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Looking at Earth: an Astronaut's Journey Induction Ceremony 2017
american academy of arts & sciences winter 2018 www.amacad.org Bulletin vol. lxxi, no. 2 Induction Ceremony 2017 Class Speakers: Jane Mayer, Ursula Burns, James P. Allison, Heather K. Gerken, and Gerald Chan Annual David M. Rubenstein Lecture Looking at Earth: An Astronaut’s Journey David M. Rubenstein and Kathryn D. Sullivan ALSO: How Are Humans Different from Other Great Apes?–Ajit Varki, Pascal Gagneux, and Fred H. Gage Advancing Higher Education in America–Monica Lozano, Robert J. Birgeneau, Bob Jacobsen, and Michael S. McPherson Redistricting and Representation–Patti B. Saris, Gary King, Jamal Greene, and Moon Duchin noteworthy Select Prizes and Andrea Bertozzi (University of James R. Downing (St. Jude Chil- Barbara Grosz (Harvard Univer- California, Los Angeles) was se- dren’s Research Hospital) was sity) is the recipient of the Life- Awards to Members lected as a 2017 Simons Investi- awarded the 2017 E. Donnall time Achievement Award of the gator by the Simons Foundation. Thomas Lecture and Prize by the Association for Computational American Society of Hematology. Linguistics. Nobel Prize in Chemistry, Clara D. Bloomfield (Ohio State 2017 University) is the recipient of the Carol Dweck (Stanford Univer- Christopher Hacon (University 2017 Robert A. Kyle Award for sity) was awarded the inaugural of Utah) was awarded the Break- Joachim Frank (Columbia Univer- Outstanding Clinician-Scientist, Yidan Prize. through Prize in Mathematics. sity) presented by the Mayo Clinic Di- vision of Hematology. Felton Earls (Harvard Univer- Naomi Halas (Rice University) sity) is the recipient of the 2018 was awarded the 2018 Julius Ed- Nobel Prize in Economic Emmanuel J. -
Cosmology After WMAP (5)
Cosmology After WMAP (5) DavidDavid SpergelSpergel Geneve June 2008 StandardStandard cosmologicalcosmological modelmodel StillStill FitsFits thethe DataData ! General Relativity + Uniform Universe Big Bang " Density of universe determines its fate + shape ! Universe is flat (total density = critical density) " Atoms 4% " Dark Matter 23% " Dark Energy (cosmological constant?) 72% ! Universe has tiny ripples " Adiabatic, scale invariant, Gaussian Fluctuations " Harrison-Zeldovich-Peebles " Inflationary models QuickQuick HistoryHistory ofof thethe UniverseUniverse " Universe starts out hot, dense and filled with radiation " As the universe expands, it cools. • During the first minutes, light elements form • After 500,000 years, atoms form • After 100,000,000 years, stars start to form • After 1 Billion years, galaxies and quasars ThermalThermal HistoryHistory ofof UniverseUniverse radiation matter NEUTRAL r IONIZED 104 103 z GrowthGrowth ofof FluctuationsFluctuations •Linear theory •Basic elements have been understood for 30 years (Peebles, Sunyaev & Zeldovich) •Numerical codes agree at better than 0.1% (Seljak et al. 2003) Sunyaev & Zeldovich CMBCMB OverviewOverview ! We can detect both CMB temperature and polarization fluctuations ! Polarization Fluctuations can be decomposed into E and B modes q ~180/l ADIABATIC DENSITY FLUCTUATIONS ISOCURVATURE ENTROPY FLUCTUATIONS DeterminingDetermining BasicBasic ParametersParameters Baryon Density 2 Wbh = 0.015,0.017..0.031 also measured through D/H DeterminingDetermining BasicBasic ParametersParameters -
Small-Scale Anisotropies of the Cosmic Microwave Background: Experimental and Theoretical Perspectives
Small-Scale Anisotropies of the Cosmic Microwave Background: Experimental and Theoretical Perspectives Eric R. Switzer A DISSERTATION PRESENTED TO THE FACULTY OF PRINCETON UNIVERSITY IN CANDIDACY FOR THE DEGREE OF DOCTOR OF PHILOSOPHY RECOMMENDED FOR ACCEPTANCE BY THE DEPARTMENT OF PHYSICS [Adviser: Lyman Page] November 2008 c Copyright by Eric R. Switzer, 2008. All rights reserved. Abstract In this thesis, we consider both theoretical and experimental aspects of the cosmic microwave background (CMB) anisotropy for ℓ > 500. Part one addresses the process by which the universe first became neutral, its recombination history. The work described here moves closer to achiev- ing the precision needed for upcoming small-scale anisotropy experiments. Part two describes experimental work with the Atacama Cosmology Telescope (ACT), designed to measure these anisotropies, and