Nobel Laureate Prof Eric Cornell's Visit to SPMS
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Fotonica Ed Elettronica Quantistica
Fotonica ed elettronica quantistica http://www.dsf.unica.it/~fotonica/teaching/fotonica.html Fotonica ed elettronica quantistica Quantum optics - Quantization of electromagnetic field - Statistics of light, photon counting and noise; - HBT and correlation; g1 e g2 coherence; antibunching; single photons - Squeezing - Quantum cryptography - Quantum computer, entanglement and teleportation Light-matter Interaction - Two-level atom - Laser physics - Spectroscopy - Electronics and photonics at the nanometer scale - Cold atoms - Photodetectors - Solar cells http://www.dsf.unica.it/~fotonica/teaching/fotonica.html Energy Temperature LHC at CERN, Higgs, SUSY, ??? TeV 15 q q particle accelerators 10 K q GeV proton rest mass - quarks 1012K MeV electron rest mass / gamma rays 109K keV Nuclear Fusion, x rays, Sun center 106K Atoms ionize - visible light eV Sun surface fundamental components components fundamental room temperature 103K meV Liquid He, superconductors, space 1K dilution refrigerators, quantum Hall µeV laser-cooled atoms 10-3K neV Bose-Einstein condensates 10-6K peV low T record 480 picokelvin 10-9K -12 complexity, organization organization complexity, 10 K Nobel Prizes in Physics 2010 - Andre Geims, Konstantin Novoselov 2009 - Charles K. Kao, Willard S. Boyle, George E. Smith 2007 - Albert Fert, Peter Gruenberg 2005 - Roy J. Glauber, John L. Hall, Theodor W. Hänsch 2001 - Eric A. Cornell, Wolfgang Ketterle, Carl E. Wieman 1997 - Steven Chu, Claude Cohen-Tannoudji, William D. Phillips 1989 - Norman F. Ramsey, Hans G. Dehmelt, Wolfgang Paul 1981 - Nicolaas Bloembergen, Arthur L. Schawlow, Kai M. Siegbahn 1966 - Alfred Kastler 1964 - Charles H. Townes, Nicolay G. Basov, Aleksandr M. Prokhorov 1944 - Isidor Isaac Rabi 1930 - Venkata Raman 1921 - Albert Einstein 1907 - Albert A. -
Nobel Laureates Endorse Joe Biden
Nobel Laureates endorse Joe Biden 81 American Nobel Laureates in Physics, Chemistry, and Medicine have signed this letter to express their support for former Vice President Joe Biden in the 2020 election for President of the United States. At no time in our nation’s history has there been a greater need for our leaders to appreciate the value of science in formulating public policy. During his long record of public service, Joe Biden has consistently demonstrated his willingness to listen to experts, his understanding of the value of international collaboration in research, and his respect for the contribution that immigrants make to the intellectual life of our country. As American citizens and as scientists, we wholeheartedly endorse Joe Biden for President. Name Category Prize Year Peter Agre Chemistry 2003 Sidney Altman Chemistry 1989 Frances H. Arnold Chemistry 2018 Paul Berg Chemistry 1980 Thomas R. Cech Chemistry 1989 Martin Chalfie Chemistry 2008 Elias James Corey Chemistry 1990 Joachim Frank Chemistry 2017 Walter Gilbert Chemistry 1980 John B. Goodenough Chemistry 2019 Alan Heeger Chemistry 2000 Dudley R. Herschbach Chemistry 1986 Roald Hoffmann Chemistry 1981 Brian K. Kobilka Chemistry 2012 Roger D. Kornberg Chemistry 2006 Robert J. Lefkowitz Chemistry 2012 Roderick MacKinnon Chemistry 2003 Paul L. Modrich Chemistry 2015 William E. Moerner Chemistry 2014 Mario J. Molina Chemistry 1995 Richard R. Schrock Chemistry 2005 K. Barry Sharpless Chemistry 2001 Sir James Fraser Stoddart Chemistry 2016 M. Stanley Whittingham Chemistry 2019 James P. Allison Medicine 2018 Richard Axel Medicine 2004 David Baltimore Medicine 1975 J. Michael Bishop Medicine 1989 Elizabeth H. Blackburn Medicine 2009 Michael S. -
Having a Good Time: a Triumph of Science & Technology
