Scientists and War 1916-2016 by Dave Webb Leeds Beckett University and Scientists for Global Responsibility
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2019 in the Academic Ranking of World Universities (ARWU)
THE UNIVERSITY OF MANCHESTER FACTS AND FIGURES 2020 2 The University 4 World ranking 6 Academic pedigree 8 World-class research CONTENTS 10 Students 12 Making a difference 14 Global challenges, Manchester solutions 16 Stellify 18 Graduate careers 20 Staff 22 Faculties and Schools 24 Alumni 26 Innovation 28 Widening participation UNIVERSITY OF MANCHESTER 30 Cultural institutions UNIVERSITY OF MANCHESTER 32 Income 34 Campus investment 36 At a glance 1 THE UNIVERSITY OF MANCHESTER Our vision is to be recognised globally for the excellence of our people, research, learning and innovation, and for the benefits we bring to society and the environment. Our core goals and strategic themes Research and discovery Teaching and learning Social responsibility Our people, our values Innovation Civic engagement Global influence 2 3 WORLD RANKING The quality of our teaching and the impact of our research are the cornerstones of our success. We have risen from 78th in 2004* to 33rd – our highest ever place – in 2019 in the Academic Ranking of World Universities (ARWU). League table World ranking European ranking UK ranking 33 8 6 ARWU 33 8 6 WORLD EUROPE UK QS 27 8 6 Times Higher Education 55 16 8 *2004 ranking refers to the Victoria University of Manchester prior to the merger with UMIST. 4 5 ACADEMIC PEDIGREE 1906 1908 1915 1922 1922 We attract the highest-calibre researchers and teachers, with 25 Nobel Prize winners among J Thomson Ernest Rutherford William Archibald V Hill Niels Bohr Physics Chemistry Larence Bragg Physiology or Medicine Physics our current and former staff and students. -
Hendrik Antoon Lorentz's Struggle with Quantum Theory A. J
Hendrik Antoon Lorentz’s struggle with quantum theory A. J. Kox Archive for History of Exact Sciences ISSN 0003-9519 Volume 67 Number 2 Arch. Hist. Exact Sci. (2013) 67:149-170 DOI 10.1007/s00407-012-0107-8 1 23 Your article is published under the Creative Commons Attribution license which allows users to read, copy, distribute and make derivative works, as long as the author of the original work is cited. You may self- archive this article on your own website, an institutional repository or funder’s repository and make it publicly available immediately. 1 23 Arch. Hist. Exact Sci. (2013) 67:149–170 DOI 10.1007/s00407-012-0107-8 Hendrik Antoon Lorentz’s struggle with quantum theory A. J. Kox Received: 15 June 2012 / Published online: 24 July 2012 © The Author(s) 2012. This article is published with open access at Springerlink.com Abstract A historical overview is given of the contributions of Hendrik Antoon Lorentz in quantum theory. Although especially his early work is valuable, the main importance of Lorentz’s work lies in the conceptual clarifications he provided and in his critique of the foundations of quantum theory. 1 Introduction The Dutch physicist Hendrik Antoon Lorentz (1853–1928) is generally viewed as an icon of classical, nineteenth-century physics—indeed, as one of the last masters of that era. Thus, it may come as a bit of a surprise that he also made important contribu- tions to quantum theory, the quintessential non-classical twentieth-century develop- ment in physics. The importance of Lorentz’s work lies not so much in his concrete contributions to the actual physics—although some of his early work was ground- breaking—but rather in the conceptual clarifications he provided and his critique of the foundations and interpretations of the new ideas. -
Goverdhan Mehta Chemistry - a 21St Century Science for Global Sustainability: Is It Future Ready?
