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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. -
A Cultural Analysis of a Physicist ''Trio'' Supporting the Backlash Against
ARTICLE IN PRESS Global Environmental Change 18 (2008) 204–219 www.elsevier.com/locate/gloenvcha Experiences of modernity in the greenhouse: A cultural analysis of a physicist ‘‘trio’’ supporting the backlash against global warming Myanna Lahsenà Center for Science and Technology Policy Research, University of Colorado and Instituto Nacional de Pesquisas Epaciais (INPE), Av. dos Astronautas, 1758, Sa˜o Jose´ dos Campos, SP 12227-010 Brazil Received 18 March 2007; received in revised form 5 October 2007; accepted 29 October 2007 Abstract This paper identifies cultural and historical dimensions that structure US climate science politics. It explores why a key subset of scientists—the physicist founders and leaders of the influential George C. Marshall Institute—chose to lend their scientific authority to this movement which continues to powerfully shape US climate policy. The paper suggests that these physicists joined the environmental backlash to stem changing tides in science and society, and to defend their preferred understandings of science, modernity, and of themselves as a physicist elite—understandings challenged by on-going transformations encapsulated by the widespread concern about human-induced climate change. r 2007 Elsevier Ltd. All rights reserved. Keywords: Anti-environmental movement; Human dimensions research; Climate change; Controversy; United States; George C. Marshall Institute 1. Introduction change itself, what he termed a ‘‘strong theory of culture.’’ Arguing that the essential role of science in our present age Human Dimensions Research in the area of global only can be fully understood through examination of environmental change tends to integrate a limited con- individuals’ relationships with each other and with ‘‘mean- ceptualization of culture. -
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. -
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. -
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 . -
PUZZLES and PROSPECTS in PLANETARY RING DYNAMICS PETER GOLDREICH California Institute of Technology Abstract. I Outline Some Of
PUZZLES AND PROSPECTS IN PLANETARY RING DYNAMICS PETER GOLDREICH California Institute of Technology Abstract. I outline some of the main processes that shape planetary rings. Then I focus on two outstanding issues, the role of self-gravity in the precession of narrow rings and the dynamics of Neptune's arcs. By airing these well-defined but unsolved problems, I hope to encourage others to join me in the quest for their solutions. 1. Introduction The 15 years just past have witnessed an explosion in our knowledge of planetary rings. Jupiter, Uranus, and Neptune have joined Saturn as members of the family of ringed planets. We have come to appreciate that a few simple physical mechanisms account for the bewildering variety of structures displayed by ring systems. With the completion of the Voyager missions, the level of activity in this field will decline. Major new discoveries probably must await the arrival of the Cassini spacecraft at Saturn a decade hence. Planetary rings were the focus of my research for several years. Although this has not been the case for some time, and may never be again, they still hold my interest. After struggling to understand various issues, I feel well-situated to offer a commentary on unsolved problems. That is my aim here. After a brief review of some of the processes at work in rings, I shall focus attention on two outstanding puzzles. The first involves the precession of narrow rings and, in particular, the role played by the self-gravity of the ring material. The second concerns the mechanisms responsible for the unusual morphology of Neptune's ring arcs. -
The I Nstitute L E T T E R
THE I NSTITUTE L E T T E R INSTITUTE FOR ADVANCED STUDY PRINCETON, NEW JERSEY · FALL 2004 ARNOLD LEVINE APPOINTED FACULTY MEMBER IN THE SCHOOL OF NATURAL SCIENCES he Institute for Advanced Study has announced the appointment of Arnold J. Professor in the Life Sciences until 1998. TLevine as professor of molecular biology in the School of Natural Sciences. Profes- He was on the faculty of the Biochemistry sor Levine was formerly a visiting professor in the School of Natural Sciences where he Department at Princeton University from established the Center for Systems Biology (see page 4). “We are delighted to welcome 1968 to 1979, when he became chair and to the Faculty of the Institute a scientist who has made such notable contributions to professor in the Department of Microbi- both basic and applied biological research. Under Professor Levine’s leadership, the ology at the State University