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The Physical Tourist Physics and New York City
Phys. perspect. 5 (2003) 87–121 © Birkha¨user Verlag, Basel, 2003 1422–6944/05/010087–35 The Physical Tourist Physics and New York City Benjamin Bederson* I discuss the contributions of physicists who have lived and worked in New York City within the context of the high schools, colleges, universities, and other institutions with which they were and are associated. I close with a walking tour of major sites of interest in Manhattan. Key words: Thomas A. Edison; Nikola Tesla; Michael I. Pupin; Hall of Fame for GreatAmericans;AlbertEinstein;OttoStern;HenryGoldman;J.RobertOppenheimer; Richard P. Feynman; Julian Schwinger; Isidor I. Rabi; Bronx High School of Science; StuyvesantHighSchool;TownsendHarrisHighSchool;NewYorkAcademyofSciences; Andrei Sakharov; Fordham University; Victor F. Hess; Cooper Union; Peter Cooper; City University of New York; City College; Brooklyn College; Melba Phillips; Hunter College; Rosalyn Yalow; Queens College; Lehman College; New York University; Courant Institute of Mathematical Sciences; Samuel F.B. Morse; John W. Draper; Columbia University; Polytechnic University; Manhattan Project; American Museum of Natural History; Rockefeller University; New York Public Library. Introduction When I was approached by the editors of Physics in Perspecti6e to prepare an article on New York City for The Physical Tourist section, I was happy to do so. I have been a New Yorker all my life, except for short-term stays elsewhere on sabbatical leaves and other visits. My professional life developed in New York, and I married and raised my family in New York and its environs. Accordingly, writing such an article seemed a natural thing to do. About halfway through its preparation, however, the attack on the World Trade Center took place. -
Of Charles D. Ferguson, on Behalf Of
FEDERATION OF AMERICAN SCIENTISTS T: 202/546-3300 1725 DeSales Street, NW 6th Floor Washington, DC 20036 www.fas.org F: 202/675-1010 [email protected] PRM-70-9 DOCKETED Board of Sponsors (75FR80730) USNRC (PartialList) March 4, 2011 March 7, 2011 (10:30 am) •Pacr Agre * SidnheyAman * Philip W. Anderson *Kenneth J. Arrow To: Secretary, U.S. Nuclear Regulatory Commission OFFICE OF SECRETARY * David Baltimore RULEMAKINGS AND * Bamj Be.....ea Washington, DC 20555-0001 SPaulBerg ADJUDICATIONS STAFF * J. Michael Bishop AT-TN: Rulemakings and Adjudications Staff * Guther Blobel * Nicolaas Bloensbergen * Paul Boyce Ann Pitts Carter Subject: Comment on Docket ID NRC-2010-0372, "Petition for Rulemaking, * Stanley Cohen * Leon N. Cooper Francis Slakey on Behalf of the American Physical Society" * E. J. Corey 'James Cronin * Johann Deismehofer ArmDruyan *RenatoDulbeomo As Board Members of the Federation of American Scientists, an independent, Paul L Ehrlich George Field nonpartisan think tank, we strongly support the petition submitted by the Vat L. Fitch * JeromeI. Friedman American Physical Society that requests proliferation risk assessments become a * Riccardo Giacoani * Walter Gilbert required part of the NRC licensing process. * Alfed G. Gilman " Donald Glaser * Sheldon L. Glashow Marvin L. Goidhergr * Joseph L. Goldstein Emerging nuclear fuel technologies such as laser enrichment of uranium can pose Roger C. L. Gaillemin * L[land H. Hartwell significant proliferation risks due to difficulties in detecting facilities using these * Herbert A. Hauptman " Dudley RKHIaechach technologies. If such technologies are developed without a clear, objective, and * Roald Hoff-aan John P. Hoidren detailed assessment, they can dangerously undermine U.S. nuclear * -l Robert Horvitz * David H. -
