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Boletín De La RSME
Boletín de la RSME Número 297, 16 de enero de 2012 Sumario Noticias de la RSME Noticias de la RSME Encuentro Conjunto RSME-SMM. Antonio Campillo. Torremolinos, Málaga, 17-20 de enero El programa científico consta de veinticuatro • Encuentro Conjunto RSME- La Real Sociedad Matemática Española y la sesiones especiales, ocho conferencias ple- SMM. Torremolinos, Málaga, Sociedad Matemática Mexicana celebran el narias y la conferencia de clausura del profe- 17-20 de enero Segundo Encuentro Conjunto RSME-SMM en sor Federico Mayor Zaragoza con el título preciso “La comunidad científica ante los de- • Noticias del CIMPA el Hotel Meliá Costa del Sol de Torremolinos (Málaga) los próximos días 17, 18, 19 y 20 de safíos presentes”. Como en la primera edi- • Acuerdo entre cuatro insti- enero. El Primer Encuentro Conjunto se ce- ción, el congreso ha programado alrededor tuciones para la creación del lebró en Oaxaca en julio de 2009 y la serie de doscientas conferencias invitadas, la mitad IEMath. Documento de In- continuará cada tres años a partir de 2014, de las cuales corresponden a la parte mexi- cana y la otra mitad a la española. vestigación de la RSME año en el que está prevista la tercera edición en México. El comité organizador está presi- Las conferencias plenarias están a cargo de • Ampliación del orden del dido por Daniel Girela, e integrado por José Samuel Gitler, José Luis Alías, José María día de la Junta General Ordi- Luis Flores, Cristóbal González, Francisco Pérez Izquierdo, Jorge Velasco, María Emilia naria de la RSME Javier Martín Reyes, María Lina Martínez, Caballero, Javier Fernández de Bobadilla, Francisco José Palma, José Ángel Peláez y • Noticia de la COSCE: Nue- Xavier Gómez-Mont y Eulalia Nulart. -
Lecture Notes in Mathematics
Lecture Notes in Mathematics Edited by A. Oold and B. Eckmann 1185 Group Theory, Beijing 1984 Proceedings of an International Symposium held in Beijing, Aug. 27-Sep. 8, 1984 Edited by Tuan Hsio-Fu Springer-Verlag Berlin Heidelberg New York Tokyo Editor TUAN Hsio-Fu Department of Mathematics, Peking University Beijing, The People's Republic of China Mathematics Subject Classification (1980): 05-xx, 12F-xx, 14Kxx, 17Bxx, 20-xx ISBN 3-540-16456-1 Springer-Verlag Berlin Heidelberg New York Tokyo ISBN 0-387-16456-1 Springer-Verlag New York Heidelberg Berlin Tokyo This work is subject to copyright. All rights are reserved, whether the whole or part of the material is concerned, specifically those of translation, reprinting, re-use of illustrations, broadcasting, reproduction by photocopying machine or similar means, and storage in data banks. Under § 54 of the German Copyright Law where copies are made for other than private use, a fee is payable to "Verwertungsgesellschaft Wort", Munich. © by Springer-Verlag Berlin Heidelberg 1986 Printed in Germany Printing and binding: Beltz Offsetdruck, Hemsbach/Bergstr. 2146/3140-543210 PREFACE From August 27 to September 8, 1984 there was held in Peking Uni• versity, Beijing an International Symposium on Group Theory. As well said by Hermann Wey1: "Symmetry is a vast subject signi• ficant in art and nature. Whenever you have to do with a structure endowed entity, try to determine the group of those transformations which leave all structural relations undisturbed." This passage underlies that the group concept is one of the most fundamental and most important in modern mathematics and its applications. -
Nima Arkani-Hamed, Juan Maldacena, Nathan Both Particle Physicists and Astrophysicists, We Are in an Ideal Seiberg, and Edward Witten
