Early Period

Total Page:16

File Type:pdf, Size:1020Kb

Early Period Miranda, AzelAnn T. 2PSY01 Foreign Physicists Early Period 1544-1603 William Gilbert hypothesized that the Earth is a giant magnet English 1564-1642 Galileo Galilei performed fundamental observations, experiments, and mathematical Italian analyses in astronomy and physics; discovered mountains and craters on the moon, the phases of Venus, and the four largest satellites of Jupiter: Io, Europa, Callisto, and Ganymede 1580-1626 Willebrod Snell discovered law of refraction (Snell's law) Dutch 1623-1662 Blaise Pascal discovered that pressure applied to an enclosed fluid is transmitted French undiminished to every part of the fluid and to the walls of its container (Pascal's principle) 1629-1695 Christiaan Huygens proposed a simple geometrical wave theory of light, now known as Dutch ``Huygen's principle''; pioneered use of the pendulum in clocks 1635-1703 Robert Hooke discovered Hooke's law of elasticity English 1643-1727 Sir Isaac Newton developed theories of gravitation and mechanics, and invented English differential calculus 1700-1782 Daniel Bernoulli developed the fundamental relationship of fluid flow now known as Swiss Bernoulli's principle 1706-1790 Benjamin Franklin the first American physicist; characterized two kinds of electric charge, American which he named ``positive'' and ``negative'' 1707-1783 Leonard Euler made fundamental contributions to fluid dynamics, lunar orbit theory Swiss (tides), and mechanics; also contributed prolifically to all areas of classical mathematics 1731-1810 Henry Cavendish discovered and studied hydrogen; first to measure Newton's gravitational British constant; calculated mass and mean density of Earth 1736-1806 Charles Augustin de experiments on elasticity, electricity, and magnetism; established French Coulomb experimentally nature of the force between two charges 1736-1813 Joseph-Louis developed new methods of analytical mechanics French Lagrange 1736-1819 James Watt invented the modern condensing steam engine and a centrifugal Scottish governor 1745-1827 Count Alessandro pioneer in study of electricity; invented the first electric battery Italian Volta 1768-1830 Joseph Fourier established the differential equation governing heat diffusion and solved French it by devising an infinite series of sines and cosines capable of approximating a wide variety of functions 1773-1829 Thomas Young studied light and color; known for his double-slit experiment that British demonstrated the wave nature of light 1774-1862 Jean-Babtiste Biot studied polarization of light; co-discovered that intensity of magnetic field French set up by a current flowing through a wire varies inversely with the distance from the wire 1775-1836 André Marie Ampère father of electrodynamics French 1776-1856 Amadeo Avogadro developed hypothesis that all gases at same volume, pressure, and Italian temperature contain same number of atoms 1777-1855 Johann Carl Friedrich formulated separate electrostatic and electrodynamical laws, including German Gauss ``Gauss' law''; contributed to development of number theory, differential geometry, potential theory, theory of terrestrial magnetism, and methods of calculating planetary orbits 1777-1851 Hans Christian discovered that a current in a wire can produce magnetic effects Danish Oersted 1781-1868 Sir David Brewster deduced ``Brewster's law'' giving the angle of incidence that produces English reflected light which is completely polarized; invented the kaleidoscope and the stereoscope, and improved the spectroscope 1788-1827 Augustin-Jean studied transverse nature of light waves French Fresnel 1789-1854 Georg Ohm discovered that current flow is proportional to potential difference and German inversely proportional to resistance (Ohm's law) 1791-1867 Michael Faraday discovered electromagnetic induction and devised first electrical English transformer 1791-1841 Felix Savart co-discovered that intensity of magnetic field set up by a current flowing French through a wire varies inversely with the distance from the wire 1796-1832 Sadi Carnot