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The Second Lepton Family Klaus Winter, CERN The Nobel Prize for Physics for 1988 was awarded to L. Lederman, M. Schwartz and J. Steinberger for work on neutrinos in the early 1960s. In a letter [1] addressed to the "dear radioactive ladies and gentlemen", writ ten in December 1930, Wolfgang Pauli proposed, as a "desperate remedy" to save the principle of conservation of energy in beta-decay, the idea of the neutrino, a neutral particle of spin 1/2 and with a mass not larger than 0.01 proton mass. "The continuous beta-spectrum [2] would then become understandable by the assumption that in beta-decay a neutrino is emitted together with the electron, in such a way that the sum of the energies of the neutrino and electron is constant." Pauli did not specify at that time Fig. 1 — A recent photograph taken at CERN of Leon Lederman (left), whether the neutrino was to be ejected Jack Steinberger (centre) and Melvin Schwartz. or created. In his famous paper "An attempt of a theory of beta-decay" [3] the muon not decay into e + at the rate ween 1 and 2 GeV should be achievable. E. Fermi used the neutrino concept of predicted if such a non-locality exis Would these synchrotrons though, deli Pauli together with the concept of the ted ? ". On this view the muon would vir ver enough neutrinos? According to nucleon of Heisenberg. He assumed tually dissociate into W + v, the charged their specifications they should accele that in beta-decay a pair comprising an W would radiate a and W + v would rate 1011 protons per second, an unpre electron and a neutrino is created, analo recombine to an electron. -
CERN Courier Is Distributed to Member-State Governments, Institutes and Laboratories Affiliated with CERN, and to Their Personnel
I n t e r n at I o n a l J o u r n a l o f H I g H - e n e r g y P H y s I c s CERN COURIERV o l u m e 4 6 n u m b e r 9 n o V e m b e r 2 0 0 6 OPERA makes its grand debut ACCELERATORS COMPUTING NEWS INTERVIEW Laser-wakefield device Business signs up to Stephen Hawking pays reaches 1 GeV p5 work with EGEE p12 a visit to CERN p28 CCENovCover1.indd 1 18/10/06 08:53:59 CERN & ProCurve Networking 15 petabytes of data And a network that can handle it “CERN uses ProCurve Switches because we generate a colossal amount of data, making dependability a top priority.” —David Foster, Communication Systems Group Leader, CERN CERN has joined with ProCurve to build their network based on high-performance security, reliability and flexibility, along with a lifetime warranty.* From the world’s largest applications, to a company-wide email, just think what ProCurve could do for your network. Get a closer look at CERN and the world’s biggest physics experiment. Visit www.hp.com/eur/procurvecern1 *For as long as you own the product, with next-business-day advance replacement (available in most countries). For details, refer to the ProCurve Software License, Warranty and Support booklet at www.hp.com/rnd/support/warranty/index.htm The ProCurve Routing Switch 9300m series, ProCurve Routing Switch 9408sl, ProCurve Switch 8100fl series, and the ProCurve Access Control Server 745wl have a one-year- warranty with extensions available. -
Date: To: September 22, 1 997 Mr Ian Johnston©
22-SEP-1997 16:36 NOBELSTIFTELSEN 4& 8 6603847 SID 01 NOBELSTIFTELSEN The Nobel Foundation TELEFAX Date: September 22, 1 997 To: Mr Ian Johnston© Company: Executive Office of the Secretary-General Fax no: 0091-2129633511 From: The Nobel Foundation Total number of pages: olO MESSAGE DearMrJohnstone, With reference to your fax and to our telephone conversation, I am enclosing the address list of all Nobel Prize laureates. Yours sincerely, Ingr BergstrSm Mailing address: Bos StU S-102 45 Stockholm. Sweden Strat itddrtSMi Suircfatan 14 Teleptelrtts: (-MB S) 663 » 20 Fsuc (*-«>!) «W Jg 47 22-SEP-1997 16:36 NOBELSTIFTELSEN 46 B S603847 SID 02 22-SEP-1997 16:35 NOBELSTIFTELSEN 46 8 6603847 SID 03 Professor Willis E, Lamb Jr Prof. Aleksandre M. Prokhorov Dr. Leo EsaJki 848 North Norris Avenue Russian Academy of Sciences University of Tsukuba TUCSON, AZ 857 19 Leninskii Prospect 14 Tsukuba USA MSOCOWV71 Ibaraki Ru s s I a 305 Japan 59* c>io Dr. Tsung Dao Lee Professor Hans A. Bethe Professor Antony Hewlsh Department of Physics Cornell University Cavendish Laboratory Columbia University ITHACA, NY 14853 University of Cambridge 538 West I20th Street USA