General Relativity Conflict and Rivalries

Total Page:16

File Type:pdf, Size:1020Kb

General Relativity Conflict and Rivalries General Relativity Conflict and Rivalries General Relativity Conflict and Rivalries: Einstein's Polemics with Physicists By Galina Weinstein General Relativity Conflict and Rivalries: Einstein's Polemics with Physicists By Galina Weinstein This book first published 2015 Cambridge Scholars Publishing Lady Stephenson Library, Newcastle upon Tyne, NE6 2PA, UK British Library Cataloguing in Publication Data A catalogue record for this book is available from the British Library Copyright © 2015 by Galina Weinstein 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): 1-4438-8362-X ISBN (13): 978-1-4438-8362-7 “When I accompanied him [Einstein] home the first day we met, he told me something that I heard from him many times later: ‘In Princeton they regard me as an old fool.’ (‘Hier in Princeton betrachten sie mich als einen alten Trottel’.) […] Before he was thirty-five, Einstein had made the four great discoveries of his life. In order of increasing importance they are: the theory of Brownian motion; the theory of the photoelectric effect; the special theory of relativity; the general theory of relativity. Very few people in the history of science have done half as much. […] For years he looked for a theory which would embrace gravitational, electromagnetic, and quantum phenomena. […] Einstein pursued it relentlessly through ideas which he changed repeatedly and down avenues that led nowhere. The very distinguished professors in Princeton did not understand that Einstein’s mistakes were more important than their correct results. Einstein, during my stay in Princeton, was regarded by most of the professors there more like a historic relic than as an active scientist”. Leopold Infeld, “As I see It”, Bulletin of the Atomic Scientists, 1965, 9. CONTENTS Preface ........................................................................................................ ix Chapter One ................................................................................................. 2 From Zurich to Berlin 1. Einstein and Heinrich Zangger .......................................................... 2 2. From Zurich to Prague ....................................................................... 3 3. Back to Zurich ................................................................................... 9 4. From Zurich to Berlin ...................................................................... 12 Chapter Two .............................................................................................. 28 General Relativity between 1912 and 1916 1. The Equivalence Principle .............................................................. 28 2. Einstein's 1912 Polemic with Max Abraham: Static Gravitational Field.......................................................................... 37 3. Einstein's 1912 Polemic with Gunnar Nordström: Static Gravitational Field.......................................................................... 47 4. Einstein's 1912-1913 Collaboration with Marcel Grossmann: Zurich Notebook to Entwurf Theory .............................................. 50 5. Einstein's 1913-1914 Polemic with Nordström: Scalar Theory versus Tensor Theory ..................................................................... 84 6. Einstein's Polemic with Gustav Mie: Matter and Gravitation ...... 101 7. 1914 Collaboration with Grossmann and Final Entwurf Theory ............................................................................ 105 8. Einstein's Polemic with Tullio Levi-Civita on the Entwurf Theory ............................................................................ 117 9. Einstein's 1915 Competition with David Hilbert and General Relativity ...................................................................................... 131 10. Einstein Answers Paul Ehrenfest's Queries: 1916 General Relativity ............................................................... 172 11. The Third Prediction of General Relativity: Gravitational RedShift .................................................................. 182 12. Erich Kretschmann's Critiques of Einstein's Point Coincidence Argument ................................................................. 192 13. Einstein and Mach's Ideas ............................................................ 206 14. Einstein's Reaction to Karl Schwarzschild's Solution .................. 211 viii Contents 15. The Fourth Classic Test of General Relativity: Light Delay ........ 239 Chapter Three .......................................................................................... 242 General Relativity after 1916 1. Einstein's 1916 Polemic with Willem de Sitter, Levi-Civita and Nordström on Gravitational Waves ....................................... 242 2. Einstein's Polemic with de Sitter: Matter World and Empty World ......................................................................... 267 3. Bending of Light and Gravitational Lens: Einstein and Arthur Stanley Eddington ...................................................... 285 4. Einstein's Interaction with Hermann Weyl and the Cosmological Constant ................................................................ 306 5. Einstein's 1920 Matter World, Mach's Ether and the Dark Matter ...................................................................... 322 6. Einstein's 1920 Polemic with Eddington on de Sitter's World ..... 327 7. Einstein's Reaction to the Aleksandr Friedmann Solution ........... 331 8. Einstein's Reaction to the Georges Lemaître Solution ................. 