LANCZOS's FUNCTIONAL THEORY of ELECTRODYNAMICS a Commentary on Lanczos's Ph.D. Dissertation
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REVIEWS and DESCRIPTIONS of TABLES and BOOKS the Numbers
MATHEMATICS OF COMPUTATION Volume 65, Number 213, January 1996, Pages 429{443 S 0025-5718-96-00698-9 REVIEWS AND DESCRIPTIONS OF TABLES AND BOOKS The numbers in brackets are assigned according to the American Mathematical Society classification scheme. The 1991 Mathematics Subject Classification can be found in the annual subject index of Mathematical Reviews starting with the December 1990 issue. 1[65-00, 41-00, 41A05, 41A21, 41A55, 41A65, 65C05, 65H05, 65T20, 73C50, 73V20]—Handbook of numerical analysis, Vol. III, P. G. Ciarlet and J. L. Lions (Editors), Techniques of scientific computing (Part 1), Numerical methods for solids (Part 1), Solution of equations in Rn (Part 2), North-Holland, 1 Amsterdam, 1994, x+778 pp., 24 2 cm, $154.25/Dfl. 270.00 This book contains three parts: 1) Techniques of Scientific Computing; 2) Nu- merical Methods for Solids; 3) Solution of Equations in Rn. Nevertheless, only the second part gets close to “numerical methods for large-scale computation”. The aims of the book are rather “constructive methods”, which are often the background to numerical methods. The first part is concerned with three aspects of approximation theory. First, Claude Brezinski provides an interesting historical perspective on interpolation, ap- proximation and numerical quadrature since the year 1611. His main contribution, however, is a survey on Pad´e approximation, written jointly with van Iseghen. The algebraic theory naturally elucidates the connections with orthogonal polynomi- als and continued fractions. The convergence theory contains, on the one hand, a complete theory for Stieltjes functions and, on the other hand, only convergence in capacity for the general case. -
ITS FIRST FIFTY YEARS Carl Β
THE MATHEMATICAL ASSOCIATION OF AMERICA: ITS FIRST FIFTY YEARS Carl Β. Boyer Brooklyn College, CUNY Richard W. Feldmann Lycoming College Harry M. Gehman SUN Yat Buffalo Phillip S. Jones University of Michigan Kenneth O. May University of Toronto Harriet F. Montague SUNYat Buffalo Gregory H. Moore University of Toronto Robert A. Rosenbaum Wesleyan University Emory P. Starke Rutgers University Dirk J. Struik Massachusetts Institute of Technology THE MATHEMATICAL ASSOCIATION OF AMERICA: ITS FIRST FIFTY YEARS Kenneth O. May, editor University of Toronto, Canada Published and distributed by The Mathematical Association of America Copyright 1972 by THE MATHEMATICAL ASSOCIATION OF AMERICA (INCORPORATED) PREFACE The fiftieth anniversary of the founding of the Mathematical Association of America was celebrated at the 1965 summer meeting at Cornell University [MONTHLY 72, 1053-1059]. The invited addresses on that occasion dealing with the past, present, and future of the Association and of mathematics, were published in the fiftieth anniversary issue [MONTHLY 74, Num. !, Part II] under the editorship of Carl B. Allendoerfer. The historical addresses by A. A. Bennett, R. A. Rosenbaum, W. L. Duren, Jr., and P. S. Jones whetted appetites for a more complete story of the Association. Early in 1966, on a recommendation of the Committee on Publications, President R. L. Wilder appointed a Committee on the Preparation of a Fifty-Year History of the Association consisting of Carl B. Boyer, Kenneth O. May (Chairman), and Dirk J. Struik. An appropriation of one thousand dollars was set aside to meet incidental expenses. The Committee began its work with very ambitious plans, hoping to get financial support for interviewing older members of the Association and the preparation of special studies on particular aspects of the Association's work. -
Einstein's Gravitational Field
