EUROPEAN FACILITIES and PLANS John Ellis CERN CH-1211 Geneva

Total Page:16

File Type:pdf, Size:1020Kb

EUROPEAN FACILITIES and PLANS John Ellis CERN CH-1211 Geneva EUROPEAN FACILITIES AND PLANS John Ellis CERN CH-1211 Geneva 23, Switzerland Summary provision for excavating two other RF galleries and filling them with superconducting RF which should give The capabilities and time schedules of present 32 2 and planned accelerators in Europe are reviewed. The rs= 180 GeV at a luminosity of 10 cm- sec-l • history of the Large Hadron Collider (LHC) project is The cost of LEP II is estimated to be about 8 recalled, and the results of machine feasibility 10 $, 1 1/2 times the part of the annual CERN budget studies are summarized. It seems possible to build available for LEP construction. The additional RF for in the LEP tunnel a pp collider with ;; = 10 to LEP II could be installed during shutdowns of LEP I, 33 2 18 TeV and a luminosity of 10 cm- sec-l Results which is not expected to run for more than about 2000 hours per year. It is not unreasonable to foresee from the Lausa"ne Workshop on LHC physics are reviewed, and some aspects of Higgs and supersymmetric LEP II starting to operate above the w+w- threshold in 1992, and then running there for at least two years. particle production are discussed. Four detectors are currently under construction for Present and Planned Accelerators LEP. Among these are ALEPH and DELPHI which feature TPC's and other slow drift devices, and OPAL and L3 which do not have such slow drift devices, and could Spps Collider. In the past this machine has perhaps be used in a modified form at the LHC. operated at a centre-of-mass energy rs = 546 GeV at 29 -2 -1 an instantaneous luminosity up to 2 x 10 cm sec , HERA. This ep collider was finally approved in and has accumulated an integrated luminosity of about April 1984, and civil engineering is expected to start 102 nb-l • Plans for this year include a test for an soon. It is planned to collide 30 GeV e± with 820 GeV protons for a total center-of-mass energy of exploratory run in a pulsed mode, with the beam energy 32 2 oscillating between 120 and 450 GeV on a time-scale 314 GeV, with a luminosity around 10 cm- sec-l • measured in tens of seconds. It is hoped to achieve A simpler, cheaper and higher field magnet design is next year an instantaneous luminosity of order now being prepared, which might enable higher proton energies of 0(1) TeV to be achieved. It is expected 10 25 cm -2 at vsr 900 GeV , which should enable = to have electrons in their ring by early 1988, and the searches for Centauro events 01. any other novel protons in mid 1989, with ep collisions in mid phenomena with a threshold below /S = 1 TeV • Also 1990. Intensive e+e- physics is not a priority for planned for this year is a conventional physics run at the machine, and going to 40 GeV per beam in the 118 = 620 GeV for about 12 weeks between September and e-+ ri.. ngs would require superconducting RF: this makes December 1984, during which, with the aid of some it unlikely that HERA will be suitable for a toponium improvement in the instantaneous luminosity, one factory. As for possible subsequent developments of should be able to increase the present integrated HERA, the internal diameter of the tunnel is large luminosity by a factor of 3 to 5. In the future, it enough to contain another ring. There are no prizes If is planned to upgrade the Spps Collider with a new for guessing what that ring might be! The present accumulator ring called ACOL, which should increase cost of the HERA projected is estimated at around the peak luminosity by 0(10) from 1987 onwards. One 8 may hope to accumulate an integrated luminosity of 2.5 x 10 $ • About a third of this is being covered 4 by contributions of labour, materials and components 0(103) nb-l before then, and perhaps 0(10 ) nb-l by countries outside West Germany, including Italy, afterwards. Plans for detector upgrades include a Canada, France, the Netherlands, Great Britain and microvertex detector for UAl during 1984, and Israel. This is a novel model for international subsequently improved calorimetry. UA2 plans include participation in accelerator construction, which Ring Imaging Cerenkov (RICH) in the forward direction might be interesting for future projects such as the during 1984, and improved solid angle coverage for SSC. No experiments for HERA have yet been chosen their calorimetry in 1987. and it is expected that decisions will be made in iate 1985. LEP. Access