ESSAY a Most Rare Vision: Eddington's Thinking on the Relation Between Science and Religion1
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Strange Bedfellows: C. S. Lewis and Fred Hoyle
Inklings Forever: Published Colloquium Proceedings 1997-2016 Volume 10 A Collection of Essays Presented at the Tenth Frances White Ewbank Colloquium on Article 73 C.S. Lewis & Friends 6-5-2016 Strange Bedfellows: C. S. Lewis and Fred Hoyle Kristine Larsen Central Connecticut State University Follow this and additional works at: https://pillars.taylor.edu/inklings_forever Part of the English Language and Literature Commons, History Commons, Philosophy Commons, and the Religion Commons Recommended Citation Larsen, Kristine (2016) "Strange Bedfellows: C. S. Lewis and Fred Hoyle," Inklings Forever: Published Colloquium Proceedings 1997-2016: Vol. 10 , Article 73. Available at: https://pillars.taylor.edu/inklings_forever/vol10/iss1/73 This Essay is brought to you for free and open access by the Center for the Study of C.S. Lewis & Friends at Pillars at Taylor University. It has been accepted for inclusion in Inklings Forever: Published Colloquium Proceedings 1997-2016 by an authorized editor of Pillars at Taylor University. For more information, please contact [email protected]. Strange Bedfellows: C. S. Lewis and Fred Hoyle By Kristine Larsen Kristine Larsen is Professor of Astronomy at Central Connecticut State University. She is the author of Stephen Hawking: A Biography and Cosmology 101, and co-editor of The Mythological Dimensions of Doctor Who and The Mythological Dimensions of Neil Gaiman. In a May 15, 1952 letter to Genia Goelz, a recent convert to Christianity, C. S. Lewis urges “If Hoyle answers your letter, then let the correspondence drop. He is not a great philosopher (and none of my scientific colleagues think much of him as a scientist)” Letters( 3: 192). -
Living Philosophies by ALBERT EINSTEIN JOHN DEWEY SIR
Living Philosophies BY ALBERT EINSTEIN JOHN DEWEY SIR JAMES JEANS H. G. WELLS THEODORE DREISER H. L. MENCKEN JAMES TRUSLOW ADAMS JULIA PETERKIN SIR ARTHUR KEITH IRVING BABBITT BEATRICE WEBB JOSEPH WOOD KRUTCH FRIDTJOF NANSEN LEWIS MUMFORD ROBERT ANDREWS MILLIKAN HU SHIH HILAIRE BELLOC J. B. S. HALDANE GEORGE JEAN NATHAN IRWIN EDMAN BERTRAND RUSSELL WILLIAM RALPHINGE 1931 SIMON AND SCHUSTER · NEW YORK ALL RIGHTS RESERVED Copyright, 1930, by Forum Publishing Company Copyright, 1931, by Simon and Schuster, Inc. Manufactured in the United States of America NOTES T HE publishers wish to acknowledge their indebtedness to DR. HENRY GODDARD LEACH, Editor of The Forum Magazine, for his invaluable coöperation in the arranging and publication of this symposium. THE contributions of Sir James Jeans, Hilaire Belloc, William Ralph Inge and J. B. S. Haldane are reprinted, with the kind permission of George Allen and Unwin, Ltd., from two symposiums entitled Points of View and More Points of View . [This page intentionally left blank.] CONTENTS I. ALBERT EINSTEIN 3 II. BERTRAND RUSSELL 9 III. JOHN DEWEY 21 IV. ROBERT ANDREWS MILLIKAN 37 V. THEODORE DREISER 55 VI. H. G. WELLS 79 VII. FRIDTJOF NANSEN 93 VIII. SIR JAMES JEANS 107 IX. IRVING BABBITT 121 X. SIR ARTHUR KEITH 139 XI. JAMES TRUSLOW ADAMS 153 XII. H. L. MENCKEN 179 XIII. JULIA PETERKIN 195 XIV. LEWIS MUMFORD 205 XV. GEORGE JEAN NATHAN 221 XVI. HU SHIH 235 XVII. JOSEPH WOOD KRUTCH 265 XVIII. IRWIN EDMAN 277 XIX. HILAIRE BELLOC 287 XX. BEATRICE WEBB 295 XXI. WILLIAM RALPH INGE 307 XXII. J. B. S. -
Physics Celebrity #24 (Neil's Bohr)
Niels Bohr (Danish) 1885 – 1962) made foundational contributions to understanding atomic structure and quantum mechanics, for which he received Neils Bohr (1885 - 1962) the Nobel Prize in Physics in 1922. Bohr was also a philosopher and a promoter of scientific research. He developed the Bohr model of the atom with the atomic nucleus at the centre and electrons in orbit around it, which he compared to the planets orbiting the Sun. He helped develop quantum mechanics, in which electrons move from one energy level to another in discrete steps, instead of continuously. He founded the Institute of Theoretical Physics at the University of Copenhagen, now known as the Niels Bohr Institute, which opened in 1920. Bohr mentored and collaborated with physicists including Hans Kramers, Oskar Klein, George de