Physics and the Totalitarian Principle
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Unrestricted Immigration and the Foreign Dominance Of
Unrestricted Immigration and the Foreign Dominance of United States Nobel Prize Winners in Science: Irrefutable Data and Exemplary Family Narratives—Backup Data and Information Andrew A. Beveridge, Queens and Graduate Center CUNY and Social Explorer, Inc. Lynn Caporale, Strategic Scientific Advisor and Author The following slides were presented at the recent meeting of the American Association for the Advancement of Science. This project and paper is an outgrowth of that session, and will combine qualitative data on Nobel Prize Winners family histories along with analyses of the pattern of Nobel Winners. The first set of slides show some of the patterns so far found, and will be augmented for the formal paper. The second set of slides shows some examples of the Nobel families. The authors a developing a systematic data base of Nobel Winners (mainly US), their careers and their family histories. This turned out to be much more challenging than expected, since many winners do not emphasize their family origins in their own biographies or autobiographies or other commentary. Dr. Caporale has reached out to some laureates or their families to elicit that information. We plan to systematically compare the laureates to the population in the US at large, including immigrants and non‐immigrants at various periods. Outline of Presentation • A preliminary examination of the 609 Nobel Prize Winners, 291 of whom were at an American Institution when they received the Nobel in physics, chemistry or physiology and medicine • Will look at patterns of -
Steven Weinberg Cv Born
STEVEN WEINBERG CV BORN: May 3, 1933, in New York, N.Y. EDUCATION: Cornell University, 1950–1954 (A.B., 1954) Copenhagen Institute for Theoretical Physics, 1954–1955 Princeton University, 1955–1957 (Ph.D.,1957). HONORARY DEGREES: Harvard University, A.M., 1973 Knox College, D.Sc., 1978 University of Chicago, Sc.D., 1978 University of Rochester, Sc.D., l979 Yale University, Sc.D., 1979 City University of New York,Sc.D., 1980 Clark University, Sc.D., 1982 Dartmouth College, Sc.D., 1984 Weizmann Institute, Ph.D. Hon.Caus., 1985 Washington College, D.Litt., 1985 Columbia University, Sc.D., 1990 University of Salamanca, Sc.D., 1992 University of Padua, Ph.D. Hon.Caus., 1992 University of Barcelona, Sc.D., 1996 Bates College, Sc. D., 2002 McGill University, Sc. D., 2003 University of Waterloo, Sc. D., 2004 Renssalear Polytechnic Institue, Sc. D., 2016 Rockefeller University, Sc. D., 2017 PRESENT POSITION: Josey Regental Professor of Science, University of Texas, 1982– PAST POSITIONS: Columbia University, 1957–1959 Lawrence Radiation Laboratory, 1959–1960 University of California, Berkeley, 1960–1969 On leave, Imperial College, London, 1961–1962 Steven Weinberg 2 Became full professor, 1964 On leave, Harvard University, 1966–1967 On leave, Massachusetts Institute of Technology, 1967–1969 Massachusetts Institute of Technology, 1969–1973, Professor of Physics Harvard University, 1973–1983, Higgins Professor of Physics On leave 1976–1977, as Visiting Professor of Physics, Stanford University Smithsonian Astrophysical Observatory, 1973-1983, Senior -
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. -
Nobel Prize for Physics, 1979
Nobel Prize for Physics, 1979 Abdus Sal am Physics' most prestigious accolade forces is a significant milestone in goes this year to Sheldon Glashow, the constant quest to describe as Abdus Salam and Steven Weinberg much as possible of the world for their work in elucidating the inter around us from a minimal set of actions of elementary particles, and initial ideas. in particular for the development of 'At first sight there may be little or the theory which unifies the electro no similarity between electromag magnetic and weak forces. netic effects and the phenomena This synthesis of two of the basic associated with weak interactions', forces of nature must be reckoned as wrote Sheldon Glashow in 1960. one of the crowning achievements 'Yet remarkable parallels emerge...' of a century which has already seen Both kinds of interactions affect the birth of both quantum mechanics leptons and hadrons; both appear to and relativity. be 'vector' interactions brought Electromagnetism and the weak about by the exchange of particles force might appear to have little to carrying unit spin and negative pari do with each other. Electromagne ty; both have their own universal tism is our everyday world — it holds coupling constant which governs the atoms together and produces light, strength of the interactions. while the weak force was for a long These vital clues led Glashow to time known only for the relatively propose an ambitious theory which obscure phenomenon of beta-decay attempted to unify the two forces. radioactivity. However there was one big difficul The successful unification of these ty, which Glashow admitted had to two apparently highly dissimilar be put to one side. -
Thesis Reference