pits are being dug, as well as the part ~the tunnel under the Jura mountains. The History of the Large. Hadron Collider (LHC) Idea. first e+e- collisions are expected towards the end There were many informal discussions of a possible of 1988. In its first phase (LEP I) the centre-of­ hadron collider in the LEP tunnel even before LEP was mass energy rs ~ 103 GeV with an instantaneous officially approved. Indeed, the possible subsequent 31 -2 -1 luminosity ~ 10 cm sec . The cost of LEP I is installation of a hadron ring or rings was taken into 8 consideration when choosing the LEP tunnel radius (as about 4.5 x 10 $ • Probably it will be run for at large as possible, since it might be the last piece of least two years at the Z0 peak, gathering up to 107 0 real estate available for accelerator construction in Z decays. Also, the latest data on the t quark Europe, as well as to get to the highest possible make it seem quite likely that toponium is too heavy e+e- energies) and diameter (large enough to leave to be produced at previous lower energy e+e­ room for hadron magnets). Discussion of an LHC was machines, and that LEP may provide the first detailed greatly stimulated by the recent success of the SppS exploration of the toponium system, something which Collider. Serious work was, however, triggered by the might take a year or more. Beyond LEP I there are initiation of the SSC project in the United States. options for increasing the available rs . called There were prepatory meetings at CERN in December 1983 generically LEP II. One possibility is to fill up the and February 1984, in which about 40 leading European first two planned RF galleries with superconducting physicists participated. Also during the winter RF. This would provide rs up to 140 GeV at 1983/1984 there was an LHC machine study group at CERN 2 luminosities up to 1032 cm- sec-l There is also which produced the feasibility studyl reviewed in the -799- next section. Then, in March 1984, about 150 physicists met and worked on LHC physics at Lausanne for four days, with a subsequent two day open presen­ tation at CERN.2 All this activity was summarized in presentations3 at the ICFA meeting at KEK near Tokyo in May 1984. LHC Machine Studies Possible Options. Although I am a total ignoramus about accelerators, I have been asked to review here the "feasibility study of possible options" for a Large Hadron Collider in the LEP tunnel 1033 made by the CERN Machine Group, so I will do the best that I can. The three main options considered have •.,, been: N I E (A) pp in a single beam channel, with either u present day or futuristic high-field magnets. Such a device would yield relatively low luminosity and ...J 1032 need a relatively large aperture so as to allow separation of the beams (Fig. la). (a) (b) (c) 1030 1.-----1.--1--l......L.J...LL.L.l....----''--.1-J.-'-'..u.J"'-~.__..._..._,__..........., I 10 100 1000 Figure 1 Possible Options for LHC Beam Channels Figure 2 Luminosity and Bunch Separation (B) Two beam channels with a common magnetic circuit (Fig. lb). The space available in the LEP a Large Hadron Collider suggest that it may be diffi­ tunnel can only accommodate one cryostat to contain cult to imagine working with n larger than 1, while both beam channels. The most interesting possibility one can do experiments with TX ~ 25 ns. If these are is to put them side by side, which permits a high strict limits, then the luminosity of a collider in luminosity pp machine with many bunches. If one 32 2 1 uses present-day lower-field magnets one can have the the LEP tunnel is restricted to L ~ 4 x 10 cm- s- • magnetic fields in the two channels either antiparal­ However, if higher values of n are tolerable, one can 33 2 lel (allowing pp in separated channels or pp in increase L to 1.5 x 10 cm- s-l (corresponding to the same channel) or parallel (allowing pp in n ~ 4 ) before hitting the beam-beam tune-shift limit separated channels). If one goes to high-field mag­ of 0.0025 reached at the Spps collider. Such a nets only the antiparallel possibility (permitting luminosity is feasible with the pp option, but would pp ) is available. require between 3000 and 4000 bunches. Matching the RF in the SPS and the LHC is only possible for a few (C) Two beam channels with independent magnetic choi ces of bunch number, and the only choice in this circuits (Fig. le). In this case one is restricted 13 range is 3564. With N = 5 x 10 protons the to moderate magnetic fields, but either pp or pp p could be realized.
