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Families of Picard Modular Forms and an Application to the Bloch-Kato Conjecture
Families of Picard modular forms and an application to the Bloch-Kato conjecture. Valentin Hernandez Abstract In this article we construct a p-adic three dimensional Eigenvariety for the group U(2,1)(E), where E is a quadratic imaginary field and p is inert in E. The Eigenvariety parametrizes Hecke eigensystems on the space of overconvergent, locally analytic, cuspidal Picard mod- ular forms of finite slope. The method generalized the one developed in Andreatta-Iovita- Pilloni by interpolating the coherent automorphic sheaves when the ordinary locus is empty. As an application of this construction, we reprove a particular case of the Bloch-Kato con- jecture for some Galois characters of E, extending the results of Bellaiche-Chenevier to the case of a positive sign. Contents 1 Introduction 2 2 Shimura datum 6 2.1 Globaldatum ................................... 6 2.2 Complex Picard modular forms and automorphic forms . ....... 7 2.3 Localgroups.................................... 10 3 Weight space 10 4 Induction 11 5 Hasse Invariants and the canonical subgroups 13 5.1 Classical modular sheaves and geometric modular forms . 14 5.2 Localconstructions .............................. 15 arXiv:1711.03196v2 [math.NT] 15 Mar 2019 6 Construction of torsors 17 6.1 Hodge-Tatemapandimagesheaves . 17 6.2 Thetorsors..................................... 19 7 The Picard surface and overconvergent automorphic sheaves 21 7.1 Constructingautomorphicsheaves. 21 7.2 Changingtheanalyticradius . 23 7.3 Classical and Overconvergent forms in rigid fiber. 24 8 Hecke Operators, Classicity 26 8.1 Hecke operators outside p ............................ 27 8.2 Hecke operator at p ................................ 28 8.3 Remarksontheoperatorsonthesplitcase . 32 8.4 Classicityresults................................ 32 2010 Mathematics Subject Classification 11G18, 11F33, 14K10 (primary), 11F55, 11G40, 14L05, 14G35, 14G22 (secondary). -
Asian Nobel Prize' for Mapping the Universe 27 May 2010
Scientists win 'Asian Nobel Prize' for mapping the universe 27 May 2010 Three US scientists whose work helped map the category. universe are among the recipients of the one- million-US-dollar Shaw Prize, known as the "Asian (c) 2010 AFP Nobel," the competition's organisers said Thursday. Princeton University professors Lyman Page and David Spergel and Charles Bennett of Johns Hopkins University, won the award for an experiment that helped to determine the "geometry, age and composition of the universe to unprecedented precision." The trio will share the Shaw Prize's award for astronomy, with one-million-US-dollar prizes also awarded in the categories for mathematical sciences and life sciences and medicine. The University of California's David Julius won the award for life sciences and medicine for his "seminal discoveries" of how the skin senses pain and temperature, the organisers' statement said. "(Julius's) work has provided insights into fundamental mechanisms underlying the sense of touch as well as knowledge that opens the door to rational drug design for the treatment of chronic pain," the statement said. Princeton's Jean Bourgain won an award for his "profound work" in mathematical sciences, it said. The Shaw Prize, funded by Hong Kong film producer and philanthropist Run Run Shaw and first awarded in 2004, honours exceptional contributions "to the advancement of civilization and the well-being of humankind." The awards will be presented at a ceremony in Hong Kong on September 28. Last year, two scientists whose work challenged the assumption that obesity is caused by a lack of will power won the life sciences and medicine 1 / 2 APA citation: Scientists win 'Asian Nobel Prize' for mapping the universe (2010, May 27) retrieved 27 September 2021 from https://phys.org/news/2010-05-scientists-asian-nobel-prize-universe.html This document is subject to copyright. -
Professor Peter Goldreich Member of the Board of Adjudicators Chairman of the Selection Committee for the Prize in Astronomy
