Henri Poincaré, Theoretical Physics, and Relativity Theory in Paris Scott Walter
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The Scientific Content of the Letters Is Remarkably Rich, Touching on The
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Elsevier - Publisher Connector Reviews / Historia Mathematica 33 (2006) 491–508 497 The scientific content of the letters is remarkably rich, touching on the difference between Borel and Lebesgue measures, Baire’s classes of functions, the Borel–Lebesgue lemma, the Weierstrass approximation theorem, set theory and the axiom of choice, extensions of the Cauchy–Goursat theorem for complex functions, de Geöcze’s work on surface area, the Stieltjes integral, invariance of dimension, the Dirichlet problem, and Borel’s integration theory. The correspondence also discusses at length the genesis of Lebesgue’s volumes Leçons sur l’intégration et la recherche des fonctions primitives (1904) and Leçons sur les séries trigonométriques (1906), published in Borel’s Collection de monographies sur la théorie des fonctions. Choquet’s preface is a gem describing Lebesgue’s personality, research style, mistakes, creativity, and priority quarrel with Borel. This invaluable addition to Bru and Dugac’s original publication mitigates the regrets of not finding, in the present book, all 232 letters included in the original edition, and all the annotations (some of which have been shortened). The book contains few illustrations, some of which are surprising: the front and second page of a catalog of the editor Gauthier–Villars (pp. 53–54), and the front and second page of Marie Curie’s Ph.D. thesis (pp. 113–114)! Other images, including photographic portraits of Lebesgue and Borel, facsimiles of Lebesgue’s letters, and various important academic buildings in Paris, are more appropriate. -
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. -
Evolution of Mathematics: a Brief Sketch
Open Access Journal of Mathematical and Theoretical Physics Mini Review Open Access Evolution of mathematics: a brief sketch Ancient beginnings: numbers and figures Volume 1 Issue 6 - 2018 It is no exaggeration that Mathematics is ubiquitously Sujit K Bose present in our everyday life, be it in our school, play ground, SN Bose National Center for Basic Sciences, Kolkata mobile number and so on. But was that the case in prehistoric times, before the dawn of civilization? Necessity is the mother Correspondence: Sujit K Bose, Professor of Mathematics (retired), SN Bose National Center for Basic Sciences, Kolkata, of invenp tion or discovery and evolution in this case. So India, Email mathematical concepts must have been seen through or created by those who could, and use that to derive benefit from the Received: October 12, 2018 | Published: December 18, 2018 discovery. The creative process of discovery and later putting that to use must have been arduous and slow. I try to look back from my limited Indian perspective, and reflect up on what might have been the course taken up by mathematics during 10, 11, 12, 13, etc., giving place value to each digit. The barrier the long journey, since ancient times. of writing very large numbers was thus broken. For instance, the numbers mentioned in Yajur Veda could easily be represented A very early method necessitated for counting of objects as Dasha 10, Shata (102), Sahsra (103), Ayuta (104), Niuta (enumeration) was the Tally Marks used in the late Stone Age. In (105), Prayuta (106), ArA bud (107), Nyarbud (108), Samudra some parts of Europe, Africa and Australia the system consisted (109), Madhya (1010), Anta (1011) and Parartha (1012). -
Henry Andrews Bumstead 1870-1920
NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA BIOGRAPHICAL MEMOIRS VOLUME XIII SECOND MEMOIR BIOGRAPHICAL MEMOIR OF HENRY ANDREWS BUMSTEAD 1870-1920 BY LEIGH PAGE PRESENTED TO THE ACADEMY AT THE ANNUAL MEETING, 1929 HENRY ANDREWS BUMSTEAD BY LIUGH PAGE Henry Andrews Bumstead was born in the small town of Pekin, Illinois, on March 12th, 1870, son of Samuel Josiah Bumstead and Sarah Ellen Seiwell. His father, who was a physician of considerable local prominence, had graduated from the medical school in Philadelphia and was one of the first American students of medicine to go to Vienna to complete his studies. While the family was in Vienna, Bumstead, then a child three years of age, learned to speak German as fluently as he spoke English, an accomplishment which was to prove valuable to him in his subsequent career. Bumstead was descended from an old New England family which traces its origin to Thomas Bumstead, a native of Eng- land, who settled in Boston, Massachusetts, about 1640. Many of his ancestors were engaged in the professions, his paternal grandfather, the Reverend Samuel Andrews Bumstead, being a graduate of Princeton Theological Seminary and a minister in active service. From them he inherited a keen mind and an unusually retentive memory. It is related that long before he had learned to read, his Sunday school teacher surprised his mother by complimenting her on the ease with which her son had rendered the Sunday lesson. It turned out that his mother made a habit of reading the lesson to Bumstead before he left for school, and the child's remarkable performance there was due to his ability to hold in his memory every word of the lesson after hearing it read to him a single time. -
Paul Langevin (1872-1946), La Relativité Et Les Quanta, Bulletin De La Société Française De Physique, N° 119, Mai 1999, 15-20
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Hal-Diderot M ICHEL P ATY LANGEVIN, LA RELATIVITE ET LES QUANTA 1 Paul Langevin (1872-1946), la relativité et les quanta, Bulletin de la Société Française de Physique, n° 119, mai 1999, 15-20. Paul Langevin (1872-1946), la relativité et les quanta Michel PATY* Formation et profil scientifique: entre l'expérience et la théorie.- Les nouveaux phénomènes sur la constitution des corps et le «fondement électromagnétique de la matière» - La théorie de la relativité restreinte interprétée comme dynamique électromagnétique. Les phénomènes quantiques.- L'interprétation de la mécanique quantique.- Mémoire de Langevin. “Résumer l'œuvre de Langevin, écrivait Louis de Broglie en 1947, c'est reprendre toute l'histoire de la physique depuis cinquante ans” 1. Aussi bien telle n'est pas l'intention de cet article. Mais cette remarque de son célèbre élève est propre à rappeler d'emblée la dimension de ce physicien considérable, qui était l'une des meilleures et des plus sûres têtes pensantes de son époque, et d'ailleurs pas seulement en physique. Mais c'est à la physique que nous nous limiterons ici, et même à l'évocation d'un aspect relativement circonscrit de son histoire: comment, et en quoi, ce physicien clairvoyant et profond que fut Paul Langevin s'est-il trouvé amené à prendre sa part des renouvellements radicaux qui ont transformé la physique au début du XXè siècle, à savoir la relativité et les quanta. Il nous faut commencer par rappeler quelques éléments de sa biographie, et surtout de sa formation2. -
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. -
Sur Ma Généalogie Scientifique Française
Sur ma g´en´ealogie scientifique fran¸caise Didier Henrion Octobre 2010 1 Motivation Durant l'´et´e2010 j'ai effectu´equelques recherches sur ma g´en´ealogiescientifique, afin de compl´eterla base de donn´ees[Mathematics Genealogy Project]. Dans ce document j'ai regroup´equelques informations sur le profil des scientifiques constituant ma branche g´en´ealogiquefran¸caise. Le 12 octobre 1999 j'ai obtenu ma th`esede doctorat fran¸caise[Henrion, 1999] de l'Institut National des Sciences Appliqu´ees(INSA) de Toulouse, devant un jury constitu´ede Christian Burgat (pr´esident), Luc Dugard, Michel Malabre (rapporteurs), Jacques Bernussou, Vladim´ırKuˇcera,Bernard Pradin (examinateurs) et Sophie Tar- bouriech (directrice de