focuses on its electronics and software, on the site stability, and on calibration and diagnostics. Cosmological recombination occurs when the universe has cooled sufficiently for neutral atomic species to form. The atomic processes in this era determine the evolution of the free electron abundance, which in turn determines the optical depth to Thomson scattering. The Thomson optical depth drops rapidly (cosmologically) as the electrons are captured. The radiation is then decoupled from the matter, and so travels almost unimpeded to us today as the CMB. Studies of the CMB provide a pristine view of this early stage of the universe (at around 300,000 years old), and the statistics of the CMB anisotropy inform a model of the universe which is precise and consistent with cosmological studies of the more recent universe from optical astronomy. -
Lars Hernquist and Volker Springel Receive $500,000 Gruber Cosmology Prize
Media Contact: A. Sarah Hreha +1 (203) 432‐6231 [email protected] Online Newsroom: https://gruber.yale.edu/news‐media Lars Hernquist and Volker Springel Receive $500,000 Gruber Cosmology Prize Lars Hernquist Volker Springel New Haven, CT — The 2020 Gruber Cosmology Prize recognizes Lars Hernquist, Center for Astrophysics | Harvard & Smithsonian, and Volker Springel, Max Planck Institute for Astrophysics, for their defining contributions to cosmological simulations, a method that tests existing theories of, and inspires new investigations into, the formation of structures at every scale from stars to galaxies to the universe itself. Hernquist and Springel will divide the $500,000 award, and each will receive a gold laureate pin at a ceremony that will take place later this year. The award recognizes their transformative work on structure formation in the universe, and development of numerical algorithms and community codes further used by many other researchers to significantly advance the field. Hernquist was a pioneer in cosmological simulations when he joined the fledgling field in the late 1980s, and since then he has become one of its most influential figures. Springel, who entered the field in 1998 and first partnered with Hernquist in the early 2000s, has written and applied several of the most widely used codes in cosmological research. Together Hernquist and Springel constitute, in the words of one Gruber Prize nominator, “one of the most productive collaborations ever in cosmology.” Computational simulations in cosmology begin with the traditional source of astronomical data: observations of the universe. Then, through a combination of theory and known physics that might approximate initial conditions, the simulations recreate the subsequent processes that would have led to the current structure. -
1St Edition of Brown Physics Imagine, 2017-2018
A note from the chair... "Fellow Travelers" Ladd Observatory.......................11 Sci-Toons....................................12 Faculty News.................. 15-16, 23 At-A-Glance................................18 s the current academic year draws to an end, I’m happy to report that the Physics Department has had Newton's Apple Tree................. 23 an exciting and productive year. At this year's Commencement, the department awarded thirty five "Untagling the Fabric of the undergraduate degrees (ScB and AB), twenty two Master’s degrees, and ten Ph.D. degrees. It is always Agratifying for me to congratulate our graduates and meet their families at the graduation ceremony. This Universe," Professor Jim Gates..26 Alumni News............................. 27 year, the University also awarded my colleague, Professor J. Michael Kosterlitz, an honorary degree for his Events this year......................... 28 achievement in the research of low-dimensional phase transitions. Well deserved, Michael! Remembering Charles Elbaum, Our faculty and students continue to generate cutting-edge scholarships. Some of their exciting Professor Emeritus.................... 29 research are highlighted in this magazine and have been published in high impact journals. I encourage you to learn about these and future works by watching the department YouTube channel or reading faculty’s original publications. Because of their excellent work, many of our undergraduate and graduate students have received students prestigious awards both from Brown and externally. As Chair, I feel proud every time I hear good news from our On the cover: PhD student Shayan Lame students, ranging from receiving the NSF Graduate Fellowship to a successful defense of thier senior thesis or a Class of 2018............................. -