founded the science of thermodynamics French 1797-1878 Joseph Henry performed extensive fundamental studies of electromagnetic American phenomena; devised first practical electric motor Middle Period 1803-1853 Christian Doppler experimented with sound waves; derived an expression for the apparent Austrian change in wavelength of a wave due to relative motion between the source and observer 1804-1891 Wilhelm E. Weber developed sensitive magnetometers; worked in electrodynamics and the German electrical structure of matter 1805-1865 Sir William Hamilton developed the principle of least action and the Hamiltonian form of Irish classical mechanics 1818-1889 James Prescott Joule discovered mechanical equivalent of heat British 1819-1896 Armand-Hippolyte- made the first terrestrial measurement of the speed of light; invented French Louis Fizeau one of the first interferometers; took the first pictures of the Sun on daguerreotypes; argued that the Doppler effect with respect to sound should also apply to any wave motion, particularly that of light 1819-1868 Jean-Bernard-Léon accurately measured speed of light; invented the gyroscope; French Foucault demonstrated the Earth's rotation 1819-1903 Sir George Gabriel described the motion of viscous fluids by independently discovering the British Stokes Navier-Stokes equations of fluid mechanics (or hydrodynamics); developed Stokes theorem by which certain surface integrals may be reduced to line integrals; discovered fluorescence 1821-1894 Hermann von developed first law of thermodynamics, a statement of conservation of German Helmholtz energy 1822-1888 Rudolf Clausius developed second law of thermodynamics, a statement that the entropy German of the Universe always increases 1824-1907 Lord Kelvin proposed absolute temperature scale, of essence to development of British (born William thermodynamics Thomson) 1824-1887 Gustav Kirchhoff developed three laws of spectral analysis and three rules of electric circuit German analysis; also contributed to optics 1825-1898 Johann Balmer developed empirical formula to describe hydrogen spectrum Swiss 1828-1914 Sir Joseph Wilson developed a carbon-filament incandescent light; patented the carbon British Swan process for printing photographs in permanent pigment 1831-1879 James Clerk Maxwell propounded the theory of electromagnetism; developed the kinetic Scottish theory of gases 1835-1893 Josef Stefan studied blackbody radiation Austrian 1838-1916 Ernst Mach studied conditions that occur when an object moves through a fluid at Austrian high speed (the ``Mach number'' gives the ratio of the speed of the object to the speed of sound in the fluid); proposed ``Mach's principle,'' which states that the inertia of an object is due to the interaction between the object and the rest of the universe 1839-1903 Josiah Gibbs developed chemical thermodynamics; introduced concepts of free energy American and chemical potential 1842-1923 James Dewar liquified nitrogen and invented the Dewar flask, which is critical for low- British temperature work 1842-1912 Osborne Reynolds contributed to the fields of hydraulics and hydrodynamics; developed British mathematical framework for turbulence and introduced the ``Reynolds number,'' which provides a criterion for dynamic similarity and correct modeling in many fluid-flow experiments 1844-1906 Ludwig Boltzmann developed statistical mechanics and applied it to kinetic theory of gases Austrian 1848-1919 Roland Eötvös demonstrated equivalence of gravitational and inertial mass Hungarian 1850-1925 Oliver Heaviside contributed to the development of electromagnetism; introduced English operational calculus and invented the modern notation for vector calculus; predicted existence of the Heaviside layer (a layer of the Earth's ionosphere) 1851-1901 George Francis hypothesized foreshortening of moving bodies (Lorentz-FitzGerald Irish FitzGerald contraction) to explain the result of the Michelson-Morley experiment 1852-1914 John Henry Poynting demonstrated that the energy flow of electromagnetic waves could be British calculated by an equation (now