Report on the 2016 Morningside Medals by Jing Yu*
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Kloosterman Sheaves for Reductive Groups
Annals of Mathematics 177 (2013), 241{310 http://dx.doi.org/10.4007/annals.2013.177.1.5 Kloosterman sheaves for reductive groups By Jochen Heinloth, Bao-Chau^ Ngo,^ and Zhiwei Yun Abstract 1 Deligne constructed a remarkable local system on P − f0; 1g attached to a family of Kloosterman sums. Katz calculated its monodromy and asked whether there are Kloosterman sheaves for general reductive groups and which automorphic forms should be attached to these local systems under the Langlands correspondence. Motivated by work of Gross and Frenkel-Gross we find an explicit family of such automorphic forms and even a simple family of automorphic sheaves in the framework of the geometric Langlands program. We use these auto- morphic sheaves to construct `-adic Kloosterman sheaves for any reductive group in a uniform way, and describe the local and global monodromy of these Kloosterman sheaves. In particular, they give motivic Galois rep- resentations with exceptional monodromy groups G2;F4;E7 and E8. This also gives an example of the geometric Langlands correspondence with wild ramification for any reductive group. Contents Introduction 242 0.1. Review of classical Kloosterman sums and Kloosterman sheaves 242 0.2. Motivation and goal of the paper 244 0.3. Method of construction 246 0.4. Properties of Kloosterman sheaves 247 0.5. Open problems 248 0.6. Organization of the paper 248 1. Structural groups 249 P1 1.1. Quasi-split group schemes over nf0;1g 249 1.2. Level structures at 0 and 1 250 1.3. Affine generic characters 252 1.4. Principal bundles 252 2. -
Orbital Resonances and GPU Acceleration of Binary Black Hole Inspiral Simulations
Orbital resonances and GPU acceleration of binary black hole inspiral simulations by Adam Gabriel Marcel Lewis A thesis submitted in conformity with the requirements for the degree of Doctor of Philosophy Department of Physics University of Toronto c Copyright 2018 by Adam Gabriel Marcel Lewis Abstract Orbital resonances and GPU acceleration of binary black hole inspiral simulations Adam Gabriel Marcel Lewis Doctor of Philosophy Department of Physics University of Toronto 2018 Numerical relativity, the direct numerical integration of the Einstein field equations, is now a mature subfield of computational physics, playing a critical role in the generation of signal templates for comparison with data from ground-based gravitational wave de- tectors. The application of numerical relativity techniques to new problems is at present complicated by long wallclock times and intricate code. In this thesis we lay groundwork to improve this situation by presenting a GPU port of the numerical relativity code SpEC. Our port keeps code maintenance feasible by relying on various layers of automation, and achieves high performance across a variety of GPUs. We secondly introduce a C++ soft- ware package, TLoops, which allows numerical manipulation of tensors using single-line C++ source-code expressions resembling familiar tensor calculus notation. These expres- sions may be compiled and executed immediately, but also can be used to automatically generate equivalent GPU or low-level CPU code, which then executes in their place. The GPU code in particular achieves near-peak performance. Finally, we present simulations of eccentric binary black holes. We develop new methods to extract the fundamental fre- quencies of these systems. -
Comments on the 2011 Shaw Prize in Mathematical Sciences - - an Analysis of Collectively Formed Errors in Physics by C
Global Journal of Science Frontier Research Physics and Space Science Volume 12 Issue 4 Version 1.0 June 2012 Type : Double Blind Peer Reviewed International Research Journal Publisher: Global Journals Inc. (USA) Online ISSN: 2249-4626 & Print ISSN: 0975-5896 Comments on the 2011 Shaw Prize in Mathematical Sciences - - An Analysis of Collectively Formed Errors in Physics By C. Y. Lo Applied and Pure Research Institute, Nashua, NH Abstract - The 2011 Shaw Prize in mathematical sciences is shared by Richard S. Hamilton and D. Christodoulou. However, the work of Christodoulou on general relativity is based on obscure errors that implicitly assumed