Revealing the Hidden Nature of Space and Time Charting The

Total Page:16

File Type:pdf, Size:1020Kb

Revealing the Hidden Nature of Space and Time Charting The PREPUBLICATION COPY SUBJECT TO EDITORIAL CORRECTIONS Revealing the Hidden Nature of Space and Time Charting the Course for Elementary Particle Physics Committee on Elementary Particle Physics in the 21st Century Board on Physics and Astronomy Division on Engineering and Physical Sciences THE NATIONAL ACADEMIES PRESS 500 Fifth Street, N.W. Washington, DC 20001 NOTICE: The project that is the subject of this report was approved by the Governing Board of the National Research Council, whose members are drawn from the councils of the National Academy of Sciences, the National Academy of Engineering, and the Institute of Medicine. The members of the committee responsible for the report were chosen for their special competences and with regard for appropriate balance. This study was supported by Grant No. PHY-0432486 between the National Academy of Sciences and the National Science Foundation and Contract No. DE-FG02-04ER41327 between the National Academy of Sciences and the Department of Energy. Any opinions, findings, conclusions, or recommendations expressed in this publication are those of the author(s) and do not necessarily reflect the views of the organizations or agencies that provided support for the project. International Standard Book Number 0-309-10195-6 (Book) Additional copies of this report are available from the National Academies Press, 500 Fifth Street, N.W., Lockbox 285, Washington, DC 20055; (800) 624-6242 or (202) 334-3313 (in the Washington metropolitan area); Internet, http://www.nap.edu. Cover: Industrial designer Jan-Henrik Anderson, working with particle physicists, portrays the collision of a proton and an anti-proton in the Fermilab Tevatron accelerator. By parameterizing the different properties of subatomic particles with different visual elements (color, number and direction of helical turns, visual weight of solid and void space, and so on), Anderson creates a visual interpretation of the particle physics at work. [Courtesy of J-H. Anderson] Copyright 2006 by the National Academy of Sciences. All rights reserved. Printed in the United States of America The National Academy of Sciences is a private, nonprofit, self-perpetuating society of distinguished scholars engaged in scientific and engineering research, dedicated to the furtherance of science and technology and to their use for the general welfare. Upon the authority of the charter granted to it by the Congress in 1863, the Academy has a mandate that requires it to advise the federal government on scientific and technical matters. Dr. Ralph J. Cicerone is president of the National Academy of Sciences. The National Academy of Engineering was established in 1964, under the charter of the National Academy of Sciences, as a parallel organization of outstanding engineers. It is autonomous in its administration and in the selection of its members, sharing with the National Academy of Sciences the responsibility for advising the federal government. The National Academy of Engineering also sponsors engineering programs aimed at meeting national needs, encourages education and research, and recognizes the superior achievements of engineers. Dr. Wm. A. Wulf is president of the National Academy of Engineering. The Institute of Medicine was established in 1970 by the National Academy of Sciences to secure the services of eminent members of appropriate professions in the examination of policy matters pertaining to the health of the public. The Institute acts under the responsibility given to the National Academy of Sciences by its congressional charter to be an adviser to the federal government and, upon its own initiative, to identify issues of medical care, research, and education. Dr. Harvey V. Fineberg is president of the Institute of Medicine. The National Research Council was organized by the National Academy of Sciences in 1916 to associate the broad community of science and technology with the Academy’s purposes of furthering knowledge and advising the federal government. Functioning in accordance with general policies determined by the Academy, the Council has become the principal operating agency of both the National Academy of Sciences and the National Academy of Engineering in providing services to the government, the public, and the scientific and engineering communities. The Council is administered jointly by both Academies and the Institute of Medicine. Dr. Ralph J. Cicerone and Dr. Wm. A. Wulf are chair and vice chair, respectively, of the National Research Council. www.national-academies.org COMMITTEE ON ELEMENTARY PARTICLE PHYSICS IN THE 21ST CENTURY HAROLD T. SHAPIRO, Princeton University, Chair SALLY DAWSON, Brookhaven National Laboratory, Vice Chair NORMAN R. AUGUSTINE, Lockheed Martin Corporation (retired) JONATHAN A. BAGGER, Johns Hopkins University PHILIP N. BURROWS, Oxford University SANDRA M. FABER, University of California Observatories