ESI NEWS Volume 3, Issue 2, Autumn 2008

Total Page:16

File Type:pdf, Size:1020Kb

ESI NEWS Volume 3, Issue 2, Autumn 2008 The Erwin Schrodinger¨ International Boltzmanngasse 9/2 Institute for Mathematical Physics A-1090 Vienna, Austria ESI NEWS Volume 3, Issue 2, Autumn 2008 Editorial final report of the evaluation was sent to the Austrian Ministry of Science in June 2008. Contents Klaus Schmidt Apart from praising the quality of the Editorial 1 programmes which had taken place at the The 15th anniversary Nobel Prize in Physics 2008 2 ESI during the past five years, he review the ESI in April 2008 panel noted that the Institute had ‘gen- Metastability and Rare Events in was an occasion not tly and wisely’ increased its scope of the Complex Systems 4 only for celebration, programmes in recent years, into areas of but also for an evalu- pure mathematics more remote at present Josef Stefan, Josef Loschmidt and ation of the Institute’s Stigler’s Law 7 from theoretical physics, and into areas of performance over the physics and biology beyond those usually Remarks on Boltzmann’s Philoso- past 5 years and its characterized as mathematical physics. The phy 8 scope for future development. panel felt that this process should be con- The previous evaluation of the ESI ESI News 12 tinued in the same judicious fashion as in in 2003 had been chaired by Nigel recent years. Current and Future Activities of Hitchin (Oxford), who had recruited as The report also contains a number of the ESI 13 co-evaluators Robbert Dijkgraaf (Ams- terdam), Jurgen¨ Jost (Leipzig), Nicolai recommendations for the development of Schrodinger¨ Lectures 2008/2009 15 Reshetikhin (Berkeley) and Vincent Ri- the ESI over the next years. These pro- posals and their financial implications are Senior Research Fellows’ Lecture vasseau (Orsay). currently under further discussion with the Courses 2008/2009 15 The evaluation in 2008 followed essen- tially the same pattern: Peter Goddard (IAS University of Vienna and the Austrian Min- Workshop on Mathematics at the Princeton) agreed to chair the evaluation istry of Science. Turn of the 20th Century 15 and chose for his panel of co-evaluators Jean-Michel Bismut (Orsay), Robbert Di- On behalf of the Erwin Schrodinger¨ In- jkgraaf (Amsterdam), Felix Otto (Bonn) stitute I would like to send seasons greet- and Scott Sheffield (Courant Institute). Af- ings and my best wishes for a happy and ter a site visit by the panel in April 2008 the peaceful year 2009. EVALUATION OF THE ESI, APRIL 2008 The scientific directors of the ESI, Joachim Schwermer and Jakob Yngvason, together with the evaluators Peter Goddard (IAS Princeton, chair), Scott Sheffield (Courant Institute), Jean-Michel Bismut (Orsay) and Felix Otto (Bonn) – from left to right. 2 Volume 3, Issue 2, Autumn 2008 ESI NEWS Nobel Prize in Physics Till the middle of the last century, symme- The main inspiration for Nambu came try principles were thought to express the from the BCS theory of superconductivity 2008: Symmetry Violation basic simplicity of nature. The discovery [2]. In certain metals, the electron-phonon in Subatomic Physics that some of the “sacred” symmetries such interaction can lead to the formation of as parity (P), time reversal or charge con- Cooper pairs (two electrons with opposite Gerhard Ecker and Walter Grimus jugation (C) were only approximate came momenta and spins) that condense in the therefore as a surprise. In his Nobel Lec- ground state. The ground state is there- tures of 1979 Weinberg expressed this feel- fore charged implying the spontaneous vi- The No- ing as a question: “Is nature only approxi- olation of gauge invariance. In an impor- bel Prize in mately simple?” By now there is a general tant paper [3], Nambu demonstrated that Physics 2008 consensus that also approximate symme- gauge invariance, although not manifest in was awarded tries may reveal fundamental properties of the BCS theory, is nevertheless fully main- to Yoichiro nature. For instance, CP violation is essen- tained. Nambu (Enrico tial for the baryon asymmetry of the uni- That was the starting point for Nambu Fermi Institute, verse and thus for our existence [1]. and Jona-Lasinio to investigate the struc- Chicago, USA) for “the discovery of the Symmetries in particle physics can be clas- ture of the ground state in relativistic mechanism of spontaneous broken symme- sified in four groups: quantum field theories relevant for parti- try in subatomic physics” and to Makoto cle physics. The Lagrangian of the Nambu– Kobayashi (KEK, Tsukuba, Japan) and 1. Exact symmetries leave the field Jona-Lasinio (NJL) model [4] Toshihide Maskawa (Yukawa Institute for equations and the ground state µ Theoretical Physics, Kyoto, Japan) for “the of the theory invariant. Examples LNJL = γ i@µ + are the Poincare´ transformations discovery of the origin of the broken sym- metry which predicts the existence of at (Lorentz transformations and space- g0 − γ5 γ5 time translations) and the gauge least three families of quarks in nature.” describes the self-interaction of a single nu- symmetries of