The Mind That Created the Bohr Atom∗
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10. Interlude in Denmark (PDF)
10 Interlude in Denmark In my early student days -- as I have mentioned in chapter 3 -- my friend Christiansen-Weniger and I won an election as German student representatives on the ticket by striking a mathematical funny bone: Christiansen-Weniger - von Hippel [Christiansen minus von Hippel]. In the meantime, "Krischan" had become a professor of agriculture and had been called to Ankara in that capacity. He was an "unblemished Aryan," still a German citizen, and his lovely wife, Luise, alias "Körnchen," also a youth-movement friend, came to visit us. She intended to fly to Warsaw, and I wanted to fly to Copenhagen via Danzig, in order to visit Olga, who was directing a training school for agricultural helpers in that neighborhood. We therefore decided to fly together from Istanbul. In those early years of aviation, this was a major undertaking. Istanbul did not yet have a real airport and our six-passenger plane, with semi-open cockpit, took off from a meadow at night with the headlights of carefully stationed cars outlining a runway. Before our departure, we received the reassuring news that the plane flying the reverse route had crashed in the Albanian mountains. Our flight proved glorious, however. We passed over the Balkans in semi-darkness. No light shone from the ground there because practically all of its settlements had then been wiped out in the Balkan Wars and World War I. At sunrise we reached the Carpathian mountains and flew along that stunning semi-circle separating Hungary from Poland. The air became turbulent and we had to throw up "par la fenêtre [out the window]." At noon we landed in Warsaw, where Luise left me. -
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. -
Working Papers in Scandina Vian Syntax
WORKING PAPERS IN SCANDINA VIAN SYNTAX Volume 55 Sten Vikner: V0-to-l0 Mavement and Inflection for Person in AllTenses 1-27 Anders Holmberg and Gorel Sandstrom: Scandinavian Possessive Construerions from a Northem Swedish Viewpoint 29-49 Hoskuldur Thrainsson and Sten Vikner: Modals and Double Modals in the Scandinavian Languages 51-88 Øystein Alexander Vangsnes Referentiality and Argument Positions in leelandie 89-109 June 1995 Working Papers in Scandinavian Syntax Department of Scandinavian Languages Helgonabacken 14 S-223 62 Lund Sweden V0-TO-JO MOVEMENT AND INFLECTION FOR PERSON IN ALL TENSES Sten Vilener Institut furLinguistik/Germanistik, Universitat Stuttgart, Postfach 10 60 37, D-70049 Stuttgart, Germany E-mail: [email protected] ABSTRACf Differentways are considered of formulating a conneelion between the strength of verbal inflectional morphology and the obligatory m ovement of the flnite verb to J• (i.e. to the lefl of a medial adverbial or of negation), and two main alternatives are anived at. One is from Rohrbacher (1994:108):V"-to-1• movement iff 151 and 2nd person are distinctively marked at least once. The other will be suggesled insection 3: v•-to-J• mavement iff all"core' tenses are inflectedfor person. It is argued that the latter approach has certain both conceptual and empirical advantages ( e.g. w hen considering the loss of v•-to-J• movement in English). CONTENTS 1. Introduction: v•-to-J• movement ...................................................................................................................................... -
Germanic Standardizations: Past to Present (Impact: Studies in Language and Society)
<DOCINFO AUTHOR ""TITLE "Germanic Standardizations: Past to Present"SUBJECT "Impact 18"KEYWORDS ""SIZE HEIGHT "220"WIDTH "150"VOFFSET "4"> Germanic Standardizations Impact: Studies in language and society impact publishes monographs, collective volumes, and text books on topics in sociolinguistics. The scope of the series is broad, with special emphasis on areas such as language planning and language policies; language conflict and language death; language standards and language change; dialectology; diglossia; discourse studies; language and social identity (gender, ethnicity, class, ideology); and history and methods of sociolinguistics. General Editor Associate Editor Annick De Houwer Elizabeth Lanza University of Antwerp University of Oslo Advisory Board