Hevesy and Werner Heisenberg. He predicted the existence of a new zirconium-like element, which was named hafnium, after Copenhagen, when it was discovered. Later, the element bohrium was named after him. He conceived the principle of complementarity: that items could be separately analysed as having contradictory properties, like behaving as a wave or a stream of particles. The notion of complementarity dominated his thinking on both science and philosophy. During the 1930s, Bohr gave refugees from Nazism temporary jobs at the Institute, provided them with financial support, arranged for them to be awarded fellowships from the Rockefeller Foundation, and ultimately found them places at various institutions around the world. After Denmark was occupied by the Germans, he had a dramatic meeting in Copenhagen with Heisenberg, who had become the head of the German nuclear energy project. -
L. Susan Stebbing, CEM Joad, and Philipp Frank on the Philosophy Of
Knowledge Missemination: L. Susan Stebbing, C.E.M. Joad, and Philipp Frank on the Philosophy of the Physicists Adam Tamas Tuboly Institute of Philosophy, Hungarian Academy of Sciences; Institute of Transdisciplinary Discoveries, University of Pecs Science popularization might take different forms. In the early twentieth cen- tury, Sir James Jeans and Sir Arthur Eddington presented the most successful endeavors. Philosophers were highly unimpressed and disturbed by these pop- ular works and various authors declared their disagreement with the physi- cists’ philosophical books against their own philosophical background. I will discuss three different philosophers, L. Susan Stebbing, C. E. M. Joad, and Philipp Frank, whose three lines of criticism represent three different forms of philosophy, social engagement, and scientific outlook. What is interesting is that there was a point when the most diverse philosophers (of science) agreed in contrast of their common enemy, namely, those popularizing scientists that have their reputation and use it to propagate false, or at least misleading views about science, culture, and values. What we shall see is how far this agreement went among these figures and how the divergent strategies culminated in very similar results regarding knowledge dissemination. Keywords: Susan Stebbing, Arthur Eddington, James Jeans, philosophy of physics, popularization of science, C.E.M. Joad, Philipp Frank, logical empiricism The paper was first presented at the Matter and Life: Historico-logical Issues in Post-1800 Physics and Biology workshop (Sarton Centre for History of Science, Ghent University, 27. 08. 2018). I am indebted to Bohang Chen, Maarten van Dyck and Charles T. Wolfe. I am also grateful to George Reisch for the many discussions on Frank’s philosophy, the two anonymous reviewers of the journal and to Alexander Levine and Michael Whitworth for their kindness and help. -
Georges Lemaître: Life, Science and Legacy 17 July 1894 —22 June 1966
Georges Lemaître: Life, science and legacy 17 July 1894 —22 June 1966 Simon MiBon St Edmund’s College, University of Cambridge With the fruiKul collaboraon of: Rodney Holder (Cambridge), Michael Robson (Cambridge), Cormac O’Raifeartaigh (Waterford Inst. Technology) Principal sources of biographical informaon: Dominique Lambert (Louvain), Un Atome d’Universe, 2000 Thomas Herzog (Louvain), 2012 Nussbaumer and Bieri, Discovering the Expanding Universe, 2009 25 November 1915 Prussian Academy of Sciences Albert Einstein, age 36, a ciLzen of Switzerland, a subject of the Kingdom of Prussia, and quite a dandy, unveils a consistent set of gravitaonal field equaons… (… but only aer a race against Lme with David Hilbert) The Lemaître family and the Birth of Georges, 1894 Charleroi. The ancestry of Georges can be traced through five generaons: a great great grandfather Clément enlisted in Napoléon’s army and fought at Waterloo. The family was strongly patrioLc. His parents married on 30 August 1893. Georges was born on 17 July 1894, the first of four sons. Georges’ father started a glassworks and conducted experiments on the industrial producLon of glass. Young Georges was familiar with fiery furnaces where decorave glasswork was created. In 1910 fire reduced the factory to a heap of ashes. They moved to Brussels, where father secured a well-paid posiLon with Société Générale Educaon 1904-10. Age 10-16. Enrolled at a grammar school (Lan and Greek) run by Jesuits. Makes his mark as an excepLonal pupil of mathemacs, physics and chemistry. 1910-14. Studies civil engineering at the Catholic University of Louvain. The Western front 1914-18 9 August 1914. -
