DEPARTMENT of PHYSICS COLLOQUIA Fall 1999 Schedule
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CERN Courier–Digital Edition
CERNMarch/April 2021 cerncourier.com COURIERReporting on international high-energy physics WELCOME CERN Courier – digital edition Welcome to the digital edition of the March/April 2021 issue of CERN Courier. Hadron colliders have contributed to a golden era of discovery in high-energy physics, hosting experiments that have enabled physicists to unearth the cornerstones of the Standard Model. This success story began 50 years ago with CERN’s Intersecting Storage Rings (featured on the cover of this issue) and culminated in the Large Hadron Collider (p38) – which has spawned thousands of papers in its first 10 years of operations alone (p47). It also bodes well for a potential future circular collider at CERN operating at a centre-of-mass energy of at least 100 TeV, a feasibility study for which is now in full swing. Even hadron colliders have their limits, however. To explore possible new physics at the highest energy scales, physicists are mounting a series of experiments to search for very weakly interacting “slim” particles that arise from extensions in the Standard Model (p25). Also celebrating a golden anniversary this year is the Institute for Nuclear Research in Moscow (p33), while, elsewhere in this issue: quantum sensors HADRON COLLIDERS target gravitational waves (p10); X-rays go behind the scenes of supernova 50 years of discovery 1987A (p12); a high-performance computing collaboration forms to handle the big-physics data onslaught (p22); Steven Weinberg talks about his latest work (p51); and much more. To sign up to the new-issue alert, please visit: http://comms.iop.org/k/iop/cerncourier To subscribe to the magazine, please visit: https://cerncourier.com/p/about-cern-courier EDITOR: MATTHEW CHALMERS, CERN DIGITAL EDITION CREATED BY IOP PUBLISHING ATLAS spots rare Higgs decay Weinberg on effective field theory Hunting for WISPs CCMarApr21_Cover_v1.indd 1 12/02/2021 09:24 CERNCOURIER www. -
Stsci Newsletter: 1997 Volume 014 Issue 01
January 1997 • Volume 14, Number 1 SPACE TELESCOPE SCIENCE INSTITUTE Highlights of this issue: • AURA science and functional awards to Leitherer and Hanisch — pages 1 and 23 • Cycle 7 to be extended — page 5 • Cycle 7 approved Newsletter program listing — pages 7-13 Astronomy with HST Climbing the Starburst Distance Ladder C. Leitherer Massive stars are an important and powerful star formation events in sometimes dominant energy source for galaxies. Even the most luminous star- a galaxy. Their high luminosity, both in forming regions in our Galaxy are tiny light and mechanical energy, makes on a cosmic scale. They are not them detectable up to cosmological dominated by the properties of an distances. Stars ~100 times more entire population but by individual massive than the Sun are one million stars. Therefore stochastic effects times more luminous. Except for stars prevail. Extinction represents a severe of transient brightness, like novae and problem when a reliable census of the supernovae, hot, massive stars are Galactic high-mass star-formation the most luminous stellar objects in history is atempted, especially since the universe. massive stars belong to the extreme Massive stars are, however, Population I, with correspondingly extremely rare: The number of stars small vertical scale heights. Moreover, formed per unit mass interval is the proximity of Galactic regions — roughly proportional to the -2.35 although advantageous for detailed power of mass. We expect to find very studies of individual stars — makes it few massive stars compared to, say, difficult to obtain integrated properties, solar-type stars. This is consistent with such as total emission-line fluxes of observations in our solar neighbor- the ionized gas. -
Small Wonders the US National Nanotechnology Initiative Has Spent Billions of Dollars on Submicroscopic Science in Its First 10 Years
