75 Years of Fission
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Prehistory of CERN: the First Suggestions (1949-Jun 1950)
CHS-3 March 1984 STUDIES IN CERN HISTORY Prehistory of CERN : the first suggestions (1949 - June 1950) Dominique Pestre GENEVA 1984 The Study of CERN History is a project financed by Institutions in several CERN Member Countries. This report presents preliminary findings. and is intended for incorporation into a more comprehensive study of CERN's history. It is distributed primarily to historians and scientists to provoke discussion, and no part of it should be cited or reproduced without written permission from the Team Leacier. Comments are welcome and should be sent to: Study Team for CERN History c/oCERN CH-1211 GENEVE23 Switzerland © Copyright Study Team for CERN History, Geneva 1984 CERN-Service d'information scientifique - 300 - mars 1984 PREHISTORY OF CERN THE FIRST SUGGESTIONS (1949 - June 1950) I The years following the war II Two proposals of European collaboration in November 1949 III The European Cultural Conference, Lausanne, December 8-12, 1949 IV Attempts to implement the suggestions a - The European Movement initiative b - The French attempts V The fifth General Conference of UNESCO, Florence, June 1950 PREHISTORY OF CERN: THE FIRST SUGGESTIONS (1949-June 1950) 1 The official date of the foundation of CERN is easily established. The convention setting up CERN, signed on July 1, 1953 was ratified by France and Germany on September 29, 1954. By then nine States had signed, and CERN came officially into being. However, the interest of this date is rather limited. It ended a process initiated several years before and understanding this process is far more interesting than having a date of birth. -
1 the Equation of a Light Leptonic Magnetic Monopole and Its
The equation of a Light Leptonic Magnetic Monopole and its Experimental Aspects Georges Lochak Fondation Louis de Broglie 23, rue Marsoulan F-75012 Paris [email protected] Abstract. The present theory is closely related to Dirac’s equation of the electron, but not to his magnetic monopole theory, except for his relation between electric and magnetic charge. The theory is based on the fact, that the massless Dirac equation admits a second electromagnetic coupling, deduced from a pseudo-scalar gauge invariance. The equation thus obtained has the symmetry laws of a massless leptonic, magnetic monopole, able to interact weakly. We give a more precise form of the Dirac relation between electric and magnetic charges and a quantum form of the Poincaré first integral. In the Weyl representation our equation splits into P-conjugated monopole and antimonopole equations with the correct electromagnetic coupling and opposite chiralities, predicted by P. Curie. Charge conjugated monopoles are symmetric in space and not in time (contrary to the electric particles) : an important fact for the vacuum polarization. Our monopole is a magnetically excited neutrino, which leads to experimental consequences. These monopoles are assumed to be produced by electromagnetic pulses or arcs, leading to nuclear transmutations and, for beta radioactive elements, a shortening of the life time and the emission of monopoles instead of neutrinos in a magnetic field. A corresponding discussion is given in section 15. 1. Introduction. The hypothesis of separated magnetic poles is very old. In the 2nd volume of his famous Treatise of Electricity and Magnetism [1], devoted to Magnetism, Maxwell considered the existence of free magnetic charges as an evidence, just as the evidence of electric charges. -
Unerring in Her Scientific Enquiry and Not Afraid of Hard Work, Marie Curie Set a Shining Example for Generations of Scientists
Historical profile Elements of inspiration Unerring in her scientific enquiry and not afraid of hard work, Marie Curie set a shining example for generations of scientists. Bill Griffiths explores the life of a chemical heroine SCIENCE SOURCE / SCIENCE PHOTO LIBRARY LIBRARY PHOTO SCIENCE / SOURCE SCIENCE 42 | Chemistry World | January 2011 www.chemistryworld.org On 10 December 1911, Marie Curie only elements then known to or ammonia, having a water- In short was awarded the Nobel prize exhibit radioactivity. Her samples insoluble carbonate akin to BaCO3 in chemistry for ‘services to the were placed on a condenser plate It is 100 years since and a chloride slightly less soluble advancement of chemistry by the charged to 100 Volts and attached Marie Curie became the than BaCl2 which acted as a carrier discovery of the elements radium to one of Pierre’s electrometers, and first person ever to win for it. This they named radium, and polonium’. She was the first thereby she measured quantitatively two Nobel prizes publishing their results on Boxing female recipient of any Nobel prize their radioactivity. She found the Marie and her husband day 1898;2 French spectroscopist and the first person ever to be minerals pitchblende (UO2) and Pierre pioneered the Eugène-Anatole Demarçay found awarded two (she, Pierre Curie and chalcolite (Cu(UO2)2(PO4)2.12H2O) study of radiactivity a new atomic spectral line from Henri Becquerel had shared the to be more radioactive than pure and discovered two new the element, helping to confirm 1903 physics prize for their work on uranium, so reasoned that they must elements, radium and its status. -
Rutherford's Nuclear World: the Story of the Discovery of the Nuc