STUART J. FREEDMAN, University of California at Berkeley JEROME I. FRIEDMAN, Massachusetts Institute of Technology DAVID J. GROSS, Kavli Institute for Theoretical Physics JOSEPH S. HEZIR, EOP Group, Inc. NORBERT HOLTKAMP, Oak Ridge National Laboratory TAKAAKI KAJITA, University of Tokyo NEAL F. LANE, Rice University NIGEL LOCKYER, University of Pennsylvania SIDNEY R. NAGEL, University of Chicago HOMER A. NEAL, University of Michigan J. RITCHIE PATTERSON, Cornell University HELEN QUINN, Stanford Linear Accelerator Center CHARLES V. SHANK, Lawrence Berkeley National Laboratory PAUL STEINHARDT, Princeton University HAROLD E. VARMUS, Memorial Sloan-Kettering Cancer Center EDWARD WITTEN, Institute for Advanced Study Staff DONALD C. SHAPERO, Director TIMOTHY I. MEYER, Senior Program Officer DAVID B. LANG, Research Associate VAN AN, Financial Associate STEVE OLSON, Consultant Editor iv Unedited Prepublication Draft BOARD ON PHYSICS AND ASTRONOMY BURTON RICHTER, Stanford University, Chair ANNEILA L. SARGENT, California Institute of Technology, Vice Chair ELIHU ABRAHAMS, Rutgers University JONATHAN A. BAGGER, Johns Hopkins University RONALD C. DAVIDSON, Princeton University RAYMOND J. FONCK, University of Wisconsin at Madison ANDREA M. GHEZ, University of California at Los Angeles PETER F. GREEN, University of Michigan LAURA H. GREENE, University of Illinois at Urbana-Champaign WICK HAXTON, University of Washington FRANCES HELLMAN, University of California at Berkeley ERICH P. IPPEN, Massachusetts Institute of Technology MARC A. KASTNER, Massachusetts Institute of Technology CHRISTOPHER F. McKEE, University of California at Berkeley JULIA M. PHILLIPS, Sandia National Laboratories WILLIAM PHILLIPS, National Institute of Standards and Technology THOMAS M. THEIS, IBM T.J. Watson Research Center C. MEGAN URRY, Yale University Staff DONALD C. SHAPERO, Director TIMOTHY I. MEYER, Senior Program Officer MICHAEL H. MOLONEY, Senior Program Officer ROBERT L. RIEMER, Senior Program Officer NATALIA J. MELCER, Program Officer BRIAN D. DEWHURST, Senior Program Associate DAVID B. LANG, Research Associate PAMELA A. LEWIS, Program Associate PHILLIP D. LONG, Senior Program Assistant VAN AN, Financial Associate v Preface he principal charge to the Committee on Elementary Particle Physics in the 21st Century was to recommend priorities for the U.S. particle physics program for the next 15 years. T Described in the Executive Summary and more fully presented in the Overview, the committee’s considered response is laid out in detail in the main text of this report, which begins by discussing the scientific challenges in particle physics and conveying the current status of the U.S. program, and then presents the committee’s consensus on the best way to sustain a competitive and globally relevant U.S. particle physics program. Given the charge (see Appendix B), the composition of this committee was something of an experiment for the National Academies. The committee included but went well beyond particle physicists and accelerator scientists to comprise condensed matter physicists, astrophysicists, astronomers, biologists, industrialists, and a variety of experts in public policy, particularly science policy. As a result, a good deal of education was necessary during the course of the study, and those of us who are not particle physicist would like to express our gratitude for the intellectual generosity and patience of the committee’s physicists as they provided us with the level of understanding necessary to proceed with our task. In the same vein, the committee owes a great deal for their assistance to our colleagues at the major particle physics laboratories in the United States (Argonne National Laboratory, Brookhaven National Laboratory, Cornell Laboratory for Elementary Particle Physics, Fermi National Accelerator Laboratory, Lawrence Berkeley National Laboratory, and Stanford Linear Accelerator Center), and to colleagues abroad at the DESY laboratory in Hamburg, the CERN laboratory in Geneva, and the J-PARC and KEK laboratories in Japan. For the non-physicists on the committee, the task was both intellectually exciting and sobering. Simply stated, we were not fully aware of the challenge faced by the U.S. particle physics program in sustaining its tradition of leadership. Given the globalization of particle physics (and with Europe investing twice as much as the United States and Japan investing nearly half of the U.S. annual budget for particle physics), identifying a compelling leadership role for the United States was not simple. Since the unfortunate demise of the Superconducting Super Collider in the early 1990s
Recommended publications
  • 2015 Annual Report
