NIKHEF Annual Report 2002
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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. -
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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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. -
Bringing the Heavens Down to Earth
International Journal of High-Energy Physics CERN I COURIER Volume 44 Number 3 April 2004 Bringing the heavens down to Earth ACCELERATORS NUCLEAR PHYSICS Ministers endorse NuPECC looks to linear collider p6 the future p22 POWER CONVERTERS Principles : Technologies : • Linear, Switch Node primary or secondary, Current or voltage stabilized • Hani, or résonant» Buck, from % to the sub ppm level • Boost, 4-quadrant operation Limits : Control : * 1A up to 25kA • Local manual and/or computer control * 3V to 50kV • Interfaces: RS232, RS422, RS485, IEEE488/GPIB, •O.lkVAto 3MVA • CANbus, Profibus DP, Interbus S, Ethernet • Adaptation to EPICS • DAC and ADC 16 to 20 bit resolution and linearity Applications : Electromagnets and coils Superconducting magnets or short samples Resistive or capacitive loads Klystrons, lOTs, RF transmitters 60V/350OM!OkW Thyristor controlled (S£M®) I0"4, Profibus 80V/600A,50kW 5Y/30Ô* for supraconducting magnets linear technology < Sppm stability with 10 extra shims mm BROKER BIOSPIN SA • France •m %M W\. WSÊ ¥%, 34 rue de l'industrie * F-67166 Wissembourg Cedex Tél. +33 (0)3 88 73 68 00 • Fax. +33 (0)3 88 73 68 79 lOSPIN power@brukerir CONTENTS Covering current developments in high- energy physics and related fields worldwide CERN Courier is distributed to member-state governments, institutes and laboratories affiliated with CERN, and to their personnel. It is published monthly, except for January and August, in English and French editions. The views expressed are not CERN necessarily those of the CERN management. -
Annual Report 2001
2001 NATIONAL INSTITUTE FOR NUCLEAR PHYSICS AND HIGH-ENERGY PHYSICS ANNUAL REPORT 2001 Kruislaan 409, 1098 SJ Amsterdam P.O. Box 41882, 1009 DB Amsterdam Colofon Publication edited for NIKHEF: Address: Postbus 41882, 1009 DB Amsterdam Kruislaan 409, 1098 SJ Amsterdam Phone: +31 20 592 2000 Fax: +31 20 592 5155 E-mail: [email protected] Editors: Louk Lapik´as & Marcel Vreeswijk Layout & art-work: Kees Huyser Organisation: Anja van Dulmen Cover Photograph: A 3-D drawing of the LHCb Vertex detector URL: http://www.nikhef.nl The National Institute for Nuclear Physics and High-Energy Physics (NIKHEF) is a joint venture of the Stichting voor Fundamenteel Onderzoek der Materie (FOM), the Universiteit van Amsterdam (UVA), the Katholieke Universiteit Nijmegen (KUN), the Vrije Univer- siteit Amsterdam (VUA) and the Universiteit Utrecht (UU). The NIKHEF laboratory is located at the Science and Technology Centre Watergraafsmeer (WCW) in Amsterdam. The activities in experimental subatomic physics are coordinated and supported by NIKHEF with locations at Amsterdam, Nijmegen and Utrecht. The scientific programme is carried out by FOM, UVA, KUN,VUAandUUstaff.Experimentsaredone at the European accelerator centre CERN in Geneva, where NIKHEF participates in two LEP experiments (L3andDELPHI),inaneutrino experiment (CHORUS) and in SPS heavy ion experiments (NA57 and NA49). NIKHEF participates in the Tevatron experiment D0 at Fermilab, Chicago. At DESY in Hamburg NIKHEF participates in the ZEUS, HERMES and HERA-B experiments. Research and development activities are in progress for the future experiments ATLAS, ALICE and LHCb with the Large Hadron Collider (LHC) at CERN. NIKHEF is closely cooperating with the University of Twente. -
National Institute for Subatomic Physics Annual Report 2014