334 9. Edwin Hubble's Experimental Results ......................................... 337 10. The Lemaître-Eddington Model ................................................... 341 11. Einstein and the Matter World: the Steady State Solution ........... 350 12. Einstein's Collaboration with de Sitter ......................................... 354 13. Einstein's Reaction to Lemaître's Big Bang Model ...................... 359 14. Einstein's Interaction with George Gamow: Cosmological Constant is the Biggest Blunder ............................ 366 15. Einstein, Gödel and Backward Time Travel ................................ 373 References ............................................................................................... 382 Index ........................................................................................................ 405 PREFACE We can pose many thought-provoking questions in regards to Einstein's achievements: Was the theory of general relativity the invention of Albert Einstein, who would close himself off in an office with his violin, pipe and a pile of papers? Or, was it a culmination of Einstein's multilateral interactions with other scientists? And, to what extent did Einstein's loyal friend from school, Marcel Grossmann, contribute to the mathematics of the general theory of relativity? Other questions focus on the general topic of how scientists debate and, in the process, modify their ideas. Was the theory of general relativity a physical-conceptual theory containing innovations in a synthesis developed from his interactions with friends and colleagues? Was the theory of general relativity a product of debates and conflicts between Einstein and other scientists? In this book I present an approach that focuses on the work of an individual scientist, Albert Einstein, and his interaction with and response to many eminent and non-eminent scientists. According to this approach, the ongoing discussions between Einstein and other scientists have all contributed to the edifice of general relativity and relativistic cosmology. Mara Beller argues that, the scientists, with whom Einstein implicitly or explicitly interacted, form a complicated web of collaboration (Beller 1999). I have analysed the works of those scientists who were, in any way, connected to the development of the general theory of relativity and relativistic cosmology, focusing on their implicit and explicit responses to Einstein's work. This analysis has uncovered latent undercurrents, which could not have been exposed by means of tracking the intellectual pathway of Einstein to his general theory of relativity. The new interconnections and meanings disclosed have revealed the central figures who influenced Einstein during his development of the general theory of relativity and in the construction of the edifice of relativistic cosmology; this includes the themes, outlooks, suppositions and contributions of these scientists as opposed to Einstein's Weltanschauung (worldview). x Preface Furthermore, current history presupposes that all the efforts invested by physicists like Max Abraham, Gunnar Nordström, Gustav Mie and David Hilbert, which presented differing outlooks and discussions revolving around the theory of gravitation, were relegated to the background. Thus, those works that did not embrace Einstein's overall conceptual concerns (these primarily included the heuristic equivalence principle and "Mach's ideas") were rejected, and authors focused on Einstein's prodigious scientific achievements. I emphasise the limits of the simplistic hero worship narrative, and the associated problems tracing Einstein's intellectual pathway to the general theory of relativity. I demonstrate in this book that one should not discard Einstein's response to the works
Recommended publications
  • Ricci, Levi-Civita, and the Birth of General Relativity Reviewed by David E
    BOOK REVIEW Einstein’s Italian Mathematicians: Ricci, Levi-Civita, and the Birth of General Relativity Reviewed by David E. Rowe Einstein’s Italian modern Italy. Nor does the author shy away from topics Mathematicians: like how Ricci developed his absolute differential calculus Ricci, Levi-Civita, and the as a generalization of E. B. Christoffel’s (1829–1900) work Birth of General Relativity on quadratic differential forms or why it served as a key By Judith R. Goodstein tool for Einstein in his efforts to generalize the special theory of relativity in order to incorporate gravitation. In This delightful little book re- like manner, she describes how Levi-Civita was able to sulted from the author’s long- give a clear geometric interpretation of curvature effects standing enchantment with Tul- in Einstein’s theory by appealing to his concept of parallel lio Levi-Civita (1873–1941), his displacement of vectors (see below). For these and other mentor Gregorio Ricci Curbastro topics, Goodstein draws on and cites a great deal of the (1853–1925), and the special AMS, 2018, 211 pp. 211 AMS, 2018, vast secondary literature produced in recent decades by the world that these and other Ital- “Einstein industry,” in particular the ongoing project that ian mathematicians occupied and helped to shape. The has produced the first 15 volumes of The Collected Papers importance of their work for Einstein’s general theory of of Albert Einstein [CPAE 1–15, 1987–2018]. relativity is one of the more celebrated topics in the history Her account proceeds in three parts spread out over of modern mathematical physics; this is told, for example, twelve chapters, the first seven of which cover episodes in [Pais 1982], the standard biography of Einstein.
