Robert Harry Kraichnan Scient Undergraduate Thesis, “Quantum Several Years, and Strong Evidence Has

Total Page:16

File Type:pdf, Size:1020Kb

Robert Harry Kraichnan Scient Undergraduate Thesis, “Quantum Several Years, and Strong Evidence Has witty presentations of quantum me- Theory of the Linear Gravitational chromodynamics and quantum gravity. chanics and quantum field theory. Field”; he received a PhD from MIT in Kraichnan’s field-theoretic approach to Some of his legendary lectures were 1949 for his thesis, “Relativistic Scatter- nonequilibrium quantum statistical recorded for posterity; others were ing of Pseudoscalar Mesons by Nucle- mechanics is equivalent to the formal- saved as lecture notes by diligent stu- ons,” supervised by Herman Feshbach. ism developed by Julian Schwinger and dents so that their successors might He was one of Albert Einstein’s last as- Leonid Keldysh around the same time. have a taste of Sidney’s inimitable style. sistants at the Institute for Advanced In the late 1950s, Kraichnan tackled In 2005 Harvard hosted a festival to Study in Princeton, New Jersey, in the famously difficult subject of fluid honor Sidney. In attendance were many 1949–50. Kraichnan developed an ap- turbulence. He became a world leader of his former students and many dis- proach to gravitation that started from on the subject and drove major devel- tinguished physicists. Steven Weinberg the linear wave equation of a spin-2 opments for a remarkable 40-year span remarked that “Sidney is a theorist’s massless particle and recovered nonlin- beginning around 1957. For many theorist. He has not been so much con- ear general relativity by a bootstrap. workers in fluid turbulence, it was cerned with accounting for the latest His viewpoint is now popular among enough to say “Bob said. .” In 1962 data from experiments as with under- high-energy physicists, but Einstein Kraichnan decided on an unusual ca- standing deeply what our theories re- viewed it with disfavor. Some of reer path, leaving academia and setting ally mean. I can say I learned more Kraichnan’s ideas were rediscovered by up his own scientific consulting busi- about physics from Sidney than from Richard Feynman when he taught a ness. He became an independent re- anyone else.” In that connection let me course on gravity in 1962–63. The bril- search scientist, located first in New recall an oft-told tale: Working late into liance and strong individualist streak Hampshire and later in New Mexico. the night as was his wont, Sidney rarely that were evidenced in his early work His work was funded by grants from appeared at Harvard much before became hallmarks of Kraichnan’s entire agencies such as the Office of Naval noon. He once arrived so late at a sem- career. Research, NSF, and the Department of inar by Weinberg that all he heard was After leaving the institute, Kraich- Energy. He had long associations with Steve’s uncertain response to a question nan worked at Columbia University the National Center for Atmospheric from the audience. “I know the an- and the Courant Institute of New York Research and Los Alamos National swer!” shouted Sidney on entering the University. In the 1950s and 1960s, he Laboratory. room, “What’s the question?” Indeed, made important contributions to sev- Kraichnan made deep and seminal he often answered questions before eral areas of theoretical physics, in par- discoveries on turbulence in many they were asked. Theorists who con- ticular to quantum field theory and the physical systems, as varied as magneto- sulted him were often astounded as quantum many-body problem. At the hydrodynamics, Rayleigh–Benard con- Sidney would patiently explain the im- time, so-called self-consistent ap- vection, and superfluids. In 1957 he plications of their own ideas. proaches, which resummed infinite used the same ideas as in his work on Sidney