The Shaw Prize The Shaw Prize is an international award to honour individuals who are currently active in their respective fields and who have recently achieved distinguished and significant advances, who have made outstanding contributions in academic and scientific research or applications, or who in other domains have achieved excellence. The award is dedicated to furthering societal progress, enhancing quality of life, and enriching humanity’s spiritual civilization. Preference is to be given to individuals whose significant work was recently achieved and who are currently active in their respective fields. Founder's Biographical Note The Shaw Prize was established under the auspices of Mr Run Run Shaw. Mr Shaw, born in China in 1907, was a native of Ningbo County, Zhejiang Province. He joined his brother’s film company in China in the 1920s. During the 1950s he founded the film company Shaw Brothers (HK) Limited in Hong Kong. He was one of the founding members of Television Broadcasts Limited launched in Hong Kong in 1967. Mr Shaw also founded two charities, The Shaw Foundation Hong Kong and The Sir Run Run Shaw Charitable Trust, both dedicated to the promotion of education, scientific and technological research, medical and welfare services, and culture and the arts. ~ 1 ~ Message from the Chief Executive I warmly congratulate the six Shaw Laureates of 2014. Established in 2002 under the auspices of Mr Run Run Shaw, the Shaw Prize is a highly prestigious recognition of the role that scientists play in shaping the development of a modern world. Since the first award in 2004, 54 leading international scientists have been honoured for their ground-breaking discoveries which have expanded the frontiers of human knowledge and made significant contributions to humankind. -
David Spergel Is the Director of the Center for Computational Astrophysics and the Charles Young Professor of Astronomy at Princeton University
David Spergel is the director of the Center for Computational Astrophysics and the Charles Young Professor of Astronomy at Princeton University. He is the former chair of the Space Studies Board. Using microwave background observations from the Wilkinson Microwave Anisotropy Probe (WMAP) and the Atacama Cosmology Telescope, Spergel has measured the age, shape and composition of the universe. These observations have played a significant role in establishing the standard model of cosmology. He is one of the leaders of the Simons Observatory, which will include a planned millimeter-wave telescope that will allow us to take the next step in studying the microwave sky and probing the history of the universe. Spergel is currently co-chair of the Wide Field Infrared Survey Telescope (WFIRST) science team. WFIRST will study the nature of dark energy, complete the demographic survey of extrasolar planets, characterize the atmospheres of nearby planets and survey the universe with more than 100 times the field of view of the Hubble Space Telescope. Spergel has played a significant role in designing the coronagraph and in shaping the overall mission. Since completing my Ph.D. work, Spergel has been interested in using laboratory experiments and astronomical observations to probe the nature of dark matter and look for new physics. Recently, Spergel has been active in the exploration of data from the Gaia satellite and observations made by Subaru’s Hyper Suprime-Cam. Spergel serves as co-chair of the Global Coordination of Ground and Space Astrophysics working group of the International Astronomical Union. At Princeton, Spergel was department chair for a decade. -
277 — 18 January 2016 Editor: Bo Reipurth ([email protected]) List of Contents
THE STAR FORMATION NEWSLETTER An electronic publication dedicated to early stellar/planetary evolution and molecular clouds No. 277 — 18 January 2016 Editor: Bo Reipurth ([email protected]) List of Contents The Star Formation Newsletter Interview ...................................... 3 Abstracts of Newly Accepted Papers ........... 5 Editor: Bo Reipurth [email protected] Abstracts of Newly Accepted Major Reviews . 30 Technical Editor: Eli Bressert Dissertation Abstracts ........................ 31 [email protected] New Jobs ..................................... 32 Technical Assistant: Hsi-Wei Yen Meetings ..................................... 33 [email protected] Summary of Upcoming Meetings ............. 