    [Show full text]
  • Philosophical Rhetoric in Early Quantum Mechanics, 1925-1927
    b1043_Chapter-2.4.qxd 1/27/2011 7:30 PM Page 319 b1043 Quantum Mechanics and Weimar Culture FA 319 Philosophical Rhetoric in Early Quantum Mechanics 1925–27: High Principles, Cultural Values and Professional Anxieties Alexei Kojevnikov* ‘I look on most general reasoning in science as [an] opportunistic (success- or unsuccessful) relationship between conceptions more or less defined by other conception[s] and helping us to overlook [danicism for “survey”] things.’ Niels Bohr (1919)1 This paper considers the role played by philosophical conceptions in the process of the development of quantum mechanics, 1925–1927, and analyses stances taken by key participants on four main issues of the controversy (Anschaulichkeit, quantum discontinuity, the wave-particle dilemma and causality). Social and cultural values and anxieties at the time of general crisis, as identified by Paul Forman, strongly affected the language of the debate. At the same time, individual philosophical positions presented as strongly-held principles were in fact flexible and sometimes reversible to almost their opposites. One can understand the dynamics of rhetorical shifts and changing strategies, if one considers interpretational debates as a way * Department of History, University of British Columbia, 1873 East Mall, Vancouver, British Columbia, Canada V6T 1Z1; [email protected]. The following abbreviations are used: AHQP, Archive for History of Quantum Physics, NBA, Copenhagen; AP, Annalen der Physik; HSPS, Historical Studies in the Physical Sciences; NBA, Niels Bohr Archive, Niels Bohr Institute, Copenhagen; NW, Die Naturwissenschaften; PWB, Wolfgang Pauli, Wissenschaftlicher Briefwechsel mit Bohr, Einstein, Heisenberg a.o., Band I: 1919–1929, ed. A. Hermann, K.V.
    [Show full text]
  • Abraham-Solution to Schwarzschild Metric Implies That CERN Miniblack Holes Pose a Planetary Risk
    Abraham-Solution to Schwarzschild Metric Implies That CERN Miniblack Holes Pose a Planetary Risk O.E. Rössler Division of Theoretical Chemistry, University of Tübingen, 72076 F.R.G. Abstract A recent mathematical re-interpretation of the Schwarzschild solution to the Einstein equations implies global constancy of the speed of light c in fulfilment of a 1912 proposal of Max Abraham. As a consequence, the horizon lies at the end of an infinitely long funnel in spacetime. Hence black holes lack evaporation and charge. Both features affect the behavior of miniblack holes as are expected to be produced soon at the Large Hadron Collider at CERN. The implied nonlinearity enables the “quasar-scaling conjecture.“ The latter implies that an earthbound minihole turns into a planet-eating attractor much earlier than previously calculated – not after millions of years of linear growth but after months of nonlinear growth. A way to turn the almost disaster into a planetary bonus is suggested. (September 27, 2007) “Mont blanc and black holes: a winter fairy-tale.“ What is being referred to is the greatest and most expensive and potentially most important experiment of history: to create miniblack holes [1]. The hoped-for miniholes are only 10–32 cm large – as small compared to an atom (10–8 cm) as the latter is to the whole solar system (1016 cm) – and are expected to “evaporate“ within less than a picosecond while leaving behind a much hoped-for “signature“ of secondary particles [1]. The first (and then one per second and a million per year) miniblack hole is expected to be produced in 2008 at the Large Hadron Collider of CERN near Geneva on the lake not far from the white mountain.