was both an incomparable subsets of diagrams, became popular. quantum statistics to develop a self- teacher and the most learned sage and In 1957–62 Kraichnan developed an in- consistent theory called the direct- sharpest critic in the world of theoreti- genious method of realizing such ap- interaction approximation (DIA), whose cal physics: He was Pauli’s tongue in proximations as exact solutions of Lagrangian reformulation in 1964–66 Einstein’s image. We have been de- large-N random-coupling models that yielded a quantitative mean-field the- prived all too soon of one of our gener- couple N copies of the microscopic ation’s most profound and imaginative ory of turbulence. Those works were equations with quenched random pa- the first to provide fundamental in- minds. rameters. Similar techniques using ran- Sheldon Lee Glashow sights into the origin of Lord Kelvin’s dom matrices were rediscovered by concept of “vitiating rearrangement” Boston University Gerard ‘t Hooft, Alexander Migdal, and Boston, Massachusetts and the consequent loss of memory and others in the 1980s and applied to eddy viscosity in turbulent flow. The DIA has been applied to diverse prob- Robert Harry lems in fluid turbulence and was an im- portant predecessor to the modern Kraichnan field-theory formalism of Paul Martin, When Robert Kraichnan died on 26 Feb- Eric Siggia, and Harvey Rose. ruary 2008 at his residence in Santa Fe, Kraichnan also discovered the phe- New Mexico, after a long illness, the nomenon of inverse energy cascade in world lost a profound and original the- two-dimensional turbulence. Building oretical physicist. He contributed much on earlier work of Lars Onsager, T. D. to our current understanding of fluid Lee, and others, Kraichnan predicted in turbulence, the subject that occupied 1967 that there should be a Kolmogorov- him for most of his career, and also like energy cascade in 2D fluids with a made fundamental contributions to −5/3 power-law energy spectrum but general relativity, quantum field theory, with energy transferred from small quantum many-body theory, and statis- scales to large scales, the opposite tical physics. direction as in 3D. That idea has proved Kraichnan was born in Philadelphia extremely influential in our current on 15 January 1928. His earliest scien- understanding of the fluid dynamics of tific interest was in general relativity, Earth’s atmosphere and oceans. Inverse which he began to study on his own at cascade has been cleanly observed in age 13. At age 18 he wrote at MIT a pre- laboratory experiments in the past Robert Harry Kraichnan scient undergraduate thesis, “Quantum several years, and strong evidence has 70 May 2008 Physics Today www.physicstoday.org been found for the process in the oceans Charge Sensitive Preamplifiers and atmosphere. COOLFET® STATE-OF-THE-ART Additionally, Kraichnan contributed A250 a large body of work on passive scalars in a turbulent flow, including his intro- External FET duction in 1968 of an exactly soluble FET can be cooled model of advection by a velocity field Noise: <100 e- RMS (Room Temp.) white-noise in time. In a pivotal 1994 <20 e- RMS (Cooled FET) Physical Review Letter, Kraichnan pro- Gain-Bandwidth fT>1.5 GHz posed that the scalar field in that model Power: 19 mW typical should develop anomalous scaling not Slew rate: >475 V/Ms captured by mean-field theory. The ob- Noise @ 0 pF: 670 eV FWHM (Si) servation led to spectacular develop- ~76 electrons RMS ments in turbulence theory in the 1990s, Noise Slope: 13 eV/pF with Low C FET with successful calculations of the scal- iss 11.5 eV/pF with high C FET ing exponents of the passive scalar. The iss Kraichnan model is now widely hailed Fast Rise Time: 2.5 ns as the “Ising model of turbulence.” THE INDUSTRY STANDARD Kraichnan received the 1993 FEATURES A111 Medaille de l’ADION from France’s Ob- servatoire de