Lars Vegard, Atomic Structure, and the Periodic System
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Evolution of Mathematics: a Brief Sketch
Open Access Journal of Mathematical and Theoretical Physics Mini Review Open Access Evolution of mathematics: a brief sketch Ancient beginnings: numbers and figures Volume 1 Issue 6 - 2018 It is no exaggeration that Mathematics is ubiquitously Sujit K Bose present in our everyday life, be it in our school, play ground, SN Bose National Center for Basic Sciences, Kolkata mobile number and so on. But was that the case in prehistoric times, before the dawn of civilization? Necessity is the mother Correspondence: Sujit K Bose, Professor of Mathematics (retired), SN Bose National Center for Basic Sciences, Kolkata, of invenp tion or discovery and evolution in this case. So India, Email mathematical concepts must have been seen through or created by those who could, and use that to derive benefit from the Received: October 12, 2018 | Published: December 18, 2018 discovery. The creative process of discovery and later putting that to use must have been arduous and slow. I try to look back from my limited Indian perspective, and reflect up on what might have been the course taken up by mathematics during 10, 11, 12, 13, etc., giving place value to each digit. The barrier the long journey, since ancient times. of writing very large numbers was thus broken. For instance, the numbers mentioned in Yajur Veda could easily be represented A very early method necessitated for counting of objects as Dasha 10, Shata (102), Sahsra (103), Ayuta (104), Niuta (enumeration) was the Tally Marks used in the late Stone Age. In (105), Prayuta (106), ArA bud (107), Nyarbud (108), Samudra some parts of Europe, Africa and Australia the system consisted (109), Madhya (1010), Anta (1011) and Parartha (1012). -
Henry Andrews Bumstead 1870-1920
NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA BIOGRAPHICAL MEMOIRS VOLUME XIII SECOND MEMOIR BIOGRAPHICAL MEMOIR OF HENRY ANDREWS BUMSTEAD 1870-1920 BY LEIGH PAGE PRESENTED TO THE ACADEMY AT THE ANNUAL MEETING, 1929 HENRY ANDREWS BUMSTEAD BY LIUGH PAGE Henry Andrews Bumstead was born in the small town of Pekin, Illinois, on March 12th, 1870, son of Samuel Josiah Bumstead and Sarah Ellen Seiwell. His father, who was a physician of considerable local prominence, had graduated from the medical school in Philadelphia and was one of the first American students of medicine to go to Vienna to complete his studies. While the family was in Vienna, Bumstead, then a child three years of age, learned to speak German as fluently as he spoke English, an accomplishment which was to prove valuable to him in his subsequent career. Bumstead was descended from an old New England family which traces its origin to Thomas Bumstead, a native of Eng- land, who settled in Boston, Massachusetts, about 1640. Many of his ancestors were engaged in the professions, his paternal grandfather, the Reverend Samuel Andrews Bumstead, being a graduate of Princeton Theological Seminary and a minister in active service. From them he inherited a keen mind and an unusually retentive memory. It is related that long before he had learned to read, his Sunday school teacher surprised his mother by complimenting her on the ease with which her son had rendered the Sunday lesson. It turned out that his mother made a habit of reading the lesson to Bumstead before he left for school, and the child's remarkable performance there was due to his ability to hold in his memory every word of the lesson after hearing it read to him a single time. -
Nuclear Fragmentation Reactions: from Basic Research to Medical Applications Igor N
Nuclear fragmentation reactions: from basic research to medical applications Igor N. Mishustin Frankfurt Institute for Advanced Studies (FIAS), J.W. Goethe Universität, Frankfurt am Main National Research Center “Kurchatov Institute”, Moscow Part 1: Introduction: Nuclear break-up processes Basic Research Statistical description of nuclear break-up Multifragmentation of nuclei Nuclear Liquid-Gas phase transition Applications Propagation of heavy ions through extended medium Cancer therapy with ion beams Transmutation of radioactive waste Conclusions Introduction: Nuclear break-up processes, historical remarks Anticipation of nuclear “explosions” Nobel prize in Physics (1922) “for his services in the investigation of the structure of atoms and of Niels Bohr (1885 – 1962) the radiation emanating from them" Evaporation/fission of compound nucleus t=0 fm/c t>1000 fm/c p A CN low excitation fission Compound Nucleus (CN) is an equilibrated hot nucleus whose excitation energy is distributed over many microscopic d.o.f. (introduced by Niels Bohr in 1936-39) Sequential evaporation model—Weiskopf 1937, Statistical fission model—Bohr-Wheeler 1939, Frenkel 1939 Nuclear break-up: multifragmentation t=0 fm/c t>100 fm/c p A pA collision spectator A or B spectator A moderate excitation peripheral spectator AB collision B slow expansion equilibrated system at freeze-out Power-low fragment mass distribution around critical point, Y(A)~A-τ Can be well understood within an equilibrium statistical approach Early 80s: Randrup&Koonin, D.H.E. Gross et al, Bondorf-Mishustin-Botvina, Hahn&Stoecker; Later: S. Das Gupta et al., Gulminelli et al, Raduta et al,... Explosive disintegration of nuclei t ≈ R/v < 50 fm/c t = 0 fm/c f hot foreball central AA collision compression+heating E>50 AMeV collective flow fast expansion of fragments Typically, exponential fragment mass distributions, Y(A)~exp(-bA) The stronger is flow-the smaller are fragments-mechanical rupture Dynamical modeling is required: QMD, IQMD, NMD, AMD, .. -
