Fundamental Physics Heisenberg and Beyond
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University of Cincinnati
! "# $ % & % ' % !" #$ !% !' &$ &""! '() ' #$ *+ ' "# ' '% $$(' ,) * !$- .*./- 0 #!1- 2 *,*- Atomic Apocalypse – ‘Nuclear Fiction’ in German Literature and Culture A dissertation submitted to the Graduate School of the University of Cincinnati In partial fulfillment of the requirements for the degree of DOCTORATE OF PHILOSOPHY (Ph.D.) in the Department of German Studies of the College of Arts and Sciences 2010 by Wolfgang Lueckel B.A. (equivalent) in German Literature, Universität Mainz, 2003 M.A. in German Studies, University of Cincinnati, 2005 Committee Chair: Sara Friedrichsmeyer, Ph.D. Committee Members: Todd Herzog, Ph.D. (second reader) Katharina Gerstenberger, Ph.D. Richard E. Schade, Ph.D. ii Abstract In my dissertation “Atomic Apocalypse – ‘Nuclear Fiction’ in German Literature and Culture,” I investigate the portrayal of the nuclear age and its most dreaded fantasy, the nuclear apocalypse, in German fictionalizations and cultural writings. My selection contains texts of disparate natures and provenance: about fifty plays, novels, audio plays, treatises, narratives, films from 1946 to 2009. I regard these texts as a genre of their own and attempt a description of the various elements that tie them together. The fascination with the end of the world that high and popular culture have developed after 9/11 partially originated from the tradition of nuclear fiction since 1945. The Cold War has produced strong and lasting apocalyptic images in German culture that reject the traditional biblical apocalypse and that draw up a new worldview. In particular, German nuclear fiction sees the atomic apocalypse as another step towards the technical facilitation of genocide, preceded by the Jewish Holocaust with its gas chambers and ovens. -
LIGO's Unsung Heroes : Nature News & Comment
NATURE | NEWS LIGO's unsung heroes Nature highlights just a few of the people who played a crucial part in the discovery of gravitational waves — but didn’t win the Nobel Prize. Davide Castelvecchi 09 October 2017 Corrected: 19 October 2017 Joe McNally/Getty LIGO hunts gravitational waves with the help of two laser interferometers — and hundreds of people. Expand Every October, the announcements of the Nobel Prizes bring with them some controversy. This year’s physics prize — in recognition of the Laser Interferometer Gravitational-Wave Observatory (LIGO) in the United States — was less debated than most. The three winners — Kip Thorne and Barry Barish, both at the California Institute of Technology (Caltech) in Pasadena, and Rainer Weiss at the Massachusetts Institute of Technology (MIT) in Cambridge — had attracted near-universal praise for their roles in the project’s success. But the award has still put into stark relief the difficulty of singling out just a few individuals from the large collaborations of today’s 'Big Science'. The LIGO collaboration uses two giant laser interferometers to listen for deformations in space-time caused by some of the Universe’s most cataclysmic events. Physicists detected their first gravitational waves — interpreted as being produced by the collision of two black holes more than a billion years ago — in September 2015. The resulting paper, published in February 20161, has a mind-boggling 1,004 authors. Some of those are members of the LIGO Laboratory, the Caltech–MIT consortium that manages LIGO’s two interferometers in Louisiana and Washington State. But the list also includes the larger LIGO Scientific Collaboration: researchers from 18 countries, some of which — such as Germany and the United Kingdom — have made crucial contributions to the detectors. -
A Brief History of Gravitational Waves