THE I NSTITUTE L E T T E R INSTITUTE FOR ADVANCED STUDY PRINCETON, NEW JERSEY · SUMMER 2008 PROBING THE DARK SIDE OF THE UNIVERSE ne of The remarkable dis - erTies of dark maTTer, and a Ocoveries in asTrophysics has more precise accounTing of The been The recogniTion ThaT The composiTion of The universe, maTerial we see and are familiar The Two fields of asTrophysics wiTh, which makes up The earTh, (The physics of The very large) The sun, The sTars, and everyday and parTicle physics (The objecTs, such as a Table, is only a physics of The very small) are small fracTion of all of The maTTer each providing some of The in The universe. The resT is dark mosT imporTanT new experi - maTTer, possibly a new form of menTal daTa and TheoreTical elemenTary parTicle ThaT does concepTs for The oTher. Re- noT emiT or absorb lighT, and can search aT The InsTiTuTe for only be deTecTed from iTs gravi - Advanced STudy has played a These three images created by Member Douglas Rudd show the various matter components in a simulation encompassing a volume 86 TaTional effecTs. Megaparsec on a side (for reference, the distance between the Milky Way and its nearest neighbor is 0.75 Mpc). The three compo - significanT role in This develop - In The lasT decade, asTro - nents are dark matter (blue), gas (green), and stars (orange). The stars form in galaxies which lie at the intersection of filaments as menT. The laTe InsTiTuTe Pro - nomical observaTions of several seen in the dark matter and gas profiles. -
Fundamental Theorems in Mathematics
SOME FUNDAMENTAL THEOREMS IN MATHEMATICS OLIVER KNILL Abstract. An expository hitchhikers guide to some theorems in mathematics. Criteria for the current list of 243 theorems are whether the result can be formulated elegantly, whether it is beautiful or useful and whether it could serve as a guide [6] without leading to panic. The order is not a ranking but ordered along a time-line when things were writ- ten down. Since [556] stated “a mathematical theorem only becomes beautiful if presented as a crown jewel within a context" we try sometimes to give some context. Of course, any such list of theorems is a matter of personal preferences, taste and limitations. The num- ber of theorems is arbitrary, the initial obvious goal was 42 but that number got eventually surpassed as it is hard to stop, once started. As a compensation, there are 42 “tweetable" theorems with included proofs. More comments on the choice of the theorems is included in an epilogue. For literature on general mathematics, see [193, 189, 29, 235, 254, 619, 412, 138], for history [217, 625, 376, 73, 46, 208, 379, 365, 690, 113, 618, 79, 259, 341], for popular, beautiful or elegant things [12, 529, 201, 182, 17, 672, 673, 44, 204, 190, 245, 446, 616, 303, 201, 2, 127, 146, 128, 502, 261, 172]. For comprehensive overviews in large parts of math- ematics, [74, 165, 166, 51, 593] or predictions on developments [47]. For reflections about mathematics in general [145, 455, 45, 306, 439, 99, 561]. Encyclopedic source examples are [188, 705, 670, 102, 192, 152, 221, 191, 111, 635]. -
UT Austin Professor, Luis Caffarelli, Wins Prestigious Wolf Prize Porto Students Conduct Exploratory Visits
JANUARY//2012 NUMBER//41 UT Austin Professor, Luis Caffarelli, wins prestigious Wolf Prize Luis Caffarelli, a mathematician, Caffarelli’s research interests include Professor at the Institute for Compu- nonlinear analysis, partial differential tational Engineering and Sciences equations and their applications, (ICES) at the University of Texas at calculus of variations and optimiza- Austin and Director of CoLab tion. The ICES Professor is also widely Mathematics Program, has been recognized as the world’s leading named a winner of Israel’s prestigious specialist in free-boundary problems Wolf Prize, in the mathematics for nonlinear partial differential category. equations. This prize, which consists of a cer- Each year this prize is awarded to tificate and a monetary award of specialists in the fields of agriculture, $100,000, “is further evidence of chemistry, mathematics, physics Luis’ huge impact”, according to and the arts. Caffarelli will share the Alan Reid (Chair of the Department 2012 mathematics prize with of Mathematics). “I feel deeply Michael Aschbacher, a professor at honored”, states Caffarelli, who joins the California Institute of Technology. the UT Austin professors John Tate (Mathematics, 2002) and Allen Bard Link for Institute for Computational UT Austin Professor, Luis Caffarelli (Chemistry, 2008) as a Wolf Prize Engineering and Sciences: winner. http://www.ices.utexas.edu/ Porto Students Conduct Exploratory Visits UT Austin welcomed several visitors at the end of the Fall animation. Bastos felt he benefited greatly from the visit, 2011 semester, including Digital Media doctoral students commenting, “The time I spent in Austin and in College Pedro Bastos, Rui Dias, Filipe Lopes, and George Siorios of Station was everything I expected and more. -
