Matter and Spirit in the Universe : Scientific and Religious Preludes to Modern Cosmology

Total Page:16

File Type:pdf, Size:1020Kb

Matter and Spirit in the Universe : Scientific and Religious Preludes to Modern Cosmology Matter andSpirit in the Universe Scientific and Religious Preludes to Modem Cosmology This page intentionally left blank HISTORY OF MODERN PHYSICAL SCIENCES – VOL. 3 Matter andSpirit in the Universe Scientific and Religious Preludes to Moddern Cosmology Helge Kragh Aarthus University, Denmark Imperial College Press Published by Imperial College Press 57 Shelton Street Covent Garden London WC2H 9HE Distributed by World Scientific Publishing Co. Pte. Ltd. 5 Toh Tuck Link, Singapore 596224 USA office: 27 Warren Street, Suite 401-402, Hackensack, NJ 07601 UK office: 57 Shelton Street, Covent Garden, London WC2H 9HE British Library Cataloguing-in-Publication Data A catalogue record for this book is available from the British Library. History of Modern Physical Sciences — Vol. 3 MATTER AND SPIRIT IN THE UNIVERSE Scientific and Religious Preludes to Modern Cosmology Copyright © 2004 by Imperial College Press All rights reserved. This book, or parts thereof, may not be reproduced in any form or by any means, electronic or mechanical, including photocopying, recording or any information storage and retrieval system now known or to be invented, without written permission from the Publisher. For photocopying of material in this volume, please pay a copying fee through the Copyright Clearance Center, Inc., 222 Rosewood Drive, Danvers, MA 01923, USA. In this case permission to photocopy is not required from the publisher. ISBN 1-86094-469-8 ISBN 1-86094-485-X (pbk) Typeset by Stallion Press Email: [email protected] Printed in Singapore. Ian_Matter and Spirit in the Universe.pmd1 10/4/2005, 6:37 PM B239_FM.qxd 09/23/04 11:24 AM Page v To Line and Mikkel This page intentionally left blank B239_FM.qxd 09/23/04 11:24 AM Page vi Preface The relationship between religion and science has for a long time been a central area in the history of science and ideas. Presently, it is cultivated as actively as ever. During the 20th century and the last half of the 19th century, scholars have in particular focused on evolu- tionary theory and its implications for religious belief. Cosmology, although distinctly a modern science and undeniably of great rele- vance to theology, has received curiously little attention. To wit, in John Hedley Brooke’s widely acclaimed Science and Religion: Some Historical Perspectives, an authoritative introduction and critical guide to the subject, modern cosmology is almost completely ignored. Nor have historians of physics and astronomy paid much attention to how cosmological and religious thought have interacted in the mod- ern period. I believe there is a need for a book on the issue, which is too rich and fascinating not to be dealt with in a comprehensive way. Being primarily a historian of modern physical science, I am not a specialist in the relationship between science and religious belief. My own interest in the field mostly emerged as a result of my studies in the history of cosmology, such as they appear most fully in my book, Cosmology and Controversy from 1996, which analyses in detail the emergence of the big-bang theory and its clash with the rival steady- state model. The present work relies in some respects on the material covered in my earlier book, but is broader in both chronology and scope. The focus of my study is the period between the 1850s and the B239_FM.qxd 09/23/04 11:24 AM Page vii 1960s. I start with a brief introductory chapter in which I refer to a few earlier ideas and developments, from the high Middle Ages to William Herschel’s cosmological ideas of the 1780s. The purpose is solely to introduce certain key concepts in the relationship between cosmology and religion, and also to remind the reader that the rela- tionship is an old one. It has a great past indeed. About its future I dare not prophesy. Chapter 2 deals comprehensively with the second half of the 19th century, not least with the law of entropy increase and its assumed implications for cosmology and religion. This theme, which involves nothing less than the origin and end of the universe, runs through much of the book. Chapter 3 discusses the religious views of some of the important figures in cosmological research in the early part of the 20th century, including Einstein, Eddington and Jeans. Attention is also directed to Robert Millikan and other scientists who resisted the idea of an expanding universe and favoured, in part for religious reasons, a kind of recurrent cosmology. In earlier writings I have on several occa- sions drawn attention to George Lemaître, the relatively unknown Belgian who was arguably the single