Women in Physics in Vienna
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Women in Physics, 2000 Highlights
By Rachel Ivie AIP Publication Number R-430 June, 2000 Katie Stowe Women in Physics, 2000 Highlights • An increasingly large number of girls have some exposure to physics by taking it in high school. By 1997, almost one-half of high school physics students were girls (Figure 1) . About 400,000 girls take high school physics each year. • Women’s participation in physics decreases with each step up the academic ladder. For example, more than two-fifths of high school physics students in 1993 were girls, but women earned less than one-fifth of bachelor’s degrees in physics five years later (Figures 1 and 3) . • Although women now earn more than one half of all bachelor’s degrees in the U.S., physics is not attracting women as quickly as other fields, including life sciences, chemistry, and engineering (Figures 4 and 5) . Compared to other fields, women are sorely underrepresented in physics at both the bachelor’s and PhD levels (Figures 4, 5, 6, 7, and Table 1) . • Twenty U.S. physics departments (excluding women’s colleges) had more than 40% female bachelor’s degree recipients during the five academic years 1994-98. This report lists these departments as well as women’s colleges that grant bachelor’s degrees in physics (Tables 2 and 3) . • The proportion of women teaching physics decreases as academic rank and level of the department increases (Table 4) . However, the percentage of women faculty members at each rank is at least as high as the percentage of women earning PhDs at various points in the past. -
Development Plan 2021–2023
Approved by the general assembly of 12/13/2019. OeAW Development Plan 2021–2023 Glossary AI Artificial Intelligence BMBWF Bundesministerium für Bildung, Wissenschaft und Forschung (Federal Ministry of Education, Science and Research) CLARIN Common Language Resources and Technology Infrastructure DARIAH Digital Research Infrastructure for the Arts and Humanities DH Digital Humanities ESQ Erwin Schrödinger Center for Quantum Science & Technology ESS Earth System Sciences Research Program FWF Fonds zur Förderung der wissenschaftlichen Forschung (Austrian Science Fund) FTI Forschung, Technologie und Innovation (Research, Technology and Innovation) GSK Geistes-, Sozial- und Kulturwissenschaften (Humanities, Social Sciences and Cultural Studies) GUEP Entwurf des Gesamtösterreichischen Universitätsentwicklungsplans 2022–2027 in der Fassung vom 01.08.2019 (draft Austrian University Development Plan 2022–2027 as of 08/01/2019) HI Rom Historisches Institut beim Österreichischen Kulturforum in Rom (Historical Institute of the Austrian Cultural Forum, Rome) HPDA High Performance Data Analysis IP Intellectual Property IPR Intellectual Property Rights JESH Joint Excellence in Science and Humanities funding program at the OeAW NFTE Nationalstiftung für Forschung, Technologie und Entwicklung (National Foundation for Research, Technology and Development) PA Performance agreement between the OeAW and the BMBWF SDG Sustainable Development Goals STEM Science, Technology, Engineering and Mathematics Page 2 of 30 OeAW Development Plan 2021–2023 Table of Contents -
Physics in Your Future Introduces Physics and Careers in Physics to Young People, Their Parents, Teachers and Advisors
TM American Physical Society • Committee on the Status of Women in Physics Chiara La Tessa of Brookhaven National Laboratory is inside the target room of the NASA Space Radiation Laboratory at Brookhaven. She is aligning a detector called EGG counter in the center of a beam – something that’s done before each experiment. Physics helps us understand the world around us, the world inside us, and the world beyond us. Physics is the most basic and fundamental science; it deals with how and why matter and energy act as they do. The laws of physics apply to force and motion, gravity, electricity, magnetism, sound, light and heat. They help us understand the physical world and develop products that people need. Mastering physics is fun and challenging. It involves working with others, as well as alone. You learn how to solve problems, observe things carefully, make measurements and keep accurate records. You can use these valuable skills for the rest of your life. They open doors to many good jobs. Physicists ask questions about the physical world and try to find exact answers. They are creative and persistent. Some do basic research. Their goal is to increase our knowledge of the universe. Others do applied research. They use basic knowledge to solve world problems such as food and energy supply, environmental protection, transportation, communication and defense. Physicists work in industry, educational institutions, government, and medical centers today. Most are active scientists and engineers. They do research and development, administration, and teaching. Others use their physics background in fields like publishing, sales, law, accounting and medicine. -