electromagnetic and cleon field and is modeled after the BCS strong interactions. Symmetries in physics Lagrangian. Because of the absence of a The modern view of symmetries as groups 2. Spontaneously broken symmetries mass term m the Lagrangian and the of transformations that leave the equations still leave the field equations invari- field equations are invariant with respect of motion invariant emerges in the 19th ant, but not the ground state. Nambu to two independent phase transformations century. With the advent of quantum me- was the first to realize the impor- (chiral symmetry) chanics in the 1920s, symmetries were tance of this concept in relativistic (x) ! eiα (x); (x) ! eiβγ5 (x) : found to explain degeneracies in spectra quantum field theories. Examples are and to give rise to relations between mea- the chiral symmetry of the strong in- Depending on the size of the coupling surable quantities such as cross sections teractions (in the limit of vanishing constant g , the ground state of the the- and decay rates. In addition to the classical 0 quark masses) and the electroweak ory may exhibit spontaneous breakdown of space-time symmetries (Galilei, Poincare),´ gauge symmetry. the chiral symmetry, generating both a fi- a new type of symmetries occurs in quan- nite mass for the initially massless nucleon tum field theories: the so-called “internal” 3. Approximate symmetries do not and a massless collective excitation (pion). symmetries do not affect space and time even leave the field equations in- The modern version of the NJL model but they transform the fields of the theory. variant, but traces of the symme- is Quantum Chromodynamics (QCD), the The gauge symmetries of the fundamental tries are still visible in measurable gauge theory of quarks and gluons for the interactions are prominent examples. quantities. Symmetries violated only strong interaction. Chiral symmetry holds by the weak interactions (P, CP, Symmetries play an important role in sub- for massless quarks, which is a good ap- strangeness, . ) are of this type. atomic physics: proximation for the two lightest quarks Kobayashi and Maskawa received u; d. Spontaneous breaking of chiral sym- i. Unlike gravitational and electromag- the Nobel Prize for their explanation metry provides the only plausible expla- netic forces, nuclear forces are re- of CP violation in the SM. nation why pions are by far the lightest mote from our everyday experience. hadrons. From the study of spectra and other 4. Anomalous symmetries leave the observables, physicists extract clues classical field equations invariant, In the NJL model, most of the nucleon for underlying symmetries to be but are violated by quantum effects. mass arises from spontaneous chiral sym- implemented in the corresponding metry breaking. According to our present quantum field theories. Spontaneous symmetry breaking understanding, the small u and d masses The notion of spontaneous symmetry contribute actually only about 5% to the ii. Theoretical physics often proceeds breaking originated in solid state physics. nucleon mass. In other words, 95% of our by analogies and extrapolations: ex- For example, the Hamiltonian describing a mass and of the visible universe are due to tending the gauge symmetry of the ferromagnet is rotationally invariant in the the strong quark-gluon interaction in QCD. electromagnetic interaction to the absence of an external magnetic field, yet Only the small remainder requires a differ- weak and strong interactions led the ground state exhibits spontaneous mag- ent mechanism for mass generation. to the modern theory of the fun- netization along some arbitrary direction: Inspired by the work of Nambu and Jona- damental interactions, the Standard rotational symmetry is spontaneously bro- Lasinio, Goldstone demonstrated [5] that Model (SM) of particle physics. ken in the ferromagnet. spontaneously broken symmetries lead to Erwin Schrodinger¨ Institute of Mathematical Physics http://www.esi.ac.at/ ESI NEWS Volume 3, Issue 2, Autumn 20083 massless excitations in general. In the case V–A (vector minus axial vector current) Hamiltonian density is given by of so-called global symmetries (e.g., chi- theory of weak interactions in which both ral symmetries), these excitations would be P and C are maximally violated. Hcc = massless particles (pions for mu = md = g µ + In the V–A theory, CP was conserved in p u¯γ (1 − γ5)V d W + H.c. ; 0). As shown a few years later by Brout µ a natural way. Therefore, the discovery 2 2 and Englert [6] and by Higgs [7], the situ- + of the decay K ! π+π− in 1964 at where W is the W-boson field, g is the ation is different for gauge symmetries (lo- L the Brookhaven National Laboratory [8], SU(2) gauge coupling constant and u and cal symmetries): the Nambu-Goldstone ex- a manifestation of CP violation, was com- d are the column vectors containing the citations are not physical particles but they pletely unanticipated and provided a new quark fields with charge 2=3 and −1=3, re- render some of the initially massless gauge puzzlement which did not diminish with spectively.
