Annual Report 2000
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Search for New Particles at LEP
Search for New Particles at LEP S. Rosier-Lees LAPP (INPPS-CNRS) Annecy-Le-Vieux - France Abstract The LEP energy upgrade up to fi =189 GeV has allowed us to extend substantially the potential of searches for new physics. Results on searches for Higgs bosoms and supersymmetric particles obtained by the ALEPH, DELPHI, L3, and OPAL exper- iments are reported. No evidence of any signal is observed. Therefore, new limits on the Higgs boson masses as well as on the masses of the various supersymmetric particles are derived. They significantly improve those obtained either at LEPl or LEP1.5. The LEPBOO discovery potential for the neutral Higgs bosons is also shown. @ 1998 by S. Rosier-Lees. -409- . be discovered at LEP200 when running at &=200 GeV and assuming an integrated luminosity of 200 pb-’ collected by each experiment. LEP PRELIMINARY Individual Limit LEP Combined 11 Table 1: Individual and LEP combined observed and expected mass limits for the Stan- dard Model Higgs boson [3], up to fi = 183 GeV. 4 _?I: 80 82 84 86 88 90 92 94 10 80 82 84 86 88 90 92 mH(GeV/ z5 k --- HZ-Signal(mn=85GeV) 2 1.5 1 0.5 0 0 20 40 60 80 loo 0 mF(GeV) Figure 1: Mass distribution for the candidate events selected by the OPAL experiment in the searches for e+e- + HZ at center-of-mass energies up to 183 GeV [3]. I,,,I,,,,,,/,I lo 80 82 84 86 88 90 92 94. 80 82 84 86 88 90 92 94 mH(GeV/c’) mH(Ge V/c2) 2.2 The MSSM Higgs Bosons Figure 2: Average expected (dashed lines) and observed (solid lines) confidence levels, CL,, obtained In the MSSM, all SUSY particle masses, their couplings, and their production cross sec- from combining the results of the four LEP Collaborations using the four statistical methods. -
Arxiv:2001.07837V2 [Hep-Ex] 4 Jul 2020 Scale Funding Will Be Requested at Different Stages Across the Globe
Brazilian Participation in the Next-Generation Collider Experiments W. L. Aldá Júniora C. A. Bernardesb D. De Jesus Damiãoa M. Donadellic D. E. Martinsd G. Gil da Silveirae;a C. Henself H. Malbouissona A. Massafferrif E. M. da Costaa C. Mora Herreraa I. Nastevad M. Rangeld P. Rebello Telesa T. R. F. P. Tomeib A. Vilela Pereiraa aDepartamento de Física Nuclear e Altas Energias, Universidade do Estado do Rio de Janeiro (UERJ), Rua São Francisco Xavier, 524, CEP 20550-900, Rio de Janeiro, Brazil bUniversidade Estadual Paulista (Unesp), Núcleo de Computação Científica Rua Dr. Bento Teobaldo Ferraz, 271, 01140-070, Sao Paulo, Brazil cInstituto de Física, Universidade de São Paulo (USP), Rua do Matão, 1371, CEP 05508-090, São Paulo, Brazil dUniversidade Federal do Rio de Janeiro (UFRJ), Instituto de Física, Caixa Postal 68528, 21941-972 Rio de Janeiro, Brazil eInstituto de Física, Universidade Federal do Rio Grande do Sul , Av. Bento Gonçalves, 9550, CEP 91501-970, Caixa Postal 15051, Porto Alegre, Brazil f Centro Brasileiro de Pesquisas Físicas (CBPF), Rua Dr. Xavier Sigaud, 150, CEP 22290-180 Rio de Janeiro, RJ, Brazil E-mail: [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected] Abstract: This proposal concerns the participation of the Brazilian High-Energy Physics community in the next-generation collider experiments. -
HERA Collisions CERN LHC Magnets