On Arthur Eddington's Theory of Everything
1 On Arthur Eddington’s Theory of Everything Helge Kragh Abstract: From 1929 to his death in 1944, A. Eddington worked on developing a highly ambitious theory of fundamental physics that covered everything in the physical world, from the tiny electron to the universe at large. His unfinished theory included abstract mathematics and spiritual philosophy in a mix which was peculiar to Eddington but hardly intelligible to other scientists. The constants of nature, which he claimed to be able to deduce purely theoretically, were of particular significance to his project. Although highly original, Eddington’s attempt to provide physics with a new foundation had to some extent parallels in the ideas of other British physicists, including P. Dirac and E. A. Milne. Eddington’s project was however a grand failure in so far that it was rejected by the large majority of physicists. A major reason was his unorthodox view of quantum mechanics. 1. Introduction Arthur Stanley Eddington is recognized as one of the most important scientists of the first half of the twentieth century (Douglas 1956). He owes this elevated position primarily to his pioneering work in astronomy and astrophysics, and secondarily to his expositions of and contributions to the general theory of relativity. Eddington developed a standard model of the interior structure of stars and was the first to suggest nuclear reactions as the basic source of stellar energy. In 1919 he rose to public fame when he, together with Frank Dyson, confirmed Einstein’s prediction of the bending of starlight around the Sun. Six years later he applied general relativity to white dwarf stars, and in 1930 he developed one of the first relativistic models of the expanding universe known as the Lemaître-Eddington model. -
Georges Lemaître and the Foundations of Big Bang Cosmology.’ the Antiquarian Astronomer 14 (June 2020), 2–20
To cite this article: Simon A. Mitton, ‘Georges Lemaître and the foundations of Big Bang cosmology.’ The Antiquarian Astronomer 14 (June 2020), 2–20. Keywords. Georges Lemaître, Einstein universe, De Sitter universe, cosmological constant, Hubble law, expanding universe, dark energy, general relativity, science and religion Author: Simon A. Mitton, [email protected]. St Edmund’s College, Cambridge CB3 0BN, United Kingdom Georges Lemaître and the foundations of Big Bang cosmology Simon A. Mitton Georges Lemaître was a remarkable contributor to the advancement of cosmol- ogy in the heady years following the two great revolutions in theoretical physics in the last century: general relativity and quantum mechanics. In the past two decades the impact of his key publications has advanced from very little to enor- mous. Among other landmark achievements, Lemaître was the first cosmologist to estimate the rate of expansion of the Universe, later known as the Hubble constant. In 2018 the International Astronomical Union renamed the Hubble law as the Hubble–Lemaître law in recognition of his foundational contribution to the theory of the expanding Universe. This biographical review examines: factors that influenced his approach to the philosophy of science, particularly cosmology; his engagement with the network of contemporary cosmologists; and the circumstances of his withdrawal from research in cosmology and the further promotion of ‘the fireworks universe’ after the early 1930s. 1. Recognition by the International 2. Early life and education Astronomical Union 2018 Georges Lemaître had a fascinating and varied life in Georges Henri Joseph Édouard Lemaître (1894–1966) science. As a Catholic priest he made an intriguing aca- died three days after learning from his successor at the demic, working in both heavenly theology and cosmical Catholic University of Louvain, the Belgian mathemati- theory. -
Lord Rutherford (1871–1937): the Newton of the Atom and the Winner