Recommended publications
  • Ludwig Boltzmann Was Born in Vienna, Austria. He Received His Early Education from a Private Tutor at Home
    Ludwig Boltzmann (1844-1906) Ludwig Boltzmann was born in Vienna, Austria. He received his early education from a private tutor at home. In 1863 he entered the University of Vienna, and was awarded his doctorate in 1866. His thesis was on the kinetic theory of gases under the supervision of Josef Stefan. Boltzmann moved to the University of Graz in 1869 where he was appointed chair of the department of theoretical physics. He would move six more times, occupying chairs in mathematics and experimental physics. Boltzmann was one of the most highly regarded scientists, and universities wishing to increase their prestige would lure him to their institutions with high salaries and prestigious posts. Boltzmann himself was subject to mood swings and he joked that this was due to his being born on the night between Shrove Tuesday and Ash Wednesday (or between Carnival and Lent). Traveling and relocating would temporarily provide relief from his depression. He married Henriette von Aigentler in 1876. They had three daughters and two sons. Boltzmann is best known for pioneering the field of statistical mechanics. This work was done independently of J. Willard Gibbs (who never moved from his home in Connecticut). Together their theories connected the seemingly wide gap between the macroscopic properties and behavior of substances with the microscopic properties and behavior of atoms and molecules. Interestingly, the history of statistical mechanics begins with a mathematical prize at Cambridge in 1855 on the subject of evaluating the motions of Saturn’s rings. (Laplace had developed a mechanical theory of the rings concluding that their stability was due to irregularities in mass distribution.) The prize was won by James Clerk Maxwell who then went on to develop the theory that, without knowing the individual motions of particles (or molecules), it was possible to use their statistical behavior to calculate properties of a gas such as viscosity, collision rate, diffusion rate and the ability to conduct heat.
    [Show full text]
  • Chapter 1 the Biography of a Trafficking Material
    Trafficking Materials and Maria Rentetzi Gendered Experimental Practices Chapter 1 The Biography of a Trafficking Material In 1904, an article titled "Radium and Radioactivity" appeared in Century 1 Magazine, a monthly popular magazine published from 1881 to 1930. The article presents Marie Curie's personal account of the discovery of radium and radioactivity. In the article, Curie discusses in depth her arduous attempts to study the radiation of the compounds of uranium and that of known chemical elements, hoping to discover more which are endowed with atomic radioactivity. She revels that it was the chemists who supplied her with the materials she needed. "As I desired to make a very thorough investigation, I had resource to different chemists, who put at my disposal specimens—in some cases the only ones in existence—containing very rare elements." Her next step was to examine different minerals, especially the oxide of uranium 2 ore (pitchblende). To her great surprise, this specimen was found to be four times more active than oxide of uranium itself. The explanation was more than obvious. "The ore must contain a substance more radioactive than uranium and thorium, and this substance must necessarily be a chemical element as yet unknown."1 Her attempts to isolate the new element would lead Marie and Pierre Curie, who joined her research shortly after, to the discovery of both polonium and radium, to the Nobel Prize in Physics in 1903, and to a second Nobel Prize in 1911, this time in chemistry. This chapter attempts to present a cultural
    [Show full text]
  • Light and the Electromagnetic Spectrum