On the Stability of the Gliese 876 System of Planets and the Importance of the Inner Planet
On the Stability of the Gliese 876 System of Planets and the Importance of the Inner Planet By: Ricky Leon Murphy Major Project – HET617 – Computational Astrophysics S2 – 2005 | Supervisor: Professor James Murray Background Image Credits: HIRES Echelleogram: http://exoplanets.org/gl876_web/gl876_tech.html Above: Gliese 876d Artist Rendition: http://exoplanets.org/gl876_web/gl876_graphics.html Abstract: Above: Above: Above: Using the SWIFT simulator code, a 5,000 Changing the mass of the inner body has In addition to mass, the eccentricity of the inner year simulation of the current Gliese 876 resulted in the middle planet to take on a body also severely affects system stability. A third planet with a mass of 0.023 MJ was found orbiting the star Gliese 876. system was performed (Monte Carlo more distant orbit. The eccentricity of this Here the mass of the inner body is the same simulations - to determine the best Cartesian body was very high, so the mass of the inner The initial two body system was found to have a perfect orbital resonance as the stable system (0.023M J ) with a change of 2/1. This paper will demonstrate the orbital stability to maintain this coordinates). The result is a system that is body was not available to ensure system in the orbital eccentricity from 0 to 0.1. None of stable. These parameters will be used for the stability. The mass of the inner body was the planets are able to hold their orbits. ratio is highly dependant on the presence of the small, inner planet. In remaining simulations of Gliese 876. -
A Sketch of the History and State of Automated Deduction
A Sketch of the History and State of Automated Deduction David A. Plaisted October 19, 2015 Introduction • Ed Reingold influenced me to do algorithms research early in my career, and this led to some good work. However, my main research area now is automatic theorem proving, so I will discuss this instead. • This talk will be a survey touching on some aspects of the state of the field of automated deduction at present. The content of the talk will be somewhat more general than the original title indicated; thus the change in title. This talk should be about 20 minutes long. I’m planning to put these notes on the internet soon. There is a lot to cover in 20 minutes, so it is best to leave most questions until the end. Proofs in Computer Science • There is a need for formal proofs in computer science, for example, to prove the correctness of software, or to prove theorems in a theoretical paper. • There is also a need for proofs in other areas such as mathematics. • It can be helpful to have programs that check proofs or even help to find the proofs. 1 Automated Deduction • This talk emphasizes systems that do a lot of proof search on their own, either to find the whole proof automatically or large parts of it, without the user specifying each application of each rule of inference. • There are also systems that permit the user to construct a proof and check that the rules of inference are properly applied. History of Automated Deduction Our current state of knowledge in automated deduction came to us by a long and complicated process of intellectual development. -
Scott Duncan Tremaine