UDC’s Office of Research & Graduate Studies, SEAS, LSAMP, & STEM Center Invite You to a Seminar on Having a Good Time: A Triumph of Science & Technology Presented by Dr. William D. Phillips, NIST Nobel Laureate in Physics, 1997 © Robert Rathe © Robert Rathe Date: Tuesday, March 13, 2012 Time: 12:30 PM Location: Building 41-A03 Abstract: People have long been interested in timekeeping. In the 18th century, this interest became particularly keen because of technological demands: the need for accurate navigation on the high seas. While many people believed that the answer to sufficiently good timekeeping at sea would be found in astronomical measurements, it was earthbound engineering that literally won the prize. The construction of accurate seagoing clocks revolutionized navigation in the 18th and 19th centuries. The advent of even more accurate clocks—atomic clocks—in the 20th century gave birth to a new revolution in navigation—the Global Positioning System. This ever-more advanced system for satellite navigation owes its success both to excellent engineering and to seemingly arcane science. Dr. William D. Phillips is a Senior Fellow at the National Institute of Standards and Technology (NIST), where he leads the Laser Cooling and Trapping Group. He shared the 1997 Nobel Prize in physics with Dr. Steven Chu, now Secretary of Energy, and with Dr. Claude Cohen-Tannoudji, an Algerian-born French physicist, “for development of methods to cool and trap atoms with laser light.” With a physics bachelor’s degree from Juniata College in Pennsylvania and a Ph.D. from MIT, Phillips started his career at NIST only a few years after it left UDC’s Van Ness campus for its location in Gaithersburg. -
Advances in Theoretical & Computational Physics
ISSN: 2639-0108 Research Article Advances in Theoretical & Computational Physics Supreme Theory of Everything Ulaanbaatar Tarzad *Corresponding author Ulaanbaatar Tarzad, Department of Physics, School of Applied Sciences, Department of Physics, School of Applied Sciences, Mongolian Mongolian University of Science and Technology, Ulaanbaatar, Mongolia, University of Science and Technology E-mail: [email protected] Submitted: 27 Mar 2019; Accepted: 24 Apr 2019; Published: 06 June 2019 Abstract Not only universe, but everything has general characters as eternal, infinite, cyclic and wave-particle duality. Everything from elementary particles to celestial bodies, from electromagnetic wave to gravity is in eternal motions, which dissects only to circle. Since everything is described only by trigonometry. Without trigonometry and mathematical circle, the science cannot indicate all the beauty of harmonic universe. Other method may be very good, but it is not perfect. Some part is very nice, another part is problematic. General Theory of Relativity holds that gravity is geometric. Quantum Mechanics describes all particles by wave function of trigonometry. In this paper using trigonometry, particularly mathematics circle, a possible version of the unification of partial theories, evolution history and structure of expanding universe, and the parallel universes are shown. Keywords: HRD, Trigonometry, Projection of Circle, Singularity, The reality of universe describes by geometry, because of that not Celestial Body, Black Hole and Parallel Universes. only gravity is geometrical, but everything is it and nothing is linear. One of the important branches of geometry is trigonometry dealing Introduction with circle and triangle. For this reason, it is easier to describe nature Today scientists describe the universe in terms of two basic partial of universe by mathematics circle. -
Nobel Lectures™ 2001-2005
World Scientific Connecting Great Minds 逾10 0 种 诺贝尔奖得主著作 及 诺贝尔奖相关图书 我们非常荣幸得以出版超过100种诺贝尔奖得主著作 以及诺贝尔奖相关图书。 我们自1980年代开始与诺贝尔奖得主合作出版高品质 畅销书。一些得主担任我们的编辑顾问、丛书编辑, 并于我们期刊发表综述文章与学术论文。 世界科技与帝国理工学院出版社还邀得其中多位作了公 开演讲。 Philip W Anderson Sir Derek H R Barton Aage Niels Bohr Subrahmanyan Chandrasekhar Murray Gell-Mann Georges Charpak Nicolaas Bloembergen Baruch S Blumberg Hans A Bethe Aaron J Ciechanover Claude Steven Chu Cohen-Tannoudji Leon N Cooper Pierre-Gilles de Gennes Niels K Jerne Richard Feynman Kenichi Fukui Lawrence R Klein Herbert Kroemer Vitaly L Ginzburg David Gross H Gobind Khorana Rita Levi-Montalcini Harry M Markowitz Karl Alex Müller Sir Nevill F Mott Ben Roy Mottelson 诺贝尔奖相关图书 THE PERIODIC TABLE AND A MISSED NOBEL PRIZES THAT CHANGED MEDICINE NOBEL PRIZE edited by Gilbert Thompson (Imperial College London) by Ulf Lagerkvist & edited by Erling Norrby (The Royal Swedish Academy of Sciences) This book brings together in one volume fifteen Nobel Prize- winning discoveries that have had the greatest impact upon medical science and the practice of medicine during the 20th “This is a fascinating account of how century and up to the present time. Its overall aim is to groundbreaking scientists think and enlighten, entertain and stimulate. work. This is the insider’s view of the process and demands made on the Contents: The Discovery of Insulin (Robert Tattersall) • The experts of the Nobel Foundation who Discovery of the Cure for Pernicious Anaemia, Vitamin B12 assess the originality and significance (A Victor Hoffbrand) • The Discovery of -
