Heinz Billing
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Early Life: 1924–1945
An interview with FRITZ BAUER Conducted by Ulf Hashagen on 21 and 26 July, 2004, at the Technische Universität München. Interview conducted by the Society for Industrial and Applied Mathematics, as part of grant # DE-FG02-01ER25547 awarded by the US Department of Energy. Transcript and original tapes donated to the Computer History Museum by the Society for Industrial and Applied Mathematics © Computer History Museum Mountain View, California ABSTRACT: Professor Friedrich L. Bauer describes his career in physics, computing, and numerical analysis. Professor Bauer was born in Thaldorf, Germany near Kelheim. After his schooling in Thaldorf and Pfarrkirchen, he received his baccalaureate at the Albertinium, a boarding school in Munich. He then faced the draft into the German Army, serving first in the German labor service. After training in France and a deployment to the Eastern Front in Kursk, he was sent to officer's school. His reserve unit was captured in the Ruhr Valley in 1945 during the American advance. He returned to Pfarrkirchen in September 1945 and in spring of 1946 enrolled in mathematics and physics at the Ludwig-Maximilians-Universitäat, München. He studied mathematics with Oscar Perron and Heinrich Tietze and physics with Arnold Sommerfeld and Paul August Mann. He was offered a full assistantship with Fritz Bopp and finished his Ph.D. in 1951 writing on group representations in particle physics. He then joined a group in Munich led by a professor of mathematics Robert Sauer and the electrical engineer Hans Piloty, working with a colleague Klaus Samelson on the design of the PERM, a computer based in part on the Whirlwind concept. -
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. -
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. -
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. -
CV of Prof. Dietrich
CURRICULUM VITAE PERSONAL DETAILS Name & Surname Tim Dietrich Address University of Potsdam Institute for Physics and Astronomy Karl-Liebknecht-Str. 24/25 14476, Potsdam Email [email protected] Telephone +49/331977230160 Birth date 23th of April 1988 Nationality German Marital Status Married; 1 child EDUCATION 2016 PhD (”summa cum laude”–excellent 1.0) Faculty of Physics and Astronomy, Friedrich-Schiller-University Jena, Germany 2012 Master of Science in Physics (1.0) Faculty of Physics and Astronomy, Friedrich-Schiller-University Jena, Germany 2010 Bachelor of Science in Physics (1.0) Institute of Physics, Martin-Luther-University Halle-Wittenberg, Germany 2007 High school diploma (1.0) – Gymnasium Philanthropinum Dessau PROFESSIONAL EXPERIENCE since 2020 Professor for Theoretical Astrophysics (W1) at the University of Potsdam since 2020 Adjunct Researcher at Max Planck Institute for Gravitational Physics Potsdam 2018-2020 Marie Sklodowska-Curie Fellow at Nikhef, Amsterdam 2015-2018 Postdoc at the Max Planck Institute for Gravitational Physics Potsdam 2015 Research assistant at the Friedrich-Schiller-University Jena 2011-2014 Research assistant for the CRC/TR-7 Gravitational Wave Astronomy 2008-2010 Research assistant at the Martin-Luther-University Halle-Wittenberg Fellowships and Awards Scholarships: 2013-2015 Scholarship of the Landesgraduiertenstipendium Thuringia 2010 Gustav-Mie Scholarship of Martin-Luther-University [declined] 2009-2012 Scholarship of the German National Academic Foundation Grants: 2017 Individual Marie-Curie Fellowship Awards/Prizes: 2019 Heinz Billing Prize for the Advancement of Computational Science 2017 PhD thesis prize of the German Physical Society of the sections “Gravitation and Relativity”, “Hadrons and Nucleons”, and “Particle physics” 2017 PhD thesis prize of the Friedrich Schiller University Jena 2010 Gustav-Mie-Bachelor-Prize Host for Fellowships 2021 Host for the Humboldt Fellowship of Dr. -
Scientific Background
3 OCTOBER 2017 Scientifc Background on the Nobel Prize in Physics 2017 THE LASER INTERFEROMETER GRAVITATIONAL-WAVE OBSERVATORY AND THE FIRST DIRECT OBSERVATION OF GRAVITATIONAL WAVES The Nobel Committee for Physics THE ROYAL SWEDISH ACADEMY OF SCIENCES has as its aim to promote the sciences and strengthen their infuence in society. BOX 50005 (LILLA FRESCATIVÄGEN 4 A), SE-104 05 STOCKHOLM, SWEDEN Nobel Prize® and the Nobel Prize® medal design mark TEL +46 8 673 95 00, [email protected] WWW.KVA.SE are registrated trademarks of the Nobel Foundation The Laser Interferometer Gravitational-Wave Observatory and the first direct observation of gravitational waves Introduction Our knowledge and understanding of the Universe is based on millennia of observations of the quanta of electromagnetic radiation – photons – in a wide range of wavelengths. These studies have taught us a lot – not only about planets, stars and galaxies but also about the origins of structure, the evolution and