Goverdhan Mehta Chemistry - A 21st Century Science for Global Sustainability: Is it future ready? Goverdhan Mehta A ‘selfie’ with theSchool chemical of Chemistry world…… University of Hyderabad National Geophysical Research Institute, CSIR Foundation Day, Sept. 27, 2019 Introducing Chemistry through the Lens of Earth's Systems: What Role Can Systems Thinking Play in Developing Chemically and Environmentally Literate Citizens? J. Kornfeld, S. Stokoe. J. Chemical Education 2019, 96, 2910-2917 A bouquet of ‘matters’ that matter New symbols Passion Sustainability Legacies Ethics & values Responsible Connections Systems Directions Humility Ideas & icons Inspirations Un mélange de beaucoup de choses “Chemistry ought not to be for chemists alone” - Miguel de Unamuno ‘…Life, Universe and Everything’ Chemistry – a source of happiness…. Chem -Connectome ‘...I feel sorry for people who don’t know anything about chemistry. They are missing an important source of happiness....’ - Linus Pauling 1901-1994 S.A. Matlin, G. Mehta, H. Hopf. Chemistry Embraced by All. Science 2015, 347, 1179 Chemistry is in everything. and everything is in it, it is the basis of life, without it we wouldn't exist. Green tea has ~ 200 chemicals Coffee has ~ 1000 chemicals Wine has >1000 chemicals Light cigarette ~ 4000 chemicals Chemistry is ubiquitous/omnipresent Chemistry – Tracing the roots and to the present BCE Art & craft of mixing substances A giant knowledge leap Alchemy to modern science Evidence based science Discipline in a Table - systematization Mendeleev’s Periodic Law ‘Molecularization’ of chemical matter 20th Century A century of evolutionary march of chemistry 20h Century Value added products from almost anything “Utility science” and everything Molecular understanding of life processes and “Core Science” chemical matter Interdisciplinarity in forefront “Integrative Science” Resource stressed planet “Sustainability Science” 21st Century S. -
George De Hevesy in America
Journal of Nuclear Medicine, published on July 13, 2019 as doi:10.2967/jnumed.119.233254 George de Hevesy in America George de Hevesy was a Hungarian radiochemist who was awarded the Nobel Prize in Chemistry in 1943 for the discovery of the radiotracer principle (1). As the radiotracer principle is the foundation of all diagnostic and therapeutic nuclear medicine procedures, Hevesy is widely considered the father of nuclear medicine (1). Although it is well-known that he spent time at a number of European institutions, it is not widely known that he also spent six weeks at Cornell University in Ithaca, NY, in the fall of 1930 as that year’s Baker Lecturer in the Department of Chemistry (2-6). “[T]he Baker Lecturer gave two formal presentations per week, to a large and diverse audience and provided an informal seminar weekly for students and faculty members interested in the subject. The lecturer had an office in Baker Laboratory and was available to faculty and students for further discussion.” (7) There is also evidence that, “…Hevesy visited Harvard [University, Cambridge, MA] as a Baker Lecturer at Cornell in 1930…” (8). Neither of the authors of this Note/Letter was aware of Hevesy’s association with Cornell University despite our longstanding ties to Cornell until one of us (WCK) noticed the association in Hevesy’s biographical page on the official Nobel website (6). WCK obtained both his undergraduate degree and medical degree from Cornell in Ithaca and New York City, respectively, and spent his career in nuclear medicine. JRO did his nuclear medicine training at Columbia University and has subsequently been a faculty member of Weill Cornell Medical College for the last eleven years (with a brief tenure at Memorial Sloan Kettering Cancer Center (affiliated with Cornell)), and is now the program director of the Nuclear Medicine residency and Chief of the Molecular Imaging and Therapeutics Section. -
Einstein's Mistakes
Einstein’s Mistakes Einstein was the greatest genius of the Twentieth Century, but his discoveries were blighted with mistakes. The Human Failing of Genius. 1 PART 1 An evaluation of the man Here, Einstein grows up, his thinking evolves, and many quotations from him are listed. Albert Einstein (1879-1955) Einstein at 14 Einstein at 26 Einstein at 42 3 Albert Einstein (1879-1955) Einstein at age 61 (1940) 4 Albert Einstein (1879-1955) Born in Ulm, Swabian region of Southern Germany. From a Jewish merchant family. Had a sister Maja. Family rejected Jewish customs. Did not inherit any mathematical talent. Inherited stubbornness, Inherited a roguish sense of humor, An inclination to mysticism, And a habit of grüblen or protracted, agonizing “brooding” over whatever was on its mind. Leading to the thought experiment. 