    © Jones & Bartlett Learning, LLC © Jones & Bartlett Learning, LLC NOT FOR SALE OR DISTRIBUTION NOT FOR SALE OR DISTRIBUTION © Jones & Bartlett Learning, LLC © Jones & Bartlett Learning, LLC NOT FOR SALE OR DISTRIBUTION NOT FOR SALE OR DISTRIBUTION © Jones & Bartlett Learning, LLC © Jones & Bartlett Learning, LLC NOT FOR SALE OR DISTRIBUTION NOT FOR SALE OR DISTRIBUTION © Jones & Bartlett Learning, LLC © Jones & Bartlett Learning, LLC NOT FOR SALE OR DISTRIBUTION NOT FOR SALE OR DISTRIBUTION © Jones & Bartlett Learning, LLC © Jones & Bartlett Learning, LLC NOT FOR SALE OR DISTRIBUTION NOT FOR SALE OR DISTRIBUTION © JonesLight & Bartlett and Learning, LLCthe © Jones & Bartlett Learning, LLC NOTElectromagnetic FOR SALE OR DISTRIBUTION NOT FOR SALE OR DISTRIBUTION4 Spectrum © Jones & Bartlett Learning, LLC © Jones & Bartlett Learning, LLC NOT FOR SALEJ AMESOR DISTRIBUTIONCLERK MAXWELL WAS BORN IN EDINBURGH, SCOTLANDNOT FOR IN 1831. SALE His ORgenius DISTRIBUTION was ap- The Milky Way seen parent early in his life, for at the age of 14 years, he published a paper in the at 10 wavelengths of Proceedings of the Royal Society of Edinburgh. One of his first major achievements the electromagnetic was the explanation for the rings of Saturn, in which he showed that they con- spectrum. Courtesy of Astrophysics Data Facility sist of small particles in orbit around the planet. In the 1860s, Maxwell began at the NASA Goddard a study of electricity© Jones and & magnetismBartlett Learning, and discovered LLC that it should be possible© Jones Space & Bartlett Flight Center. Learning, LLC to produce aNOT wave FORthat combines SALE OR electrical DISTRIBUTION and magnetic effects, a so-calledNOT FOR SALE OR DISTRIBUTION electromagnetic wave.
    [Show full text]
  • Kerne, Kooperation Und Konkurrenz. Kernforschung In
    Wissenschaft, Macht und Kultur in der modernen Geschichte Herausgegeben von Mitchell G. Ash und Carola Sachse Band 3 Silke Fengler Kerne, Kooperation und Konkurrenz Kernforschung in Österreich im internationalen Kontext (1900–1950) 2014 Böhlau Verlag Wien Köln Weimar The research was funded by the Austrian Science Fund (FWF) : P 19557-G08 Bibliografische Information der Deutschen Nationalbibliothek: Die Deutsche Nationalbibliothek verzeichnet diese Publikation in der Deutschen Nationalbibliografie; detaillierte bibliografische Datensind im Internet über http://dnb.d-nb.de abrufbar. Umschlagabbildung: Zusammentreffen in Hohenholte bei Münster am 18. Mai 1932 anlässlich der 37. Hauptversammlung der deutschen Bunsengesellschaft für angewandte physikalische Chemie in Münster (16. bis 19. Mai 1932). Von links nach rechts: James Chadwick, Georg von Hevesy, Hans Geiger, Lili Geiger, Lise Meitner, Ernest Rutherford, Otto Hahn, Stefan Meyer, Karl Przibram. © Österreichische Zentralbibliothek für Physik, Wien © 2014 by Böhlau Verlag Ges.m.b.H & Co. KG, Wien Köln Weimar Wiesingerstraße 1, A-1010 Wien, www.boehlau-verlag.com Alle Rechte vorbehalten. Dieses Werk ist urheberrechtlich geschützt. Jede Verwertung außerhalb der engen Grenzen des Urheberrechtsgesetzes ist unzulässig. Lektorat: Ina Heumann Korrektorat: Michael Supanz Umschlaggestaltung: Michael Haderer, Wien Satz: Michael Rauscher, Wien Druck und Bindung: Prime Rate kft., Budapest Gedruckt auf chlor- und säurefrei gebleichtem Papier Printed in Hungary ISBN 978-3-205-79512-4 Inhalt 1. Kernforschung in Österreich im Spannungsfeld von internationaler Kooperation und Konkurrenz ....................... 9 1.1 Internationalisierungsprozesse in der Radioaktivitäts- und Kernforschung : Eine Skizze ...................... 9 1.2 Begriffsklärung und Fragestellungen ................. 10 1.2.2 Ressourcenausstattung und Ressourcenverteilung ......... 12 1.2.3 Zentrum und Peripherie ..................... 14 1.3 Forschungsstand ........................... 16 1.4 Quellenlage .............................