Einstein’s gravitational field Abstract: There exists some confusion, as evidenced in the literature, regarding the nature the gravitational field in Einstein’s General Theory of Relativity. It is argued here that this confusion is a result of a change in interpretation of the gravitational field. Einstein identified the existence of gravity with the inertial motion of accelerating bodies (i.e. bodies in free-fall) whereas contemporary physicists identify the existence of gravity with space-time curvature (i.e. tidal forces). The interpretation of gravity as a curvature in space-time is an interpretation Einstein did not agree with. 1 Author: Peter M. Brown e-mail: [email protected] 2 INTRODUCTION Einstein’s General Theory of Relativity (EGR) has been credited as the greatest intellectual achievement of the 20th Century. This accomplishment is reflected in Time Magazine’s December 31, 1999 issue 1, which declares Einstein the Person of the Century. Indeed, Einstein is often taken as the model of genius for his work in relativity. It is widely assumed that, according to Einstein’s general theory of relativity, gravitation is a curvature in space-time. There is a well- accepted definition of space-time curvature. As stated by Thorne 2 space-time curvature and tidal gravity are the same thing expressed in different languages, the former in the language of relativity, the later in the language of Newtonian gravity. However one of the main tenants of general relativity is the Principle of Equivalence: A uniform gravitational field is equivalent to a uniformly accelerating frame of reference. This implies that one can create a uniform gravitational field simply by changing one’s frame of reference from an inertial frame of reference to an accelerating frame, which is rather difficult idea to accept. -
Selected Papers
Selected Papers Volume I Arizona, 1968 Peter D. Lax Selected Papers Volume I Edited by Peter Sarnak and Andrew Majda Peter D. Lax Courant Institute New York, NY 10012 USA Mathematics Subject Classification (2000): 11Dxx, 35-xx, 37Kxx, 58J50, 65-xx, 70Hxx, 81Uxx Library of Congress Cataloging-in-Publication Data Lax, Peter D. [Papers. Selections] Selected papers / Peter Lax ; edited by Peter Sarnak and Andrew Majda. p. cm. Includes bibliographical references and index. ISBN 0-387-22925-6 (v. 1 : alk paper) — ISBN 0-387-22926-4 (v. 2 : alk. paper) 1. Mathematics—United States. 2. Mathematics—Study and teaching—United States. 3. Lax, Peter D. 4. Mathematicians—United States. I. Sarnak, Peter. II. Majda, Andrew, 1949- III. Title. QA3.L2642 2004 510—dc22 2004056450 ISBN 0-387-22925-6 Printed on acid-free paper. © 2005 Springer Science+Business Media, Inc. All rights reserved. This work may not be translated or copied in whole or in part without the written permission of the publisher (Springer Science+Business Media, Inc., 233 Spring Street, New York, NY 10013, USA), except for brief excerpts in connection with reviews or scholarly analysis. Use in connection with any form of information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed is forbidden. The use in this publication of trade names, trademarks, service marks, and similar terms, even if they are not identified as such, is not to be taken as an expression of opinion as to whether or not they are subject to proprietary rights. Printed in the United States of America. -
Theory of Relativity
Christian Bar¨ Theory of Relativity Summer Term 2013 OTSDAM P EOMETRY IN G Version of August 26, 2013 Contents Preface iii 1 Special Relativity 1 1.1 Classical Kinematics ............................... 1 1.2 Electrodynamics ................................. 5 1.3 The Lorentz group and Minkowski geometry .................. 7 1.4 Relativistic Kinematics .............................. 20 1.5 Mass and Energy ................................. 36 1.6 Closing Remarks about Special Relativity .................... 41 2 General Relativity 43 2.1 Classical theory of gravitation .......................... 43 2.2 Equivalence Principle and the Einstein Field Equations ............. 49 2.3 Robertson-Walker spacetime ........................... 55 2.4 The Schwarzschild solution ............................ 66 Bibliography 77 Index 79 i Preface These are the lecture notes of an introductory course on relativity theory that I gave in 2013. Ihe course was designed such that no prior knowledge of differential geometry was required. The course itself also did not introduce differential geometry (as it is often done in relativity classes). Instead, students unfamiliar with differential geometry had the opportunity to learn the subject in another course precisely set up for this purpose. This way, the relativity course could concentrate on its own topic. Of course, there is a price to pay; the first half of the course was dedicated to Special Relativity which does not require much mathematical background. Only the second half then deals with General Relativity. This gave the students time to acquire the geometric concepts. The part on Special Relativity briefly recalls classical kinematics and electrodynamics empha- sizing their conceptual incompatibility. It is then shown how Minkowski geometry is used to unite the two theories and to obtain what we nowadays call Special Relativity. -
