Woodstock of Physics” Revisited by Bill Evenson
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2005 CERN–CLAF School of High-Energy Physics
CERN–2006–015 19 December 2006 ORGANISATION EUROPÉENNE POUR LA RECHERCHE NUCLÉAIRE CERN EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH 2005 CERN–CLAF School of High-Energy Physics Malargüe, Argentina 27 February–12 March 2005 Proceedings Editors: N. Ellis M.T. Dova GENEVA 2006 CERN–290 copies printed–December 2006 Abstract The CERN–CLAF School of High-Energy Physics is intended to give young physicists an introduction to the theoretical aspects of recent advances in elementary particle physics. These proceedings contain lectures on field theory and the Standard Model, quantum chromodynamics, CP violation and flavour physics, as well as reports on cosmic rays, the Pierre Auger Project, instrumentation, and trigger and data-acquisition systems. iii Preface The third in the new series of Latin American Schools of High-Energy Physics took place in Malargüe, lo- cated in the south-east of the Province of Mendoza in Argentina, from 27 February to 12 March 2005. It was organized jointly by CERN and CLAF (Centro Latino Americano de Física), and with the strong support of CONICET (Consejo Nacional de Investigaciones Científicas y Técnicas). Fifty-four students coming from eleven different countries attended the School. While most of the students stayed in Hotel Rio Grande, a few students and the Staff stayed at Microtel situated close by. However, all the participants ate their meals to- gether at Hotel Rio Grande. According to the tradition of the School the students shared twin rooms mixing nationalities and in particular Europeans together with Latin Americans. María Teresa Dova from La Plata University was the local director for the School. -
The Physical Tourist Physics and New York City
Phys. perspect. 5 (2003) 87–121 © Birkha¨user Verlag, Basel, 2003 1422–6944/05/010087–35 The Physical Tourist Physics and New York City Benjamin Bederson* I discuss the contributions of physicists who have lived and worked in New York City within the context of the high schools, colleges, universities, and other institutions with which they were and are associated. I close with a walking tour of major sites of interest in Manhattan. Key words: Thomas A. Edison; Nikola Tesla; Michael I. Pupin; Hall of Fame for GreatAmericans;AlbertEinstein;OttoStern;HenryGoldman;J.RobertOppenheimer; Richard P. Feynman; Julian Schwinger; Isidor I. Rabi; Bronx High School of Science; StuyvesantHighSchool;TownsendHarrisHighSchool;NewYorkAcademyofSciences; Andrei Sakharov; Fordham University; Victor F. Hess; Cooper Union; Peter Cooper; City University of New York; City College; Brooklyn College; Melba Phillips; Hunter College; Rosalyn Yalow; Queens College; Lehman College; New York University; Courant Institute of Mathematical Sciences; Samuel F.B. Morse; John W. Draper; Columbia University; Polytechnic University; Manhattan Project; American Museum of Natural History; Rockefeller University; New York Public Library. Introduction When I was approached by the editors of Physics in Perspecti6e to prepare an article on New York City for The Physical Tourist section, I was happy to do so. I have been a New Yorker all my life, except for short-term stays elsewhere on sabbatical leaves and other visits. My professional life developed in New York, and I married and raised my family in New York and its environs. Accordingly, writing such an article seemed a natural thing to do. About halfway through its preparation, however, the attack on the World Trade Center took place. -
Real Time Density Functional Simulations of Quantum Scale
Real Time Density Functional Simulations of Quantum Scale Conductance by Jeremy Scott Evans B.A., Franklin & Marshall College (2003) Submitted to the Department of Chemistry in partial fulfillment of the requirements for the degree of Doctor of Philosophy at the MASSACHUSETTS INSTITUTE OF TECHNOLOGY June 2009 c Massachusetts Institute of Technology 2009. All rights reserved. Author............................................... ............... Department of Chemistry February 2, 2009 Certified by........................................... ............... Troy Van Voorhis Associate Professor of Chemistry Thesis Supervisor Accepted by........................................... .............. Robert W. Field Chairman, Department Committee on Graduate Theses This doctoral thesis has been examined by a Committee of the Depart- ment of Chemistry as follows: Professor Robert J. Silbey.............................. ............. Chairman, Thesis Committee Class of 1942 Professor of Chemistry Professor Troy Van Voorhis............................... ........... Thesis Supervisor Associate Professor of Chemistry Professor Jianshu Cao................................. .............. Member, Thesis Committee Associate Professor of Chemistry 2 Real Time Density Functional Simulations of Quantum Scale Conductance by Jeremy Scott Evans Submitted to the Department of Chemistry on February 2, 2009, in partial fulfillment of the requirements for the degree of Doctor of Philosophy Abstract We study electronic conductance through single molecules by subjecting -
The INT @ 20 the Future of Nuclear Physics and Its Intersections July 1 – 2, 2010
