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Literature Compass Editing Humphry Davy's
1 ‘Work in Progress in Romanticism’ Literature Compass Editing Humphry Davy’s Letters Tim Fulford, Andrew Lacey, Sharon Ruston An editorial team of Tim Fulford (De Montfort University) and Sharon Ruston (Lancaster University) (co-editors), and Jan Golinski (University of New Hampshire), Frank James (the Royal Institution of Great Britain), and David Knight1 (Durham University) (advisory editors) are currently preparing The Collected Letters of Sir Humphry Davy: a four-volume edition of the c. 1200 surviving letters of Davy (1778-1829) and his immediate circle, for publication with Oxford University Press, in both print and electronic forms, in 2020. Davy was one of the most significant and famous figures in the scientific and literary culture of early nineteenth-century Britain, Europe, and America. Davy’s scientific accomplishments were varied and numerous, including conducting pioneering research into the physiological effects of nitrous oxide (laughing gas); isolating potassium, calcium, and several other metals; inventing a miners’ safety lamp (the bicentenary of which was celebrated in 2015); developing the electrochemical protection of the copper sheeting of Royal Navy vessels; conserving the Herculaneum papyri; writing an influential text on agricultural chemistry; and seeking to improve the quality of optical glass. But Davy’s endeavours were not merely limited to science: he was also a poet, and moved in the same literary circles as Lord Byron, Samuel Taylor Coleridge, Robert Southey, and William Wordsworth. Since his death, Davy has rarely been out of the public mind. He is still the frequent subject of biographies (by, 1 David Knight died in 2018. David gave generously to the Davy Letters Project, and a two-day conference at Durham University was recently held in his memory. -
1 the Equation of a Light Leptonic Magnetic Monopole and Its
The equation of a Light Leptonic Magnetic Monopole and its Experimental Aspects Georges Lochak Fondation Louis de Broglie 23, rue Marsoulan F-75012 Paris [email protected] Abstract. The present theory is closely related to Dirac’s equation of the electron, but not to his magnetic monopole theory, except for his relation between electric and magnetic charge. The theory is based on the fact, that the massless Dirac equation admits a second electromagnetic coupling, deduced from a pseudo-scalar gauge invariance. The equation thus obtained has the symmetry laws of a massless leptonic, magnetic monopole, able to interact weakly. We give a more precise form of the Dirac relation between electric and magnetic charges and a quantum form of the Poincaré first integral. In the Weyl representation our equation splits into P-conjugated monopole and antimonopole equations with the correct electromagnetic coupling and opposite chiralities, predicted by P. Curie. Charge conjugated monopoles are symmetric in space and not in time (contrary to the electric particles) : an important fact for the vacuum polarization. Our monopole is a magnetically excited neutrino, which leads to experimental consequences. These monopoles are assumed to be produced by electromagnetic pulses or arcs, leading to nuclear transmutations and, for beta radioactive elements, a shortening of the life time and the emission of monopoles instead of neutrinos in a magnetic field. A corresponding discussion is given in section 15. 1. Introduction. The hypothesis of separated magnetic poles is very old. In the 2nd volume of his famous Treatise of Electricity and Magnetism [1], devoted to Magnetism, Maxwell considered the existence of free magnetic charges as an evidence, just as the evidence of electric charges. -
Alfred Nobel
www.bibalex.org/bioalex2004conf The BioVisionAlexandria 2004 Conference Newsletter November 2003 Volume 1, Issue 2 BioVisionAlexandria ALFRED NOBEL 2004 aims to celebrate the The inventor, the industrialist outstanding scientists and scholars, in a he Nobel Prize is one of the highest distinctions recognized, granting its winner century dominated by instant fame. However, many do not know the interesting history and background technological and T that led to this award. scientific revolutions, through its It all began with a chemist, known as Alfred Nobel, born in Stockholm, Sweden in 1833. Nobel Day on 3 April Alfred Nobel moved to Russia when he was eight, where his father, Immanuel Nobel, 2004! started a successful mechanical workshop. He provided equipment for the Russian Army and designed naval mines, which effectively prevented the British Royal Navy from moving within firing range of St. Petersburg during the Crimean War. Immanuel Nobel was also a pioneer in the manufacture of arms, and in designing steam engines. INSIDE Scientific awards .........3 Immanuel’s success enabled him to Alfred met Ascanio Sobrero, the Italian Confirmed laureates ....4 Lady laureates ............7 provide his four sons with an excellent chemist who had invented Nitroglycerine education in natural sciences, languages three years earlier. Nitroglycerine, a and literature. Alfred, at an early age, highly explosive liquid, was produced by acquired extensive literary knowledge, mixing glycerine with sulfuric and nitric mastering many foreign languages. His acid. It was an invention that triggered a Nobel Day is interest in science, especially chemistry, fascination in the young scientist for many dedicated to many of was also apparent. -
