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Old Soldiers by Michael Riordan
Old soldiers by Michael Riordan Twenty years ago this month, an this deep inelastic region in excru experiment began at the Stanford ciating detail, the new quark-parton Linear Accelerator Center in Cali picture of a nucleon's innards fornia that would eventually redraw gradually took a firmer and firmer the map of high energy physics. hold upon the particle physics com In October 1967, MIT and SLAC munity. These two massive spec physicists started shaking down trometers were our principal 'eyes' their new 20 GeV spectrometer; into the new realm, by far the best by mid-December they were log ones we had until more powerful ging electron-proton scattering in muon and neutrino beams became the so-called deep inelastic region available at Fermilab and CERN. where the electrons probed deep They were our Geiger and Marsd- inside the protons. The huge ex en, reporting back to Rutherford cess of scattered electrons they the detailed patterns of ricocheting encountered there-about ten times projectiles. Through their magnetic the expected rate-was later inter lenses we 'observed' quarks for preted as evidence for pointlike, the very first time, hard 'pits' inside fractionally charged objects inside hadrons. the proton. These two goliaths stood reso Michael Riordan (above) did The quarks we take for granted lutely at the front as a scientific research using the 8 GeV today were at best 'mathematical' revolution erupted all about them spectrometer at SLAC as an entities in 1967 - if one allowed during the late 1960s and early MIT graduate student during them any true existence at all. -
Harry Truman, the Atomic Bomb and the Apocalyptic Narrative
Volume 5 | Issue 7 | Article ID 2479 | Jul 12, 2007 The Asia-Pacific Journal | Japan Focus The Decision to Risk the Future: Harry Truman, the Atomic Bomb and the Apocalyptic Narrative Peter J. Kuznick The Decision to Risk the Future: Harry stressed that the future of mankind would be Truman, the Atomic Bomb and theshaped by how such bombs were used and Apocalyptic Narrative subsequently controlled or shared.[3] Truman recalled Stimson “gravely” expressing his Peter J. Kuznick uncertainty about whether the U.S. should ever use the bomb, “because he was afraid it was so I powerful that it could end up destroying the whole world.” Truman admitted that, listening In his personal narrative Atomic Quest, Nobel to Stimson and Groves and reading Groves’s Prize-winning physicist Arthur Holly Compton, accompanying memo, he “felt the same who directed atomic research at the University fear.”[4] of Chicago’s Metallurgical Laboratory during the Second World War, tells of receiving an urgent visit from J. Robert Oppenheimer while vacationing in Michigan during the summer of 1942. Oppenheimer and the brain trust he assembled had just calculated the possibility that an atomic explosion could ignite all the hydrogen in the oceans or the nitrogen in the atmosphere. If such a possibility existed, Compton concluded, “these bombs must never be made.” As Compton said, “Better to accept the slavery of the Nazis than to run a chance of drawing the final curtain on mankind.”[1] Certainly, any reasonable human being could be expected to respond similarly. Three years later, with Hitler dead and the Nazis defeated, President Harry Truman faced Truman and Byrnes en route to Potsdam, July a comparably weighty decision. -
Atomic Physics & Quantum Effects
KEY CONCEPTS ATOMIC PHYSICS & QUANTUM EFFECTS 1. PHOTONS & THE PHOTOELECTRIC EFFECT Max Planck explained blackbody radiation with his quantum hypothesis, which states that the energy of a thermal oscillator, Eosc, is not continuous, but instead is a discrete quantity given by the equation: Eosc = nhf n = 1, 2, 3,... where f is the frequency and h is a constant now known as Planck’s constant. Albert Einstein extended the idea by adding that all emitted radiation is quantized. He suggested that light is composed of discrete quanta, rather than of waves. According to his theory, each particle of light, known as a photon, has an energy E given by: E = hf Einstein’s theory helped him explain a