The Scientific Content of the Letters Is Remarkably Rich, Touching on The
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Carl Runge 1 Carl Runge
Carl Runge 1 Carl Runge Carl David Tolmé Runge (30. august 1856 Bremen – 3. jaanuar 1927 Göttingen) oli saksa matemaatik. Ta pani aluse tänapäeva praktilisele matemaatikale kui õpetusele matemaatilistest meetoditest loodusteaduslike ja tehniliste ülesannete arvutuslikul lahendamisel. Ta sündis jõuka kaupmees Julius Runge ja inglanna Fanny Tolmé pojana. Oma esimesed aastad veetis ta Havannas, kus tema isa haldas Taani konsulaati. Kodune keel oli eeskätt inglise keel. Carl Runge ja tema vennad omandasid Briti kombed ja vaated, eriti spordi, aususe, õigluse ja enesekindluse kohta. Hiljem kolis perekond Bremenisse, kus Carli isa 1864 suri. Aastal 1875 lõpetas ta Bremenis gümnaasiumi. Seejärel saatis ta oma ema pool aastat kultuurireisil Itaalias. Siis läks ta Münchenisse, kus ta algul õppis kirjandusteadust ja filosoofias kuid otsustas pärast kuuenädalast õppimist 1876 matemaatika ja füüsika kasuks. Ta õppis koos Max Planckiga, kellega ta sõbrunes. Müncheni ülikoolis oli ta populaarne uisutaja. Aastal 1877 jätkas ta (koos Planckiga) oma õpinguid Berliinis, mis oli Saksamaa matemaatika keskus ja kus teda mõjutasid eriti Leopold Carl Runge Kronecker ja Karl Weierstraß. Viimase loengute kuulamine kallutas ta keskenduma füüsika asemel puhtale matemaatikale. Aastal 1880 promoveerus ta Weierstraßi ning Ernst Eduard Kummeri juures tööga "Über die Krümmung, Torsion und geodätische Krümmung der auf einer Fläche gezogenen Curven". Tol ajal tuli doktorieksamil püstitada kolm teesi ja neid kaitsta. Üks Runge teesidest oli: "Matemaatilise distsipliini väärtust tuleb hinnata tema rakendatavuse järgi empiirilistele teadustele." Ta habiliteerus 1883. Runge tegeles algul puhta matemaatikaga. Kronecker oli teda innustanud tegelema arvuteooriaga ja Weierstraß funktsiooniteooriaga. Funktsiooniteoorias uuris ta holomorfsete funktsioonide aproksimeeritavust ratsionaalsete funktsioonidega, rajades Runge teooria. Berliini ajal sai ta oma tulevaselt äialt (kelle perekonnas ta oli sagedane külaline) teada Balmeri seeriast. -
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. -
Herbert Busemann (1905--1994)
HERBERT BUSEMANN (1905–1994) A BIOGRAPHY FOR HIS SELECTED WORKS EDITION ATHANASE PAPADOPOULOS Herbert Busemann1 was born in Berlin on May 12, 1905 and he died in Santa Ynez, County of Santa Barbara (California) on February 3, 1994, where he used to live. His first paper was published in 1930, and his last one in 1993. He wrote six books, two of which were translated into Russian in the 1960s. Initially, Busemann was not destined for a mathematical career. His father was a very successful businessman who wanted his son to be- come, like him, a businessman. Thus, the young Herbert, after high school (in Frankfurt and Essen), spent two and a half years in business. Several years later, Busemann recalls that he always wanted to study mathematics and describes this period as “two and a half lost years of my life.” Busemann started university in 1925, at the age of 20. Between the years 1925 and 1930, he studied in Munich (one semester in the aca- demic year 1925/26), Paris (the academic year 1927/28) and G¨ottingen (one semester in 1925/26, and the years 1928/1930). He also made two 1Most of the information about Busemann is extracted from the following sources: (1) An interview with Constance Reid, presumably made on April 22, 1973 and kept at the library of the G¨ottingen University. (2) Other documents held at the G¨ottingen University Library, published in Vol- ume II of the present edition of Busemann’s Selected Works. (3) Busemann’s correspondence with Richard Courant which is kept at the Archives of New York University. -
Voigt Transformations in Retrospect: Missed Opportunities?