la Côte d’Azur, the Amer- • Thermoelectrically Cooled FET ican Physical Society’s 1993 Otto La- • 3 internal FETs to match detector porte Award and 1997 Lars Onsager • Lowest Noise and Noise Slope Prize, and the 2003 Dirac Medal from • AC or DC coupling to the detector the Abdus Salam International Centre • Both Energy and Timing outputs for Theoretical Physics. Kraichnan was • Optional input protection A Microchannel Plate elected in 2000 to the National Acad- (MCP) Array Connected emy of Sciences and became in 2003 • Easy to use to Multiple A111s Homewood Professor of the Johns Hop- kins University. Your complete source for high performance preamplifiers and amplifiers In addition to his achievements in AMPTEK INC. Visit Us Now www.amptek.com physics, Kraichnan enjoyed classical 14 DeAngelo Drive, Bedford, MA 01730-2204 U.S.A. Tel: Fax: e-mail: music and was an accomplished violin- +1 781 275-2242 +1 781 275-3470 [email protected] ist. He was also, in better days, an avid See www.pt.ims.ca/16300-31 hiker who took long daily walks and thought deeply about science as he hiked. Much of his best work was done while walking the hills of New Hamp- Don’t Miss This Rare Opportunity! shire and the canyons of New Mexico. With Kraichnan’s passing, the Niels Bohr Collected Works physics community has lost a truly 13-Volume Limited Edition Collector’s Set original theorist. He was a unique and solitary thinker, but never isolated. A new and final opportunity to purchase all of the most relevant and Throughout his career, he took special authenticated materials and facts from Niels Bohr’s life and work as well as interest in mentoring new researchers personal documents previously unpublished. The limited edition set published and was extraordinarily generous in in agreement with and supported by the official Niels Bohr Archive in sharing his own ideas. His many col- Denmark will provide libraries and the scientific community with the leagues and friends will remember his ONLY comprehensive print and online reference of the Nobel Prize winner. warm and kind presence and his pene- trating insights.
Recommended publications
  • Executive Committee Meeting 6:00 Pm, November 22, 2008 Marriott Rivercenter Hotel
    Executive Committee Meeting 6:00 pm, November 22, 2008 Marriott Rivercenter Hotel Attendees: Steve Pope, Lex Smits, Phil Marcus, Ellen Longmire, Juan Lasheras, Anette Hosoi, Laurette Tuckerman, Jim Brasseur, Paul Steen, Minami Yoda, Martin Maxey, Jean Hertzberg, Monica Malouf, Ken Kiger, Sharath Girimaji, Krishnan Mahesh, Gary Leal, Bill Schultz, Andrea Prosperetti, Julian Domaradzki, Jim Duncan, John Foss, PK Yeung, Ann Karagozian, Lance Collins, Kimberly Hill, Peggy Holland, Jason Bardi (AIP) Note: Attachments related to agenda items follow the order of the agenda and are appended to this document. Key Decisions The ExCom voted to move $100k of operating funds to an endowment for a new award. The ExCom voted that a new name (not Otto Laporte) should be chosen for this award. In the coming year, the Award committee (currently the Fluid Dynamics Prize committee) should establish the award criteria, making sure to distinguish the criteria from those associated with the Batchelor prize. The committee should suggest appropriate wording for the award application and make a recommendation on the naming of the award. The ExCom voted to move Newsletter publication to the first weeks of June and December each year. The ExCom voted to continue the Ad Hoc Committee on Media and Public Relations for two more years (through 2010). The ExCom voted that $15,000 per year in 2009 and 2010 be allocated for Media and Public Relations activities. Most of these funds would be applied toward continuing to use AIP media services in support of news releases and Virtual Pressroom activities related to the annual DFD meeting. Meeting Discussion 1.