The Gallex (gallium-based) solar neutrino experiment in the Gran Sasso underground Laboratory in Italy has seen evidence for neutrinos from the proton-proton fusion reaction deep inside the sun. A detailed report will be published in our next edition. again, with particles taken to 26.5 aperture models are also foreseen to GeV and initial evidence for electron- CERN test coil and collar assemblies and a proton collisions being seen. new conductor distribution will further Earlier this year, the big Zeus and LHC magnets improve multipole components. H1 detectors were moved into A number of other models and position to intercept the first HERA With test magnets for CERN's LHC prototypes are being built elsewhere collisions, and initial results from this proton-proton collider regularly including a twin-aperture model at new physics frontier are eagerly attaining field strengths which show the Japanese KEK Laboratory and awaited. that 10 Tesla is not forbidden terri another in the Netherlands (FOM-UT- tory, attention turns to why and NIHKEF). The latter will use niobium- where quenches happen. If 'training' tin conductor, reaching for an even can be reduced, superconducting higher field of 11.5 T. At KEK, a magnets become easier to commis single aperture configuration was sion. Tests have shown that successfully tested at 4.3 K, reaching quenches occur mainly at the ends of the short sample limit of the cable the LHC magnets. This should be (8 T) in three quenches. This magnet rectifiable, and models incorporating was then shipped to CERN for HERA collisions improvements will soon be reassem testing at the superfluid helium bled by the industrial suppliers. -
Physical and Chemical Sciences 2010-2015 Utrecht University
RESEARCH REVIEW PHYSICAL AND CHEMICAL SCIENCES 2010-2015 UTRECHT UNIVERSITY Quality Assurance Netherlands Universities (QANU) Catharijnesingel 56 PO Box 8035 3503 RA Utrecht The Netherlands Phone: +31 (0) 30 230 3100 E-mail: [email protected] Internet: www.qanu.nl Project number: 0630 © 2017 QANU Text and numerical material from this publication may be reproduced in print, by photocopying or by any other means with the permission of QANU if the source is mentioned. 2 QANU / Research Review Physical and Chemical Sciences, Utrecht University REPORT ON THE RESEARCH REVIEW OF PHYSICAL AND CHEMICAL SCIENCES OF UTRECHT UNIVERSITY CONTENT 1. Foreword committee chair 5 2. The review committee and the procedures 7 2.1 Scope of the review 7 2.2 Composition of the committee 7 2.3 Independence 7 2.4 Data provided to the committee 7 2.5 Procedures followed by the committee 8 3. Quantitative and qualitative assessment of Physical and Chemical Sciences 9 3.1 Broader context 9 3.2 Research quality 10 3.3 Relevance to Society 11 3.4 Viability 13 3.5 PhD programmes 15 3.6 Research integrity policy 17 3.7 Diversity 18 3.8 Conclusion 19 3.9 Quantitative assessment of Physical and Chemical Sciences 20 4. Quantitative and qualitative assessment of the separate research institutes 21 4.1 Debye Institute for Nanomaterial Science 21 4.2 Institute for Marine and Atmospheric research 24 4.3 Institute for Theoretical Physics 27 4.4 Institute for Sub-Atomic Physics 30 5. Recommendations 33 Appendices 35 Appendix 1: Explanation of the SEP criteria and categories 37 Appendix 2: Curricula Vitae of the committee members 39 Appendix 3: Programme of the site visit 41 Appendix 4: Quantitative Data 47 QANU / Research Review Physical and Chemical Sciences, Utrecht University 3 4 QANU / Research Review Physical and Chemical Sciences, Utrecht University 1. -
Seismic Characterization of the Euregio Meuse-Rhine in View of Einstein Telescope