NEWS FEATURE NATURE|Vol 467|2 September 2010 Simulation of the flow pattern for electrons travelling over a random nanoscale landscape. Small wonders The US National Nanotechnology Initiative has spent billions of dollars on submicroscopic science in its first 10 years. Corie Lok finds out where the money went and what the initiative plans to do next. ichard Smalley’s cheeks were gaunt and promised to conduct electricity better than It was a message that Washington was ready his hair was nearly gone when he testi- copper, but also had the potential to produce to hear. US President Bill Clinton formally fied before the US House of Representa- fibres 100 times stronger than steel at one- announced the initiative in 2000, with bipar- tives in June 1999. The Nobel laureate sixth of the weight. Smalley also predicted tisan support from Congress. The initiative R, HARVARD UNIV. HARVARD R, R E chemist had been diagnosed with non-Hodg- that the “very blunt tool” of chemotherapy that has faced some criticism in the decade since LL kin’s lymphoma a few months earlier, chemo- had ravaged his own body would be obsolete — most notably for its slowness to address E therapy was taking its toll, and the journey within 20 years, because scientists would engi- environmental, health and safety concerns H J. E. from Rice University in Houston, Texas, had neer nanoscale drugs that were “essentially about nanomaterials. But it has also created been exhausting. But none of that dimmed his cancer-seeking missiles” able more than 70 nano-related obvious passion for a subject that his listen- to target mutant cells with “As chemists, we academic or government ers found both mystifying and enthralling: minimal side effects. -
2007-2008 Physics at Brown Newsletter
Physics at Brown NEWS FOR ALUM N I an D FRIE N DS 2007 ISSUE GREETINGS FROM THE CHAIR - SP RING 2008 elcome to another issue of the Brown Physics newsletter. the rank of Associate Professor with tenure. We also report on WI wrote three years ago, during my first term as the some notable faculty achievements for the past year. department chair--with a committed faculty, dedicated staff, enthusiastic students, supportive administration, and engaged e continue the tradition of highlighting the research of alumni and friends--that the future of physics at Brown looked Wour 2007 Galkin Foundation Fellow on page 2. Also bright. Many things have taken place since then. Here we the effort in enriching our physics instruction continues. Three highlight some of the activities of the past year. new courses are offered this year and proposals for three new physics concentrations are under way. Other noteworthy 007 marked the 50th anniversary of the BCS Theory activities include WiSE, Poster Session, UTRA Awards, 2of Superconductivity. We honored Prof. Leon Resource Center, etc. In addition, community outreach Cooper with a two-day symposium on April remains a priority for the Department with a weekly 12-13. A brief description of this event is open house at Ladd and a greatly expanded five- provided on page 3. year NSF supported GK-12 program. e also report on the establishment hanks to a generous gift from his family, an Wof the Institute for Molecular and TAnthony Houghton Prize will be awarded Nanoscale Innovation, which represents an annually for the best theoretical thesis. -
2008 Annual Report
2008 Annual Report NATIONAL ACADEMY OF ENGINEERING ENGINEERING THE FUTURE 1 Letter from the President 3 In Service to the Nation 3 Mission Statement 4 Program Reports 4 Engineering Education 4 Center for the Advancement of Scholarship on Engineering Education 6 Technological Literacy 6 Public Understanding of Engineering Developing Effective Messages Media Relations Public Relations Grand Challenges for Engineering 8 Center for Engineering, Ethics, and Society 9 Diversity in the Engineering Workforce Engineer Girl! Website Engineer Your Life Project Engineering Equity Extension Service 10 Frontiers of Engineering Armstrong Endowment for Young Engineers-Gilbreth Lectures 12 Engineering and Health Care 14 Technology and Peace Building 14 Technology for a Quieter America 15 America’s Energy Future 16 Terrorism and the Electric Power-Delivery System 16 U.S.-China Cooperation on Electricity from Renewables 17 U.S.-China Symposium on Science and Technology Strategic Policy 17 Offshoring of Engineering 18 Gathering Storm Still Frames the Policy Debate 20 2008 NAE Awards Recipients 22 2008 New Members and Foreign Associates 24 2008 NAE Anniversary Members 28 2008 Private Contributions 28 Einstein Society 28 Heritage Society 29 Golden Bridge Society 29 Catalyst Society 30 Rosette Society 30 Challenge Society 30 Charter Society 31 Other Individual Donors 34 The Presidents’ Circle 34 Corporations, Foundations, and Other Organizations 35 National Academy of Engineering Fund Financial Report 37 Report of Independent Certified Public Accountants 41 Notes to Financial Statements 53 Officers 53 Councillors 54 Staff 54 NAE Publications Letter from the President Engineering is critical to meeting the fundamental challenges facing the U.S. economy in the 21st century. -