Recommended publications
  • Judicial Review of Uncertain Risks in Scientific Research
    Chapter 6 Judicial Review of Uncertain Risks in Scientific Research Eric E. Johnson Abstract It is difficult to neutrally evaluate the risks posed by large-scale leading- edge science experiments. Traditional risk assessment is problematic in this context for multiple reasons. Also, such experiments can be insulated from challenge by manipulating how questions of risk are framed. Yet courts can and must evaluate these risks. In this chapter, I suggest modes of qualitative reasoning to facilitate such evaluation. Keywords Risk · Risk scenarios · Law · Courts · Science · Scientific research · Particle physics · Black holes · LHC 6.1 Introduction In the world of engineering, uncertainty is anathema. Whether designing a nuclear power plant or planning a system of levees, engineers do not like surprises. Exper- imental scientific research, however, thrives on uncertainty. Reaching beyond the current state of knowledge is the whole point of the enterprise. Whether probing the planets or trying to create new particles, scientists would love to see a surprise around every corner. Uncertainty goes hand in hand with aspirations to explore and discover. This special role for uncertainty in scientific research makes questions of catastrophic risk from science experiments particularly interesting. What is more, 1See Hawai‘i County Green Party v. Clinton, 980 F. Supp. 1160, 1168-69 (D. Haw. 1997); Karl Grossman, The Risk of Cassini Probe Plutonium, The Christian Science Monitor (Oct. 10, 1997) http://www.csmonitor.com/1997/1010/101097.opin.opin.1.html; CNN, Cassini roars into space, CNN (Oct. 15, 1997) http://www.cnn.com/TECH/9710/15/cassini.launch/; Najmedin Meshkati, Probability, Plutonium Don’t Mix (op-ed), Los Angeles Times (Oct.
    [Show full text]
  • John Ellis Sergerudaz
    SLAC-PUB-3101 April 1983 (T/E) SEARCH FOR SUPERSYMMETRY IN TOPONIUM DECAYS* JOHN ELLIS Stanjord Linear Accelerator Center Stanford Uniueraity, Stanford, California 9@05 and SERGERUDAZ School of Physics and Astronomy University of Minnesota, Minneapolis, Minnesota 55455 ABSTRACT Although cosmology and unification suggest that the mass of the gluino is larger than about 14 GeV, in many theories of broken supersymmetry the photino 5, gluino S and one of the spin-zero partners i of the t quark can be lighter than mt. We calculate Z-T- the decay rates for toponium + 5 S, r 5 and t t and show that in many models they can be as large as, or larger than, the rate for toponium ---, e+e- decay. If it is kinematically accessible, the decay t --* t+q dominates the decays of toponium as well as those of naked top states. Submitted to Physics Letters B * Work supported by the Department of Energy, contracts DEAC03-76SF00515 and DEAC02-83ER40051. One obstacle to the experimental search [l] for supersymmetry (susy) is our the- oretical ignorance about the likely masses of supersymmetric particles. This means that we cannot be sure where susy will first appear, and must plan a broad-band search. The production and detection of supersymmetric particles in hadron-hadron collisions (21, lepton-hadron collisions [3,4] and e+e- annihilation [3,5,6] have been extensively discussed. In the case of e+e- annihilation, there have been discussions of the production of squarks and gluinos in the continuum and of gluinos in heavy quarkonium decays [3,5,6].