    [Show full text]
  • Arxiv:Quant-Ph/0510180V1 24 Oct 2005 Einstein and the Quantum
    TIFR/TH/05-39 27.9.2005 Einstein and the Quantum Virendra Singh Tata Institute of Fundamental Research Homi Bhabha Road, Mumbai 400 005, India Abstract We review here the main contributions of Einstein to the quantum theory. To put them in perspective we first give an account of Physics as it was before him. It is followed by a brief account of the problem of black body radiation which provided the context for Planck to introduce the idea of quantum. Einstein’s revolutionary paper of 1905 on light-quantum hypothesis is then described as well as an application of this idea to the photoelectric effect. We next take up a discussion of Einstein’s other contributions to old quantum theory. These include (i) his theory of specific heat of solids, which was the first application of quantum theory to matter, (ii) his discovery of wave-particle duality for light and (iii) Einstein’s A and B coefficients relating to the probabilities of emission and absorption of light by atomic systems and his discovery of radiation stimulated emission of light which provides the basis for laser action. We then describe Einstein’s contribution to quantum statistics viz Bose- Einstein Statistics and his prediction of Bose-Einstein condensation of a boson gas. Einstein played a pivotal role in the discovery of Quantum mechanics and this is briefly mentioned. After 1925 Einstein’s contributed mainly to the foundations of Quantum Mechanics. We arXiv:quant-ph/0510180v1 24 Oct 2005 choose to discuss here (i) his Ensemble (or Statistical) Interpretation of Quantum Mechanics and (ii) the discovery of Einstein-Podolsky-Rosen (EPR) correlations and the EPR theorem on the conflict between Einstein-Locality and the completeness of the formalism of Quantum Mechanics.
    [Show full text]
  • 1 Historical Background
    1 Historical Background 1.1 Introduction The purpose of this chapter is to explain how and why Planck introduced his famous quantum hypothesis and the constant h. I have added a few contributions from Einstein that are relevant for this book. We shall see that results based on the wave nature of light alternate with results based on its corpuscular nature. Eventually, it will be Planck’s constant that will bridge the gap between these two viewpoints and lead to the foundation of quantum physics, unifying the two aspects of light, and much more. But first a warning! This chapter is difficult to read because we are no longer used to thinking and reasoning along the same lines as our prede- cessors. Still, I think that it is of interest to follow the chain that started with Kirchhoff’s second law and ended with Planck’s hypothesis of quan- tized emission of radiation, using the tools available in their time. It gives a flavor of what physics was at that time. It also shows how much we have progressed since then. 1.2 Kirchhoff (1859) 1.2.1 The Birth of Spectroscopy The physicist Kirchhoff1 was collaborating with the chemist Bunsen2 (Fig. 1.1). Out of this collaboration emerged the science of spectroscopy. An early discovery was the phenomenon of spectral line inversion. The experiment is displayed schematically in Fig. 1.2. 1Gustav Robert Kirchhoff (b. Königsberg, 1824; d. Berlin, 1887). 2Robert Wilhelm Bunsen (b. Göttingen, 1811; d. Heidelberg, 1899). Nonlinear Optics: An Analytic Approach. Paul Mandel Copyright © 2010 Wiley-VCH Verlag GmbH & Co.
    [Show full text]
  • Ht2009-88060
    Proceedings HT 2009 2009 ASME Summer Heat Transfer Conference July 19-23, 2009, San Francisco, California USA HT2009-88060 A BRIEF HISTORY OF THE T4 RADIATION LAW John Crepeau University of Idaho Department of Mechanical Engineering PO Box 440902 Moscow, ID 83844-0902 USA ABSTRACT he combined his Displacement Law with the T4 law to give a Since the 1700s, natural philosophers understood that heat blackbody spectrum which was accurate over some ranges, but exchange between two bodies was not precisely linearly diverged in the far infrared. dependent on the temperature difference, and that at high Max Planck, at the University of Berlin, built on temperatures the discrepancy became greater. Over the years, Wien’s model but, as Planck himself stated, “the energy of many models were developed with varying degrees of success. radiation is distributed in a completely irregular manner among The lack of success was due to the difficulty obtaining accurate the individual partial vibrations...” This “irregular” or discrete experimental data, and a lack of knowledge of the fundamental treatment of the radiation became the basis for quantum mechanisms underlying radiation heat exchange. Josef Stefan, mechanics and a revolution in physics. of the University of Vienna, compiled data taken by a number This paper will present brief biographies of the four of researchers who used various methods to obtain their data, pillars of the T4 radiation law, Stefan, Boltzmann, Wien and and in 1879 proposed a unique relation to model the Planck, and outline the methodologies used to obtain their dependence of radiative heat exchange on the temperature: the results.