most important cosmologist of the 20th century. Lemaître was also a Catholic priest, and it has sometimes been claimed that his belief in a divine creator served as a motive for the big-bang concept he introduced in 1931. This and other aspects of Lemaître’s work form the major part of Chapter 4. B239_FM.qxd 09/23/04 11:24 AM Page viii The subsequent chapter is mostly devoted to the cosmo-physical tradition of the interwar period, a tradition characterized by a strong interest in rationalistic and numerological approaches to physics and astronomy. These approaches were in some cases associated with reli- gious beliefs, although the connection was never strong. The main fig- ures of the chapter are Arthur Eddington and Paul Dirac, but I also deal in some detail with Pascual Jordan and Arthur Haas, whose contribu- tions to cosmology are less known and deserve to be recalled. Edward Milne, a prominent cosmo-physicist, is of particular interest, not only because his views were highly original but also because he explicitly linked them to his belief in God. His works and thoughts, such as they culminated in his book, Modern Cosmology and the Christian Idea of God from 1952, are described in Chapter 6. This chapter also includes aspects of the controversy in the 1950s between big-bang cosmology and the new steady-state theory of the universe. More details about the controversy can be found in Cosmology and Controversy. My story essentially ends in the mid-1960s, with the emergence of the standard hot big-bang theory, but in a final chapter I indicate some of the later developments, if only in a fragmentary and incomplete way. The book is a contribution to the history of scientific ideas, but it is neither a systematic account of cosmology’s relation to theology nor a personal opinion of how the two fields should relate. It might be tempting to include an analysis of the intense discussion which has B239_FM.qxd 09/23/04 11:24 AM Page ix occurred during the last few decades. However, this would require a new book and possibly also an author with a better knowledge of theology. It should be noted that I use the words “universe,” “cosmos” and “world” synonymously, as did most of the actors in the story I recount. What is more significant, I follow a tradition in history of science by writing about “religion” not in the broadest sense but, in most cases, in the sense of Christian belief. This is not an expression of religious intolerance or Euro-chauvinism. It merely reflects the fact that modern scientific cosmology has exclusively been devel- oped in Europe and North America. I am fully aware that the issue also involves other religions, but in so far as it relates to the historical development of modern cosmology, it is a matter of fact that Christianity has occupied (and still occupies) a unique position. I would like to express my thanks to Simon Rebsdorf, who has kindly gone through the manuscript and pointed out a number of errors. Helge Kragh B239_FM.qxd 09/23/04 11:24 AM Page x Contents Preface Introduction: Cosmo-theology before Einstein 1 1 A Thermodynamic Universe 2 17 Expanding Horizons 3 71 The Primeval-atom Universe 4 123 B239_FM.qxd 09/23/04 11:24 AM Page xi Cosmo-physics 5 161 Cosmology between Theism and Atheism 6 199 Epilogue: From Standard Model to Quantum Cosmology 7 247 Bibliography 262 Index 290 B239_Ch01.qxd 09/23/04 11:25 AM Page 1 1 Introduction: Cosmo-theology before Einstein B239_Ch01.qxd 09/23/04 11:25 AM Page 2 1 Introduction: Cosmo-theology before Einstein t is sometimes said that there is nothing new under the sun, which is surely an exaggeration. The proverb generally fails miserably in Ithe history of science—after all, to make new discoveries is the business of science, and a quite successful business it is. On the other hand, for centuries astronomy and cosmology have been concerned with essentially the same kind of questions. These can be identified at the time of Kepler, or even earlier, and 350 years later they were still subjects of debate. Some of the problems were these: (i) Has the world always existed, or did it have an origin? And, will it ever come to an end? (ii) Is the world finite or infinite in spatial content? (iii) What is the relationship between the spatial and the material universe? (iv) Is the world static or in a state of evolution? (v) From where did matter (and energy) originate? Is it still being created? (vi) Are the laws of nature, as known from the local environment, applicable to the universe at large? There are other questions of a similar cosmic nature, some of them even more comprehensive. Thus, philosophers and theologians may want to know why the world exists, or why there is something rather B239_Ch01.qxd 09/23/04 11:25 AM Page 3 3 Cosmo-theology before Einstein than nothing.