Voigt transformations in retrospect: missed opportunities? Olga Chashchina Ecole´ Polytechnique, Palaiseau, France∗ Natalya Dudisheva Novosibirsk State University, 630 090, Novosibirsk, Russia† Zurab K. Silagadze Novosibirsk State University and Budker Institute of Nuclear Physics, 630 090, Novosibirsk, Russia.‡ The teaching of modern physics often uses the history of physics as a didactic tool. However, as in this process the history of physics is not something studied but used, there is a danger that the history itself will be distorted in, as Butterfield calls it, a “Whiggish” way, when the present becomes the measure of the past. It is not surprising that reading today a paper written more than a hundred years ago, we can extract much more of it than was actually thought or dreamed by the author himself. We demonstrate this Whiggish approach on the example of Woldemar Voigt’s 1887 paper. From the modern perspective, it may appear that this paper opens a way to both the special relativity and to its anisotropic Finslerian generalization which came into the focus only recently, in relation with the Cohen and Glashow’s very special relativity proposal. With a little imagination, one can connect Voigt’s paper to the notorious Einstein-Poincar´epri- ority dispute, which we believe is a Whiggish late time artifact. We use the related historical circumstances to give a broader view on special relativity, than it is usually anticipated. PACS numbers: 03.30.+p; 1.65.+g Keywords: Special relativity, Very special relativity, Voigt transformations, Einstein-Poincar´epriority dispute I. INTRODUCTION Sometimes Woldemar Voigt, a German physicist, is considered as “Relativity’s forgotten figure” [1]. -
Theory and Experiment in the Quantum-Relativity Revolution
Theory and Experiment in the Quantum-Relativity Revolution expanded version of lecture presented at American Physical Society meeting, 2/14/10 (Abraham Pais History of Physics Prize for 2009) by Stephen G. Brush* Abstract Does new scientific knowledge come from theory (whose predictions are confirmed by experiment) or from experiment (whose results are explained by theory)? Either can happen, depending on whether theory is ahead of experiment or experiment is ahead of theory at a particular time. In the first case, new theoretical hypotheses are made and their predictions are tested by experiments. But even when the predictions are successful, we can’t be sure that some other hypothesis might not have produced the same prediction. In the second case, as in a detective story, there are already enough facts, but several theories have failed to explain them. When a new hypothesis plausibly explains all of the facts, it may be quickly accepted before any further experiments are done. In the quantum-relativity revolution there are examples of both situations. Because of the two-stage development of both relativity (“special,” then “general”) and quantum theory (“old,” then “quantum mechanics”) in the period 1905-1930, we can make a double comparison of acceptance by prediction and by explanation. A curious anti- symmetry is revealed and discussed. _____________ *Distinguished University Professor (Emeritus) of the History of Science, University of Maryland. Home address: 108 Meadowlark Terrace, Glen Mills, PA 19342. Comments welcome. 1 “Science walks forward on two feet, namely theory and experiment. ... Sometimes it is only one foot which is put forward first, sometimes the other, but continuous progress is only made by the use of both – by theorizing and then testing, or by finding new relations in the process of experimenting and then bringing the theoretical foot up and pushing it on beyond, and so on in unending alterations.” Robert A. -
The Legacy of Leonhard Euler: a Tricentennial Tribute (419 Pages)
P698.TP.indd 1 9/8/09 5:23:37 PM This page intentionally left blank Lokenath Debnath The University of Texas-Pan American, USA Imperial College Press ICP P698.TP.indd 2 9/8/09 5:23:39 PM 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. THE LEGACY OF LEONHARD EULER A Tricentennial Tribute Copyright © 2010 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-13 978-1-84816-525-0 ISBN-10 1-84816-525-0 Printed in Singapore. LaiFun - The Legacy of Leonhard.pmd 1 9/4/2009, 3:04 PM September 4, 2009 14:33 World Scientific Book - 9in x 6in LegacyLeonhard Leonhard Euler (1707–1783) ii September 4, 2009 14:33 World Scientific Book - 9in x 6in LegacyLeonhard To my wife Sadhana, grandson Kirin,and granddaughter Princess Maya, with love and affection. -
Ether and Electrons in Relativity Theory (1900-1911) Scott Walter