possibly the fate of the Universe. It turns out, however, that highly energetic photons do not reach us from the furthest recesses of the cosmos. So, during the past few decades, new kinds of telescopes have been developed, leading to unexpected breakthroughs. These detectors exploit other forms of radiation: cosmic rays, neutrinos and gravitational waves. The existence of gravitational radiation is linked to the general theory of relativity and was predicted by Einstein a century ago [1, 2]. Gravitational waves are travelling ripples in space-time. They arise when heavy objects accelerate and hence generate disturbances in the gravitational fields. These distortions, described as waves, move outward from the source at the speed of light and give rise to effects that, in principle, are measurable when they reach Earth given sufficiently sensitive detectors. -
Grundprogramme
Research Collection Report Did Alan Turing interrogate Konrad Zuse in Göttingen in 1947? Author(s): Bruderer, Herbert Publication Date: 2013 Permanent Link: https://doi.org/10.3929/ethz-a-009782023 Rights / License: In Copyright - Non-Commercial Use Permitted This page was generated automatically upon download from the ETH Zurich Research Collection. For more information please consult the Terms of use. ETH Library Departement Informatik Did Alan Turing interrogate Konrad Zuse in Göttingen in 1947? Herbert Bruderer Abstract Turing and Zuse had many similar ideas. But they did not know each other, they were isolated. It was not until the end of World War II that they heard about their respective achievements. And in late summer 1947 there was a mysterious meeting in Göttingen. British scientists of the National Physical Laboratory (Teddington, London) interrogated German researchers. Participants included Arthur Porter, Alan Turing and John Womersley (England) as well as Heinz Billing, Helmut Schreyer, Alwin Walther and Konrad Zuse. This reunion is described by the memoir of the German computer pioneer Billing from the Max Planck Institute for Physics (Munich). However, in the memoirs published by Porter and Zuse the colloquium at Göttingen is not mentioned. With the exception of Heinz Billing all the actors have died. Therefore it is difficult to verify the story. We are still looking for further evidence. Keywords: Alan Turing, Konrad Zuse, Heinz Billing, National Physical Laboratory (London), Max Planck In- stiute for Physics (Göttingen/Munich), interrogation 1. Introduction This paper discusses the question of an unknown potential meeting between the computer pioneers Alan Turing and Konrad Zuse. -
Chrillys Goldpreis-Report Inhaltsverzeichnis
Chrillys Goldpreis-Report Oktober 2019 von Dr. Chrilly Donninger, Chef für Alles Univ. Prof. Ingo Althöfer, Wissenschaft Anni Donninger, Illustration&Lektorat. Inhaltsverzeichnis: Lothar Collatz in ernsten Jahren von Univ. Prof. Ingo Althöfer Prof. Althöfer hat eine Biografie über den bedeutenden deutschen Mathematiker Lother Collatz geschrieben. Ausgehend von den Recherchen zu Lothar Collatz hat er auch eine ganze Menge Material über die Rolle mathematisch begabter junger Frauen im 2. Weltkrieg gefunden. Lokale Erderwärmung von Chrilly Donninger Chrilly hat sich österreichische Wetterdaten angeschaut und diese analysiert. Das Ergebnis ist: Es gibt einen langfristigen Anstieg der Temperatur. Es gibt jedoch auch eine Reihe von kurzfristigen Schwankungen. Ein Zeitraum von 10 Jahren ist zu kurz um sinnvolle Aussagen zu machen. Musikverein von Anni und Chrilly Donninger Das alte Ehepaar hat nach Jahrzehnten wieder ein klassisches Konzert im Wiener Musikverein besucht. Es hat diesmal besser funktioniert, der Chief wird alt. Die Illustration von Anni bezieht sich auf das mexikanische Fest El Dia de los Muertos (Tag der Toten). Das unmittelbare Datum ist der 2. November, die Vorbereitungen darauf beginnen bereits Mitte Oktober. El Dia de los Muertos gehört zum immateriellen Kulturerbe der Menschheit. An Herrn Collatz Lachen ist gesund, mein Kleiner. Tot gelacht hat sich noch keiner. Wenn's auch schwer fällt, lache doch, flenne kannste immer noch. (Aus dem IPM-Gedichtband zur Weihnacht 1940) Lothar Collatz in ernsten Jahren Ingo Althöfer, Jena Institut für Mathematik Friedrich-Schiller Universität [email protected] Einleitung Lothar Collatz (1910 - 1990) war ein berühmter Mathematiker, mit Spezialgebiet Numerik. Aktuell beträgt die Anzahl seiner akademischen Nachkommen (Doktoranden, deren Doktoranden usw.) 1.325, darunter viele Professoren. -
The Race for the First Reactor When the Max Planck Institute for Physics Relocated to Munich 50 Years Ago, It Found More Than Just a New Home