Review A Brief History of Gravitational Waves Jorge L. Cervantes-Cota 1, Salvador Galindo-Uribarri 1 and George F. Smoot 2,3,4,* 1 Department of Physics, National Institute for Nuclear Research, Km 36.5 Carretera Mexico-Toluca, Ocoyoacac, Mexico State C.P.52750, Mexico; [email protected] (J.L.C.-C.); [email protected] (S.G.-U.) 2 Helmut and Ana Pao Sohmen Professor at Large, Institute for Advanced Study, Hong Kong University of Science and Technology, Clear Water Bay, 999077 Kowloon, Hong Kong, China. 3 Université Sorbonne Paris Cité, Laboratoire APC-PCCP, Université Paris Diderot, 10 rue Alice Domon et Leonie Duquet 75205 Paris Cedex 13, France. 4 Department of Physics and LBNL, University of California; MS Bldg 50-5505 LBNL, 1 Cyclotron Road Berkeley, CA 94720, USA. * Correspondence: [email protected]; Tel.:+1-510-486-5505 Abstract: This review describes the discovery of gravitational waves. We recount the journey of predicting and finding those waves, since its beginning in the early twentieth century, their prediction by Einstein in 1916, theoretical and experimental blunders, efforts towards their detection, and finally the subsequent successful discovery. Keywords: gravitational waves; General Relativity; LIGO; Einstein; strong-field gravity; binary black holes 1. Introduction Einstein’s General Theory of Relativity, published in November 1915, led to the prediction of the existence of gravitational waves that would be so faint and their interaction with matter so weak that Einstein himself wondered if they could ever be discovered. Even if they were detectable, Einstein also wondered if they would ever be useful enough for use in science. -
Kerne, Kooperation Und Konkurrenz. Kernforschung In
Wissenschaft, Macht und Kultur in der modernen Geschichte Herausgegeben von Mitchell G. Ash und Carola Sachse Band 3 Silke Fengler Kerne, Kooperation und Konkurrenz Kernforschung in Österreich im internationalen Kontext (1900–1950) 2014 Böhlau Verlag Wien Köln Weimar The research was funded by the Austrian Science Fund (FWF) : P 19557-G08 Bibliografische Information der Deutschen Nationalbibliothek: Die Deutsche Nationalbibliothek verzeichnet diese Publikation in der Deutschen Nationalbibliografie; detaillierte bibliografische Datensind im Internet über http://dnb.d-nb.de abrufbar. Umschlagabbildung: Zusammentreffen in Hohenholte bei Münster am 18. Mai 1932 anlässlich der 37. Hauptversammlung der deutschen Bunsengesellschaft für angewandte physikalische Chemie in Münster (16. bis 19. Mai 1932). Von links nach rechts: James Chadwick, Georg von Hevesy, Hans Geiger, Lili Geiger, Lise Meitner, Ernest Rutherford, Otto Hahn, Stefan Meyer, Karl Przibram. © Österreichische Zentralbibliothek für Physik, Wien © 2014 by Böhlau Verlag Ges.m.b.H & Co. KG, Wien Köln Weimar Wiesingerstraße 1, A-1010 Wien, www.boehlau-verlag.com Alle Rechte vorbehalten. Dieses Werk ist urheberrechtlich geschützt. Jede Verwertung außerhalb der engen Grenzen des Urheberrechtsgesetzes ist unzulässig. Lektorat: Ina Heumann Korrektorat: Michael Supanz Umschlaggestaltung: Michael Haderer, Wien Satz: Michael Rauscher, Wien Druck und Bindung: Prime Rate kft., Budapest Gedruckt auf chlor- und säurefrei gebleichtem Papier Printed in Hungary ISBN 978-3-205-79512-4 Inhalt 1. Kernforschung in Österreich im Spannungsfeld von internationaler Kooperation und Konkurrenz ....................... 9 1.1 Internationalisierungsprozesse in der Radioaktivitäts- und Kernforschung : Eine Skizze ...................... 9 1.2 Begriffsklärung und Fragestellungen ................. 10 1.2.2 Ressourcenausstattung und Ressourcenverteilung ......... 12 1.2.3 Zentrum und Peripherie ..................... 14 1.3 Forschungsstand ........................... 16 1.4 Quellenlage ............................. -
Heisenberg and the Nazi Atomic Bomb Project, 1939-1945: a Study in German Culture
