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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. -
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. -
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 -
(Owen Willans) Richardson
O. W. (Owen Willans) Richardson: An Inventory of His Papers at the Harry Ransom Center Descriptive Summary Creator: Richardson, O. W. (Owen Willans), 1879-1959 Title: O. W. (Owen Willans) Richardson Papers Dates: 1898-1958 (bulk 1920-1940) Extent: 112 document boxes, 2 oversize boxes (49.04 linear feet), 1 oversize folder (osf), 5 galley folders (gf) Abstract: The papers of Sir O. W. (Owen Willans) Richardson, the Nobel Prize-winning British physicist who pioneered the field of thermionics, contain research materials and drafts of his writings, correspondence, as well as letters and writings from numerous distinguished fellow scientists. Call Number: MS-3522 Language: Primarily English; some works and correspondence written in French, German, or Italian . Note: The Ransom Center gratefully acknowledges the assistance of the Center for History of Physics, American Institute of Physics, which provided funds to support the processing and cataloging of this collection. Access: Open for research Administrative Information Additional The Richardson Papers were microfilmed and are available on 76 Physical Format reels. Each item has a unique identifying number (W-xxxx, L-xxxx, Available: R-xxxx, or M-xxxx) that corresponds to the microfilm. This number was recorded on the file folders housing the papers and can also be found on catalog slips present with each item. Acquisition: Purchase, 1961 (R43, R44) and Gift, 2005 Processed by: Tessa Klink and Joan Sibley, 2014 Repository: The University of Texas at Austin, Harry Ransom Center Richardson, O. W. (Owen Willans), 1879-1959 MS-3522 2 Richardson, O. W. (Owen Willans), 1879-1959 MS-3522 Biographical Sketch The English physicist Owen Willans Richardson, who pioneered the field of thermionics, was also known for his work on photoelectricity, spectroscopy, ultraviolet and X-ray radiation, the electron theory, and quantum theory. -
Commentary & Notes Hans Bethe
J. Natn.Sci.Foundation Sri Lanka 2005 33(1): 57-58 COMMENTARY & NOTES HANS BETHE (1906-2005) Hans Albrecht Bethe who died on 6 March 2005 within the sun is hydrogen which is available in at the age of 98, was one of the most influential tremendous volume. Near the centre of the sun, and innovative theoretical physicists of our time. hydrogen nuclei can be squeezed under enormous pressure to become the element helium. If the Bethe was born in Strasbourg, Alsace- mass of hydrogen nucleus can be written as 1, Lorraine (then part of Germany) on 2 July 1906. Bethe showed that each time four nuclei of His father was a University physiologist and his hydrogen fused together as helium, their sum was mother Jewish, the daughter of a Strasbourg not equal to 4. The helium nucleus weighs about professor of Medicine. Bethe moved to Kiel and 0.7% less, or just 3.993 units of weight. It is this Frankfurt from where he went to Munich to carry missing 0.7% that comes out as a burst of explosive out research in theoretical physics under Arnold energy. The sun is so powerful that it pumps 4 Sommerfeld, who was not only a great teacher, million tons of hydrogen into pure energy every but an inspiring research supervisor as well. second. Einstein's famous equation, E = mc2, Bethe received his doctorate in 1928, for the work provides a clue to the massive energy that reaches he did on electron diffraction. He then went to the earth from the sun, when 4 million tons of the Cavendish laboratory in Cambridge on a hydrogen are multiplied by the figure c2 (square Rockefeller Fellowship, and Rome, before of the speed of light). -
James Chadwick and E.S
What is the Universe Made Of? Atoms - Electrons Nucleus - Nucleons Antiparticles And ... http://www.parentcompany.com/creation_explanation/cx6a.htm What Holds it Together? Gravitational Force Electromagnetic Force Strong Force Weak Force Timeline - Ancient 624-547 B.C. Thales of Miletus - water is the basic substance, knew attractive power of magnets and rubbed amber. 580-500 B.C. Pythagoras - Earth spherical, sought mathematical understanding of universe. 500-428 B.C. Anaxagoras changes in matter due to different orderings of indivisible particles (law of the conservation of matter) 484-424 B.C. Empedocles reduced indivisible particles into four elements: earth, air, fire, and water. 460-370 B.C. Democritus All matter is made of indivisible particles called atoms. 384-322 B.C. Aristotle formalized the gathering of scientific knowledge. 310-230 B.C. Aristarchus describes a cosmology identical to that of Copernicus. 287-212 B.C. Archimedes provided the foundations of hydrostatics. 70-147 AD Ptolemy of Alexandria collected the optical knowledge, theory of planetary motion. 1214-1294 AD Roger Bacon To learn the secrets of nature we must first observe. 1473-1543 AD Nicholaus Copernicus The earth revolves around the sun Timeline – Classical Physics 1564-1642 Galileo Galilei - scientifically deduced theories. 1546-1601, Tycho Brahe accurate celestial data to support Copernican system. 1571-1630, Johannes Kepler. theory of elliptical planetary motion 1642-1727 Sir Isaac Newton laws of mechanics explain motion, gravity . 1773-1829 Thomas Young - the wave theory of light and light interference. 1791-1867 Michael Faraday - the electric motor, and electromagnetic induction, electricity and magnetism are related. electrolysis, conservation of energy. -
