Annual Report 2010 Report Annual IPMU ANNUAL REPORT 2010 April 2010 April – March 2011March
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Emerging Issues in Cosmology & Particle Physics
Organizing Committee Patron Principal, Siksha Bhavana, Visva-Bharati Conveners Swarup Kumar Majee & Biswajit Pandey Program Advisory Committee AJIT KEMBHAVI, IUCAA, India AJIT SRIVASTAVA, IOPB , India International Conference on ALAKABHA DATTA, Univ. of Mississippi, USA AMITAVA RAYCHAUDHURI, Univ. Of Calcutta, India AMOL DIGHE, TIFR, India Emerging Issues ASANTHA R. COORAY, UC-Irvine, USA BISWARUP MUKHOPADHYAYA, HRI, India CHENG-WEI CHIANG, NTU, Taiwan in DIEGO PAVON, AUB, Spain EUNG JIN CHUN, KIAS, South Korea GORAN SENJANOVIC, INFN, Italy Cosmology & KAI-FENG CHEN, NTU, Taiwan NABA KUMAR MONDAL, SINP, India NOBUCHIKA OKADA, Univ. of Alabama, USA Particle Physics Organized by QAISAR SHAFI, Univ. of Delaware, USA RABINDRA MOHAPATRA, Univ. of Maryland, USA Department of Physics, RENNAN BARKANA, Tel Aviv University, Israel January 12 -14, 2020 SOMAK RAYCHAUDHURY, IUCAA, India VISVA-BHARATI UNIVERSITY SOMNATH BHARADWAJ, IIT, Kharagpur, India Visva-Bharati University THOMAS BUCHERT, CRAL, Univ. of Lyon, France Santiniketan Email: [email protected] UTPAL SARKAR, IIT, Kharagpur, India Mob.: (+91) 7908272177/ 7602198961 / 8972889271 VOLKER SPRINGEL, MPA, Garching, Germany India Conference webpage: https://indico.cern.ch/event/849205/ Local Organizing Committee Registration Fee Details All faculty members of the Department Indian participants Foreign participants of Physics, Visva-Bharati university Faculty Members INR 4000 USD 200 Ph.D. Students/ Postdocs INR 2000 USD 100 Conference Topics Undergraduate/M.Sc. Students INR 500 USD 75 The registration fee will cover registration kits, refreshments, lunch, dinner, conference dinner and Dark Matter & Dark Energy local transportation. Neutrino Physics Accelerator Physics The main objective of the conference is to provide a common platform to discuss the emerging issues Physics Beyond the Standard Model in cosmology and particle physics, to set out possible future collaborative research works and to nail 21 cm Cosmology down some existing common problems. -
Table of Contents (Print)
PERIODICALS PHYSICAL REVIEW Dä For editorial and subscription correspondence, Postmaster send address changes to: please see inside front cover (ISSN: 1550-7998) APS Subscription Services P.O. Box 41 Annapolis Junction, MD 20701 THIRD SERIES, VOLUME 90, NUMBER 5 CONTENTS D1 SEPTEMBER 2014 RAPID COMMUNICATIONS Measurement of the electric charge of the top quark in tt¯ events (8 pages) ........................................................ 051101(R) V. M. Abazov et al. (D0 Collaboration) BRST-symmetry breaking and Bose-ghost propagator in lattice minimal Landau gauge (5 pages) ............................. 051501(R) Attilio Cucchieri, David Dudal, Tereza Mendes, and Nele Vandersickel ARTICLES pffiffiffi Search for supersymmetry in events with four or more leptons in s ¼ 8 TeV pp collisions with the ATLAS detector (33 pages) ................................................................................................................................. 052001 G. Aad et al. (ATLAS Collaboration) pffiffiffi Low-mass vector-meson production at forward rapidity in p þ p collisions at s ¼ 200 GeV (12 pages) .................. 052002 A. Adare et al. (PHENIX Collaboration) Measurement of Collins asymmetries in inclusive production of charged pion pairs in eþe− annihilation at BABAR (26 pages) 052003 J. P. Lees et al. (BABAR Collaboration) Measurement of the Higgs boson mass from the H → γγ and H → ZZÃ → 4l channels in pp collisions at center-of-mass energies of 7 and 8 TeV with the ATLAS detector (35 pages) ................................................................... 052004 G. Aad et al. (ATLAS Collaboration) pffiffiffi Search for high-mass dilepton resonances in pp collisions at s ¼ 8 TeV with the ATLAS detector (30 pages) .......... 052005 G. Aad et al. (ATLAS Collaboration) Search for low-mass dark matter with CsI(Tl) crystal detectors (6 pages) .......................................................... 052006 H. -