Heisenberg and the Nazi Atomic Bomb Project http://content.cdlib.org/xtf/view?docId=ft838nb56t&chunk.id=0&doc.v... Preferred Citation: Rose, Paul Lawrence. Heisenberg and the Nazi Atomic Bomb Project, 1939-1945: A Study in German Culture. Berkeley: University of California Press, c1998 1998. http://ark.cdlib.org/ark:/13030/ft838nb56t/ Heisenberg and the Nazi Atomic Bomb Project A Study in German Culture Paul Lawrence Rose UNIVERSITY OF CALIFORNIA PRESS Berkeley · Los Angeles · Oxford © 1998 The Regents of the University of California In affectionate memory of Brian Dalton (1924–1996), Scholar, gentleman, leader, friend And in honor of my father's 80th birthday Preferred Citation: Rose, Paul Lawrence. Heisenberg and the Nazi Atomic Bomb Project, 1939-1945: A Study in German Culture. Berkeley: University of California Press, c1998 1998. http://ark.cdlib.org/ark:/13030/ft838nb56t/ In affectionate memory of Brian Dalton (1924–1996), Scholar, gentleman, leader, friend And in honor of my father's 80th birthday ― ix ― ACKNOWLEDGMENTS For hospitality during various phases of work on this book I am grateful to Aryeh Dvoretzky, Director of the Institute of Advanced Studies of the Hebrew University of Jerusalem, whose invitation there allowed me to begin work on the book while on sabbatical leave from James Cook University of North Queensland, Australia, in 1983; and to those colleagues whose good offices made it possible for me to resume research on the subject while a visiting professor at York University and the University of Toronto, Canada, in 1990–92. Grants from the College of the Liberal Arts and the Institute for the Arts and Humanistic Studies of The Pennsylvania State University enabled me to complete the research and writing of the book. -
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. -
A Brief History of Gravitational Waves
universe Review A Brief History of Gravitational Waves Jorge L. Cervantes-Cota 1, Salvador Galindo-Uribarri 1 and George F. Smoot 2,3,4,* 1 Department of Physics, National Institute for Nuclear Research, Km 36.5 Carretera Mexico-Toluca, Ocoyoacac, C.P. 52750 Mexico, Mexico; [email protected] (J.L.C.-C.); [email protected] (S.G.-U.) 2 Helmut and Ana Pao Sohmen Professor at Large, Institute for Advanced Study, Hong Kong University of Science and Technology, Clear Water Bay, Kowloon, 999077 Hong Kong, China 3 Université Sorbonne Paris Cité, Laboratoire APC-PCCP, Université Paris Diderot, 10 rue Alice Domon et Leonie Duquet, 75205 Paris Cedex 13, France 4 Department of Physics and LBNL, University of California; MS Bldg 50-5505 LBNL, 1 Cyclotron Road Berkeley, 94720 CA, USA * Correspondence: [email protected]; Tel.:+1-510-486-5505 Academic Editors: Lorenzo Iorio and Elias C. Vagenas Received: 21 July 2016; Accepted: 2 September 2016; Published: 13 September 2016 Abstract: This review describes the discovery of gravitational waves. We recount the journey of predicting and finding those waves, since its beginning in the early twentieth century, their prediction by Einstein in 1916, theoretical and experimental blunders, efforts towards their detection, and finally the subsequent successful discovery. Keywords: gravitational waves; General Relativity; LIGO; Einstein; strong-field gravity; binary black holes 1. Introduction Einstein’s General Theory of Relativity, published in November 1915, led to the prediction of the existence of gravitational waves that would be so faint and their interaction with matter so weak that Einstein himself wondered if they could ever be discovered. -
Heinz Billing
Heinz Billing Born April 7, 1914, Salzwedel, Germany; an inventor1, of magnetic drum storage and built the first working electronic computer in Germany; searched for gravity waves and became unsurpassed in not finding them. Education: doctoral degree, University of Göttingen, 1938. Professional Experience: Aerodynamic Test Centre, Göttingen (Aerodynamische Versuchsanstalt, AVA) 1938-1946; German Air Force, 1938-1941; Institute für Instrumentenkunde (Institute for Scientific Instruments), Kaiser-Wilhelm-Gesellschaft (later Max-Planck- Gesellschaft), 1946-1949, and again in 1950-1972; Commonwealth Scientific and Industrial Organization, Sydney, Australia, 1949-1950; Max Planck Institute, Garching, Germany, 1972-1982. Honors and Awards: honorary professorship in computing, Erlangen University, 1967; Konrad Zuse Prize, 1987. Heinz Billing was born on April 7, 1914 in Salzwedel, a small town some 30 miles north of Wolfsburg, where Volkswagen automobiles are made. He went to school at Salzwedel, graduated from high school (“Abitur”-examination) at 18 and, after studies at