Essays DOI: 10.1002/anie.200803876 History of Science Lord Rutherford (1871–1937): The Newton of the Atom and the Winner of the Nobel Prize for Chemistry, 1908 John Meurig Thomas* atomic physics · history of science · radiochemistry · Rutherford, Ernest 1. Introduction three towering achievements associated was largely his “boys”—a term which he with his name—the theory of nuclear used affectionately to describe his stu- When Ernest Rutherford, later disintegration (with Frederick Soddy, dents and collaborators—who had de- known as Lord Rutherford of Nelson, 1902–1903), his model of the nuclear veloped radar and other devices of died unexpectedly in 1937, the New atom (1911), and the discovery of the strategic military significance. It was York Times stated: “…It is given to but artificial disintegration of the nucleus his assistants Chadwick and Cockcroft few men to achieve immortality, still less (1919)—the first two, while based on (later Nobel Prize winners each in their to achieve Olympian rank, during their experimental evidence, were theoretical own right) who built the UK Atomic own lifetime. Lord Rutherford achieved concepts. Even more ironic is that Energy Authority. both. In a generation that witnessed one Rutherford was awarded the Nobel of the greatest revolutions in the entire Prize in Chemistry (not Physics) in history of science he was universally 1908. When news of this award reached 2. The Trajectory of Rutherford’s acknowledged as the leading explorer of him he laughingly commented that he Life the vast infinitely complex -
The Legacy of James Clerk Maxwell and Herrmann Von Helmholtz Peter Skiff Bard College
Bard College Bard Digital Commons Faculty Books & Manuscripts Bard Faculty Publications 2016 The hP ysicist - Philosophers: The Legacy of James Clerk Maxwell and Herrmann von Helmholtz Peter Skiff Bard College Follow this and additional works at: http://digitalcommons.bard.edu/facbooks Part of the History of Science, Technology, and Medicine Commons, Philosophy of Science Commons, and the Physics Commons Recommended Citation Skiff, Peter, "The hP ysicist - Philosophers: The Legacy of James Clerk Maxwell and Herrmann von Helmholtz" (2016). Faculty Books & Manuscripts. 1. http://digitalcommons.bard.edu/facbooks/1 This Book is brought to you for free and open access by the Bard Faculty Publications at Bard Digital Commons. It has been accepted for inclusion in Faculty Books & Manuscripts by an authorized administrator of Bard Digital Commons. For more information, please contact [email protected]. THE PHYSICIST - PHILOSOPHERS The Legacy of James Clerk Maxwell and Herrmann von Helmholtz Peter Skiff Bard College, 2016 ACKNOWLEDGMENTS This work was begun 25 years into a 50 year career at Bard College. This position gave me access to an extraordinary range of exceptional faculty, distinguished visiting scholars, and brilliant student researchers, all of whom inspired and informed im investigating academic fields I pursued: mathematical physics and the history and philosophy of science. In addition the editors of the American Library Association’s Choice magazine provided literally hundreds of books for review for college libraries. It is from this trove of ideas and information I have been assembling this book. I am particularly grateful to particular advice and information from Hannah Arendt, Heinrich Bluecher, Irma Brandeis, and A. -
Chapter Four the Mysterious Universe of James Jeans
Durham E-Theses Popular Theology from Popular Scientists: Assessing the Legacy of Eddington and Jeans as Apologists REYNOLDS, JONATHAN,OWEN How to cite: REYNOLDS, JONATHAN,OWEN (2017) Popular Theology from Popular Scientists: Assessing the Legacy of Eddington and Jeans as Apologists , Durham theses, Durham University. Available at Durham E-Theses Online: http://etheses.dur.ac.uk/12370/ Use policy The full-text may be used and/or reproduced, and given to third parties in any format or medium, without prior permission or charge, for personal research or study, educational, or not-for-prot purposes provided that: • a full bibliographic reference is made to the original source • a link is made to the metadata record in Durham E-Theses • the full-text is not changed in any way The full-text must not be sold in any format or medium without the formal permission of the copyright holders. Please consult the full Durham E-Theses policy for further details. Academic Support Oce, Durham University, University Oce, Old Elvet, Durham