The Cosmos - Before the Big Bang
From issue 2601 of New Scientist magazine, 28 April 2007, page 28-33 The cosmos - before the big bang How did the universe begin? The question is as old as humanity. Sure, we know that something like the big bang happened, but the theory doesn't explain some of the most important bits: why it happened, what the conditions were at the time, and other imponderables. Many cosmologists think our standard picture of how the universe came to be is woefully incomplete or even plain wrong, and they have been dreaming up a host of strange alternatives to explain how we got here. For the first time, they are trying to pin down the initial conditions of the big bang. In particular, they want to solve the long-standing mystery of how the universe could have begun in such a well- ordered state, as fundamental physics implies, when it seems utter chaos should have reigned. Several models have emerged that propose intriguing answers to this question. One says the universe began as a dense sea of black holes. Another says the big bang was sparked by a collision between two membranes floating in higher-dimensional space. Yet another says our universe was originally ripped from a larger entity, and that in turn countless baby universes will be born from the wreckage of ours. Crucially, each scenario makes unique and testable predictions; observations coming online in the next few years should help us to decide which, if any, is correct. Not that modelling the origin of the universe is anything new. -
Relative Mirror Symmetry and Ramifications of a Formula for Gromov-Witten Invariants
Relative Mirror Symmetry and Ramifications of a Formula for Gromov-Witten Invariants Thesis by Michel van Garrel In Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy California Institute of Technology Pasadena, California 2013 (Defended May 21, 2013) ii c 2013 Michel van Garrel All Rights Reserved iii To my parents Curt and Danielle, the source of all virtues that I possess. To my brothers Cl´ement and Philippe, my best and most fun friends. iv Acknowledgements My greatest thanks go to my advisor Professor Tom Graber, whose insights into the workings of algebraic geometry keep astonishing me and whose ideas were of enormous benefit to me during the pursuit of my Ph.D. My special thanks are given to Professor Yongbin Ruan, who initiated the project on relative mirror symmetry and to whom I am grateful many enjoyable discussions. I am grateful that I am able to count on the continuing support of Professor Eva Bayer and Professor James Lewis. Over the past few years I learned a lot from Daniel Pomerleano, who, among others, introduced me to homological mirror symmetry. Mathieu Florence has been a figure of inspiration and motivation ever since he casually introduced me to algebraic geometry. Finally, my thanks go to the innumerable enjoyable math conversations with Roland Abuaf, Dori Bejleri, Adam Ericksen, Anton Geraschenko, Daniel Halpern-Leistner, Hadi Hedayatzadeh, Cl´ement Hongler, Brian Hwang, Khoa Nguyen, Rom Rains, Mark Shoemaker, Zhiyu Tian, Nahid Walji, Tony Wong and Gjergji Zaimi. v Abstract For a toric Del Pezzo surface S, a new instance of mirror symmetry, said relative, is introduced and developed. -
Stringy T3-Fibrations, T-Folds and Mirror Symmetry
Stringy T 3-fibrations, T-folds and Mirror Symmetry Ismail Achmed-Zade Arnold-Sommerfeld-Center Work to appear with D. L¨ust,S. Massai, M.J.D. Hamilton March 13th, 2017 Ismail Achmed-Zade (ASC) Stringy T 3-fibrations and applications March 13th, 2017 1 / 24 Overview 1 String compactifications and dualities T-duality Mirror Symmetry 2 T-folds The case T 2 The case T 3 3 Stringy T 3-bundles The useful T 4 4 Conclusion Recap Open Problems Ismail Achmed-Zade (ASC) Stringy T 3-fibrations and applications March 13th, 2017 2 / 24 Introduction Target space Super string theory lives on a 10-dimensional pseudo-Riemannian manifold, e.g. 4 6 M = R × T with metric η G = µν GT 6 In general we have M = Σµν × X , with Σµν a solution to Einsteins equation. M is a solution to the supergravity equations of motion. Non-geometric backgrounds X need not be a manifold. Exotic backgrounds can lead to non-commutative and non-associative gravity. Ismail Achmed-Zade (ASC) Stringy T 3-fibrations and applications March 13th, 2017 3 / 24 T-duality Example Somtimes different backgrounds yield the same physics IIA IIB 9 1 2 2 ! 