A New Perspective on Relativity B1197-Ch01
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Belated Decision in the Hilbert-Einstein Priority Dispute
(10). As described above, the severely opis- Dinosauria (Univ. of California Press, Berkeley, CA, However, the overall similarity of the pelvis of Archae- 1990). opteryx to those of the enantiornithine birds, espe- thopubic condition of their pelvis is consis- 10. L. Hou, L. D. Martin, Z. Zhou, A. Feduccia, Science cially the presence of the hypopubic cup, as well as tent with the notion that these birds roost- 274, 1164 (1996). the morphology of the London and Berlin Archae- ed in trees. In contrast, based primarily on 11. Q. Ji and S. Ji, Chin. Geol. 10, 30 (1996); see also V. opteryx specimens, offer support for our interpreta- disputed measurements of claw curvature, Morell, Audubon 99, 36 (1997). tion of the pelvic structure of these early birds [L. D. 12. Rather than representing primitive archosaurian Martin, in Origin of the Higher Groups of Tetrapods, Archaeopteryx has been interpreted as structures, it is probable that the hepatic-piston dia- H. P. Schultze and L. Trueb, Eds. (Cornell Univ. adapted primarily for a terrestrial rather phragm systems in crocodilians and theropods are Press, Ithaca, NY, 1991), pp. 485–540. than an arboreal existence (18). However, convergently derived. Pelvic anatomy in early “pro- 18. D. S. Peters and E. Go¨ rgner, in Proceedings of the II todinosaurs” such as Lagosuchus, as well as in all International Symposium of Avian Paleontology, K. as in the enantiornithines, the morphology ornithischian dinosaurs, shows no evidence of the Campbell, Ed. (Los Angeles Museum of Natural His- of Archaeopteryx’s pelvis is best interpreted pubis having served as a site of origin for similar tory Press, Los Angeles, CA, 1992), pp. -
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. -
Einstein's Life and Legacy
Reflections Einstein's Life and Legacy Introduction Albert Einstein is the most luminous scientist of the past century, and ranks with Isaac Newton as one among the greatest physicists of all time. There is an enormous amount of material to choose from in talking about Einstein. He is without doubt also the most written about scientist of the past century, may be of all time. The Einstein Archives contain about 43,000 documents, and so far as I know the "Collected Papers of Albert Einstein" have only come upto 1917 with Volume 8 in English translation; another 32 volumes remain to be produced. In the face of all this, this account must be severely selective, and coherent as well. Einstein's life was incredibly rich and intense in the intellectual sense. This will become clear as I go along. In any case let me begin by presenting in Box 1 a brieflisting of a few important dates in his life, howsoever inadequate it may be. He was scientifically active essentially from 1902 upto 1935 at the highest imaginable levels, thus for more than three decades. The Miraculous Year Now let us turn to technical matters. First, a brief mention of his creative outburst of 1905, whose centenary we are celebrating this year. There were four fundamental papers, and the doctoral thesis, all in the six months from March to September. The first paper on the light quantum concept and explanation of the photo electric effect was submitted to Annalen der Physik in March; the second on Brownian Motion in May; and the third setting out the Special Theory of Relativity in June. -
Einstein and Hilbert: the Creation of General Relativity
EINSTEIN AND HILBERT: THE CREATION OF GENERAL RELATIVITY ∗ Ivan T. Todorov Institut f¨ur Theoretische Physik, Universit¨at G¨ottingen, Friedrich-Hund-Platz 1 D-37077 G¨ottingen, Germany; e-mail: [email protected] and Institute for Nuclear Research and Nuclear Energy, Bulgarian Academy of Sciences Tsarigradsko Chaussee 72, BG-1784 Sofia, Bulgaria;∗∗e-mail: [email protected] ABSTRACT It took eight years after Einstein announced the basic physical ideas behind the relativistic gravity theory before the proper mathematical formulation of general relativity was mastered. The efforts of the greatest physicist and of the greatest mathematician of the time were involved and reached a breathtaking concentration during the last month of the work. Recent controversy, raised by a much publicized 1997 reading of Hilbert’s proof- sheets of his article of November 1915, is also discussed. arXiv:physics/0504179v1 [physics.hist-ph] 25 Apr 2005 ∗ Expanded version of a Colloquium lecture held at the International Centre for Theoretical Physics, Trieste, 9 December 1992 and (updated) at the International University Bremen, 15 March 2005. ∗∗ Permanent address. Introduction Since the supergravity fashion and especially since the birth of superstrings a new science emerged which may be called “high energy mathematical physics”. One fad changes the other each going further away from accessible experiments and into mathe- matical models, ending up, at best, with the solution of an interesting problem in pure mathematics. The realization of the grand original design seems to be, decades later, nowhere in sight. For quite some time, though, the temptation for mathematical physi- cists (including leading mathematicians) was hard to resist. -