SEISMIC CHARACTERIZATION OF THE EUREGIO MEUSE-RHINE IN VIEW OF EINSTEIN TELESCOPE 13 September 2019 First results of seismic studies of the Belgian-Dutch-German site for Einstein Telescope Soumen Koley1, Maria Bader1, Alessandro Bertolini1, Jo van den Brand1,2, Henk Jan Bulten1,3, Stefan Hild1,2, Frank Linde1,4, Bas Swinkels1, Bjorn Vink5 1. Nikhef, National Institute for Subatomic Physics, Amsterdam, The Netherlands 2. Maastricht University, Maastricht, The Netherlands 3. VU University Amsterdam, Amsterdam, The Netherlands 4. University of Amsterdam, Amsterdam, The Netherlands 5. Antea Group, Maastricht, The Netherlands CONFIDENTIAL Figure 1: Artist impression of the Einstein Telescope gravitational wave observatory situated at a depth of 200-300 meters in the Euregio Meuse-Rhine landscape. The triangular topology with 10 kilometers long arms allows for the installation of multiple so-called laser interferometers. Each of which can detect ripples in the fabric of space-time – the unique signature of a gravitational wave – as minute relative movements of the mirrors hanging at the bottom of the red and white towers indicated in the illustration at the corners of the triangle. 1 SEISMIC CHARACTERIZATION OF THE EUREGIO MEUSE-RHINE IN VIEW OF EINSTEIN TELESCOPE Figure 2: Drill rig for the 2018-2019 campaign used for the completion of the 260 meters deep borehole near Terziet on the Dutch-Belgian border in South Limburg. Two broadband seismic sensors were installed: one at a depth of 250 meters and one just below the surface. Both sensors are accessible via the KNMI portal: http://rdsa.knmi.nl/dataportal/. 2 SEISMIC CHARACTERIZATION OF THE EUREGIO MEUSE-RHINE IN VIEW OF EINSTEIN TELESCOPE Executive summary The European 2011 Conceptual Design Report for Einstein Telescope identified the Euregio Meuse-Rhine and in particular the South Limburg border region as one of the prospective sites for this next generation gravitational wave observatory. -
The ATLAS Pixel Detector
The ATLAS Pixel Detector Maurice Garcia-Sciveres Lawrence Berkeley National Laboratory DEC 9, 2005 SRI Workshop --- the ATLAS pixel detector --- M. Garcia-Sciveres 1 ATLAS Pixel Collaboration • ~100 collaborators • 17 institutions • 8 countries DEC 9, 2005 SRI Workshop --- the ATLAS pixel detector --- M. Garcia-Sciveres 2 The Large Hadron Colloder will be the world’s most powerful microscope Camera goes here p p 14TeV ~10-19m resolution but… ¾Need high intensity ¾At design intensity LHC beam has 330MJ stored energy Iron yoke ¾1% will blow up dipole ¾Driving factor in vertex detector design 2 beam pipes Channels for superconducting wire DEC 9, 2005 SRI Workshop --- the ATLAS pixel detector --- M. Garcia-Sciveres 3 ATLAS 45m DEC 9, 2005 SRI Workshop --- the ATLAS pixel detector --- M. Garcia-Sciveres 4 ATLAS Pixel Detector p p Along axis 80M pixels (2m2 active area) 1744 parallel modules covering 3 barrels + 6 disks 1.3 m DEC 9, 2005 SRI Workshop --- the ATLAS pixel detector --- M. Garcia-Sciveres 5 Top Quark Photo Zoom in x10 Zoom in again x10 Actual Top Quark Decay Recorded by the CDF experiment with a silicon strip detector DEC 9, 2005 SRI Workshop --- the ATLAS pixel detector --- M. Garcia-Sciveres 6 Hybrid pixel detectors in particle physics • Silicon strip detectors have been used in particle physics for some 20 years (and are here to stay). This is a type of hybrid imager with resolution in only 1 dimension. ISL detector of CDF experiment • A hybrid pixel detector is a conceptually trivial (but technically difficult) generalization of a strip detector to 2 dimensions. -
Information for Guides