essentially what is to be proved, and thus gives misleading results. The problem of Einstein’s equation was discovered by Gullstrand of the 1921 Nobel Committee. In 1955, Gullstrand is proven correct. The fundamental errors of Christodoulou were due to his failure to distinguish the difference between mathematics and physics. His subsequent errors in mathematics and physics were accepted since judgments were based not on scientific evidence as Galileo advocates, but on earlier incorrect speculations. Nevertheless, the Committee for the Nobel Prize in Physics was also misled as shown in their 1993 press release. Here, his errors are identified as related to accumulated mistakes in the field, and are illustrated with examples understandable at the undergraduate level. Another main problem is that many theorists failed to understand the principle of causality adequately. It is unprecedented to award a prize for mathematical errors. Keywords : Nobel Prize; general relativity; Einstein equation, Riemannian Space; the non- existence of dynamic solution; Galileo. GJSFR-A Classification : 04.20.-q, 04.20.Cv Comments on the 2011 Shaw Prize in Mathematical Sciences -- An Analysis of Collectively Formed Errors in Physics Strictly as per the compliance and regulations of : © 2012. -
New Publications Offered by The
New Publications Offered by the AMS To subscribe to email notification of new AMS publications, please go to www.ams.org/bookstore-email. Algebra and Algebraic Geometry theorem in noncommutative geometry; M. Guillemard, An overview of groupoid crossed products in dynamical systems. Contemporary Mathematics, Volume 676 Noncommutative November 2016, 222 pages, Softcover, ISBN: 978-1-4704-2297-4, LC 2016017993, 2010 Mathematics Subject Classification: 00B25, 46L87, Geometry and Optimal 58B34, 53C17, 46L60, AMS members US$86.40, List US$108, Order Transport code CONM/676 Pierre Martinetti, Università di Genova, Italy, and Jean-Christophe Wallet, CNRS, Université Paris-Sud 11, Orsay, France, Editors Differential Equations This volume contains the proceedings of the Workshop on Noncommutative Geometry and Optimal Transport, held on November 27, 2014, in Shock Formation in Besançon, France. The distance formula in noncommutative geometry was introduced Small-Data Solutions to by Connes at the end of the 1980s. It is a generalization of Riemannian 3D Quasilinear Wave geodesic distance that makes sense in a noncommutative setting, and provides an original tool to study the geometry of the space of Equations states on an algebra. It also has an intriguing echo in physics, for it yields a metric interpretation for the Higgs field. In the 1990s, Jared Speck, Massachusetts Rieffel noticed that this distance is a noncommutative version of the Institute of Technology, Cambridge, Wasserstein distance of order 1 in the theory of optimal transport. MA More exactly, this is a noncommutative generalization of Kantorovich dual formula of the Wasserstein distance. Connes distance thus offers In 1848 James Challis showed that an unexpected connection between an ancient mathematical problem smooth solutions to the compressible and the most recent discovery in high energy physics. -
Finite-Time Degeneration of Hyperbolicity Without Blowup for Quasilinear Wave Equations
Finite-time degeneration of hyperbolicity without blowup for quasilinear wave equations The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Speck, Jared. “Finite-Time Degeneration of Hyperbolicity Without Blowup for Quasilinear Wave Equations.” Analysis & PDE 10, 8 (August 2017): 2001–2030 As Published http://dx.doi.org/10.2140/APDE.2017.10.2001 Publisher Mathematical Sciences Publishers Version Author's final manuscript Citable link http://hdl.handle.net/1721.1/116021 Terms of Use Creative Commons Attribution-Noncommercial-Share Alike Detailed Terms http://creativecommons.org/licenses/by-nc-sa/4.0/ FINITE-TIME DEGENERATION OF HYPERBOLICITY WITHOUT BLOWUP FOR QUASILINEAR WAVE EQUATIONS JARED SPECK∗† Abstract. In three spatial dimension, we study the Cauchy problem for the wave equation 2 P ∂t Ψ+(1+Ψ) ∆Ψ = 0 for P 1, 2 . We exhibit a form of stable Tricomi-type degen- eracy− formation that has not previously∈ { } been studied in more than one spatial dimension. Specifically, using only energy methods and ODE techniques, we exhibit an open set of data such that Ψ is initially near 0 while 1 + Ψ vanishes in finite time. In fact, generic data, when appropriately rescaled, lead to this phenomenon. The solution remains regular in the following sense: there is a high-order L2-type energy, featuring degenerate weights only at the top-order, that remains bounded. When P = 1, we show that any C1 extension of Ψ to the future of a point where 1+Ψ = 0 must exit the regime of hyperbolicity. Moreover, the Kretschmann scalar of the Lorentzian metric corresponding to the wave equation blows up at those points. -