called Poynting's vector) 1854-1912 Henri Poincaré founded qualitative dynamics (the mathematical theory of dynamical French systems); created topology; contributed to solution of the three-body problem; first described many properties of deterministic chaos; contributed to the development of special relativity 1854-1919 Janne Rydberg analyzed the spectra of many elements; discovered many line series were Swedish described by a formula that depended on a universal constant (the Rydberg constant) 1855-1938 Edwin H. Hall discovered the ``Hall effect,'' which occurs when charge carriers moving American through a material are deflected because of an applied magnetic field - the deflection results in a potential difference across the side of the material that is transverse to both the magnetic field and the current direction 1857-1894 Heinrich Hertz worked on electromagnetic phenomena; discovered radio waves and the German photoelectric effect 1857-1943 Nikola Tesla created alternating current (Serbian-born American) 1837-1923 Johannes van der worked on equations of state for gases and liquids Dutch Waals 1842-1919 Lord Rayleigh discovered argon; explained how light scattering is responsible for red British (born John William color of sunset and blue color of sky Strutt) 1845-1923 Wilhelm Röntgen discovered and studied x rays German 1852-1908 Antoine Henri discovered natural radioactivity French Becquerel 1852-1931
Recommended publications
  • Measurements of Elastic Electron-Proton Scattering at Large Momentum Transfer*
    SLAC-PUB-4395 Rev. January 1993 m Measurements of Elastic Electron-Proton Scattering at Large Momentum Transfer* A. F. SILL,(~) R. G. ARNOLD,P. E. BOSTED,~. C. CHANG,@) J. GoMEz,(~)A. T. KATRAMATOU,C. J. MARTOFF, G. G. PETRATOS,(~)A. A. RAHBAR,S. E. ROCK,AND Z. M. SZALATA Department of Physics The American University, Washington DC 20016 D.J. SHERDEN Stanford Linear Accelerator Center , Stanford University, Stanford, California 94309 J. M. LAMBERT Department of Physics Georgetown University, Washington DC 20057 and R. M. LOMBARD-NELSEN De’partemente de Physique Nucle’aire CEN Saclay, Gif-sur- Yvette, 91191 Cedex, France Submitted to Physical Review D *Work supported by US Department of Energy contract DE-AC03-76SF00515 (SLAC), and National Science Foundation Grants PHY83-40337 and PHY85-10549 (American University). R. M. Lombard-Nelsen was supported by C. N. R. S. (French National Center for Scientific Research). Javier Gomez was partially supported by CONICIT, Venezuela. (‘)Present address: Department of Physics and Astronomy, University of Rochester, NY 14627. (*)Permanent address: Department of Physics and Astronomy, University of Maryland, College Park, MD 20742. (C)Present address: Continuous Electron Beam Accelerator Facility, Newport News, VA 23606. (d)Present address: Temple University, Philadelphia, PA 19122. (c)Present address: Stanford Linear Accelerator Center, Stanford CA 94309. ABSTRACT Measurements of the forward-angle differential cross section for elastic electron-proton scattering were made in the range of momentum transfer from Q2 = 2.9 to 31.3 (GeV/c)2 using an electron beam at the Stanford Linear Accel- erator Center. The data span six orders of magnitude in cross section.
    [Show full text]
  • 2007 Abstracts Und Curricula Bewusstsein Und Quantencomputer
    BEWUSSTSEIN UND QUANTENCOMPUTER CONSCIOUSNESS AND QUANTUMCOMPUTERS ______________________________________________________________ 7. SCHWEIZER BIENNALE ZU WISSENSCHAFT, TECHNIK + ÄSTHETIK THE 7th SWISS BIENNIAL ON SCIENCE, TECHNICS + AESTHETICS 20. / 21. Januar 2007 / January 20 - 21, 2007 Verkehrshaus der Schweiz, Luzern Swiss Museum of Transport, Lucerne Veranstalter: Neue Galerie Luzern, www.neugalu.ch Organized by: New Gallery Lucerne, www.neugalu.ch ______________________________________________________________ A B S T R A C T S Samstag, 20. Januar 2007 / Saturday, January 20, 2007 Verkehrshaus der Schweiz / Swiss Museum of Transport Keynote 12.15 - 12.45 BRIAN JOSEPHSON Quantenphysik Cambridge / UK IS QUANTUM MECHANICS OR COMPUTATION MORE FUNDAMENTAL? IST