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. -
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. -
Prof. Walther Ritz
Professor Walther Ritz (1878 – 1909) From Wikipedia, the free encyclopedia: http://en.wikipedia.org/wiki/Walther_Ritz Walther Ritz (b. February 22, 1878 in Sion, Switzerland - d. 7 July 1909 in Göttingen) was a Swiss theoretical physicist. His father, Raphael Ritz, a native of Valais, was a well-known landscape and interior scenes artist. His mother was the daughter of the engineer Noerdlinger of Tübingen. Ritz studied in Zurich and Göttingen. He is most famous for his work with Johannes Rydberg on the Rydberg–Ritz combination principle. Ritz is also known for the variational method named after him, the Ritz method. Ritz died in 1909, at the age of 31. According to Forman's Dictionary of Scientific Biography, Ritz contracted tuberculosis in 1900, which led to his death in 1909. According to Ritz's collected works (Œuvres) the disease was pleurisy. Criticism of Maxwell-Lorentz electromagnetic theory Not so well known is the fact that in 1908 Walter Ritz produced a lengthy criticism of Maxwell-Lorentz electromagnetic theory, in which he contended that the theory's connection with the luminescent ether (see Lorentz ether theory) made it "essentially inappropriate to express the comprehensive laws for the propagation of electrodynamic actions." Walter Ritz pointed out seven problems with Maxwell-Lorentz electromagnetic field equations: 1 Electric and magnetic forces really express relations about space and time and should be replaced with non- instantaneous elementary actions (his emission theory). 2 Advanced potentials don't exist (and their erroneous use led to the Rayleigh-Jeans ultraviolet catastrophe). 3 Localization of energy in the ether is vague. -
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. -
Project GREAT PTTI-2006 PPT-PDF
Project GREAT (2005) General Relativity Einstein / Essen Anniversary Test Tom Van Baak [email protected] PTTI 2006 Washington DC Introduction • Project GREAT in 2005 – Attempt to prove the theory of relativity – Take cesium clocks up a mountain – Do clocks really speed up or slow down? • Celebrate 100th anniversary of 1905 – Albert Einstein’s “Annus Mirabilis” • Celebrate 50th anniversary of 1955 – Louis Essen’s NPL cesium clock 06-Dec-2006 Project GREAT 2 Albert Einstein • Who was Einstein? – Need I say more… – Theory of relativity – Time is not absolute – SR, GR, space-time – Bold predictions – Later confirmed – Enormous influence 06-Dec-2006 Project GREAT 3 Einstein and 2005 •100th anniversary of relativity: books, magazines, radio, TV, web sites, “Physics Year”, lectures… 06-Dec-2006 Project GREAT 4 Louis Essen • Who was Essen? –First Cesium Clock – Joint NPL USNO project to calibrate atomic time against astronomical time – 9 192 631 770 Hz – Book: “Famous for a second” 06-Dec-2006 Project GREAT 5 Essen and 2005 •50th anniversary of atomic time •NPL Caesium Jack Parry and Louis Essen Photo from www.npl.co.uk/essen/ 06-Dec-2006 Project GREAT 6 Cs Second • 1954…1958 •How long is a second? 06-Dec-2006 Project GREAT 7 Louis Essen •10 years later … • Essen at NPL with a HP 5060A “Flying Clock” 06-Dec-2006 Project GREAT 8 Flying Clocks in the 1960’s • Starting in 1964 with HP 5060A • Portable transistorized cesium clock • Hundreds of clock trips • Remote synchronization to µs levels • See HP Journals: 1964, 65, 66, 67 • 1965 world-wide time synchronization • Paved the way for flying clock relativity experiments in the 1970’s 06-Dec-2006 Project GREAT 9 Relativity and Clocks • High-level summary: – Clocks run slower if they move at high velocity (SR) – Clocks run slower in the presence of greater gravity (GR) – Clocks lose time traveling East (Sagnac) •This implies: – According to general relativity, stationary clocks on mountains run faster. -
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.