    [Show full text]
  • SHELDON LEE GLASHOW Lyman Laboratory of Physics Harvard University Cambridge, Mass., USA
    TOWARDS A UNIFIED THEORY - THREADS IN A TAPESTRY Nobel Lecture, 8 December, 1979 by SHELDON LEE GLASHOW Lyman Laboratory of Physics Harvard University Cambridge, Mass., USA INTRODUCTION In 1956, when I began doing theoretical physics, the study of elementary particles was like a patchwork quilt. Electrodynamics, weak interactions, and strong interactions were clearly separate disciplines, separately taught and separately studied. There was no coherent theory that described them all. Developments such as the observation of parity violation, the successes of quantum electrodynamics, the discovery of hadron resonances and the appearance of strangeness were well-defined parts of the picture, but they could not be easily fitted together. Things have changed. Today we have what has been called a “standard theory” of elementary particle physics in which strong, weak, and electro- magnetic interactions all arise from a local symmetry principle. It is, in a sense, a complete and apparently correct theory, offering a qualitative description of all particle phenomena and precise quantitative predictions in many instances. There is no experimental data that contradicts the theory. In principle, if not yet in practice, all experimental data can be expressed in terms of a small number of “fundamental” masses and cou- pling constants. The theory we now have is an integral work of art: the patchwork quilt has become a tapestry. Tapestries are made by many artisans working together. The contribu- tions of separate workers cannot be discerned in the completed work, and the loose and false threads have been covered over. So it is in our picture of particle physics. Part of the picture is the unification of weak and electromagnetic interactions and the prediction of neutral currents, now being celebrated by the award of the Nobel Prize.
    [Show full text]
  • Nobel Pris Og NBI
    Hvilke forskere, både danske og udenlandske, med tilknytning til NBI har gennem tiden modtaget en nobelpris? M I Nobelpristagere med tilknytning til NBI Der er en lang række Nobelpristagere, som har været ansat i en eller anden form på NBI (Niels Bohr Institutet). Der er desuden en del, der har opholdt sig og arbejdet på institutet i en periode, men ikke har været ansat. De har så været lønnet af deres hjemmeuniversitet og brugt tiden til et samarbejde med en eller flere forskere på NBI, som oftest med en videnskabelig artikel som resultat. Endeligt har der i ”utallige” år været en skik, at fysik nobelpristagere blev inviteret til at komme til København, give en forelæsning, og efter eget ønske blive lidt tid umiddelbart efter modtagelsen af Nobelprisen (hvor de jo alligevel var i Stockholm). I den form har en meget stor del af nobelpristagerne efter institutets oprettelse, været på besøg.. Jeg husker selv fra et af mine første studieår en strålende forelæsning af: Donald Arthur Glaser f: 1926 i USA nobelpris i 1960, med en efterfølgende animeret fest med nobelpristageren i fysik- matematik- og kemi- studerendes forening (som hed parentesen). Der har især i Bohrs tid men været en lang række konferencer og møder, hvor stort set hele den videnskabelige verdens store, har været tilstede f.eks.: Max Karl Ernst Ludwig Planck f: D 1858 d: 1947 nobelpris 1916, Albert Einstein f: D 1879 d: 1955 nobelrpis 1921, Douglas D. Osheroff f: USA 1945 nobelpris 1996 og mange, mange andre. I den nedenstående liste er udvalgt de, der dokumenterbart har haft en eller anden form for regulær ansættelse på NBI.
    [Show full text]
  • Turner Takes Over at the NSF
    PEOPLE APPOINTMENTS Turner takes over at the NSF On 1 October 2003 the astrophysicist the Physics of the Universe, which earlier this Michael Turner, from the University of year produced a comprehensive report Chicago in the US, took over as assistant entitled: "Connecting Quarks with the director for mathematical and physical Cosmos: Eleven Science Questions for the sciences at the US National Science New Century". This report contributed to the Foundation (NSF). This $1 billion directorate current US administration's science planning supports research in mathematics, physics, agenda. Turner, who will serve at the NSF for chemistry, materials and astronomy, as well a two-year term, replaces Robert Eisenstein, as multidisciplinary and educational pro­ who was recently appointed as president of grammes. Turner recently chaired the US the Santa Fe Institute in New Mexico National Research Council's Committee on (see CERN Courier June 2003 p29). Institute of Advanced Study announces its next director Peter Goddard is to become the new director what was to become string theory. Goddard of the Institute for Advanced Study, is currently master of St John's College, Princeton, from 1 January 2004. Goddard, a Cambridge, UK, and is professor of mathematical physicist, is well known for his theoretical physics at the University of work in string theory and conformal field Cambridge, where he was instrumental in theory, for which he received the ICTP's helping to establish the Isaac Newton Dirac prize in 1997, together with David Institute for Mathematical Sciences. Olive. This work dates back to 1970-1972, Photograph courtesy of the Institute for when he held a position as a visiting scientist Advanced Study, Princeton.