Ulrich Ammon William Labov Gerhard Mercator University University of Pennsylvania Jan Blommaert Joseph Lo Bianco Ghent University The Australian National University Paul Drew Peter Nelde University of York Catholic University Brussels Anna Escobar Dennis Preston University of Illinois at Urbana Michigan State University Guus Extra Jeanine Treffers-Daller Tilburg University University of the West of England Margarita Hidalgo Vic Webb San Diego State University University of Pretoria Richard A. Hudson University College London Volume 18 Germanic Standardizations: Past to Present Edited by Ana Deumert and Wim Vandenbussche Germanic Standardizations Past to Present Edited by Ana Deumert Monash University Wim Vandenbussche Vrije Universiteit Brussel/FWO-Vlaanderen John Benjamins Publishing Company Amsterdam/Philadelphia TM The paper used in this publication meets the minimum requirements 8 of American National Standard for Information Sciences – Permanence of Paper for Printed Library Materials, ansi z39.48-1984. Library of Congress Cataloging-in-Publication Data Germanic standardizations : past to present / edited by Ana Deumert, Wim Vandenbussche. -
Experiencing Hubble
PRESCOTT ASTRONOMY CLUB PRESENTS EXPERIENCING HUBBLE John Carter August 7, 2019 GET OUT LOOK UP • When Galaxies Collide https://www.youtube.com/watch?v=HP3x7TgvgR8 • How Hubble Images Get Color https://www.youtube.com/watch? time_continue=3&v=WSG0MnmUsEY Experiencing Hubble Sagittarius Star Cloud 1. 12,000 stars 2. ½ percent of full Moon area. 3. Not one star in the image can be seen by the naked eye. 4. Color of star reflects its surface temperature. Eagle Nebula. M 16 1. Messier 16 is a conspicuous region of active star formation, appearing in the constellation Serpens Cauda. This giant cloud of interstellar gas and dust is commonly known as the Eagle Nebula, and has already created a cluster of young stars. The nebula is also referred to the Star Queen Nebula and as IC 4703; the cluster is NGC 6611. With an overall visual magnitude of 6.4, and an apparent diameter of 7', the Eagle Nebula's star cluster is best seen with low power telescopes. The brightest star in the cluster has an apparent magnitude of +8.24, easily visible with good binoculars. A 4" scope reveals about 20 stars in an uneven background of fainter stars and nebulosity; three nebulous concentrations can be glimpsed under good conditions. Under very good conditions, suggestions of dark obscuring matter can be seen to the north of the cluster. In an 8" telescope at low power, M 16 is an impressive object. The nebula extends much farther out, to a diameter of over 30'. It is filled with dark regions and globules, including a peculiar dark column and a luminous rim around the cluster. -
The Copenhagen Interpretation: Exploring Science on Stage
The Copenhagen Interpretation: Exploring Science on Stage Michael Frayn’s play Copenhagen, which opened and was known for his experimental, as well as in London in 1998, in New York in 2000, and theoretical, work; Diana Barkan Buchwald, finally made it to Los Angeles in late 2001, ex- associate professor of history, and general editor plores what might have been said during a 1941 and director of the Einstein Papers Project; Hank meeting of Niels Bohr and Werner Heisenberg at Stratton, who plays Werner Heisenberg in the Los Bohr’s home in the German-occupied capital city Angeles production of the play; Marge Leighton, a of Denmark. Although in the end all the ambigu- close friend of the Bohr family (and widow twice- ities and “uncertainties” remain, the three charac- over of Caltech physics professors Tommy Laurit- ters (including Bohr’s wife, Margrethe), with the sen and Bob Leighton); and Jay Labinger, admin- knowledge of hindsight “when all are dead and istrator of the Beckman Institute, who often writes gone,” reenact various drafts of the purpose of on the historical, cultural, social, and literary Heisenberg’s visit—and the ultimate question of aspects of science (see his review of two other why Heisenberg did not build an atomic bomb for science plays in E&S, 2001, no. 1). the Nazis. After Hank Stratton described the play briefly Caltech interest in the play naturally ran quite (but told the audience they’d have to “spend 55 high, and on December 10, in a packed Beckman bucks” to get the rest of it), Diana Barkan Auditorium, Caltech hosted a panel, “The Copen- Buchwald, a historian of science, outlined what hagen Interpretation,” convened “to consider the was going on in physics at the time: fission had broader scientific, historical, philosophical, and been discovered in Berlin in 1938 by Lise Meitner, artistic dimensions of this encounter and its Otto Hahn, and Fritz Strassmann. -
