which housed the Department of Geodesy and Geophysics of the University of Cambridge at that time. 1. INTRODUCTION Bullard, Everett and Smith’s (1965) computer fit of the circum-Atlantic continents has become something of a geophysical icon. It gave rise to new ideas and set new approaches in motion, whose consequences are still being worked out today.