    [Show full text]
  • Albert Einstein
    THE COLLECTED PAPERS OF Albert Einstein VOLUME 15 THE BERLIN YEARS: WRITINGS & CORRESPONDENCE JUNE 1925–MAY 1927 Diana Kormos Buchwald, József Illy, A. J. Kox, Dennis Lehmkuhl, Ze’ev Rosenkranz, and Jennifer Nollar James EDITORS Anthony Duncan, Marco Giovanelli, Michel Janssen, Daniel J. Kennefick, and Issachar Unna ASSOCIATE & CONTRIBUTING EDITORS Emily de Araújo, Rudy Hirschmann, Nurit Lifshitz, and Barbara Wolff ASSISTANT EDITORS Princeton University Press 2018 Copyright © 2018 by The Hebrew University of Jerusalem Published by Princeton University Press, 41 William Street, Princeton, New Jersey 08540 In the United Kingdom: Princeton University Press, 6 Oxford Street, Woodstock, Oxfordshire OX20 1TW press.princeton.edu All Rights Reserved LIBRARY OF CONGRESS CATALOGING-IN-PUBLICATION DATA (Revised for volume 15) Einstein, Albert, 1879–1955. The collected papers of Albert Einstein. German, English, and French. Includes bibliographies and indexes. Contents: v. 1. The early years, 1879–1902 / John Stachel, editor — v. 2. The Swiss years, writings, 1900–1909 — — v. 15. The Berlin years, writings and correspondence, June 1925–May 1927 / Diana Kormos Buchwald... [et al.], editors. QC16.E5A2 1987 530 86-43132 ISBN 0-691-08407-6 (v.1) ISBN 978-0-691-17881-3 (v. 15) This book has been composed in Times. The publisher would like to acknowledge the editors of this volume for providing the camera-ready copy from which this book was printed. Princeton University Press books are printed on acid-free paper and meet the guidelines for permanence and durability of the Committee on Production Guidelines for Book Longevity of the Council on Library Resources. Printed in the United States of America 13579108642 INTRODUCTION TO VOLUME 15 The present volume covers a thrilling two-year period in twentieth-century physics, for during this time matrix mechanics—developed by Werner Heisenberg, Max Born, and Pascual Jordan—and wave mechanics, developed by Erwin Schrödinger, supplanted the earlier quantum theory.
    [Show full text]
  • An Analysis of Gravitational Redshift from Rotating Body
    An analysis of gravitational redshift from rotating body Anuj Kumar Dubey∗ and A K Sen† Department of Physics, Assam University, Silchar-788011, Assam, India. (Dated: July 29, 2021) Gravitational redshift is generally calculated without considering the rotation of a body. Neglect- ing the rotation, the geometry of space time can be described by using the spherically symmetric Schwarzschild geometry. Rotation has great effect on general relativity, which gives new challenges on gravitational redshift. When rotation is taken into consideration spherical symmetry is lost and off diagonal terms appear in the metric. The geometry of space time can be then described by using the solutions of Kerr family. In the present paper we discuss the gravitational redshift for rotating body by using Kerr metric. The numerical calculations has been done under Newtonian approximation of angular momentum. It has been found that the value of gravitational redshift is influenced by the direction of spin of central body and also on the position (latitude) on the central body at which the photon is emitted. The variation of gravitational redshift from equatorial to non - equatorial region has been calculated and its implications are discussed in detail. I. INTRODUCTION from principle of equivalence. Snider in 1972 has mea- sured the redshift of the solar potassium absorption line General relativity is not only relativistic theory of grav- at 7699 A˚ by using an atomic - beam resonance - scat- itation proposed by Einstein, but it is the simplest theory tering technique [5]. Krisher et al. in 1993 had measured that is consistent with experimental data. Predictions of the gravitational redshift of Sun [6].
