The 1984 Nobel Prize in Physics Goes to Carlo Rubbia and Simon Vm Der Meer: R

Total Page:16

File Type:pdf, Size:1020Kb

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. Theorists specu- genious” method for chemical synthesis lated that, in the same way that tiny par- on a solid matrix.J ticles of light called photons communi- Physics cate electromagnetism, the weak force is transmitted by another, related group of Rubbia and van der Meer were select- particles. These very dense communica- ed less than two years after the identifi- tors of the weak force-the so-called in- cation of the W and Z particles, a re- termediate vector bosons designated markably short period for recognition by W+, W –, and Z~had been predicted the Nobel committee. The scient~lc by Weinberg and Salam, independently achievement of these two physicists and of one another, in the late 1960s.6,7 The their colleagues culminated a half-cen- task of actually finding these particles tury of theory and experiments on the remained. Groups of scientists at CERN so-called “weak force. ” Along with grav- and at the National Accelerator Labora- ity, electromagnetism, and the “strong tory (Fermilab), Batavia, Illinois, had at- force” that binds together particles in tempted to release the W particle. But the atomic nucleus, the weak force is the particle accelerators at these facili- one of the four fundamental forces in the ties did not have enough power to pro- universe. The weak force is responsible duce particles of the mass that Weinberg for certain kinds of radioactive decay. It and Salam had predicted.a also controls the reactions that result in Rubbia proposed the use of a collider, the sun’s generation of energy.d which would smash together two coun- 432 ter-rotating beams—one composed of can be collided with the counter-rotat- protons, the other of antiprotons. The ing beam of protons. resulting collkions, according to Rubbia Another problem facing the scientists and his colleagues, would provide suffi- at CERN was detecting the effects of cient energy to reveal the W and Z parti- these proton-antiproton collisions. In cles. However, this idea presented for- 1978 Rubbia turned his efforts to the cre- midable obstacles. Rubbia had proposed ation of a detector in which the collision converting the existing accelerator at experiments would actually take place. Fermilab into a proton-antiproton col- This 2,000-ton device, named Under- lider, but his idea was rejected. He then ground Area 1 (UA 1), took three years took his plan to the European scientific and $20 million to build. 11Designed es- community and CERN. There, the idea sentially as a series of boxes within box- was approved. In 1978 the tremendous es, UA 1 comprised an intricate collec- effort began to convert CERNS four- tion of sensing devices and processors mile, underground Super Proton Syn- that enabled the scientists to detect the chrotrons into a proton-antiproton col- fleeting presence of the W and Z parti- lider. cles in the midst of all the particles creat- One of the most serious problems was ed in the collision of the two beams. An the production and storage of antipro- immensely complicated device, UA 1 set tons inside the collider. Antiprotons do new standards for detectors in collidlng- not exist in ordinary matter and must be beam experiments. A second, somewhat produced in h~gh-energy particle colh simpler detector, UA2, was added as a sions.z Accumulating the necessary mil- backup.z lions of antiprotons and regulating their Collision experiments began in 1981, passage around the collider was a key ex- but much of the key data were taken perimental problem. Rubbia turned to a from collider runs late the next year. Af- CERN colleague, Sirnon van der Meer. ter examining information from millions In 1968 van der Meer had written a of collision “events,” the scientists fo- paper (not published until 1972) that de- cused their attention on a handful of col- scribed “stochastic cooling”—a method lisions that seemed