phenomenon known as the photoelectric effect, in which a photon of light strikes a photosensitive material and causes an electron to be ejected from the material. A photocell constructed from photosensitive material can produce an electrical current when light shines on it. The kinetic energy, K, of a photoelectron displaced by a photon of energy, hf, is given by: K = hf - φ where the work function, φ, is the minimum energy needed to free the electron from the photosensitive material. No photoemission occurs if the frequency of the incident light falls below a certain cutoff frequency – or threshold frequency – given by: φ f0 = h Einstein's theory explained several aspects of the photoelectric effect that could not be explained by classical theory: • The kinetic energy of photoelectrons is dependent on the light’s frequency. • No photoemission occurs for light below a certain threshold frequency. -
Minutes of the High Energy Physics Advisory Panel Meeting February 14-15, 2008 Palomar Hotel, Washington, D.C
Minutes of the High Energy Physics Advisory Panel Meeting February 14-15, 2008 Palomar Hotel, Washington, D.C. HEPAP members present: Jonathan A. Bagger, Vice Chair Lisa Randall Daniela Bortoletto Tor Raubenheimer James E. Brau Kate Scholberg Patricia Burchat Melvyn J. Shochet, Chair Robert N. Cahn Sally Seidel Priscilla Cushman (Thursday only) Henry Sobel Larry D. Gladney Maury Tigner Robert Kephart William Trischuk William R. Molzon Herman White Angela V. Olinto Guy Wormser (Thursday only) Saul Perlmutter HEPAP members absent: Hiroaki Aihara Joseph Lykken Alice Bean Stephen L. Olsen Sarah Eno Also participating: Charles Baltay, Department of Physics, Yale University Barry Barish, Director, Global Design Effort, International Linear Collider William Carithers, Physics Division, Lawrence Berkeley National Laboratory Tony Chan, Assistant Director for Mathematics and Physical Sciences, National Science Foundation Glen Crawford, Program Manager, Office of High Energy Physics, Office of Science, Department of Energy Joseph Dehmer, Director, Division of Physics, National Science Foundation Persis Drell, Director, Stanford Linear Accelerator Center Thomas Ferbel, Department of Physics and Astronomy, University of Rochester Marvin Goldberg, Program Director, Division of Physics, National Science Foundation Paul Grannis, Department of Physics and Astronomy, State University of New York Michael Harrison, Physics Department, Brookhaven National Laboratory Abolhassan Jawahery, BaBar Collaboration Spokesman, Stanford Linear Accelerator Center Steve -
NMD, National Security Issues Featured at 2001 April Meeting In
April 2001 NEWS Volume 10, No. 4 A Publication of The American Physical Society http://www.aps.org/apsnews NMD, National Security Issues Featured Phase I CPU Report to be at 2001 April Meeting in Washington Discussed at Attendees of the 2001 APS April include a talk on how the news me- Meeting, which returns to Wash- dia cover science by David April Meeting ington, DC, this year, should arrive Kestenbaum, a self-described “es- The first phase of a new Na- just in time to catch the last of the caped physicist who is hiding out tional Research Council report of cherry blossom season in between at National Public Radio,” and a lec- the Committee on the Physics of scheduled sessions and special ture on entangled photons for the Universe (CPU) will be the events. The conference will run quantum information by the Uni- topic of discussion during a spe- April 28 through May 1, and will versity of Illinois’ Paul Kwiat. Other cial Sunday evening session at the feature the latest results in nuclear scheduled topics include imaging APS April Meeting in Washing- physics, astrophysics, chemical the cosmic background wave back- ton, DC. The session is intended physics, particles and fields, com- ground, searching for extra to begin the process of collect- putational physics, plasma physics, dimensions, CP violation in B me- ing input from the scientific the physics of beams, and physics sons, neutrino oscillations, and the community on some of the is- history, among other subdisci- amplification of atoms and light in The White House and (inset) some of its famous fictional sues outlined in the draft report, plines. -