Recommended publications
  • Anthropic Explanations in Cosmology
    View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by PhilSci Archive 1 Jesús Mosterín ANTHROPIC EXPLANATIONS IN COSMOLOGY In the last century cosmology has ceased to be a dormant branch of speculative philosophy and has become a vibrant part of physics, constantly invigorated by new empirical inputs from a legion of new terrestrial and outer space detectors. Nevertheless cosmology continues to be relevant to our philosophical world view, and some conceptual and methodological issues arising in cosmology are in need of epistemological analysis. In particular, in the last decades extraordinary claims have been repeatedly voiced for an alleged new type of scientific reasoning and explanation, based on a so-called “anthropic principle”. “The anthropic principle is a remarkable device. It eschews the normal methods of science as they have been practiced for centuries, and instead elevates humanity's existence to the status of a principle of understanding” [Greenstein 1988, p. 47]. Steven Weinberg has taken it seriously at some stage, while many physicists and philosophers of science dismiss it out of hand. The whole issue deserves a detailed critical analysis. Let us begin with a historical survey. History of the anthropic principle After Herman Weyl’s remark of 1919 on the dimensionless numbers in physics, several eminent British physicists engaged in numerological or aprioristic speculations in the 1920's and 1930's (see Barrow 1990). Arthur Eddington (1923) calculated the number of protons and electrons in the universe (Eddington's number, N) and found it to be around 10 79 . He noticed the coincidence between N 1/2 and the ratio of the electromagnetic to gravitational 2 1/2 39 forces between a proton and an electron: e /Gm emp ≈ N ≈ 10 .
    [Show full text]
  • The Big Bang: Fact Or Fiction?
    Steady-state cosmologies in context From Arrhenius to Einstein, from Hoyle to Linde The Big Bang: Fact or Fiction? Cormac O’Raifeartaigh FRAS Waterford Institute of Technology Dublin Institute for Advanced Studies Overview Steady-state cosmology (static) The ideas of Arrhenius; Nernst MacMillan; Millikan Steady-state cosmology (non-static) Tolman; Einstein; Mimura; Schrödinger Einstein’s steady-state model The cosmologies of Hoyle, Bondi and Gold Einstein vs Hoyle Steady-state cosmology today Eternal inflation and the steady-state universe The steady-state universe (static) 2nd law of thermodynamics (1850-) Irreversible degenerating universe? ‘Heat death’ Replenishment of energy lost by the stars? William Rankine (1852); Arthur Holmes (1914) William Crookes (1886); George Toulmin (1789) Svante Arrhenius (1859-1927) Catastrophism vs uniformitarianism Svante Arrhenius: infinite, perpetual universe Continuous replenishment of celestial bodies via radiation pressure and galactic collisions (1903) Walther Nernst (1912, 1916) Walther Nernst (1864-1941) Zero point energy of the ether = energy resevoir The static steady-state universe (1920s) William Duncan MacMillan (1918, 1925) Radiant energy from the stars absorbed by the ether Energy reconstituted as new matter Robert Millikan (1928) William MacMillan (1871-1948) Support for MacMillan Cosmic rays from interstellar space (1925) Birth cry of creation of heavier elements (1928) Replenishment of protons from stellar radiation Atom building in interstellar space: media attention James Jeans (1928)
    [Show full text]
  • An Interpretation of Milne Cosmology
    An Interpretation of Milne Cosmology Alasdair Macleod University of the Highlands and Islands Lews Castle College Stornoway Isle of Lewis HS2 0XR UK [email protected] Abstract The cosmological concordance model is consistent with all available observational data, including the apparent distance and redshift relationship for distant supernovae, but it is curious how the Milne cosmological model is able to make predictions that are similar to this preferred General Relativistic model. Milne’s cosmological model is based solely on Special Relativity and presumes a completely incompatible redshift mechanism; how then can the predictions be even remotely close to observational data? The puzzle is usually resolved by subsuming the Milne Cosmological model into General Relativistic cosmology as the special case of an empty Universe. This explanation may have to be reassessed with the finding that spacetime is approximately flat because of inflation, whereupon the projection of cosmological events onto the observer’s Minkowski spacetime must always be kinematically consistent with Special Relativity, although the specific dynamics of the underlying General Relativistic model can give rise to virtual forces in order to maintain consistency between the observation and model frames. I. INTRODUCTION argument is that a clear distinction must be made between models, which purport to explain structure and causes (the Edwin Hubble’s discovery in the 1920’s that light from extra- ‘Why?’), and observational frames which simply impart galactic nebulae is redshifted in linear proportion to apparent consistency and causality on observation (the ‘How?’). distance was quickly associated with General Relativity (GR), and explained by the model of a closed finite Universe curved However, it can also be argued this approach does not actually under its own gravity and expanding at a rate constrained by the explain the similarity in the predictive power of Milne enclosed mass.
