Belief and Observation: the Top Quark and Other Tales of “Discovery”
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Subnuclear Physics: Past, Present and Future
Subnuclear Physics: Past, Present and Future International Symposium 30 October - 2 November 2011 – The purpose of the Symposium is to discuss the origin, the status and the future of the new frontier of Physics, the Subnuclear World, whose first two hints were discovered in the middle of the last century: the so-called “Strange Particles” and the “Resonance #++”. It took more than two decades to understand the real meaning of these two great discoveries: the existence of the Subnuclear World with regularities, spontaneously plus directly broken Symmetries, and totally unexpected phenomena including the existence of a new fundamental force of Nature, called Quantum ChromoDynamics. In order to reach this new frontier of our knowledge, new Laboratories were established all over the world, in Europe, in USA and in the former Soviet Union, with thousands of physicists, engineers and specialists in the most advanced technologies, engaged in the implementation of new experiments of ever increasing complexity. At present the most advanced Laboratory in the world is CERN where experiments are being performed with the Large Hadron Collider (LHC), the most powerful collider in the world, which is able to reach the highest energies possible in this satellite of the Sun, called Earth. Understanding the laws governing the Space-time intervals in the range of 10-17 cm and 10-23 sec will allow our form of living matter endowed with Reason to open new horizons in our knowledge. Antonino Zichichi Participants Prof. Werner Arber H.E. Msgr. Marcelo Sánchez Sorondo Prof. Guido Altarelli Prof. Ignatios Antoniadis Prof. Robert Aymar Prof. Rinaldo Baldini Ferroli Prof. -
CURRICULUM VITAE – Paul D. Grannis April 6, 2021 DATE of BIRTH: June 26, 1938 EDUCATION
CURRICULUM VITAE { Paul D. Grannis July 15, 2021 EDUCATION: B. Eng. Phys., with Distinction, Cornell University (1961) Ph.D. University of California, Berkeley (1965) Thesis: Measurement of the Polarization Parameter in Proton-Proton Scattering from 1.7 to 6.1 BeV Advisor, Owen Chamberlain EMPLOYMENT: Research Professor of Physics, State Univ. of New York at Stony Brook, 2007 { Distinguished Professor Emeritus, State Univ. of New York at Stony Brook, 2007 { Chair, Department of Physics and Astronomy, Stony Brook, 2002 { 2005 Distinguished Professor of Physics, State Univ. of New York at Stony Brook, 1997 { 2006 Professor of Physics, Stony Brook, 1975 { 1997 Associate Professor of Physics, Stony Brook, 1969 { 1975 Assistant Professor of Physics, Stony Brook, 1966 { 1969 Research Associate, Lawrence Radiation Laboratory, 1965 { 1966 1 AWARDS: Danforth Foundation Fellow, 1961 { 1965 Alfred P. Sloan Foundation Fellow, 1969 { 1971 Fellow, American Physical Society Fellow, American Association for the Advancement of Science Exceptional Teaching Award, Stony Brook, 1992 Exceptional Service Award, U.S. Department of Energy, 1997 John S. Guggenheim Fellowship, 2000 { 2001 American Physical Society W.K.H. Panofsky Prize, 2001 Honorary Doctor of Science, Ohio University, 2009 W. V. Houston Memorial Lectureship, Rice University 2012 Foreign member, Russian Academy of Science, 2016 Co-winner with the members of the DØ Collaboration, European Physical Society High Energy Particle Physics Prize, 2019 2 OTHER ACTIVITIES: Visiting Scientist, Rutherford -
Course Syllabus
University of Science and Technology of Hanoi Address: Building 2H, 18 Hoang Quoc Viet, Cau Giay, Hanoi Telephone/ Fax: +84-4 37 91 69 60 Email: [email protected] Website: http://www.usth.edu.vn COURSE SYLLABUS Subject: Intrumentation in Ground and Academic field: Astronomy Space Astrophysics Lecturer: Dr. Pham Ngoc Diep Phone: 01689677899 E-mail: [email protected] Academic year: 2013-2014 COURSE DESCRIPTION Credit points 2 Level Undergraduate Teaching time University of Science and Technology of Hanoi Location Lecture 16 hrs Exercises 8 hrs Time Commitment Practicals 6 hrs Total 30 hrs elementary of waves, classical mechanics, quantum mechanics, nuclear Prerequisites physics and particle physics Recommended