Technology and Components of Accelerator-Driven Systems, © Oecd 2015 Nea/Nsc/Doc(2015)7
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People and Things
People and things On 15 April, Haim Harari of the Weizmann Institute, Israel, was guest speaker at a symposium to mark 20 years of accelerator operation at the Paul Scherrer Institute, Maurice Jacob's roving camera caught Murray Villigen, Switzerland. Gell Mann in a London pub with the manu (Photo Armin Muller) script of his book 'The Quark and the Jaguar'. 20 years of PSI In April the Swiss Paul Scherrer Institute celebrated 20 years of accelerator operations. Originally built for particle research, these facilities now extend over a wide spectrum of applications, from molecular structure to cancer therapy. Each year over 400 visiting researchers make use of PSI particle beams. Meetings An international symposium on strangeness and quark matter will be held from 1-5 September in Crete, covering 1. strangeness and quark- gluon plasma, 2. strangeness con LAPP, Annecy, well known authority French Academy of Sciences densation, 3. strange astrophysics, 4. on non-Abelian gauge theories, and strangelets, 5. dedicated instrumen Michel Davier, long-time specialist in tation for strangeness and quark Among the new corresponding electron-positron collision physics matter. Information from the Secre members of the French Academy of and former Director of the Orsay tariat, University of Athens, Physics Sciences (Academie des Sciences Linear Accelerator Laboratory. Other Dept., Nuclear & Particle Physics de Paris) are Raymond Stora of new members are Alain Aspect, Division, Panepistimioupolis, Greece- 15771 Athens, tel. (30-1)7247502, 7243362, 7243143, fax (30- 1)7235089, email gvassils ©atlas, uoa.ariadne-t.gr At a special colloquium held at CERN on 20 April to mark Carlo Rubbia's 60th birthday and the tenth anniversary of his Nobel Prize award with Simon van der Meer, left to right - Canadian TRIUMF Laboratory Director and former UA1 co-spokesman Alan Astbury, LHC Project Director Lyn Evans, Carlo Rubbia, Director General Chris Llewellyn Smith, and former UA 1 co-spokesman John Dowel I. -
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! -
The 1984 Nobel Prize in Physics Goes to Carlo Rubbia and Simon Vm Der Meer: R
arrent Comments” EUGENE GARFIELD INSTITUTE FOR SCIENTIFIC INFORMATION* 3501 MARKET ST,, PHILADELPHIA, PA !9104 The 1984 Nobel Prize in Physics Goes to Carlo Rubbia and Simon vm der Meer: R. Bruce Merrifield Is Awarded the Chemistry Prize I Number 46 November 18, 1985 Last week we reviewed the 1984 Nobel Rubbia, van der Meer, and the hun- laureates in medicine: immunologists dreds of scientists and technicians at Niels K. Jerne, Georges J.F. Kohler, and CERN were seeking the ultimate confir- C6sar Milstein. 1 In this week’s essay the mation of what is known as the electro- prizewinners in physics and chemistry weak theory. Thk theory states that two are discussed. of the fundamental forces—electromag- The 1984 physics prize was shared by netism and the weak force-are actually Carlo Rubbia, Harvard University and facets of the same phenomenon. The the European Center for Nuclear Re- 1979 Nobel Prize in physics was shared search (CERN), Geneva, Switzerland, by Sheldon Glashow and Steven Wein- and Simon van der Meer, also of CERN. berg, Harvard, and Abdus Salam, Impe- The Nobel committee honored “their rial College of London, for their contri- decisive contributions.. which led to the butions to the eiectroweak theory. I dk- discovery of the field particles W and Z, cussed their work in my examination of communicators of the weak interac- the 1979 Nobel Iaureates.s tion. ”z The 1984 Nobel Prize in chemis- The daunting task facing the scientists try was awarded to R. Bruce Mertileld, at CERN was to find evidence of the sub- Rockefeller University, New York, for atomic exchange particles that commu- his development of a “simple and in- nicate the weak force. -
1 Nothing Is New Under the Sun ! Prof. Dr. Dr. Carlo Rubbia Scientific
Nothing is new under the Sun ! Prof. Dr. Dr. Carlo Rubbia Scientific Director, Institute for Advanced Sustainability Studies e.V. Potsdam, Germany -Accompanying document to Prof. Rubbia’s keynote address during the 3rd Dii Desert Energy Conference (Berlin, November 7-9 2012). The beginning of the practical use of solar power goes back some 23 centuries ago with Archimedes of Syracuse, (287 BC to 212 BC) in sunny Sicily. Mathematician, physicist, engineer, inventor and astronomer, he has been one of the leading scientists of the classical antiquity. The written work of Archimedes has not survived as well as that of Euclid, and seven of his treatises are known to have existed only through references made to them by other authors. Only few details are known. However, the relatively few copies of Archimedes' written work that survived through the Middle