    [Show full text]
  • Resolving Hubble Tension with the Milne Model 3
    Resolving Hubble tension with the Milne model* Ram Gopal Vishwakarma Unidad Acade´mica de Matema´ticas Universidad Auto´noma de Zacatecas, Zacatecas C. P. 98068, ZAC, Mexico [email protected] Abstract The recent measurements of the Hubble constant based on the standard ΛCDM cos- mology reveal an underlying disagreement between the early-Universe estimates and the late-time measurements. Moreover, as these measurements improve, the discrepancy not only persists but becomes even more significant and harder to ignore. The present situ- ation places the standard cosmology in jeopardy and provides a tantalizing hint that the problem results from some new physics beyond the ΛCDM model. It is shown that a non-conventional theory - the Milne model - which introduces a different evolution dynamics for the Universe, alleviates the Hubble tension significantly. Moreover, the model also averts some long-standing problems of the standard cosmology, for instance, the problems related with the cosmological constant, the horizon, the flat- ness, the Big Bang singularity, the age of the Universe and the non-conservation of energy. Keywords: Milne model; ΛCDM model; Hubble tension; SNe Ia observations; CMB observations. arXiv:2011.12146v1 [physics.gen-ph] 20 Nov 2020 1 Introduction The Hubble constant H0 is one of the most important parameters in cosmology which mea- sures the present rate of expansion of the Universe, and thereby estimates its size and age. This is done by assuming a cosmological model. However, the two values of H0 predicted by the standard ΛCDM model, one inferred from the measurements of the early Universe and the other from the late-time local measurements, seem to be in sever tension.
    [Show full text]
  • Title Spons Agency Bureau No Pub Date Contract Note
    DOCUMENT LIZSUME ED 071' C87 82 015 524 TITLE Project Musics Reader 2,Motion in the Heavens. .INSTITUTION Harvard Univ., Cambridge,Mass. Harvard Project _Physics. SPONS AGENCY Office of Education (DREW), Washington, D.C.,Bureau of Research. BUREAU NO BK-5-1038 PUB DATE 68 CONTRACT 08C-5-10-058 NOTE 233p.; Authorized InterimVersion EDRS PRICE MF -$0.65 HC-89.87 _DESCRIPTORS Astronomy; Instructional Materials;.*Motion; *Physics; Science, Fiction;. Science Materials; _Secondary Grades; *Secondary School Science; *Space; *Supplementary Reading Materials IDENTIFIER'S Harvard Project Physics ABSTRACT As a supplement to.Projpct Physics Unit 2, specially, selected articles are presented in this reader for student browsing. _Eight excerpts are given under headings:,the starry messenger, Newton_. And the principia, an appreciation of the earth, space the unconquerable, Is there intelligent life beyond the earth3,11 the life story of a galaxy, expansion of the universe, and Dyson sphere. Seven book passages. are included under. the, headings of the black cloud, roll call, a night at the observatory, Repler's celestial music, universal gravitation, a table of stars within twenty-two light years that could have habitable planets, and three poetic _fragments about astronomy. The remaining articles includea preface to the books of the ,revolutions, Kepler, Kepler on. Mars, laws of ..motion and proposition one,, garden of Epicurus, a search for life on earth at Kilometer resolution, the. boy who redeemed his father's _name, great comet of 1965, gravity experiments, unidentified flying objects, and negative mass. Illustrations for explanationpurposes . are provided. The work of Harvard. Project Physics has been .financially supported by: the Carnegie Corporation of New York, the Ford.