2005 Annual Report American Physical Society
1 2005 Annual Report American Physical Society APS 20052 APS OFFICERS 2006 APS OFFICERS PRESIDENT: PRESIDENT: Marvin L. Cohen John J. Hopfield University of California, Berkeley Princeton University PRESIDENT ELECT: PRESIDENT ELECT: John N. Bahcall Leo P. Kadanoff Institue for Advanced Study, Princeton University of Chicago VICE PRESIDENT: VICE PRESIDENT: John J. Hopfield Arthur Bienenstock Princeton University Stanford University PAST PRESIDENT: PAST PRESIDENT: Helen R. Quinn Marvin L. Cohen Stanford University, (SLAC) University of California, Berkeley EXECUTIVE OFFICER: EXECUTIVE OFFICER: Judy R. Franz Judy R. Franz University of Alabama, Huntsville University of Alabama, Huntsville TREASURER: TREASURER: Thomas McIlrath Thomas McIlrath University of Maryland (Emeritus) University of Maryland (Emeritus) EDITOR-IN-CHIEF: EDITOR-IN-CHIEF: Martin Blume Martin Blume Brookhaven National Laboratory (Emeritus) Brookhaven National Laboratory (Emeritus) PHOTO CREDITS: Cover (l-r): 1Diffraction patterns of a GaN quantum dot particle—UCLA; Spring-8/Riken, Japan; Stanford Synchrotron Radiation Lab, SLAC & UC Davis, Phys. Rev. Lett. 95 085503 (2005) 2TESLA 9-cell 1.3 GHz SRF cavities from ACCEL Corp. in Germany for ILC. (Courtesy Fermilab Visual Media Service 3G0 detector studying strange quarks in the proton—Jefferson Lab 4Sections of a resistive magnet (Florida-Bitter magnet) from NHMFL at Talahassee LETTER FROM THE PRESIDENT APS IN 2005 3 2005 was a very special year for the physics community and the American Physical Society. Declared the World Year of Physics by the United Nations, the year provided a unique opportunity for the international physics community to reach out to the general public while celebrating the centennial of Einstein’s “miraculous year.” The year started with an international Launching Conference in Paris, France that brought together more than 500 students from around the world to interact with leading physicists. -
AAS NEWSLETTER a Publication for the Members of the American Astronomical Society October 2004 Issue 122 PRESIDENT’S COLUMN Robert Kirshner, [email protected]
AAS NEWSLETTER A Publication for the members of the American Astronomical Society October 2004 Issue 122 PRESIDENT’S COLUMN Robert Kirshner, [email protected] After a year of having my rough edges sanded off as President-elect, I am now actually in the Oval Inside Office (it is really an ellipse with Bob Milkey as one focus). The physical proof of this is a large box of stationery with my return address that says (I am not making this up) “Office of the President.” If you receive a letter from me, you can check it out for yourself. But check the signature, since the 4 Washington AAS office has a JPG of my personal calligraphy. For Official Use Only. AAS Elections Final Slate As incoming President, I got to sit at the left hand of NASA Administrator Sean O’Keefe during lunch before his presentation at the Denver meeting. He had a little trouble with the vacuum seal on the coffee 6 pot, and there were no dexterous robots at the table, so I used my human ingenuity to hold the top Committee News firmly while rotating the coffee pot clockwise with the handle. Exactly like opening a bottle of champagne: hold the cork and rotate the bottle. But not as much fun. 7 International Travel O’Keefe’s speech was quite passionate and made it very clear that he does not want to send astronauts Grant Application to refurbish the Hubble Space Telescope. The preliminary report from the NRC Committee headed by Louis Lanzerotti, and including astronomers Sandy Faber, Riccardo Giacconni, and Joe Taylor gives another perspective, and is well worth reading (http://books.nap.edu/catalog/11051.html). -