December 4, 1954 NATURE 1037
No. 4440 December 4, 1954 NATURE 1037 COPLEY MEDALLISTS, 1915-54 is that he never ventured far into interpretation or 1915 I. P. Pavlov 1934 Prof. J. S. Haldane prediction after his early studies in fungi. Here his 1916 Sir James Dewar 1935 Prof. C. T. R. Wilson interpretation was unfortunate in that he tied' the 1917 Emile Roux 1936 Sir Arthur Evans word sex to the property of incompatibility and 1918 H. A. Lorentz 1937 Sir Henry Dale thereby led his successors astray right down to the 1919 M. Bayliss W. 1938 Prof. Niels Bohr present day. In a sense the style of his work is best 1920 H. T. Brown 1939 Prof. T. H. Morgan 1921 Sir Joseph Larmor 1940 Prof. P. Langevin represented by his diagrams of Datura chromosomes 1922 Lord Rutherford 1941 Sir Thomas Lewis as packets. These diagrams were useful in a popular 1923 Sir Horace Lamb 1942 Sir Robert Robinson sense so long as one did not take them too seriously. 1924 Sir Edward Sharpey- 1943 Sir Joseph Bancroft Unfortunately, it seems that Blakeslee did take them Schafer 1944 Sir Geoffrey Taylor seriously. To him they were the real and final thing. 1925 A. Einstein 1945 Dr. 0. T. Avery By his alertness and ingenuity and his practical 1926 Sir Frederick Gow 1946 Dr. E. D. Adrian sense in organizing the Station for Experimental land Hopkins 1947 Prof. G. H. Hardy Evolution at Cold Spring Harbor (where he worked 1927 Sir Charles Sherring- 1948 . A. V. Hill Prof in 1942), ton 1949 Prof. G. -
Can Science Advance Effectively Through Philosophical Criticism and Reflection?
Can science advance effectively through philosophical criticism and reflection? ROBERTO TORRETTI Universidad de Puerto Rico ABSTRACT Prompted by Hasok Chang’s conception of the history and philosophy of science (HPS) as the continuation of science by other means, I examine the possibility of obtaining scientific knowledge through philosophical criticism and reflection, in the light of four historical cases, concerning (i) the role of absolute space in Newtonian dynamics, (ii) the purported contraction of rods and retardation of clocks in Special Relativity, (iii) the reality of the electromagnetic ether, and (iv) the so-called problem of time’s arrow. In all four cases it is clear that a better understanding of such matters can be achieved —and has been achieved— through conceptual analysis. On the other hand, however, it would seem that this kind of advance has more to do with philosophical questions in science than with narrowly scientific questions. Hence, if HPS in effect continues the work of science by other means, it could well be doing it for other ends than those that working scientists ordinarily have in mind. Keywords: Absolute space – Inertial frames – Length contraction – Clock retardation – Special relativity – Ether – Time – Time directedness – Entropy – Boltzmann entropy Philosophical criticism and the advancement of science 2 The mind will not readily give up the attempt to apprehend the exact formal character of the latent connexions between different physical agencies: and the history of discovery may be held perhaps to supply the strongest reason for estimating effort towards clearness of thought as of not less importance in its own sphere than exploration of phenomena. -
Lawrence Bragg's “Brainwave” Drives Father-Son Collaboration
www.mrs.org/publications/bulletin HISTORICAL NOTE Lawrence Bragg’s “Brainwave” Drives Father-Son Collaboration In 1912, some 17 years after the serendip- and quickly began to learn what he could itous discovery of x-rays by Wilhelm on the subject. Röntgen, a debate raged as to the wave or Until this point in his life, at age 42, particle nature of this radiation phenome- William later recalled, “It had never non. William Henry Bragg, a 50-year-old entered my head that I should do any professor of physics at Leeds University in research work.” His curiosity aroused by England, came down firmly on the side of his reading on radiation, he soon obtained particles, citing the bullet-like nature of the some radium samples and began the rays, and how they were preferentially experiments that were to make him a lead- scattered in the forward direction when ing figure in radiation theory in a few colliding with matter. Max von Laue of years’ time. He quickly developed novel Germany, having produced elegant spot- hypotheses about the nature of radioactiv- diffraction photographs of CuS by aiming ity. The penetrating power of x-rays, and x-rays at crystal samples, used the diffrac- the fact that they are not deflected by a tion behavior as evidence for the wave magnetic field, were accounted for by the argument. Experiments by Charles G. “neutral pair hypothesis,” which stated Barkla that demonstrated the polarization that x-rays consisted of “an electron which of x-rays confirmed the wave theory in the has assumed a cloak of darkness in the minds of many scientists. -