36 Editorial Board Joao Alves Alan Boss Jerome Bouvier Cover Picture Lee Hartmann Thomas Henning The Rosette Nebula is a large HII region in Mono- Paul Ho ceros at a distance of about 1.6 - 1.7 kpc. It is Jes Jorgensen illuminated by the OB cluster NGC 2244, which Charles J. Lada contains seven O-stars, dominated by the O4V star Thijs Kouwenhoven HD 46223. The northwestern edge of the HII region Michael R. Meyer contains a large complex of globules and elephant Ralph Pudritz trunks. Luis Felipe Rodr´ıguez Ewine van Dishoeck Image courtesy Don Goldman http://astrodonimaging.com Hans Zinnecker ( ). The Star Formation Newsletter is a vehicle for fast distribution of information of interest for as- tronomers working on star and planet formation and molecular clouds. You can submit material for the following sections: Abstracts of recently Submitting your abstracts accepted papers (only for papers sent to refereed journals), Abstracts of recently accepted major re- Latex macros for submitting abstracts views (not standard conference contributions), Dis- and dissertation abstracts (by e-mail to sertation Abstracts (presenting abstracts of new [email protected]) are appended to Ph.D dissertations), Meetings (announcing meet- each Call for Abstracts. -
Order-Of-Magnitude Physics: Understanding the World with Dimensional Analysis, Educated Guesswork, and White Lies Peter Goldreic
Order-of-Magnitude Physics: Understanding the World with Dimensional Analysis, Educated Guesswork, and White Lies Peter Goldreich, California Institute of Technology Sanjoy Mahajan, University of Cambridge Sterl Phinney, California Institute of Technology Draft of 1 August 1999 c 1999 Send comments to [email protected] ii Contents 1 Wetting Your Feet 1 1.1 Warmup problems 1 1.2 Scaling analyses 13 1.3 What you have learned 21 2 Dimensional Analysis 23 2.1 Newton’s law 23 2.2 Pendula 27 2.3 Drag in fluids 31 2.4 What you have learned 41 3 Materials I 43 3.1 Sizes 43 3.2 Energies 51 3.3 Elastic properties 53 3.4 Application to white dwarfs 58 3.5 What you have learned 62 4 Materials II 63 4.1 Thermal expansion 63 4.2 Phase changes 65 4.3 Specific heat 73 4.4 Thermal diffusivity of liquids and solids 77 4.5 Diffusivity and viscosity of gases 79 4.6 Thermal conductivity 80 4.7 What you have learned 83 5 Waves 85 5.1 Dispersion relations 85 5.2 Deep water 88 5.3 Shallow water 106 5.4 Combining deep- and shallow-water gravity waves 108 5.5 Combining deep- and shallow-water ripples 108 5.6 Combining all the analyses 109 5.7 What we did 109 Bibliography 110 1 1 Wetting Your Feet Most technical education emphasizes exact answers. If you are a physicist, you solve for the energy levels of the hydrogen atom to six decimal places. If you are a chemist, you measure reaction rates and concentrations to two or three decimal places. -
MATTERS of GRAVITY Contents Editor
MATTERS OF GRAVITY The newsletter of the Topical Group on Gravitation of the American Physical Society Number 17 Spring 2001 Contents APS TGG News: APS Prize on gravitation, by Clifford Will .................. 3 TGG Elections, by David Garfinkle ...................... 3 We hear that, by Jorge Pullin ......................... 3 Research Briefs: Experimental Unruh Radiation?, by Matt Visser ............... 4 Why is the Universe accelerating?, by Beverly Berger ............ 6 The Lazarus Project, by Richard Price .................... 9 LIGO locks its first detector!, by Stan Whitcomb ............... 12 Progress on the nonlinear r-mode problem, by Keith Lockitch ........ 13 Conference Reports Analog Models of General Relativity, by Matt Visser ............. 17 Astrophysical Sources of Gravitational radiation, by Joan Centrella ..... 19 Numerical relativity at the 20th Texas meeting, by Pablo Laguna ...... 21 Editor Jorge Pullin Center for Gravitational Physics and Geometry The Pennsylvania State University University Park, PA 16802-6300 Fax: (814)863-9608 Phone (814)863-9597 Internet: [email protected] WWW: http://www.phys.psu.edu/~pullin ISSN: 1527-3431 1 Editorial Not much to report here. If you are burning to have Matters of Gravity with you all the time, the newsletter is now available for Palm Pilots, Palm PC's and web-enabled cell phones as an Avantgo channel. Check out http://www.avantgo.com under technology science. The next newsletter is due September 1st. If everything goes well this newsletter should! be available in the gr-qc Los Alamos archives (http://xxx.lanl.gov) under number gr-qc/yymmnnn. To retrieve it send email to [email protected] with Subject: get yymmnnn (numbers 2-16 are also available in gr-qc). -