Ether and electrons in relativity theory (1900-1911) Scott Walter To cite this version: Scott Walter. Ether and electrons in relativity theory (1900-1911). Jaume Navarro. Ether and Moder- nity: The Recalcitrance of an Epistemic Object in the Early Twentieth Century, Oxford University Press, 2018, 9780198797258. hal-01879022 HAL Id: hal-01879022 https://hal.archives-ouvertes.fr/hal-01879022 Submitted on 21 Sep 2018 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. Ether and electrons in relativity theory (1900–1911) Scott A. Walter∗ To appear in J. Navarro, ed, Ether and Modernity, 67–87. Oxford: Oxford University Press, 2018 Abstract This chapter discusses the roles of ether and electrons in relativity the- ory. One of the most radical moves made by Albert Einstein was to dismiss the ether from electrodynamics. His fellow physicists felt challenged by Einstein’s view, and they came up with a variety of responses, ranging from enthusiastic approval, to dismissive rejection. Among the naysayers were the electron theorists, who were unanimous in their affirmation of the ether, even if they agreed with other aspects of Einstein’s theory of relativity. The eventual success of the latter theory (circa 1911) owed much to Hermann Minkowski’s idea of four-dimensional spacetime, which was portrayed as a conceptual substitute of sorts for the ether. -
On the Shoulders of Giants: a Brief History of Physics in Göttingen
1 6 ON THE SHO UL DERS OF G I A NTS : A B RIEF HISTORY OF P HYSI C S IN G Ö TTIN G EN On the Shoulders of Giants: a brief History of Physics in Göttingen 18th and 19th centuries Georg Ch. Lichtenberg (1742-1799) may be considered the fore- under Emil Wiechert (1861-1928), where seismic methods for father of experimental physics in Göttingen. His lectures were the study of the Earth's interior were developed. An institute accompanied by many experiments with equipment which he for applied mathematics and mechanics under the joint direc- had bought privately. To the general public, he is better known torship of the mathematician Carl Runge (1856-1927) (Runge- for his thoughtful and witty aphorisms. Following Lichtenberg, Kutta method) and the pioneer of aerodynamics, or boundary the next physicist of world renown would be Wilhelm Weber layers, Ludwig Prandtl (1875-1953) complemented the range of (1804-1891), a student, coworker and colleague of the „prince institutions related to physics proper. In 1925, Prandtl became of mathematics“ C. F. Gauss, who not only excelled in electro- the director of a newly established Kaiser-Wilhelm-Institute dynamics but fought for his constitutional rights against the for Fluid Dynamics. king of Hannover (1830). After his re-installment as a profes- A new and well-equipped physics building opened at the end sor in 1849, the two Göttingen physics chairs , W. Weber and B. of 1905. After the turn to the 20th century, Walter Kaufmann Listing, approximately corresponded to chairs of experimen- (1871-1947) did precision measurements on the velocity depen- tal and mathematical physics. -
Introduction 8
© Copyright, Princeton University Press. No part of this book may be distributed, posted, or reproduced in any form by digital or mechanical means without prior written permission of the publisher. Introduction 8 “It’s a crying shame that Weyl is leaving Zurich. He is a great master.”1 Thus Albert Einstein described Hermann Weyl (1885–1955), who remains a leg- endary figure, “one of the greatest mathematicians of the first half of the twentieth century.... No other mathematician could claim to have initi- ated more of the theories that are now being explored,” as Michael Atiyah put it.2 Weyl deserves far wider renown not only for his importance in math- ematics and physics but also because of his deep philosophical concerns and thoughtful writing. Tothat end, this anthology gathers together some of Weyl’s most important general writings, especially those that have become unavail- able, have not previously been translated into English, or were unpublished. Together, they form a portrait of a complex and fascinating man, poetic and insightful, whose “vision has stood the test of time.”3 This vision has deeply affected contemporary physics, though Weyl always considered himself a mathematician, not a physicist.4 The present volume emphasizes his treatment of philosophy and physics, but another complete anthology could be made of Weyl’s general writings oriented more directly toward mathematics. Here, I have chosen those writings that most accessibly show how Weyl synthesized philosophy, physics, and mathematics. Weyl’s philosophical reflections began in early youth. He recollects vividly the worn copy of a book about Immanuel Kant’s Critique of Pure Reason he found in the family attic and read avidly at age fifteen. -
Gravity, Metaphysics Or Physics?