RM Calendar 2017
Rudi Mathematici x3 – 6’135x2 + 12’545’291 x – 8’550’637’845 = 0 www.rudimathematici.com 1 S (1803) Guglielmo Libri Carucci dalla Sommaja RM132 (1878) Agner Krarup Erlang Rudi Mathematici (1894) Satyendranath Bose RM168 (1912) Boris Gnedenko 1 2 M (1822) Rudolf Julius Emmanuel Clausius (1905) Lev Genrichovich Shnirelman (1938) Anatoly Samoilenko 3 T (1917) Yuri Alexeievich Mitropolsky January 4 W (1643) Isaac Newton RM071 5 T (1723) Nicole-Reine Etable de Labrière Lepaute (1838) Marie Ennemond Camille Jordan Putnam 2002, A1 (1871) Federigo Enriques RM084 Let k be a fixed positive integer. The n-th derivative of (1871) Gino Fano k k n+1 1/( x −1) has the form P n(x)/(x −1) where P n(x) is a 6 F (1807) Jozeph Mitza Petzval polynomial. Find P n(1). (1841) Rudolf Sturm 7 S (1871) Felix Edouard Justin Emile Borel A college football coach walked into the locker room (1907) Raymond Edward Alan Christopher Paley before a big game, looked at his star quarterback, and 8 S (1888) Richard Courant RM156 said, “You’re academically ineligible because you failed (1924) Paul Moritz Cohn your math mid-term. But we really need you today. I (1942) Stephen William Hawking talked to your math professor, and he said that if you 2 9 M (1864) Vladimir Adreievich Steklov can answer just one question correctly, then you can (1915) Mollie Orshansky play today. So, pay attention. I really need you to 10 T (1875) Issai Schur concentrate on the question I’m about to ask you.” (1905) Ruth Moufang “Okay, coach,” the player agreed. -
Post-Newtonian Approximations and Applications
Monash University MTH3000 Research Project Coming out of the woodwork: Post-Newtonian approximations and applications Author: Supervisor: Justin Forlano Dr. Todd Oliynyk March 25, 2015 Contents 1 Introduction 2 2 The post-Newtonian Approximation 5 2.1 The Relaxed Einstein Field Equations . 5 2.2 Solution Method . 7 2.3 Zones of Integration . 13 2.4 Multi-pole Expansions . 15 2.5 The first post-Newtonian potentials . 17 2.6 Alternate Integration Methods . 24 3 Equations of Motion and the Precession of Mercury 28 3.1 Deriving equations of motion . 28 3.2 Application to precession of Mercury . 33 4 Gravitational Waves and the Hulse-Taylor Binary 38 4.1 Transverse-traceless potentials and polarisations . 38 4.2 Particular gravitational wave fields . 42 4.3 Effect of gravitational waves on space-time . 46 4.4 Quadrupole formula . 48 4.5 Application to Hulse-Taylor binary . 52 4.6 Beyond the Quadrupole formula . 56 5 Concluding Remarks 58 A Appendix 63 A.1 Solving the Wave Equation . 63 A.2 Angular STF Tensors and Spherical Averages . 64 A.3 Evaluation of a 1PN surface integral . 65 A.4 Details of Quadrupole formula derivation . 66 1 Chapter 1 Introduction Einstein's General theory of relativity [1] was a bold departure from the widely successful Newtonian theory. Unlike the Newtonian theory written in terms of fields, gravitation is a geometric phenomena, with space and time forming a space-time manifold that is deformed by the presence of matter and energy. The deformation of this differentiable manifold is characterised by a symmetric metric, and freely falling (not acted on by exter- nal forces) particles will move along geodesics of this manifold as determined by the metric. -
On a Stationary Cosmology in the Sense of Einstein's