DIE QUANTENMECHANIK ODER DAS RECHNEN FUNDAMENTALER? Is quantum mechanics as currently conceived the ultimate theory of nature? In his book "Atomic Physics and Human Knowledge", Niels Bohr argued that because of the uncertainty principle quantum methodology might not be applicable to the study of the ultimate details of life. Delbruck disagreed, claiming that biosystems are robust to quantum disturbances, an assertion that is only partially valid rendering Bohr's argument still significant, even though normally ignored. The methods of the quantum physicist and of the biological sciences can be seen to involve two alternative approaches to the understanding of nature that can usefully complement each other, neither on its own containing the full story. That full story, taking into
    [Show full text]
  • James Clerk Maxwell
    James Clerk Maxwell JAMES CLERK MAXWELL Perspectives on his Life and Work Edited by raymond flood mark mccartney and andrew whitaker 3 3 Great Clarendon Street, Oxford, OX2 6DP, United Kingdom Oxford University Press is a department of the University of Oxford. It furthers the University’s objective of excellence in research, scholarship, and education by publishing worldwide. Oxford is a registered trade mark of Oxford University Press in the UK and in certain other countries c Oxford University Press 2014 The moral rights of the authors have been asserted First Edition published in 2014 Impression: 1 All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, without the prior permission in writing of Oxford University Press, or as expressly permitted by law, by licence or under terms agreed with the appropriate reprographics rights organization. Enquiries concerning reproduction outside the scope of the above should be sent to the Rights Department, Oxford University Press, at the address above You must not circulate this work in any other form and you must impose this same condition on any acquirer Published in the United States of America by Oxford University Press 198 Madison Avenue, New York, NY 10016, United States of America British Library Cataloguing in Publication Data Data available Library of Congress Control Number: 2013942195 ISBN 978–0–19–966437–5 Printed and bound by CPI Group (UK) Ltd, Croydon, CR0 4YY Links to third party websites are provided by Oxford in good faith and for information only.
    [Show full text]
  • Rutherford's Nuclear World: the Story of the Discovery of the Nuc
    Rutherford's Nuclear World: The Story of the Discovery of the Nuc... http://www.aip.org/history/exhibits/rutherford/sections/atop-physic... HOME SECTIONS CREDITS EXHIBIT HALL ABOUT US rutherford's explore the atom learn more more history of learn about aip's nuclear world with rutherford about this site physics exhibits history programs Atop the Physics Wave ShareShareShareShareShareMore 9 RUTHERFORD BACK IN CAMBRIDGE, 1919–1937 Sections ← Prev 1 2 3 4 5 Next → In 1962, John Cockcroft (1897–1967) reflected back on the “Miraculous Year” ( Annus mirabilis ) of 1932 in the Cavendish Laboratory: “One month it was the neutron, another month the transmutation of the light elements; in another the creation of radiation of matter in the form of pairs of positive and negative electrons was made visible to us by Professor Blackett's cloud chamber, with its tracks curled some to the left and some to the right by powerful magnetic fields.” Rutherford reigned over the Cavendish Lab from 1919 until his death in 1937. The Cavendish Lab in the 1920s and 30s is often cited as the beginning of modern “big science.” Dozens of researchers worked in teams on interrelated problems. Yet much of the work there used simple, inexpensive devices — the sort of thing Rutherford is famous for. And the lab had many competitors: in Paris, Berlin, and even in the U.S. Rutherford became Cavendish Professor and director of the Cavendish Laboratory in 1919, following the It is tempting to simplify a complicated story. Rutherford directed the Cavendish Lab footsteps of J.J. Thomson. Rutherford died in 1937, having led a first wave of discovery of the atom.
