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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. -
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 Mar (E) K of QGP: Strangeness
The Mar(e)k of QGP: Strangeness∗ Jan Rafelski Department of Physics, The University of Arizona Tucson, AZ 85721, USA Strangeness signature of of quark-gluon plasma (QGP) is central to the exploration of baryon-dense matter: the search for the critical point and onset of deconfinement. I report on the discovery of QGP by means of strangeness: The key historical figures and their roles in this quest are introduced and the experimental results obtained are discussed. The im- portant role of antihyperons is emphasized. The statistical hadronization model, and sudden hadronization are described. Results of present day data analysis: strangeness and entropy content of a large fireball, and the universal hadronization condition describing key features of all explored collision systems are presented. PACS numbers: 25.75.-qRelativistic heavy-ion collisions 12.38.MhQuark-gluon plasma 24.10.PaThermal and statistical models 1. Introduction The introduction in 1964 of the new quark paradigm [1] `happened' nearly in parallel to the rise of the thermal model of hadron production pre- cipitated by Hagedorn's invention of the statistical bootstrap model, for a review of Hagedorn's work, see Ref. [2]. The paradigm of quarks explained a large number of properties of elementary particles, allowing at the time one prediction, a new particle, the triple-strange Ω−(sss). On the other hand Hagedorn was following fragmentary experimental data on particle produc- tion; these data were not in agreement with the rudimentary statistical arXiv:1701.00296v2 [hep-ph] 6 Feb 2017 particle production models proposed by Koppe [3] and Fermi [4]. Hage- dorn's work is a classic example of a discovery case where theory preceded experiment, focusing the direction of future experimental work. -
Before Matter As We Know It Emerged, the Universe Was Filled with The
Cambridge University Press 0521385369 - Hadrons and Quark–Gluon Plasma Jean Letessier and Johann Rafelski Frontmatter More information HADRONS AND QUARK–GLUON PLASMA Before matter as we know it emerged, the universe was filled with the primordial state of hadronic matter called quark–gluon plasma. This hot soup of quarks and gluons is effectively an inescapable consequence of our current knowledge about the fundamental hadronic interactions: quantum chromodynamics. This book covers the ongoing search to verify the prediction experimentally and discusses the physical properties of this novel form of matter. It provides an accessible introduction to the recent developments in this interdisciplinary field, covering the basics as well as more advanced material. It begins with an overview of the subject, followed by discussion of experimental methods and results. The second half of the book covers hadronic matter in confined and deconfined form, and strangeness as a signature of the quark–gluon phase. A firm background in quantum mechanics, special relativity, and statistical physics is assumed, as well as some familiarity with particle and nuclear physics. However, the essential introductory elements from these fields are presented as needed. This text is suitable as an introduction for graduate students, as well as pro- viding a valuable reference for researchers already working in this and related fields. JEAN LETESSIER has been CNRS researcher at the University of Paris since 1978. Prior to that he worked at the Institut de Physique Nucleaire, Orsay, where he wrote his thesis on hyperon–nucleon interaction in 1970, under the direction of Professor R. Vinh Mau, and was a teaching assistant at the University of Bordeaux. -
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! -
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. -
Subnuclear Physics: Past, Present and Future