    2015 AMERICAN PHYSICAL SOCIETY ANNUAL TM ADVANCING PHYSICS REPORT TM THE AMERICAN PHYSICAL SOCIETY STRIVES TO Be the leading voice for physics and an authoritative source of physics information for the advancement of physics and the benefit of humanity Collaborate with national scientific societies for the advancement of science, science education, and the science community Cooperate with international physics societies to promote physics, to support physicists worldwide, and to foster international collaboration Have an active, engaged, and diverse membership, and support the activities of its units and members © 2016 American Physical Society During 2015, APS worked to institute the governance objective: “the advancement and diffusion of the knowledge changes approved by the membership in late 2014. In of physics.” APS is fully committed to the principles of OA accordance with the new Constitution & Bylaws, in to the extent that we can continue to support the production February the Board appointed our first Chief Executive of high-quality peer-reviewed journals. For many years APS Officer—Kate Kirby, the former Executive Officer—to has supported “green” OA and we have been fully compliant head the APS. Kate’s major task has been to transition with the 2013 directive from the Office of Science and the management of APS to a CEO model with a Senior Technology Policy that the publications resulting from Management Team. She appointed Mark Doyle as Chief U.S. federally funded research be accessible to the public 12 Information Officer, James Taylor as Chief Operating months after publication. Since APS is a major international Officer, and Matthew Salter as the new Publisher.
    [Show full text]
  • HOPE Meetings Are Held for Excellent Graduate Students and Young Researchers Specially Selected from Countries Around the 9Th Asia-Pacific and Africa Region
    For Overseas Cooperating Institutions Objective HOPE Meetings are held for excellent graduate students and young researchers specially selected from countries around the 9th Asia-Pacific and Africa region. These meetings give an opportunity for the participants to engage in interdisciplinary discussions with Nobel laureates and other distinguished HOPE MEETING scientists pioneering the frontiers of knowledge. They also give the participants, who lodge together over the course of the event, a chance to make friends and form collegial networks with Nobel Laureates with peers from the regions. The title “HOPE Meeting” signifies the promise held for the future roles of young researchers and optimism for creating a bright S&T future within the global community. Date F ebruary 26- ■ Saturday, February 25: Orientation & Registration M arch 2, 2017 ■ Sunday, February 26: Nobel Prize Dialogue Tokyo 2017 Organizer Venue Tokyo , JAPAN Office of the HOPE Meetings, JSPS E-mail [email protected] Tel: +81-3-3263-2414 Fax:+81-3-3234-3700 HOPE MEETINGS with Nobel Laureates Organizing Committee of the HOPE Meetings ■ Chair Makoto Kobayashi <Nobel Laureate in Physics 2008> Honorary Professor Emeritus, High Energy Accelerator Research Organization (KEK) ■ Members Noriko Osumi Mitsuhiko Shionoya Tohoku University The University of Tokyo Takaaki Kajita <Nobel Laureate in Physics 2015> Yousuke Takahama The University of Tokyo Tokushima University Kazuhiro Kosuge Fumio Hanaoka Tohoku University Tsukuba University Program of the HOPE Meeting The program
    [Show full text]
  • Final Report
    Revealing the Hidden Nature of Space and Time: Charting the Course for Elementary Particle Physics Committee on Elementary Particle Physics in the 21st Century, National Research Council ISBN: 0-309-66039-4, 176 pages, 7 x 10, (2006) This free PDF was downloaded from: http://www.nap.edu/catalog/11641.html Visit the National Academies Press online, the authoritative source for all books from the National Academy of Sciences, the National Academy of Engineering, the Institute of Medicine, and the National Research Council: • Download hundreds of free books in PDF • Read thousands of books online, free • Sign up to be notified when new books are published • Purchase printed books • Purchase PDFs • Explore with our innovative research tools Thank you for downloading this free PDF. If you have comments, questions or just want more information about the books published by the National Academies Press, you may contact our customer service department toll-free at 888-624-8373, visit us online, or send an email to [email protected]. This free book plus thousands more books are available at http://www.nap.edu. Copyright © National Academy of Sciences. Permission is granted for this material to be shared for noncommercial, educational purposes, provided that this notice appears on the reproduced materials, the Web address of the online, full authoritative version is retained, and copies are not altered. To disseminate otherwise or to republish requires written permission from the National Academies Press. Revealing the Hidden Nature of Space and Time: Charting the Course for Elementary Particle Physics http://www.nap.edu/catalog/11641.html REVEALING THE HIDDEN NATURE OF SPACE AND TIME Charting the Course for Elementary Particle Physics Committee on Elementary Particle Physics in the 21st Century Board on Physics and Astronomy Division on Engineering and Physical Sciences THE NATIONAL ACADEMIES PRESS Washington, D.C.