Sastra Prize 2010
UF SASTRA PRIZE Mathematics 2010 Research Courses Undergraduate Graduate News Resources People WEI ZHANG TO RECEIVE 2010 SASTRA RAMANUJAN PRIZE The 2010 SASTRA Ramanujan Prize will be awarded to Wei Zhang, who is now a Benjamin Pierce Instructor at the Department of Mathematics, Harvard University, USA. This annual prize which was established in 2005, is for outstanding contributions by very young mathematicians to areas influenced by the genius Srinivasa Ramanujan. The age limit for the prize has been set at 32 because Ramanujan achieved so much in his brief life of 32 years. The $10,000 prize will be awarded at the International Conference on Number Theory and Automorphic Forms at SASTRA University in Kumbakonam, India (Ramanujan's hometown) on December 22, Ramanujan's birthday. Dr. Wei Zhang has made far reaching contributions by himself and in collaboration with others to a broad range of areas in mathematics including number theory, automorphic forms, L-functions, trace formulas, representation theory and algebraic geometry. We highlight some of his path-breaking contributions: In 1997, Steve Kudla constructed a family of cycles on Shimura varieties and conjectured that their generating functions are actually Siegel modular forms. The proof of this conjecture for Kudla cycles of codimension 1 is a major theorem of the Fields Medalist Borcherds. In his PhD thesis, written under the direction of Professor Shou Wu Zhang at Columbia University, New York, Wei Zhang established conditionally, among other things, a generalization of the results of Borcherds to higher dimensions, and in that process essentially settled the Kudla conjecture. His thesis, written when he was just a second year graduate student, also extended earlier fundamental work of Hirzebruch-Zagier and of Gross-Kohnen- Zagier. -
Is String Theory Holographic? 1 Introduction
Holography and large-N Dualities Is String Theory Holographic? Lukas Hahn 1 Introduction1 2 Classical Strings and Black Holes2 3 The Strominger-Vafa Construction3 3.1 AdS/CFT for the D1/D5 System......................3 3.2 The Instanton Moduli Space.........................6 3.3 The Elliptic Genus.............................. 10 1 Introduction The holographic principle [1] is based on the idea that there is a limit on information content of spacetime regions. For a given volume V bounded by an area A, the state of maximal entropy corresponds to the largest black hole that can fit inside V . This entropy bound is specified by the Bekenstein-Hawking entropy A S ≤ S = (1.1) BH 4G and the goings-on in the relevant spacetime region are encoded on "holographic screens". The aim of these notes is to discuss one of the many aspects of the question in the title, namely: "Is this feature of the holographic principle realized in string theory (and if so, how)?". In order to adress this question we start with an heuristic account of how string like objects are related to black holes and how to compare their entropies. This second section is exclusively based on [2] and will lead to a key insight, the need to consider BPS states, which allows for a more precise treatment. The most fully understood example is 1 a bound state of D-branes that appeared in the original article on the topic [3]. The third section is an attempt to review this construction from a point of view that highlights the role of AdS/CFT [4,5]. -
2Nd Announcement 2018 Poster-1