    [Show full text]
  • Chapter 1 Blackbody Radiation
    Chapter 1 Blackbody Radiation Experiment objectives: explore radiation from objects at certain temperatures, commonly known as \blackbody radiation"; make measurements testing the Stefan-Boltzmann law in high- and low-temperature ranges; measure the inverse-square law for thermal radiation. Theory A familiar observation to us is that dark-colored objects absorb more thermal radiation (from the sun, for example) than light-colored objects. You may have also observed that a good absorber of radiation is also a good emitter (like dark-colored seats in an automobile). Although we observe thermal radiation (\heat") mostly through our sense of touch, the range of energies at which the radiation is emitted can span the visible spectrum (thus we speak of high-temperature objects being \red hot" or \white hot"). For temperatures below about 600◦C, however, the radiation is emitted in the infrared, and we cannot see it with our eyes, although there are special detectors (like the one you will use in this lab) that can measure it. An object which absorbs all radiation incident on it is known as an \ideal blackbody". In 1879 Josef Stefan found an empirical relationship between the power per unit area radiated by a blackbody and the temperature, which Ludwig Boltzmann derived theoretically a few years later. This relationship is the Stefan-Boltzmann law: S = σT 4 (1.1) where S is the radiated power per unit area (W=m2), T is the temperature (in Kelvins), and σ = 5:6703 × 10−8W=m2K4 is the Stefan's constant. Most hot, opaque objects can be approximated as blackbody emitters, but the most ideal blackbody is a closed volume (a cavity) with a very small hole in it.
    [Show full text]
  • Chronological Table for the Development of Atomic and Molecular Physics
    Chronological Table for the Development of Atomic and Molecular Physics ≈ 440 Empedocles assumes, that the whole world is constant proportions”: Each chemical element BC composed of 4 basic elements: Fire, Water, Air consists of equal atoms which form with sim- and Soil. ple number ratios molecules as building blocks ≈ 400 Leucippos and his disciple Democritus claim, of chemical compounds. BC that the world consists of small indivisible 1811 Amedeo Avogadro derives from the laws particles, called atoms, which are stable and of Gay-Lussac (Δp/p = ΔT/T ) and Boyle- nondestructable. Marriot (p · V = constant for T = constant) ≈ 360 Plato attributes four regular regular geometric the conclusion that all gases contain under BC structures composed of triangles and squares equal conditions (pressure and temperature) (Platonic bodies) to the four elements and the same number of particles per volume. postulates that these structures and their inter- 1820 John Herapath publishes his conception of a change represent the real building blocks of the Kinetic theory of gases. world. 1857 Rudolf J.E. Clausius develops further the ki- ≈ 340 Aristotle contradicts the atomic theory and as- netic gas theory, founded by J. Herapath and BC sumes that the mater is continuous and does D. Bernoulli. not consist of particles. 1860 Gustav Robert Kirchhoff and Robert Bunsen 300 Epicurus revives the atomic model and as- create the foundations of spectral analysis of BC sumes that the atoms have weight and spatial the chemical elements. extension. 1865 Joseph Lohschmidt calculates the absolute 200 BC no real progress in atomic physics. number of molecules contained in 1 cm3 of –1600 AC a gas under normal conditions (p = 1atm, 1661 Robert Boyle fights in his book: “The Sceptical T = 300 K).