    [Show full text]
  • Sacred Rhetorical Invention in the String Theory Movement
    University of Nebraska - Lincoln DigitalCommons@University of Nebraska - Lincoln Communication Studies Theses, Dissertations, and Student Research Communication Studies, Department of Spring 4-12-2011 Secular Salvation: Sacred Rhetorical Invention in the String Theory Movement Brent Yergensen University of Nebraska-Lincoln, [email protected] Follow this and additional works at: https://digitalcommons.unl.edu/commstuddiss Part of the Speech and Rhetorical Studies Commons Yergensen, Brent, "Secular Salvation: Sacred Rhetorical Invention in the String Theory Movement" (2011). Communication Studies Theses, Dissertations, and Student Research. 6. https://digitalcommons.unl.edu/commstuddiss/6 This Article is brought to you for free and open access by the Communication Studies, Department of at DigitalCommons@University of Nebraska - Lincoln. It has been accepted for inclusion in Communication Studies Theses, Dissertations, and Student Research by an authorized administrator of DigitalCommons@University of Nebraska - Lincoln. SECULAR SALVATION: SACRED RHETORICAL INVENTION IN THE STRING THEORY MOVEMENT by Brent Yergensen A DISSERTATION Presented to the Faculty of The Graduate College at the University of Nebraska In Partial Fulfillment of Requirements For the Degree of Doctor of Philosophy Major: Communication Studies Under the Supervision of Dr. Ronald Lee Lincoln, Nebraska April, 2011 ii SECULAR SALVATION: SACRED RHETORICAL INVENTION IN THE STRING THEORY MOVEMENT Brent Yergensen, Ph.D. University of Nebraska, 2011 Advisor: Ronald Lee String theory is argued by its proponents to be the Theory of Everything. It achieves this status in physics because it provides unification for contradictory laws of physics, namely quantum mechanics and general relativity. While based on advanced theoretical mathematics, its public discourse is growing in prevalence and its rhetorical power is leading to a scientific revolution, even among the public.
    [Show full text]
  • Starobinsky-Like Inflation and Neutrino Masses in a No-Scale
    Journal of Cosmology and Astroparticle Physics OPEN ACCESS Related content - Resurrecting quadratic inflation in no-scale Starobinsky-like inflation and neutrino masses in a supergravity in light of BICEP2 John Ellis, Marcos A.G. García, Dimitri V. no-scale SO(10) model Nanopoulos et al. - Calculations of inflaton decays and reheating: with applications to no-scale To cite this article: John Ellis et al JCAP11(2016)018 inflation models John Ellis, Marcos A.G. Garcia, Dimitri V. Nanopoulos et al. - Hilltop supernatural inflation and SUSY unified models View the article online for updates and enhancements. Kazunori Kohri, C.S. Lim, Chia-Min Lin et al. Recent citations - Starobinsky Inflation: From Non-SUSY to SUGRA Realizations Constantinos Pallis and Nicolaos Toumbas - Starobinsky-like inflation, supercosmology and neutrino masses in no-scale flipped SU(5) John Ellis et al This content was downloaded from IP address 131.169.4.70 on 14/12/2017 at 22:40 ournal of Cosmology and Astroparticle Physics JAn IOP and SISSA journal Starobinsky-like inflation and neutrino masses in a no-scale SO(10) model JCAP11(2016)018 John Ellis,a;b Marcos A.G. Garcia,c Natsumi Nagata,d Dimitri V. Nanopoulose and Keith A. Oliveh aTheoretical Particle Physics and Cosmology Group, Department of Physics, King's College London, WC2R 2LS London, U.K. bTheoretical Physics Department, CERN, CH-1211 Geneva 23, Switzerland cPhysics and Astronomy Department, Rice University, 6100 Main Street, Houston, TX 77005, U.S.A. dDepartment of Physics, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan eGeorge P. and Cynthia W.
    [Show full text]
  • UK News from CERN Issue 53: 11 November 2014
    UK news from CERN Issue 53: 11 November 2014 In this issue: Top job for Edinburgh professor – CERN’s new Director-General is announced Testing times Spotlight on dark matter Resources for your A* LHC project Volcanic bread and butter physics P-p- p-pick up a (woolly) penguin Dates for the diary Top job for Edinburgh Professor Testing times The next Director General of CERN will be Dr Safety is serious matter at CERN. The nature of Fabiola Gianotti, the former spokesperson of the the experiments means that many gases and ATLAS collaboration who co-announced the chemicals are used routinely, and each one has discovery of the Higgs boson in July 2012. its own set of potential hazards. Chemical safety engineer, Jon Gulley is a member of the In 2013, in addition to many other honours from Health and Safety team. UKNFC met up with universities and institutes around the world, him to learn more about a typical day. Fabiola was appointed an Honorary Professor in the School of Physics and Astronomy at the University of Edinburgh. She is also a member of the International Advisory Committee of the Higgs Centre for Theoretical Physics at Edinburgh. Jon Gulley (r) giving advice at the CERN Safety Day 2014 © CERN Jon is often out and about around CERN providing on-site advice about chemicals and gases or inspecting equipment to ensure that it has been correctly installed, maintained or used. Fabiola Gianotti (centre) with colleagues from the University of “I’ll be checking risk assessments or layouts and Edinburgh including Peter Higgs © CERN providing advice.