Rutherford's Nuclear World: The Story of the Discovery of the Nuc... http://www.aip.org/history/exhibits/rutherford/sections/atop-physic... HOME SECTIONS CREDITS EXHIBIT HALL ABOUT US rutherford's explore the atom learn more more history of learn about aip's nuclear world with rutherford about this site physics exhibits history programs Atop the Physics Wave ShareShareShareShareShareMore 9 RUTHERFORD BACK IN CAMBRIDGE, 1919–1937 Sections ← Prev 1 2 3 4 5 Next → In 1962, John Cockcroft (1897–1967) reflected back on the “Miraculous Year” ( Annus mirabilis ) of 1932 in the Cavendish Laboratory: “One month it was the neutron, another month the transmutation of the light elements; in another the creation of radiation of matter in the form of pairs of positive and negative electrons was made visible to us by Professor Blackett's cloud chamber, with its tracks curled some to the left and some to the right by powerful magnetic fields.” Rutherford reigned over the Cavendish Lab from 1919 until his death in 1937. The Cavendish Lab in the 1920s and 30s is often cited as the beginning of modern “big science.” Dozens of researchers worked in teams on interrelated problems. Yet much of the work there used simple, inexpensive devices — the sort of thing Rutherford is famous for. And the lab had many competitors: in Paris, Berlin, and even in the U.S. Rutherford became Cavendish Professor and director of the Cavendish Laboratory in 1919, following the It is tempting to simplify a complicated story. Rutherford directed the Cavendish Lab footsteps of J.J. Thomson. Rutherford died in 1937, having led a first wave of discovery of the atom. -
State of the Nation 2008 Canada’S Science, Technology and Innovation System
State of the Nation 2008 Canada’s Science, Technology and Innovation System Science, Technology and Innovation Council Science, Technology and Innovation Council Permission to Reproduce Except as otherwise specifically noted, the information in this publication may be reproduced, in part or in whole and by any means, without charge or further permission from the Science, Technology and Innovation Council (STIC), provided that due diligence is exercised in ensuring the accuracy of the information, that STIC is identified as the source institution, and that the reproduction is not represented as an official version of the information reproduced, nor as having been made in affiliation with, or with the endorsement of, STIC. © 2009, Government of Canada (Science, Technology and Innovation Council). Canada’s Science, Technology and Innovation System: State of the Nation 2008. All rights reserved. Aussi disponible en français sous le titre Le système des sciences, de la technologie et de l’innovation au Canada : l’état des lieux en 2008. This publication is also available online at www.stic-csti.ca. This publication is available upon request in accessible formats. Contact the Science, Technology and Innovation Council Secretariat at the number listed below. For additional copies of this publication, please contact: Science, Technology and Innovation Council Secretariat 235 Queen Street 9th Floor Ottawa ON K1A 0H5 Tel.: 613-952-0998 Fax: 613-952-0459 Web: www.stic-csti.ca Email: [email protected] Cat. No. 978-1-100-12165-9 50% ISBN Iu4-142/2009E recycled 60579 fiber State of the Nation 2008 Canada’s Science, Technology and Innovation System Science, Technology and Innovation Council Canada’s Science, Technology and Innovation System iii State of the Nation 2008 Canada’s Science, Technology and Innovation System Context and Executive Summary . -
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. -
HEAVY WATER and NONPROLIFERATION Topical Report
HEAVY WATER AND NONPROLIFERATION Topical Report by MARVIN M. MILLER MIT Energy Laboratory Report No. MIT-EL 80-009 May 1980 COO-4571-6 MIT-EL 80-009 HEAVY WATER AND NONPROLIFERATION Topical Report Marvin M. Miller Energy Laboratory and Department of Nuclear Engineering Massachusetts Institute of Technology Cambridge, Massachusetts 02139 May 1980 Prepared For THE U.S. DEPARTMENT OF ENERGY UNDER CONTRACT NO. EN-77-S-02-4571.A000 NOTICE This report was prepared as an account of work sponsored by the United States Government. Neither the United States nor the United States Department of Energy, nor any of their employees, nor any of their contractors, subcontractors, or their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or useful- ness of any information, apparatus, product or process disclosed or represents that its use would not infringe privately owned rights. A B S T R A C T The following report is a study of various aspects of the relationship between heavy water and the development of the civilian and military uses of atomic energy. It begins with a historical sketch which traces the heavy water storyfrom its discovery by Harold Urey in 1932 through its coming of age from scientific curiosity to strategic nuclear material at the eve of World War II and finally into the post-war period, where the military and civilian strands have some- times seemed inextricably entangled. The report next assesses the nonproliferation implications of the use of heavy water- moderated power reactors; several different reactor types are discussed, but the focus in on the natural uranium, on- power fueled, pressure tube reactor developed in Canada, the CANDU. -
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. -