Marietta Blau in the History of Cosmic Rays Per Carlson
Physics Today Marietta Blau in the history of cosmic rays Per Carlson Citation: Physics Today 65(10), 8 (2012); doi: 10.1063/PT.3.1729 View online: http://dx.doi.org/10.1063/PT.3.1729 View Table of Contents: http://scitation.aip.org/content/aip/magazine/physicstoday/65/10?ver=pdfcov Published by the AIP Publishing Reuse of AIP Publishing content is subject to the terms at: https://publishing.aip.org/authors/rights-and-permissions. Download to IP: 149.28.91.2 On: Thu, 30 Jun 2016 17:53:16 readers’ forum Marietta Blau in the history of cosmic rays er Carlson, in his article “A century have been formed by cosmic particles ex- contributions deserve a prominent and Pof cosmic rays” (PHYSICS TODAY, plosively disintegrating heavy nuclei in permanent place in any history of February 2012, page 30), states that the emulsion. That discovery, in 1937, cosmic-ray and particle physics. And I the investigation of cosmic rays opened created a sensation among nuclear and believe it is also important, given the up the field of particle physics. How- cosmic-ray physicists worldwide, and by much-discussed problem of the under- ever, he neglects the importance of nu- demonstrating that nuclear emulsions representation of women in physics, clear emulsions in the progress of par- had come of age for recording rare high- that PHYSICS TODAY take care not to ticle physics, and he fails to mention a energy nuclear events, it paved the way overlook women who, like Blau, made key figure, Austrian physicist Marietta for further research in particle physics. -
Marietta Blau's Work After World War II Arnold Perlmutter Department Of
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server Marietta Blau's Work After World War II Arnold Perlmutter Department of Physics University of Miami Coral Gables, Florida 33124 completed, October 27, 2000 This paper has been translated into German and will be included, in a somewhat altered form, in a book Sterne der Zertrummerung, Marietta Blau, Wegbereiterin der Moderne Teilchenphysik, Brigitte Strohmaier and Robert Rosner, eds., Boehlau Verlag, Wien. 1 A. Introduction While it is clear that the seminal work of Dr. Marietta Blau was done in the 1920’s and especially in the 1930’s, it is also evident that her separation from the great research centers from 1938 to 1944 had a devastating effect on her productivity. It was during this period that Cecil F. Powell, at Bristol University, made use of Blau’s earlier tutelage on the preparation and analysis of photographic emulsions. According to Blau’s conversations with me (much later), she consulted with Ilford in the 1930’s to improve emulsion sensitivity and uniformity, and presumably had also imparted crucial lore of the technique to Powell. C.F. Powell, who had been a student of C.T.R. Wilson, had employed cloud chambers in a wide variety of studies in vulcanology, mechanical engineering, and nuclear physics. In 1938 and 1939 Powell’s experimental efforts turned to the use of photographic emulsions to investigate neutron interactions, and then to nuclear reactions1. With the coming of the war and then the British nuclear atomic bomb project, Powell established a formidable laboratory and collaboration for the analysis of emulsions and for their improvement by Ilford and Kodak. -
Chapter 6 the Aftermath of the Cambridge-Vienna Controversy: Radioactivity and Politics in Vienna in the 1930S
Trafficking Materials and Maria Rentetzi Gendered Experimental Practices Chapter 6 The Aftermath of the Cambridge-Vienna Controversy: Radioactivity and Politics in Vienna in the 1930s Consequences of the Cambridge-Vienna episode ranged from the entrance of other 1 research centers into the field as the study of the atomic nucleus became a promising area of scientific investigation to the development of new experimental methods. As Jeff Hughes describes, three key groups turned to the study of atomic nucleus. Gerhard Hoffman and his student Heinz Pose studied artificial disintegration at the Physics Institute of the University of Halle using a polonium source sent by Meyer.1 In Paris, Maurice de Broglie turned his well-equipped laboratory for x-ray research into a center for radioactivity studies and Madame Curie started to accumulate polonium for research on artificial disintegration. The need to replace the scintillation counters with a more reliable technique also 2 led to the extensive use of the cloud chamber in Cambridge.2 Simultaneously, the development of electric counting methods for measuring alpha particles in Rutherford's laboratory secured quantitative investigations and prompted Stetter and Schmidt from the Vienna Institute to focus on the valve amplifier technique.3 Essential for the work in both the Cambridge and the Vienna laboratories was the use of polonium as a strong source of alpha particles for those methods as an alternative to the scintillation technique. Besides serving as a place for scientific production, the laboratory was definitely 3 also a space for work where tasks were labeled as skilled and unskilled and positions were divided to those paid monthly and those supported by grant money or by research fellowships. -