The London School of Economics and Political Science
The London School of Economics and Political Science Modelling High Superconductivity: A Philosophical In Experiment a Maria Elena Di Bucchianico A thesis submitted to the Department of Philosophy, Logic and Scientific Method of the London School of Economics for the degree of Doctor of Philosophy, London, September 2009 UMI Number: U615704 All rights reserved INFORMATION TO ALL USERS The quality of this reproduction is dependent upon the quality of the copy submitted. In the unlikely event that the author did not send a complete manuscript and there are missing pages, these will be noted. Also, if material had to be removed, a note will indicate the deletion. Dissertation Publishing UMI U615704 Published by ProQuest LLC 2014. Copyright in the Dissertation held by the Author. Microform Edition © ProQuest LLC. All rights reserved. This work is protected against unauthorized copying under Title 17, United States Code. ProQuest LLC 789 East Eisenhower Parkway P.O. Box 1346 Ann Arbor, Ml 48106-1346 -rUr cr .c f ^IC7 Library &*shLto^yDfPo,|llcal an*eara"K*"K» I2-IS6H Declaration I certify that the thesis I have presented for examination for the PhD degree of the London School of Economics and Political Science is solely my own work other than where I have clearly indicated that it is the work of others (in which case the extent of any work carried out jointly by me and any other person is clearly identified in it). The copyright of this thesis rests with the author. Quotation from it is permitted, provided that full acknowledgement is made. This thesis may not be reproduced without the prior written consent of the author. -
Report for the Academic Year 1999
l'gEgasag^a3;•*a^oggMaBgaBK>ry^vg^.g^._--r^J3^JBgig^^gqt«a»J^:^^^^^ Institute /or ADVANCED STUDY REPORT FOR THE ACADEMIC YEAR 1998-99 PRINCETON • NEW JERSEY HISTORICAL STUDIES^SOCIAl SC^JCE LIBRARY INSTITUTE FOR ADVANCED STUDY PRINCETON, NEW JERSEY 08540 Institute /or ADVANCED STUDY REPORT FOR THE ACADEMIC YEAR 1 998 - 99 OLDEN LANE PRINCETON • NEW JERSEY • 08540-0631 609-734-8000 609-924-8399 (Fax) http://www.ias.edu Extract from the letter addressed by the Institute's Founders, Louis Bamberger and Mrs. FeUx Fuld, to the Board of Trustees, dated June 4, 1930. Newark, New Jersey. It is fundamental m our purpose, and our express desire, that in the appointments to the staff and faculty, as well as in the admission of workers and students, no account shall be taken, directly or indirectly, of race, religion, or sex. We feel strongly that the spirit characteristic of America at its noblest, above all the pursuit of higher learning, cannot admit of any conditions as to personnel other than those designed to promote the objects for which this institution is established, and particularly with no regard whatever to accidents of race, creed, or sex. ni' TABLE OF CONTENTS 4 • BACKGROUND AND PURPOSE 7 • FOUNDERS, TRUSTEES AND OFFICERS OF THE BOARD AND OF THE CORPORATION 10 • ADMINISTRATION 12 • PRESENT AND PAST DIRECTORS AND FACULTY 15 REPORT OF THE CHAIRMAN 18 • REPORT OF THE DIRECTOR 22 • OFFICE OF THE DIRECTOR - RECORD OF EVENTS 27 ACKNOWLEDGMENTS 41 • REPORT OF THE SCHOOL OF HISTORICAL STUDIES FACULTY ACADEMIC ACTIVITIES MEMBERS, VISITORS, -
Astro2020 Science White Paper Primordial Non-Gaussianity
Astro2020 Science White Paper Primordial Non-Gaussianity Thematic Areas: Cosmology and Fundamental Physics Principal Author: Name: P. Daniel Meerburg Institution: University of Cambridge Email: [email protected] Abstract: Our current understanding of the Universe is established through the pristine measurements of structure in the cosmic microwave background (CMB) and the distribution and shapes of galaxies tracing the large scale structure (LSS) of the Universe. One key ingredient that underlies cosmological observables is that the field that sources the observed structure is assumed to be initially Gaussian with high precision. Nevertheless, a minimal deviation from Gaussianity is perhaps the most robust theoretical prediction of models that explain the observed