The Discovery of Asymptotic Freedom
The Discovery of Asymptotic Freedom The 2004 Nobel Prize in Physics, awarded to David Gross, Frank Wilczek, and David Politzer, recognizes the key discovery that explained how quarks, the elementary constituents of the atomic nucleus, are bound together to form protons and neutrons. In 1973, Gross and Wilczek, working at Princeton, and Politzer, working independently at Harvard, showed that the attraction between quarks grows weaker as the quarks approach one another more closely, and correspondingly that the attraction grows stronger as the quarks are separated. This discovery, known as “asymptotic freedom,” established quantum chromodynamics (QCD) as the correct theory of the strong nuclear force, one of the four fundamental forces in Nature. At the time of the discovery, Wilczek was a 21-year-old graduate student working under Gross’s supervision at Princeton, while Politzer was a 23-year-old graduate student at Harvard. Currently Gross is the Director of the Kavli Institute for Theoretical Physics at the University of California at Santa Barbara, and Wilczek is the Herman Feshbach Professor of Physics at MIT. Politzer is Professor of Theoretical Physics at Caltech; he joined the Caltech faculty in 1976. Of the four fundamental forces --- the others besides the strong nuclear force are electromagnetism, the weak nuclear force (responsible for the decay of radioactive nuclei), and gravitation --- the strong force was by far the most poorly understood in the early 1970s. It had been suggested in 1964 by Caltech physicist Murray Gell-Mann that protons and neutrons contain more elementary objects, which he called quarks. Yet isolated quarks are never seen, indicating that the quarks are permanently bound together by powerful nuclear forces. -
Advanced Information on the Nobel Prize in Physics, 5 October 2004
Advanced information on the Nobel Prize in Physics, 5 October 2004 Information Department, P.O. Box 50005, SE-104 05 Stockholm, Sweden Phone: +46 8 673 95 00, Fax: +46 8 15 56 70, E-mail: [email protected], Website: www.kva.se Asymptotic Freedom and Quantum ChromoDynamics: the Key to the Understanding of the Strong Nuclear Forces The Basic Forces in Nature We know of two fundamental forces on the macroscopic scale that we experience in daily life: the gravitational force that binds our solar system together and keeps us on earth, and the electromagnetic force between electrically charged objects. Both are mediated over a distance and the force is proportional to the inverse square of the distance between the objects. Isaac Newton described the gravitational force in his Principia in 1687, and in 1915 Albert Einstein (Nobel Prize, 1921 for the photoelectric effect) presented his General Theory of Relativity for the gravitational force, which generalized Newton’s theory. Einstein’s theory is perhaps the greatest achievement in the history of science and the most celebrated one. The laws for the electromagnetic force were formulated by James Clark Maxwell in 1873, also a great leap forward in human endeavour. With the advent of quantum mechanics in the first decades of the 20th century it was realized that the electromagnetic field, including light, is quantized and can be seen as a stream of particles, photons. In this picture, the electromagnetic force can be thought of as a bombardment of photons, as when one object is thrown to another to transmit a force. -
Reversed out (White) Reversed