From the Discovery of Radioactivity to the First Accelerator Experiments
Chapter 2 From the Discovery of Radioactivity to the First Accelerator Experiments Michael Walter 2.1 Introduction The article reviews the historical phases of cosmic ray research from the very be- ginning around 1900 until the 1940s, when the first particle accelerators replaced cosmic particles as a source for elementary particle interactions. Contrary to the discovery of X-rays or the ionising α-, β- and γ -rays, it was an arduous path to the definite acceptance of the new radiation. The development in the years before the discovery is described in Sect. 2.2. The following section deals with the work of Victor F. Hess, especially with the detection of extraterrestrial radiation in 1912 and the years until the final acceptance by the scientific community. In Sect. 2.4 the study of the properties of cosmic rays is discussed. Innovative detectors and meth- ods like the cloud chamber, the Geiger–Müller counter and the coincidence circuit brought new stimuli. The origin of cosmic rays was and is still an unsolved ques- tion. The different hypotheses of the early time are summarised in Sect. 2.5.Inthe 1930s a scientific success story started which nobody of the first protagonists might have imagined. The discovery of the positron by C.D. Anderson was the birth of elementary particle physics. The 15 years until a new era started in 1947 with first accelerator experiments at the Berkeley synchro-cyclotron are described in Sect. 2.6. It is obvious that this article can only cover the main steps of the historical de- velopment. An excellent description of the research on the “Höhenstrahlung” in the years between 1900 and 1936 was given by Miehlnickel (1938). -
Chronological List of Correspondence, 1895–1920
CHRONOLOGICAL LIST OF CORRESPONDENCE, 1895–1920 In this chronological list of correspondence, the volume and document numbers follow each name. Documents abstracted in the calendars are listed in the Alphabetical List of Texts in this volume. 1895 13 or 20 Mar To Mileva Maric;;, 1, 45 29 Apr To Rosa Winteler, 1, 46 Summer To Caesar Koch, 1, 6 18 May To Rosa Winteler, 1, 47 28 Jul To Julia Niggli, 1, 48 Aug To Rosa Winteler, 5: Vol. 1, 48a 1896 early Aug To Mileva Maric;;, 1, 50 6? Aug To Julia Niggli, 1, 51 21 Apr To Marie Winteler, with a 10? Aug To Mileva Maric;;, 1, 52 postscript by Pauline Einstein, after 10 Aug–before 10 Sep 1,18 From Mileva Maric;;, 1, 53 7 Sep To the Department of Education, 10 Sep To Mileva Maric;;, 1, 54 Canton of Aargau, 1, 20 11 Sep To Julia Niggli, 1, 55 4–25 Nov From Marie Winteler, 1, 29 11 Sep To Pauline Winteler, 1, 56 30 Nov From Marie Winteler, 1, 30 28? Sep To Mileva Maric;;, 1, 57 10 Oct To Mileva Maric;;, 1, 58 1897 19 Oct To the Swiss Federal Council, 1, 60 May? To Pauline Winteler, 1, 34 1900 21 May To Pauline Winteler, 5: Vol. 1, 34a 7 Jun To Pauline Winteler, 1, 35 ? From Mileva Maric;;, 1, 61 after 20 Oct From Mileva Maric;;, 1, 36 28 Feb To the Swiss Department of Foreign Affairs, 1, 62 1898 26 Jun To the Zurich City Council, 1, 65 29? Jul To Mileva Maric;;, 1, 68 ? To Maja Einstein, 1, 38 1 Aug To Mileva Maric;;, 1, 69 2 Jan To Mileva Maric;; [envelope only], 1 6 Aug To Mileva Maric;;, 1, 70 13 Jan To Maja Einstein, 8: Vol. -
Der Mythos Der Deutschen Atombombe
Langsame oder schnelle Neutronen? Der Mythos der deutschen Atombombe Prof. Dr. Manfred Popp Karlsruher Institut für Technologie Ringvorlesung zum Gedächtnis an Lise Meitner Freie Universität Berlin 29. Oktober 2018 In diesem Beitrag geht es zwar um Arbeiten zur Kernphysik in Deutschland während des 2.Weltkrieges, an denen Lise Meitner wegen ihrer Emigration 1938 nicht teilnahm. Es geht aber um das Thema Kernspaltung, zu dessen Verständnis sie wesentliches beigetragen hat, um die Arbeit vieler, gut vertrauter, ehemaliger Kollegen und letztlich um das Schicksal der deutschen Physik unter den Nationalsozialisten, die ihre geistige Heimat gewesen war. Da sie nach dem Abwurf der Bombe auf Hiroshima auch als „Mutter der Atombombe“ diffamiert wurde, ist es ihr gewiss nicht gleichgültig gewesen, wie ihr langjähriger Partner und Freund Otto Hahn und seine Kollegen während des Krieges mit dem Problem der möglichen Atombombe umgegangen sind. 1. Stand der Geschichtsschreibung Die Geschichtsschreibung über das deutsche Uranprojekt 1939-1945 ist eine Domäne amerikanischer und britischer Historiker. Für die deutschen Geschichtsforscher hatte eines der wenigen im Ergebnis harmlosen Kapitel der Geschichte des 3. Reiches keine Priorität. Unter den alliierten Historikern hat sich Mark Walker seit seiner Dissertation1 durchgesetzt. Sein Beitrag zur Geschichte der Kaiser Wilhelm-Gesellschaft im 3. Reich beginnt mit den Worten: „The Kaiser Wilhelm Institute for Physics is best known as the place where Werner Heisenberg worked on nuclear weapons for Hitler.