of New York Center for Systems Biology will continue working in close collaboration with the Can- at Stony Brook, School of Medicine. cer Institute of New Jersey, Robert Wood Johnson Medical School, Lewis-Sigler Center The recipient of many honors, among for Integrative Genomics at Princeton University, and BioMaPS Institute at Rutgers, his most recent are: the Medal for Out- The State University of New Jersey, as well as such industrial partners as IBM, Siemens standing Contributions to Biomedical Corporate Research, Inc., Bristol-Myers Squibb, and Merck & Co.,” commented Peter Research from Memorial Sloan-Kettering Goddard, Director of the Institute. Cancer Center (2000); the Keio Medical Arnold J. Levine’s research has centered on the causes of cancer in humans and ani- Science Prize of the Keio University mals. -
Interview with Peter Goldreich
PETER GOLDREICH (b. 1939) INTERVIEWED BY SHIRLEY K. COHEN March, April and November 1998 ARCHIVES CALIFORNIA INSTITUTE OF TECHNOLOGY Pasadena, California Preface to the LIGO Series Interviews The interview of Peter Goldreich (1998) was originally done as part of a series of 15 oral histories conducted by the Caltech Archives between 1996 and 2000 on the beginnings of the Laser Interferometer Gravitational-Wave Observatory (LIGO). Many of those interviews have already been made available in print form with the designation “The LIGO Interviews: Series I.” A second series of interviews was planned to begin after LIGO became operational (August 2002); however, current plans are to undertake Series II after the observatory’s improved version, known as Advanced LIGO, begins operations, which is expected in 2014. Some of the LIGO Series I interviews (with the “Series I” designation dropped) have now been placed online within Caltech’s digital repository, CODA. All Caltech interviews that cover LIGO, either exclusively or in part, will be indexed and keyworded for LIGO to enable online discovery. The original LIGO partnership was formed between Caltech and MIT. It was from the start the largest and most costly scientific project ever undertaken by Caltech. Today it has expanded into an international endeavor with partners in Europe, Japan, India, and Australia. As of this writing, 760 scientists from 11 countries are participating in the LSC—the LIGO Scientific Collaboration. http://resolver.caltech.edu/CaltechOH:OH_Goldreich_P Subject area Physics, geology, planetary science, astronomy, astrophysics, LIGO Abstract Interview in five sessions in March, April, and November 1998 with Peter Goldreich, Lee A. -
Statement of William Happer at the Public Hearing of the Bundestag, 21 July, 2021
Statement of William Happer at the public hearing of the Bundestag, 21 July, 2021. Ausschuss für Umwelt, Naturschutz und nukleare Sicherheit I am Dr. William Happer a Professor of Physics, Emeritus at Princeton University, located in the state of New Jersey of the United States of America. Let me suggest why my comments today should be taken seriously. I have published over 200 peer-reviewed scientific papers, many of them on the interaction of radiation with matter, the basic physics that determines how greenhouse gases influence Earth’s climate. I am the inventor of the sodium guide star, which is used in most new ground-based telescopes to measure and correct for the degradation of astronomical images by atmospheric turbulence. I served as the Director of the Office of Energy Research of the US Department of Energy from 1990 to 1993, where I supervised a research budget of some $3.5 billion. A sizable part of this was directed toward environmental and climate science. From 2018 to 2019, I served as the Deputy Assistant to the President and Senior Director for Emerging Technologies at the National Security Council in the White House. I have received a number of scientific awards, and I am a member of several scientific societies, including the American Physical Society, the US National Academy of Sciences and the Philosophical Society. With this background, I know more than most scientists about how greenhouse gases work. Increasing levels of the main anthropogenic greenhouse gas, carbon dioxide (CO2), will cause a small, beneficial warming of Earth’s climate. More CO2 will be very good for agriculture, forestry, and all photosynthetic life. -
January 1998 Communication, APS Centennial Are Sessler’S Top Priorities in 1998
