Some Remarks on the Impact of Computers on Mathematics and Physics ∗
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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. -
GEORGE ELMER FORSYTHE January 8, 1917—April 9, 1972
MATHEMATICS OF COMPUTATION, VOLUME 26, NUMBER 120, OCTOBER 1972 GEORGE ELMER FORSYTHE January 8, 1917—April9, 1972 With the sudden death of George Forsythe, modern numerical analysis has lost one of its earliest pioneers, an influential leader who helped bring numerical analysis and computer science to their present positions. We in computing have been fortunate to have benefited from George's abilities, and we all feel a deep sense of personal and professional loss. Although George's interest in calculation can be traced back at least to his seventh grade attempt to see how the digits repeated in the decimal expansion of 10000/7699, his early research was actually in summability theory, leading to his Ph.D. in 1941 under J. D. Tamarkin at Brown University. A brief period at Stanford thereafter was interrupted by his Air Force service, during which he became interested in meteor- ology, co-authoring an influential book in that field. George then spent a year at Boeing, where his interest in scientific computing was reawakened, and in 1948 he began his fruitful association with the Institute for Numerical Analysis of the National Bureau of Standards on the UCLA campus, remaining at UCLA for three years after leaving the Institute in 1954. In 1957 he rejoined the Mathematics Department at Stanford as Professor, became director of the Computation Center, and eventually Chairman of the Computer Science Department when it was founded in 1965. George greatly influenced the development of modern numerical analysis, especially in numerical linear algebra where his 1953 classification of methods for solving linear systems gave structure to a field of great importance. -
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. -
Know Your Discipline: Teaching the Philosophy of Computer Science
Journal of Information Technology Education Volume 6, 2007 Know Your Discipline: Teaching the Philosophy of Computer Science Matti Tedre University of Joensuu, Dept. of Computer Science and Statistics Joensuu, Finland [email protected] Executive Summary The diversity and interdisciplinarity of computer science and the multiplicity of its uses in other sciences make it hard to define computer science and to prescribe how computer science should be carried out. The diversity of computer science also causes friction between computer scien- tists from different branches. Computer science curricula, as they stand, have been criticized for being unable to offer computer scientists proper methodological training or a deep understanding of different research traditions. At the Department of Computer Science and Statistics at the Uni- versity of Joensuu we decided to include in our curriculum a course that offers our students an awareness of epistemological and methodological issues in computer science, and we wanted to design the course to be meaningful for practicing computer scientists. In this article the needs and aims of our course on the philosophy of computer science are discussed, and the structure and arrangements—the whys, whats, and hows—of that course are explained. The course, which is given entirely on-line, was designed for advanced graduate or postgraduate computer science students from two Finnish universities: the University of Joensuu and the Uni- versity of Kuopio. The course has four relatively broad themes, and all those themes are tied to the students’ everyday work or their own research topics. I have prepared course readings about each of those four themes. -
The Scholarly Work of Reliable and Well-Designed Mathematical Software a Personal Perspective
The Scholarly Work of Reliable and Well-Designed Mathematical Software A personal perspective Tim Davis July 9, 2014 1 The Scholarly Work of Reliable and Well-Designed Mathematical Software Outline: What defines a scholarly work? Does mathematical software fit that definition? Why publish prototype-quality mathematical software? Why publish robust, reliable, and full-featured mathematical software? Troubling trends and a troubling status quo My recommendations for you and for SIAM 2 Definition of \scholarly work" Scholarly or artistic works, regardless of their form of expression: intended purpose is to disseminate the results of academic research, scholarly study, or artistic expression, ... in any medium. When is a work scholarly (software or any other form)? Proposed metrics: 1 peer-reviewed 2 published in reputable academic journals 3 published in academic-quality books 4 topic of discussion at academic conferences 5 citation for academic society fellow 3 Peer-reviewed software ACM Transactions on Mathematical Software Founded in 1975 Purpose: As a scientific journal, ACM Transactions on Mathematical Software (TOMS) documents the theoretical underpinnings of numeric, symbolic, algebraic, and geometric computing applications. It focuses on analysis and construction of algorithms and programs, and the interaction of programs and architecture. Algorithms documented in TOMS are available as the Collected Algorithms of the ACM in print, on microfiche, on disk, and online. 