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 -
President's Message
Journal of the Northern Sydney Astronomical Society Inc. February 2019 In this issue President’s Message Page 1: President’s message Editorial i everyone. Object of the Month as it had been an idea Page 2: Results of the Photo HWhat a magnificent summer! waiting for someone to bring it to life for Competition It seems ages since the lovely summer days some time. Page 5: Results of the Article have landed on our holiday period in such This past two months’ contributions have Competition a comprehensive way. It has been a great been interesting and seen some wonderful Page 7: The Jupiter/Venus Conjunction holiday period for me and I hope you have images come to life. all had such a great time as I have had. It showcases the skills that some of our The last month’s images and videos I am equally pleased to see the Reflections members have and a big congratulation to of Wirtanen 46P comet, along with magazine has had a resurgence and I Kym Haines, the winner for this month, this month’s incredible photo of M42 encourage everyone to take an interest in Phil Angilley and Daniel Patos, the runner- exemplify the talents that can be found it. ups, for their excellent work. amongst our club members. We are expanding the source of A quick shout out to some upcoming contributions for the magazine with the Kym’s M42 photo as seen on page 2 is events. inclusion of the Object of the Month and magnificent and the colours and framing In April we will be running our New other items of interest to our community. -
The Discovery of Oxygen in the Universe
! ! ! The discovery of oxygen in the Universe The discovery of oxygen! ! Carl Scheele (1742-1786) ! is the first (1773;1777)! to isolate oxygen! Georg Ernst Stahl ! by heating HgO he found ! (1659-1734)! that it released a gas ! the father of the ! which enhanced combustion. ! phlogiston theory. ! ! phlogiston is the fire! Joseph Priestley (1733-1804)! that escapes from matter ! was the first (1774)! when it burns! to publish this result! (which he interpreted within ! the phlogiston theory)! Antoine de Lavoisier (1743-1794) ! discovered that air contains about 20 % oxygen ! and that when any substance burns,! it actually combines chemically with oxygen (1775) ! he gave oxygen its present name (oxy-gen = acid-forming)! he stated the law of the conservation of matter! ! Before the “discovery” of oxygen! Leonardo da Vinci (1452-1519) ! •" air is a mixture of gases! •" breathing ~ combustion! "Where flame cannot live no animal that draw breath can live." ! Michael Sendivogius (1566-1636) ! (Micha" S#dziwój) ! produced a gas he called ! “food of life” ! by heating saltpeter (KNO3) ! ! Cornelius Drebbel (1572-1633)! constructed in 1621 the first submarine . ! To “refresh” the air inside it, he generated oxygen by heating saltpeter as Sendivogius had tought him! “chemistry” before Lavoisier! ! Anaxagoras of Clazomenes (500 BC - 428 BC)! had already expressed “the law of Lavoisier”: ! “Rien ne se perd, rien ne se crée, tout se transforme“! ! ! ! ! Robert Boyle (1627- 1691)! •" noted that it was impossible to combine ! the four Greek elements to form -
A Brief History of Mangnetism