    [Show full text]
  • The Short History of Science
    PHYSICS FOUNDATIONS SOCIETY THE FINNISH SOCIETY FOR NATURAL PHILOSOPHY PHYSICS FOUNDATIONS SOCIETY THE FINNISH SOCIETY FOR www.physicsfoundations.org NATURAL PHILOSOPHY www.lfs.fi Dr. Suntola’s “The Short History of Science” shows fascinating competence in its constructively critical in-depth exploration of the long path that the pioneers of metaphysics and empirical science have followed in building up our present understanding of physical reality. The book is made unique by the author’s perspective. He reflects the historical path to his Dynamic Universe theory that opens an unparalleled perspective to a deeper understanding of the harmony in nature – to click the pieces of the puzzle into their places. The book opens a unique possibility for the reader to make his own evaluation of the postulates behind our present understanding of reality. – Tarja Kallio-Tamminen, PhD, theoretical philosophy, MSc, high energy physics The book gives an exceptionally interesting perspective on the history of science and the development paths that have led to our scientific picture of physical reality. As a philosophical question, the reader may conclude how much the development has been directed by coincidences, and whether the picture of reality would have been different if another path had been chosen. – Heikki Sipilä, PhD, nuclear physics Would other routes have been chosen, if all modern experiments had been available to the early scientists? This is an excellent book for a guided scientific tour challenging the reader to an in-depth consideration of the choices made. – Ari Lehto, PhD, physics Tuomo Suntola, PhD in Electron Physics at Helsinki University of Technology (1971).
    [Show full text]
  • In Honour of Marie Sklodowska-Curie
    health and prosperity throughout the world". It will continue to "ensure, so far as it is able, that assistance provided by it or at its request or under its super­ vision or control is not used in such a way as to further any military purpose". IN HONOUR OF MARIE SKLODOWSKA-CURIE This year marks the hundredth anniversary of the birth in Poland of Marie Sklodowska-Curie, originator of the word "radioactivity", whose early research in the subject has had far-reaching consequences for the nuclear sciences. The Government of Poland's arrangements for marking the occasion include an international symposium, restoration of her house in Warsaw, publications and films, and the Agency is happy to collaborate. This article from a distinguished Austrian scientist indicates how her work was carried out in an atmosphere of co-operation between scientists of many nations. By Dr. Berta Karlik (The author has been since 1945 Director of the Institute for Radium Research and Nuclear Physics, Austrian Academy of Sciences, where she succeeded Professor Stefan Meyer. A graduate of Vienna Uni­ versity and member of a number of learned societies, she has produced many scienti­ fic papers, including one published in 1944 dealing with the occurrence in nature of element 85, Astatine. This element was the last in the atomic table to be identified and occurs naturally only in minute quantities. It was first produced artificially by E.C.Segre, D.R.Corson and K.R.Mac- Kenzie in 1940 at the University of Cali­ fornia). The fact that the International Atomic Energy Agency has established its headquarters in Vienna prompts one to consider briefly, on the occasion of the 100th anniversary of Marie Curie's birth, the important part played by 18 Austria, and particularly by the Academy of Sciences in Vienna, in the dis­ coveries of this great scientist and in the further development of her work.
    [Show full text]
  • Timeline: “Modern” Physics 450-300 BC Leucippus, Democritos, Epicurus
    Timeline: “Modern” Physics 450-300 BC Leucippus, Democritos, Epicurus . Greek Atomists: 335 BC Aristotle continuous elements (earth, air, fire, water) 300 BC Zeno of Cition (founder of Stoics) popularizes Aristotelian view. 60 BC Titus Lucretius Carus of Rome epitomizes “Atomist” philosophy. 1879 Josef Stefan [expt] power emitted as blackbody radiation P = AσT 4 1884 Ludwig Boltzmann [theor] explains Stefan’s empirical law 1885 Johann Jakob Balmer [expt] empirical description of line spectra emitted by H atoms 1890 Johannes Robert Rydberg [expt] 1893 Wilhelm Wien [expt] blackbody spectrum displacement law: peak wavelength varies as T −1 1895 Wilhelm Conrad Roentgen [expt] discovers X-rays 1897 Joseph John Thomson [expt] measures boldmath q/m of the electron 1900 Max Planck [theor] derives correct blackbody radiation spectrum 1902 Philipp E.A. von Lenard [expt] measures photoelectric effect 1905 Albert Einstein [theor] explains photoelectric effect 1905 Albert Einstein [theor] publishes Special Theory of Relativity (STR) 1905 Albert Einstein [theor] explains Brownian motion (gives mass of atoms!) 1905 Ernest Rutherford [expt] performs first alpha-scattering experiments at McGill Univ. (Canada) 1907 Robert A. Milliken [expt] measures electron charge (now know both qe and me). 1912 William (H. & L.) Bragg [expt] shows that X-rays scatter off crystal lattices 1913 Hans Geiger & Ernest Marsden [expt] confirm Rutherford scattering results at Univ. of Manchester (U.K.) 1913 Niels Henrik David Bohr [theor] pictures H atom with quantized angular momentum
    [Show full text]