Göttingen (a famous university town south of Hanover) and Munich, he received his doctorate in physics at the age of 24. His thesis under Walter Gerlach was on Light Interference with Canal Rays. He began his career June 1, 1938, at the Aerodynamic Test Centre at Göttingen (Aerodynamische Versuchsanstalt, AVA) connected with Ludwig Prandt], the famous director of the Kaiser- Wilhelm-Institut für Strömungsforschung (fluid mechanics). By October 1, 1938, he was drafted to the Air Force, where he worked in weather forecasting. He was released from these duties in May 1941 to do research in aeronautical acoustics. Magnetic Sound Recording In those days German engineering was well known for excellent results with magnetic sound recording, first on steel wire and then on tape. -
LIGO Magazine Issue #14 !
LIGO Scientific Collaboration Scientific LIGO issue 14 3/2019 LIGO MAGAZINE The Gravitational Weather Forecast: Predicting sources for O3 Upgrades to Hanford, Livingston and Virgo sites Getting ready for O3 p.12 The LVC‘s first Gravitational Wave Transient Catalog Inventorizing the dark side p. 15 ... and an interview with Sir James Hough on the early days p.19 Front cover A new study using Chandra data of GW170817 indicates that the event that produced gravitational waves likely created the lowest mass black hole known. The artist’s illustration shows the black hole that resulted from the merger, along with a disk of infalling matter and a jet of high-energy particles. (Credit: NASA/CXC/M.Weiss) The top inset shows the view from below the ‘north input test mass’ of Virgo. The bottom inset shows a schematic of binary mergers observed by LIGO and Virgo so far. Image credits Photos and graphics appear courtesy of Caltech/MIT LIGO Laboratory and LIGO Scientific Collaboration unless otherwise noted. Cover: Main illustration from NASA/CXC/M.Weiss. Top inset from M. Perciballi / The Virgo collaboration. Bottom inset from LIGO-Virgo / Frank Elavsky / Northwestern University p. 3 Comic strip by Nutsinee Kijbunchoo p. 6-9 Colliding neutron stars illustration by NASA/CXC/M.Weiss. Gravitational wave sources by Chris Messenger. Sensitivity curves from LIGO/Virgo/KAGRA p. 12-14 Livingston photo by Matthew Heintze. Hanford photo by Nutsinee Kijbunchoo, Virgo photo by M. Perciballi / The Virgo Collaboration. p. 15-18 Time frequency plots and waveforms by S. Ghonge, K. Janu / Georgia Tech. Masses in the Stellar Graveyard by LIGO-Virgo / Frank Elavsky / Northwestern University. -
The Virus House -
David Irving The Virus House - F FOCAL POINT Copyright © by David Irving Electronic version copyright © by Parforce UK Ltd. All rights reserved No reproduction, copy or transmission of this publication may be made without written permission. Copies may be downloaded from our website for research purposes only. No part of this publication may be commercially reproduced, copied, or transmitted save with written permission in accordance with the provisions of the Copyright Act (as amended). Any person who does any unauthorised act in relation to this publication may be liable to criminal prosecution and civil claims for damages. To Pilar is the son of a Royal Navy commander. Imper- fectly educated at London’s Imperial College of Science & Tech- nology and at University College, he subsequently spent a year in Germany working in a steel mill and perfecting his fluency in the language. In he published The Destruction of Dresden. This became a best-seller in many countries. Among his thirty books (including three in German), the best-known include Hitler’s War; The Trail of the Fox: The Life of Field Marshal Rommel; Accident, the Death of General Sikorski; The Rise and Fall of the Luftwaffe; Göring: a Biography; and Nuremberg, the Last Battle. The second volume of Churchill's War appeared in and he is now completing the third. His works are available as free downloads at www.fpp.co.uk/books. Contents Author’s Introduction ............................. Solstice.......................................................... A Letter to the War Office ........................ The Plutonium Alternative....................... An Error of Consequence ......................... Item Sixteen on a Long Agenda............... Freshman................................................... Vemork Attacked..................................... -