    [Show full text]
  • Quantum Theory of the Hydrogen Atom
    Quantum Theory of the Hydrogen Atom Chemistry 35 Fall 2000 Balmer and the Hydrogen Spectrum n 1885: Johann Balmer, a Swiss schoolteacher, empirically deduced a formula which predicted the wavelengths of emission for Hydrogen: l (in Å) = 3645.6 x n2 for n = 3, 4, 5, 6 n2 -4 •Predicts the wavelengths of the 4 visible emission lines from Hydrogen (which are called the Balmer Series) •Implies that there is some underlying order in the atom that results in this deceptively simple equation. 2 1 The Bohr Atom n 1913: Niels Bohr uses quantum theory to explain the origin of the line spectrum of hydrogen 1. The electron in a hydrogen atom can exist only in discrete orbits 2. The orbits are circular paths about the nucleus at varying radii 3. Each orbit corresponds to a particular energy 4. Orbit energies increase with increasing radii 5. The lowest energy orbit is called the ground state 6. After absorbing energy, the e- jumps to a higher energy orbit (an excited state) 7. When the e- drops down to a lower energy orbit, the energy lost can be given off as a quantum of light 8. The energy of the photon emitted is equal to the difference in energies of the two orbits involved 3 Mohr Bohr n Mathematically, Bohr equated the two forces acting on the orbiting electron: coulombic attraction = centrifugal accelleration 2 2 2 -(Z/4peo)(e /r ) = m(v /r) n Rearranging and making the wild assumption: mvr = n(h/2p) n e- angular momentum can only have certain quantified values in whole multiples of h/2p 4 2 Hydrogen Energy Levels n Based on this model, Bohr arrived at a simple equation to calculate the electron energy levels in hydrogen: 2 En = -RH(1/n ) for n = 1, 2, 3, 4, .
    [Show full text]
  • Harry Truman, the Atomic Bomb and the Apocalyptic Narrative
    Volume 5 | Issue 7 | Article ID 2479 | Jul 12, 2007 The Asia-Pacific Journal | Japan Focus The Decision to Risk the Future: Harry Truman, the Atomic Bomb and the Apocalyptic Narrative Peter J. Kuznick The Decision to Risk the Future: Harry stressed that the future of mankind would be Truman, the Atomic Bomb and theshaped by how such bombs were used and Apocalyptic Narrative subsequently controlled or shared.[3] Truman recalled Stimson “gravely” expressing his Peter J. Kuznick uncertainty about whether the U.S. should ever use the bomb, “because he was afraid it was so I powerful that it could end up destroying the whole world.” Truman admitted that, listening In his personal narrative Atomic Quest, Nobel to Stimson and Groves and reading Groves’s Prize-winning physicist Arthur Holly Compton, accompanying memo, he “felt the same who directed atomic research at the University fear.”[4] of Chicago’s Metallurgical Laboratory during the Second World War, tells of receiving an urgent visit from J. Robert Oppenheimer while vacationing in Michigan during the summer of 1942. Oppenheimer and the brain trust he assembled had just calculated the possibility that an atomic explosion could ignite all the hydrogen in the oceans or the nitrogen in the atmosphere. If such a possibility existed, Compton concluded, “these bombs must never be made.” As Compton said, “Better to accept the slavery of the Nazis than to run a chance of drawing the final curtain on mankind.”[1] Certainly, any reasonable human being could be expected to respond similarly. Three years later, with Hitler dead and the Nazis defeated, President Harry Truman faced Truman and Byrnes en route to Potsdam, July a comparably weighty decision.