“2 Im Jahr 2016 habe ich zum ersten Mal belegt, dass diese Schlussfolgerung auf Fehlinterpretationen der Dokumente und auf dem Ignorieren physikalischer Fakten beruht.3 Seit Walker gilt: Nicht an fehlenden Kenntnissen sei die deutsche Atombombe gescheitert, sondern nur an den ökonomischen Engpässen der deutschen Kriegswirtschaft: „An eine Bombenentwicklung wäre [...] auch bei voller Unterstützung des Regimes nicht zu denken gewesen. -
Progress Report
Progress Report 2008–2009 We owe special thanks to the Austrian Science Fund (FWF) for its financial support for numerous projects of the research facilities of the Austrian Academy of Sciences All rights reserved Copyright © 2009 by Austrian Academy of Sciences Layout: Art Quarterly Publishing House Werbe- und PR-Agentur GmbH. Printed and bound: Wograndl 3 Table of contents Preface . 5 RESEARCH FACILITIES OF THE SECTION FOR MATHEMATICS AND NATURAL SCIENCES Biology and Medicine CeMM – Research Center for Molecular Medicine GmbH . 11 Breath Research Institute . 14 GMI – Gregor Mendel Institute of Molecular Plant Biology . 18 IMBA – Institute of Molecular Biotechnology GmbH . 22 Institute for Biomedical Aging Research . 26 Institute for Biophysics and Nanosystems Research . 30 Konrad Lorenz Institute for Ethology . 34 Earth Sciences Institute for Geographic Information Science . 37 Center for Geosciences . 40 Commission for the Palaeontological and Stratigraphical Research of Austria . 42 Commission for Geophysical Research . 45 Commission for Quaternary Research . 48 Commission for Basic Research on Mineral Raw Materials . 51 Mathematics, Simulation and Metrology Institute for Integrated Sensor Systems . 55 Acoustics Research Institute . 58 Johann Radon Institute for Computational and Applied Mathematics . 61 Commission for Scientific Visualization . 65 Physics and Materials Sciences Erich Schmid Institute of Materials Science . 68 Institute of High Energy Physics . 71 Institute for Quantum Optics and Quantum Information . 74 Stefan Meyer Institute for Subatomic Physic. 77 Environmental Research Institute for Limnology . 80 Institute of Technology Assessment . 83 Commission for Interdisciplinary Ecological Studies . 86 Space Research Space Research Institute . 89 Commission for Astronomy . 92 Interdepartmental Research Tasks Commission for Scientific Co-operation with the Austrian Federal Ministry of Defence and Sports . -
Reversed out (White) Reversed
Berkeley rev.( white) Berkeley rev.( FALL 2014 reversed out (white) reversed IN THIS ISSUE Berkeley’s Space Sciences Laboratory Tabletop Physics Bringing More Women into Physics ALUMNI NEWS AND MORE! Cover: The MAVEN satellite mission uses instrumentation developed at UC Berkeley's Space Sciences Laboratory to explore the physics behind the loss of the Martian atmosphere. It’s a continuation of Berkeley astrophysicist Robert Lin’s pioneering work in solar physics. See p 7. photo credit: Lockheed Martin Physics at Berkeley 2014 Published annually by the Department of Physics Steven Boggs: Chair Anil More: Director of Administration Maria Hjelm: Director of Development, College of Letters and Science Devi Mathieu: Editor, Principal Writer Meg Coughlin: Design Additional assistance provided by Sarah Wittmer, Sylvie Mehner and Susan Houghton Department of Physics 366 LeConte Hall #7300 University of California, Berkeley Berkeley, CA 94720-7300 Copyright 2014 by The Regents of the University of California FEATURES 4 12 18 Berkeley’s Space Tabletop Physics Bringing More Women Sciences Laboratory BERKELEY THEORISTS INVENT into Physics NEW WAYS TO SEARCH FOR GOING ON SIX DECADES UC BERKELEY HOSTS THE 2014 NEW PHYSICS OF EDUCATION AND SPACE WEST COAST CONFERENCE EXPLORATION Berkeley theoretical physicists Ashvin FOR UNDERGRADUATE WOMEN Vishwanath and Surjeet Rajendran IN PHYSICS Since the Space Lab’s inception are developing new, small-scale in 1959, Berkeley physicists have Women physics students from low-energy approaches to questions played important roles in many California, Oregon, Washington, usually associated with large-scale of the nation’s space-based scientific Alaska, and Hawaii gathered on high-energy particle experiments. -
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 .............................