Bruno Touschek in Germany After the War: 1945-46
LABORATORI NAZIONALI DI FRASCATI INFN–19-17/LNF October 10, 2019 MIT-CTP/5150 Bruno Touschek in Germany after the War: 1945-46 Luisa Bonolis1, Giulia Pancheri2;† 1)Max Planck Institute for the History of Science, Boltzmannstraße 22, 14195 Berlin, Germany 2)INFN, Laboratori Nazionali di Frascati, P.O. Box 13, I-00044 Frascati, Italy Abstract Bruno Touschek was an Austrian born theoretical physicist, who proposed and built the first electron-positron collider in 1960 in the Frascati National Laboratories in Italy. In this note we reconstruct a crucial period of Bruno Touschek’s life so far scarcely explored, which runs from Summer 1945 to the end of 1946. We shall describe his university studies in Gottingen,¨ placing them in the context of the reconstruction of German science after 1945. The influence of Werner Heisenberg and other prominent German physicists will be highlighted. In parallel, we shall show how the decisions of the Allied powers, towards restructuring science and technology in the UK after the war effort, determined Touschek’s move to the University of Glasgow in 1947. Make it a story of distances and starlight Robert Penn Warren, 1905-1989, c 1985 Robert Penn Warren arXiv:1910.09075v1 [physics.hist-ph] 20 Oct 2019 e-mail: [email protected], [email protected]. Authors’ ordering in this and related works alternates to reflect that this work is part of a joint collaboration project with no principal author. †) Also at Center for Theoretical Physics, Massachusetts Institute of Technology, USA. Contents 1 Introduction2 2 Hamburg 1945: from death rays to post-war science4 3 German science and the mission of the T-force6 3.1 Operation Epsilon . -
Heisenberg in the Atomic Age: Science and the Public Sphere Cathryn Carson Frontmatter More Information
Excerpt Index Cambridge University Press 978-1-107-43695-4 - Heisenberg in the Atomic Age: Science and the Public Sphere Cathryn Carson Frontmatter More information Heisenberg in the Atomic Age The end of the Second World War opened a new era for science in public life. Heisenberg in the Atomic Age explores the transformations of science’s public presence in the postwar Federal Republic of Germany. It shows how Werner Heisenberg’s philosophical commentaries, circulated in the mass media, secured his role as science’s public philosopher, and it reflects on his policy engagements and public political stands, which helped redefine the relationship between science and the state. With deep archival grounding, the book tracks Heisenberg’s interactions with intellectuals from Heidegger to Habermas and political leaders from Adenauer to Brandt. It also traces his evolving statements about his wartime research on nuclear fission for the National Socialist regime. Working between the history of science and German history, the book’s central theme is the place of scientific rationality in public life – after the atomic bomb, inthewakeoftheThirdReich. Cathryn Carson is Associate Professor of History and Director of the Office for History of Science and Technology at the University of California, Berkeley. She is coeditor, with David A. Hollinger, of Reappraising Oppenheimer: Centennial Studies and Reflections and chair of the editorial board of Historical Studies in the Natural Sciences. © in this web service Cambridge University Press www.cambridge.org Excerpt Index Cambridge University Press 978-1-107-43695-4 - Heisenberg in the Atomic Age: Science and the Public Sphere Cathryn Carson Frontmatter More information © in this web service Cambridge University Press www.cambridge.org Excerpt Index Cambridge University Press 978-1-107-43695-4 - Heisenberg in the Atomic Age: Science and the Public Sphere Cathryn Carson Frontmatter More information publications of the german historical institute Washington, D.C.