G en eral Relativity an d G ravitation , Vol. 29, No. 3, 1997 Editor’s Note: On a Stationary Cosm ology in the Sense of Einstein’s Theory of Grav itation by Kornel Lanczos, Zeitschrift furÈ Physik 21 (1924) , 73± 110 When asked who found the ® rst exact solution of Einstein’ s equations with rotating matter source and when, most physicist s would answer that it was Godel,È in 1949 [1]. In fact, the correct answer is Lanczos in 1924, in the paper print ed in this issue. Setting the historical record straight is the ® rst reason for republishing Lanczos’ paper. (To be sure, Godel’È s solution was new in 1949 because it is diŒerent from Lanczos’ , it is very important and was discussed by GodelÈ with illuminat ing insight s, but the credit for historical priority that it enjoys is not deserved.) There is one more reason. Back in 1924, exact solutions of Einstein’s equations were still a rarity. Nevertheless, the author was not satis® ed just to derive a new exact solution. He felt obliged to investigate what the solution implies for our Universe, and he did so with such breadth, depth and clarity that the paper can set standards and provide inspirat ion to readers even today. The modern reader will have to forgive the author for a few inconsis- tencies with the now commonly accepted terminology (such as the notion of static vs. stationary solut ions discussed in the introduct ion) and, in places, for an old-fashioned, long-forgot ten notation. Also, in 1924 no- body was yet aware that our Galaxy is not the whole Universe, and that the Sun is not at the center of the Galaxy. -
Descriptions of Relativistic Dynamics with World Line Condition
quantum reports Article Descriptions of Relativistic Dynamics with World Line Condition Florio Maria Ciaglia 1 , Fabio Di Cosmo 2,3,* , Alberto Ibort 2,3 and Giuseppe Marmo 4,5 1 Max-Planck-Institut für Mathematik in den Naturwissenschaften, Inselstraße 22, 04103 Leipzig, Germany; [email protected] 2 Dep.to de Matematica, Univ. Carlos III de Madrid. Av. da de la Universidad, 30, 28911 Leganes, Madrid, Spain; [email protected] 3 ICMAT, Instituto de Ciencias Matematicas (CSIC-UAM-UC3M-UCM), Nicolás Cabrera, 13-15, Campus de Cantoblanco, UAM, 28049 Madrid, Spain 4 INFN-Sezione di Napoli, Complesso Universitario di Monte S. Angelo. Edificio 6, via Cintia, 80126 Napoli, Italy; [email protected] 5 Dipartimento di Fisica “E. Pancini”, Università di Napoli Federico II, Complesso Universitario di Monte S. Angelo Edificio 6, via Cintia, 80126 Napoli, Italy * Correspondence: [email protected] Received: 14 September 2019; Accepted: 15 October 2019; Published: 19 October 2019 Abstract: In this paper, a generalized form of relativistic dynamics is presented. A realization of the Poincaré algebra is provided in terms of vector fields on the tangent bundle of a simultaneity surface in R4. The construction of this realization is explicitly shown to clarify the role of the commutation relations of the Poincaré algebra versus their description in terms of Poisson brackets in the no-interaction theorem. Moreover, a geometrical analysis of the “eleventh generator” formalism introduced by Sudarshan and Mukunda is outlined, this formalism being at the basis of many proposals which evaded the no-interaction theorem. Keywords: relativistic dynamics; no-interaction theorem; world line condition In memory of E.C.G. -
Quantum Fluctuations and Thermodynamic Processes in The
Quantum fluctuations and thermodynamic processes in the presence of closed timelike curves by Tsunefumi Tanaka A thesis submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in Physics Montana State University © Copyright by Tsunefumi Tanaka (1997) Abstract: A closed timelike curve (CTC) is a closed loop in spacetime whose tangent vector is everywhere timelike. A spacetime which contains CTC’s will allow time travel. One of these spacetimes is Grant space. It can be constructed from Minkowski space by imposing periodic boundary conditions in spatial directions and making the boundaries move toward each other. If Hawking’s chronology protection conjecture is correct, there must be a physical mechanism preventing the formation of CTC’s. Currently the most promising candidate for the chronology protection mechanism is the back reaction of the metric to quantum vacuum fluctuations. In this thesis the quantum fluctuations for a massive scalar field, a self-interacting field, and for a field at nonzero temperature are calculated in Grant space. The stress-energy tensor is found to remain finite everywhere in Grant space for the massive scalar field with sufficiently large field mass. Otherwise it diverges on chronology horizons like the stress-energy tensor for a massless scalar field. If CTC’s exist they will have profound effects on physical processes. Causality can be protected even in the presence of CTC’s if the self-consistency condition is imposed on all processes. Simple classical thermodynamic processes of a box filled with ideal gas in the presence of CTC’s are studied. If a system of boxes is closed, its state does not change as it travels through a region of spacetime with CTC’s. -