significant. Analysis for increasing the density of a beam of of the data showed signs of the predicted protons.g Work began at CERN to adapt “signature” of the W particle: a single van der Meer’s technique to the accumu- electron shooting off at a wide angle lation of an unprecedented quantity of from the colliding beams. Measure- antiprotons. ments of the energy expended during The efforts of van der Meer and his these collisions-the so-called “missing coworkers led to the construction of the energy’’-pointed to the existence of an- Antiproton Accumulator, a storage ring other signature particle, a neutrino. ThM 154 feet in diameter in which millions of all-but-invisible particle veered off from newly created antiprotons are “cooled” the collision in the opposite direction into a dense beam. Inside the ring, sen- with force equal to that of the electron. sors detect deviations in the individual Calculations showed that the mass of the orbits of the antiprotons, and, in mil- W particle was equivalent to that pre- lionths of a second, an electronic signal dicted by theoretical models. Rubbia’s is flashed across the chord of the circle UA1 group announced the discovery of to intercept and tighten the beam of an- the W particle in 1983, closely followed tiprotons as it races around the ring. by the UA2 group. 12.13The discovery of Both the beam and the correcting signal the Z particle came a few months lat- travel near the speed of light. 10The pro- er.14,15 cess is repeated millions of times until, after approximately 24 hours, enough Rubbia antiprotons have been accumulated to Rubbia was born in Gorizia, Italy, in be fed into the larger ring, where they 1934 and attended the University of Piss. 433 His graduate work in physics was com- our forthcoming study of the most-cited pleted at Columbia University, New 1983 articles in the physical sciences. York. In 1961 Rubbia returned to Eu- The most-cited paper, “Observation rope to join CERN. 16Since 1970 he has of new-particle production by high-en- divided his time between CERN, where ergy neutrinos and antineutrinos,” has he is senior physicist, and Harvard Uni- received over 300 citations since its pub- versit y, where he is a professor of phys- lication in 1975.17 Another highly cited ics. paper is “Small-angle proton-proton Using the Science Citation Index” elastic scattering at very high energies (SCF ), w have determined Rubbia’s (460 GeVz < s < 2900 GeVz),” pub- most-cited works for the period 1955- fished in 1972. la The work has been cited 1984. The list is based on ISI@’s internal 249 times. “all-author” data, since Rubbia does not Table 1 lists some of the 1S1 research appear as first author in any of the pa- fronts in which works by Rubbia, van pers. The fifth most-cited work is the der Meer, and colleagues are core docu- Physics Letters B paper in which Rubbia ments. The fronts cover 10 years of re- and colleagues announced the discovery search in high-energy particle physics. of the W particle. 12Although only two Some of these papers appear regularly in years old, this paper has already been our annual inventory of research fronts. cited over 170 times—a dramatic dem- A 1974 paper from Physical Revie w Let- onstration of its immediacy and impact. ters, for example, “Observation of mu- The bimonthly SCIS show that the paper onless neutrino-induced inelastic inter- also was cited in 56 publications in the actions, “ 1’3is core to six fronts, covering first six months of 1985. Also highly cited the years 1974 to 1980. is the paper by Rubbia and colleagues Three of the research fronts in Table 1 that discusses the identification of the Z appear in Figure 1, which presents the particle. 14This work has been cited over Klgher level map of cluster #83-0021, 160 times in the two years since publica- “Gauge theory of quark interactions and tion—and over 80 times in the first half jet production in high-energy collisions of 1985.
Recommended publications
  • 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.