Copyright by Paul Harold Rubinson 2008
Copyright by Paul Harold Rubinson 2008 The Dissertation Committee for Paul Harold Rubinson certifies that this is the approved version of the following dissertation: Containing Science: The U.S. National Security State and Scientists’ Challenge to Nuclear Weapons during the Cold War Committee: —————————————————— Mark A. Lawrence, Supervisor —————————————————— Francis J. Gavin —————————————————— Bruce J. Hunt —————————————————— David M. Oshinsky —————————————————— Michael B. Stoff Containing Science: The U.S. National Security State and Scientists’ Challenge to Nuclear Weapons during the Cold War by Paul Harold Rubinson, B.A.; M.A. Dissertation Presented to the Faculty of the Graduate School of The University of Texas at Austin in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy The University of Texas at Austin August 2008 Acknowledgements Thanks first and foremost to Mark Lawrence for his guidance, support, and enthusiasm throughout this project. It would be impossible to overstate how essential his insight and mentoring have been to this dissertation and my career in general. Just as important has been his camaraderie, which made the researching and writing of this dissertation infinitely more rewarding. Thanks as well to Bruce Hunt for his support. Especially helpful was his incisive feedback, which both encouraged me to think through my ideas more thoroughly, and reined me in when my writing overshot my argument. I offer my sincerest gratitude to the Smith Richardson Foundation and Yale University International Security Studies for the Predoctoral Fellowship that allowed me to do the bulk of the writing of this dissertation. Thanks also to the Brady-Johnson Program in Grand Strategy at Yale University, and John Gaddis and the incomparable Ann Carter-Drier at ISS. -
6 8 Myriam Sarachik Elected APS Vice President
November 2000 NEWS Volume 9, No. 10 A Publication of The American Physical Society http://www.aps.org/apsnews Myriam Sarachik Elected APS Vice President Members of the APS have chosen Sciences Research at Lucent. Only and government labs, and to pro- Myriam Sarachik, a distinguished two new general councillors were vide the next generation of professor of physics at City College elected, compared to the four educators at our universities,” she of New York’s City University of New elected in previous years, to reflect says. One of her goals as President York, to be the Society’s next vice recent changes in the APS Consti- will be to strengthen the society’s president. Sarachik is the third tution, designed to reduce the size efforts to make a career in physics woman to be elected to the presi- of the APS Council. These changes attractive. “We need to be more ef- dential line in the Society’s 101-year were published in the March 2000 fective in explaining the pleasures history, following C.S. Wu of Colum- issue of APS News. that a career in physics can bring, bia in 1975, and Mildred the satisfaction garnered from VICE PRESIDENT CHAIR-ELECT OF THE Dresselhaus of MIT (who became VICE PRESIDENT teaching, and the excitement of re- Myriam Sarachik NOMINATING COMMITTEE Director of the Department of MYRIAM SARACHIK search and discovery; we must also Susan Coppersmith Energy’s Office of Science in August) City College of New York/CUNY have salaries competitive with other in 1984. Sarachik’s term begins Born in Antwerp, Belgium, professional options,” she says. -
From Theory to the First Working Laser Laser History—Part I