Essay‐Contest 2017/18 Leon Ritterbach, International School Kufstein, 9. Schulstufe, Fremdsprachenerwerb: 5 Jahre Scott Duncan Tremaine Astrophysics is a very interesting field of science. You explore the whole universe, from tiny Asteroids to huge black holes. Every time you solve one of the mind breaking riddles that the universe has to offer, it raises new questions. You can find out how the universe works and how forces like gravity form the universe we know and act on us. Scott Duncan Tremaine is one of the people who were lucky enough to be able to study astrophysics. Today, he is 68 years old and one of the world’s leading astrophysicists. He is a fellow of the Royal Society and a member of the National Academy of Sciences. He made predictions about planetary rings, has written an outstanding book “Galactic Dynamics” and named the Kuiper belt. Scott Tremaine’s research is focused on the dynamics of a wide range of astrophysical systems, including planetary rings, comets, planetary systems, galaxies, and clusters of galaxies (structures that consists of anywhere from hundreds to thousands of galaxies). He is known for his contributions to the theory of Solar Systems, Galactic Dynamics and his prediction of small moons keeping the belts of planets in place. Tremaine is so popular that there is even an asteroid named after him, 3806 Tremaine. (Canada under the stars/ 2007), (Princeton University, Department of astrophysical sciences, 2018), (Perimeter Institute for Theoretical Physics/ 2012), (National Academy of Sciences/ 2002), (The Royal Society/ 1994), (Scott Tremaine ‐ Video Learning ‐ WizScience.com/ 2015), (IAS/ 2018) Tremaine grew up in Toronto. -
Daniel Gorenstein 1923-1992
Daniel Gorenstein 1923-1992 A Biographical Memoir by Michael Aschbacher ©2016 National Academy of Sciences. Any opinions expressed in this memoir are those of the author and do not necessarily reflect the views of the National Academy of Sciences. DANIEL GORENSTEIN January 3, 1923–August 26, 1992 Elected to the NAS, 1987 Daniel Gorenstein was one of the most influential figures in mathematics during the last few decades of the 20th century. In particular, he was a primary architect of the classification of the finite simple groups. During his career Gorenstein received many of the honors that the mathematical community reserves for its highest achievers. He was awarded the Steele Prize for mathemat- New Jersey University of Rutgers, The State of ical exposition by the American Mathematical Society in 1989; he delivered the plenary address at the International Congress of Mathematicians in Helsinki, Finland, in 1978; Photograph courtesy of of Photograph courtesy and he was the Colloquium Lecturer for the American Mathematical Society in 1984. He was also a member of the National Academy of Sciences and of the American By Michael Aschbacher Academy of Arts and Sciences. Gorenstein was the Jacqueline B. Lewis Professor of Mathematics at Rutgers University and the founding director of its Center for Discrete Mathematics and Theoretical Computer Science. He served as chairman of the universi- ty’s mathematics department from 1975 to 1982, and together with his predecessor, Ken Wolfson, he oversaw a dramatic improvement in the quality of mathematics at Rutgers. Born and raised in Boston, Gorenstein attended the Boston Latin School and went on to receive an A.B. -
Physics Today
Physics Today The Dynamical Evidence for Dark Matter Scott Tremaine Citation: Physics Today 45(2), 28 (1992); doi: 10.1063/1.881329 View online: http://dx.doi.org/10.1063/1.881329 View Table of Contents: http://scitation.aip.org/content/aip/magazine/physicstoday/45/2?ver=pdfcov Published by the AIP Publishing This article is copyrighted as indicated in the article. Reuse of AIP content is subject to the terms at: http://scitation.aip.org/termsconditions. Downloaded to IP: 128.112.203.62 On: Mon, 25 Aug 2014 15:15:09 THE DYNAMICAL EVIDENCE FOR DARK MATTER 'The Starry Night/ by Vincent van Gogh. The 1889 oil painting suggests how the night sky might look if all of the mass in the universe were luminous. Observations of galaxy dynamics and modern theories of galaxy formation imply that the visible components of galaxies, composed mostly of stars, lie at the centers of vast halos of dark matter that may be 30 or more times larger than the visible galaxy. In most models of galaxy formation, the halos are comparable in size to the distance between galaxies. The halos form as a result of the gravitational instability of small density fluctuations in the early universe; the star-forming gas collects at the minima of the halo potential wells. Infall of outlying material into existing halos and mergers of small halos with larger ones continue at the present time. If the halos were visible to the naked eye, there would be well over 1000 nearby galaxies with halo diameters larger than the full Moon. -