    [Show full text]
  • Panel Discussion on the Nobel Prize in Physics 2015 Tommy Ohlsson Motivation for the Nobel Prize in Physics 2015
    KTH ROYAL INSTITUTE OF TECHNOLOGY Panel Discussion on the Nobel Prize in Physics 2015 Tommy Ohlsson Motivation for the Nobel Prize in Physics 2015 The Nobel Prize in Physics 2015 was awarded jointly to Takaaki Kajita and Arthur B. McDonald "for the discovery of neutrino oscillations, which shows that neutrinos have mass" Takaaki Kajita Arthur B. McDonald (Super-Kamiokande) (SNO) Motivation for the Nobel Prize in Physics 2015 The Nobel Prize in Physics 2015 was awarded jointly to Takaaki Kajita and Arthur B. McDonald "for the discovery of neutrino oscillations, which shows that neutrinos have mass" Ed Kearns Takaaki Kajita Arthur B. McDonald Dave Wark (Super-Kamiokande) (Super-Kamiokande) (SNO) (SNO) Super-Kamiokande (in Japan) In June 1998, the Super-Kamiokande collaboration presented its first results of measurements of atmospheric neutrinos that give evidence for neutrino oscillations (i.e. quantum mechanical effects over distances of thousands of kilometers). This result is the first solid evidence for physics beyond the Standard Model of particle physics. The atmospheric neutrino analysis of the Super-Kamiokande collaboration was led by Takaaki Kajita. SNO (in Canada) In April 2002, the SNO collaboration presented the first direct measurement of the total flux of all active boron-8 neutrinos arriving from the Sun, which provided additional evidence for neutrino flavor transitions. The SNO collaboration was led by Art McDonald. ) -1 8 SNO SNO s q q -2 7 ES CC cm 6 6 (10 o 5 µ q SNO 4 qNC 3 qSSM 2 1 0 0123456 6 -2 -1 qe (10 cm s ) Other neutrino oscillation experiments • KamLAND • first results on anti-electron neutrino flux from distant nuclear reactors • demonstrated disappearance of anti-electron neutrinos and showed that the LMA solution is the only remaining solar neu.
    [Show full text]
  • Communications-Mathematics and Applied Mathematics/Download/8110
    A Mathematician's Journey to the Edge of the Universe "The only true wisdom is in knowing you know nothing." ― Socrates Manjunath.R #16/1, 8th Main Road, Shivanagar, Rajajinagar, Bangalore560010, Karnataka, India *Corresponding Author Email: [email protected] *Website: http://www.myw3schools.com/ A Mathematician's Journey to the Edge of the Universe What’s the Ultimate Question? Since the dawn of the history of science from Copernicus (who took the details of Ptolemy, and found a way to look at the same construction from a slightly different perspective and discover that the Earth is not the center of the universe) and Galileo to the present, we (a hoard of talking monkeys who's consciousness is from a collection of connected neurons − hammering away on typewriters and by pure chance eventually ranging the values for the (fundamental) numbers that would allow the development of any form of intelligent life) have gazed at the stars and attempted to chart the heavens and still discovering the fundamental laws of nature often get asked: What is Dark Matter? ... What is Dark Energy? ... What Came Before the Big Bang? ... What's Inside a Black Hole? ... Will the universe continue expanding? Will it just stop or even begin to contract? Are We Alone? Beginning at Stonehenge and ending with the current crisis in String Theory, the story of this eternal question to uncover the mysteries of the universe describes a narrative that includes some of the greatest discoveries of all time and leading personalities, including Aristotle, Johannes Kepler, and Isaac Newton, and the rise to the modern era of Einstein, Eddington, and Hawking.