    [Show full text]
  • Date: To: September 22, 1 997 Mr Ian Johnston©
    22-SEP-1997 16:36 NOBELSTIFTELSEN 4& 8 6603847 SID 01 NOBELSTIFTELSEN The Nobel Foundation TELEFAX Date: September 22, 1 997 To: Mr Ian Johnston© Company: Executive Office of the Secretary-General Fax no: 0091-2129633511 From: The Nobel Foundation Total number of pages: olO MESSAGE DearMrJohnstone, With reference to your fax and to our telephone conversation, I am enclosing the address list of all Nobel Prize laureates. Yours sincerely, Ingr BergstrSm Mailing address: Bos StU S-102 45 Stockholm. Sweden Strat itddrtSMi Suircfatan 14 Teleptelrtts: (-MB S) 663 » 20 Fsuc (*-«>!) «W Jg 47 22-SEP-1997 16:36 NOBELSTIFTELSEN 46 B S603847 SID 02 22-SEP-1997 16:35 NOBELSTIFTELSEN 46 8 6603847 SID 03 Professor Willis E, Lamb Jr Prof. Aleksandre M. Prokhorov Dr. Leo EsaJki 848 North Norris Avenue Russian Academy of Sciences University of Tsukuba TUCSON, AZ 857 19 Leninskii Prospect 14 Tsukuba USA MSOCOWV71 Ibaraki Ru s s I a 305 Japan 59* c>io Dr. Tsung Dao Lee Professor Hans A. Bethe Professor Antony Hewlsh Department of Physics Cornell University Cavendish Laboratory Columbia University ITHACA, NY 14853 University of Cambridge 538 West I20th Street USA CAMBRIDGE CB3 OHE NEW YORK, NY 10027 England USA S96 014 S ' Dr. Chen Ning Yang Professor Murray Gell-Mann ^ Professor Aage Bohr The Institute for Department of Physics Niels Bohr Institutet Theoretical Physics California Institute of Technology Blegdamsvej 17 State University of New York PASADENA, CA91125 DK-2100 KOPENHAMN 0 STONY BROOK, NY 11794 USA D anni ark USA 595 600 613 Professor Owen Chamberlain Professor Louis Neel ' Professor Ben Mottelson 6068 Margarldo Drive Membre de rinstitute Nordita OAKLAND, CA 946 IS 15 Rue Marcel-Allegot Blegdamsvej 17 USA F-92190 MEUDON-BELLEVUE DK-2100 KOPENHAMN 0 Frankrike D an m ar k 599 615 Professor Donald A.
    [Show full text]
  • 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!
    [Show full text]
  • De Nobelprijzen Komen Eraan!
    De Nobelprijzen komen eraan! De Nobelprijzen komen eraan! In de loop van volgende week worden de Nobelprijswinnaars van dit jaar aangekondigd. Daarna weten we wie in december deze felbegeerde prijzen in ontvangst mogen gaan nemen. De Nobelprijzen zijn wellicht de meest prestigieuze en bekende academische onderscheidingen ter wereld, maar waarom eigenlijk? Hoe zijn de prijzen ontstaan, en wie was hun grondlegger, Alfred Nobel? Afbeelding 1. Alfred Nobel.Alfred Nobel (1833-1896) was de grondlegger van de Nobelprijzen. Volgende week is de jaarlijkse aankondiging van de prijswinnaard. Alfred Nobel Alfred Nobel was een belangrijke negentiende-eeuwse Zweedse scheikundige en uitvinder. Hij werd geboren in Stockholm in 1833 in een gezin met acht kinderen. Zijn vader, Immanuel Nobel, was een werktuigkundige en uitvinder die succesvol was met het maken van wapens en stoommotoren. Immanuel wou dat zijn zonen zijn bedrijf zouden overnemen en stuurde Alfred daarom op een twee jaar durende reis naar onder andere Duitsland, Frankrijk en de Verenigde Staten, om te leren over chemische werktuigbouwkunde. In Parijs ontmoette bron: https://www.quantumuniverse.nl/de-nobelprijzen-komen-eraan Pagina 1 van 5 De Nobelprijzen komen eraan! Alfred de Italiaanse scheikundige Ascanio Sobrero, die drie jaar eerder het explosief nitroglycerine had ontdekt. Nitroglycerine had een veel grotere explosieve kracht dan het buskruit, maar was ook veel gevaarlijker om te gebruiken omdat het instabiel is. Alfred raakte geinteresseerd in nitroglycerine en hoe het gebruikt kon worden voor commerciele doeleinden, en ging daarom werken aan de stabiliteit en veiligheid van de stof. Een makkelijk project was dit niet, en meerdere malen ging het flink mis.
    [Show full text]
  • 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”.
    [Show full text]
  • 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.