5 Portrait in 1947 – age 68, and his habit of agonizing brooding over whatever was on its mind. He was in Princeton, NJ, USA. 6 Einstein the mystic •“Everyone who is seriously involved in pursuit of science becomes convinced that a spirit is manifest in the laws of the universe, one that is vastly superior to that of man..” •“When I assess a theory, I ask myself, if I was God, would I have arranged the universe that way?” •His roguish sense of humor was always there. •When asked what will be his reactions to observational evidence against the bending of light predicted by his general theory of relativity, he said: •”Then I would feel sorry for the Good Lord. The theory is correct anyway.” 7 Einstein: Mathematics •More quotations from Einstein: •“How it is possible that mathematics, a product of human thought that is independent of experience, fits so excellently the objects of physical reality?” •Questions asked by many people and Einstein: •“Is God a mathematician?” •His conclusion: •“ The Lord is cunning, but not malicious.” 8 Einstein the Stubborn Mystic “What interests me is whether God had any choice in the creation of the world” Some broadcasters expunged the comment from the soundtrack because they thought it was blasphemous. -
Copyright by Paul Harold Rubinson 2008
Copyright by Paul Harold Rubinson 2008 The Dissertation Committee for Paul Harold Rubinson certifies that this is the approved version of the following dissertation: Containing Science: The U.S. National Security State and Scientists’ Challenge to Nuclear Weapons during the Cold War Committee: —————————————————— Mark A. Lawrence, Supervisor —————————————————— Francis J. Gavin —————————————————— Bruce J. Hunt —————————————————— David M. Oshinsky —————————————————— Michael B. Stoff Containing Science: The U.S. National Security State and Scientists’ Challenge to Nuclear Weapons during the Cold War by Paul Harold Rubinson, B.A.; M.A. Dissertation Presented to the Faculty of the Graduate School of The University of Texas at Austin in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy The University of Texas at Austin August 2008 Acknowledgements Thanks first and foremost to Mark Lawrence for his guidance, support, and enthusiasm throughout this project. It would be impossible to overstate how essential his insight and mentoring have been to this dissertation and my career in general. Just as important has been his camaraderie, which made the researching and writing of this dissertation infinitely more rewarding. Thanks as well to Bruce Hunt for his support. Especially helpful was his incisive feedback, which both encouraged me to think through my ideas more thoroughly, and reined me in when my writing overshot my argument. I offer my sincerest gratitude to the Smith Richardson Foundation and Yale University International Security Studies for the Predoctoral Fellowship that allowed me to do the bulk of the writing of this dissertation. Thanks also to the Brady-Johnson Program in Grand Strategy at Yale University, and John Gaddis and the incomparable Ann Carter-Drier at ISS. -
Network Map of Knowledge And
Humphry Davy George Grosz Patrick Galvin August Wilhelm von Hofmann Mervyn Gotsman Peter Blake Willa Cather Norman Vincent Peale Hans Holbein the Elder David Bomberg Hans Lewy Mark Ryden Juan Gris Ian Stevenson Charles Coleman (English painter) Mauritz de Haas David Drake Donald E. Westlake John Morton Blum Yehuda Amichai Stephen Smale Bernd and Hilla Becher Vitsentzos Kornaros Maxfield Parrish L. Sprague de Camp Derek Jarman Baron Carl von Rokitansky John LaFarge Richard Francis Burton Jamie Hewlett George Sterling Sergei Winogradsky Federico Halbherr Jean-Léon Gérôme William M. Bass Roy Lichtenstein Jacob Isaakszoon van Ruisdael Tony Cliff Julia Margaret Cameron Arnold Sommerfeld Adrian Willaert Olga Arsenievna Oleinik LeMoine Fitzgerald Christian Krohg Wilfred Thesiger Jean-Joseph Benjamin-Constant Eva Hesse `Abd Allah ibn `Abbas Him Mark Lai Clark Ashton Smith Clint Eastwood Therkel Mathiassen Bettie Page Frank DuMond Peter Whittle Salvador Espriu Gaetano Fichera William Cubley Jean Tinguely Amado Nervo Sarat Chandra Chattopadhyay Ferdinand Hodler Françoise Sagan Dave Meltzer Anton Julius Carlson Bela Cikoš Sesija John Cleese Kan Nyunt Charlotte Lamb Benjamin Silliman Howard Hendricks Jim Russell (cartoonist) Kate Chopin Gary Becker Harvey Kurtzman Michel Tapié John C. Maxwell Stan Pitt Henry Lawson Gustave Boulanger Wayne Shorter Irshad Kamil Joseph Greenberg Dungeons & Dragons Serbian epic poetry Adrian Ludwig Richter Eliseu Visconti Albert Maignan Syed Nazeer Husain Hakushu Kitahara Lim Cheng Hoe David Brin Bernard Ogilvie Dodge Star Wars Karel Capek Hudson River School Alfred Hitchcock Vladimir Colin Robert Kroetsch Shah Abdul Latif Bhittai Stephen Sondheim Robert Ludlum Frank Frazetta Walter Tevis Sax Rohmer Rafael Sabatini Ralph Nader Manon Gropius Aristide Maillol Ed Roth Jonathan Dordick Abdur Razzaq (Professor) John W. -
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. -
William Lawrence Bragg