    [Show full text]
  • 25.3 Bc Arising MH
    brief communications arising Cosmology Lorentz-invariant dispersion relation, avoid- ing other constraints5,6. Synchrotron radiation and quantum gravity The strong bound of Jacobson et al.1 on Arising from: Jacobson, T., Liberati, S. & Mattingly, D. Nature 424, 1019–1021 (2003) the electron underlines the interest in probing directly the dispersion relation of uantum gravity may cause the vacuum leaving measurements on time profiles of very the photon. The study of the arrival times of to act as a non-trivial medium remote g-ray bursts2,7 as the best approach for photons from g-ray bursts2 still appears to be Q(space–time foam), which alters the probing quantum-gravity effects. the best experimental probe of any possible standard Lorentz relation between the The basic reason for this violation of the refractive index for photons, and should be energy and momentum of matter particles, equivalence principle in the quantum-gravity pursued further. It has already established a 3 16 thereby modifying their dispersion model is its description of space–time foam lower limit on MQG close to 10 GeV (ref. 7), relations. Jacobson, Liberati and Mattingly1 by using quantum defects in space–time with and current (HETE,INTEGRAL) and future argue that synchrotron radiation from the vacuum quantum numbers, as in one inter- (GLAST, AMS) high-energy space missions Crab nebula imposes a stringent constraint pretation of Liouville string theory8. These have the potential to reach the Planck scale on any modification of the dispersion rela- can be excited only by particles that are neutral for any linear quantum-gravity modifica- tion of the electron that might be induced by under the gauge group of the standard model, tion of the photon’s dispersion relation.
    [Show full text]
  • With John Ellis Interviewer: Hitoshi Murayama
    Interview with John Ellis Interviewer: Hitoshi Murayama “A” Higgs Boson or“ the” Murayama: Okay. That’s Higgs Boson? right, according to the ofcial Murayama: Great to see you statement... three times in a month. It was Ellis: ...they discovered at the in Berkeley, the BrunoFest,1 LHC. then the Nobel Symposium,2 Murayama: Yeah, so let and now here. us actually follow on that. Ellis: Yeah. It’s great to be Now that‘ a’ Higgs boson is here at Kavli IPMU. It’s been a discovered, what is the future really exciting time in particle for the eld? What shall we physics recently. It’s great to be working on? catch up on a few things. Ellis: I think one thing At Berkeley, obviously, the obviously we want to focus was on supersymmetry understand is whether this which is one of our best is just‘ a’ Higgs boson or hopes in physics beyond the whether it really is‘ the’ Standard Model. At the Nobel Higgs boson as predicted in Symposium, the focus was on the Standard Model. There’re the Higgs boson. a number of theories that Murayama: Right. suggested that something, Ellis: We should be a little bit some sort of scalar particle careful – on‘ a’ Higgs boson. might appear in the LHC but with properties rather different from the Standard John Ellis is Clerk Maxwell Professor Model Higgs boson; some of Theoretical Physics at King’s College London since 2010. He composite models for was Staff Member at CERN from example. 1974, and served as Division Leader of the theory “( TH”) division in I think one can say that all 1988–1994.