CAMBRIDGE CB3 OHE NEW YORK, NY 10027 England USA S96 014 S ' Dr. Chen Ning Yang Professor Murray Gell-Mann ^ Professor Aage Bohr The Institute for Department of Physics Niels Bohr Institutet Theoretical Physics California Institute of Technology Blegdamsvej 17 State University of New York PASADENA, CA91125 DK-2100 KOPENHAMN 0 STONY BROOK, NY 11794 USA D anni ark USA 595 600 613 Professor Owen Chamberlain Professor Louis Neel ' Professor Ben Mottelson 6068 Margarldo Drive Membre de rinstitute Nordita OAKLAND, CA 946 IS 15 Rue Marcel-Allegot Blegdamsvej 17 USA F-92190 MEUDON-BELLEVUE DK-2100 KOPENHAMN 0 Frankrike D an m ar k 599 615 Professor Donald A. -
Particle Detectors Lecture Notes
Lecture Notes Heidelberg, Summer Term 2011 The Physics of Particle Detectors Hans-Christian Schultz-Coulon Kirchhoff-Institut für Physik Introduction Historical Developments Historical Development γ-rays First 1896 Detection of α-, β- and γ-rays 1896 β-rays Image of Becquerel's photographic plate which has been An x-ray picture taken by Wilhelm Röntgen of Albert von fogged by exposure to radiation from a uranium salt. Kölliker's hand at a public lecture on 23 January 1896. Historical Development Rutherford's scattering experiment Microscope + Scintillating ZnS screen Schematic view of Rutherford experiment 1911 Rutherford's original experimental setup Historical Development Detection of cosmic rays [Hess 1912; Nobel prize 1936] ! "# Electrometer Cylinder from Wulf [2 cm diameter] Mirror Strings Microscope Natrium ! !""#$%&'()*+,-)./0)1&$23456/)78096$/'9::9098)1912 $%&!'()*+,-.%!/0&1.)%21331&10!,0%))0!%42%!56784210462!1(,!9624,10462,:177%&!(2;! '()*+,-.%2!<=%4*1;%2%)%:0&67%0%&!;1&>!Victor F. Hess before his 1912 balloon flight in Austria during which he discovered cosmic rays. ?40! @4)*%! ;%&! /0%)),-.&1(8%! A! )1,,%2! ,4-.!;4%!BC;%2!;%,!D)%:0&67%0%&,!(7!;4%! EC2F,1-.,%!;%,!/0&1.)%21331&10,!;&%.%2G!(7!%42%!*H&!;4%!A8)%,(2F!FH2,04F%!I6,40462! %42,0%))%2! J(! :K22%2>! L10&4(7! =4&;! M%&=%2;%0G! (7! ;4%! E(*0! 47! 922%&%2! ;%,! 9624,10462,M6)(7%2!M62!B%(-.04F:%40!*&%4!J(!.1)0%2>! $%&!422%&%G!:)%42%&%!<N)42;%&!;4%20!;%&!O8%&3&H*(2F!;%&!9,6)10462!;%,!P%&C0%,>!'4&;!%&! H8%&! ;4%! BC;%2! F%,%2:0G! ,6! M%&&42F%&0! ,4-.!;1,!1:04M%!9624,10462,M6)(7%2!1(*!;%2! -
Scientific and Related Works of Chen Ning Yang
Scientific and Related Works of Chen Ning Yang [42a] C. N. Yang. Group Theory and the Vibration of Polyatomic Molecules. B.Sc. thesis, National Southwest Associated University (1942). [44a] C. N. Yang. On the Uniqueness of Young's Differentials. Bull. Amer. Math. Soc. 50, 373 (1944). [44b] C. N. Yang. Variation of Interaction Energy with Change of Lattice Constants and Change of Degree of Order. Chinese J. of Phys. 5, 138 (1944). [44c] C. N. Yang. Investigations in the Statistical Theory of Superlattices. M.Sc. thesis, National Tsing Hua University (1944). [45a] C. N. Yang. A Generalization of the Quasi-Chemical Method in the Statistical Theory of Superlattices. J. Chem. Phys. 13, 66 (1945). [45b] C. N. Yang. The Critical Temperature and Discontinuity of Specific Heat of a Superlattice. Chinese J. Phys. 6, 59 (1945). [46a] James Alexander, Geoffrey Chew, Walter Salove, Chen Yang. Translation of the 1933 Pauli article in Handbuch der Physik, volume 14, Part II; Chapter 2, Section B. [47a] C. N. Yang. On Quantized Space-Time. Phys. Rev. 72, 874 (1947). [47b] C. N. Yang and Y. Y. Li. General Theory of the Quasi-Chemical Method in the Statistical Theory of Superlattices. Chinese J. Phys. 7, 59 (1947). [48a] C. N. Yang. On the Angular Distribution in Nuclear Reactions and Coincidence Measurements. Phys. Rev. 74, 764 (1948). 2 [48b] S. K. Allison, H. V. Argo, W. R. Arnold, L. del Rosario, H. A. Wilcox and C. N. Yang. Measurement of Short Range Nuclear Recoils from Disintegrations of the Light Elements. Phys. Rev. 74, 1233 (1948). [48c] C. -
1 Restoring Scientific Integrity in Policy Making February 18, 2004