Knowledge from Prof. Quynh Lan’s lectures background knowledge This course involves an elementary introduction to astrophysics, cosmology and instrumentation in ground and space astrophysics. The logic is that students should know about the basics of astrophysics and cosmology, the major unanswered questions in the fields. Therefore, they will understand why, what and how we measure astrophysical quantities. Emphases are on understanding the principles of detecting electromagnetic waves at different wavelengths and some different Subject description: particles. It is an exploratory, first course in instrumentation designed primarily for students planning to enrol in the regular-program astrophysics or related field such as space and application courses upon completion of this course. However, it also meets the needs of many students with other interests. Each UNIT is planed to be discussed in 2 hours. With practical work and/or visit to astrophysics labs, students will see in reality how a telescope works, they will have chance to operate it, take data and make some simple data analysis. -
Finding the W and Z Products, Etc
CERN Courier May 2013 CERN Courier May 2013 Reminiscence Anniversary on precisely the questions that the physicists at CERN would be interested in: the cross-sections for W and Z production; the expected event rates; the angular distribution of the W and Z decay Finding the W and Z products, etc. People would also want to know how uncertain the predictions for the W and Z masses were and why certain theorists (J J Sakurai and James Bjorken among them) were cautioning that the masses could turn out to be different. The writing of the trans- parencies turned out to be time consuming. I had to make frequent revisions, trying to anticipate what questions might be asked. To Thirty years ago, CERN made scientifi c make corrections on the fi lm transparencies, I was using my after- shave lotion, so that the whole room was reeking of perfume. I history with the discoveries of the W and was preparing the lectures on a day-by-day basis, not getting much sleep. To stay awake, I would go to the cafeteria for a coffee shortly Z bosons. Here, we reprint an extract from before it closed. Thereafter I would keep going to the vending the special issue of CERN Courier that machines in the basement for chocolate – until the machines ran out of chocolate or I ran out of coins. commemorated this breakthrough. After the fourth lecture, the room in the dormitory had become such a mess (papers everywhere and the strong smell of after- shave) that I decided to ask the secretariat for an offi ce where I Less than 11 months after Lalit Sehgal’s visit to CERN, Carlo could work. -
RESEARCH ASSOCIATE in Particle Physics THEORETICAL NUCLEAR PHYSICS
Andrei Dimitrievich Sakharov 1921-1989 People and things Andrei Dimitrievich Sakharov, the quark model, and pioneer talented and versatile scientist, ideas in the quantum theory of fearless activist and staunch gravity. proponent of human rights, fig• He was not able to receive his urehead for Soviet perestroika, Nobel Award in person. From described in the citation for his 1980, during his exile in Gorki, 1975 Nobel Peace Prize as he tried to keep in touch with CERN elections and appointments 'spokesman for the conscience developments in science, receiv• of mankind', died on 14 Decem• ing physics literature, including At its December meetings, CERN ber. the CERN Courier, by registered Council elected C. Lopez, Rector of Beginning research at Lenin• mail. the Autonomous University of Ma• grad's Lebedev Institute in 1945 With the new direction in So• drid, and E. W.J. Mitchell, Chairman under Igor Tamm, he first came viet policy he reemerged as a of the UK Science and Engineering to prominence with his early popular champion in the USSR. Research Council, as Vice-Presi• 1950s contributions to thermo• Last year, accompanied by his dents, and Chris Llewellyn-Smith of nuclear fusion with Tamm, in• wife Elena Bonner, he embarked Oxford as Chairman of the Science cluding the idea to contain plas• on a visit of major world physics Policy Committee. ma in a magnetic 'bottle', later Laboratories. In 1990, the CERN Directorate to become known as the toka- In a message entitled 'The re• consists of Research Directors mak. For his fusion work he be• sponsibility of scientists' to a Pierre Darriulat, Walter Hoogland came an Academician in 1953 1981 New York meeting in his and John Thresher; Gunther Plass at the age of only 32, the youn• honour, he wrote 'scientists are as Director of Accelerators; gest ever to be so honoured. -