Arxiv:1111.3682V1 [Astro-Ph.EP] 15 Nov 2011 Ant Planets, As Well As Their Dynamical Architecture (I.E
Draft version November 17, 2011 Preprint typeset using LATEX style emulateapj v. 11/10/09 INSTABILITY-DRIVEN DYNAMICAL EVOLUTION MODEL OF A PRIMORDIALLY 5 PLANET OUTER SOLAR SYSTEM Konstantin Batygin1, Michael E. Brown1 & Hayden Betts2 1Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125 and 2Polytechnic School, Pasadena, CA 91106 Draft version November 17, 2011 ABSTRACT Over the last decade, evidence has mounted that the solar system's observed state can be favorably reproduced in the context of an instability-driven dynamical evolution model, such as the \Nice" model. To date, all successful realizations of instability models have concentrated on evolving the four giant planets onto their current orbits from a more compact configuration. Simultaneously, the possibility of forming and ejecting additional planets has been discussed, but never successfully implemented. Here we show that a large array of 5-planet (2 gas giants + 3 ice giants) multi-resonant initial states can lead to an adequate formation of the outer solar system, featuring an ejection of an ice giant during a phase of instability. Particularly, our simulations demonstrate that the eigenmodes which characterize the outer solar system's secular dynamics can be closely matched with a 5-planet model. Furthermore, provided that the ejection timescale of the extra planet is short, orbital excitation of a primordial cold classical Kuiper belt can also be avoided in this scenario. Thus the solar system is one of many possible outcomes of dynamical relaxation and can originate from a wide variety of initial states. This deems the construction of a unique model of solar system's early dynamical evolution impossible. -
Formation of Massive Stars and Black Holes in Self-Gravitating AGN Discs
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 1 November 2018 (MN LATEX style file v1.4) Formation of massive stars and black holes in self-gravitating AGN discs, and gravitational waves in LISA band. Yuri Levin1,2 (1)601 Campbell Hall, University of California, Berkeley, California, 94720 (2) Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St. George Street, Toronto, ON M5S 3H8, Canada printed 1 November 2018 ABSTRACT We propose a scenario in which massive stars form at the outer edges of an AGN accretion disc. We analyze the dynamics of a disc forming around a supermassive black hole, in which the angular momentum is transported by turbulence induced by the disc’s self-gravity. We find that once the surface density of the disc exceeds a critical value, the disc fragments into dense clumps. We argue that the clumps accrete material from the remaining disc and merge into larger clumps; the upper mass of a merged clump is a few tens to a few hundreds of solar mass. The biggest clumps collapse and form massive stars, which produce few-tens-solar-mass black holes at the end of their evolution. We construct a model of the AGN disc which includes extra heat sources from the embedded black holes. If the embedded black holes can accrete at the Bondi rate, then the feedback from accretion onto the embedded black holes may stabilize the AGN disc against the Toomre instability for an interesting range of the model parameters. By contrast, if the rate of accretion onto the embedded holes is below the Eddington limit, then the extra heating is insufficient to stabilize the disc. -
08-20-PPC.Pdf
WELCOME TO THE PPC 2018: XII INTERNATIONAL CONFERENCE ON INTERCONNECTIONS BETWEEN PARTICLE PHYSICS AND COSMOLOGY August 20, 2018 2 / 9 Conference scientific programme A venue to discuss particle physics, cosmology and astrophysics: 1 Gravitational waves: Monday August 20 – 24, 2018, Zurich, Switzerland 2 Early Universe cosmology: Monday PPC 2018 XIIth International Workshop on the Interconnection between Particle Physics and Cosmology 3 Late Universe cosmology: Monday and Tuesday The objectives of PPC 2018 are to analyze the connection between dark matter and particle physics models, discuss the connections among dark matter, grand unification models and recent neutrino results, explore predictions for ongoing and forthcoming experiments, and to provide a stimulating venue for exchange of scientific ideas among experts in these areas. 