W ILLIAM L AWRENCE B R A G G The diffraction of X-rays by crystals Nobel Lecture, September 6, 1922* It is with the very greatest pleasure that I take this opportunity of expressing my gratitude to you for the great honour which you bestowed upon me, when you awarded my father and myself the Nobel Prize for Physics in the year 1915. In other years scientists have come here to express their thanks to you, who have received this great distinction for the work of an illustrious career devoted to research. That you should have given me, at the very out- set of my scientific career, even the most humble place amongst their ranks, is an honour of which I cannot but be very proud. You invited me here two years ago, after the end of the war, but a series of unfortunate circumstances made it impossible for me to accept your invi- tation. I have always profoundly regretted this, and it was therefore with the very greatest satisfaction that I received the invitation of Prof. Arrhenius a few months ago, and arranged for this visit. I am at last able to tell you how deeply grateful I am to you, and to give you my thanks in person. You have already honoured with the Nobel Prize Prof. von Laue, to whom we owe the great discovery which has made possible all progress in a new realm of science, the study of the structure of matter by the diffraction of X-rays. Prof von Laue, in his Nobel Lecture, has described to you how he was led to make his epochal discovery. -
Named Organic Reactions (U – Z)
Dr. John Andraos, http://www.careerchem.com/NAMED/Named-Rxns(U-Z).pdf 1 NAMED ORGANIC REACTIONS (U – Z) © Dr. John Andraos, 2000 - 2014 Department of Chemistry, York University 4700 Keele Street, Toronto, ONTARIO M3J 1P3, CANADA For suggestions, corrections, additional information, and comments please send e-mails to [email protected] http://www.chem.yorku.ca/NAMED/ Sakae Uemura Japanese, b. Japan Uemura oxidation Nishimura, T.; Onoue, T.; Ohe, K.; Uemura S. Tetrahedron Lett. 1998 , 39 , 6011 Nishimura, T.; Onoue, T.; Ohe, K.; Uemura S. J. Org. Chem. 1999 , 64 , 6750 Biographical references: Ivar Karl Ugi 5 September 1930 – 29 September 2005 German, b. Kuressaare, Estland, Germany Ugi condensation Ugi, I.; Meyr, R.; Fetzer, U.; Steinbrueckner, C. Angew. Chem. 1959 , 71 , 386 Urban, R.; Ugi, I., Angew. Chem. Int. Engl. Ed . 1975 , 14 , 61 Biographical references: Chemical Research Faculties: An International Directory 1996 , American Chemical Society: Washington, D.C., 1996 Wer ist Wer? Das Deutsche Who’s Who 1999/2000 , Schmidt-Römhild: Lübeck, 1999 Lemmen, P.; Fontain, E.; Bauer, J. Angew. Chem. Int. Ed. 2006 , 45 , 193 Fritz Ullmann 2 July 1875 - 17 March 1939 German, b. Fürth, Germany Ullmann reaction Ullmann, F. Ann. Chem . 1904 , 332 , 38 Dr. John Andraos, http://www.careerchem.com/NAMED/Named-Rxns(U-Z).pdf 2 Biographical references: Meyer, K.H., Helv. Chim. Acta 1940 , 23 , 93 Upjohn reaction Van Rheenen, V.; Kelly, R.C.; Cha, D.Y. Tetrahedron Lett. 1976 , 1973 A. Verley French, b. ? Meerwein-Pondorff-Verley reduction see Hans Leberecht Meerwein Biographical references: Victor Villiger 1 September 1868 - 1934 Swiss, b. -
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 -
4. Marie Curie, Ethics and Research
CATHERINE MILNE 4. MARIE CURIE, ETHICS AND RESEARCH INTRODUCTION Recently Chemistry and Engineering News (Bard, Prestwich, Wight, Heller, & Zimmerman, 2010) carried a series of commentaries on the culture of academic research in chemistry with a focus on the role of funding in research. Initially, Alan Bard decried how decisions about tenure seem more and more to focus on grant getting rather than consideration of the applicant’s accomplishments generated because of access to this funding. Bard argued further that often this funding was based, not on the quality of the proposed research but on a researcher’s ability to “hype their research” and damming truth in the process (Bard et al., 2010, p. 27). According to him, there was a disturbing trend in universities for researchers to be encouraged, almost expected, to generate patents and from there, even to be involved in initiating “start up” companies. Other researchers responded. Glen Prestwich and Charles Wight (Bard et al., 2010) argue that if researchers were able to present a clear connection between “taxpayer dollars” and funded research, the public would realize the value that science delivers. Prestwich and Wight argue further that a new cadre of researchers is involved in identifying real world problems, translating basic research into applications, and creating products as well as publications. Moving from basic research to applications that address real world problems is called translational research, and Prestwich and Wight see this research as a positive development in chemistry. Adam Heller (Bard et al., 2010) weighs in claiming that the pursuit of “patent-protected, people-serving products” was not “a sad sign of our times but a reawakening of the proud history of academic chemistry and chemical engineering” (p.