Ages were an influential source of ideas for scientists during the Renaissance. His contributions in mathematics have been immense: the initiator of the infinitesimals, anticipating the modern calculus of the ratio between the square of the radius and the area of a circle, the quadrature of a parabola as the solution of an infinite series, the centre of gravity of geometric figures and so on. The Fields Medal, the equivalent of the Nobel in mathematics carries his portrait along with a carving illustrating his proof on the sphere and the cylinder. The inscription is a quote attributed to him, which reads in Latin: "Transire suum pectus mundoque potiri" (Rise above oneself and grasp the world). Among his advances in physics are the foundations of hydrostatics, refraction and parabolic concentration of light, statics and an explanation of the principle of the lever, where he said “Give me a place to stand on, and I will move the Earth”. -
Advanced Information on the Nobel Prize in Physics, 5 October 2004
Advanced information on the Nobel Prize in Physics, 5 October 2004 Information Department, P.O. Box 50005, SE-104 05 Stockholm, Sweden Phone: +46 8 673 95 00, Fax: +46 8 15 56 70, E-mail: [email protected], Website: www.kva.se Asymptotic Freedom and Quantum ChromoDynamics: the Key to the Understanding of the Strong Nuclear Forces The Basic Forces in Nature We know of two fundamental forces on the macroscopic scale that we experience in daily life: the gravitational force that binds our solar system together and keeps us on earth, and the electromagnetic force between electrically charged objects. Both are mediated over a distance and the force is proportional to the inverse square of the distance between the objects. Isaac Newton described the gravitational force in his Principia in 1687, and in 1915 Albert Einstein (Nobel Prize, 1921 for the photoelectric effect) presented his General Theory of Relativity for the gravitational force, which generalized Newton’s theory. Einstein’s theory is perhaps the greatest achievement in the history of science and the most celebrated one. The laws for the electromagnetic force were formulated by James Clark Maxwell in 1873, also a great leap forward in human endeavour. With the advent of quantum mechanics in the first decades of the 20th century it was realized that the electromagnetic field, including light, is quantized and can be seen as a stream of particles, photons. In this picture, the electromagnetic force can be thought of as a bombardment of photons, as when one object is thrown to another to transmit a force. -
Abundant Thorium As an Alternative Nuclear Fuel Important Waste Disposal and Weapon Proliferation Advantages
Energy Policy 60 (2013) 4–12 Contents lists available at SciVerse ScienceDirect Energy Policy journal homepage: www.elsevier.com/locate/enpol Abundant thorium as an alternative nuclear fuel Important waste disposal and weapon proliferation advantages Marvin Baker Schaffer n RAND Corporation, 1776 Main Street, Santa Monica, CA 90407, United States HIGHLIGHTS Thorium is an abundant nuclear fuel that is well suited to three advanced reactor configurations. Important thorium reactor configurations include molten salt, CANDU, and TRISO systems. Thorium has important nuclear waste disposal advantages relative to pressurized water reactors. Thorium as a nuclear fuel has important advantages relative to weapon non-proliferation. article info abstract Article history: It has long been known that thorium-232 is a fertile radioactive material that can produce energy in Received 10 May 2012 nuclear reactors for conversion to electricity. Thorium-232 is well suited to a variety of reactor types Accepted 26 April 2013 including molten fluoride salt designs, heavy water CANDU configurations, and helium-cooled TRISO- Available online 30 May 2013 fueled systems. Keywords:: Among contentious commercial nuclear power issues are the questions of what to do with long-lived Thorium radioactive waste and how to minimize weapon proliferation dangers. The substitution of thorium for Non-proliferation uranium as fuel in nuclear reactors has significant potential for minimizing both problems. Nuclear waste reduction Thorium is three times more abundant in nature than uranium. Whereas uranium has to be imported, there is enough thorium in the United States alone to provide adequate grid power for many centuries. A well-designed thorium reactor could produce electricity less expensively than a next-generation coal- fired plant or a current-generation uranium-fueled nuclear reactor. -
The Energy Amplifier, an "Ecological" Reactor