th`ese).Les travaux de th`esecombinaient des r´esultatsd'automatique dans la lign´ee des travaux d'Aleksandr Lyapunov (chercheur russe du d´ebutdu XX`emesi`ecle,contemporain d'Henri Poin- car´e,et pr´ecurseurde l'´etudedes syst`emesdynamiques), pour ´etudierla stabilit´ede syst`emeslin´eairesdont les actionneurs saturent, et des r´esultatsd'optimisation convexe et de math´ematiquesappliqu´ees,concernant les in´egalit´esmatricielles lin´eaires,particuli`erement adapt´ees`ala commande des syst`emesen pr´esenced'incertitudes param´etriqueset de mod´elisation. On notera la pr´esencedans le jury de th`esede Bernard Pradin, alors professeur d'automatique `al'INSA de Toulouse. Ses cours, ainsi que ceux de Germain Garcia, Christian Mira et Andr´eTitli, sont `al'origine de ma vocation. En 1998 j'ai ´egalement obtenu un doctorat de l'Acad´emiedes Sciences de la R´epubliqueTch`eque,mais je compte d´ecrirema g´en´ealogietch`equedans un autre document. -
Max Abraham's and Tullio Levi-Civita's Approach to Einstein
Alma Mater Studiorum Universita` di · Bologna DOTTORATO DI RICERCA IN Matematica Ciclo XXV Settore concorsuale di afferenza: 01/A4 Settore Scientifico disciplinare: MAT/07 Max Abraham’s and Tullio Levi-Civita’s approach to Einstein Theory of Relativity Presentata da: Michele Mattia Valentini Coordinatore Dottorato: Relatore: Chiar.ma Prof.ssa Chiar.mo Prof. Giovanna Citti Sandro Graffi Esame finale anno 2014 Introduction This thesis deals with the theory of relativity and its diffusion in Italy in the first decades of the XX century. Albert Einstein’s theory of Special and General relativity is deeply linked with Italy and Italian scientists. Not many scientists really involved themselves in that theory understanding, but two of them, Max Abraham and Tullio Levi-Civita left a deep mark in the theory development. Max Abraham engaged a real battle against Ein- stein between 1912 and 1914 about electromagnetic theories and gravitation theories, while Levi-Civita played a fundamental role in giving Einstein the correct mathematical instruments for the general relativity formulation since 1915. Many studies have already been done to explain their role in the develop- ment of Einstein theory from both a historical and a scientific point of view. This work, which doesn’t have the aim of a mere historical chronicle of the events, wants to highlight two particular perspectives. 1. Abraham’s objections against Einstein focused on three important con- ceptual kernels of theory of relativity: the constancy of light speed, the relativity principle and the equivalence hypothesis. Einstein was forced by Abraham to explain scientific and epistemological reasons of the formulation of his theory. -
Bibliographie
Bibliographie Abraham, M. Dynamik des Electrons. Nachrichten von der Königlichen Gesellschaft der Wissenschaften zu Göttingen, mathematisch-physikalische Klasse (1902) : 20–41. —. Prinzipien der Dynamik des Elektrons. Physikalische Zeitschrift 4 (1903) : 57–63. —. Die Grundhypothesen der Elektronentheorie. Physikalische Zeitschrift 5 (1904) : 576–579. Académie des sciences, dir. Index biographique des membres et correspondants de l’Aca- démie des sciences. Paris : Gauthier-Villars, 1968. Accademia dei Lincei, dir. Tullio Levi-Civita, Convegno internazionale celebrativo del Centenario. Rome : Accademia dei Lincei, 1975. Ames, J.S. L’équivalent mécanique de la chaleur. In Guillaume et Poincaré (1900–1901), 1 : 178–213, 1900. Andersson, K. Poincaré’s discovery of homoclinic points. Archive for History of Exact Sciences 48 (1994) : 135–147. Armstrong, H.E., Foster, M., Klein, F., Köppen, T.P., Poincaré, H., Rücker, A.W., Schwalbe, B., et Weiss, E. International catalogue of scientific literature : Report of the Provisional International Committee. Science 10 (1899) : 482–487. Arnoux, G. Essais de psychologie et de métaphysique positives ; la méthode graphique en mathématiques. Association française pour l’avancement des sciences 20 (1891) : 2 : 241–259. Arrhenius, S. Lehrbuch der kosmischen Physik. Leipzig : Hirzel, 1903. —. L’évolution des mondes. Paris : Librairie polytechnique, 1910. —. Conférénces sur quelques thèmes choisis de la chimie physique pure et appliquée : faites à l’université de Paris du 6 au 13 mars 1911. Paris : Hermann, 1912a. —. Die Verteilung der Himmelskörper. Meddelanden från Kungl. Vetenskaps-Akad- emiens Nobelinstitut 2.21 (1912b). Arzeliès, H. La dynamique relativiste et ses applications. 