the Pontifical academy of ScienceS International Symposium on Subnuclear Physics: Past, Present and Future 30 Octobe r- 2 November 2011 • Casina Pio IV Introduction p . 3 Programme p. 4 List of Participants p. 8 Biographies of Participants p. 11 Memorandum p. 20 em ad ia c S a c i e a n i t c i i a f i r t V n m o P VatICaN CIty 2011 H.H. Benedict XVI in the garden of the Basilica di Santa Maria degli angeli e dei Martiri with the statue of “Galilei Divine Man” donated to the Basilica by CCaSt of Beijing. he great Galileo said that God wrote the book of nature in the form of the language of mathematics. He was convinced that God has given us two tbooks: the book of Sacred Scripture and the book of nature. and the lan - guage of nature – this was his conviction – is mathematics, so it is a language of God, a language of the Creator. Encounter of His Holiness Benedict XVI with the Youth , St Peter’s Square, thursday, 6 april 2006. n the last century, man certainly made more progress – if not always in his knowledge of himself and of God, then certainly in his knowledge of the macro- Iand microcosms – than in the entire previous history of humanity. ... Scientists do not create the world; they learn about it and attempt to imitate it, following the laws and intelligibility that nature manifests to us. the scientist’s experience as a human being is therefore that of perceiving a constant, a law, a logos that he has not created but that he has instead observed: in fact, it leads us to admit the existence of an all-powerful Reason, which is other than that of man, and which sustains the world. -
Program ICGAC10
RENCONTRES DU VIETNAM Qui Nhon, Vietnam December 17-22, 2011 Xth International Conference on Gravitation, Astrophysics and Cosmology ( I C G A C 1 0 ) P ROGRAM Saturday 17 December 2011 07:30 - 12:00 : Arrival of participants 12:00 - 14:00 : Lunch 14:30 - 18:30 : Registration 18:30 - 19:15 : Welcome cocktail 19:15 - 21:00 : Dinner Sunday 18 December 2011 07:30 - 10:00 : Ground breaking of the International Center of Interdisciplinary Science Education (ICISE) Departure to ICISE (07:30) from Seagull Hotel — Ceremony (08:00 - 09:15) — Departure to Seagull Hotel (09:15) — PL E N A R Y S E S S I O N — 09:45 - 10:30 : Opening of ICGAC10 & EDS 10:30 - 11:00 : Refreshment — Coffee Break 11:00 - 11:40 :Viscosity and black holes | Dam Thanh Son — Institute for Nuclear Theory, University of Washington 11:40 - 12:30 : Comparison of Hadronic Interaction Models with LHC Data | Tanguy Pirog — Karlsruhe Institute of Technology 12:30 - 13:00 : Discussion about ICISE 13:00 - 14:00 : Lunch 14:00 - 14:30 : Did the universe have a beginning ? | Alex Vilenkin — Tufts University 14:30 - 15:00 : G-inflation | Masahide Yamaguchi — Tokyo Institute of Technology 15:00 - 15:30 : Confronting Inflation with Observations | Viatcheslav Mukhanov — Ludwig Maximilians Universität 15:30 - 16:00 : Coffee Break 16:00 - 16:30 : Cosmic Microwave Background | Naoshi Sugiyama — Nagoya University 16:30 - 17:00 : Recent results on measurements and interpretation of the CMB fluctuations | Andrey Doroshkevich — Astro Space Center of the Lebedev Physical Institute 17:00 - 17:30 : Measurements of the CMB with WMAP and ACT | Mark Halpern — University of British Columbia 17:30 - 18:00 : Gravitational Lensing in Plasma | Oleg Tsupko — Space Research Institute of Russian Academy of Sciences 18:00 - 18:30 : The Primordial Abundance of 4^He | Evidence for Non-Standard Big Bang Nucleosynthesis | Trinh Xuan Thuan — Univ. -
The W and Z Particles: a Personal Recollection
W AND Z DISCOVERY The W and Z particles: a personal recollection Pierre Darriulat, who was spokesperson for the UA2 collaboration between 1978 and 1985, looks back at the events surrounding the discovery of the W and Z particles at CERN in 1983. The decade between 1967 and 1976 witnessed an impressive sequence of experimental and theoretical discoveries that changed the vision we had of the world - from the prediction of electroweak unification in the lepton sector (1967-1980) and the discovery of deep-inelastic electron scattering (1969), to asymptotic freedom and quantum chromodynamics (1973) and the discoveries of the J/W (1974) and naked charm (1976). By 1976 the Standard Model of particle physics was in place, ready to confront experi As soon as it was known that the 1984 Nobel Prize for Physics ments, and it was clear that a new accelerator was required to had been awarded to Carlo Rubbia and Simon Van der Meer, a explore the electroweak unification sector. This is where the weak celebration was organized in an experimental hall at CERN. The gauge bosons, W and Z, were expected, with approximate masses of happiness they radiate in this photograph was shared by the 65 and 80 GeV/c2, respectively. The arguments for the future LEP participants in the proton-antiproton project, who attended the machine were already strong. event and drank a glass in their honour. Undoubtedly, this was I remember being asked by John Adams (then executive director- one of the happiest days in the distinguished history of CERN. general of CERN) to convene the Large Electron Positron Collider (LEP) study group in April 1976, and to edit the report.