Abraham Seiden Santa Cruz Institue for Particle Physics (SCIPP) UC Santa Cruz Department of Physics
Abraham Seiden Santa Cruz Institue for Particle Physics (SCIPP) UC Santa Cruz Department of Physics PROFESSIONAL PREPARATION Columbia University Applied Physics B.S. 1967 California Institute of Technology Physics M.S. 1970 University of California, Santa Cruz Physics Ph.D. 1974 POST DOCTORAL APPOINTMENTS 1975-1976 Postdoctoral Research Scientist, High Energy Physics, University of California, Santa Cruz 1974-1975 Visiting Scientist, CERN APPOINTMENTS 2008-present Distinguished Professor of Physics, University of California, Santa Cruz 1981-2010 Director, Santa Cruz Institute for Particle Physics 1986-2008 Professor of Physics, University of California, Santa Cruz 1985-1986 Visiting Scientist, European Laboratory for Particle Physics (CERN) 1981-1985 Associate Professor of Physics, University of California, Santa Cruz 1978-1981 Assistant Professor of Physics, University of California, Santa Cruz 1976-1978 Assistant Professor of Physics in Residence, University of California, Santa Cruz SELECTED PUBLICATIONS PERTINENT TO THIS PROPOSAL (Primary Author Only) 1. Characteristics of the ATLAS and CMS Detectors. A. Seiden, Phil. Trans. R. Soc., 370 no. 1961, 892 (2012). 2. Comparing radiation tolerant materials and devices for ultra rad-hard tracking detectors. M. Bruzzi, H.F.W. Sadrozinski, A. Seiden, Nucl.Instrum.Meth. A579:754 (2007). 3. Radiation-hard semiconductor detectors for Super LHC. M. Bruzzi et al. Nucl. Instrum. Meth. A 541: 189 (2005). 4. Tracking detectors for the sLHC, the LHC upgrade. H.F.W. Sadrozinski and A. Seiden, Nucl. Instrum. Meth. A 541: 434 (2005) 5. Ionization Damage on Atlas-SCT Front-End Electronics considering Low-Dose-Rate Effects. M. Ullan et al., IEEE Trans. Nucl. Sci. 49:1106, (2002). -
The ISR Legacy
! Subnuclear Physics: Past, Present and Future ! Pontifical Academy of Sciences, Scripta Varia 119, Vatican City 2014 ! www.pas.va/content/dam/accademia/pdf/sv119/sv119-darriulat.pdf ! ! The ISR Legacy P!IERRE D!ARRIULAT ! ! ! VATLY!Astrophysics!Laboratory,!Hanoi,!Vietnam! ! ! 1.!Introduction! It!so!happens!that!the!life!time!of!the!CERN!Intersecting!Storage!Rings!(ISR),! roughly!!speaking!!the!!seventies,!!coincides!!with!!a!!giant!!leap!!in!!our!!understanding!!of! particle!physics:!the!genesis!of!the!Standard!Model.!Those!of!us!who!have!worked!at!the! ISR!remember!these!times!with!the!conviction!that!we!were!not!merely!spectators!of!the! ongoing!progress,!but!also!–!admittedly!modest!–!actors.!While!the!ISR!contribution!to! the!!electroweak!!sector!!is!!indeed!!negligible,!!its!!contribution!!to!!the!!strong!!sector!!is! essential!and!too!often!unjustly!forgotten!in!the!accounts!that!are!commonly!given!of!the! progress!of!particle!physics!during!that!!period.!In!the!present!article,!I!shall!use!three! topics!to!illustrate!how!important!it!has!been:!the!production!of!hadrons,!large!transverse! momentum!final!states!and!the!rising!total!cross-section.! When!!Vicky!!Weisskopf,!!in!!December!!1965,!!in!!his!!last!!Council!!session!!as! Director-General,!obtained!approval!for!the!construction!of!the!ISR,!there!was!no!specific! physics!issue!at!stake,!which!the!machine!was!supposed!to!address;!its!only!justification! was!!to!!explore!!the!terra!!incognita!!of!higher!!centre!of!mass!energy!collisions!(to!!my! knowledge,!!since!!then,!!all!!new!!machines!!have!!been!!proposed!!and!!approved!!with!!a! -
Jan/Feb 2015