    [Show full text]
  • Standard Model of Particle Physics, Or Beyond?
    Standard Model of Particle Physics, or Beyond? Mariano Quir´os High Energy Phys. Inst., BCN (Spain) ICTP-SAIFR, November 13th, 2019 Outline The outline of this colloquium is I Standard Model: reminder I Electroweak interactions I Strong interactions I The Higgs sector I Experimental successes I Theoretical and observational drawbacks I Beyond the Standard Model I Supersymmetry I Large extra dimensions I Warped extra dimensions/composite Higgs I Concluding remarks Disclaimer: I will not discuss any technical details. With my apologies to my theorist (and experimental) colleagues The Standard Model: reminder I The knowledge of the Standard Model of strong and electroweak interactions requires (as any other physical theory) the knowledge of I The elementary particles or fields (the characters of the play) I How particles interact (their behavior) The characters of the play I Quarks: spin-1/2 fermions I Leptons: spin-1/2 fermions I Higgs boson: spin-0 boson I Carriers of the interactions: spin-1 (gauge) bosons I All these particles have already been discovered and their mass, spin, and charge measured \More in detail the characters of the play" - Everybody knows the Periodic Table of the Elements - Compare elementary particles with some (of course composite) very heavy nuclei What are the interactions between the elementary building blocks of the Standard Model? I Interactions are governed by a symmetry principle I The more symmetric the theory the more couplings are related (the less of them they are) and the more predictive it is Strong interactions:
    [Show full text]
  • James Chadwick and E.S
    What is the Universe Made Of? Atoms - Electrons Nucleus - Nucleons Antiparticles And ... http://www.parentcompany.com/creation_explanation/cx6a.htm What Holds it Together? Gravitational Force Electromagnetic Force Strong Force Weak Force Timeline - Ancient 624-547 B.C. Thales of Miletus - water is the basic substance, knew attractive power of magnets and rubbed amber. 580-500 B.C. Pythagoras - Earth spherical, sought mathematical understanding of universe. 500-428 B.C. Anaxagoras changes in matter due to different orderings of indivisible particles (law of the conservation of matter) 484-424 B.C. Empedocles reduced indivisible particles into four elements: earth, air, fire, and water. 460-370 B.C. Democritus All matter is made of indivisible particles called atoms. 384-322 B.C. Aristotle formalized the gathering of scientific knowledge. 310-230 B.C. Aristarchus describes a cosmology identical to that of Copernicus. 287-212 B.C. Archimedes provided the foundations of hydrostatics. 70-147 AD Ptolemy of Alexandria collected the optical knowledge, theory of planetary motion. 1214-1294 AD Roger Bacon To learn the secrets of nature we must first observe. 1473-1543 AD Nicholaus Copernicus The earth revolves around the sun Timeline – Classical Physics 1564-1642 Galileo Galilei - scientifically deduced theories. 1546-1601, Tycho Brahe accurate celestial data to support Copernican system. 1571-1630, Johannes Kepler. theory of elliptical planetary motion 1642-1727 Sir Isaac Newton laws of mechanics explain motion, gravity . 1773-1829 Thomas Young - the wave theory of light and light interference. 1791-1867 Michael Faraday - the electric motor, and electromagnetic induction, electricity and magnetism are related. electrolysis, conservation of energy.