    [Show full text]
  • Atomic Physics & Quantum Effects
    KEY CONCEPTS ATOMIC PHYSICS & QUANTUM EFFECTS 1. PHOTONS & THE PHOTOELECTRIC EFFECT Max Planck explained blackbody radiation with his quantum hypothesis, which states that the energy of a thermal oscillator, Eosc, is not continuous, but instead is a discrete quantity given by the equation: Eosc = nhf n = 1, 2, 3,... where f is the frequency and h is a constant now known as Planck’s constant. Albert Einstein extended the idea by adding that all emitted radiation is quantized. He suggested that light is composed of discrete quanta, rather than of waves. According to his theory, each particle of light, known as a photon, has an energy E given by: E = hf Einstein’s theory helped him explain a phenomenon known as the photoelectric effect, in which a photon of light strikes a photosensitive material and causes an electron to be ejected from the material. A photocell constructed from photosensitive material can produce an electrical current when light shines on it. The kinetic energy, K, of a photoelectron displaced by a photon of energy, hf, is given by: K = hf - φ where the work function, φ, is the minimum energy needed to free the electron from the photosensitive material. No photoemission occurs if the frequency of the incident light falls below a certain cutoff frequency – or threshold frequency – given by: φ f0 = h Einstein's theory explained several aspects of the photoelectric effect that could not be explained by classical theory: • The kinetic energy of photoelectrons is dependent on the light’s frequency. • No photoemission occurs for light below a certain threshold frequency.
    [Show full text]
  • Wolfgang Pauli Niels Bohr Paul Dirac Max Planck Richard Feynman
    Wolfgang Pauli Niels Bohr Paul Dirac Max Planck Richard Feynman Louis de Broglie Norman Ramsey Willis Lamb Otto Stern Werner Heisenberg Walther Gerlach Ernest Rutherford Satyendranath Bose Max Born Erwin Schrödinger Eugene Wigner Arnold Sommerfeld Julian Schwinger David Bohm Enrico Fermi Albert Einstein Where discovery meets practice Center for Integrated Quantum Science and Technology IQ ST in Baden-Württemberg . Introduction “But I do not wish to be forced into abandoning strict These two quotes by Albert Einstein not only express his well­ more securely, develop new types of computer or construct highly causality without having defended it quite differently known aversion to quantum theory, they also come from two quite accurate measuring equipment. than I have so far. The idea that an electron exposed to a different periods of his life. The first is from a letter dated 19 April Thus quantum theory extends beyond the field of physics into other 1924 to Max Born regarding the latter’s statistical interpretation of areas, e.g. mathematics, engineering, chemistry, and even biology. beam freely chooses the moment and direction in which quantum mechanics. The second is from Einstein’s last lecture as Let us look at a few examples which illustrate this. The field of crypt­ it wants to move is unbearable to me. If that is the case, part of a series of classes by the American physicist John Archibald ography uses number theory, which constitutes a subdiscipline of then I would rather be a cobbler or a casino employee Wheeler in 1954 at Princeton. pure mathematics. Producing a quantum computer with new types than a physicist.” The realization that, in the quantum world, objects only exist when of gates on the basis of the superposition principle from quantum they are measured – and this is what is behind the moon/mouse mechanics requires the involvement of engineering.
    [Show full text]
  • 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]
  • Rydberg Constant and Emission Spectra of Gases
    Page 1 of 10 Rydberg constant and emission spectra of gases ONE WEIGHT RECOMMENDED READINGS 1. R. Harris. Modern Physics, 2nd Ed. (2008). Sections 4.6, 7.3, 8.9. 2. Atomic Spectra line database https://physics.nist.gov/PhysRefData/ASD/lines_form.html OBJECTIVE - Calibrating a prism spectrometer to convert the scale readings in wavelengths of the emission spectral lines. - Identifying an "unknown" gas by measuring its spectral lines wavelengths. - Calculating the Rydberg constant RH. - Finding a separation of spectral lines in the yellow doublet of the sodium lamp spectrum. INSTRUCTOR’S EXPECTATIONS In the lab report it is expected to find the following parts: - Brief overview of the Bohr’s theory of hydrogen atom and main restrictions on its application. - Description of the setup including its main parts and their functions. - Description of the experiment procedure. - Table with readings of the vernier scale of the spectrometer and corresponding wavelengths of spectral lines of hydrogen and helium. - Calibration line for the function “wavelength vs reading” with explanation of the fitting procedure and values of the parameters of the fit with their uncertainties. - Calculated Rydberg constant with its uncertainty. - Description of the procedure of identification of the unknown gas and statement about the gas. - Calculating resolution of the spectrometer with the yellow doublet of sodium spectrum. INTRODUCTION In this experiment, linear emission spectra of discharge tubes are studied. The discharge tube is an evacuated glass tube filled with a gas or a vapor. There are two conductors – anode and cathode - soldered in the ends of the tube and connected to a high-voltage power source outside the tube.