Unerring in Her Scientific Enquiry and Not Afraid of Hard Work, Marie Curie Set a Shining Example for Generations of Scientists
Historical profile Elements of inspiration Unerring in her scientific enquiry and not afraid of hard work, Marie Curie set a shining example for generations of scientists. Bill Griffiths explores the life of a chemical heroine SCIENCE SOURCE / SCIENCE PHOTO LIBRARY LIBRARY PHOTO SCIENCE / SOURCE SCIENCE 42 | Chemistry World | January 2011 www.chemistryworld.org On 10 December 1911, Marie Curie only elements then known to or ammonia, having a water- In short was awarded the Nobel prize exhibit radioactivity. Her samples insoluble carbonate akin to BaCO3 in chemistry for ‘services to the were placed on a condenser plate It is 100 years since and a chloride slightly less soluble advancement of chemistry by the charged to 100 Volts and attached Marie Curie became the than BaCl2 which acted as a carrier discovery of the elements radium to one of Pierre’s electrometers, and first person ever to win for it. This they named radium, and polonium’. She was the first thereby she measured quantitatively two Nobel prizes publishing their results on Boxing female recipient of any Nobel prize their radioactivity. She found the Marie and her husband day 1898;2 French spectroscopist and the first person ever to be minerals pitchblende (UO2) and Pierre pioneered the Eugène-Anatole Demarçay found awarded two (she, Pierre Curie and chalcolite (Cu(UO2)2(PO4)2.12H2O) study of radiactivity a new atomic spectral line from Henri Becquerel had shared the to be more radioactive than pure and discovered two new the element, helping to confirm 1903 physics prize for their work on uranium, so reasoned that they must elements, radium and its status. -
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. -
Arthur S. Eddington the Nature of the Physical World
Arthur S. Eddington The Nature of the Physical World Arthur S. Eddington The Nature of the Physical World Gifford Lectures of 1927: An Annotated Edition Annotated and Introduced By H. G. Callaway Arthur S. Eddington, The Nature of the Physical World: Gifford Lectures of 1927: An Annotated Edition, by H. G. Callaway This book first published 2014 Cambridge Scholars Publishing 12 Back Chapman Street, Newcastle upon Tyne, NE6 2XX, UK British Library Cataloguing in Publication Data A catalogue record for this book is available from the British Library Copyright © 2014 by H. G. Callaway All rights for this book reserved. No part of this book may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, electronic, mechanical, photocopying, recording or otherwise, without the prior permission of the copyright owner. ISBN (10): 1-4438-6386-6, ISBN (13): 978-1-4438-6386-5 CONTENTS Note to the Text ............................................................................... vii Eddington’s Preface ......................................................................... ix A. S. Eddington, Physics and Philosophy .......................................xiii Eddington’s Introduction ................................................................... 1 Chapter I .......................................................................................... 11 The Downfall of Classical Physics Chapter II ......................................................................................... 31 Relativity Chapter III -
Funding of the Papal Army's Campaign to Germany During The
9 Petr VOREL Funding of the Papal Army’s Campaign to Germany during the Schmalkaldic War (Edition of the original accounting documentation “Conto de la Guerra de Allemagna” kept by the Pope’s accountant Pietro Giovanni Aleotti from 22 June 1546 to 2 September 1547) Abstract: This article is based on the recently discovered text of accounting documentation led by the Papal secret accountant Pietro Giovanni Aleotti. He kept records of income and expenses of Papal chamber connected with the campaign of Papal army that was sent from Italy to Germany by Pope Paul III (Alessandro Farnese) in the frame of the first period of so called Smalkaldic War (1546–1547). The author publishes this unique source in extenso and completes the edition by the detailed analysis of the incomes and expenses of this documentation. The analysis is extended by three partial texts dealing with 1) so called Jewish tax that was announced by Paul III in the financial support of military campaign, 2) credit granting of this campaign by the bank house of Benvenuto Olivieri in connection with the collection of Papal tithe in the Romagna region and 3) staffing of the commanding officers of Papal army during this campaign (in the attachment one can find a reconstruction of the officers’ staff with identification of the most important commanders). In the conclusion the author tries to determine the real motives why Paul III decided to take part in this campaign. In comparison to the previous works the author accents mainly the efforts of the Farnese family to raise their prestige at the end of the pontificate of Paul III and their immediate financial interests that are reflected in the account documentation. -
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. -
Atomic History Project Background: If You Were Asked to Draw the Structure of an Atom, What Would You Draw?