    [Show full text]
  • Remarkable Properties of the Eddington Number 137 and Electric Parameter 137.036 Excluding the Multiverse Hypothesis Francis M
    Remarkable Properties of the Eddington Number 137 and Electric Parameter 137.036 excluding the Multiverse Hypothesis Francis M. Sanchez February-May 2015 Abstract. Considering that the Large Eddington Number has correctly predicted the number of atoms in the Universe, the properties of the Eddington electric number 137 are studied. This number shows abnormal arithmetic properties, in liaison with the 5th harmonic number 137/60. It seems that Egyptians was aware of this, as the architecture of the Hypostyle Karnak room reveals, as well as the Ptolemaic approximation π ≈ 2 + 137/120, together with a specific mention in the Bible, and overhelming connexions with musical canonic numbers. The SO(32) characteristic superstring number 496, the third perfect number, connects directly with the three main interaction parameters, and is very close to the square root of the Higgs boson-electron mass ratio, so the Higgs boson discovery excludes the Multiverse, favoring rather a unique Cosmos being a finite computer using 137 and its extension 137.036 as calculation basis. The direct liaison between the mean value of the two main cosmic radiuses and the Bohr radius through the simplest harmonic series excludes any role of chance. Precise symmetric relations involving the Kotov non-Doppler period permit to propose precise (100 ppb) values for the weak and strong interaction constants, as well as G ≈ 6.675464346 × 10-11 kg-1 m3 s-2, at 2σ higher than the tabulated value.. This value is confirmed by a direct connection with the Superspeed ratio C/c ≈ 6.945480 × 1060. 1. Eddington and 137 Eddington has established [1] that, in reduced units, the square of the inverse electric charge must be 137.
    [Show full text]
  • Remarkables Properties of the Eddington Number 137 and Electric Parameter 137.036 Excluding the Multiverse Hypothesis Francis M
    Remarkables Properties of the Eddington Number 137 and Electric Parameter 137.036 excluding the Multiverse Hypothesis Francis M. Sanchez, February 2015 Abstract. Considering that the Large Eddington Number has correctly predicted the number of atoms in the Universe, the properties of the Eddington electric number 137 are studied. This number shows abnormal arithmetic properties, in liaison with canonic numbers of the string and superstring theories including overwhelming relations with musical canonic numbers. The liaison with the harmonic series is so tight that it seems that Egyptians was aware of them, as the architecture of the Hypostyle Karnak room reveals. The direct liaison between the mean value of two Universe radiuses and the Bohr radius through the simplest harmonic series excludes any role of chance. It is concluded that the Cosmos is a finite computer using 137 and its extension 137.036 as calculation basis. 1. The Large Eddington Number: the most astonishing prediction in Physics of all times Eddington believed he had identified an algebraic basis for fundamental physics, which he termed "E-numbers" (representing a certain group– a Clifford algebra). These in effect incorporated spacetime into a higher-dimensional structure. While his theory has long been neglected by the general physics community, similar algebraic notions underlie many modern attempts at a grand unified theory. Moreover, Eddington's emphasis on the values of the fundamental constants, and specifically upon dimensionless numbers derived from them, is nowadays a central concern of physics. In particular, he predicted a number of hydrogen atoms in the Universe [1] 136 x 2256, or equivalently the half of the total number of particles protons + electrons.