Hitler's Uranium Club, the Secret Recordings at Farm Hall
HITLER’S URANIUM CLUB DER FARMHALLER NOBELPREIS-SONG (Melodie: Studio of seiner Reis) Detained since more than half a year Ein jeder weiss, das Unglueck kam Sind Hahn und wir in Farm Hall hier. Infolge splitting von Uran, Und fragt man wer is Schuld daran Und fragt man, wer ist Schuld daran, So ist die Antwort: Otto Hahn. So ist die Antwort: Otto Hahn. The real reason nebenbei Die energy macht alles waermer. Ist weil we worked on nuclei. Only die Schweden werden aermer. Und fragt man, wer ist Schuld daran, Und fragt man, wer ist Schuld daran, So ist die Antwort: Otto Hahn. So ist die Antwort: Otto Hahn. Die nuclei waren fuer den Krieg Auf akademisches Geheiss Und fuer den allgemeinen Sieg. Kriegt Deutschland einen Nobel-Preis. Und fragt man, wer ist Schuld daran, Und fragt man, wer ist Schuld daran, So ist die Antwort: Otto Hahn. So ist die Antwort: Otto Hahn. Wie ist das moeglich, fragt man sich, In Oxford Street, da lebt ein Wesen, The story seems wunderlich. Die wird das heut’ mit Thraenen lesen. Und fragt man, wer ist Schuld daran Und fragt man, wer ist Schuld daran, So ist die Antwort: Otto Hahn. So ist die Antwort: Otto Hahn. Die Feldherrn, Staatschefs, Zeitungsknaben, Es fehlte damals nur ein atom, Ihn everyday im Munde haben. Haett er gesagt: I marry you madam. Und fragt man, wer ist Schuld daran, Und fragt man, wer ist Schuld daran, So ist die Antwort: Otto Hahn. So ist die Antwort: Otto Hahn. Even the sweethearts in the world(s) Dies ist nur unsre-erste Feier, Sie nennen sich jetzt: “Atom-girls.” Ich glaub die Sache wird noch teuer, Und fragt man, wer ist Schuld daran, Und fragt man, wer ist Schuld daran, So ist die Antwort: Otto Hahn. -
Some Famous Physicists Ing Weyl’S Book Space, Time, Matter, the Same Book That Heisenberg Had Read As a Young Man
Heisenberg’s first graduate student was Felix Bloch. One day, while walking together, they started to discuss the concepts of space and time. Bloch had just finished read- Some Famous Physicists ing Weyl’s book Space, Time, Matter, the same book that Heisenberg had read as a young man. Still very much Anton Z. Capri† under the influence of this scholarly work, Bloch declared that he now understood that space was simply the field of Sometimes we are influenced by teachers in ways that, affine transformations. Heisenberg paused, looked at him, although negative, lead to positive results. This happened and replied, “Nonsense, space is blue and birds fly through to Werner Heisenberg1 and Max Born,2 both of whom it.” started out to be mathematicians, but switched to physics There is another version of why Heisenberg switched to due to encounters with professors. physics. At an age of 19, Heisenberg went to the University As a young student at the University of Munich, Heisen- of G¨ottingen to hear lectures by Niels Bohr.4 These lec- berg wanted to attend the seminar of Professor F. von tures were attended by physicists and their students from Lindemann,3 famous for solving the ancient problem of various universities and were jokingly referred to as “the squaring the circle. Heisenberg had Bohr festival season.” Here, Bohr expounded on his latest read Weyl’s book Space, Time, Matter theories of atomic structure. The young Heisenberg in the and, both excited and disturbed by the audience did not hesitate to ask questions when Bohr’s abstract mathematical arguments, had explanations were less than clear. -
Father of the Shell Model
CENTENARY Father of the shell model Heidelberg University held a symposium on fundamental physics and the shell model this summer to celebrate the 100th anniversary of the birth of Hans Jensen, the German who created the nuclear shell model with Maria Goeppert-Mayer of Argonne. Hans Jensen (1907–1973) is the only theorist among the three winners from Heidelberg University of the Nobel Prize for Physics. He shared the award with Maria Goeppert-Mayer in 1963 for the development of the nuclear shell model, which they published independently in 1949. The model offered the first coherent expla- nation for the variety of properties and structures of atomic nuclei. In particular, the “magic numbers” of protons and neutrons, which had been determined experimentally from the stability properties and observed abundances of chemical elements, found a natural explanation in terms of the spin-orbit coupling of the nucleons. These numbers play a decisive role in the synthesis of the ele- ments in stars, as well as in the artificial synthesis of the heaviest elements at the borderline of the periodic table of elements. Hans Jensen was born in Hamburg on 25 June 1907. He studied physics, mathematics, chemistry and philosophy in Hamburg and Freiburg, obtaining his PhD in 1932. After a short period in the Hans Jensen in his study at 16 Philosophenweg, Heidelberg German army’s weather service, he became professor of theo- in 1963. (Courtesy Bettmann/UPI/Corbis.) retical physics in Hannover in 1940. Jensen then accepted a new chair for theoretical physics in Heidelberg in 1949 on the initiative Mayer 1949). -