Annual Report 2014 Nikhef National Institute for Subatomic Physics Annual Report 2014 National Institute for Subatomic Physics Nikhef Colophon Nikhef Nationaal instituut voor subatomaire fysica National Institute for Subatomic Physics Visiting address Post address Science Park 105 P.O. Box 41882 1098 XG Amsterdam 1009 DB Amsterdam The Netherlands The Netherlands Telephone: +31 (0)20 592 2000 Fax: +31 (0)20 592 5155 E-mail: [email protected] URL: http://www.nikhef.nl Science communication Contact: Vanessa Mexner Telephone: +31 (0)20 592 5075 E-mail: [email protected] Editors: Stan Bentvelsen, Wouter Hulsbergen, Kees Huyser, Louk Lapikás, Frank Linde, Melissa van der Sande Layout: Kees Huyser Printer: Gildeprint Drukkerijen, Enschede Photos: Kees Huyser, Stan Bentvelsen, Jan Koopstra, Marco Kraan, Arne de Laat, Hanne Nijhuis, CERN Front cover: First full KM3NeT string of 18 optical modules assembled at Nikhef. Deployment in the Mediterranean Sea follows early 2015. Back cover: The Standard Model of particles since the discovery of the Higgs boson. Nikhef is the National Institute for Subatomic Physics in the Netherlands, in which the Foundation for Fundamental Research on Matter, the University of Amsterdam, VU University Amsterdam, Radboud University Nijmegen and Utrecht University collaborate. Nikhef coordinates and supports most activities in experimental particle and astroparticle physics in the Netherlands. Nikhef participates in experiments at the Large Hadron Collider at CERN, notably ATLAS, LHCb and ALICE. Astroparticle physics activities at Nikhef are fourfold: the ANTARES and KM3NeT neutrino telescope projects in the Mediterranean Sea; the Pierre Auger Observatory for cosmic rays, located in Argentina; gravitational-wave detection via the Virgo interferometer in Italy, and the projects eLISA and Einstein Telescope; and the direct search for Dark Matter with the XENON detector in the Gran Sasso underground laboratory in Italy. -
Input from the Netherlands for the European Strategy for Particle Physics – Update 2020
Input from the Netherlands for the European Strategy for Particle Physics – Update 2020 Stan Bentvelsen On behalf of Nikhef Particle- and Astroparticle Physics in the Netherlands The programme for Particle Physics in the Netherlands is co-ordinated by Nikhef, the National Institute for Particle Physics (www.nikhef.nl). Nikhef presently comprises groups from the NWO (Dutch national funding agency) Institute for Subatomic Physics and five universities: Free University of Amsterdam, Radboud University, University of Amsterdam, University of Groningen and Utrecht University. The historical aim of Nikhef was to be the Dutch home base for Particle Physics experiments at CERN. While this aim is still being honoured, Nikhef is now the home base for experiments at a larger variety of labs all around the world. The current Nikhef strategy is described in the Nikhef Strategy 2017-2020 and Beyond. The strategy is divided in three pillars: Proven Approaches, New Opportunities and Beyond Scientific goals. For the Proven Approaches Nikhef takes part in the particle physics experiments ATLAS, LHCb and ALICE. The Astroparticle Physics portfolio comprises of Advanced Virgo on gravitational waves, KM3NeT (and a small effort in protoDUNE) for the neutrino program, Pierre Auger Observatory for Ultra High Energetic Cosmic Rays and Xenon for the direct search of Dark matter. Further, Nikhef is building a precision atomic physics programme to determine the electric dipole moment of the electron. Next to these programs, Nikhef has a vivid theory department, a dedicated R&D group and a Physics Data Processing group. Together with SARA Nikhef houses a Tier-1 computing centre. In the Nikhef strategic plan the importance of a healthy theory community is underlined as essential for progress in Particle and Astroparticle Physics. -