DH1 3HP e-mail: [email protected] Tel: +44 0191 334 6107 http://etheses.dur.ac.uk 2 Popular Theology from Popular Scientists: Assessing the Legacy of Eddington and Jeans as Apologists Abstract This thesis asserts and demonstrates that the current historical evaluation of the significance of Arthur Eddington and James Jeans is inadequate. Not only has their importance in the years between the two World Wars been forgotten, but their transitional role in the science and religion debate post-Darwin is now largely unrecognised. Both had a major influence on subsequent popular apologists and Eddington in particular influenced post war academic theologians as diverse as Thomas Torrance and Eric Mascall. -
Sir Edmund Taylor Whittaker (1873–1956)
British Journal for the History of Mathematics ISSN: 2637-5451 (Print) 2637-5494 (Online) Journal homepage: https://www.tandfonline.com/loi/tbsh21 ‘A man who has infinite capacity for making things go’: Sir Edmund Taylor Whittaker (1873–1956) Alison Maidment & Mark McCartney To cite this article: Alison Maidment & Mark McCartney (2019): ‘A man who has infinite capacity for making things go’: Sir Edmund Taylor Whittaker (1873–1956), British Journal for the History of Mathematics, DOI: 10.1080/26375451.2019.1619410 To link to this article: https://doi.org/10.1080/26375451.2019.1619410 Published online: 25 May 2019. Submit your article to this journal View Crossmark data Full Terms & Conditions of access and use can be found at https://www.tandfonline.com/action/journalInformation?journalCode=tbsh21 British Journal for the History of Mathematics, 2019 https://doi.org/10.1080/26375451.2019.1619410 ‘A man who has infinite capacity for making things go’: Sir Edmund Taylor Whittaker (1873–1956) ALISON MAIDMENT The Open University, UK MARK MCCARTNEY Ulster University, UK Among the leading mathematicians of the nineteenth and twentieth centuries was British mathematician and astronomer, Sir Edmund Taylor Whittaker. Born in Southport, in the north of England, Whittaker began his career at the University of Cambridge, before moving to Dunsink to become Royal Astronomer of Ireland and Andrews Professor of Astronomy at Trinity College, Dublin, and finishing in Scotland as Professor of Mathematics at the University of Edinburgh. Whittaker completed original work in a variety of fields, ranging from pure mathematics to mathematical physics and astronomy, as well as publishing on topics in philosophy, history, and theology. -
Cold Dark Matter Cosmology Conflicts with Fluid Mechanics and Observations
Journal of Applied Fluid Mechanics (accepted) 1 Cold Dark Matter Cosmology Conflicts with Fluid Mechanics and Observations Carl H. Gibson1 1 University of California at San Diego, La Jolla, California, 92122-0411, USA Email: [email protected] ABSTRACT Cold dark matter hierarchical clustering (CDMHC) cosmology based on the Jeans 1902 criterion for gravitational instability gives predictions about the early universe contrary to fluid mechanics and observations. Jeans neglected viscosity, diffusivity, and turbulence: factors that determine gravitational structure formation and contradict small structures (CDM halos) forming from non-baryonic dark matter particle candidates. From hydro- gravitational-dynamics (HGD) cosmology, viscous-gravitational fragmentation produced supercluster (1046 kg), cluster, and galaxy-mass (1042 kg) clouds in the primordial plasma with the large fossil density turbulence -17 -3 12 (ρ0= 3 ! 10 kg m ) of the first fragmentation at 10 s, and a protogalaxy linear and spiral clump morphology reflecting maximum stretching near vortex lines of the plasma turbulence at the 1013 s plasma-gas transition. Gas protogalaxies fragmented into proto-globular-star-cluster mass (1036 kg) clumps of protoplanet gas clouds that are now frozen as earth-mass (1024-25 kg) Jovian planets of the baryonic dark matter, about 30,000,000 rogue planets per star. All stars form from these planets. They appear in planetary nebulae and are misinterpreted as dark energy. Observations contradict the CDMHCC prediction of large explosive Population III first stars at 1016 s, but support the immediate gentle formation of small Population II first stars in globular-star-clusters from HGD. Keywords: Cold Dark Matter, Gravitational Structure Formation, Dark Energy, Turbulence 1.