Under the Auspices of H. E. the President of the Hellenic Republic Mr. Prokopios Pavlopoulos First Congress of Greek Mathematicians FCGM-2018 June 25–30, 2018 Athens, Greece Organizers Hellenic Mathematical Society (HMS) in cooperation with the Cyprus Mathematical Society (CMS) and the Mathematical Society of Southeastern Europe (MASSEE) Department of Mathematics, National and Kapodistrian University of Athens (NKUA) School of Applied Mathematical and Physical Sciences, National Technical University of Athens (NTUA) 1 Department of Mathematics, Aristotle University of Thessaloniki Department of Mathematics, University of Patras Department of Mathematics, University of Ioannina Department of Mathematics and Applied Mathematics, University of Crete Department of Statistics, Athens University of Economics and Business Department of Mathematics, University of the Aegean School of Science and Technology Hellenic Open University and the General Secretariat for Greeks Abroad Second Announcement and Call for Abstracts The Hellenic Mathematical Society (HMS) was founded in 1918 with the main goal to further and encourage the study and research in Mathematics and its numerous applications, as well as the evolvement of Mathematical Education in Greece. The First Congress of Greek Mathematicians aims to make Athens a city of reunion of all Greek Mathematicians living in Greece and abroad. The programme of the Congress will cover all areas of pure and applied mathematics. It will host plenary lectures, invited lectures, and several sessions and mini-symposia tentatively in: Algebra and Combinatorics; Analysis; Computer Science (Mathematical Aspects); Control Theory, Operations Research and Optimization; Differential Equations and Dynamical Systems; Geometry; History and Philosophy of Mathematics; Logic and Foundations of Mathematics; Mathematical Physics; Mathematical Finance; Mathematics Education; Number Theory, Arithmetic Geometry and Cryptography; Numerical Analysis and Scientific Computing; Probability and Statistics; Topology and Applications. -
Hawking Radiation and Black Hole Thermodynamics
HAWKING RADIATION AND BLACK HOLE THERMODYNAMICS ∗ Don N. Page † Institute for Theoretical Physics Department of Physics, University of Alberta Edmonton, Alberta, Canada T6G 2J1 (2004 September 3; additional section added 2004 December 31 ‡) Abstract An inexhaustive review of Hawking radiation and black hole thermody- namics is given, focusing especially upon some of the historical aspects as seen from the biased viewpoint of a minor player in the field on and off for the past thirty years. arXiv:hep-th/0409024v3 31 Dec 2004 ∗Alberta-Thy-18-04, hep-th/0409024, review article solicited for a celebratory Focus Issue on Relativity, “Spacetime 100 Years Later,” to be published in New Journal of Physics. †Internet address: [email protected] ‡On this date the author reached an age which is an integer divisor of the number of references. 1 1 Historical Background Black holes are perhaps the most perfectly thermal objects in the universe, and yet their thermal properties are not fully understood. They are described very accurately by a small number of macroscopic parameters (e.g., mass, angular mo- mentum, and charge), but the microscopic degrees of freedom that lead to their thermal behavior have not yet been adequately identified. Strong hints of the thermal properties of black holes came from the behavior of their macroscopic properties that were formalized in the (classical) four laws of black hole mechanics [1], which have analogues in the corresponding four laws of thermodynamics: The zeroth law of black hole mechanics is that the surface gravity κ of a stationary black hole is constant over its event horizon [2, 1]. -
The University of Tokyo's Newly Founded Institute for the Physics
hosted by IPMU was held on 17 - 21 with new projects. The success of the News December 2007. The workshop,“ Focus workshop also clarified the importance Week on LHC Phenomenology”, was of follow-up visitor programs, such as organized by Mihoko Nojiri (PI of IPMU) one month stays to finalize the projects and held at the IPMU, Research Center started in this meeting.” Building, on the Kashiwa campus. Many theorists found the discussion The Large Hadron Collider (LHC) at with experimentalists extremely CERN in Switzerland will start operating important, and vice verse.