Thesis On Testing Modified Gravity : with Solar System Experiments and Gravitational Radiation SANCTUARY, Hillary Adrienne Abstract Three theories of gravitation – general relativity, the chameleon and Horava gravity - are confronted with experiment, using standard and adapted post-Newtonian (PN) tools. The laboratory is provided by the Solar System, binary pulsars and future detections at gravitational wave observatories. We test Horava gravity by studying emission of gravitational radiation in the weak-field limit for PN sources using techniques that take full advantage of the parametrized post-Newtonian (PPN) formalism. In particular, we provide a generalization of Einstein’s quadrupole formula and show that a monopole persists even in the limit in which the PPN parameters are identical to those of General Relativity. Based on a technique called non-relativistic General Relativity, we propose a phenomenological way to measure deviations from General Relativity coming from an unknown UV completion. Finally, we systematically show that the self-interacting chameleon at orders three and higher do not jeopardize the chameleon theory for Solar System type objects. Reference SANCTUARY, Hillary Adrienne. On Testing Modified Gravity : with Solar System Experiments and Gravitational Radiation. Thèse de doctorat : Univ. Genève, 2012, no. Sc. 4524 Available at: http://archive-ouverte.unige.ch/unige:28935 Disclaimer: layout of this document may differ from the published version. [ Downloaded 07/04/2015 at 08:06:08 ] 1 / 1 UNIVERSITÉ DE GENÈVE FACULTÉ DES SCIENCES Département de physique théorique Professeur Michele Maggiore On Testing Modified Gravity with Solar System Experiments and Gravitational Radiation THÈSE présentée à la Faculté des Sciences de l’Université de Genève pour obtenir le grade de Docteur ès Sciences, mention Physique par Hillary Sanctuary de Montréal, Canada Thèse No 4524 Genève, juillet 2012 Reprographie EPFL Publications D. -
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. -
Quantum Chaos in the Quantum Fluid
Quantum chaos in the quantum fluid Raju Venugopalan Brookhaven Na<onal Laboratory Joe Fest, McGill, Montreal, June 12-14, 2012 Smoking Joe and Holy Indian Lone ranger: I think we are surrounded, Kemo sabe Tonto: What do you mean “we” $@!# Smoking Joe and Holy Indian Lone ranger: I think we are surrounded, Kemo sabe Tonto: Indeed, Lone Ranger – no worries – they are all here to praise you on your 60th ! Talk Mo<va<on: the unreasonable effec<veness of hydrodynamics in heavy ion collisions to paraphrase E. P. Wigner An ab ini<o weak coupling approach: Classical coherence of wee partons in nuclear wavefunc<ons Quantum fluctua<ons: Factoriza<on, Evolu<on, Decoherence Isotropizaon, Bose-Einstein Condensaon, Thermalizaon ? 4 Ab inio approach to heavy ion collisions RV, ICHEP review talk, 1012.4699 Color Glass Inial Glasma sQGP - Hadron Condensates Singularity perfect fluid! Gas t τ0 ? Compute properes of relevant degrees of freedom of wave fns. in a systema<c framework (as opposed to a “model”)? How is maer formed ? What are its non-equilibrium properes & lifeme? Can one “prove” thermalizaon or is the system “parally” thermal ? When is hydrodynamics applicable? How much jet quenching occurs in the Glasma? Are there novel topological effects (sphaleron transions?) Ab inio approach to heavy ion collisions RV, ICHEP review talk, 1012.4699 Color Glass Inial Glasma sQGP - Hadron Condensates Singularity perfect fluid! Gas t τ0 ? Compute properes of relevant degrees of freedom of wave fns. in a systema<c framework (as opposed to a “model”)? How -
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. -
Quarks and Quantum Statistics
Quarks and quantum statistics O.W. Greenberg∗† Center for Fundamental Physics, Department of Physics University of Maryland, College Park, MD 20742-4111, USA and Helsinki Institute for Physics P.O.Box 64 (Gustaf Hällströmin katu 2) FIN-00014 University of Helsinki, Finland E-mail: [email protected] I write about Héctor, his contributions to the early work in the quark model, and a general discus- sion of quantum statistics arXiv:1102.0764v1 [physics.hist-ph] 3 Feb 2011 Quarks, Strings and the Cosmos - Héctor Rubinstein Memorial Symposium August 09-11, 2010 AlbaNova )Stockholm) Sweden ∗Speaker. †University of Maryland Preprint PP-11-001 c Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence. http://pos.sissa.it/ Quarks and quantum statistics O.W. Greenberg 1. Introduction Héctor and I first met at a summer workshop in Bebek, near Istanbul, Turkey. The workshop photograph is at the end of this paper. At first sight, Héctor is nowhere to be seen. Actually, he is there, but he is turned around talking or arguing with somebody behind him. That is Héctor, too full of energy to pose passively for a photo. The tallest person above the left of the last row is Shelly Glashow, to his left is Nick Bur- goyne. One row down, from the left, are Arthur Jaffe, Joe Dothan, Sidney Coleman, Gian-Fausto Dell’Antonio, Bruria Kaufman, and Eduardo Caianiello, among others. On the left of the third row down is H.R. Mani, and on the right of that row, there is Héctor, turned facing backwards as just mentioned. -
Arxiv:0801.2562V2 [Hep-Ph]