    [Show full text]
  • Nobel Prize 2015 , Vol
    The Royal Swedish Academy of Sciences has decided to award the Nobel Prize in Physics 2015 to Takaaki Kajita and Arthur B. McDonald “for the discovery of neutrino oscillations, which shows that The Nobel Prize 2015 in Physics neutrinos have mass”. the Nobel Foundation. Nobel the Nobel Prize® and the Nobel Prize® medal design mark are registered trademarks of Only electron neutrinos Atmospheric neutrinos are produced in the Sun. are produced in collisions between Chameleons cosmic rays and the Earth’s atmosphere. of space Takaaki Kajita in Japan and Arthur B. McDonald in Canada were key scientists in two large research groups that discovered that neutrinos change identities, which requires that neutrinos have mass. The discovery has changed our understanding of the innermost workings of matter and may prove crucial to our view of the universe. B The discovery of neutrino identity changes between cosmic radiation and the Earth's A Sudbury Neutrino Observatory has resolved a neutrino puzzle that physicists atmosphere. Others are produced in nuclear The detector measured neutrinos from the Sun. had wrestled with for decades. Compared reactions inside the Sun. Thousands of billions Its tank, filled with heavy water, was placed to theoretical calculations of the number of neutrinos stream through our bodies every two kilometres under the surface of the Earth. of neutrinos, up to two-thirds of them were second. The combined weight of neutrinos Signals from all three types of neutrinos were missing in measurements performed on Earth. is estimated to be roughly equal to that of all registered in the tank. The sum of the neutrinos The two research groups discovered that the visible stars in the universe.
    [Show full text]
  • Research in Kamioka and Kakenhi Takaaki Kajita Director of Institute for Cosmic Ray Research (ICRR) the University of Tokyo Rese
    Research in Kamioka and Kakenhi Takaaki Kajita Director of Institute for Cosmic Ray Research (ICRR) The University of Tokyo Research Theme Implemented in FY2017: First Detection of Gravitational Waves Using Cryogenic Laser Interferometer (Grant-in-Aid for Specially Promoted Research) I have conducted research underground Kamioka, Gifu Prefecture, since I was a graduate student. The first experiment I participated in was the Kamioka Nucleon Decay Experiment (Kamiokande). The experiment was initially proposed by Professor Masatoshi Koshiba, who was my thesis advisor, to search for proton decay. Professor Koshiba collaborated with a company to develop an unprecedentedly large 50-centimeter diameter photomultiplier tube (PMT) for the Kamiokande experiment. The PMT served a very important role in supernova neutrino observations that verified the supernova explosion mechanism and solar neutrino observations that confirmed the so-called solar neutrino problem. It is well known that, due to these achievements, Professor Koshiba received the Nobel Prize in physics in 2002. It is common for a large apparatus such as this to be realized by submitting a budget request from a host institute after long, vigorous discussions in relevant researcher communities. In this case, however, the enthusiasm of the relevant researchers in view of the importance of Kamiokande experiments made it possible to realize the experiment quickly with funds from various sources. Kamiokande initially materialized through collaboration with the University of Tokyo’s School of Science, to which Professor Koshiba belonged, the former National Laboratory for High Energy Physics (KEK), and the Institute for Cosmic Ray Research (ICRR) of the University of Tokyo. Although I was only a graduate student at that time and knew nothing about budgets, all of us participating in the effort recognized that people thought that this experiment was very important and endeavored to realize it as soon as possible.