“ We in 2008. The aim of the meeting was to developed a consensus that it is bring together leading experimentalists important to set a series of workshops and phenomenologists working on LHC, to understand phenomena at the LHC to come up with new idea on physics and to maximize the performance of beyond the standard model. To reach the new physics searches,”remarked Launch of IPMU this goal, it is necessary to understand Nojiri. The University of Tokyo’s newly phenomena in the standard model: founded Institute for the Physics and deep theoretical understanding of the Mathematics of the Universe (IPMU) , standard model, and thus processes was launched on October 1, 2007. and responses involved in the LHC IPMU has been approved as one of the experiments, is essential to identify World Premier International Research effects of the new physics in the Center Initiatives (WPI) of the Ministry experiments. of Education, Culture, Sports, Science The following invited speakers with a and Technology (MEXT). IPMU is an range of expertise were invited. -
Shamit Kachru Professor of Physics and Director, Stanford Institute for Theoretical Physics
Shamit Kachru Professor of Physics and Director, Stanford Institute for Theoretical Physics CONTACT INFORMATION • Administrative Contact Dan Moreau Email [email protected] Bio BIO Starting fall of 2021, I am winding down a term as chair of physics and then taking an extended sabbatical/leave. My focus during this period will be on updating my background and competence in rapidly growing new areas of interest including machine learning and its application to problems involving large datasets. My recent research interests have included mathematical and computational studies of evolutionary dynamics; field theoretic condensed matter physics, including study of non-Fermi liquids and fracton phases; and mathematical aspects of string theory. I would characterize my research programs in these three areas as being in the fledgling stage, relatively recently established, and well developed, respectively. It is hard to know what the future holds, but you can get some idea of the kinds of things I work on by looking at my past. Highlights of my past research include: - The discovery of string dualities with 4d N=2 supersymmetry, and their use to find exact solutions of gauge theories (with Cumrun Vafa) - The construction of the first examples of AdS/CFT duality with reduced supersymmetry (with Eva Silverstein) - Foundational papers on string compactification in the presence of background fluxes (with Steve Giddings and Joe Polchinski) - Basic models of cosmic acceleration in string theory (with Renata Kallosh, Andrei Linde, and Sandip Trivedi) -
A Proof of Price's Law for the Collapse of a Self-Gravitating Scalar Field
A proof of Price’s law for the collapse of a self-gravitating scalar field Mihalis Dafermos∗and Igor Rodnianski† October 23, 2018 Abstract A well-known open problem in general relativity, dating back to 1972, has been to prove Price’s law for an appropriate model of gravitational collapse. This law postulates inverse-power decay rates for the gravita- tional radiation flux on the event horizon and null infinity with respect to appropriately normalized advanced and retarded time coordinates. It is intimately related both to astrophysical observations of black holes and to the fate of observers who dare cross the event horizon. In this paper, we prove a well-defined (upper bound) formulation of Price’s law for the collapse of a self-gravitating scalar field with spherically symmetric initial data. We also allow the presence of an additional gravitationally coupled Maxwell field. Our results are obtained by a new mathematical technique for understanding the long-time behavior of large data solutions to the resulting coupled non-linear hyperbolic system of p.d.e.’s in 2 indepen- dent variables. The technique is based on the interaction of the conformal geometry, the celebrated red-shift effect, and local energy conservation; we feel it may be relevant for the problem of non-linear stability of the Kerr solution. When combined with previous work of the first author concerning the internal structure of charged black holes, which assumed the validity of Price’s law, our results can be applied to the strong cos- arXiv:gr-qc/0309115v3 9 Nov 2004 mic censorship conjecture for the Einstein-Maxwell-real scalar field system with complete spacelike asymptotically flat spherically symmetric initial data.