    [Show full text]
  • Einstein, Nordström and the Early Demise of Scalar, Lorentz Covariant Theories of Gravitation
    JOHN D. NORTON EINSTEIN, NORDSTRÖM AND THE EARLY DEMISE OF SCALAR, LORENTZ COVARIANT THEORIES OF GRAVITATION 1. INTRODUCTION The advent of the special theory of relativity in 1905 brought many problems for the physics community. One, it seemed, would not be a great source of trouble. It was the problem of reconciling Newtonian gravitation theory with the new theory of space and time. Indeed it seemed that Newtonian theory could be rendered compatible with special relativity by any number of small modifications, each of which would be unlikely to lead to any significant deviations from the empirically testable conse- quences of Newtonian theory.1 Einstein’s response to this problem is now legend. He decided almost immediately to abandon the search for a Lorentz covariant gravitation theory, for he had failed to construct such a theory that was compatible with the equality of inertial and gravitational mass. Positing what he later called the principle of equivalence, he decided that gravitation theory held the key to repairing what he perceived as the defect of the special theory of relativity—its relativity principle failed to apply to accelerated motion. He advanced a novel gravitation theory in which the gravitational potential was the now variable speed of light and in which special relativity held only as a limiting case. It is almost impossible for modern readers to view this story with their vision unclouded by the knowledge that Einstein’s fantastic 1907 speculations would lead to his greatest scientific success, the general theory of relativity. Yet, as we shall see, in 1 In the historical period under consideration, there was no single label for a gravitation theory compat- ible with special relativity.
    [Show full text]
  • Simply-Riemann-1588263529. Print
    Simply Riemann Simply Riemann JEREMY GRAY SIMPLY CHARLY NEW YORK Copyright © 2020 by Jeremy Gray Cover Illustration by José Ramos Cover Design by Scarlett Rugers All rights reserved. No part of this publication may be reproduced, distributed, or transmitted in any form or by any means, including photocopying, recording, or other electronic or mechanical methods, without the prior written permission of the publisher, except in the case of brief quotations embodied in critical reviews and certain other noncommercial uses permitted by copyright law. For permission requests, write to the publisher at the address below. [email protected] ISBN: 978-1-943657-21-6 Brought to you by http://simplycharly.com Contents Praise for Simply Riemann vii Other Great Lives x Series Editor's Foreword xi Preface xii Introduction 1 1. Riemann's life and times 7 2. Geometry 41 3. Complex functions 64 4. Primes and the zeta function 87 5. Minimal surfaces 97 6. Real functions 108 7. And another thing . 124 8. Riemann's Legacy 126 References 143 Suggested Reading 150 About the Author 152 A Word from the Publisher 153 Praise for Simply Riemann “Jeremy Gray is one of the world’s leading historians of mathematics, and an accomplished author of popular science. In Simply Riemann he combines both talents to give us clear and accessible insights into the astonishing discoveries of Bernhard Riemann—a brilliant but enigmatic mathematician who laid the foundations for several major areas of today’s mathematics, and for Albert Einstein’s General Theory of Relativity.Readable, organized—and simple. Highly recommended.” —Ian Stewart, Emeritus Professor of Mathematics at Warwick University and author of Significant Figures “Very few mathematicians have exercised an influence on the later development of their science comparable to Riemann’s whose work reshaped whole fields and created new ones.