Europe's Biggest General Science Conference Concludes Successfully
SCIENCEScience PagesPAGES Special Report - ESOF 2016 Europe’s biggest generalSpecial Report science conference concludes successfully ESOF 2016, Europe's biggest general science conference concludes successfully in Manchester,in Manchester,UK UK Theme: Science as Revolution Theme: Science as Revolution - Veena Patwardhan rom 23rd to 27th July, 2016, FManchester flaunted its City of Science status as the host city of the seventh edition of EuroScience Open Forum (ESOF 2016). A bi- ennial event held in a different European city every two years, this time it was Manchester's turn to host this globally reputed science conference. Around 4500 delegates – scien- tists, innovators, academics, young researchers, journalists, policy makers, industry representatives and others – converged on the world's first industrial city to dis- cover and have discussions about the latest advancements in scien- rd th Manchester Central, venue of ESOF 2016 tific and technological researchFrom 23 to 27 July, 2016, Manchester flaunted its City of Science status as the host city of the across Europe and beyond. The seventhmain theme edition this of EuroScienceyear Laureates Open Forumand distinguished (ESOF 2016). Ascientists biennial inevent the held packed in a different was 'Science as Revolution', indicatingEuropean that city the every focus two of years,Exchange this time Hall it wasof Manchester Manchester's Central, turn to hostthe venuethis globally of the reputed the conference would be on how sciencescience andconference. technology conference. could transform life on the planet, revolutionise econo- The proceedings began with a string quartet render- mies, and help in overcoming challenges faced by global ing a piece of specially composed music. -
Date: To: September 22, 1 997 Mr Ian Johnston©
22-SEP-1997 16:36 NOBELSTIFTELSEN 4& 8 6603847 SID 01 NOBELSTIFTELSEN The Nobel Foundation TELEFAX Date: September 22, 1 997 To: Mr Ian Johnston© Company: Executive Office of the Secretary-General Fax no: 0091-2129633511 From: The Nobel Foundation Total number of pages: olO MESSAGE DearMrJohnstone, With reference to your fax and to our telephone conversation, I am enclosing the address list of all Nobel Prize laureates. Yours sincerely, Ingr BergstrSm Mailing address: Bos StU S-102 45 Stockholm. Sweden Strat itddrtSMi Suircfatan 14 Teleptelrtts: (-MB S) 663 » 20 Fsuc (*-«>!) «W Jg 47 22-SEP-1997 16:36 NOBELSTIFTELSEN 46 B S603847 SID 02 22-SEP-1997 16:35 NOBELSTIFTELSEN 46 8 6603847 SID 03 Professor Willis E, Lamb Jr Prof. Aleksandre M. Prokhorov Dr. Leo EsaJki 848 North Norris Avenue Russian Academy of Sciences University of Tsukuba TUCSON, AZ 857 19 Leninskii Prospect 14 Tsukuba USA MSOCOWV71 Ibaraki Ru s s I a 305 Japan 59* c>io Dr. Tsung Dao Lee Professor Hans A. Bethe Professor Antony Hewlsh Department of Physics Cornell University Cavendish Laboratory Columbia University ITHACA, NY 14853 University of Cambridge 538 West I20th Street USA CAMBRIDGE CB3 OHE NEW YORK, NY 10027 England USA S96 014 S ' Dr. Chen Ning Yang Professor Murray Gell-Mann ^ Professor Aage Bohr The Institute for Department of Physics Niels Bohr Institutet Theoretical Physics California Institute of Technology Blegdamsvej 17 State University of New York PASADENA, CA91125 DK-2100 KOPENHAMN 0 STONY BROOK, NY 11794 USA D anni ark USA 595 600 613 Professor Owen Chamberlain Professor Louis Neel ' Professor Ben Mottelson 6068 Margarldo Drive Membre de rinstitute Nordita OAKLAND, CA 946 IS 15 Rue Marcel-Allegot Blegdamsvej 17 USA F-92190 MEUDON-BELLEVUE DK-2100 KOPENHAMN 0 Frankrike D an m ar k 599 615 Professor Donald A. -
Otto Hahn Otto Hahn
R.N. 70269/98 Postal Registration No.: DL-SW-1/4082/15-17 ISSN : 0972-169X Date of posting: 26-27 of advance month Date of publication: 24 of advance month May 2017 Vol. 19 No. 8 Rs. 5.00 Otto Hahn Discoverer of Nuclear Fission Editorial: Consolidating 35 science communication activities in our country Otto Hahn: Discoverer of 34 Nuclear Fission Keep Your Eyes Healthy 31 Phenol: A Serious 30 Environmental Threat Accidental Discoveries in 28 Medical Science Cures for haemorrhoids— 24 Simple treatments and Surgeries Recent developments 21 in science and technology 36 Editorial Consolidating science communication activities in our country Dr. R. Gopichandran It is well known that the National Council of Science Museums of India’s leadership in science technology and innovation (STI) across the Ministry of Culture, Government of India, the National Institute the bilateral and multilateral framework also. The news feature service of Science Communication and Information Resources (NISCAIR) and the portal activity have well defined action plans to reach out to of CSIR, the National Council for Science and Technology fellow institutions and citizens with suitably embellished platform Communication (NCSTC) of the Department of Science and and opportunities for all to deliver together. Technology (DST), Government of India and Vigyan Prasar, also While these are interesting and extremely important, especially of DST, have been carrying out excellent science communication because they respond to the call to upscale and value add science activities over the years. It cannot be denied that the reach has been and technology communication, it is equally important to document quite significant collectively. -
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