DRAFT 27 February 2014 Information for guides for Underground Visits Document prepared by Gloria Corti 1. Introduction This document is intended to provide you with material on which you can base your discussion with the visitors, along with more detailed background information for those not familiar with LHCb. It is not be intended to provide a word-by-word account of what an ideal visit underground to LHCb (and Delphi) should contain, nor what you should say on the surface. Everyone is specialized in different fields and the best is to convey the key messages from a personal and enthusiastic angle, and react to the response from your group. The main idea while underground is to explain what the visitors can see, at each stopping point of the itinerary. Discussions of more abstract concepts such as particle physics, the Standard Model, etc, should be done on the surface, either before or after the visit underground. Guides at the Exhibit are also encouraged to explain the various detectors on display. Pages 1 to 2 may be useful to all guides, while 2 to 5 are mostly intended for underground guides. The rest gives some general background for the LHCb experiment and detector and on the DELPHI experiment. Some summary facts and numbers are listed at the end. 2. When you first meet the visitors The first thing you should do is to introduce yourself, then check they are all present and they wear closed shoes and don’t have big bags with them. You may have to wait before going underground and you can use this time and that on the lift going underground to give visitors some general information. -
NA61/SHINE Facility at the CERN SPS: Beams and Detector System
Preprint typeset in JINST style - HYPER VERSION NA61/SHINE facility at the CERN SPS: beams and detector system N. Abgrall11, O. Andreeva16, A. Aduszkiewicz23, Y. Ali6, T. Anticic26, N. Antoniou1, B. Baatar7, F. Bay27, A. Blondel11, J. Blumer13, M. Bogomilov19, M. Bogusz24, A. Bravar11, J. Brzychczyk6, S. A. Bunyatov7, P. Christakoglou1, T. Czopowicz24, N. Davis1, S. Debieux11, H. Dembinski13, F. Diakonos1, S. Di Luise27, W. Dominik23, T. Drozhzhova20 J. Dumarchez18, K. Dynowski24, R. Engel13, I. Efthymiopoulos10, A. Ereditato4, A. Fabich10, G. A. Feofilov20, Z. Fodor5, A. Fulop5, M. Ga´zdzicki9;15, M. Golubeva16, K. Grebieszkow24, A. Grzeszczuk14, F. Guber16, A. Haesler11, T. Hasegawa21, M. Hierholzer4, R. Idczak25, S. Igolkin20, A. Ivashkin16, D. Jokovic2, K. Kadija26, A. Kapoyannis1, E. Kaptur14, D. Kielczewska23, M. Kirejczyk23, J. Kisiel14, T. Kiss5, S. Kleinfelder12, T. Kobayashi21, V. I. Kolesnikov7, D. Kolev19, V. P. Kondratiev20, A. Korzenev11, P. Koversarski25, S. Kowalski14, A. Krasnoperov7, A. Kurepin16, D. Larsen6, A. Laszlo5, V. V. Lyubushkin7, M. Mackowiak-Pawłowska´ 9, Z. Majka6, B. Maksiak24, A. I. Malakhov7, D. Maletic2, D. Manglunki10, D. Manic2, A. Marchionni27, A. Marcinek6, V. Marin16, K. Marton5, H.-J.Mathes13, T. Matulewicz23, V. Matveev7;16, G. L. Melkumov7, M. Messina4, St. Mrówczynski´ 15, S. Murphy11, T. Nakadaira21, M. Nirkko4, K. Nishikawa21, T. Palczewski22, G. Palla5, A. D. Panagiotou1, T. Paul17, W. Peryt24;∗, O. Petukhov16 C.Pistillo4 R. Płaneta6, J. Pluta24, B. A. Popov7;18, M. Posiadala23, S. Puławski14, J. Puzovic2, W. Rauch8, M. Ravonel11, A. Redij4, R. Renfordt9, E. Richter-Wa¸s6, A. Robert18, D. Röhrich3, E. Rondio22, B. Rossi4, M. Roth13, A. Rubbia27, A. Rustamov9, M. -
FIAS Scientific Report 2012