I feature_ laser history From theory to the first working laser Laser history—Part I Author_Ingmar Ingenegeren, Germany _The principle of both maser (microwave am- 19 US patents) using a ruby laser. Both were nom- plification by stimulated emission of radiation) inated for the Nobel Prize. Gábor received the 1971 and laser (light amplification by stimulated emis- Nobel Prize in Physics for the invention and devel- sion of radiation) were first described in 1917 by opment of the holographic method. To a friend he Albert Einstein (Fig.1) in “Zur Quantentheorie der wrote that he was ashamed to get this prize for Strahlung”, as the so called ‘stimulated emission’, such a simple invention. He was the owner of more based on Niels Bohr’s quantum theory, postulated than a hundred patents. in 1913, which explains the actions of electrons in- side atoms. Einstein (born in Germany, 14 March In 1954 at the Columbia University in New York, 1879–18 April 1955) received the Nobel Prize for Charles Townes (born in the USA, 28 July 1915–to- physics in 1921, and Bohr (born in Denmark, 7 Oc- day, Fig. 2) and Arthur Schawlow (born in the USA, tober 1885–18 November 1962) in 1922. 5 Mai 1921–28 April 1999, Fig. 3) invented the maser, using ammonia gas and microwaves which In 1947 Dennis Gábor (born in Hungarian, 5 led to the granting of a patent on March 24, 1959. June 1900–8 February 1972) developed the theory The maser was used to amplify radio signals and as of holography, which requires laser light for its re- an ultra sensitive detector for space research. -
Title: the Distribution of an Illustrated Timeline Wall Chart and Teacher's Guide of 20Fh Century Physics
REPORT NSF GRANT #PHY-98143318 Title: The Distribution of an Illustrated Timeline Wall Chart and Teacher’s Guide of 20fhCentury Physics DOE Patent Clearance Granted December 26,2000 Principal Investigator, Brian Schwartz, The American Physical Society 1 Physics Ellipse College Park, MD 20740 301-209-3223 [email protected] BACKGROUND The American Physi a1 Society s part of its centennial celebration in March of 1999 decided to develop a timeline wall chart on the history of 20thcentury physics. This resulted in eleven consecutive posters, which when mounted side by side, create a %foot mural. The timeline exhibits and describes the millstones of physics in images and words. The timeline functions as a chronology, a work of art, a permanent open textbook, and a gigantic photo album covering a hundred years in the life of the community of physicists and the existence of the American Physical Society . Each of the eleven posters begins with a brief essay that places a major scientific achievement of the decade in its historical context. Large portraits of the essays’ subjects include youthful photographs of Marie Curie, Albert Einstein, and Richard Feynman among others, to help put a face on science. Below the essays, a total of over 130 individual discoveries and inventions, explained in dated text boxes with accompanying images, form the backbone of the timeline. For ease of comprehension, this wealth of material is organized into five color- coded story lines the stretch horizontally across the hundred years of the 20th century. The five story lines are: Cosmic Scale, relate the story of astrophysics and cosmology; Human Scale, refers to the physics of the more familiar distances from the global to the microscopic; Atomic Scale, focuses on the submicroscopic This report was prepared as an account of work sponsored by an agency of the United States Government. -
DPF NEWSLETTER - April 15, 1996
DPF NEWSLETTER - April 15, 1996 To: Members of the Division of Particles and Fields From: Jonathan Bagger, Secretary-Treasurer, [email protected] 1995 DPF Elections Howard Georgi was elected Vice-Chair of the DPF. Tom Devlin and Heidi Schellman were elected to the Executive Committee. George Trilling was elected as a Division Councillor. The current members of the DPF Executive Committee and the final years of their terms are Chair: Frank Sciulli (1996) Chair-Elect: Paul Grannis (1996) Vice-Chair: Howard Georgi (1996) Past Chair: David Cassel (1996) Secretary-Treasurer: Jonathan Bagger (1997) Division Councillor: Henry Frisch (1997), George Trilling (1998) Executive Board: Sally Dawson (1996), Tom Devlin (1998), Martin Einhorn (1997), John Rutherfoord (1997), Heidi Schellman (1998), Michael Shaevitz (1996) Call for Nominations: 1996 DPF Elections The 1996 Nominating Committee is hard at work. Please send suggestions for candidates to the Chair, Abe Seiden of Santa Cruz ([email protected]). The other members of the Nominating Committee are Melissa Franklin, Robert Jaffe, Michael Murtagh, Helen Quinn, and Bill Reay. DPF Members are also entitled to nominate candidates by petition. Twenty signatures from DPF members are required. Nominations will be accepted by Jonathan Bagger until May 15, 1996. Snowmass 1996: New Directions for High Energy Physics The 1996 Snowmass Workshop on New Directions in High Energy Physics will be held in Snowmass, Colorado, from June 24 to July 12, 1996. Arrival, registration, and a reception will be on June 24. Full-day plenary sessions will be held on June 25-26 and July 11-12. This workshop will provide an opportunity to begin to develop a coherent plan for the longer term future for U.S. -