    [Show full text]
  • Gravitational Redshift/Blueshift of Light Emitted by Geodesic
    Eur. Phys. J. C (2021) 81:147 https://doi.org/10.1140/epjc/s10052-021-08911-5 Regular Article - Theoretical Physics Gravitational redshift/blueshift of light emitted by geodesic test particles, frame-dragging and pericentre-shift effects, in the Kerr–Newman–de Sitter and Kerr–Newman black hole geometries G. V. Kraniotisa Section of Theoretical Physics, Physics Department, University of Ioannina, 451 10 Ioannina, Greece Received: 22 January 2020 / Accepted: 22 January 2021 / Published online: 11 February 2021 © The Author(s) 2021 Abstract We investigate the redshift and blueshift of light 1 Introduction emitted by timelike geodesic particles in orbits around a Kerr–Newman–(anti) de Sitter (KN(a)dS) black hole. Specif- General relativity (GR) [1] has triumphed all experimental ically we compute the redshift and blueshift of photons that tests so far which cover a wide range of field strengths and are emitted by geodesic massive particles and travel along physical scales that include: those in large scale cosmology null geodesics towards a distant observer-located at a finite [2–4], the prediction of solar system effects like the perihe- distance from the KN(a)dS black hole. For this purpose lion precession of Mercury with a very high precision [1,5], we use the killing-vector formalism and the associated first the recent discovery of gravitational waves in Nature [6–10], integrals-constants of motion. We consider in detail stable as well as the observation of the shadow of the M87 black timelike equatorial circular orbits of stars and express their hole [11], see also [12]. corresponding redshift/blueshift in terms of the metric physi- The orbits of short period stars in the central arcsecond cal black hole parameters (angular momentum per unit mass, (S-stars) of the Milky Way Galaxy provide the best current mass, electric charge and the cosmological constant) and the evidence for the existence of supermassive black holes, in orbital radii of both the emitter star and the distant observer.
    [Show full text]
  • Shs-17-2018-14.Pdf
    Science beyond borders Nobukata Nagasawa ORCID 0000-0002-9658-7680 Emeritus Professor of University of Tokyo [email protected] On social and psychological aspects of a negligible reception of Natanson’s article of 1911 in the early history of quantum statistics Abstract Possible reasons are studied why Ladislas (Władysław) Natanson’s paper on the statistical theory of radiation, published in 1911 both in English and in the German translation, was not cited properly in the early history of quantum statistics by outstanding scientists, such as Arnold Sommerfeld, Paul Ehrenfest, Satyendra Nath Bose and Albert Einstein. The social and psychological aspects are discussed as back- ground to many so far discussions on the academic evaluation of his theory. In order to avoid in the future such Natansonian cases of very limited reception of valuable scientific works, it is pro- posed to introduce a digital tag in which all the information of PUBLICATION e-ISSN 2543-702X INFO ISSN 2451-3202 DIAMOND OPEN ACCESS CITATION Nagasawa, Nobukata 2018: On social and psychological aspects of a negligible reception of Natanson’s article of 1911 in the early history of quantum statistics. Studia Historiae Scientiarum 17, pp. 391–419. Available online: https://doi.org/10.4467/2543702XSHS.18.014.9334. ARCHIVE RECEIVED: 13.06.2017 LICENSE POLICY ACCEPTED: 12.09.2018 Green SHERPA / PUBLISHED ONLINE: 12.12.2018 RoMEO Colour WWW http://www.ejournals.eu/sj/index.php/SHS/; http://pau.krakow.pl/Studia-Historiae-Scientiarum/ Nobukata Nagasawa On social and psychological aspects of a negligible reception... relevant papers published so far should be automatically accu- mulated and updated.
    [Show full text]
  • A Hypothesis About the Predominantly Gravitational Nature of Redshift in the Electromagnetic Spectra of Space Objects Stepan G
    A Hypothesis about the Predominantly Gravitational Nature of Redshift in the Electromagnetic Spectra of Space Objects Stepan G. Tiguntsev Irkutsk National Research Technical University 83 Lermontov St., Irkutsk, 664074, Russia [email protected] Abstract. The study theoretically substantiates the relationship between the redshift in the electromagnetic spectrum of space objects and their gravity and demonstrates it with computational experiments. Redshift, in this case, is a consequence of a decrease in the speed of the photons emitted from the surface of objects, which is caused by the gravity of these objects. The decline in the speed of photons due to the gravity of space gravitating object (GO) is defined as ΔC = C-C ', where: C' is the photon speed changed by the time the receiver records it. Then, at a change in the photon speed between a stationary source and a receiver, the redshift factor is determined as Z = (C-C ')/C'. Computational experiments determined the gravitational redshift of the Earth, the Sun, a neutron star, and a quasar. Graph of the relationship between the redshift and the ratio of sizes to the mass of any space GOs was obtained. The findings indicate that the distance to space objects does not depend on the redshift of these objects. Keywords: redshift, computational experiment, space gravitating object, photon, radiation source, and receiver. 1. Introduction In the electromagnetic spectrum of space objects, redshift is assigned a significant role in creating a physical picture of the Universe. Redshift is observed in almost all space objects (stars, galaxies, quasars, and others). As a consequence of the Doppler effect, redshift indicates the movement of almost all space objects from an observer on the Earth [1].