    [Show full text]
  • Report and Opinion 2016;8(6) 1
    Report and Opinion 2016;8(6) http://www.sciencepub.net/report Beyond Einstein and Newton: A Scientific Odyssey Through Creation, Higher Dimensions, And The Cosmos Manjunath R Independent Researcher #16/1, 8 Th Main Road, Shivanagar, Rajajinagar, Bangalore: 560010, Karnataka, India [email protected], [email protected] “There is nothing new to be discovered in physics now. All that remains is more and more precise measurement.” : Lord Kelvin Abstract: General public regards science as a beautiful truth. But it is absolutely-absolutely false. Science has fatal limitations. The whole the scientific community is ignorant about it. It is strange that scientists are not raising the issues. Science means truth, and scientists are proponents of the truth. But they are teaching incorrect ideas to children (upcoming scientists) in schools /colleges etc. One who will raise the issue will face unprecedented initial criticism. Anyone can read the book and find out the truth. It is open to everyone. [Manjunath R. Beyond Einstein and Newton: A Scientific Odyssey Through Creation, Higher Dimensions, And The Cosmos. Rep Opinion 2016;8(6):1-81]. ISSN 1553-9873 (print); ISSN 2375-7205 (online). http://www.sciencepub.net/report. 1. doi:10.7537/marsroj08061601. Keywords: Science; Cosmos; Equations; Dimensions; Creation; Big Bang. “But the creative principle resides in Subaltern notable – built on the work of the great mathematics. In a certain sense, therefore, I hold it astronomers Galileo Galilei, Nicolaus Copernicus true that pure thought can
    [Show full text]
  • Highlights of Modern Physics and Astrophysics
    Highlights of Modern Physics and Astrophysics How to find the “Top Ten” in Physics & Astrophysics? - List of Nobel Laureates in Physics - Other prizes? Templeton prize, … - Top Citation Rankings of Publication Search Engines - Science News … - ... Nobel Laureates in Physics Year Names Achievement 2020 Sir Roger Penrose "for the discovery that black hole formation is a robust prediction of the general theory of relativity" Reinhard Genzel, Andrea Ghez "for the discovery of a supermassive compact object at the centre of our galaxy" 2019 James Peebles "for theoretical discoveries in physical cosmology" Michel Mayor, Didier Queloz "for the discovery of an exoplanet orbiting a solar-type star" 2018 Arthur Ashkin "for groundbreaking inventions in the field of laser physics", in particular "for the optical tweezers and their application to Gerard Mourou, Donna Strickland biological systems" "for groundbreaking inventions in the field of laser physics", in particular "for their method of generating high-intensity, ultra-short optical pulses" Nobel Laureates in Physics Year Names Achievement 2017 Rainer Weiss "for decisive contributions to the LIGO detector and the Kip Thorne, Barry Barish observation of gravitational waves" 2016 David J. Thouless, "for theoretical discoveries of topological phase transitions F. Duncan M. Haldane, and topological phases of matter" John M. Kosterlitz 2015 Takaaki Kajita, "for the discovery of neutrino oscillations, which shows that Arthur B. MsDonald neutrinos have mass" 2014 Isamu Akasaki, "for the invention of
    [Show full text]
  • Professor Takaaki Kajita Donates Two Types of Photomultiplier Tubes to the Nobel Museum
    Professor Takaaki Kajita donates two types of photomultiplier tubes to the Nobel Museum December 6, 2015 — 2015 Nobel Laureate Professor Takaaki Kajita, Director of the University of Tokyo Institute for Cosmic Ray Research, has donated two types of photomultiplier tubes to the Nobel Museum in Stockholm as artifacts related to his research. A photomultiplier tube is a type of photosensor used in the Super-Kamiokande experiment at the Kamioka Observatory in central Japan. Professor Kajita has donated one sensor each from the Super-Kamiokande inner and outer detectors to the museum. The Super-Kamiokande detector is filled with 50,000 tons of purified water and is divided into an inner detector, which holds 32,000 tons, and a two meter-wide outer detector that contains the remainder (Figure 1). The wall of the inner detector is lined with around 11,000 photomultiplier tubes, each with a 20 inch (50 cm) diameter (Figure 2), that detect Cherenkov light originating from reactions between neutrinos and water in the inner detector. The 20-inch photomultiplier tube was first developed in 1981 by Hamamatsu Photonics K.K. in collaboration with the University of Tokyo and KEK for the Kamiokande detector. The photomultiplier tubes used in the Super-Kamiokande detector are the result of continuous improvements to this original model. In 2014 the 20-inch photomultiplier tube was recognized with an IEEE milestone award. IEEE Milestones in Electrical Engineering and Computing honor significant technical achievements in electrical, electronics, informatics and communications fields. The outer detector is fitted with 1,885 photomultiplier tubes that are 8 inches (20 cm) in diameter (Figure 3).