The Classification of the Finite Simple
http://dx.doi.org/10.1090/surv/040.4 Selected Titles in This Series 68 David A. Cox and Sheldon Katz, Mirror symmetry and algebraic geometry, 1999 67 A. Borel and N. Wallach, Continuous cohomology, discrete subgroups, and representations of reductive groups, Second Edition, 1999 66 Yu. Ilyashenko and Weigu Li, Nonlocal bifurcations, 1999 65 Carl Faith, Rings and things and a fine array of twentieth century associative algebra, 1999 64 Rene A. Carmona and Boris Rozovskii, Editors, Stochastic partial differential equations: Six perspectives, 1999 63 Mark Hovey, Model categories, 1999 62 Vladimir I. Bogachev, Gaussian measures, 1998 61 W. Norrie Everitt and Lawrence Markus, Boundary value problems and symplectic algebra for ordinary differential and quasi-differential operators, 1999 60 Iain Raeburn and Dana P. Williams, Morita equivalence and continuous-trace C*-algebras, 1998 59 Paul Howard and Jean E. Rubin, Consequences of the axiom of choice, 1998 58 Pavel I. Etingof, Igor B. Frenkel, and Alexander A. Kirillov, Jr., Lectures on representation theory and Knizhnik-Zamolodchikov equations, 1998 57 Marc Levine, Mixed motives, 1998 56 Leonid I. Korogodski and Yan S. Soibelman, Algebras of functions on quantum groups: Part I, 1998 55 J. Scott Carter and Masahico Saito, Knotted surfaces and their diagrams, 1998 54 Casper Goffman, Togo Nishiura, and Daniel Waterman, Homeomorphisms in analysis, 1997 53 Andreas Kriegl and Peter W. Michor, The convenient setting of global analysis, 1997 52 V. A. Kozlov, V. G. Maz'ya, and J. Rossmann, Elliptic boundary value problems in domains with point singularities, 1997 51 Jan Maly and William P. Ziemer, Fine regularity of solutions of elliptic partial differential equations, 1997 50 Jon Aaronson, An introduction to infinite ergodic theory, 1997 49 R. -
Letter from the Chair Celebrating the Lives of John and Alicia Nash
Spring 2016 Issue 5 Department of Mathematics Princeton University Letter From the Chair Celebrating the Lives of John and Alicia Nash We cannot look back on the past Returning from one of the crowning year without first commenting on achievements of a long and storied the tragic loss of John and Alicia career, John Forbes Nash, Jr. and Nash, who died in a car accident on his wife Alicia were killed in a car their way home from the airport last accident on May 23, 2015, shock- May. They were returning from ing the department, the University, Norway, where John Nash was and making headlines around the awarded the 2015 Abel Prize from world. the Norwegian Academy of Sci- ence and Letters. As a 1994 Nobel Nash came to Princeton as a gradu- Prize winner and a senior research ate student in 1948. His Ph.D. thesis, mathematician in our department “Non-cooperative games” (Annals for many years, Nash maintained a of Mathematics, Vol 54, No. 2, 286- steady presence in Fine Hall, and he 95) became a seminal work in the and Alicia are greatly missed. Their then-fledgling field of game theory, life and work was celebrated during and laid the path for his 1994 Nobel a special event in October. Memorial Prize in Economics. After finishing his Ph.D. in 1950, Nash This has been a very busy and pro- held positions at the Massachusetts ductive year for our department, and Institute of Technology and the In- we have happily hosted conferences stitute for Advanced Study, where 1950s Nash began to suffer from and workshops that have attracted the breadth of his work increased.