942 Collected Algorithms of the ACM since 1975: peer-reviewed scholarly software I serve as an Associate Editor of this journal 4 ACM TOMS Editorial Charter The purpose of the ACM Transactions on Mathematical Software (TOMS) is to communicate important research results addressing the development, evaluation and use of mathematical software. -
George and Alexandra Forsythe Papers Dates: 1936-1979 Physical Description: 40 Linear Feet Language(S): the Materials Are in English
http://oac.cdlib.org/findaid/ark:/13030/tf158001gt Online items available Guide to the Daniel Hartwig Stanford University. Libraries.Department of Special Collections and University Archives Stanford, California 2000 Copyright © 2015 The Board of Trustees of the Leland Stanford Junior University. All rights reserved. Note This encoded finding aid is compliant with Stanford EAD Best Practice Guidelines, Version 1.0. Guide to the SC0098 1 Overview Call Number: SC0098 Creator: Forsythe, Alexandra I. Creator: Forsythe, George E. , (George Elmer), 1917-1972. Title: George and Alexandra Forsythe papers Dates: 1936-1979 Physical Description: 40 Linear feet Language(s): The materials are in English. Repository: Department of Special Collections and University Archives Green Library 557 Escondido Mall Stanford, CA 94305-6064 Email: [email protected] Phone: (650) 725-1022 URL: http://library.stanford.edu/spc Custodial History Gift of Mrs. Sandra Forsythe, 1972, and Dianne and Warren Forsythe, 1979. Information about Access The materials are open for research use. Ownership & Copyright Property rights reside with the repository. Literary rights reside with the creators of the documents or their heirs. To obtain permission to publish or reproduce, please contact the Public Services Librarian of the Dept. of Special Collections and University Archives. Cite As [Identification of item], George and Alexandra Forsythe Papers, SC 098, Stanford University Archives, Stanford, Calif. Biography Memorial Resolution: George Elmer Forsythe 1917-1972 George E. Forsythe, Professor and Chairman of the Department of Computer Science, died on April 9, 1972, at the age of 55. He founded the Stanford Computer Science Department, one of the first such departments in the nation, on January 1, 1965. -
Programming Using MATLAB
Preface Numerical Computing with MATLAB is a textbook for an introductory course in numerical methods, Matlab, and technical computing. The emphasis is on in- formed use of mathematical software. We want you learn enough about the mathe- matical functions in Matlab that you will be able to use them correctly, appreciate their limitations, and modify them when necessary to suit your own needs. The topics include ² introduction to Matlab, ² linear equations, ² interpolation, ² zero and roots, ² least squares, ² quadrature, ² ordinary di®erential equations, ² random numbers, ² Fourier analysis, ² eigenvalues and singular values, ² partial di®erential equations. George Forsythe initiated a software-based numerical methods course at Stan- ford University in the late 1960s. The textbooks by Forsythe, Malcolm, and Moler [1] and Kahaner, Moler, and Nash [2] that evolved from the Stanford course were based upon libraries of Fortran subroutines. This textbook is based upon Matlab. NCM, a collection of over 70 M- ¯les, forms an essential part of the book. Many of the over 200 exercises involve modifying and extending the programs in NCM. The book also makes extensive use of computer graphics, including interactive graphical expositions of numerical algorithms. The prerequisites for the course, and the book, include December 26, 2005 1 2 Preface ² calculus, ² some familiarity with ordinary di®erential equations, ² some familiarity with matrices, ² some computer programming experience. If you've never used Matlab before, the ¯rst chapter will help you get started. If you're already familiar with Matlab, you can glance over most of the ¯rst chapter quickly. Everyone should read the section in the ¯rst chapter about floating-point arithmetic. -
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.