    [Show full text]
  • Prospects for Future Collider Physics
    November 5, 2018 11:35 WSPC/INSTRUCTION FILE JE-HKUST-IAS- HEP International Journal of Modern Physics A c World Scientific Publishing Company Prospects for Future Collider Physics John Ellis Theoretical Particle Physics and Cosmology Group, Department of Physics, King's College London, Strand, London WC2R 2LS, United Kingdom; Theoretical Physics Department, CERN, CH 1211 Geneva 23, Switzerland [email protected] One item on the agenda of future colliders is certain to be the Higgs boson. What is it trying to tell us? The primary objective of any future collider must surely be to iden- tify physics beyond the Standard Model, and supersymmetry is one of the most studied options. Is supersymmetry waiting for us and, if so, can LHC Run 2 find it? The big surprise from the initial 13-TeV LHC data has been the appearance of a possible signal for a new boson X with a mass ' 750 GeV. What are the prospects for future colliders if the X(750) exists? One of the most intriguing possibilities in electroweak physics would be the discovery of non-perturbative phenomena. What are the prospects for observing sphalerons at the LHC or a future collider? Contribution to the Hong Kong UST IAS Programme and Conference on High-Energy Physics, based largely on personal research with various collaborators. KCL-PH-TH-2016-16, LCTS-2016-12, CERN-TH-2016-075 Keywords: Higgs boson; beyond the Standard Model; supersymmetry; LHC; future col- liders. PACS numbers: 12.15.-y, 12.60.Jv, 14.80.Bn, 14.80.Ly 1. The Higgs Boson arXiv:1604.00333v1 [hep-ph] 1 Apr 2016 We already know the mass of the Higgs boson with an accuracy 0:2%: ∼ mH = 125:09 0:21 0:11 GeV ; (1) ± ± where the first (dominant) uncertainty is statistical and the second is systematic.1 We can expect that the LHC experiments will reduce the overall uncertainty to below 100 MeV, setting a hot pace for future collider experiments to follow.
    [Show full text]
  • Theoretical Aspects of Dark Matter Detection 3
    hep-ph/0106148 CERN–TH/2001-153 UMN–TH–2012/01, TPI–MINN–01/28 THEORETICAL ASPECTS OF DARK MATTER DETECTION JOHN ELLIS ([email protected]) TH Division, CERN, Geneva, Switzerland ANDREW FERSTL ([email protected]) Department of Physics, Winona State University, Winona, MN USA KEITH A. OLIVE ([email protected]) TH Division, CERN, Geneva, Switzerland and Theoretical Physics Institute, University of Minnesota, Minneapolis, MN 55455, USA Received . , accepted . Abstract. Direct and indirect dark matter detection relies on the scattering of the dark matter candidate on nucleons or nuclei. Here, attention is focused on dark matter candidates (neutralinos) predicted in the minimal supersymmetric standard model and its constrained version with universal input soft supersymmetry-breaking masses. Current expectations for elastic scattering cross sections for neutralinos on protons are discussed with particular attention to satisfying all current accelerator constraints as well as insuring a sufficient cosmological relic density to account for the dark matter in the Universe. 1. Introduction Minimal supersymmetric theories with R-parity conservation are particularly at- tractive for the study of dark matter as they predict the existence of a new stable particle which is the lightest R-odd state (the LSP). Furthermore, for parameter values of interest to resolve the gauge hierarchy problem, the LSP has an annihi- arXiv:hep-ph/0106148v1 14 Jun 2001 lation cross section which yields a relic density of cosmological interest (Ellis et al., 1984). Recent accelerator constraints have made a great impact on the available parameter space in the MSSM and in particular the constrained version or CMSSM in which all scalar masses are assumed to be unified at a grand unified scale (Ellis et al., 1998; Ellis et al., 2000a; Ellis et al., 2001b; Ellis, Nanopoulos, & Olive, 2001).