4 Low energy precision experiments: Monday International Program Advisory Committee Ben Allanach (Cambridge) John Ellis (King’s College London/CERN) Vernon Barger (Wisconsin) V.A. Bednyakov (JINR) Wim de Boer (Karlsruhe) 5 Dark matter: Tuesday and Thursday Joel Butler (FNAL/CERN) Tiziano Camporesi (CERN) Johnathan Ellis (CERN) JoAnne Hewett (SLAC) Ian Hinchliffe (LBL) Fabio Iocco (ICTP-SAIFR & IFT-UNESP) Karl Jakobs (U. Freiburg) Gordon Kane (Michigan) 6 Neutrinos: Tuesday Dmitri I. Kazakov (JINR, Dubna) Robert Kirshner (Harvard) Tomio Kobayashi (Tokyo) Pran Nath (NEU) Mihoko Nojiri (KEK) Frank Paige (BNL) Saul Perlmutter (LBNL) Michael Peskin (SLAC) 7 Collider physics: Wednesday and Thursday Adam Riess (Johns -
Annual Report 2010 Report Annual IPMU ANNUAL REPORT 2010 April 2010 April – March 2011March
IPMU April 2010–March 2011 Annual Report 2010 IPMU ANNUAL REPORT 2010 April 2010 – March 2011 World Premier International Institute for the Physics and Mathematics of the Universe (IPMU) Research Center Initiative Todai Institutes for Advanced Study Todai Institutes for Advanced Study The University of Tokyo 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583, Japan TEL: +81-4-7136-4940 FAX: +81-4-7136-4941 http://www.ipmu.jp/ History (April 2010–March 2011) April • Workshop “Recent advances in mathematics at IPMU II” • Press Release “Shape of dark matter distribution” • Mini-Workshop “Cosmic Dust” May • Shaw Prize to David Spergel • Press Release “Discovery of the most distant cluster of galaxies” • Press Release “An unusual supernova may be a missing link in stellar evolution” June • CL J2010: From Massive Galaxy Formation to Dark Energy • Press Conference “Study of type Ia supernovae strengthens the case for the dark energy” July • Institut d’Astrophysique de Paris Medal (France) to Ken’ichi Nomoto • IPMU Day of Extra-galactic Astrophysics Seminars: Chemical Evolution August • Workshop “Galaxy and cosmology with Thirty Meter Telescope (TMT)” September • Subaru Future Instrumentation Workshop • Horiba International Conference COSMO/CosPA October • The 3rd Anniversary of IPMU, All Hands Meeting and Reception • Focus Week “String Cosmology” • Nishinomiya-Yukawa Memorial Prize to Eiichiro Komatsu • Workshop “Evolution of massive galaxies and their AGNs with the SDSS-III/BOSS survey” • Open Campus Day: Public lecture, mini-lecture and exhibits November -
CV Background
Steven Soter CV 2013 Research Associate, Department of Astrophysics, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024. Visiting Professor, Environmental Studies Program, New York University, 285 Mercer Street, 9th Floor, New York, NY 10003, and Email: <[email protected]>. Tel: 212-769-5230. RECENT ACTIVITIES Research in astronomy and geoarchaeology. Teaching at NYU: courses on Scientific Thinking and Speculation, Geology and Antiquity in the Mediterranean, Life in the Universe, Climate Change, and Energy and Environment. BACKGROUND AND EDUCATION Born in Los Angeles, California, May 1943 BSc in Astronomy/Physics, 1965 University of California at Los Angeles (Advisors: George Abell and Peter Goldreich) PhD in Astronomy, 1971 Cornell University, Ithaca, New York (Advisors: Thomas Gold, Carl Sagan, Joseph Burns) PREVIOUS POSITIONS 1964-66 Research Assistant, Radio Astronomy Project, Aerospace Corporation, El Segundo, California 1966-71 Research Assistant, Center for Radiophysics and 1973-79 Space Research, Cornell University, Ithaca, N.Y. 1971-73 Postdoctoral Fellow, Miller Institute for Basic Research in Science, UC Berkeley 1973-79 Assistant Editor, ICARUS: International Journal of Solar System Studies (Carl Sagan, editor) 1977-80 Co-Writer and Head of Research, COSMOS Television Series, KCET/Los Angeles 1980-87 Senior Research Associate, Center for Radiophyscs and Space Research, Cornell University 1988-97 Special Assistant to the Director, National Air and Space Museum, Smithsonian Institution, Washington, DC 1997-03 Scientist, Hayden Planetarium American Museum of Natural History, New York 2004-13 Research Associate, Department of Astrophysics, American Museum of Natural History, New York 2005-07 Scientist-in-Residence, Center for Ancient Studies, New York University, New York 2008-12 Visiting Professor, Environmental Studies Program, New York University, New York .