NATURALLY SPEAKING: The Naturalness Criterion and Physics at the LHC Gian Francesco GIUDICE CERN, Theoretical Physics Division Geneva, Switzerland 1 Naturalness in Scientific Thought Everything is natural: if it weren’t, it wouldn’t be. Mary Catherine Bateson [1] Almost every branch of science has its own version of the “naturalness criterion”. In environmental sciences, it refers to the degree to which an area is pristine, free from human influence, and characterized by native species [2]. In mathematics, its meaning is associated with the intuitiveness of certain fundamental concepts, viewed as an intrinsic part of our thinking [3]. One can find the use of naturalness criterions in computer science (as a measure of adaptability), in agriculture (as an acceptable level of product manipulation), in linguistics (as translation quality assessment of sentences that do not reflect the natural and idiomatic forms of the receptor language). But certainly nowhere else but in particle physics has the mutable concept of naturalness taken a form which has become so influential in the development of the field. The role of naturalness in the sense of “æsthetic beauty” is a powerful guiding principle for physicists as they try to construct new theories. This may appear surprising since the final product is often a mathematically sophisticated theory based on deep fundamental principles, arXiv:0801.2562v2 [hep-ph] 30 Mar 2008 and one could believe that subjective æsthetic arguments have no place in it. Nevertheless, this is not true and often theoretical physicists formulate their theories inspired by criteria of simplicity and beauty, i.e. by what Nelson [4] defines as “structural naturalness”. -
Sam Treiman Was Born in Chicago to a First-Generation Immigrant Family
NATIONAL ACADEMY OF SCIENCES SAM BARD TREIMAN 1925–1999 A Biographical Memoir by STEPHEN L. ADLER Any opinions expressed in this memoir are those of the author and do not necessarily reflect the views of the National Academy of Sciences. Biographical Memoirs, VOLUME 80 PUBLISHED 2001 BY THE NATIONAL ACADEMY PRESS WASHINGTON, D.C. Courtesy of Robert P. Matthews SAM BARD TREIMAN May 27, 1925–November 30, 1999 BY STEPHEN L. ADLER AM BARD TREIMAN WAS a major force in particle physics S during the formative period of the current Standard Model, both through his own research and through the training of graduate students. Starting initially in cosmic ray physics, Treiman soon shifted his interests to the new particles being discovered in cosmic ray experiments. He evolved a research style of working closely with experimen- talists, and many of his papers are exemplars of particle phenomenology. By the mid-1950s Treiman had acquired a lifelong interest in the weak interactions. He would preach to his students that “the place to learn about the strong interactions is through the weak and electromagnetic inter- actions; the problem is half as complicated.’’ The history of the subsequent development of the Standard Model showed this philosophy to be prophetic. After the discovery of parity violation in weak interactions, Treiman in collaboration with J. David Jackson and Henry Wyld (1957) worked out the definitive formula for allowed beta decays, taking into account the possible violation of time reversal symmetry, as well as parity. Shortly afterwards Treiman embarked with Marvin Goldberger on a dispersion relations analysis (1958) of pion and nucleon beta decay, a 3 4 BIOGRAPHICAL MEMOIRS major outcome of which was the famed Goldberger-Treiman relation for the charged pion decay amplitude. -
Deconstruction: Standard Model Discoveries
deconstruction: standard model discoveries elementary types of particles form the basis for the theoretical framework known as the Sixteen Standard Model of fundamental particles and forces. J.J. Thomson discovered the electron in 1897, while scientists at Fermilab saw the first direct interaction of a tau neutrino with matter less than 10 years ago. This graphic names the 16 particle types and shows when and where they were discovered. These particles also exist in the form of antimatter particles, with the same mass and the opposite electric charge. Together, they account for about 300 subatomic particles observed in experiments so far. The Standard Model also predicts the Higgs boson, which still eludes experimental detection. Experiments at Fermilab and CERN could see the first signals for this particle in the next couple of years. Other funda- mental particles must exist, too. The Standard Model does not account for dark matter, which appears to make up 83 percent of all matter in the universe. 1968: SLAC 1974: Brookhaven & SLAC 1995: Fermilab 1979: DESY u c t g up quark charm quark top quark gluon 1968: SLAC 1947: Manchester University 1977: Fermilab 1923: Washington University* d s b γ down quark strange quark bottom quark photon 1956: Savannah River Plant 1962: Brookhaven 2000: Fermilab 1983: CERN νe νμ ντ W electron neutrino muon neutrino tau neutrino W boson 1897: Cavendish Laboratory 1937 : Caltech and Harvard 1976: SLAC 1983: CERN e μ τ Z electron muon tau Z boson *Scientists suspected for several hundred years that light consists of particles. Many experiments and theoretical explana- tions have led to the discovery of the photon, which explains both wave and particle properties of light.