    [Show full text]
  • Math, Physics, and Calabi–Yau Manifolds
    Math, Physics, and Calabi–Yau Manifolds Shing-Tung Yau Harvard University October 2011 Introduction I’d like to talk about how mathematics and physics can come together to the benefit of both fields, particularly in the case of Calabi-Yau spaces and string theory. This happens to be the subject of the new book I coauthored, THE SHAPE OF INNER SPACE It also tells some of my own story and a bit of the history of geometry as well. 2 In that spirit, I’m going to back up and talk about my personal introduction to geometry and how I ended up spending much of my career working at the interface between math and physics. Along the way, I hope to give people a sense of how mathematicians think and approach the world. I also want people to realize that mathematics does not have to be a wholly abstract discipline, disconnected from everyday phenomena, but is instead crucial to our understanding of the physical world. 3 There are several major contributions of mathematicians to fundamental physics in 20th century: 1. Poincar´eand Minkowski contribution to special relativity. (The book of Pais on the biography of Einstein explained this clearly.) 2. Contributions of Grossmann and Hilbert to general relativity: Marcel Grossmann (1878-1936) was a classmate with Einstein from 1898 to 1900. he was professor of geometry at ETH, Switzerland at 1907. In 1912, Einstein came to ETH to be professor where they started to work together. Grossmann suggested tensor calculus, as was proposed by Elwin Bruno Christoffel in 1868 (Crelle journal) and developed by Gregorio Ricci-Curbastro and Tullio Levi-Civita (1901).
    [Show full text]
  • Marcel Grossmann Awards
    MG15 MARCEL GROSSMANN AWARDS ROME 2018 ICRANet and ICRA MG XV MARCEL GROSSMANN AWARDS ROME 2018 and TEST The 15th Marcel Grossmann Meeting – MG XV 2nd July 2018, Rome (Italy) Aula Magna – University “Sapienza” of Rome Institutional Awards Goes to: PLANCK SCIENTIFIC COLLABORATION (ESA) “for obtaining important constraints on the models of inflationary stage of the Universe and level of primordial non-Gaussianity; measuring with unprecedented sensitivity gravitational lensing of Cosmic Microwave Background fluctuations by large-scale structure of the Universe and corresponding B- polarization of CMB, the imprint on the CMB of hot gas in galaxy clusters; getting unique information about the time of reionization of our Universe and distribution and properties of the dust and magnetic fields in our Galaxy” - presented to Jean-Loup Puget, the Principal Investigator of the High Frequency Instrument (HFI) HANSEN EXPERIMENTAL PHYSICS LABORATORY AT STANFORD UNIVERSITY “to HEPL for having developed interdepartmental activities at Stanford University at the frontier of fundamental physics, astrophysics and technology” - presented to Research Professor Leo Hollberg, HEPL Assistant Director Individual Awards Goes to LYMAN PAGE “for his collaboration with David Wilkinson in realizing the NASA Explorer WMAP mission and as founding director of the Atacama Cosmology Telescope” Goes to RASHID ALIEVICH SUNYAEV “for the development of theoretical tools in the scrutinising, through the CMB, of the first observable electromagnetic appearance of our Universe” Goes to SHING-TUNG YAU “for the proof of the positivity of total mass in the theory of general relativity and perfecting as well the concept of quasi-local mass, for his proof of the Calabi conjecture, for his continuous inspiring role in the study of black holes physics” Each recipient is presented with a silver casting of the TEST sculpture by the artist A.
    [Show full text]