2 vols. Paris : Gauthier-Villars, 1957–1958. Arzeliès, H. et Henry, J. Milieux conducteurs ou polarisables en mouvement. -
December 4, 1954 NATURE 1037
No. 4440 December 4, 1954 NATURE 1037 COPLEY MEDALLISTS, 1915-54 is that he never ventured far into interpretation or 1915 I. P. Pavlov 1934 Prof. J. S. Haldane prediction after his early studies in fungi. Here his 1916 Sir James Dewar 1935 Prof. C. T. R. Wilson interpretation was unfortunate in that he tied' the 1917 Emile Roux 1936 Sir Arthur Evans word sex to the property of incompatibility and 1918 H. A. Lorentz 1937 Sir Henry Dale thereby led his successors astray right down to the 1919 M. Bayliss W. 1938 Prof. Niels Bohr present day. In a sense the style of his work is best 1920 H. T. Brown 1939 Prof. T. H. Morgan 1921 Sir Joseph Larmor 1940 Prof. P. Langevin represented by his diagrams of Datura chromosomes 1922 Lord Rutherford 1941 Sir Thomas Lewis as packets. These diagrams were useful in a popular 1923 Sir Horace Lamb 1942 Sir Robert Robinson sense so long as one did not take them too seriously. 1924 Sir Edward Sharpey- 1943 Sir Joseph Bancroft Unfortunately, it seems that Blakeslee did take them Schafer 1944 Sir Geoffrey Taylor seriously. To him they were the real and final thing. 1925 A. Einstein 1945 Dr. 0. T. Avery By his alertness and ingenuity and his practical 1926 Sir Frederick Gow 1946 Dr. E. D. Adrian sense in organizing the Station for Experimental land Hopkins 1947 Prof. G. H. Hardy Evolution at Cold Spring Harbor (where he worked 1927 Sir Charles Sherring- 1948 . A. V. Hill Prof in 1942), ton 1949 Prof. G. -
Can Science Advance Effectively Through Philosophical Criticism and Reflection?
Can science advance effectively through philosophical criticism and reflection? ROBERTO TORRETTI Universidad de Puerto Rico ABSTRACT Prompted by Hasok Chang’s conception of the history and philosophy of science (HPS) as the continuation of science by other means, I examine the possibility of obtaining scientific knowledge through philosophical criticism and reflection, in the light of four historical cases, concerning (i) the role of absolute space in Newtonian dynamics, (ii) the purported contraction of rods and retardation of clocks in Special Relativity, (iii) the reality of the electromagnetic ether, and (iv) the so-called problem of time’s arrow. In all four cases it is clear that a better understanding of such matters can be achieved —and has been achieved— through conceptual analysis. On the other hand, however, it would seem that this kind of advance has more to do with philosophical questions in science than with narrowly scientific questions. Hence, if HPS in effect continues the work of science by other means, it could well be doing it for other ends than those that working scientists ordinarily have in mind. Keywords: Absolute space – Inertial frames – Length contraction – Clock retardation – Special relativity – Ether – Time – Time directedness – Entropy – Boltzmann entropy Philosophical criticism and the advancement of science 2 The mind will not readily give up the attempt to apprehend the exact formal character of the latent connexions between different physical agencies: and the history of discovery may be held perhaps to supply the strongest reason for estimating effort towards clearness of thought as of not less importance in its own sphere than exploration of phenomena. -
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].