    [Show full text]
  • INMUNOTERAPIA CONTRA EL CÁNCER ESPECIAL Inmunoterapia Contra El Cáncer
    ESPECIAL INMUNOTERAPIA CONTRA EL CÁNCER ESPECIAL Inmunoterapia contra el cáncer CONTENIDO Una selección de nuestros mejores artículos sobre las distintas estrategias de inmunoterapia contra el cáncer. Las defensas contra el cáncer El científico paciente Karen Weintraub Katherine Harmon Investigación y Ciencia, junio 2016 Investigación y Ciencia, octubre 2012 Desactivar el cáncer Un interruptor Jedd D. Wolchok Investigación y Ciencia, julio 2014 para la terapia génica Jim Kozubek Investigación y Ciencia, mayo 2016 Una nueva arma contra el cáncer Viroterapia contra el cáncer Avery D. Posey Jr., Carl H. June y Bruce L. Levine Douglas J. Mahoney, David F. Stojdl y Gordon Laird Investigación y Ciencia, mayo 2017 Investigación y Ciencia, enero 2015 Vacunas contra el cáncer Inmunoterapia contra el cáncer Eric Von Hofe Lloyd J. Old Investigación y Ciencia, diciembre 2011 Investigación y Ciencia, noviembre 1996 EDITA Prensa Científica, S.A. Muntaner, 339 pral. 1a, 08021 Barcelona (España) [email protected] www.investigacionyciencia.es Copyright © Prensa Científica, S.A. y Scientific American, una división de Nature America, Inc. ESPECIAL n.o 36 ISSN: 2385-5657 En portada: iStock/royaltystockphoto | Imagen superior: iStock/man_at_mouse Takaaki Kajita Angus Deaton Paul Modrich Arthur B. McDonald Shuji Nakamura May-Britt Moser Edvard I. Moser Michael Levitt James E. Rothman Martin KarplusMÁS David DE J. 100 Wineland PREMIOS Serge Haroche NÓBEL J. B. Gurdon Adam G.han Riess explicado André K. Geim sus hallazgos Carol W. Greider en Jack W. Szostak E. H. Blackburn W. S. Boyle Yoichiro Nambu Luc MontagnierInvestigación Mario R. Capecchi y Ciencia Eric Maskin Roger D. Kornberg John Hall Theodor W.
    [Show full text]
  • Symposium Celebrating CERN's Discoveries and Looking Into the Future
    CERN–EP–2003–073 CERN–TH–2003–281 December 1st, 2003 Proceedings Symposium celebrating the Anniversary of CERN’s Discoveries and a Look into the Future 111999777333::: NNNeeeuuutttrrraaalll CCCuuurrrrrreeennntttsss 111999888333::: WWW±±± &&& ZZZ000 BBBooosssooonnnsss Tuesday 16 September 2003 CERN, Geneva, Switzerland Editors: Roger Cashmore, Luciano Maiani & Jean-Pierre Revol Table of contents Table of contents 2 Programme of the Symposium 4 Foreword (L. Maiani) 7 Acknowledgements 8 Selected Photographs of the Event 9 Contributions: Welcome (L. Maiani) 13 The Making of the Standard Model (S. Weinberg) 16 CERN’s Contribution to Accelerators and Beams (G. Brianti) 30 The Discovery of Neutral Currents (D. Haidt) 44 The Discovery of the W & Z, a personal recollection (P. Darriulat) 57 W & Z Physics at LEP (P. Zerwas) 70 Physics at the LHC (J. Ellis) 85 Challenges of the LHC: – the accelerator challenge (L. Evans) 96 – the detector challenge (J. Engelen) 103 – the computing challenge (P. Messina) 110 Particle Detectors and Society (G. Charpak) 126 The future for CERN (L. Maiani) 136 – 2 – Table of contents (cont.) Panel discussion on the Future of Particle Physics (chaired by Carlo Rubbia) 145 Participants: Robert Aymar, Georges Charpak, Pierre Darriulat, Luciano Maiani, Simon van der Meer, Lev Okun, Donald Perkins, Carlo Rubbia, Martinus Veltman, and Steven Weinberg. Statements from the floor by: Fabiola Gianotti, Ignatios Antoniadis, S. Glashow, H. Schopper, C. Llewellyn Smith, V. Telegdi, G. Bellettini, and V. Soergel. Additional contributions: Comment on the occasion (S. L. Glashow) 174 Comment on Perturbative QCD in early CERN experiments (D. H. Perkins) 175 Personal remarks on the discovery of Neutral Currents (A.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]