Annual Report 2016 | University of Amsterdam 1
annual report 2016 | university of amsterdam 1 Annual Report 2016 uva.nl 2 annual report 2016 | university of amsterdam annual report 2016 | university of amsterdam 1 Annual Report 2016 University of Amsterdam 2 annual report 2016 | university of amsterdam Publication details Published by University of Amsterdam May 2017 Composition Strategy & Information Department Design April Design Cover photography Niké Dolman & Lisa Helder Photography AIAS | AMC | Andrea Kane | API | Bastiaan Aalbergsen | Bob Bronshoff | Bram Belloni | Carlos Fitzsimons | CLHC | Daan van Eijndhoven | David Cohen de Lara | Dirk Gillissen | DSM | Eduard Lampe | Faungg (Via Flickr) | FEB | Frank Linde | Free Press Media | GRAPPA | HIMS | Ingrid de Groot | Jan Willem Steenmeijer | Jeroen Oerlemans | KHMV | Liesbeth Dingemans | LinkedIn | Maarten van Haaff | Maartje Strijbis | Merijn Soeters | Judith van de Kamp | Monique Kooijmans | Nottingham Trent University | NTR | Rogier Fokke | RUG | Sander Nieuwenhuys | Sacha Epskamp | Stefan Pickee | Suzanne Blanchard | Teska Overbeeke | Ties Korstanje | University of Melbourne | Ursula Jernberg | VU Information University of Amsterdam Communications Office Postbus 19268 1000 GG Amsterdam +31 (0)20-525 2929 www.uva.nl No rights can be derived from the content of this Annual Report. © Universiteit van Amsterdam Disclaimer: Every effort has been made to provide an accurate translation of the text. However, the official text is the Dutch text: any differences in the translation are not binding and have no legal effect. annual report 2016 | university of amsterdam 3 Contents 5 a. Foreword by the Executive Board 7 b. Key data 9 c. Message from the Supervisory Board 14 d. Members of the Executive Board and the Supervisory Board 15 e. Faculty deans and directors of the organisational units 16 f. -
From the Web to the Grid and Beyond
The Frontiers Collection From the Web to the Grid and Beyond Computing Paradigms Driven by High-Energy Physics Bearbeitet von René Brun, Frederico Carminati, Giuliana Galli-Carminati 1. Auflage 2012. Buch. xx, 360 S. Hardcover ISBN 978 3 642 23156 8 Format (B x L): 15,5 x 23,5 cm Gewicht: 726 g Weitere Fachgebiete > EDV, Informatik > Hardwaretechnische Grundlagen > Grid- Computing & Paralleles Rechnen schnell und portofrei erhältlich bei Die Online-Fachbuchhandlung beck-shop.de ist spezialisiert auf Fachbücher, insbesondere Recht, Steuern und Wirtschaft. Im Sortiment finden Sie alle Medien (Bücher, Zeitschriften, CDs, eBooks, etc.) aller Verlage. Ergänzt wird das Programm durch Services wie Neuerscheinungsdienst oder Zusammenstellungen von Büchern zu Sonderpreisen. Der Shop führt mehr als 8 Millionen Produkte. Preface Modern High Energy Physics (HEP), as a science studying the results of accelerator- driven particle collisions, was born after the Second World War, at the same time as computers. HEP research has been constantly limited by technology, both in the accelerator and detector domains as well as that of computing. At the same time High Energy physicists have greatly contributed to the development of Information Technology. During all these years, the Conseil Europeen´ pour la Recherche Nucleaire´ 1 (CERN [1], located in Geneva, Switzerland) has been a privileged place for the evolution of HEP computing. Several applications conceived for HEP have found applications well beyond it, the World Wide Web (see Chap. 2) being the most notable example. During all these years HEP computing has faced the chal- lenge of software development within distributed communities, and of exploiting geographically distributed computing resources.