Berkeley rev.( white) Berkeley rev.( FALL 2014 reversed out (white) reversed IN THIS ISSUE Berkeley’s Space Sciences Laboratory Tabletop Physics Bringing More Women into Physics ALUMNI NEWS AND MORE! Cover: The MAVEN satellite mission uses instrumentation developed at UC Berkeley's Space Sciences Laboratory to explore the physics behind the loss of the Martian atmosphere. It’s a continuation of Berkeley astrophysicist Robert Lin’s pioneering work in solar physics. See p 7. photo credit: Lockheed Martin Physics at Berkeley 2014 Published annually by the Department of Physics Steven Boggs: Chair Anil More: Director of Administration Maria Hjelm: Director of Development, College of Letters and Science Devi Mathieu: Editor, Principal Writer Meg Coughlin: Design Additional assistance provided by Sarah Wittmer, Sylvie Mehner and Susan Houghton Department of Physics 366 LeConte Hall #7300 University of California, Berkeley Berkeley, CA 94720-7300 Copyright 2014 by The Regents of the University of California FEATURES 4 12 18 Berkeley’s Space Tabletop Physics Bringing More Women Sciences Laboratory BERKELEY THEORISTS INVENT into Physics NEW WAYS TO SEARCH FOR GOING ON SIX DECADES UC BERKELEY HOSTS THE 2014 NEW PHYSICS OF EDUCATION AND SPACE WEST COAST CONFERENCE EXPLORATION Berkeley theoretical physicists Ashvin FOR UNDERGRADUATE WOMEN Vishwanath and Surjeet Rajendran IN PHYSICS Since the Space Lab’s inception are developing new, small-scale in 1959, Berkeley physicists have Women physics students from low-energy approaches to questions played important roles in many California, Oregon, Washington, usually associated with large-scale of the nation’s space-based scientific Alaska, and Hawaii gathered on high-energy particle experiments. -
Yang-Mills Theory, Lattice Gauge Theory and Simulations
Yang-Mills theory, lattice gauge theory and simulations David M¨uller Institute of Analysis Johannes Kepler University Linz [email protected] May 22, 2019 1 Overview Introduction and physical context Classical Yang-Mills theory Lattice gauge theory Simulating the Glasma in 2+1D 2 Introduction and physical context 3 Yang-Mills theory I Formulated in 1954 by Chen Ning Yang and Robert Mills I A non-Abelian gauge theory with gauge group SU(Nc ) I A non-linear generalization of electromagnetism, which is a gauge theory based on U(1) I Gauge theories are a widely used concept in physics: the standard model of particle physics is based on a gauge theory with gauge group U(1) × SU(2) × SU(3) I All fundamental forces (electromagnetism, weak and strong nuclear force, even gravity) are/can be formulated as gauge theories 4 Classical Yang-Mills theory Classical Yang-Mills theory refers to the study of the classical equations of motion (Euler-Lagrange equations) obtained from the Yang-Mills action Main topic of this seminar: solving the classical equations of motion of Yang-Mills theory numerically Not topic of this seminar: quantum field theory, path integrals, lattice quantum chromodynamics (except certain methods), the Millenium problem related to Yang-Mills . 5 Classical Yang-Mills in the early universe 6 Classical Yang-Mills in the early universe Electroweak phase transition: the electro-weak force splits into the weak nuclear force and the electromagnetic force This phase transition can be studied using (extensions of) classical Yang-Mills theory Literature: I G. D. -
Weyl Spinors and the Helicity Formalism
Weyl spinors and the helicity formalism J. L. D´ıazCruz, Bryan Larios, Oscar Meza Aldama, Jonathan Reyes P´erez Facultad de Ciencias F´ısico-Matem´aticas, Benem´erita Universidad Aut´onomade Puebla, Av. San Claudio y 18 Sur, C. U. 72570 Puebla, M´exico Abstract. In this work we give a review of the original formulation of the relativistic wave equation for parti- cles with spin one-half. Traditionally (`ala Dirac), it's proposed that the \square root" of the Klein-Gordon (K-G) equation involves a 4 component (Dirac) spinor and in the non-relativistic limit it can be written as 2 equations for two 2 component spinors. On the other hand, there exists Weyl's formalism, in which one works from the beginning with 2 component Weyl spinors, which are the fundamental objects of the helicity formalism. In this work we rederive Weyl's equations directly, starting from K-G