The Energy Amplifier, an "Ecological" Reactor Christos A. Eleftheriadis Nuclear Physics and Elementary Particles Division Aristotle University of Thessaloniki Abstract The main ideas for the Energy Amplifier (EA) are presented, as they have been developed at CERN [1]. The discussion concerns with the safety and environmental features of this new kind of reactor which are far more better than the ones of the conventional reactors. A comparison is also given with fusion reactors and other non-nuclear methods for energy production, such as coal burning. 1. Introduction It is more than certain that the role of safety and environmental features will be of major importance in any decision concerning large scale human activities, such as energy production. All the methods have an undesired impact on the environment, the nature of this impact being dependent on the specific method in use. For instance, all the methods based on carbon burning, that is release of chemical energy from coal or oil, add on the CO2 in the atmosphere and, consequently, on the Greenhouse effect. Natural gas is better in this sense, due to its high hydrogen content. Moreover, sulphur oxides coming from burning already proved to be a serious problem for the environment. Nuclear fission reactors do not contribute to the Greenhouse effect and relevant problems, since they do not produce CO2, sulphur oxides etc. On the other hand they exhibit a number of negative points, first of all the potential danger for a large scale accident, such as the one in Chernobyl. This danger is common in all power reactors, since they all operate at the critical point. -
Transmutation Potential of the Energy Amplifier Demonstration Facility Calculated with the EA-MC Code Package
the united nations educational, scientific i and cultural organization international centre for theoretical physics international atomic energy agency SMR/1326-9 Workshop on Hybrid Nuclear Systems for Energy Production, Utilisation of Actnides Si Transmutation of Long-Lived Radioactive Waste 3-7 September 2001 Miramare - Trieste, Italy Transmutation Potential of the Energy Amplifier Demonstration Facility Calculated with the EA-MC Code Package Yacine Kadi CERN, Switzerland strada costiera, II - 34014 trieste italy - tel. +39 0402240 III fax +39 040224163 - [email protected] - www.ictp.trieste.it Transmutation Potential of the Energy Amplifier Demonstration Facility Calculated with the EA-MC Code Package Yacine Kadi Emerging Energy Technologies European Organization for Nuclear Research CERN, Geneva (Switzerland) Yacine. kadi @ cern. ch Abstract The neutronic calculations presented in this paper are a result of a state-of-the-art computer code package developed by the EET group at CERN. Both high-energy particle interactions and low-energy neutron transport are treated with a sophisticated method based on a full Monte Carlo simulation, together with modern nuclear data libraries. The code is designed to run both on parallel and scalar computers. A series of experiments carried out at the CERN-PS (i) confirmed that the spallation process is correctly predicted and (ii) validated the reliability of the predictions of the integral neutronic parameters of the Energy Amplifier Demonstration Facility. 1 Introduction The sequence of phenomena from high-energy protons induced cascade in a heavy-Z material (lead or lead-bismuth eutectic), producing neutrons that subsequently interact until they are finally absorbed or escape, is rather complex. -
Standard Model Rohini M. Godbole Centre for High
Standard Model. Rohini M. Godbole Standard Model Rohini M. Godbole Centre for High Energy Physics, IISc, Bangalore, India & Currently at: Spinoza Institute, Univ. of Utrecht, Utrecht, The Netherlands July 11 - July 15, 2011. CERN Summer Student Program. Standard Model. What will the lectures cover? Issues concerning the Standard Model of particle physics: Even though we call it a model it is actually the candidate for the ’theory’ of the fundamental particles and interactions among them! Built, brick by brick, over the last 50-60 years, combining information from a lot of different types of experiments and many many innovative theoretical ideas. The basic mathematical framework is that of quantum field theories (QFT) which possess some special properties (symmetries). Some aspects of these will be covered in lectures by Prof. Deredinger. July 11 - July 15, 2011. CERN Summer Student Program. Standard Model. What will the lectures cover? Using this information I intend then to cover the following : • How did we find out about the fundamental constituents and inter- actions among them. • How did we arrive at an understanding of the symmetries and hence a gauge theory description of the same: how was the SM built? • What is the significance of the different families of quarks and leptons: flavour physics. • What is the piece of the SM still left to be checked and how does the theory guide us about how and where to look for the missing piece. July 11 - July 15, 2011. CERN Summer Student Program. Standard Model. Nobels for Standard Model Among the Nobels awarded for physics till to date, 15 are for Standard Model: 1. -