Restoring Scientific Integrity in Policy Making February 18, 2004 Science, like any field of endeavor, relies on freedom of inquiry; and one of the hallmarks of that freedom is objectivity. Now, more than ever, on issues ranging from climate change to AIDS research to genetic engineering to food additives, government relies on the impartial perspective of science for guidance. President George H.W. Bush, April 23, 1990 Successful application of science has played a large part in the policies that have made the United States of America the world’s most powerful nation and its citizens increasingly prosperous and healthy. Although scientific input to the government is rarely the only factor in public policy decisions, this input should always be weighed from an objective and impartial perspective to avoid perilous consequences. Indeed, this principle has long been adhered to by presidents and administrations of both parties in forming and implementing policies. The administration of George W. Bush has, however, disregarded this principle. When scientific knowledge has been found to be in conflict with its political goals, the administration has often manipulated the process through which science enters into its decisions. This has been done by placing people who are professionally unqualified or who have clear conflicts of interest in official posts and on scientific advisory committees; by disbanding existing advisory committees; by censoring and suppressing reports by the government’s own scientists; and by simply not seeking independent scientific advice. Other administrations have, on occasion, engaged in such practices, but not so systematically nor on so wide a front. Furthermore, in advocating policies that are not scientifically sound, the administration has sometimes misrepresented scientific knowledge and misled the public about the implications of its policies. -
Melvin Schwartz 1932-2006
MELVIN SCHWARTZ 1932-2006 A Biographical Memoir by N. P. SAMIOS AND P. YAMIN © 2012 The National Academy of Sciences Any opinions expressed in this memoir are those of the authors and do not necessarily reflect the views of the National Academy of Sciences. MELVIN SCHWARTZ Courtesy of Brookhaven National Laboratories. November 2, 1932–August 28, 2006 BY N. P. SAMIOS AND P. YAMIN MEL SCHWARTZ DIED ON August 28, 2006, in Twin Falls, Idaho. He was born on 1 November 2, 1932, in New York City. He grew up in the Great Depression, but with a sense of optimism and desire to use his mind for the betterment of human- kind. He entered the Bronx High School of Science in the fall of 1945. It was there that his interest in physics began and that he recognized the importance of interactions with peers in determining his sense of direction in life. One of his classmates and future colleagues recalled that “even then” he wanted a Nobel Prize. Mel noted: My interest in physics began at the age of 12 when I entered the Bronx High School of Science. The four years I spent there were certainly among the most exciting and stimulating in my life, mostly because of the interaction with the other students of similar background, interest, and ability. MELVIN SCHWARTZ MELVIN On Sunday afternoons he attended a school run by the secular and Zionist Yiddish and many others. As Mel commented, “This faculty [was] at this time unmatched by any in the world, largely Nationaler Arbeter Farband (Jewish National Workers Alliance). -
Dzhelepov Laboratory of Nuclear Problems
Dzhelepov Laboratory of Nuclear Problems Dmitry V.Naumov Presented by O.Smirnov Dubna JINR New elements 102, {103, 104, 105(Db), 107}, 114, 115, 116, 117, 118 are synthesized Hypothesis of neutrino oscillations (1957г.) New particles: anti-sigma- minus hyperon And many other discoveries JINR Employed ~ 5000: 1200 - scientists, 2000 - engineers 7 labs. Each lab is as a big research institute 18 member-states and 6 associated members 1500 scientific publications Collaboration with 700 scientific centers and universities in 64 countries Expected budget in 2017-2023 1, 472 billion USD History ● May, 7 1946. First discussion of «construction of a power cyclotron» at special committee of the government ● 18 August 