    [Show full text]
  • The 60Th Annual DFD Meeting
    FALL 2007 Division of Fluid Dynamics NewsletterDFD News A Division of the American Physical Society DFD ANNUAL ELECTION the 5th DFD meeting in 1952, is a popular tourist destination, and known for it’s mountains and Please vote online in the APS DFD election natural beauty. Salt Lake was the host of the website and vote for one of two candidates 2002 winter Olympics and is a 45 minute drive (Juan Lasheras or Robert Behringer for DFD from seven different ski areas, the closest being Vice Chair and two of four candidates for only 25 minutes away. Mid November usually DFD Executive Committee Members-at-Large marks the beginning of the ski season and (Anette Hosoi, Manoochehr Koochesfahani, attendees may wish to extend their stay for early Laurette Tuckerman or Daniel Lathrop). The season skiing on the “greatest snow on earth!” Vice Chair becomes the Chair-Elect the next Conference Website: year and then the DFD Chair the following http://dfd2007.eng.utah.edu year. The Members-at-Large serve for three year terms. You can easily access the election Hotel Reservations website (with a unique address for each current The main conference Hotel is the Salt Lake City DFD member) with the link that was sent to Downtown Marriott, directly across the street you via email on or about September 24, 2007 from the main entrance to the convention center. from the Division ([email protected]). Short Rooms are also reserved at a special conference biographical sketches of the candidates and rate at the Salt Lake Plaza Inn, also across their statements are included on the website.
    [Show full text]
  • Einstein's Equations for Spin 2 Mass 0 from Noether's Converse Hilbertian
    Einstein’s Equations for Spin 2 Mass 0 from Noether’s Converse Hilbertian Assertion October 4, 2016 J. Brian Pitts Faculty of Philosophy, University of Cambridge [email protected] forthcoming in Studies in History and Philosophy of Modern Physics Abstract An overlap between the general relativist and particle physicist views of Einstein gravity is uncovered. Noether’s 1918 paper developed Hilbert’s and Klein’s reflections on the conservation laws. Energy-momentum is just a term proportional to the field equations and a “curl” term with identically zero divergence. Noether proved a converse “Hilbertian assertion”: such “improper” conservation laws imply a generally covariant action. Later and independently, particle physicists derived the nonlinear Einstein equations as- suming the absence of negative-energy degrees of freedom (“ghosts”) for stability, along with universal coupling: all energy-momentum including gravity’s serves as a source for gravity. Those assumptions (all but) imply (for 0 graviton mass) that the energy-momentum is only a term proportional to the field equations and a symmetric curl, which implies the coalescence of the flat background geometry and the gravitational potential into an effective curved geometry. The flat metric, though useful in Rosenfeld’s stress-energy definition, disappears from the field equations. Thus the particle physics derivation uses a reinvented Noetherian converse Hilbertian assertion in Rosenfeld-tinged form. The Rosenfeld stress-energy is identically the canonical stress-energy plus a Belinfante curl and terms proportional to the field equations, so the flat metric is only a convenient mathematical trick without ontological commitment. Neither generalized relativity of motion, nor the identity of gravity and inertia, nor substantive general covariance is assumed.