    [Show full text]
  • Future Perspectives at CERN 3 Unprecedented Accuracy
    Future Perspectives at CERN John Ellis1 Theoretical Physics Division, CERN, Geneva, Switzerland Abstract. Current and future experiments at CERN are reviewed,with emphasis on those relevant to astrophysics and cosmology. These include experiments related to nuclear astrophysics, matter-antimatter asymmetry, dark matter, axions, gravitational waves, cosmic rays, neutrino oscillations, inflation, neutron stars and the quark-gluon plasma. The centrepiece of CERN’s future programme is the LHC, but some ideas for perspectives after the LHC are also presented. CERN-TH/2002-119 astro-ph/0206054 Talk given at the CERN-ESA-ESO Symposium, M¨unchen, April 2002 1 Outline The scientific mission of CERN is to provide Europe with unique accelerators for the study of the fundamental particles of matter and the interactions between them. The scientific programme of CERN for the next decade is centred on the LHC accelerator, which is scheduled for completion in 2006, so that its experi- ments can start taking in 2007. A description of the LHC scientific programme is the centrepiece of this talk. The motivations for this and other new accelera- tors provided by ideas about possible physics beyond the Standard Model were discussed earlier at this meeting [1]. Between now and the startup of the LHC, CERN has a very limited pro- gramme of running experiments. However, scientific diversity at CERN is en- hanced by a number of recognized experiments, that do not use the CERN ac- celerators and are not supported by CERN, but whose scientists are allowed to use other CERN facilities. In parallel with the construction of the LHC, CERN arXiv:astro-ph/0206054v1 4 Jun 2002 is also preparing to send a long-baseline neutrino beam to the Gran Sasso under- ground laboratory in Italy, in a special programme largely supported by extra contributions from interested countries.
    [Show full text]
  • John Ellis a Personal Introduction
    John Ellis A Personal Introduction • Theoretical physicist, interested in making predictions for experiments, and their interpretations • Background in particle physics, working also in cosmology and high-energy astrophysics • Worked at CERN 1973 – 2011 • Now professor at King’s College London • Advocate for global participation in research • Member of International Organization Committee of African School of Physics My Long-Term CERN Office King’s College London What are we? Where do we come from? Where are we going? The aim of particle physics: John Ellis What is matter in the Universe made of? Evolution of the Universe What will happen in the future? Big Bang cm 28 10 What happened then? 13.8What Billion is Years the universe Today made of? Gauguin’s Questions in the Language of Particle Physics • What is matter made of? – Why do things weigh? • What is the origin of matter? LHC • What is the dark matter that fills the Universe?LHC • How does the Universe evolve? • Why is the Universe so big and old? LHC • What is the future of the Universe? LHC Our job is to ask - and answer - these questions Need physics beyond what we know /Users/johne/Desktop/YoungEinsteins.png Big Bang Proton Atom Radius of Earth Earth to Sun Radius of Galaxies Universe LHC Super-Microscope ALMA Hubble Study physics laws of first moments after Big Bang increasing Symbiosis between Particle Physics, Astrophysics and Cosmology AMS VLT 300,000 Formation years of atoms 3 Formation minutes of nuclei Formation 1 micro- of protons second Appearance & neutrons 1 pico-
    [Show full text]
  • Artnodes Artnodes
    Universitat Oberta de Catalunya artnodes E-JOURNAL ON ART, SCIENCE AND TECHNOLOGY http://artnodes.uoc.edu Article NODO «DIALOGS BETWEEN ART AND FUNDAMENTAL SCIENCE» THUTOAH - The Holographic Universe Theory of Art History Suzanne Treister CERN Date of submission: October 2019 Accepted in: December 2019 Published in: January 2020 Recommended citation Treister, Suzanne. 2020. «THUTOAH - The Holographic Universe Theory Of Art History». Artnodes, Nº. 25: 1-8. UOC. [Consulta: dd/mm/yy]. http://doi.org/10.7238/a.v0i25.3323 The texts published in this journal are – unless otherwise indicated – covered by the Creative Commons Spain Attribution 4.0 International license. The full text of the license can be consulted here: http://creativecommons.org/licenses/by/4.0/ Abstract This text is an edit of the audio transcript of interviews with scientists John Ellis, Alessandra Gnecchi and Wolfgang Lerche from my video, The Holographic Universe Theory of Art History (THUTOAH). THUTOAH investigates the holographic principle and the theory that our universe could be understood as a vast and complex hologram, and hypothesises that, beyond acknowledged art historical contexts and imperatives, artists may have also been unconsciously attempting to describe the holographic nature of the universe. Projecting over 25,000 chronological images from art history (from cave painting to global contemporary art, including outsider and psychedelic art), THUTOAH echoes conceptually the actions of CERN’s particle accelerator, the Large Hadron Collider (LHC), accelerating at 25 images per second in a looped sequence. Alongside this colossal library of images is a soundtrack of interviews with, and watercolours by, the scientists at CERN - illustrations and articulations of the holographic principle.
    [Show full text]