1 X-Ray Diffraction Masatsugu Sei Suzuki Department Of
x-ray diffraction Masatsugu Sei Suzuki Department of Physics, SUNY at Binghamton (Date: January 13, 2012) Sir William Henry Bragg OM, KBE, PRS] (2 July 1862 – 10 March 1942) was a British physicist, chemist, mathematician and active sportsman who uniquely shared a Nobel Prize with his son William Lawrence Bragg - the 1915 Nobel Prize in Physics. The mineral Braggite is named after him and his son. http://en.wikipedia.org/wiki/William_Henry_Bragg ________________________________________________________________________ Sir William Lawrence Bragg CH OBE MC FRS (31 March 1890 – 1 July 1971) was an Australian-born British physicist and X-ray crystallographer, discoverer (1912) of the Bragg law of X-ray diffraction, which is basic for the determination of crystal structure. He was joint winner (with his father, Sir William Bragg) of the Nobel Prize for Physics in 1915. http://en.wikipedia.org/wiki/William_Lawrence_Bragg 1 1. x-ray source Fig. Schematic diagram for the generation of x-rays. Metal target (Cu or Mo) is bombarded by accelerating electrons. The power of the system is given by P = I(mA) V(keV), where I is the current of cathode and V is the voltage between the anode and cathode. Typically, we have I = 30 mA and V = 50 kV: P = 1.5 kW. We use two kinds of targets to generate x-rays: Cu and Mo. The wavelength of CuK1, CuK2 and CuK lines are given by K1 1.540562 Å. K 2 = 1.544390 Å, K = 1.392218 Å. The intensity ratio of CuK1 and CuK2 lines is 2:1. The weighed average wavelength K is calculated as 2 K 1 K 2 = 1.54184 Å. -
Lsu-Physics Iq Test 3 Strikes You're
LSU-PHYSICS IQ TEST 3 STRIKES YOU'RE OUT For Physics Block Party on 9 September 2016: This was run where all ~70 people start answering each question, given out one-by-one. Every time a person missed an answer, they made a 'strike'. All was done with the Honor System for answers, plus a fairly liberal statement of what constitutes a correct answer. When the person accumulates three strikes, then they are out of the game. The game continue until only one person was left standing. Actually, there had to be one extra question to decide a tie-break between 2nd and 3rd place. The prizes were: FIRST PLACE: Ravi Rau, selecting an Isaac Newton 'action figure' SECOND PLACE: Juhan Frank, selecting an Albert Einstein action figure THIRD PLACE: Siddhartha Das, winning a Mr. Spock action figure. 1. What is Einstein's equation relating mass and energy? E=mc2 OK, I knew in advance that someone would blurt out the answer loudly, and this did happen. So this was a good question to make sure that the game flowed correctly. 2. What is the short name for the physics paradox depicted on the back of my Physics Department T-shirt? Schroedinger's Cat 3. Give the name of one person new to our Department. This could be staff, student, or professor. There are many answers, for example with the new profs being Tabatha Boyajian, Kristina Launey, Manos Chatzopoulos, and Robert Parks. Many of the people asked 'Can I just use myself?', with the answer being "Sure". 4. What Noble Gas is named after the home planet of Kal-El? Krypton. -
Absolute Zero, Absolute Temperature. Absolute Zero Is the Lowest
Contents Radioactivity: The First Puzzles................................................ 1 The “Uranic Rays” of Henri Becquerel .......................................... 1 The Discovery ............................................................... 2 Is It Really Phosphorescence? .............................................. 4 What Is the Nature of the Radiation?....................................... 5 A Limited Impact on Scientists and the Public ............................ 6 Why 1896? .................................................................. 7 Was Radioactivity Discovered by Chance? ................................ 7 Polonium and Radium............................................................. 9 Marya Skłodowska .......................................................... 9 Pierre Curie .................................................................. 10 Polonium and Radium: Pierre and Marie Curie Invent Radiochemistry.. 11 Enigmas...................................................................... 14 Emanation from Thorium ......................................................... 17 Ernest Rutherford ........................................................... 17 Rutherford Studies Radioactivity: ˛-and ˇ-Rays.......................... 18 ˇ-Rays Are Electrons ....................................................... 19 Rutherford in Montreal: The Radiation of Thorium, the Exponential Decrease........................................... 19 “Induced” and “Excited” Radioactivity .................................... 20 Elster -