FIAS Scientific Report 2012 Frankfurt Institute for Advanced Studies Editor: Dr. Joachim Reinhardt Ruth-Moufang-Str. 1 reinhardt@fias.uni-frankfurt.de 60438 Frankfurt am Main Germany Tel.: +49 (0)69 798 47600 Fax: +49 (0)69 798 47611 fias.uni-frankfurt.de Vorstand: Prof. Dr. Volker Lindenstruth, Vorsitzender Regierungspräsidium Darmstadt Prof. Dr. Dirk H. Rischke Az:II21.1–25d04/11–(12)–545 Prof. Dr. Dr. h.c. mult. Wolf Singer Finanzamt Frankfurt Prof. Dr. Dres. h.c. Horst Stöcker Steuernummer: 47 250 4216 1 – XXI/101 Prof. Dr. Jochen Triesch Freistellungsbescheid vom 16.08.2010 Geschäftsführer: Gisbert Jockenhöfer FIAS Scientific Report 2012 Table of Contents Preface..........................................................................5 Research highlights 2012 . 6 1. Partner Research Centers 1.1 HIC for FAIR / EMMI . 9 1.2 Bernstein Focus Neurotechnology . 11 2. Graduate Schools 2.1 HGS-HIRe / HQM . 14 2.2 FIGSS . 16 3. FIAS Scientific Life 3.1 Seminars and Colloquia . 20 3.2 Organized Conferences. .23 3.2 FIAS Forum . 25 4. Research Reports 4.1 Nuclear Physics, Particle Physics, Astrophysics . 26 4.2 Neuroscience. .59 4.3 Biology, Chemistry, Molecules, Nanosystems . 75 4.4 Scientific Computing, Information Technology . .101 5. Talks and Publications 5.1 Conference and Seminar Talks . 117 5.2 Conference Abstracts and Posters . 126 5.3 Cumulative List of Publications . 129 3 4 Preface In the year 2012 FIAS has continued to carry out its mission as an independent research institute performing cutting-edge research in the natural and computer sciences. An account of recent scientific accomplishments can be found in the brief individual research reports collected in Section 4. -
In Experimental Particle Physics
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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. -
Letter of Interest Fundamental Physics with Gravitational Wave Detectors
Snowmass2021 - Letter of Interest Fundamental physics with gravitational wave detectors Thematic Areas: (check all that apply /) (CF1) Dark Matter: Particle Like (CF2) Dark Matter: Wavelike (CF3) Dark Matter: Cosmic Probes (CF4) Dark Energy and Cosmic Acceleration: The Modern Universe (CF5) Dark Energy and Cosmic Acceleration: Cosmic Dawn and Before (CF6) Dark Energy and Cosmic Acceleration: Complementarity of Probes and New Facilities (CF7) Cosmic Probes of Fundamental Physics (TF09) Cosmology Theory (TF10) Quantum Information Science Theory Contact Information: Emanuele Berti (Johns Hopkins University) [[email protected]], Vitor Cardoso (Instituto Superior Tecnico,´ Lisbon) [[email protected]], Bangalore Sathyaprakash (Pennsylvania State University & Cardiff University) [[email protected]], Nicolas´ Yunes (University of Illinois at Urbana-Champaign) [[email protected]] Authors: (see long author lists after the text) Abstract: (maximum 200 words) Gravitational wave detectors are formidable tools to explore black holes and neutron stars. These com- pact objects are extraordinarily efficient at producing electromagnetic and gravitational radiation. As such, they are ideal laboratories for fundamental physics and they have an immense discovery potential. The detection of merging black holes by third-generation Earth-based detectors and space-based detectors will provide exquisite tests of general relativity. Loud “golden” events and extreme mass-ratio inspirals can strengthen the observational evidence for horizons by mapping the exterior spacetime geometry, inform us on possible near-horizon modifications, and perhaps reveal a breakdown of Einstein’s gravity. Measure- ments of the black-hole spin distribution and continuous gravitational-wave searches can turn black holes into efficient detectors of ultralight bosons across ten or more orders of magnitude in mass.