1946. Soviet government approved the proposal of Academician Igor Kurchatov to construct in USSR „the installation M” for fundamental studies in nuclear physics. ● 14 December 1949. The 480 MeV proton synchrocyclotron started operation at the Hydrotechnical Laboratory in Dubna, the most powerful accelerator in the world at that time. ● 26 March 1956. Laboratory of Nuclear Problems of JINR has been founded. M.G.Meshcheryakov Synchrocyclotron 680 MeV (1953) Discoveries Half of discoveries (37) in physics recorded in Soviet Union belongs to JINR 15 of these belongs to LNP Nowadays DLNP researchers are also awarded for important discoveries. Discoveries → New Technologies→ Discoveries LNP a laboratory with largest diversity → origin of most of laboratories in JINR Institute of Nuclear Problems (now DLNP) + Electrophysical laboratory (now -
Muonium Gravity Seminar Wichita-6-17
Antimatter Gravity MICE-U.S. Plans withDaniel Muons M. Kaplan US Spokesperson, MICE Collaboration Daniel M. Kaplan Physics Seminar WichitaMuTAC State Review Univ. June Fermilab16, 2017 16–17 March, 2006 Outline • Dramatis Personae • A Bit of History - antimatter, the baryon asymmetry of the universe, and all that... • The Ideas, The Issues, The Opportunities • Required R&D • Conclusions Our story’s a bit complicated, so please bear with me! ...and stop me if you have a question! D. M. Kaplan, IIT An#ma&er Gravity Seminar 2/41 Matter & Energy • After many decades of experimentation with subatomic particles, we now know whatDramatis everything is made of... Personae Baryons & antibaryons : p== uud & p uud ΛΛ==uds & uds ... Mesons : K00== ds & K ds B00== db & B db B+ == ub & B− ub ... ∓ ∓ ∓ Leptons : e , µ , τ , ν’s D. M. Kaplan, IIT An#ma&er Gravity Seminar 3/41 Matter & Energy • After many decades of experimentation with subatomic particles, we now know whatDramatis everything is made of... Personae “Imperfect mirror” Baryons & antibaryons : Antip== uud & p uud ΛΛ==uds & uds ... Mesons : Anti K00== ds & K ds B00== db & B db Anti B+ == ub & B− ub ... Antimatter Leptons : e∓, µ∓, τ∓, ν’s • And, don’t forget: antimatter and matter annihilate on contact D. M. Kaplan, IIT An#ma&er Gravity Seminar 3/41 Outline • Dramatis Personae ➡ • A Bit of History - antimatter, the baryon asymmetry of the universe, and all that... • The Ideas, The Issues, The Opportunities • Muonium Gravity Experiment • Required R&D • Conclusions D. M. Kaplan, IIT An#ma&er Gravity Seminar 4/41 Our story begins with.. -
Liste Der Nobelpreisträger
Physiologie Wirtschafts- Jahr Physik Chemie oder Literatur Frieden wissenschaften Medizin Wilhelm Henry Dunant Jacobus H. Emil von Sully 1901 Conrad — van ’t Hoff Behring Prudhomme Röntgen Frédéric Passy Hendrik Antoon Theodor Élie Ducommun 1902 Emil Fischer Ronald Ross — Lorentz Mommsen Pieter Zeeman Albert Gobat Henri Becquerel Svante Niels Ryberg Bjørnstjerne 1903 William Randal Cremer — Pierre Curie Arrhenius Finsen Bjørnson Marie Curie Frédéric John William William Mistral 1904 Iwan Pawlow Institut de Droit international — Strutt Ramsay José Echegaray Adolf von Henryk 1905 Philipp Lenard Robert Koch Bertha von Suttner — Baeyer Sienkiewicz Camillo Golgi Joseph John Giosuè 1906 Henri Moissan Theodore Roosevelt — Thomson Santiago Carducci Ramón y Cajal Albert A. Alphonse Rudyard \Ernesto Teodoro Moneta 1907 Eduard Buchner — Michelson Laveran Kipling Louis Renault Ilja Gabriel Ernest Rudolf Klas Pontus Arnoldson 1908 Metschnikow — Lippmann Rutherford Eucken Paul Ehrlich Fredrik Bajer Theodor Auguste Beernaert Guglielmo Wilhelm Kocher Selma 1909 — Marconi Ostwald Ferdinand Lagerlöf Paul Henri d’Estournelles de Braun Constant Johannes Albrecht Ständiges Internationales 1910 Diderik van Otto Wallach Paul Heyse — Kossel Friedensbüro der Waals Allvar Maurice Tobias Asser 1911 Wilhelm Wien Marie Curie — Gullstrand Maeterlinck Alfred Fried Victor Grignard Gerhart 1912 Gustaf Dalén Alexis Carrel Elihu Root — Paul Sabatier Hauptmann Heike Charles Rabindranath 1913 Kamerlingh Alfred Werner Henri La Fontaine — Robert Richet Tagore Onnes Theodore