Vermont Energy Amplifier.Pdf
The Energy Amplifier in Vermont George Harvey The problem of what to do with nuclear waste is enormous. The approach attempted by the US federal government, burial in geologically stable ground at Yucca Mountain, has failed. This should come without surprise – even if it were a good idea, and there are those who assert it is not, no state is willing to host such a site. But it is distressing that no alternative is being seriously pursued at present. As it happens, other ideas range from dangerous to deadly. At one time it was believed nuclear waste could simply be dumped into the sea, and some of it has been, but high- level nuclear waste is a very bad pollutant because the elements present are very toxic and long-lived. It has been suggested that we shoot it into space, but given the amount we need to get rid of, a catastrophic accident would be nearly a certainty. Every year we make millions of pounds of this waste, every year we argue over what to do about it, and every year we just add it to the stockpile of what has already been produced. Here in Vermont it sits on the banks of New England’s largest river. The waste at Vermont Yankee (VY) is to be stored just out of the 500-year flood area, by elevating it five inches above the flood water line. While this is not good storage, it is at least better than shooting it into space. Every once in a while technology comes to the rescue, and it seems this may be one of those occasions. -
Thorium: an Energy Source for the World of Tomorrow
EPJ Web of Conferences 98, 000(5 2 2015) DOI: 10.1051/epjconf/2015980005 2 C Owned by the authors, published by EDP Sciences - SIF, 2015 Thorium: An energy source for the world of tomorrow J.-P. Revol Centro Studi e Ricerche “Enrico Fermi” - Roma, Italy and International Thorium Energy Committee (iThEC) - Geneva, Switzerland Summary. — To meet the tremendous world energy needs, systematic R&D has to be pursued to replace fossil fuels. Nuclear energy, which produces no green house gases and no air pollution, should be a leading candidate. How nuclear energy, based on thorium rather than uranium, could be an acceptable solution is discussed. Thorium can be used both to produce energy and to destroy nuclear waste. The thorium conference, organized by iThEC at CERN in October 2013, has shown that thorium is seriously considered by some major developing countries as a key element of their energy strategy. However, developed countries do not seem to move fast enough in that direction, while global cooperation is highly desirable in this domain. Thorium is not fissile. Various possible ways of using thorium will be reviewed. However, an elegant option is to drive an “Accelerator Driven System (ADS)” with a proton accelerator, as suggested by Nobel Prize laureate Carlo Rubbia. 1. – Burning fossil fuel till the end? If, by the end of the 21st century, people in developing countries are allowed to live as well as people do in Europe today, the world power consumption will have to increase by a factor three or more. Europe is not representative of the world. -
The “Boggart” of Particle Physics
The “Boggart” of Particle Physics Dept of Physics Pradipta Ghosh 26th March, 2021 March 26, 2021 1 / 19 “Hogwarts” of the Particle Physics The Standard Model The Inmates and Laws Elementary Particles Basic Interactions and mediators Not included in the Standard Model Image acknowledgement: Harry Potter Wiki, Wikipedia March 26, 2021 2 / 19 Hogwarts of the Particle Physics: The inmates Elementary Particles and Mediators DOD: 4 July 2012 The missing piece 1964-2012 1 eV/c2 = 1.783×10−36 kg C = 1 in natural unit system Neutrinos are Mass-less in the Standard Model Image acknowledgement: Wikipedia March 26, 2021 3 / 19 Theory: Glashow, 1961, Weinberg, 1967, Salam, 1968 1979 Sheldon Steven Abdus Glashow Weinberg Salam “Hogwarts” of Particle Physics: Founders Theory: Greenberg, 1964, Han, Nambu, 1964, Bardeen, Fritzsch, Gell-Mann, 1973 C. R. Tom Gerald Theory: Hagen Guralnik 1973 Kibble 2004 David H. D. F. Wilczek Gross Politzer François Theory: Nambu, Peter Englert Jona-Lasinio 1961 Higgs 1999 Robert Gerard Martinus 2013 Brout 2008 't Hooft J. G. Veltman Theory: Brout, Englert, Higgs, Guralnik, Hagen, Kibble, 1964 Yoichiro Nambu Image acknowledgement: Wikipedia March 26, 2021 4 / 19 Muon S. Neddermeyer Electron (1936) (1897) Theory: Pauli, 1930 Tau e-Neutrino (1975) (1956) 1995 Martin Clyde C. D. Anderson Cowan 1995 1906 Lewis Perl t-Neutrino Frederick m-Neutrino (1962) (2000) Carlo Rubbia Reines J. J. Thomson Theory: 1940 DONUT Coll. Theory: 1970 Simon van der Meer 1984 + - 1988 W ,W ,Z UA1, UA2 (1983) CERN Leon M. Melvin Jack The Seekers Theory: Glashow, Weinberg, Salam, 1968 Lederman Schwartz Steinberger Theory: 1973 Gluons Light quarks DORIS (1978) (up,down,strange) PETRA (1979) SLAC (1968) DESY 2008 Theory: Gell-Mann, 1962 T.