    [Show full text]
  • Max Planck Institute for the History of Science Aristotle And
    MAX-PLANCK-INSTITUT FÜR WISSENSCHAFTSGESCHICHTE Max Planck Institute for the History of Science 2012 PREPRINT 422 TOPOI – Towards a Historical Epistemology of Space Pietro Daniel Omodeo, Irina Tupikova Aristotle and Ptolemy on Geocentrism: Diverging Argumentative Strategies and Epistemologies TOPOI – TOWARDS A HISTORICAL EPISTEMOLOGY OF SPACE The TOPOI project cluster of excellence brings together researchers who investigate the formation and transformation of space and knowledge in ancient civilizations and their later developments. The present preprint series presents the work of members and fellows of the research group Historical Epistemology of Space which is part of the TOPOI cluster. The group is based on a cooperation between the Humboldt University and the Max Planck Institute for the History of Science in Berlin and commenced work in September 2008. Contents 1 Introduction 1 2 Aristotle 5 2.1 Aristotle’s confrontation with the cosmologies of his prede- cessors . 6 2.2 Aristotle’s presentation of his own views . 9 3 Ptolemy 15 3.1 The heavens move like a sphere . 16 3.2 The Earth, taken as a whole, is sensibly spherical . 24 3.3 The Earth is in the middle of the heavens . 24 3.4 The Earth has the ratio of a point to the heavens . 32 3.5 The Earth does not have any motion from place to place . 33 4 Conclusions and perspectives 37 Chapter 1 Introduction This paper aims at a comparison of the different argumentative strategies employed by Aristotle and Ptolemy in their approaches to geocentrism through an analysis of their discussion of the centrality of the Earth in De caelo II, 13-14 and Almagest, I, 3-7.
    [Show full text]
  • Structure Formation in a Dirac-Milne Universe: Comparison with the Standard Cosmological Model Giovanni Manfredi, Jean-Louis Rouet, Bruce N
    Structure formation in a Dirac-Milne universe: comparison with the standard cosmological model Giovanni Manfredi, Jean-Louis Rouet, Bruce N. Miller, Gabriel Chardin To cite this version: Giovanni Manfredi, Jean-Louis Rouet, Bruce N. Miller, Gabriel Chardin. Structure formation in a Dirac-Milne universe: comparison with the standard cosmological model. Physical Review D, Ameri- can Physical Society, 2020, 102 (10), pp.103518. 10.1103/PhysRevD.102.103518. hal-02999626 HAL Id: hal-02999626 https://hal.archives-ouvertes.fr/hal-02999626 Submitted on 28 Jun 2021 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Copyright PHYSICAL REVIEW D 102, 103518 (2020) Structure formation in a Dirac-Milne universe: Comparison with the standard cosmological model Giovanni Manfredi * Universit´e de Strasbourg, CNRS, Institut de Physique et Chimie des Mat´eriaux de Strasbourg, UMR 7504, F-67000 Strasbourg, France Jean-Louis Rouet Universit´ed’Orl´eans, CNRS/INSU, BRGM, ISTO, UMR7327, F-45071 Orl´eans, France Bruce N. Miller Department of Physics and Astronomy, Texas Christian University, Fort Worth, Texas 76129, USA † Gabriel Chardin Universit´e de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France (Received 15 July 2020; accepted 12 October 2020; published 13 November 2020) The presence of complex hierarchical gravitational structures is one of the main features of the observed universe.
    [Show full text]
  • (Owen Willans) Richardson
    O. W. (Owen Willans) Richardson: An Inventory of His Papers at the Harry Ransom Center Descriptive Summary Creator: Richardson, O. W. (Owen Willans), 1879-1959 Title: O. W. (Owen Willans) Richardson Papers Dates: 1898-1958 (bulk 1920-1940) Extent: 112 document boxes, 2 oversize boxes (49.04 linear feet), 1 oversize folder (osf), 5 galley folders (gf) Abstract: The papers of Sir O. W. (Owen Willans) Richardson, the Nobel Prize-winning British physicist who pioneered the field of thermionics, contain research materials and drafts of his writings, correspondence, as well as letters and writings from numerous distinguished fellow scientists. Call Number: MS-3522 Language: Primarily English; some works and correspondence written in French, German, or Italian . Note: The Ransom Center gratefully acknowledges the assistance of the Center for History of Physics, American Institute of Physics, which provided funds to support the processing and cataloging of this collection. Access: Open for research Administrative Information Additional The Richardson Papers were microfilmed and are available on 76 Physical Format reels. Each item has a unique identifying number (W-xxxx, L-xxxx, Available: R-xxxx, or M-xxxx) that corresponds to the microfilm. This number was recorded on the file folders housing the papers and can also be found on catalog slips present with each item. Acquisition: Purchase, 1961 (R43, R44) and Gift, 2005 Processed by: Tessa Klink and Joan Sibley, 2014 Repository: The University of Texas at Austin, Harry Ransom Center Richardson, O. W. (Owen Willans), 1879-1959 MS-3522 2 Richardson, O. W. (Owen Willans), 1879-1959 MS-3522 Biographical Sketch The English physicist Owen Willans Richardson, who pioneered the field of thermionics, was also known for his work on photoelectricity, spectroscopy, ultraviolet and X-ray radiation, the electron theory, and quantum theory.