    [Show full text]
  • Dynamic Similarity, the Dimensionless Science
    Dynamic similarity, the dimensionless feature science Diogo Bolster, Robert E. Hershberger, and Russell J. Donnelly Dimensional analysis, a framework for drawing physical parallels between systems of disparate scale, affords key insights into natural phenomena too expansive and too energetic to replicate in the lab. Diogo Bolster is an assistant professor of civil engineering and geological sciences at the University of Notre Dame in Notre Dame, Indiana. Robert Hershberger is a research assistant in the department of physics at the University of Oregon in Eugene. Russell Donnelly is a professor of physics at the University of Oregon. Many experiments seem daunting at first glance, in accordance with general relativity, is deflected as it passes owing to the sheer number of physical variables they involve. through the gravitational field of the Sun. Assuming the Sun To design an apparatus that circulates fluid, for instance, one can be treated as a point of mass m and that the ray of light must know how the flow is affected by pressure, by the ap- passes the mass with a distance of closest approach r, dimen- paratus’s dimensions, and by the fluid’s density and viscosity. sional reasoning can help predict the deflection angle θ.1 Complicating matters, those parameters may be temperature Expressed in terms of mass M, length L, and time T, the and pressure dependent. Understanding the role of each variables’ dimensions—denoted with square brackets—are parameter in such a high-dimensional space can be elusive or prohibitively time consuming. Dimensional analysis, a concept historically rooted in Box 1. A brief history of dimensional analysis the field of fluid mechanics, can help to simplify such prob- Going back more than 300 years, discussions of dimensional lems by reducing the number of system parameters.
    [Show full text]
  • Communications-Mathematics and Applied Mathematics/Download/8110
    A Mathematician's Journey to the Edge of the Universe "The only true wisdom is in knowing you know nothing." ― Socrates Manjunath.R #16/1, 8th Main Road, Shivanagar, Rajajinagar, Bangalore560010, Karnataka, India *Corresponding Author Email: [email protected] *Website: http://www.myw3schools.com/ A Mathematician's Journey to the Edge of the Universe What’s the Ultimate Question? Since the dawn of the history of science from Copernicus (who took the details of Ptolemy, and found a way to look at the same construction from a slightly different perspective and discover that the Earth is not the center of the universe) and Galileo to the present, we (a hoard of talking monkeys who's consciousness is from a collection of connected neurons − hammering away on typewriters and by pure chance eventually ranging the values for the (fundamental) numbers that would allow the development of any form of intelligent life) have gazed at the stars and attempted to chart the heavens and still discovering the fundamental laws of nature often get asked: What is Dark Matter? ... What is Dark Energy? ... What Came Before the Big Bang? ... What's Inside a Black Hole? ... Will the universe continue expanding? Will it just stop or even begin to contract? Are We Alone? Beginning at Stonehenge and ending with the current crisis in String Theory, the story of this eternal question to uncover the mysteries of the universe describes a narrative that includes some of the greatest discoveries of all time and leading personalities, including Aristotle, Johannes Kepler, and Isaac Newton, and the rise to the modern era of Einstein, Eddington, and Hawking.
    [Show full text]
  • 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:
    [Show full text]
  • Symposium Celebrating CERN's Discoveries and Looking Into the Future
    CERN–EP–2003–073 CERN–TH–2003–281 December 1st, 2003 Proceedings Symposium celebrating the Anniversary of CERN’s Discoveries and a Look into the Future 111999777333::: NNNeeeuuutttrrraaalll CCCuuurrrrrreeennntttsss 111999888333::: WWW±±± &&& ZZZ000 BBBooosssooonnnsss Tuesday 16 September 2003 CERN, Geneva, Switzerland Editors: Roger Cashmore, Luciano Maiani & Jean-Pierre Revol Table of contents Table of contents 2 Programme of the Symposium 4 Foreword (L. Maiani) 7 Acknowledgements 8 Selected Photographs of the Event 9 Contributions: Welcome (L. Maiani) 13 The Making of the Standard Model (S. Weinberg) 16 CERN’s Contribution to Accelerators and Beams (G. Brianti) 30 The Discovery of Neutral Currents (D. Haidt) 44 The Discovery of the W & Z, a personal recollection (P. Darriulat) 57 W & Z Physics at LEP (P. Zerwas) 70 Physics at the LHC (J. Ellis) 85 Challenges of the LHC: – the accelerator challenge (L. Evans) 96 – the detector challenge (J. Engelen) 103 – the computing challenge (P. Messina) 110 Particle Detectors and Society (G. Charpak) 126 The future for CERN (L. Maiani) 136 – 2 – Table of contents (cont.) Panel discussion on the Future of Particle Physics (chaired by Carlo Rubbia) 145 Participants: Robert Aymar, Georges Charpak, Pierre Darriulat, Luciano Maiani, Simon van der Meer, Lev Okun, Donald Perkins, Carlo Rubbia, Martinus Veltman, and Steven Weinberg. Statements from the floor by: Fabiola Gianotti, Ignatios Antoniadis, S. Glashow, H. Schopper, C. Llewellyn Smith, V. Telegdi, G. Bellettini, and V. Soergel. Additional contributions: Comment on the occasion (S. L. Glashow) 174 Comment on Perturbative QCD in early CERN experiments (D. H. Perkins) 175 Personal remarks on the discovery of Neutral Currents (A.