Universe; it is necessarily present even in the simplest scenarios. In addition, most inflationary models produce far higher levels of non-Gaussianity. Since non-Gaussianity directly probes the dynamics in the early Universe, a detection would present a monumental discovery in cosmology, providing clues about physics at energy scales as high as the GUT scale. This white paper aims to motivate a continued search to obtain evidence for deviations from Gaussianity in the primordial Universe. Since the previous decadal, important advances have been made, both theoretically and observationally, which have further established the importance of deviations from Gaussianity in cosmology. Foremost, primordial non-Gaussianities are now very tightly constrained by the CMB. Second, models motivated by stringy physics suggest detectable signatures of primordial non-Gaussianities with a unique shape which has not been considered in previous searches. Third, improving constraints using LSS requires a better understanding how to disentangle non-Gaussianities sourced at late times from those sourced by the physics in the early Universe. -
Superconductivity Record Breaks Under Pressure
NATURE | NEWS Superconductivity record breaks under pressure Everyday compound reported to conduct electricity without resistance at a record-high temperature, outstripping more exotic materials. Edwin Cartlidge 12 December 2014 Phil Degginger/Alamy Superconductors made of ceramics called cuprates have until now held the record for the warmest temperature at which they can operate, but a new class of materials could change that. For nearly 30 years, the search for a room-temperature superconductor has focused on exotic materials known as cuprates, which can carry currents without losing energy as heat at temperatures up to 164 Kelvin, or –109 ˚C. But scientists say that they have trumped that record using the common molecule hydrogen sulphide1. When they subjected a tiny sample of that material to pressures close to those inside Earth’s core, the researchers say that it was superconductive at 190 K (–83 ˚C). "If the result is reproduced, it will be quite shocking," says Robert Cava, a solid-state chemist at Princeton University in New Jersey. "It would be a historic discovery." According to the established theory of superconductivity — dubbed BCS theory after the surnames of its creators, John Bardeen, Leon Cooper and Robert Schrieffer — vibrations in a crystal's atoms can lead electrons to form ‘Cooper pairs’ that can flow through the crystal without resistance. BCS theory was developed in the 1950s, but most physicists believe that it cannot explain superconductivity in cuprates, which was discovered in 1986, or in iron pnictides2, found in 2006. Scientists hope that BCS theory can guide the search for other kinds of high-temperature superconductors, particularly in materials containing light elements such as hydrogen. -
Looking at Earth: an Astronaut's Journey Induction Ceremony 2017
american academy of arts & sciences winter 2018 www.amacad.org Bulletin vol. lxxi, no. 2 Induction Ceremony 2017 Class Speakers: Jane Mayer, Ursula Burns, James P. Allison, Heather K. Gerken, and Gerald Chan Annual David M. Rubenstein Lecture Looking at Earth: An Astronaut’s Journey David M. Rubenstein and Kathryn D. Sullivan ALSO: How Are Humans Different from Other Great Apes?–Ajit Varki, Pascal Gagneux, and Fred H. Gage Advancing Higher Education in America–Monica Lozano, Robert J. Birgeneau, Bob Jacobsen, and Michael S. McPherson Redistricting and Representation–Patti B. Saris, Gary King, Jamal Greene, and Moon Duchin Upcoming Events MARCH APRIL 1st 12th California Institute of Technology American Academy Pasadena, CA Cambridge, MA Bryson Symposium on Climate and Annual Awards Ceremony: A Celebration of the Energy Policy Arts and Sciences Featuring: Dallas Burtraw (Resources for Featuring: Martha C. Nussbaum (Univer- the Future), Ralph Cavanagh (nrdc), sity of Chicago), recipient of the Don M. Nathan S. Lewis (California Institute of Randel Award for Humanistic Studies; and Technology), Mary Nichols (California Barbara J. Meyer (University of California, Air Resources Board), Ronald O. Nichols Berkeley), recipient of the Francis Amory (Southern California Edison), Thomas F. Prize in Medicine & Physiology Rosenbaum (California Institute of Tech- nology), and Maxine L. Savitz (Honeywell, MAY Inc., ret.; formerly, President’s Council of Advisors on Science and Technology) 3rd American Academy 7th Cambridge, MA American Academy Songs of Love and Death: Sonnets by Petrarch Cambridge, MA and Others Set by Cipriano de Rore in “I madri- Building, Exploring, and Using the Tree of Life gali a cinque voci” (Venice, 1542) Featuring: Douglas E. -