    [Show full text]
  • Epistemic Beliefs and Coherence of Justification in Modern Cosmology
    Journal of Siberian Federal University. Humanities & Social Sciences 7 (2013 6) 957-1001 ~ ~ ~ УДК 24-17 The Universe as a Construct: Epistemic Beliefs and Coherence of Justification in Modern Cosmology Alexei V. Nesteruk* University of Portsmouth, Lion Gate Building, PORTSMOUTH, PO1 3HF, UK Received 12.03.2013, received in revised form 06.06.2013, accepted 19.06.2013 In this paper we continue to study the epistemic nature of cosmological claims, in particular the status of the notion of the universe as a whole. It is demonstrated that this notion has a status of a construct with some epistemic links with empirical reality. However, it is argued that the effective methodology of contemporary mathematical cosmology related to the modelling of the very early stages of the evolutionary universes, consists not in the principle of correspondence of its theoretical constructs with empirical reality, but in the coherence of epistemic justification which relates to belief-like commitments of the community of cosmologists. As a case study, the inflationary model of the early universe is analysed and it is demonstrated that the coherence of justification leads to the transcendental problems in the style of Kant. Keywords: beliefs, cosmology, coherence, correspondence principle, epistemology, extrapolation, universe. The real world is not a thing founded in itself, that can in a significant manner be established as an independent existence. Recognition of the world as it comes from God cannot … be achieved by cognitions crystallising into separate judgements that have an independent meaning and assert definite facts. It can be gained only by symbolic construction. Hermann Weyl, Mind and Nature, p.
    [Show full text]
  • The Legacy of S Chandrasekhar (1910–1995)
    PRAMANA c Indian Academy of Sciences Vol. 77, No. 1 — journal of July 2011 physics pp. 213–226 The legacy of S Chandrasekhar (1910–1995) KAMESHWAR C WALI Physics Department, Syracuse University, Syracuse, NY 13244-1130, USA E-mail: [email protected] Abstract. Subrahmanyan Chandrasekhar, known simply as Chandra in the scientific world, is one of the foremost scientists of the 20th century. In celebrating his birth centenary, I present a bio- graphical portrait of an extraordinary, but a highly private individual unknown to the world at large. Drawing upon his own “A Scientific Autobiography,” I reflect upon his legacy as a scientist and a great human being. Keywords. White dwarfs; Chandrasekhar limit; relativistic degeneracy. PACS Nos 01.65.+g; 01.60.+q; 97; 97.10.Cv 1. Introductory remarks: Man on the ladder When I stepped into Chandra’s office for the first time in 1979, I was immediately intrigued by a photograph that faced him from the wall opposite his desk. As I stood looking at it, Chandra told me the following story. He had first seen the photograph on the cover of a New York Times Magazine and had written to the magazine for a copy (figure 1). He was referred to the artist, Piero Borello. Borello replied that Chandra could have a copy, even the original, but only if he cared to explain why he wanted it. Chandra responded: “What impressed me about your picture was the extremely striking manner in which you visually portray one’s inner feelings towards one’s accomplishments: one is half-way up the ladder, but the few glimmerings of structure which one sees and to which one aspires are totally inaccessible, even if one were to climb to the top of the ladder.
    [Show full text]