    [Show full text]
  • Confusions Regarding Quantum Mechanics Gerard ’T Hooft, Reply by Sheldon Lee Glashow
    INFERENCE / Vol. 5, No. 3 Confusions Regarding Quantum Mechanics Gerard ’t Hooft, reply by Sheldon Lee Glashow In response to “The Yang–Mills Model” (Vol. 5, No. 2). began to argue about how the equation is supposed to be interpreted. Why is it that positions and velocities of par- ticles at one given moment cannot be calculated, or even To the editors: defined unambiguously? Physicists know very well how to use the equation. Quantum mechanics was one of the most significant and They use it to derive with perplexing accuracy the prop- important discoveries of twentieth-century science. It all erties of atoms, molecules, elementary particles, and the began, I think, in the year 1900 when Max Planck published forces between all of these. The way the equation is used his paper entitled “On the Theory of the Energy Distribu- is nothing to complain about, but what exactly does it say? tion Law of the Normal Spectrum.”1 In it, he describes a The first question one may rightfully ask, and that simple observation: if one attaches an entropy to the radi- has been asked by many researchers and their students, ation field as if its total energy came in packages—now is this: called quanta—then the intensity of the radiation associ- ated to a certain temperature agrees quite well with the What do these wave functions represent? In particular, what observations. Planck had described his hypothesis as “an is represented by the wave functions that are not associ- act of desperation.”2 But it was the only one that worked.
    [Show full text]
  • Steven Weinberg
    Obituary Steven Weinberg (1933–2021) Theoretical physicist whose electroweak theory won the Nobel prize. teven Weinberg brought the funda- on to positions at Columbia University, New mental understanding of nature to York; the University of Berkeley, California; new levels of power and completeness. the Massachusetts Institute of Technology in He played a central part in formulating Cambridge; and, in 1973, to Harvard University and establishing theoretical physics’ in Cambridge, where he was Higgins Professor Stwo standard models — the standard model of Physics. In 1982, he moved to the University of fundamental interactions and the standard of Texas at Austin, where he remained, teach- model of cosmology. His greatest achievement ing until earlier this year. was to propose the unified theory of electro- Scientists, no less than composers, have magnetism and weak interactions, which is still styles. Einstein and Richard Feynman were in use. This won him the Nobel Prize in Phys- rebellious, most comfortable when they were ics in 1979, shared with his school classmate ‘thinking different’. Weinberg was not like that. Sheldon Lee Glashow, and with Abdus Salam. His approach was scholarly. Most obviously, he His 1967 Physical Review Letters paper, ‘A was keenly interested in the history of physics in Model of Leptons’, combined disparate ideas the West, about which he wrote several deeply about gauge symmetry, symmetry breaking researched and unashamedly ‘Whiggish’ books, and the classification of particles into an ele- most recently To Explain the World (2015). gant whole. Given the state of knowledge at He paid close attention to other people’s CERN/SPL the time, the breakthrough still calls to mind work.
    [Show full text]