2017-2018 Perimeter Institute Annual Report English
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Emergence and Phenomenology in Quantum Gravity
Emergence and Phenomenology in Quantum Gravity by Isabeau Premont-Schwarz´ A thesis presented to the University of Waterloo in fulfillment of the thesis requirement for the degree of Doctor of Philosophy in Physics Waterloo, Ontario, Canada, 2010 © Isabeau Premont-Schwarz´ 2010 AUTHOR’S DECLARATION I hereby declare that I am the sole author of this thesis. This is a true copy of the thesis, including any required final revisions, as accepted by my examiners. I understand that my thesis may be made electronically available to the public. ii AUTHORSHIP STATEMENT This thesis is based on the following five articles: • A. Hamma, F. Markopoulou, I. Pr´emont-Schwarz and S. Severini, “Lieb-Robinson bounds and the speed of light from topological order,” Phys. Rev. Lett. 102 (2009) 017204 [arXiv:0808.2495 [quant-ph]]. • I. Pr´emont-Schwarz ,A. Hamma, I. Klich and F. Markopoulou, “Lieb-Robinson bounds for commutator-bounded operators ,” Phys. Rev. A 81, 040102(R) (2010) .[arXiv:0912.4544 [quant-ph]]. • I. Pr´emont-Schwarz and J. Hnybida, “Lieb-Robinson bounds with dependence on interaction strengths, ” [arXiv:1002.4190 [math-ph]]. • L. Modesto and I. Pr´emont-Schwarz, “Self-dual Black Holes in LQG: Theory and Phenomenology,” Phys. Rev. D 80, 064041 (2009) [arXiv:0905.3170 [hep-th]]. • S. Hossenfelder, L. Modesto and I. Pr´emont-Schwarz, “A model for non-singular black hole collapse and evaporation ,” Phys. Rev. D 81, 044036 (2010) [arXiv:0912.1823 [gr-qc]]. I did the majority of the work in the first article, but the project was initiated by Fotini Markopoulou-Kalamara and Alioscia Hamma and the manuscript was mostly written by Alioscia Hamma. -
Lecture Notes in Physics
Lecture Notes in Physics Editorial Board R. Beig, Wien, Austria J. Ehlers, Potsdam, Germany U. Frisch, Nice, France K. Hepp, Zurich,¨ Switzerland W. Hillebrandt, Garching, Germany D. Imboden, Zurich,¨ Switzerland R. L. Jaffe, Cambridge, MA, USA R. Kippenhahn, Gottingen,¨ Germany R. Lipowsky, Golm, Germany H. v. Lohneysen,¨ Karlsruhe, Germany I. Ojima, Kyoto, Japan H. A. Weidenmuller,¨ Heidelberg, Germany J. Wess, Munchen,¨ Germany J. Zittartz, Koln,¨ Germany 3 Berlin Heidelberg New York Barcelona Hong Kong London Milan Paris Singapore Tokyo Editorial Policy The series Lecture Notes in Physics (LNP), founded in 1969, reports new developments in physics research and teaching -- quickly, informally but with a high quality. Manuscripts to be considered for publication are topical volumes consisting of a limited number of contributions, carefully edited and closely related to each other. Each contribution should contain at least partly original and previously unpublished material, be written in a clear, pedagogical style and aimed at a broader readership, especially graduate students and nonspecialist researchers wishing to familiarize themselves with the topic concerned. For this reason, traditional proceedings cannot be considered for this series though volumes to appear in this series are often based on material presented at conferences, workshops and schools (in exceptional cases the original papers and/or those not included in the printed book may be added on an accompanying CD ROM, together with the abstracts of posters and other material suitable for publication, e.g. large tables, colour pictures, program codes, etc.). Acceptance Aprojectcanonlybeacceptedtentativelyforpublication,byboththeeditorialboardandthe publisher, following thorough examination of the material submitted. The book proposal sent to the publisher should consist at least of a preliminary table of contents outlining the structureofthebooktogetherwithabstractsofallcontributionstobeincluded. -
Annual Report to Industry Canada Covering The
Annual Report to Industry Canada Covering the Objectives, Activities and Finances for the period August 1, 2008 to July 31, 2009 and Statement of Objectives for Next Year and the Future Perimeter Institute for Theoretical Physics 31 Caroline Street North Waterloo, Ontario N2L 2Y5 Table of Contents Pages Period A. August 1, 2008 to July 31, 2009 Objectives, Activities and Finances 2-52 Statement of Objectives, Introduction Objectives 1-12 with Related Activities and Achievements Financial Statements, Expenditures, Criteria and Investment Strategy Period B. August 1, 2009 and Beyond Statement of Objectives for Next Year and Future 53-54 1 Statement of Objectives Introduction In 2008-9, the Institute achieved many important objectives of its mandate, which is to advance pure research in specific areas of theoretical physics, and to provide high quality outreach programs that educate and inspire the Canadian public, particularly young people, about the importance of basic research, discovery and innovation. Full details are provided in the body of the report below, but it is worth highlighting several major milestones. These include: In October 2008, Prof. Neil Turok officially became Director of Perimeter Institute. Dr. Turok brings outstanding credentials both as a scientist and as a visionary leader, with the ability and ambition to position PI among the best theoretical physics research institutes in the world. Throughout the last year, Perimeter Institute‘s growing reputation and targeted recruitment activities led to an increased number of scientific visitors, and rapid growth of its research community. Chart 1. Growth of PI scientific staff and associated researchers since inception, 2001-2009. -
A Search for Lorentz-Boosted Higgs Bosons Decaying to Charm Quarks in the CMS Experiment Using Deep Neural Networks
University of California Santa Barbara A search for Lorentz-boosted Higgs bosons decaying to charm quarks in the CMS experiment using deep neural networks A dissertation submitted in partial satisfaction of the requirements for the degree Doctor of Philosophy in Physics by Huilin Qu CERN-THESIS-2019-165 Committee in charge: Professor Joseph Incandela, Chair Associate Professor Nathaniel Craig Professor Jeffrey Richman September 2019 The Dissertation of Huilin Qu is approved. Associate Professor Nathaniel Craig Professor Jeffrey Richman Professor Joseph Incandela, Committee Chair September 2019 A search for Lorentz-boosted Higgs bosons decaying to charm quarks in the CMS experiment using deep neural networks Copyright © 2019 by Huilin Qu iii Acknowledgements The pursuit of my Ph.D. in particle physics is a long journey with many ups and downs. I am grateful to so many people who showed up along this way, influenced me greatly with their knowledge and character, and provided me with invaluable help and support. I apologize I cannot name every one of them here – the list is too long. But I have my sincere gratitude to all of them deep in my heart. First of all, I would like to express my deepest gratitude to my research advisor, Prof. Joseph Incandela, for being always so supportive and inspiring, for allowing a lot of freedom in my research, and for providing me with countless valuable suggestions not only about my research but also on how to grow as a scientist. Talking with him is like magic – his words are so inspiring, and can always clear up my doubts and leave me motivated. -
Sabine Hossenfelder on “The Case Against Beauty in Physics” Julia
Rationally Speaking #211: Sabine Hossenfelder on “The case against beauty in physics” Julia: Welcome to Rationally Speaking, the podcast where we explore the borderlands between reason and nonsense. I'm your host, Julia Galef, and I'm here with today's guest, Sabine Hossenfelder. Sabine is a theoretical physicist, focusing on quantum gravity. She's a research fellow at the Frankfurt Institute for Advanced Studies, and blogs at Back Reaction. She just published the book, "Lost in Math: How Beauty Leads Physics Astray." "Lost in Math” argues that physicists, in at least certain sub-fields, evaluate theories based heavily on aesthetics, like is this theory beautiful? Instead of simply, what does the evidence suggest is true? The book is full of interviews Sabine did with top physicists, where she tries to ask them: what's the justification for this? Why should we expect beauty to be a good guide to truth? And, spoiler alert, ultimately, she comes away rather unsatisfied with the answers. So, we're going to talk about "Lost in Math" and the case for and against beauty in physics. Sabine, welcome to the show. Sabine: Hello. Julia: So, probably best to start with: what do you mean by beauty, in this context? And is it closer to a kind of “beauty is in the eye of the beholder” thing, like, every physicist has their own sort of aesthetic sense? Or is more like there's a consensus among physicists about what constitutes a beautiful theory? Sabine: Interestingly enough, there's mostly consensus about it. Let me put ahead that I will not try to tell anyone what beauty means, I am just trying to summarize what physicists seem to mean when they speak of beauty, when they say “that theory is beautiful.” There are several ingredients to this sense of beauty. -
Gravity Without Dark Matter
Gravity Without Dark Matter John Moffat Perimeter Institute for Theoretical Physics, Waterloo, Ontario, Canada 1/13/2005 Miami 2004 1 Contents n 1. Introduction n 2. Gravity theory n 3. Action and field equations n 4. Quantum gravity and group renormalization flow n 5. Modified Newtonian acceleration n and flat galaxy rotation curves n 6. Galaxy clusters and lensing n 7. Cosmology without dark matter n 8. Conclusions 1/13/2005 Miami 2004 2 1. Introduction n Can gravity theory explain galaxy dynamics and cosmology without dominant dark matter? n We need a gravity theory that generalizes GR. Such a generalization is nonsymmetric gravitational theory (NGT). n A simpler theory is metric-skew-tensor gravity (MSTG). n There is also the problem of the nature of Dark Energy that explains the accelerating Universe. n The gravity theory must be stable and contain GR in a consistent way. It must yield agreement with solar system tests and the binary pulsar PSR 1913+16. n The cosmology without dominant dark matter must agree with the latest WMAP and CMB data. 1/13/2005 Miami 2004 3 2. Gravity theory n A popular phenomenological model that replaces dark matter is MOND (Milgrom, Beckenstein, Sanders-McGough). This phenomenology fits the flat rotation curves of galaxies, but has no acceptable relativistic gravity theory (see, however, Beckenstein 2004). n The MSTG theory can explain flat rotation curves of galaxies and cosmology without dominant dark matter. n We need to incorporate quantum gravity in a renormalization group (RG) flow framework with effective running coupling “constants” and an effective action. -
Dancing to the Tempo of LEP
INTERNATIONAL JOURNAL OF HIGH-ENERGY PHYSICS CERN COURIER VOLUME 40 NUMBER 10 DECEMBER 2000 Dancing to the tempo of LEP SPIN SUPERSYMMETRY INTERNET Polarized protons accelerated Striking suggestions for How the Web was Born, a new in new RHIC ring p8 additional physics symmetry pl7 book p43 E RI Hew Gêner CES Creative Electronic Systems 70 route du Hunt-dun*! CH-1213 Petit-Uncy, Switzerland Internet: nttp://www.ces.cft I The Ultimate VME Machine CES Switzeriand The RI03 features a twin bus architecture, a Tel: ^41.22.879.51.00 ifque fnter-processor communication mechanism Fax: +4U2.792.57.4d Email; [email protected] for ultra-high-speed data acquisitions g and user-level load balance control CES.O Germany with dedicated hardware. Tel: +49.60.51.96.97.41 Fax; +49.60,51.96.97.33 Sheer Speed: Êttuiil: [email protected] # • VME - block transfers in 2eSST at CES MSâ 300 MBytes/s, single cycles at 20 MBytes/s Tel:+ 1.518.843.1445 Fax;+1.518.643.1447 * Memory - 400 MBytes/s average, Email: [email protected] 800 MBytes/s peak • Multi-Access - VME + PCM + PCI 2 + CPU without global degradation CPU Power: PowerPC 750 or 7400 at maximum available speed I Flexible: Two Independent 64-bit PCI with simultaneous access to the memory I Scalable: Up to four additional PMC's on a PMC carrier system MFCC 844x PMC PROCESSORS • 130 KGates user-FPGA • Continuous acquisition at 50 MBytes/s In 32 or 64~bit mode • Full 750 / 7400 computing core • Full network services on PCI * Complete multi-processing software with connection oriented high-speed data transfers SOFTWARE SUPPORT VxWorics®, Lynxob®, muecat® and LINUX® development software including support for hard real-time target machines. -
Benjamin J. Owen - Curriculum Vitae