9 1 1 2 R × S ; R dt R × S ; R2 dt More generally T-duality for torus compactifications is an O(D; D; Z)-transformation (T D ; G; B; Φ) ! (T^D ; G^; B^; Φ)^ Ismail Achmed-Zade (ASC) Stringy T 3-fibrations and applications March 13th, 2017 4 / 24 Mirror Symmetry Hodge diamond of three-fold X and its mirror X^ 1 1 0 0 0 0 0 h1;1 0 0 h1;2 0 1 h1;2 h1;2 1 ! 1 h1;1 h1;1 1 0 h1;1 0 0 h1;2 0 0 0 0 0 1 1 Mirror Symmetry This operation induces the following symmetry IIA IIB ! X ; g X^; g^ Ismail Achmed-Zade (ASC) Stringy T 3-fibrations and applications March 13th, 2017 5 / 24 Mirror Symmetry is T-duality!? SYZ-conjecture [Strominger, Yau, Zaslow, '96] Consider singular bundles T 3 −! X T^3 −! X^ ! ? ? S3 S3 Apply T-duality along the smooth fibers. -
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. -
Curriculum Vitae Arthur B
CURRICULUM VITAE ARTHUR B. MCDONALD Contact Office Dept. of Physics, Engineering Physics and Astronomy, Queen's University Kingston, Ontario, Canada K7L 3N6 Tel: (613) 533-2702 Fax: (613) 533-6813 Academic Experience Position Institution Year Professor Emeritus Queen’s University 2013 - Present Director Sudbury Neutrino Observatory Collaboration 1989 - Present Gordon and Patricia Gray Chair in Particle Astrophysics Queen’s University 2006 - 2013 University Research Chair Queen’s University 2002 - 2006 Director SNO Institute 1991-2003, 2006 - 2009 Associate Director SNOLAB Institute 2009 - 2013 Professor Queen's University 1989 - 2013 Professor Princeton 1982 - 1989 Sr. Research Officer Atomic Energy of Canada 1980 - 1982 (Chalk River, Ontario) Assoc. Research Officer Chalk River 1975 - 1980 Assist. Research Officer Chalk River 1970 - 1975 Postdoctoral Fellow Chalk River 1969 - 1970 Education: Dalhousie University, Halifax, Nova Scotia - B.Sc. Physics (1964) Dalhousie University, Halifax, Nova Scotia - M.Sc. Physics (1965) California Institute of Technology, Pasadena, CA, USA - Ph.D. Physics (1969) Awards: Governor General's Medal, Dalhousie, 1964 Rutherford Memorial Fellowship, (1969-1970) Fellow of the American Physical Society, 1983 LL.D., honoris causa, Dalhousie, 1997 Fellow of Royal Society of Canada, 1997 Honorary Life Membership at Science North, Sudbury, Ontario, 1997 Killam Research Fellowship, 1998 LL.D., honoris causa, University College of Cape Breton, 1999 D. Sc., honoris causa, Royal Military College, 2001 T.W. Bonner Prize -
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. -
The Minimal Supersymmetric Leptogenesis∗
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server August 3, 1999 IASSNS-HEP-99/69 LBNL-44042 hep-ph/9908223 The Minimal Supersymmetric Leptogenesis∗ Takeo Moroi1 and Hitoshi Murayama2,3 1School of Natural Sciences, Institute for Advanced Study Princeton, New Jersey 08540 2Theoretical Physics Group Ernest Orlando Lawrence Berkeley National Laboratory University of California, Berkeley, California 94720 and 3Department of Physics University of California, Berkeley, California 94720 Abstract We reanalyze the supersymmetric leptogenesis model by one of the ˜ authors (HM) and Yanagida based on L = Hu flat direction in detail. We point out that the appropriate amount of baryon asymmetry can be generated in this model with the neutrino mass matrix consistent with the atmospheric neutrino oscillation and solutions to the solar neutrino problem, preferably the small angle MSW solution. The reheating temperature can be low enough to avoid the cosmological gravitino problem. This model is the minimal one because it does not rely on any new physics beyond supersymmetry and Majorana neutrino masses. ∗This work was supported in part by the U.S. Department of Energy under Con- tracts DE-AC03-76SF00098, in part by the National Science Foundation under grants PHY-95-13835 and PHY-95-14797. TM was also supported by the Marvin L. Goldberger Membership. HM was also supported by Alfred P. Sloan Foundation. 1. Introduction Cosmic baryon asymmetry has been one of the biggest puzzles in mod- ern cosmology. It is hoped to understand it in terms of microscopic physics and evolution of Universe, if the well-known Sakharov’s three conditions are satisfied: (1) existence of baryon-number violation, (2) existence of CP vio- lation, and (3) departure from thermal equilibrium. -