Quantum Mechanics Quantum Chromodynamics (QCD)
Quantum Mechanics_quantum chromodynamics (QCD) In theoretical physics, quantum chromodynamics (QCD) is a theory ofstrong interactions, a fundamental forcedescribing the interactions between quarksand gluons which make up hadrons such as the proton, neutron and pion. QCD is a type of Quantum field theory called a non- abelian gauge theory with symmetry group SU(3). The QCD analog of electric charge is a property called 'color'. Gluons are the force carrier of the theory, like photons are for the electromagnetic force in quantum electrodynamics. The theory is an important part of the Standard Model of Particle physics. A huge body of experimental evidence for QCD has been gathered over the years. QCD enjoys two peculiar properties: Confinement, which means that the force between quarks does not diminish as they are separated. Because of this, when you do split the quark the energy is enough to create another quark thus creating another quark pair; they are forever bound into hadrons such as theproton and the neutron or the pion and kaon. Although analytically unproven, confinement is widely believed to be true because it explains the consistent failure of free quark searches, and it is easy to demonstrate in lattice QCD. Asymptotic freedom, which means that in very high-energy reactions, quarks and gluons interact very weakly creating a quark–gluon plasma. This prediction of QCD was first discovered in the early 1970s by David Politzer and by Frank Wilczek and David Gross. For this work they were awarded the 2004 Nobel Prize in Physics. There is no known phase-transition line separating these two properties; confinement is dominant in low-energy scales but, as energy increases, asymptotic freedom becomes dominant. -
Report on HEPAP Activities
Report on HEPAP activities Mel Shochet University of Chicago 6/4/09 Fermilab Users Meeting 1 What is HEPAP? High Energy Physics Advisory Panel • Advises the DOE & NSF on the particle physics program. • Federal Advisory Committee Act rules – Public meetings – US members are Special Government Employees on meeting days. • Subject to federal conflict-of-interest rules • “Special” ⇒ paycheck = $0.00 – Appointed by DOE Under-Secretary for Science & NSF Director – Reports to Assoc. Dir. for OHEP & Asst. Dir. Math & Phys. Sciences – Broad membership: subfield, univ & labs, demographics (geography,…) • Members don’t serve as representatives of constituencies; advise on the health of the entire field. • Foreign members provide information on programs in Europe & Asia 6/4/09 Fermilab Users Meeting 2 Current Membership • Hiroaki Aihara, Tokyo • Daniel Marlow, Princeton • Marina Artuso, Syracuse • Ann Nelson, Washington • Alice Bean, Kansas • Stephen Olsen, Hawaii • Patricia Burchat, Stanford • Lisa Randall, Harvard • Priscilla Cushman, Minn. • Kate Scholberg, Duke • Lance Dixon, SLAC • Sally Seidel, New Mexico • Sarah Eno, Maryland • Melvyn Shochet, Chicago • Graciela Gelmini, UCLA • Henry Sobel, Irvine • Larry Gladney, Penn • Paris Sphicas, CERN • Boris Kayser, FNAL (DPF) • Maury Tigner, Cornell • Robert Kephart, FNAL • William Trischuk, Toronto • Steve Kettell, BNL • Herman White, FNAL • Wim Leemans, LBNL 6/4/09 Fermilab Users Meeting 3 Meetings • 3 meetings per year • Agenda – reports from the funding agencies on budgets & their impact, recent events, successes and problems – reports from specialized subpanels that need HEPAP approval to become official government documents (ex. P5) – reports from other committees that impact HEP (ex. EPP2010) – informational reports on issues that might arise in the future (ex.