equation. We also obtain the electromagnetic interaction through minimal coupling and we get the interaction with the magnetic moment. As an example of the use of that formalism, we calculate Compton scattering using the helicity methods. Keywords: Weyl spinors, helicity formalism, Compton scattering. PACS: 03.65.Pm; 11.80.Cr 1 Introduction One of the cornerstones of contemporary physics is quantum mechanics, thanks to which great advances in the comprehension of nature at the atomic, and even subatomic level have been achieved. On the other hand, its applications have given place to a whole new technological revolution. Thus, the study of quantum physics is part of our scientific culture. -
Electroweak Symmetry Breaking (Historical Perspective)
Electroweak Symmetry Breaking (Historical Perspective) 40th SLAC Summer Institute · 2012 History is not just a thing of the past! 2 Symmetry Indistinguishable before and after a transformation Unobservable quantity would vanish if symmetry held Disorder order = reduced symmetry 3 Symmetry Bilateral Translational, rotational, … Ornamental Crystals 4 Symmetry CsI Fullerene C60 ball and stick created from a PDB using Piotr Rotkiewicz's [http://www.pirx.com/iMol/ iMol]. {{gfdl}} Source: English Wikipedia, 5 Symmetry (continuous) 6 Symmetry matters. 7 8 Symmetries & conservation laws Spatial translation Momentum Time translation Energy Rotational invariance Angular momentum QM phase Charge 9 Symmetric laws need not imply symmetric outcomes. 10 symmetries of laws ⇏ symmetries of outcomes by Wilson Bentley, via NOAA Photo Library Photo via NOAA Wilson Bentley, by Studies among the Snow Crystals ... CrystalsStudies amongSnow the ... 11 Broken symmetry is interesting. 12 Two-dimensional Ising model of ferromagnet http://boudin.fnal.gov/applet/IsingPage.html 13 Continuum of degenerate vacua 14 Nambu–Goldstone bosons V Betsy Devine Yoichiro Nambu �� 2 Massless NG boson 1 Massive scalar boson NGBs as spin waves, phonons, pions, … Jeffrey Goldstone 15 Symmetries imply forces. I: scale symmetry to unify EM, gravity Hermann Weyl (1918, 1929) 16 NEW Complex phase in QM ORIGINAL Global: free particle Local: interactions 17 Maxwell’s equations; QED massless spin-1 photon coupled to conserved charge no impediment to electron mass (eL & eR have same charge) James Clerk Maxwell (1861/2) 18 19 QED Fermion masses allowed Gauge-boson masses forbidden Photon mass term 1 2 µ 2 mγ A Aµ violates gauge invariance: AµA (Aµ ∂µΛ) (A ∂ Λ) = AµA µ ⇥ − µ − µ ⇤ µ Massless photon predicted 22 observed: mγ 10− me 20 Symmetries imply forces. -
Standard Model of Particle Physics, Or Beyond?
Standard Model of Particle Physics, or Beyond? Mariano Quir´os High Energy Phys. Inst., BCN (Spain) ICTP-SAIFR, November 13th, 2019 Outline The outline of this colloquium is I Standard Model: reminder I Electroweak interactions I Strong interactions I The Higgs sector I Experimental successes I Theoretical and observational drawbacks I Beyond the Standard Model I Supersymmetry I Large extra dimensions I Warped extra dimensions/composite Higgs I Concluding remarks Disclaimer: I will not discuss any technical details. With my apologies to my theorist (and experimental) colleagues The Standard Model: reminder I The knowledge of the Standard Model of strong and electroweak interactions requires (as any other physical theory) the knowledge of I The elementary particles or fields (the characters of the play) I How particles interact (their behavior) The characters of the play I Quarks: spin-1/2 fermions I Leptons: spin-1/2 fermions I Higgs boson: spin-0 boson I Carriers of the interactions: spin-1 (gauge) bosons I All these particles have already been discovered and their mass, spin, and charge measured \More in detail the characters of the play" - Everybody knows the Periodic Table of the Elements - Compare elementary particles with some (of course composite) very heavy nuclei What are the interactions between the elementary building blocks of the Standard Model? I Interactions are governed by a symmetry principle I The more symmetric the theory the more couplings are related (the less of them they are) and the more predictive it is Strong interactions: