Annual Report Report 2019
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Group Theory
Appendix A Group Theory This appendix is a survey of only those topics in group theory that are needed to understand the composition of symmetry transformations and its consequences for fundamental physics. It is intended to be self-contained and covers those topics that are needed to follow the main text. Although in the end this appendix became quite long, a thorough understanding of group theory is possible only by consulting the appropriate literature in addition to this appendix. In order that this book not become too lengthy, proofs of theorems were largely omitted; again I refer to other monographs. From its very title, the book by H. Georgi [211] is the most appropriate if particle physics is the primary focus of interest. The book by G. Costa and G. Fogli [102] is written in the same spirit. Both books also cover the necessary group theory for grand unification ideas. A very comprehensive but also rather dense treatment is given by [428]. Still a classic is [254]; it contains more about the treatment of dynamical symmetries in quantum mechanics. A.1 Basics A.1.1 Definitions: Algebraic Structures From the structureless notion of a set, one can successively generate more and more algebraic structures. Those that play a prominent role in physics are defined in the following. Group A group G is a set with elements gi and an operation ◦ (called group multiplication) with the properties that (i) the operation is closed: gi ◦ g j ∈ G, (ii) a neutral element g0 ∈ G exists such that gi ◦ g0 = g0 ◦ gi = gi , (iii) for every gi exists an −1 ∈ ◦ −1 = = −1 ◦ inverse element gi G such that gi gi g0 gi gi , (iv) the operation is associative: gi ◦ (g j ◦ gk) = (gi ◦ g j ) ◦ gk. -
Looking at Earth: an Astronaut's Journey Induction Ceremony 2017
american academy of arts & sciences winter 2018 www.amacad.org Bulletin vol. lxxi, no. 2 Induction Ceremony 2017 Class Speakers: Jane Mayer, Ursula Burns, James P. Allison, Heather K. Gerken, and Gerald Chan Annual David M. Rubenstein Lecture Looking at Earth: An Astronaut’s Journey David M. Rubenstein and Kathryn D. Sullivan ALSO: How Are Humans Different from Other Great Apes?–Ajit Varki, Pascal Gagneux, and Fred H. Gage Advancing Higher Education in America–Monica Lozano, Robert J. Birgeneau, Bob Jacobsen, and Michael S. McPherson Redistricting and Representation–Patti B. Saris, Gary King, Jamal Greene, and Moon Duchin noteworthy Select Prizes and Andrea Bertozzi (University of James R. Downing (St. Jude Chil- Barbara Grosz (Harvard Univer- California, Los Angeles) was se- dren’s Research Hospital) was sity) is the recipient of the Life- Awards to Members lected as a 2017 Simons Investi- awarded the 2017 E. Donnall time Achievement Award of the gator by the Simons Foundation. Thomas Lecture and Prize by the Association for Computational American Society of Hematology. Linguistics. Nobel Prize in Chemistry, Clara D. Bloomfield (Ohio State 2017 University) is the recipient of the Carol Dweck (Stanford Univer- Christopher Hacon (University 2017 Robert A. Kyle Award for sity) was awarded the inaugural of Utah) was awarded the Break- Joachim Frank (Columbia Univer- Outstanding Clinician-Scientist, Yidan Prize. through Prize in Mathematics. sity) presented by the Mayo Clinic Di- vision of Hematology. Felton Earls (Harvard Univer- Naomi Halas (Rice University) sity) is the recipient of the 2018 was awarded the 2018 Julius Ed- Nobel Prize in Economic Emmanuel J. -
Download the Annual Review PDF 2016-17
Annual Review 2016/17 Pushing at the frontiers of Knowledge Portrait of Dr Henry Odili Nwume (Brasenose) by Sarah Jane Moon – see The Full Picture, page 17. FOREWORD 2016/17 has been a memorable year for the country and for our University. In the ever-changing and deeply uncertain world around us, the University of Oxford continues to attract the most talented students and the most talented academics from across the globe. They convene here, as they have always done, to learn, to push at the frontiers of knowledge and to improve the world in which we find ourselves. One of the highlights of the past twelve months was that for the second consecutive year we were named the top university in the world by the Times Higher Education Global Rankings. While it is reasonable to be sceptical of the precise placements in these rankings, it is incontrovertible that we are universally acknowledged to be one of the greatest universities in the world. This is a privilege, a responsibility and a challenge. Other highlights include the opening of the world’s largest health big data institute, the Li Ka Shing Centre for Health Information and Discovery, and the launch of OSCAR – the Oxford Suzhou Centre for Advanced Research – a major new research centre in Suzhou near Shanghai. In addition, the Ashmolean’s success in raising £1.35 million to purchase King Alfred’s coins, which included support from over 800 members of the public, was a cause for celebration. The pages that follow detail just some of the extraordinary research being conducted here on perovskite solar cells, indestructible tardigrades and driverless cars. -
Ingredients for Success 18Th HFSP Awardees Meeting
Ingredients for success In 2018, we yet again embarked on a new era in the HFSP by Guntram Bauer Fellowship program. After careful internal discussion and HFSPO Director of Scientific Affairs and Communications preparations, the review committee was presided over by a non- reviewing chair. Peter Koopman from the Institute of Molecular Bioscience of the University of Queensland took center stage as chair of this committee. Peter finished a four year tenure as a member of the fellowship review committee in 2016 and arrived back in Strasbourg after a three month sailing trip in the southern Pacific. Peer review at HFSP is not reading tea leaves but serious and demanding work for all involved. Thanks to Peter Koopman we successfully completed the first fellowship review committee run by a non-reviewing chair. We are still not sure what the magic ingredient was that made this fellowship committee stand out. Whether it was a truly committed international review panel, or the drive and oversight of its non-reviewing chair, or simply because of the HFSP Sauce which arrived in the chair's suitcase in Strasbourg. Probably all three, though be assured that we will get to the bottom of the HFSP Sauce! I don’t think we are boasting about HFSP when we say that our Program always tries to synchronize its procedures with the dynamics at the frontiers of science. This is particularly true for our peer review process. Over many years we have made more than just subtle changes to our procedures in response to feedback from the scientific community. -
Alternative Gravitational Theories in Four Dimensions
Alternative Gravitational Theories in Four Dimensionsa Friedrich W. Hehl Institute for Theoretical Physics, University of Cologne, D-50923 K¨oln, Germany email: [email protected] We argue that from the point of view of gauge theory and of an appropriate interpretation of the interferometer experiments with matter waves in a gravitational field, the Einstein- Cartan theory is the best theory of gravity available. Alternative viable theories are general relativity and a certain teleparallelism model. Objections of Ohanian & Ruffini against the Einstein-Cartan theory are discussed. Subsequently we list the papers which were read at the ‘Alternative 4D Session’ and try to order them, at least partially, in the light of the structures discussed. 1 The best alternative theory? I would call general relativity theory8 GR the best available alternative gravitational 21,14 theory and the next best one its teleparallel equivalent GR||. Because of these two theories, at least, it is good to have this alternative session during the Marcel Grossmann Meeting. Let me try to explain why I grant to GR the distinction of being the best alternative theory. After finally having set up special relativity theory in 1905, Einstein subse- quently addressed the question of how to generalize Newton’s gravitational theory as to make it consistent with special relativity, that is, how to reformulate it in a Poincar´ecovariant way. Newton’s theory was a battle tested theory in the realm of our planetary system and under normal laboratory conditions. It has predictive power as it had been shown by the prediction of the existence of the planet Neptune in the last century. -
Annual Report Fy 2018 Human Frontier Science Program Organization
APRIL 2017 APRIL 2018 — MARCH 2019 ANNUAL REPORT FY 2018 HUMAN FRONTIER SCIENCE PROGRAM ORGANIZATION The Human Frontier Science Program Organization (HFSPO) is unique, supporting international collaboration to undertake innovative, risky, basic research at the frontier of the life sciences. Special emphasis is given to the support and training of independent young investigators, beginning at the postdoctoral level. The Program is implemented by an international organisation, supported financially by Australia, Canada, France, Germany, India, Italy, Japan, the Republic of Korea, New Zealand, Norway, Singapore, Switzerland, the United Kingdom of Great Britain and Nothern Ireland, the United States of America, and the European Commission. Since 1990, over 7000 researchers from more than 70 countries have been supported. Of these, 28 HFSP awardees have gone on to receive the Nobel Prize. 2 The following documents are available on the HFSP website www.hfsp.org: Joint Communiqués (Tokyo 1992, Washington 1997, Berlin 2002, Bern 2004, Ottawa 2007, Canberra 2010, Brussels 2013, London 2016): https://www.hfsp.org/about/governance/membership Statutes of the International Human Frontier Science Program Organization: https://www.hfsp.org/about/governance/hfspo-statutes Guidelines for the participation of new members in HFSPO: https://www.hfsp.org/about/governance/membership General reviews of the HFSP (1996, 2001, 2006-2007, 2010, 2018): https://www.hfsp.org/about/strategy/reviews Updated and previous lists of awards, including titles and abstracts: -
A Comprehensive, Mechanistically Detailed, and Executable Model of the Cell Division Cycle in Saccharomyces Cerevisiae
bioRxiv preprint doi: https://doi.org/10.1101/298745; this version posted April 10, 2018. The copyright holder for this preprint (which was not certified by peer review) is the author/funder, who has granted bioRxiv a license to display the preprint in perpetuity. It is made available under aCC-BY-NC 4.0 International license. A comprehensive, mechanistically detailed, and executable model of the Cell Division Cycle in Saccharomyces cerevisiae Ulrike Münzner1, 2, Edda Klipp1 and Marcus Krantz1 1. Institute of Biology, Humboldt-Universität zu Berlin, Berlin, Germany 2. Bioinformatics Center, Institute for Chemical Research, Kyoto University, Uji, Japan [email protected] bioRxiv preprint doi: https://doi.org/10.1101/298745; this version posted April 10, 2018. The copyright holder for this preprint (which was not certified by peer review) is the author/funder, who has granted bioRxiv a license to display the preprint in perpetuity. It is made available under aCC-BY-NC 4.0 International license. ABSTRACT Understanding how cellular functions emerge from the underlying molecular mechanisms is one of the principal challenges in biology. It is widely recognised that this will require computational methods, and we expect the predictive power of these models to increase as model coverage and precision of formulation increase. The most potent examples to date are the genome-scale metabolic models that revolutionised their field and paved the way for a bacterial whole-cell model. However, to realise the potential of whole-cell models for eukaryotes, we must enable genome-scale modelling of other cellular networks. This has proven particularly challenging for the cellular regulatory networks, i.e. -
Newton-Cartan Gravity Revisited Andringa, Roel
University of Groningen Newton-Cartan gravity revisited Andringa, Roel IMPORTANT NOTE: You are advised to consult the publisher's version (publisher's PDF) if you wish to cite from it. Please check the document version below. Document Version Publisher's PDF, also known as Version of record Publication date: 2016 Link to publication in University of Groningen/UMCG research database Citation for published version (APA): Andringa, R. (2016). Newton-Cartan gravity revisited. Rijksuniversiteit Groningen. Copyright Other than for strictly personal use, it is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), unless the work is under an open content license (like Creative Commons). The publication may also be distributed here under the terms of Article 25fa of the Dutch Copyright Act, indicated by the “Taverne” license. More information can be found on the University of Groningen website: https://www.rug.nl/library/open-access/self-archiving-pure/taverne- amendment. Take-down policy If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. Downloaded from the University of Groningen/UMCG research database (Pure): http://www.rug.nl/research/portal. For technical reasons the number of authors shown on this cover page is limited to 10 maximum. Download date: 30-09-2021 1 Newton-Cartan gravity revisited Proefschrift ter verkrijging van de graad van doctor aan de Rijksuniversiteit Groningen op gezag van de rector magnificus prof. dr. E. -
2014 Annual Summary Corporate Plan
The Gairdner Foundation Corporate Plan 2014 TABLE OF CONTENTS PAGE Section I About the Gairdner Foundation 2 Objectives and Achievements to Date 5 Benefits 7 Section II Performance Results for 2013 Activities 7-8 Detailed 2013 Evaluations 9-10 Planned Activities and Anticipated Results 2014 11 Section III Financial Summary 12 Planned Receipts and Disbursements 2014 13-15 Section IV Risk Management 16 Section V Performance Monitoring 17-19 1 THE GAIRDNER FOUNDATION CORPORATE PLAN EXECUTIVE SUMMARY HISTORY The Gairdner Foundation was created by James A. Gairdner to recognize and reward the achievements of medical researchers whose work “contributes significantly to improving the quality of human life”. The Foundation is a Canadian organization that has never lost sight of its primary mission – the recognition of scientists it deemed to have made the most important breakthrough discoveries in biomedical science. It’s recipients are responsible for the discovery of the structure of DNA, the eradication of smallpox, CT scans, MRI machines, the human genome, the cure for ulcers, and the vaccine against HPV, to name a few. Since the first awards were granted in 1959, the Canada Gairdner Awards have become Canada's foremost international award- and one of the most prestigious awards in medical science. Our track record of consistent high quality adjudication and selection by the independent adjudication committees have resulted in global recognition and esteem. The Gairdner was incorporated in December 1957 as a charitable corporation under the laws of the Province of Ontario, Canada. Its funds originally derived from the personal gifts of the founder and members of his family. -
(November) 2017
ISSUE 2 (NOVEMBER) 2017 FEBS 2017 Congress FEBS Press FEBS Network 43rd FEBS Congress FEBS Advanced round-up Courses 2018 Page 3 Page 12 Page 14 Page 21 Page 24 CONTENTS Contents: The 2017 FEBS Congress Round-Up 3 Enjoy reports and photos from our big event of the year FEBS Press 12 3 Journal awards and activities at the 2017 FEBS Congress, and recent Special Issues FEBS Network 14 Wondering what it is? We introduce this exciting new initiative here 11 FEBS Education 15 A look back at key events this year aimed at 14 improving teaching in molecular life sciences ` FEBS Fellowships 17 Featuring recent distinguished Long-Term Fellows FEBS Community 18 12 Constituent Society meetings with FEBS National Lectures, and FEBS Council elections FEBS Congress 2018 21 And now to next year... Read about the plans from the Congress Chair and save the dates! 21 FEBS Advanced Courses 2018 24 Browse the list of next year’s focused-topic courses and meetings across Europe About FEBS News: This issue as well as all former issues of FEBS News are available online at www.febs.org. To receive an email when a new FEBS News issue is out, simply sign up to the e-newsletter in the News section of the FEBS website. Questions and suggestions about FEBS News should be sent to the FEBS News Editor, Carolyn Elliss ([email protected]). FEBS website postings: FEBS offers free advertising of academic positions (PhD students, postdocs, etc.) in the Career Opportunities section of the website, and scientific events can be listed in our Conference Calendar. -
A Scenario for Strong Gravity Without Extra Dimensions
A Scenario for Strong Gravity without Extra Dimensions D. G. Coyne (University of California at Santa Cruz) A different reason for the apparent weakness of the gravitational interaction is advanced, and its consequences for Hawking evaporation of a Schwarzschild black hole are investigated. A simple analytical formulation predicts that evaporating black holes will undergo a type of phase transition resulting in variously long-lived objects of reasonable sizes, with normal thermodynamic properties and inherent duality characteristics. Speculations on the implications for particle physics and for some recently-advanced new paradigms are explored. Section I. Motivation In the quest for grand unification of particle physics and gravitational interactions, the vast difference in the scale of the forces, gravity in particular, has long been a puzzle. In recent years, string theory developments [1] have suggested that the “extra” dimensions of that theory are responsible for the weakness of observed gravity, in a scenario where gravitons are unique in not being confined to a brane upon which the remaining force carriers are constrained to lie. While not a complete theory, such a scenario has interesting ramifications and even a prediction of sorts: if the extra dimensions are large enough, the Planck mass M = will be reduced to c G , G P hc GN h b b being a bulk gravitational constant >> GN. Black hole production at the CERN Large Hadron Collider is then predicted [2], together with the inability to probe high-energy particle physics at still higher energies and smaller distances. Experiments searching for consequences of the extra dimensions have not yet shown evidence for their existence, but have set upper limits on their characteristic sizes [3]. -
Hypergravity in Ads3
Physics Letters B 739 (2014) 106–109 Contents lists available at ScienceDirect Physics Letters B www.elsevier.com/locate/physletb Hypergravity in AdS3 Yu.M. Zinoviev Institute for High Energy Physics, Protvino, Moscow Region, 142280, Russia a r t i c l e i n f o a b s t r a c t Article history: Thirty years ago Aragone and Deser showed that in three dimensions there exists a consistent model Received 19 August 2014 describing interaction for massless spin-2 and spin-5/2fields. It was crucial that these fields lived in Received in revised form 18 September a flat Minkowski space and as a result it was not possible to deform such model into anti-de Sitter 2014 space. In this short note we show that such deformation becomes possible provided one compliment Accepted 17 October 2014 to the model with massless spin-4 field. Resulting theory can be considered as a Chern–Simons one Available online 24 October 2014 with a well-known supergroup OSp(1, 4). Moreover, there exists a straightforward generalization to the Editor: L. Alvarez-Gaumé OSp(1, 2n) case containing a number of bosonic fields with even spins 2, 4, ..., 2n and one fermionic field with spin n + 1/2. © 2014 Published by Elsevier B.V. This is an open access article under the CC BY license 3 (http://creativecommons.org/licenses/by/3.0/). Funded by SCOAP . 1. Introduction and show that in AdS background it describes interacting system 5 of massless spin-2, spin-4 and spin- 2 fields.