Fundamental Journals International Journal of Fundamental Physical Sciences (IJFPS) ISSN:2231-8186 IJFPS, Vol 3, No 4, pp 68-74, Dec , 2013 A.L. Guillen Gomez DOI:10.14331/ijfps.2013.330058 http://dx.doi.org/10.14331/ijfps.2013.330058 Gravity, Metaphysics or Physics? Alfonso Leon Guillen Gomez Independent scientific researcher, 127A Street 53A68 Flat 514, Bogota, Colombia Email: [email protected] (Received Sep 2013; Published Dec 2013) ABSTRACT Gravity is the foundation of the current physical paradigm. Due to that gravity is strongly linked to the curvature of space-time, we research that it lacks of a valid physical concept of space-time, nevertheless that from the science philosophy, via substantivalism, it has tried respond. We found that is due to that the gnoseological process applied from the general relativity, necessarily us leads to metaphysic because ontologically space-time is a metaphysical entity. Thus, we arrive to the super substantivalism that from metaphysics gives an answer on space-time rigorously exact with the vision of Einstein on physics. The result is that matter is nothing since all is space-time, i.e. geometry, therefore is a imperative of the physical science break the current paradigm.. Keywords: Gravity, Space-time, Metaphysics, Paradigm, DOI:10.14331/ijfps.2013.330058 INTRODUCTION threatens our ordinary distinctions between past, present and future, whilst GR suggests that space and time With the formulation of the general relativity is are not just the neutral stage upon which events take place, accepted that it has a scientific physics theory on gravity. but are themselves actors in the drama. -
Yet Another Introduction to Relativistic Astrophysics
Yet Another Introduction to Relativistic Astrophysics Luigi Foschini National Institute of Astrophysics (INAF) Brera Astronomical Observatory Milano/Merate (LC) – Italy July 8, 2021 arXiv:1703.05575v4 [astro-ph.HE] 7 Jul 2021 2 Foreword Relativistic Astrophysics deals with what we can say about the Universe by using the language of the theory of relativity. This peculiar type of language is strongly required when some conditions are verified, such as velocities close to that of light (for example, relativistic jets), and extreme energies or gravita- tional fields (for example, spacetime around black holes). This research field has wide overlaps with other fields, such as high-energy astrophysics and cos- mology. Therefore, it is necessary to make a selection of topics. These notes have been prepared for a series of short lessons for PhD students held at the Department of Physics and Astronomy of the University of Padova in March 2017. Ten hours of lessons can give only a taste of what is available. Given my researches, I selected mainly topics about black holes and jets, par- ticularly about supermassive objects in the centre of galaxies. Anyway, the large bibliography should give enough information to widen the necessarily limited horizon of these notes. In addition, I have not imported many figures from other works, but I cited them, so that I hope the reader could be further motivated to read more works. A large part of these notes deals with well-grounded knowledge. For relativity theory, I made use of many well-known textbooks, particularly Rindler [142], Cheng [32], Good [85], and d’Inverno [43]. -
Photon in a Cavity--A Gedankenexperiment
Photon in a cavity—a Gedankenexperiment Klaus Wilhelm∗ Max-Planck-Institut f¨ur Sonnensystemforschung (MPS), 37191 Katlenburg-Lindau, Germany Bhola N. Dwivedi† Dept. of Applied Physics, Indian Institute of Technology (Banaras Hindu University), Varanasi-221005, India (Dated: September 11, 2018) Abstract The inertial and gravitational mass of electromagnetic radiation (i.e., a photon distribution) in a cavity with reflecting walls has been treated by many authors for over a century. After many contending discussions, a consensus has emerged that the mass of such a photon distribution is equal to its total energy divided by the square of the speed of light. Nevertheless, questions remain unsettled on the interaction of the photons with the walls of the box. In order to understand some of the details of this interaction, a simple case of a single photon with an energy Eν = hν bouncing up and down in a static cavity with perfectly reflecting walls in a constant gravitational field g, constant in space and time, is studied and its contribution to the weight of the box is determined as a temporal average. arXiv:1307.2830v1 [physics.class-ph] 9 Jul 2013 1 I. INTRODUCTION Massive particles and electromagnetic radiation (photons) in a box have been considered by many authors.1–13 Most of them have discussed the inertia of an empty box in comparison with a box filled with a gas or radiation. In the presence of a constant gravitational field g (pointing downwards in Fig. 1), the effect on the weight of the box is another topic that has been studied.