The Confrontation Between General Relativity and Experiment
The Confrontation between General Relativity and Experiment Clifford M. Will Department of Physics University of Florida Gainesville FL 32611, U.S.A. email: [email protected]fl.edu http://www.phys.ufl.edu/~cmw/ Abstract The status of experimental tests of general relativity and of theoretical frameworks for analyzing them are reviewed and updated. Einstein’s equivalence principle (EEP) is well supported by experiments such as the E¨otv¨os experiment, tests of local Lorentz invariance and clock experiments. Ongoing tests of EEP and of the inverse square law are searching for new interactions arising from unification or quantum gravity. Tests of general relativity at the post-Newtonian level have reached high precision, including the light deflection, the Shapiro time delay, the perihelion advance of Mercury, the Nordtvedt effect in lunar motion, and frame-dragging. Gravitational wave damping has been detected in an amount that agrees with general relativity to better than half a percent using the Hulse–Taylor binary pulsar, and a growing family of other binary pulsar systems is yielding new tests, especially of strong-field effects. Current and future tests of relativity will center on strong gravity and gravitational waves. arXiv:1403.7377v1 [gr-qc] 28 Mar 2014 1 Contents 1 Introduction 3 2 Tests of the Foundations of Gravitation Theory 6 2.1 The Einstein equivalence principle . .. 6 2.1.1 Tests of the weak equivalence principle . .. 7 2.1.2 Tests of local Lorentz invariance . .. 9 2.1.3 Tests of local position invariance . 12 2.2 TheoreticalframeworksforanalyzingEEP. ....... 16 2.2.1 Schiff’sconjecture ................................ 16 2.2.2 The THǫµ formalism ............................. -
General Relativity and Geometry: Interactions and Missed Opportunities
1. Prehistory 2. Ricci 3. General Relativity 4. Weyl 5. Kaluza 6. Lanczos 7. ADM 8. Supergravity 9. Conclusion General Relativity and Geometry: Interactions and Missed Opportunities Jean-Pierre BOURGUIGNON (CNRS-Institut des Hautes Etudes´ Scientifiques) Institut Henri Poincar´e,Paris November 16, 2015 1. Prehistory 2. Ricci 3. General Relativity 4. Weyl 5. Kaluza 6. Lanczos 7. ADM 8. Supergravity 9. Conclusion Outline of the Lecture All along history, and especially in the 19th and 20th century, Geometry and Physics have interacted in a very positive way. Taking advantage of the historical dimension of this conference, this lecture presents such instances in the context of the Theory of General Relativity, some have been truly influential, others of the type \missed opportunities". Actually, the extent to which this has happened is truly remarkable, and has, in my opinion, not been stressed enough. As several lectures at this conference will be dedicated to the latest mathematical developments, some very striking and representing remarkable technical achievements, I will concentrate more on the variety of the modes of interaction, stressing the differences in the points of view of physicists and mathematicians that they reveal from an epistemological point of view. 1. Prehistory 2. Ricci 3. General Relativity 4. Weyl 5. Kaluza 6. Lanczos 7. ADM 8. Supergravity 9. Conclusion Outline of the Lecture All along history, and especially in the 19th and 20th century, Geometry and Physics have interacted in a very positive way. Taking advantage of the historical dimension of this conference, this lecture presents such instances in the context of the Theory of General Relativity, some have been truly influential, others of the type \missed opportunities".