Managing Science: Methodology and Organization of Research
Innovation, Technology, and Knowledge Management Series Editor Elias G. Carayannis, George Washington University, Washington D.C., USA For other titles published in this series, go to www.springer.com/series/8124 wwwwwwwww Frederick Betz Managing Science Methodology and Organization of Research Frederick Betz Department of Engineering and Technology Portland State University Portland, OR USA [email protected] ISBN 978-1-4419-7487-7 e-ISBN 978-1-4419-7488-4 DOI 10.1007/978-1-4419-7488-4 Springer New York Dordrecht Heidelberg London © Springer Science+Business Media, LLC 2011 All rights reserved. This work may not be translated or copied in whole or in part without the written permission of the publisher (Springer Science+Business Media, LLC, 233 Spring Street, New York, NY 10013, USA), except for brief excerpts in connection with reviews or scholarly analysis. Use in connection with any form of information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed is forbidden. The use in this publication of trade names, trademarks, service marks, and similar terms, even if they are not identified as such, is not to be taken as an expression of opinion as to whether or not they are subject to proprietary rights. Printed on acid-free paper Springer is part of Springer Science+Business Media (www.springer.com) For Nancy, my dear wife who has been with me on this journey through life, while also being a marvelously insightful editor. wwwwwwwww Series Foreword The Springer Book Series on Innovation, Technology, and Knowledge Management was launched in March 2008 as a forum and intellectual, scholarly “podium” for global/local (gloCal), transdisciplinary, trans-sectoral, public–private, leading/“bleeding”-edge ideas, theories, and perspectives on these topics. -
Rutherford's Pillow
Rutherford’s Pillow Estimated Time: 20-30 minutes SUMMARY The modern understanding of the atom with its small nucleus and cloud of electrons was supported by an early experiment by a group of scientists. It involved throwing subatomic particles at a very thin sheet of gold and noticing that the particles mostly flew through because of the empty space. Students can set up their own experiment at home to repeat this and have some fun too! WHAT YOU’LL LEARN • How scientists discovered the size and location of atomic nuclei. • How to use your senses to determine something logically. Materials Used • Pillow (more, optionally) • Blindfold • Rope • Yard stick or other long pole Resources Used Khan Academy: https://www.youtube.com/watch?v=bVlwH1kfDeg&feature=youtu.be WHAT TO DO 1. Have the student leave the room while you set up the demonstration. Before they enter the room, put a blindfold on the student so that they cannot see what you set up. 2. For the activity set up, take the pillow and tie a rope around it. Using furniture or just having someone holding it, hang the pillow in the air. 3. Give the yard stick to the blindfolded student and have them swing the stick slowly. After they connect with the pillow a few times, have the student guess how big the pillow is and what the shape is. 4. If time and materials permit, try different pillows to find different sizes and shapes. TIPS • The Geiger-Marsden experiment, usually called the “Rutherford Gold Foil Experiment” was crucial to understanding atoms. -
Rutherford and Radon
Rediscovery of the Elements Rutherford and Radon U transmutation of the elements. He was to be (1877-1956) he developed the "transformation U acknowledged as the "leading explorer of the theory" which showed radioactivity was a vast, infinitely complex universe within the nuclear property. From thorium Rutherford atom, a universe that he was the first to pene- observed a gaseous radioactive product, which trate."3 he called "emanation"-he had discovered the Ernest Rutherford, the son of a flax farmer in element radon.' New Zealand, gained his undergraduate train- The British method of developing explicit ing in his native country. In 1895 he moved to descriptive models to explain nature was per- England, where he attended Cambridge Univ- fect for the advance of nuclear chemistry at this ersity; he was entering the scientific scene in moment in history; Lord Kelvin (William Europe just as radioactivity was discovered in Thomson, 1824-1907) said he could not reason 1896 by Henri Becquerel (1852-1908) of Paris. "without making a visualizable picture" of the His first research involved hertzian (radio) phenomenon he wanted to describe. J. J. James L. Marshal, beta Eta 1971, and waves, but he then moved on to the study of Thomson of the Cavendish Laboratory at Virginia R. Marshall, Beta Eta 2003, uranium rays with J. J. Thomson (1856-1940) at Cambridge was using the idea of charged cor- Department of Chemistry, University of Cambridge. Rutherford showed that these ion- puscles to explain cathode rays, and he viewed North Texas, Denton,TX 76203-5070, izing rays consisted of two main types, which the atom as a dynamic, moving mixture of pos- he called alpha and beta "for simplicity."2 itive and negative charges.