Education Outreach A P S N E W S Insert JANUARY1998 THE AMERICAN PHYSICAL SOCIETY VOLUME 7, NO 1 APS NewsTry the enhanced APS News-online: [http://www.aps.org/apsnews] Langer Chosen as APS Vice- Shuttle Physics President in 1997 Election embers of The view, page 2). M American Physi- In other election re- cal Society have elected sults, Daniel Kleppner of James S. Langer, a profes- the Massachusetts Insti- sor of physics at the tute of Technology was University of California, elected as chair-elect of Santa Barbara, to be the the Nominating Com- Society’s next vice-presi- mittee, which will be dent. Langer’s term chaired by Wick Haxton begins on January 1 , (University of Washing- when he will succeed ton) in 1998. The Jerome Friedman (Massa- Nominating Committee chusetts Institute of selects the slate of candi- Technology), who will dates for vice-president, become president-elect. general councillors, and Langer will become APS president in its own chair-elect. Its choices are then 2000. The 1998 president is Andrew Sessler voted on by the APS membership. Beverly (Lawrence Berkeley Laboratory) (see inter- K. Berger (Oakland University), Cynthia McIntyre (George Mason University), Roberto Peccei (University of California, Life APS member, Roger K. Crouch, a payload specialist aboard the 83rd flight of the Los Angeles), and Helen Quinn (Stanford United States Space Shuttle, Columbia, volunteered to take with him an APS paperweight Inside Linear Accelerator Center) were elected commemorating the 100 year anniversary of the electron and 50 year anniversary of the News as general councillors. transistor. -
Climate Change Motivated Reasoning
1 Reasoning about climate change Bence Bago1,2*, David G. Rand3,4, & Gordon Pennycook5 1Institute for Advanced Study in Toulouse, University of Toulouse 1 - Capitole 2Artificial and Natural Intelligence Toulouse Institute 3Sloan School, Massachusetts Institute of Technology 4Department of Brain and Cognitive Sciences, Massachusetts Institute of Technology 5Hill/Levene Schools of Business, University of Regina *Corresponding author: Bence Bago, Institute for Advanced Study in Toulouse, University of Toulouse 1 - Capitole, 1 esplanade de l’Université, 31080 Toulouse, France, e-mail: [email protected] 2 Abstract Why is disbelief in anthropogenic climate change common despite broad scientific consensus to the contrary? A widely-held explanation involves politically motivated (“System 2”) reasoning: Rather than helping uncover truth, people use their reasoning abilities to protect their partisan identities and reject beliefs that threaten those identities. Despite the popularity of this account, the evidence supporting it (i) does not account for the fact that partisanship is confounded with prior beliefs about the world, and (ii) is entirely correlational with respect to the effect of reasoning. Here, we address these shortcomings by (i) measuring prior beliefs and (ii) experimentally manipulating participants’ extent of reasoning using cognitive load and time pressure while they evaluate arguments for or against anthropogenic global warming. The results challenge the politically motivated system 2 reasoning account: Rather than exacerbating the impact of partisanship per se, engaging in more reasoning led people to have greater coherence between judgments and their prior beliefs about climate change - a process that can be consistent with rational (unbiased) Bayesian reasoning. Thus, we challenge the dominant cognitive account of climate disbelief, and suggest that interventions aimed at providing accurate information about climate change may be effective in the long run. -
1979-1980.Pdf
1 1980 CALIFORNIA INSTITUTE OF TECHNOLOGY 1201 East California Boulevard a"aUClla. California 91125 795-681 Academic Calendar 4 Directory 6 Board of Truslees 9 Administrative Officers 12 Administrative Committees 13 Faculty Officers and Committees 14 Staff 16 Division of Biology Division of Chemistry and Chemical Engineering 20 Division of Engineering and Applied Science 25 Division of Geological and Planetary Sciences 34 Division of the Humanities and Social Sciences 37 Division of Physics, Mathematics and Astronomy 40 Sherman Fairchild Distinguished Scholars 47 Athletics and Physical Education 48 Willis H. Booth Computing Center 48 Environmental Quality Laboratory 48 Hale Observatories 49 Health Center 50 Industrial Relations Center 50 Jet Propulsion Laboratory 51 Institute Libraries 52 Musical Activities 52 Officers and Faculty 54 SECTION II GENERAL INFORMATION Introduction 105 Historical Sketch 107 Buildings and Facilities 110 Libraries 114 Industrial Relations Center 115 The Willis H. Booth Computing Center ll5 Postdoctoral Appointments ]]5 Sherman Fairchild Distinguished Scholars Program 116 Study and Research 116 Aeronautics 116 Applied Mathematics 118 Applied Mechanics 118 Applied 119 Astronomy 120 Biology J22 Chemical Engineering 123 Chemistry 124 Civil Engineering 25 Computer Science 126 127 128 129 130 133 135 Materials Science 135 Mathematics Mechanical Engineering 136 Physics 137 Undergraduate Research 139 Student Life 139 Student Health 143 Notices and Agreements 145 SECTION In INFORMATION AND REGULATIONS FOR THE GUIDANCE