    [Show full text]
  • HOPE MEETINGS with Nobel Laureates
    For Overseas Cooperating Institutions HOPE MEETINGS with Nobel Laureates Objective HOPE Meetings are held for excellent graduate students and young 13th researchers specially selected from countries/areas around the Asia-Pacific and Africa regions. They give an opportunity for the HOPE participants to engage in interdisciplinary discussions with Nobel laureates and other distinguished scientists pioneering the frontiers of knowledge. They also give the participants, who lodge together MEETING over the course of the event, a chance to make friends and form with Nobel Laureates collegial networks with peers from the regions. https://www.jsps.go.jp/english/e-hope/index.html Nobel Prize Dialogue (NPD) Tokyo 2021 Reception for HOPE & NPD participants jointly hosted 17-21 by JSPS & Nobel Media AB ・ arch, 2021 Sunday, 21 March, 2021 M Venue (Tentative) Organizer Yokohama, Office of the HOPE Meetings, JSPS E-mail [email protected] JAPAN Tel: +81-3-3263-2414 Fax:+81-3-3234-3700 1 HOPE MEETINGS with Nobel Laureates Organizing Committee of the 13th HOPE Meeting ■Chair KAJITA Takaaki Nobel Laureate in Physics 2015 Director, Institute for Cosmic Ray Research (ICRR) Distinguished University Professor, The University of Tokyo ■Organizing Committee Members See: https://www.jsps.go.jp/english/e-hope/sosiki13.html Participants About 100 doctoral students and young researchers from the following countries/areas: Australia, Bangladesh, China, Egypt, India, Indonesia, Israel, Japan, Kenya, Korea, Malaysia, Mongolia, Myanmar, Nepal, New Zealand, Philippines,
    [Show full text]
  • Programme 70Th Lindau Nobel Laureate Meeting 27 June - 2 July 2021
    70 Programme 70th Lindau Nobel Laureate Meeting 27 June - 2 July 2021 Sessions Speakers Access Background Scientific sessions, Nobel Laureates, Clear guidance Everything else social functions, young scientists, to all viewing there is to know partner events, invited experts, and participation for a successful networking breaks moderators options meeting 2 Welcome Two months ago, everything was well on course to celebrate And yet: this interdisciplinary our 70th anniversary with you, in Lindau. anniversary meeting will feature But with the safety and health of all our participants being the most rich and versatile programme ever. of paramount importance, we were left with only one choice: It will provide plenty of opportunity to educate, inspire, go online. connect – and to celebrate! Join us. 4 PARTICIPATING LAUREATES 4 PARTICIPATING LAUREATES 5 Henry A. Joachim Donna George P. Hartmut Michael M. Adam Hiroshi Kissinger Frank Strickland Smith Michel Rosbash Riess Amano Jeffrey A. Peter Richard R. James P. Randy W. Brian K. Barry C. Dean Agre Schrock Allison Schekman Kobilka Barish John L. Harvey J. Robert H. J. Michael Martin J. Hall Alter Grubbs Kosterlitz Evans F. Duncan David J. Ben L. Edmond H. Carlo Brian P. Kailash Elizabeth Haldane Gross Feringa Fischer Rubbia Schmidt Satyarthi Blackburn Robert B. Reinhard Aaron Walter Barry J. Harald Takaaki Laughlin Genzel Ciechanover Gilbert Marshall zur Hausen Kajita Christiane Serge Steven Françoise Didier Martin Nüsslein- Haroche Chu Barré-Sinoussi Queloz Chalfie Volhard Anthony J. Gregg L. Robert J. Saul Klaus William G. Leggett Semenza Lefkowitz Perlmutter von Klitzing Kaelin Jr. Stefan W. Thomas C. Emmanuelle Kurt Ada Konstantin S.
    [Show full text]