A Brief history of mangnetism Navinder Singh∗ and Arun M. Jayannavar∗∗ ∗Physical Research Laboratory, Ahmedabad, India, Pin: 380009. ∗∗ IOP, Bhubaneswar, India. ∗† Abstract In this article an overview of the historical development of the key ideas in the field of magnetism is presented. The presentation is semi-technical in nature.Starting by noting down important contribution of Greeks, William Gilbert, Coulomb, Poisson, Oersted, Ampere, Faraday, Maxwell, and Pierre Curie, we review early 20th century investigations by Paul Langevin and Pierre Weiss. The Langevin theory of paramagnetism and the Weiss theory of ferromagnetism were partly successful and real understanding of magnetism came with the advent of quantum mechanics. Van Vleck was the pioneer in applying quantum mechanics to the problem of magnetism and we discuss his main contributions: (1) his detailed quantum statistical mechanical study of magnetism of real gases; (2) his pointing out the importance of the crystal fields or ligand fields in the magnetic behavior of iron group salts (the ligand field theory); and (3) his many contributions to the elucidation of exchange interactions in d electron metals. Next, the pioneering contributions (but lesser known) of Dorfman are discussed. Then, in chronological order, the key contributions of Pauli, Heisenberg, and Landau are presented. Finally, we discuss a modern topic of quantum spin liquids. 1 Prologue In this presentation, the development of the conceptual structure of the field is highlighted, and the historical context is somewhat limited in scope. In that way, the presentation is not historically very rigorous. However, it may be useful for gaining a ”bird’s-eye view” of the vast field of magnetism. -
1548 the Role of the A-Bomb in The
#1548 The role of the A-bomb in the Abomination of Desolation – Pig Abominations, part 13, The Third Temples of Pig Abominations: Niels Bohr was the product of a Christian- Jewish marriage for the purpose of prophetically reflecting the Third Temple marriage of the Christian New Israel (the Body of Americans) with the Jewish new Israel (the Body of Israelis) Niels Bohr had a Christian father and a Jewish mother. Niels Bohr was born in Copenhagen, Denmark, on October 7, 1885. His father, Christian Bohr, was a devout Lutheran and was a professor of physiology at the University of Copenhagen. His mother, Ellen Adler Bohr, came from a wealthy Jewish family prominent in Danish banking and parliamentary circles. His brother was Harald Bohr, a mathematician and Olympic soccer player who played on the Danish national team. Key Understanding: Niels Bohr and the Christian-Jewish Christian Bohr marriage. Niels Bohr was the product of a Christian-Jewish marriage for the purpose of prophetically reflecting the Third Temple marriage of the Christian New Israel (the Body of Americans) with the Jewish new Israel (the Body of Israelis), a marriage that Niels Bohr prophetically was tied thoroughly to atomic bombs/nuclear weapons. Matthew 24:15 (KJV) When ye therefore shall see THE ABOMINATION OF DESOLATION [in conjunction with the Third Temple being constructed through the joining together of the Man o’ War ‘Living Stones’ Christian New Israel (the Body of Americans as the Third Temple) and (with) the Man o’ War ‘Living Stones’ Jewish new Israel (the Body -
The Origin and Evolution of Planetary Nebulae
P1: MRM/SPH P2: MRM/UKS QC: MRM/UKS T1: MRM CB211-FM CB211/Kwok October 30, 1999 1:26 Char Count= 0 THE ORIGIN AND EVOLUTION OF PLANETARY NEBULAE SUN KWOK University of Calgary, Canada iii P1: MRM/SPH P2: MRM/UKS QC: MRM/UKS T1: MRM CB211-FM CB211/Kwok October 30, 1999 1:26 Char Count= 0 PUBLISHED BY THE PRESS SYNDICATE OF THE UNIVERSITY OF CAMBRIDGE The Pitt Building, Trumpington Street, Cambridge, United Kingdom CAMBRIDGE UNIVERSITY PRESS The Edinburgh Building, Cambridge CB2 2RU, UK http://www.cup.cam.ac.uk 40 West 20th Street, New York, NY 10011-4211, USA http://www.cup.org 10 Stamford Road, Oakleigh, Melbourne 3166, Australia Ruiz de Alarc´on 13, 28014 Madrid, Spain c Cambridge University Press 2000 This book is in copyright. Subject to statutory exception and to the provisions of relevant collective licensing agreements, no reproduction of any part may take place without the written permission of Cambridge University Press. First published 2000 Printed in the United States of America Typeface Times Roman 10.5/12.5 pt. and Gill Sans System LATEX2ε [TB] A catalog record for this book is available from the British Library. Library of Congress Cataloging in Publication Data Kwok, S. (Sun) The origin and evolution of planetary nebulae / Sun Kwok. p. cm. – (Cambridge astrophysics series : 33) ISBN 0-521-62313-8 (hc.) 1. Planetary nebulae. I. Title. II. Series. QB855.5.K96 1999 523.10135 – dc21 99-21392 CIP ISBN 0 521 62313 8 hardback iv P1: MRM/SPH P2: MRM/UKS QC: MRM/UKS T1: MRM CB211-FM CB211/Kwok October 30, 1999 1:26 Char Count= 0