Ether and Electrons in Relativity Theory (1900-1911) Scott Walter
Ether and electrons in relativity theory (1900-1911) Scott Walter To cite this version: Scott Walter. Ether and electrons in relativity theory (1900-1911). Jaume Navarro. Ether and Moder- nity: The Recalcitrance of an Epistemic Object in the Early Twentieth Century, Oxford University Press, 2018, 9780198797258. hal-01879022 HAL Id: hal-01879022 https://hal.archives-ouvertes.fr/hal-01879022 Submitted on 21 Sep 2018 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Ether and electrons in relativity theory (1900–1911) Scott A. Walter∗ To appear in J. Navarro, ed, Ether and Modernity, 67–87. Oxford: Oxford University Press, 2018 Abstract This chapter discusses the roles of ether and electrons in relativity the- ory. One of the most radical moves made by Albert Einstein was to dismiss the ether from electrodynamics. His fellow physicists felt challenged by Einstein’s view, and they came up with a variety of responses, ranging from enthusiastic approval, to dismissive rejection. Among the naysayers were the electron theorists, who were unanimous in their affirmation of the ether, even if they agreed with other aspects of Einstein’s theory of relativity. The eventual success of the latter theory (circa 1911) owed much to Hermann Minkowski’s idea of four-dimensional spacetime, which was portrayed as a conceptual substitute of sorts for the ether. -
William Henry Bragg 1862 - 1942 Awarded the Nobel Prize for Physics in 1915
William Henry Bragg 1862 - 1942 Awarded the Nobel Prize for Physics in 1915 William Henry Bragg was a pioneer British scientist in solid- state physics. He was born on July 2, 1862, in Wigton, Cumberland, England. Bragg's father came from a family of farmers and merchant seamen. His mother, a sweet and kind woman, was the daughter of the local vicar. He did not remember her very well, as she died when he was about seven. The small boy was taken to the family of his uncle, the owner of a pharmacy and grocery shop. In 1875 his father took him back and sent him to school at King William’s College, Isle of Man. Bragg was good in his lessons and sports and became the head boy. He was fond of all games and played them rather well. In 1881 Bragg tried for Cambridge University,but the first interview was not a success, and he had to return to school.After the next attempt he was granted a scholarship to Trinity College. Here he worked very hard at mathematics and two years later obtained third place in the final Both he and his son examination. Bragg played tennis and hockey well. His teacher was the famous physicist J.J. lectured at the Royal Thomson with whom he also played tennis. Thomson advised him to send an application for the Institution post of professor of mathematics and physics at Adelaide University in Australia. After an interview Bragg was appointed and went to Australia where he began his career. In Adelaide the young professor became one of the best lecturers and a brilliant experimentalist. -
Beyond Einstein Perspectives on Geometry, Gravitation, and Cosmology in the Twentieth Century Editors David E
David E. Rowe • Tilman Sauer • Scott A. Walter Editors Beyond Einstein Perspectives on Geometry, Gravitation, and Cosmology in the Twentieth Century Editors David E. Rowe Tilman Sauer Institut für Mathematik Institut für Mathematik Johannes Gutenberg-Universität Johannes Gutenberg-Universität Mainz, Germany Mainz, Germany Scott A. Walter Centre François Viète Université de Nantes Nantes Cedex, France ISSN 2381-5833 ISSN 2381-5841 (electronic) Einstein Studies ISBN 978-1-4939-7706-2 ISBN 978-1-4939-7708-6 (eBook) https://doi.org/10.1007/978-1-4939-7708-6 Library of Congress Control Number: 2018944372 Mathematics Subject Classification (2010): 01A60, 81T20, 83C47, 83D05 © Springer Science+Business Media, LLC, part of Springer Nature 2018 This work is subject to copyright. All rights are reserved by the Publisher, whether the whole or part of the material is concerned, specifically the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfilms or in any other physical way, and transmission or information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed. The use of general descriptive names, registered names, trademarks, service marks, etc. in this publication does not imply, even in the absence of a specific statement, that such names are exempt from the relevant protective laws and regulations and therefore free for general use. The publisher, the authors and the editors are safe to assume that the advice and information in this book are believed to be true and accurate at the date of publication. Neither the publisher nor the authors or the editors give a warranty, express or implied, with respect to the material contained herein or for any errors or omissions that may have been made.