Atomic History Project Background: If you were asked to draw the structure of an atom, what would you draw? Throughout history, scientists have accepted five major different atomic models. Our perception of the atom has changed from the early Greek model because of clues or evidence that have been gathered through scientific experiments. As more evidence was gathered, old models were discarded or improved upon. Your task is to trace the atomic theory through history. Task: 1. You will create a timeline of the history of the atomic model that includes all of the following components: A. Names of 15 of the 21 scientists listed below B. The year of each scientist’s discovery that relates to the structure of the atom C. 1- 2 sentences describing the importance of the discovery that relates to the structure of the atom Scientists for the timeline: *required to be included • Empedocles • John Dalton* • Ernest Schrodinger • Democritus* • J.J. Thomson* • Marie & Pierre Curie • Aristotle • Robert Millikan • James Chadwick* • Evangelista Torricelli • Ernest • Henri Becquerel • Daniel Bernoulli Rutherford* • Albert Einstein • Joseph Priestly • Niels Bohr* • Max Planck • Antoine Lavoisier* • Louis • Michael Faraday • Joseph Louis Proust DeBroglie* Checklist for the timeline: • Timeline is in chronological order (earliest date to most recent date) • Equal space is devoted to each year (as on a number line) • The eight (8) *starred scientists are included with correct dates of their discoveries • An additional seven (7) scientists of your choice (from -
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. -
Appendix E Nobel Prizes in Nuclear Science
Nuclear Science—A Guide to the Nuclear Science Wall Chart ©2018 Contemporary Physics Education Project (CPEP) Appendix E Nobel Prizes in Nuclear Science Many Nobel Prizes have been awarded for nuclear research and instrumentation. The field has spun off: particle physics, nuclear astrophysics, nuclear power reactors, nuclear medicine, and nuclear weapons. Understanding how the nucleus works and applying that knowledge to technology has been one of the most significant accomplishments of twentieth century scientific research. Each prize was awarded for physics unless otherwise noted. Name(s) Discovery Year Henri Becquerel, Pierre Discovered spontaneous radioactivity 1903 Curie, and Marie Curie Ernest Rutherford Work on the disintegration of the elements and 1908 chemistry of radioactive elements (chem) Marie Curie Discovery of radium and polonium 1911 (chem) Frederick Soddy Work on chemistry of radioactive substances 1921 including the origin and nature of radioactive (chem) isotopes Francis Aston Discovery of isotopes in many non-radioactive 1922 elements, also enunciated the whole-number rule of (chem) atomic masses Charles Wilson Development of the cloud chamber for detecting 1927 charged particles Harold Urey Discovery of heavy hydrogen (deuterium) 1934 (chem) Frederic Joliot and Synthesis of several new radioactive elements 1935 Irene Joliot-Curie (chem) James Chadwick Discovery of the neutron 1935 Carl David Anderson Discovery of the positron 1936 Enrico Fermi New radioactive elements produced by neutron 1938 irradiation Ernest Lawrence