I NTERNATIONAL J OURNAL OF H IGH -E NERGY P HYSICS CERNCOURIER WELCOME V OLUME 5 5 N UMBER 1 J ANUARY /F EBRUARY 2 0 1 5 CERN Courier – digital edition Welcome to the digital edition of the January/February 2015 issue of CERN Courier. CMS and the The coming year at CERN will see the restart of the LHC for Run 2. As the meticulous preparations for running the machine at a new high energy near their end on all fronts, the LHC experiment collaborations continue LHC Run 1 legacy to glean as much new knowledge as possible from the Run 1 data. Other labs are also working towards a bright future, for example at TRIUMF in Canada, where a new flagship facility for research with rare isotopes is taking shape. To sign up to the new-issue alert, please visit: http://cerncourier.com/cws/sign-up. To subscribe to the magazine, the e-mail new-issue alert, please visit: http://cerncourier.com/cws/how-to-subscribe. TRIUMF TRIBUTE CERN & Canada’s new Emilio Picasso and research facility his enthusiasm SOCIETY EDITOR: CHRISTINE SUTTON, CERN for rare isotopes for physics The thinking behind DIGITAL EDITION CREATED BY JESSE KARJALAINEN/IOP PUBLISHING, UK p26 p19 a new foundation p50 CERNCOURIER www. V OLUME 5 5 N UMBER 1 J AARYN U /F EBRUARY 2 0 1 5 CERN Courier January/February 2015 Contents 4 COMPLETE SOLUTIONS Covering current developments in high-energy Which do you want to engage? physics and related fi elds worldwide CERN Courier is distributed to member-state governments, institutes and laboratories affi liated with CERN, and to their personnel. -
Prof. Terry Wyatt FRS Employment History Education Fellowships And
CURRICULUM VITAE — Prof. Terry Wyatt FRS Born: 29th June 1957, Watford, England. Nationality: British. Family Status: Married, with two sons. Employment History Tenured Physics Faculty: School of Physics and Astronomy, University of Manchester, UK. – Professor (2004–present) [DØ and ATLAS experiments] – Reader (1999–2004) [OPAL and DØ experiments] – Lecturer (1996–1999) [OPAL experiment] – Senior visiting appointments, on leave from usual academic duties at University of Manchester: Guest Scientist, Fermilab: 15 month period as Paid Guest Scientist at Fermilab (2002–2003) PPARC Senior Research Fellowship: 3-year period (2003-2006) STFC support for DØ spokesperson: 100% salary buy-out for 18 month period (2006–2007). As spokesperson of DØ I also received financial support from Fermilab. – I currently serve as Chair of the Accelerator, Nuclear and Particle Physics Division of the School of Physics and Astronomy, with overall responsibility for both experimental and theoretical aspects of these fields. PPARC Advanced Research Fellow: Based at CERN with University of Manchester, UK. (1989–1996). [OPAL experiment]. PPARC Research Associate: QMC, University of London, UK. (1986–1989). [OPAL experiment] CERN Fellow: CERN, Geneva, Switzerland. (1984–1986). [UA1 experiment] Education Research Student: University of Oxford, UK. (1979–1983). [TASSO experiment] Degree: D.Phil. Undergraduate Student in Physics: Imperial College, University of London, UK. (1976–1979). Degree: B.Sc. (Ist class hons. Awarded governors’ prize for top first in physics, 1979). Associateship of the Royal College of Science (A.R.C.S). Fellowships and Prizes • Elected as Fellow of the Royal Society, FRS (2013). Excerpt from citation: “Distinguished for a number of original and important contributions to the experimental verification of the Standard Model”. -
Power for Modern Detectors
I NTERNAT I ONAL J OURNAL OF H I G H - E NERGY P H YS I CS CERNCOURIER WELCOME V OLUME 5 8 N UMBER 9 N O V EMBER 2 0 1 8 CERN Courier – digital edition Welcome to the digital edition of the November 2018 issue of CERN Courier. Physics through Explaining the strong interaction was one of the great challenges facing theoretical physicists in the 1960s. Though the correct solution, quantum photography chromodynamics, would not turn up until early the next decade, previous attempts had at least two major unintended consequences. One is electroweak theory, elucidated by Steven Weinberg in 1967 when he realised that the massless rho meson of his proposed SU(2)xSU(2) gauge theory was the photon of electromagnetism. Another, unleashed in July 1968 by Gabriele Veneziano, is string theory. Veneziano, a 26-year-old visitor in the CERN theory division at the time, was trying “hopelessly” to copy the successful model of quantum electrodynamics to the strong force when he came across the idea – via a formula called the Euler beta function – that hadrons could be described in terms of strings. Though not immediately appreciated, his 1968 paper marked the beginning of string theory, which, as Veneziano describes 50 years later, continues to beguile physicists. This issue of CERN Courier also explores an equally beguiling idea, quantum computing, in addition to a PET scanner for clinical and fundamental-physics applications, the internationally renowned Beamline for Schools competition, and the growing links between high-power lasers (the subject of the 2018 Nobel Prize in Physics) and particle physics. -