STARS, PLANETS and GALAXIES 13-18 April Dahlem, Berlin
STARS, PLANETS AND GALAXIES 13-18 April Dahlem, Berlin Friday, 13 April STRUCTURE FORMATION: FROM COSMOLOGICAL TO ISM SCALES 12h15 Drinks and light lunch available 13h15 Guinevere Kauffmann Welcome 13h30 Philippe Andre The Interstellar Medium and Star Formation: Observations. 14h00 Simon White The Origin of the Cosmic Web of Structure on Large Scales 14h30 Oliver Hahn Shocks and Caustics and their importance for galaxy formation 15h00 Eva Grebel Environmental dependence of stellar chemical evolution and dependence on galaxy properties 15h30 COFFEE BREAK 16h00 Daniel Price Star formation and the role of magnetic fields and turbulence 16h30 Thorsten Naab Simulations of Interstellar Medium and Star formation in Galaxies 17h00 Volker Springel Multi-scale, multi-physics simulation methods. 17h30 DISCUSSION (organizer: G. Kauffmann) 18h30 Reception - Dinner at Harnack House ------------------------------------------------------------------------------------------------------------------- Saturday, 14 April DYNAMICAL PROCESSES IN PLANETS, STARS AND GALAXIES 9h00 Sean Andrews Small-Scale Substructures in Protoplanetary Disks 9h30 Ruth Murray-Clay Pebble Accretion in Protoplanetary Disks 10h00 Francoise Combes Dynamical Processes in Galaxies 10h30 Kathryn Johnston Physical Manifestations of Chaos and Regularity Around Galaxies 11h00 COFFEE 11h30 Scott Tremaine Statistical mechanics of self-gravitating N-body systems 12h00 Silvia Toonen Evolution & interaction in stellar binaries and multiples. 12h30 LUNCH FREE AFTERNOON FOR DISCUSSION/RECREATION -
The INT @ 20 the Future of Nuclear Physics and Its Intersections July 1 – 2, 2010
The INT @ 20 The Future of Nuclear Physics and its Intersections July 1 – 2, 2010 Program Thursday, July 1: 8:00 – 8:45: Registration (Kane Hall, Rom 210) 8:45 – 9:00: Opening remarks Mary Lidstrom, Vice Provost for Research, University of Washington David Kaplan, INT Director Session chair: David Kaplan 9:00 – 9:45: Science & Society 9:00 – 9:45 Steven Koonin, Undersecretary for Science, DOE The future of DOE and its intersections 9:45 – 10:30: Strong Interactions and Fundamental Symmetries 9:45 – 10:30 Howard Georgi, Harvard University QCD – From flavor SU(3) to effective field theory 10:30 – 11:00: Coffee Break Session chair: Martin Savage 11:00 – 11:30 Silas Beane, University of New Hampsire Lattice QCD for nuclear physics 11:30 – 12:00 Paulo Bedaque, University of Maryland Effective field theories in nuclear physics 12:00 – 12:30 Michael Ramsey-Musolf, University of Wisconsin Fundamental symmetries of nuclear physics: A window on the early Universe 12:30 – 2:00: Lunch (Mary Gates Hall) 1 Thursday, July 1 2:00 – 5:00: From Partons to Extreme Matter Session chair: Gerald Miller 2:00 – 2:30 Matthias Burkardt, New Mexico State University Transverse (spin) structure of hadrons 2:30 – 3:00 Barbara Jacak, SUNY Stony Brook Quark-gluon plasma: from particles to fields? 3:00 – 3:45 Raju Venugopalan, Brookhaven National Lab Wee gluons and their role in creating the hottest matter on Earth 3:45 – 4:15: Coffee Break Session chair: Krishna Rajagopal 4:15 – 4:45 Jean-Paul Blaizot, Saclay Is the quark-gluon plasma strongly or weakly coupled? 4:45 -
Educationinnovation2015.Pdf
Edited by: Michael Thoennessen, Michigan State University, and Graham Peaslee, Hope College Layout and design: Erin O’Donnell, NSCL, Michigan State University Front cover: Photograph of lead-tungstate scintillator crystals in a support frame for the Primakoff Experiment (PrimEx) in Hall B at Jefferson Lab. Preamble 3 1 Executive Summary 5 2 Education and Workforce 9 2.1 Workforce Development 9 2.2 Graduate and Postgraduate Education 19 2.3 Undergraduate Education 27 2.4 Outreach and K12 37 3 Innovation 43 3.1 Defense and Security 46 3.2 Energy and Climate 49 3.3 Health and Medicine 54 3.4 Art, Forensic, and other Applications 61 Appendix A: Town Meeting Program 72 Appendix B: Town Meeting Attendees 76 Appendix C: Presentation Abstracts 78 Appendix D: Examples of Outreach Activities 135 Ed Hartouni (Lawrence Livermore National Laboratory) Anna Hayes (Los Alamos National Laboratory) Calvin Howell (Duke University) Cynthia Keppel (Jefferson Lab) Micha Kilburn (University of Notre Dame) Amy McCausey (Michigan State University, conference coordinator) Graham Peaslee (Hope College, co-convener) David Robertson (University of Missouri) Gunther Roland (Massachusetts Institute of Technology) Mike Snow (Indiana University) Michael Thoennessen (Michigan State University, co-convener) The town meeting was supported by the Division of Nuclear Physics and the National Superconducting Cyclotron Laboratory. We would like to thank Kandice Carter, Jolie Cizewski, Micha Kilburn, Peggy Norris, Erich Ormand, and Warren Rogers for suggestions, proof reading, data compilation, collecting the examples of outreach activities. The DNP NSAC Long Range Plan Town Meeting on Education and Innovation was held August 6–8, 2014 on the campus of Michigan State University in East Lansing, MI. -
Neutron Stars
Neutron Stars James Lattimer [email protected] Department of Physics & Astronomy Stony Brook University J.M. Lattimer, Open Nights, 9/7/2007 – p.1/25 Pulsars: The Early History 1932 Chadwick discovers the neutron. 1934 W. Baade and F. Zwicky predict existence of neutron stars as end products of supernovae. 1939 Oppenheimer and Volkoff predict upper mass limit of neutron star. 1964 Hoyle, Narlikar and Wheeler predict neutron stars rapidly rotate. 1964 Prediction that neutron stars have intense magnetic fields. 1966 Colgate and White suggest supernovae make neutron stars. 1966 Wheeler predicts Crab nebula powered by rotating neutron star. 1967 Pacini makes first pulsar model. 1967 C. Schisler discovers a dozen pulsing radio sources, including the Crab pulsar, using secret military radar in Alaska. 1967 Hewish, Bell, Pilkington, Scott and Collins discover the pulsar PSR 1919+21, Aug 6. 1968 Pulsar discovered in Crab Nebula, and it was found to be slowing down, ruling out binary models. This also clinched their connection with Type II supernovae. 1968 T. Gold identifies pulsars with magnetized, rotating neutron stars. 1968 The term “pulsar” first appears in print, in the Daily Telegraph. 1969 “Glitches” provide evidence for superfluidity in neutron star. 1971 Accretion powered X-ray pulsar discovered by Uhuru (not the Lt.). J.M. Lattimer, Open Nights, 9/7/2007 – p.2/25 Pulsars: Later Discoveries 1974 Hewish awarded Nobel Prize (but Jocelyn Bell Burnell was not). 1974 Binary pulsar PSR 1913+16 discovered by Hulse and Taylor. It shows the orbital decay due to gravitational radiation predicted by Einstein’s General Theory of Relativity. -
50 & 100 Years A
NEWS & VIEWS NATURE|Vol 457|29 January 2009 CONDENSED-MATTER PHYSICS The pnictide code 50 YEARS AGO Jan Zaanen In previous communications, Hopes are that the emergent family of iron-based superconductors, the the existence of a third normal, pnictides, could act as a Rosetta stone in decoding the two-decade mystery embryonic haemoglobin was reported to be present in the blood of superconductivity observed at high temperatures. of foetuses up to five months of intra-uterine life ... By using About a year ago, the announcement of the against the might of this quantum simplicity. the column chromatographic discovery1 of a new family of superconductors Metaphorically, the cuprate electron world is procedure described by Huisman made from iron-based compounds prompted like a quantized form of dense traffic on a busy and Prins, with some minor an army of physicists and chemists to study highway. The electrons are subject to perpetual modifications, we were able these pnictides. But what caused — and is per- quantum motions, but can hinder each other’s to separate the three distinct petuating — this frenzy? The quest for a higher motions to such an extent that the electron fractions from the haemolysate transition temperature, Tc (the temperature ‘traffic’ jams completely, causing undoped of a four month old embryo ... above which no superconductivity is attained), cuprates to become insulating. Chemical dop- Thus, we were able to separate stalled2 at a meagre 56 kelvin, and the focus ing can clear the way on the ‘quantum highway’, not only the two haemoglobin of the excitement has shifted: it is now hoped and at low levels of doping a quantum incarna- fractions known to be present that the pnictides will be instrumental in tion of stop-and-go traffic is observed6.