    [Show full text]
  • Neutron Scattering
    Neutron Scattering Basic properties of neutron and electron neutron electron −27 −31 mass mkn =×1.675 10 g mke =×9.109 10 g charge 0 e spin s = ½ s = ½ −e= −e= magnetic dipole moment µnn= gs with gn = 3.826 µee= gs with ge = 2.0 2mn 2me =22k 2π =22k Ek== E = 2m λ 2m energy n e 81.81 150.26 Em[]eV = 2 Ee[]V = 2 λ ⎣⎡Å⎦⎤ λ ⎣⎦⎡⎤Å interaction with matter: Coulomb interaction — 9 strong-force interaction 9 — magnetic dipole-dipole 9 9 interaction Several salient features are apparent from this table: – electrons are charged and experience strong, long-range Coulomb interactions in a solid. They therefore typically only penetrate a few atomic layers into the solid. Electron scattering is therefore a surface-sensitive probe. Neutrons are uncharged and do not experience Coulomb interaction. The strong-force interaction is naturally strong but very short-range, and the magnetic interaction is long-range but weak. Neutrons therefore penetrate deeply into most materials, so that neutron scattering is a bulk probe. – Electrons with wavelengths comparable to interatomic distances (λ ~2Å ) have energies of several tens of electron volts, comparable to energies of plasmons and interband transitions in solids. Electron scattering is therefore well suited as a probe of these high-energy excitations. Neutrons with λ ~2Å have energies of several tens of meV , comparable to the thermal energies kTB at room temperature. These so-called “thermal neutrons” are excellent probes of low-energy excitations such as lattice vibrations and spin waves with energies in the meV range.
    [Show full text]
  • “Kings of Cool” Superconductivity Who Are These People? SUPERCONDUCTORS
    “““Kings of Cool” Superconductivity Who are these people? SUPERCONDUCTORS An Introduction by Prof George Walmsley Normal conductor eg copper • Current, I. • Voltage drop, V. • Resistance, R = ? • Ans: V/I = R eg 2 Volts/1 Amp = 2 Ohms I Copper I V Normal conductor eg copper • Source of resistance: • Electron collides with lattice ion to produce heat (phonon). Copper lattice Lower Temperature • What happens when we cool a metal? • Ans 1: The electrons slow down and current is reduced maybe to zero. R→∞ • Ans 2: The lattice stops vibrating and resistance disappears. R=0 How do we cool things? • Commonly used liquid refrigerants: Element Boiling Pt Oxygen 90K Nitrogen 77K Hydrogen 20K Helium 4.2K Thomas Andrews, Chemist • 9 Dec 1813 – 26 Nov 1885 • John (Flax spinner, Comber) [ggfather] • Michael (Linen, Ardoyne) [gfather] • Thomas (Linen merchant) [father] • Studied under James Thomson, RBAI • 1828 Univ of Glasgow, Thos Thomson • 1830 Paris, Dumas • 1830-34 Trinity College Dublin • 1835 MD U of Edinburgh • 1835-45 Prof of Chemistry RBAI • 1845 Vice-President, Queen’s College • 1847 Prof of Chemistry, Queen’s College • 1869 Bakerian Lecture on CO 2 • 1871 Visit by Dr Janssen of Leiden • Photo: Paris 1875 Andrews’ Isotherms • Note critical temperature NORMAL CONDUCTOR: Electrical properties Normal metal eg copper Resistance and (resistivity, ρ) >0 As temperature falls ρ falls smoothly too: ρ 0 100 200 273.15 Temperature/K SUPERCONDUCTOR: Electrical properties Superconductor eg mercury, lead Resistivity ( ρ) >0 like normal metal down to critical
    [Show full text]