DPF NEWSLETTER - July 1, 1994
DPF NEWSLETTER - July 1, 1994 To: Members of the Division of Particles and Fields From: Robert N. Cahn, Secretary-Treasurer, [email protected] HEPAP Subpanel Reports The HEPAP Subpanel on Vision for the Future of High-Energy Physics has issued its report, which was endorsed by HEPAP itself. The Conclusions and Recommendations are given below: Conclusion 1 We have inherited a great tradition of scientific inquiry. The field of particle physics has made dramatic progress in understanding the fundamental structure of matter. Recent discoveries and technological advances enable us to address such compelling scientific issues as the origin of mass, the underlying cause of the preponderance of matter over antimatter, and the nature of the invisible matter that accounts for up to 90% of the mass of the universe. Recommendation 1 As befitting a great nation with a rich and successful history of leadership in science and technology, the United States should continue to be among the leaders in the worldwide pursuit of the answers to fundamental questions of particle physics. Conclusion 2 To sustain excellence in the U.S. high-energy physics program for two decades and beyond, three elements are essential. a flexible, diverse, and dynamic ongoing research effort to address scientifically compelling questions. This implies strong support for university groups, effective use and timely upgrades of domestic accelerators, and an active program of nonaccelerator-based inquiries. vigorous studies to develop and master the technologies for future accelerators and detectors, and significant participation at the highest energy frontier, for which the best current opportunity beyond the Tevatron is through international collaboration on the LHC at CERN. -
Sandbox Studio 9 Symme
it on symmetry | volume 03 issue 10 december 06 Photos: Sandbox Studio 9 Physicist Michael Weber (right, Fermilab) and his colleagues (from left) Michael Kirby (Radboud University Nijmegen, Netherlands), Chris Neu (University of Pennsylvania), Sabine Lammers (Columbia University), Ben Kilminster (Ohio State University) as well as other experimenters at CDF and DZero are hitting upon numerous discoveries. Photo: Sandbox Studio As work continues to complete the Large Hadron Collider in Europe and plans develop around the world for an International Linear Collider, one acceler- ator at the energy frontier is open for business right now. At Fermilab in Batavia, Illinois, the Tevatron collider is making discoveries. Michael Weber is working late this Tuesday night in mid- November, crunching data from his desk in a cubicle in Fermilab’s DZero building. He’s analyzing data collected by the DZero collider experiment. He is determined to wring every drop of information from the experiment’s vast and growing hoard of data. Just across the Tevatron ring, the scene is similar for Laura Sartori, working on the CDF experi- ment. Michael and Laura are looking for discoveries that could change particle physics forever. And the clock is ticking. Michael and Laura are not alone—far from it. Almost 1400 sci- entists, members of the CDF and DZero collaborations, are pouring on the effort to make the most of the US accelerator’s final run before CERN’s Large Hadron Collider takes over the energy frontier later in the decade. Long after normal working hours, the lights burn in the cubicles of the CDF and DZero offices as experimenters search for the tell-tale tracks that might lead them toward a sighting of supersymmetry, extra dimensions, dark matter, exotic particles, and a host of other phenomena that no one on the planet has ever seen before.