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. -
Dubna, 18 March. Meeting of the Committee of Plenipotentiaries of JINR Member States
Dubna, 18 March. Meeting of the Committee of Plenipotentiaries of JINR Member States Dubna, 21 January 2005. Professor Arthur B. McDonald (left) receives Bruno Pontecorvo Prize-2004 Dubna, 19 February. Meeting of the JINR Finance Committee Dubna, 15 January. The 95th session of the JINR Scientific Council Dubna, 19–20 April. Participants of the meeting of the Programme Advisory Committee for Condensed Matter Physics Dubna, 5–6 April. Meeting of the Programme Advisory Committee for Particle Physics Dubna, 16 April. CERN delegation, headed by CERN Director-General R. Aymar, visits JINR. N. Koulberg, R. Aymar and D. Ellis (first, second and third from right) at the JINR Directorate Minsk, 13 May. Participants of the meeting of the joint expert board on JINR–Belarus projects (from left to right): N. Kazak, V. Katrasev, I. Golutvin, A. Lesnikovich, A. Sissakian, N. Shumeiko, N. Russakovich Beijing (China), 19 August. JINR Director Academician V. Kadyshevsky and Director of the Institute of High Energy Physics (Beijing) Professor Chen Hesheng during the signing of an agreement on JINR–IHEP cooperation Dubna, 15 January. Extraordinary and Plenipotentiary of the South African Republic Mochubela J. Seekoe (second from right) visits JINR Dubna, 5 February. A delegation from Ukraine headed by Plenipotentiary of the Ukrainian government to JINR V. Stognij (second from left) on a visit to JINR Dubna, 10 August. JINR CP Chairman, Plenipotentiary of Belarus to JINR V. Nedilko signs a new edition of the documents that regulate the activities at the Institute Dubna, 17 February. Participants of the 14th meeting of the Joint Steering Committee on BMBF–JINR cooperation Dubna, 26 July. -
Tata Institute of Fundamental Research Prof
Annual Report 1988-89 Tata Institute of Fundamental Research Prof. M. G. K. Menon inaugurating the Pelletron Accelerator Facility at TIFR on December 30, 1988. Dr. S. S. Kapoor, Project Director, Pelletron Accelerator Facility, explaining salient features of \ Ion source to Prof. M. G. K. Menon, Dr. M. R. Srinivasan, and others. Annual Report 1988-89 Contents Council of Management 3 School of Physics 19 Homi Bhabha Centre for Science Education 80 Theoretical Physics l'j Honorary Fellows 3 Theoretical A strophysics 24 Astronomy 2') Basic Dental Research Unit 83 Gravitation 37 A wards and Distinctions 4 Cosmic Ray and Space Physics 38 Experimental High Energy Physics 41 Publications, Colloquia, Lectures, Seminars etc. 85 Introduction 5 Nuclear and Atomic Physics 43 Condensed Matter Physics 52 Chemical Physics 58 Obituaries 118 Faculty 9 Hydrology M Physics of Semi-Conductors and Solid State Electronics 64 Group Committees 10 Molecular Biology o5 Computer Science 71 Administration. Engineering Energy Research 7b and Auxiliary Services 12 Facilities 77 School of Mathematics 13 Library 79 Tata Institute of Fundamental Research Homi Bhabha Road. Colaba. Bombav 400005. India. Edited by J.D. hloor Published by Registrar. Tata Institute of Fundamental Research Homi Bhabha Road, Colaba. Bombay 400 005 Printed bv S.C. Nad'kar at TATA PRESS Limited. Bombay 400 025 Photo Credits Front Cover: Bharat Upadhyay Inside: Bharat Upadhyay & R.A. A chary a Design and Layout by M.M. Vajifdar and J.D. hloor Council of Management Honorary Fellows Shri J.R.D. Tata (Chairman) Prof. H. Alfven Chairman. Tata Sons Limited Prof. S. Chandrasekhar Prof.