The Race for the First Reactor When the Max Planck Institute for Physics relocated to Munich 50 years ago, it found more than just a new home. Following the move from Göttingen – another instance of Werner Heisenberg’s deep commitment – the institute also changed its scientifi c focus. Instead of nuclear fi ssion, the scientists turned their attention to plasma research and nuclear fusion – not least be- Flashback cause of the research reactor being built in Karlsruhe for industrial purposes. t least one thing was clarifi ed by then: “Nuclear phys- icists not responsible for bad weather” declared the A GÖTTINGER TAGEBLATT on September 21, 1954, following a lecture by Rudolf Schulten, a reactor physicist at the Max Planck Institute for Physics. The article went on to explain that an exploding atomic bomb would not ionize the air suffi ciently to create areas of high or low pressure. As Schul- Gravitational waves were also among the targets hunted by scientists ten explained, it would take about 2,000 exploding bombs at the MPI for Physics in Munich – Heinz Billing tracked them down to do that. And after such an inferno, mankind would have with an aluminum cylinder, the centerpiece of the Weber experiment. more to worry about than bad weather – if mankind even still existed. desire that nuclear energy might free Bavaria from its de- Nuclear energy, and thus also nuclear physics, have clearly pendence on coal from the Rhineland, and that the Max always aroused more or less justifi ed fears. Werner Heisen- Planck Institute might attract an infl ux of talented students. -
Discovery of Two Historical Computers in Switzerland: Zuse
Discovery of Two Historical Computers in Switzerland: Zuse Machine M9 and Contraves Cora and Discovery of Unknown Documents on the Early History of Computing at the ETH Archives Herbert Bruderer Swiss Federal Institute of Technology, Zurich [email protected], [email protected] Abstract. Since 2009 we have been trying to find out more about the beginnings of computer science in Switzerland and abroad. Most eyewitnesses have already died or are over 80 years old. In general, early analog and digital computers have been dismantled long ago. Subject to exceptions, the few remaining devices are no longer functioning. Many documents have gone lost. Therefore investigations are difficult and very time-consuming. However, we were able to discover several unknown historical computers and hundreds of exciting documents of the 1950s. In 2012, the results have been published in a first book; a second volume will be forthcoming next year. Keywords: Cora, ERMETH, ETH archives, Hasler AG, Heinz Rutishauser, Konrad Zuse, M9 (=Z9), Mithra AG, Paillard SA, Remington Rand AG, Unesco, Z4. 1 Introduction My investigations into the history of computing started in 2009 in connection with the Zuse centenary (100th birthday of the German computer pioneer in 2010). The goal was to get a more comprehensive and deeper understanding of the events of the pioneering days. Coincidentally and to our surprise we discovered the program- controlled Zuse relay calculator M9 whose existence was unknown even to computer scientists. Shortly afterwards another machine emerged: the Swiss made transistor computer Cora. From 2010 to 2013 several contemporary eyewitness discussions concerning M9 and Cora took place. -
Gravitational Wave Detection by Interferometry (Ground and Space)
Gravitational Wave Detection by Interferometry (Ground and Space) Sheila Rowan Ginzton Laboratory Stanford University Stanford CA 94305-4085 e-mail:[email protected] Jim Hough Department of Physics and Astronomy University of Glasgow Glasgow G12 8QQ, UK e-mail:[email protected] Published on 29 June 2000 www.livingreviews.org/Articles/Volume3/2000-3hough Living Reviews in Relativity Published by the Max Planck Institute for Gravitational Physics Albert Einstein Institute, Germany Abstract Significant progress has been made in recent years on the development of gravitational wave detectors. Sources such as coalescing compact bi- nary systems, low-mass X-ray binaries, stellar collapses and pulsars are all possible candidates for detection. The most promising design of grav- itational wave detector uses test masses a long distance apart and freely suspended as pendulums on Earth or in drag-free craft in space. The main theme of this review is a discussion of the mechanical and optical principles used in the various long baseline systems being built around the world { LIGO (USA), VIRGO (Italy/France), TAMA 300 (Japan) and GEO 600 (Germany/UK) { and in LISA, a proposed space-borne interferometer. c 2000 Max-Planck-Gesellschaft and the authors. Further information on copyright is given at http://www.livingreviews.org/Info/Copyright/. For permission to reproduce the article please contact [email protected]. Article Amendments On author request a Living Reviews article can be amended to include errata and small additions to ensure that the most accurate and up-to-date infor- mation possible is provided. For detailed documentation of amendments, please go to the article's online version at http://www.livingreviews.org/Articles/Volume3/2000-3hough/.