Astro2020 Science White Paper Probing Feedback in Galaxy Formation with Millimeter-Wave Observations
Astro2020 Science White Paper Probing Feedback in Galaxy Formation with Millimeter-wave Observations Thematic Areas: Planetary Systems Star and Planet Formation Formation and Evolution of Compact Objects 3 Cosmology and Fundamental Physics Stars and Stellar Evolution Resolved Stellar Populations and their Environments 3 Galaxy Evolution Multi-Messenger Astronomy and Astrophysics Principal Authors: Names: Nicholas Battaglia, J. Colin Hill Institutions: Cornell University, Institute for Advanced Study Emails: [email protected], [email protected] Phones: (607)-255-3735, (509)-220-8589 Co-authors: Stefania Amodeo (Cornell), James G. Bartlett (APC/U. Paris Diderot), Kaustuv Basu (Uni- versity of Bonn), Jens Erler (University of Bonn), Simone Ferraro (Lawrence Berkeley Na- tional Laboratory), Lars Hernquist (Harvard), Mathew Madhavacheril (Princeton), Matthew McQuinn (University of Washington), Tony Mroczkowski (European Southern Observatory), Daisuke Nagai (Yale), Emmanuel Schaan (Lawrence Berkeley National Laboratory), Rachel Somerville (Rutgers/Flatiron Institute), Rashid Sunyaev (MPA), Mark Vogelsberger (MIT), Jessica Werk (University of Washington) Endorsers: James Aguirre (University of Pennsylvania), Zeeshan Ahmed (SLAC), Marcelo Alvarez arXiv:1903.04647v1 [astro-ph.CO] 11 Mar 2019 (UC–Berkeley), Daniel Angles-Alcazar (Flatiron Institute), Chetan Bavdhankar (National Center for Nuclear Physics), Eric Baxter (University of Pennsylvania), Andrew Benson (Carnegie Observatories), Bradford Benson (Fermi National Accelerator Laboratory/ Uni- versity of Chicago), Paolo de Bernardis (Sapienza Università di Roma), Frank Bertoldi (Uni- versity of Bonn), Fredirico Bianchini (University of Melbourne), Colin Bischoff (University of Cincinnati), Lindsey Bleem (Argonne National Laboratory/KICP), J. Richard Bond (Uni- versity of Toronto/ CITA), Greg Bryan (Columbia/Flatiron Institute), Erminia Calabrese (Cardiff), John E. Carlstrom (University of Chicago/Argonne National Laboratory/KICP), Joanne D. -
Electrically Conductive Metal−Organic Frameworks † † Lilia S
This is an open access article published under a Creative Commons Attribution (CC-BY) License, which permits unrestricted use, distribution and reproduction in any medium, provided the author and source are cited. pubs.acs.org/CR Review Electrically Conductive Metal−Organic Frameworks † † Lilia S. Xie, Grigorii Skorupskii, and Mircea Dinca*̆ Cite This: https://dx.doi.org/10.1021/acs.chemrev.9b00766 Read Online ACCESS Metrics & More Article Recommendations ABSTRACT: Metal−organic frameworks (MOFs) are intrinsically porous extended solids formed by coordination bonding between organic ligands and metal ions or clusters. High electrical conductivity is rare in MOFs, yet it allows for diverse applications in electrocatalysis, charge storage, and chemiresistive sensing, among others. In this Review, we discuss the efforts undertaken so far to achieve efficient charge transport in MOFs. We focus on four common strategies that have been harnessed toward high conductivities. In the “through-bond” approach, continuous chains of coordination bonds between the metal centers and ligands’ functional groups create charge transport pathways. In the “extended conjugation” approach, the metals and entire ligands form large delocalized systems. The “through-space” approach harnesses the π−π stacking interactions between organic moieties. The “guest-promoted” approach utilizes the inherent porosity of MOFs and host−guest interactions. Studies utilizing less defined transport pathways are also evaluated. For each approach, we give a systematic overview of the structures and transport properties of relevant materials. We consider the benefits and limitations of strategies developed thus far and provide an overview of outstanding challenges in conductive MOFs. CONTENTS 5.1. Metal-Based Hopping AA 5.2.