BENJAMIN J. OWEN - CURRICULUM VITAE Contact information Mail: Texas Tech University Department of Physics & Astronomy Lubbock, TX 79409-1051, USA E-mail: [email protected] Phone: +1-806-834-0231 Fax: +1-806-742-1182 Education 1998 Ph.D. in Physics, California Institute of Technology Thesis title: Gravitational waves from compact objects Thesis advisor: Kip S. Thorne 1993 B.S. in Physics, magna cum laude, Sonoma State University (California) Minors: Astronomy, German Research advisors: Lynn R. Cominsky, Gordon G. Spear Academic positions Primary: 2015{ Professor of Physics & Astronomy Texas Tech University 2013{2015 Professor of Physics The Pennsylvania State University 2008{2013 Associate Professor of Physics The Pennsylvania State University 2002{2008 Assistant Professor of Physics The Pennsylvania State University 2000{2002 Research Associate University of Wisconsin-Milwaukee 1998{2000 Research Scholar Max Planck Institute for Gravitational Physics (Golm) Secondary: 2015{2018 Adjunct Professor The Pennsylvania State University 2012 (2 months) Visiting Scientist Max Planck Institute for Gravitational Physics (Hanover) 2010 (6 months) Visiting Associate LIGO Laboratory, California Institute of Technology 2009 (6 months) Visiting Scientist Max Planck Institute for Gravitational Physics (Hanover) Honors and awards 2017 Princess of Asturias Award for Technical and Scientific Research (with the LIGO Scientific Collaboration) 2017 Albert Einstein Medal (with the LIGO Scientific Collaboration) 2017 Bruno Rossi Prize for High Energy Astrophysics (with the LIGO Scientific Collaboration) 2017 Royal Astronomical Society Group Achievement Award (with the LIGO Scientific Collab- oration) 2016 Gruber Cosmology Prize (with the LIGO Scientific Collaboration) 2016 Special Breakthrough Prize in Fundamental Physics (with the LIGO Scientific Collabora- tion) 2013 Fellow of the American Physical Society 1998 Milton and Francis Clauser Prize for Ph.D. -
LIGO's Unsung Heroes : Nature News & Comment
NATURE | NEWS LIGO's unsung heroes Nature highlights just a few of the people who played a crucial part in the discovery of gravitational waves — but didn’t win the Nobel Prize. Davide Castelvecchi 09 October 2017 Corrected: 19 October 2017 Joe McNally/Getty LIGO hunts gravitational waves with the help of two laser interferometers — and hundreds of people. Expand Every October, the announcements of the Nobel Prizes bring with them some controversy. This year’s physics prize — in recognition of the Laser Interferometer Gravitational-Wave Observatory (LIGO) in the United States — was less debated than most. The three winners — Kip Thorne and Barry Barish, both at the California Institute of Technology (Caltech) in Pasadena, and Rainer Weiss at the Massachusetts Institute of Technology (MIT) in Cambridge — had attracted near-universal praise for their roles in the project’s success. But the award has still put into stark relief the difficulty of singling out just a few individuals from the large collaborations of today’s 'Big Science'. The LIGO collaboration uses two giant laser interferometers to listen for deformations in space-time caused by some of the Universe’s most cataclysmic events. Physicists detected their first gravitational waves — interpreted as being produced by the collision of two black holes more than a billion years ago — in September 2015. The resulting paper, published in February 20161, has a mind-boggling 1,004 authors. Some of those are members of the LIGO Laboratory, the Caltech–MIT consortium that manages LIGO’s two interferometers in Louisiana and Washington State. But the list also includes the larger LIGO Scientific Collaboration: researchers from 18 countries, some of which — such as Germany and the United Kingdom — have made crucial contributions to the detectors. -
Einstein Not Yet Displaced Controversial Theory of Varying Speed of Light Still Lacks a Solid Foundation
books and arts Einstein not yet displaced Controversial theory of varying speed of light still lacks a solid foundation. Faster Than the Speed of Light: The Story of a Scientific Speculation MILES COLE by João Magueijo William Heinemann/Perseus: 2003. 320 pp. £16.99/$26 George Ellis João Magueijo is one of many who hope to see the epitaph ‘Einstein was wrong, I was right’ on their gravestone. He is a cosmolo- gist who, one rainy morning in Cambridge, suddenly saw the possibility of a varying speed of light (VSL) as an alternative to the inflationary-theory paradigm that domi- nates present-day theoretical cosmology. He knew from the start that it represented a fundamental challenge to physics ortho- doxy (it violates the foundations of Einstein’s special theory of relativity) and would not easily be accepted, but he worked enthusi- astically to develop the idea. He found a collaborator who wavered but eventually completed a joint paper with him on the topic. This was rejected by major journals but was eventually accepted for publication read and referred to. Why, then, his major dis- Magueijo has not gone back to the founda- after a long battle. He then discovered that content? He has had no more difficulty than tions and sorted them out. Any theory of the idea had already been proposed, in a many others who have presented challenges this kind needs, first, a viable proposal slightly different form, by John Moffat. He to orthodoxy. All major new ideas have for measuring both time and distance, as found new collaborators and with them been resisted in their time: the expanding velocity is based on this; second, a physical developed variants of his theory. -
CV Karsten Danzmann
Curriculum Vitae for Prof. Dr. Karsten Danzmann May 23, 2017 Affiliation Director, Max Planck Institute for Gravitational Physics (Albert Einstein Institute) and Director, Institute for Gravitational Physics, Leibniz Universität Hannover Callinstr. 38, D-30167 Hannover, Germany http://www.aei.mpg.de/18307/04_Laser_Interferometry_and_Gravitational_Wave_Astronomy Tel.: +49 511 762 2356, Fax: +49 511 762 5861, Email: [email protected] Personal Details Born February 6, 1955 in Rotenburg/Wümme in Germany, German citizen Education 1974 Pre-Diploma in Physics, Technical University Clausthal-Zellerfeld, Germany 1977 Diploma in Physics, University of Hannover, Germany 1980 PhD, University of Hannover, Germany Academic Employment 1978 - 1982 Staff Scientist, University of Hannover 1982 - 1983 Visiting Scientist (DFG fellowship) Stanford University, USA 1983 - 1986 Staff Scientist, PTB Berlin, Germany 1986 - 1989 Act. Ass. Professor of Physics, Stanford University, USA 1990 - 1993 Project Leader Gravitational Waves, Max Planck Institute for Quantum Optics, Garching, Germany 1993 - 2001 Head of Remote Branch Hannover, Max Planck Institute for Quantum Optics 1993 - present Professor (W3), Leibniz Universität Hannover, Director of Institute for Gravitational Physics (formerly Institute for Atomic and Molecular Physics) 2002 - present Director at Max Planck Institute for Gravitational Physics (Albert Einstein Institute) 2004 - 2005 Dean, University of Hannover, Germany Scientific Activities 1993 - present Principal Investigator of the ground-based -
Annual Report for the Fiscal Year July 1, 1980
The Institute for Advanced Study .nnual Report 1980 This Annual Report has been made possible by a generous grant from the Union Carbide Corporation. ! The Institute for Advanced Study Annual Report for the Fiscal Year July 1, 1980-June 30, 1981 The Institute for Advanced Study Olden Lane Princeton, New Jersey 08540 U.S.A. Printed by Princeton University Press Designed by Bruce Campbell x4S36 /98I It is fundamental to our purpose, and our Extract from the letter addressed by the express desire, that in the appointments to Founders to the Institute's Trustees, the staff and faculty, as well as in the dated June 6, 1930, Newark, New Jersey. admission of workers and students, no account shall be taken, directly or indirectly, of race, religion or sex. We feel strongly that the spirit characteristic of America at its noblest, above all, the pursuit of higher learning, cannot admit of any conditions as to personnel other than those designed to promote the objects for which this institution is established, and particularly with no regard whatever to accidents of race, creed or sex. /r2- S39 Table of Contents Trustees and Officers Founders Caroline Bamberger Fuld Louis Bamberger Board of Trustees Daniel Bell Howard C. Kauffmann Professor of Sociology President Harvard University Exxon Corporation Charles L. Brown John R. Opel Chairman the Board of and Chief President and Chief Executive Officer Executive Officer IBM Corporation American Telephone and Telegraph Company Howard C. Petersen Philadelphia, Pennsylvania Fletcher L. Byrom Chairman of the Board Martin E. Segal Koppers Company, Inc. Partner, Wertheim & Co.; Chairman, Martin E.