The INT @ 20 The Future of Nuclear Physics and its Intersections July 1 – 2, 2010 Program Thursday, July 1: 8:00 – 8:45: Registration (Kane Hall, Rom 210) 8:45 – 9:00: Opening remarks Mary Lidstrom, Vice Provost for Research, University of Washington David Kaplan, INT Director Session chair: David Kaplan 9:00 – 9:45: Science & Society 9:00 – 9:45 Steven Koonin, Undersecretary for Science, DOE The future of DOE and its intersections 9:45 – 10:30: Strong Interactions and Fundamental Symmetries 9:45 – 10:30 Howard Georgi, Harvard University QCD – From flavor SU(3) to effective field theory 10:30 – 11:00: Coffee Break Session chair: Martin Savage 11:00 – 11:30 Silas Beane, University of New Hampsire Lattice QCD for nuclear physics 11:30 – 12:00 Paulo Bedaque, University of Maryland Effective field theories in nuclear physics 12:00 – 12:30 Michael Ramsey-Musolf, University of Wisconsin Fundamental symmetries of nuclear physics: A window on the early Universe 12:30 – 2:00: Lunch (Mary Gates Hall) 1 Thursday, July 1 2:00 – 5:00: From Partons to Extreme Matter Session chair: Gerald Miller 2:00 – 2:30 Matthias Burkardt, New Mexico State University Transverse (spin) structure of hadrons 2:30 – 3:00 Barbara Jacak, SUNY Stony Brook Quark-gluon plasma: from particles to fields? 3:00 – 3:45 Raju Venugopalan, Brookhaven National Lab Wee gluons and their role in creating the hottest matter on Earth 3:45 – 4:15: Coffee Break Session chair: Krishna Rajagopal 4:15 – 4:45 Jean-Paul Blaizot, Saclay Is the quark-gluon plasma strongly or weakly coupled? 4:45 -
Nucleosynthesis
Nucleosynthesis Nucleosynthesis is the process that creates new atomic nuclei from pre-existing nucleons, primarily protons and neutrons. The first nuclei were formed about three minutes after the Big Bang, through the process called Big Bang nucleosynthesis. Seventeen minutes later the universe had cooled to a point at which these processes ended, so only the fastest and simplest reactions occurred, leaving our universe containing about 75% hydrogen, 24% helium, and traces of other elements such aslithium and the hydrogen isotope deuterium. The universe still has approximately the same composition today. Heavier nuclei were created from these, by several processes. Stars formed, and began to fuse light elements to heavier ones in their cores, giving off energy in the process, known as stellar nucleosynthesis. Fusion processes create many of the lighter elements up to and including iron and nickel, and these elements are ejected into space (the interstellar medium) when smaller stars shed their outer envelopes and become smaller stars known as white dwarfs. The remains of their ejected mass form theplanetary nebulae observable throughout our galaxy. Supernova nucleosynthesis within exploding stars by fusing carbon and oxygen is responsible for the abundances of elements between magnesium (atomic number 12) and nickel (atomic number 28).[1] Supernova nucleosynthesis is also thought to be responsible for the creation of rarer elements heavier than iron and nickel, in the last few seconds of a type II supernova event. The synthesis of these heavier elements absorbs energy (endothermic process) as they are created, from the energy produced during the supernova explosion. Some of those elements are created from the absorption of multiple neutrons (the r-process) in the period of a few seconds during the explosion. -
Primordial Nucleosynthesis: from Precision Cosmology To
DSF-20/2008, FERMILAB-PUB-08-216-A, IFIC/08-37 Primordial Nucleosynthesis: from precision cosmology to fundamental physics Fabio Iocco a1 , Gianpiero Mangano b, Gennaro Miele b,c, Ofelia Pisanti b, Pasquale D. Serpico d2 aINAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy bDip. Scienze Fisiche, Universit`adi Napoli Federico II & INFN, Sez. di Napoli, Complesso Univ. Monte S. Angelo, Via Cintia, I-80126 Napoli, Italy c Instituto de F´ısica Corpuscular (CSIC-Universitat de Val`encia), Ed. Institutos de Investigaci´on, Apartado de Correos 22085, E-46071 Val`encia, Spain dCenter for Particle Astrophysics, Fermi National Accelerator Laboratory, Batavia, IL 60510-0500, USA Abstract We present an up-to-date review of Big Bang Nucleosynthesis (BBN). We discuss the main improvements which have been achieved in the past two decades on the overall theoretical framework, summarize the impact of new experimental results on nuclear reaction rates, and critically re-examine the astrophysical determinations of light nuclei abundances. We report then on how BBN can be used as a powerful test of new physics, constraining a wide range of ideas and theoretical models of fundamental interactions beyond the standard model of strong and electroweak forces and Einstein’s general relativity. Key words: Primordial Nucleosynthesis; Early Universe; Physics Beyond the arXiv:0809.0631v2 [astro-ph] 16 Apr 2009 Standard Model PACS: 98.80.Ft; 26.35.+c; 98.62.Ai Contents 1 Introduction 3 2 Standard Cosmology 6 1 Present address: Institut -
The Struggle for Quantum Theory 47 5.1Aliensignals
Fundamental Forces of Nature The Story of Gauge Fields This page intentionally left blank Fundamental Forces of Nature The Story of Gauge Fields Kerson Huang Massachusetts Institute of Technology, USA World Scientific N E W J E R S E Y • L O N D O N • S I N G A P O R E • B E I J I N G • S H A N G H A I • H O N G K O N G • TA I P E I • C H E N N A I Published by World Scientific Publishing Co. Pte. Ltd. 5 Toh Tuck Link, Singapore 596224 USA office: 27 Warren Street, Suite 401-402, Hackensack, NJ 07601 UK office: 57 Shelton Street, Covent Garden, London WC2H 9HE British Library Cataloguing-in-Publication Data A catalogue record for this book is available from the British Library. FUNDAMENTAL FORCES OF NATURE The Story of Gauge Fields Copyright © 2007 by World Scientific Publishing Co. Pte. Ltd. All rights reserved. This book, or parts thereof, may not be reproduced in any form or by any means, electronic or mechanical, including photocopying, recording or any information storage and retrieval system now known or to be invented, without written permission from the Publisher. For photocopying of material in this volume, please pay a copying fee through the Copyright Clearance Center, Inc., 222 Rosewood Drive, Danvers, MA 01923, USA. In this case permission to photocopy is not required from the publisher. ISBN-13 978-981-270-644-7 ISBN-10 981-270-644-5 ISBN-13 978-981-270-645-4 (pbk) ISBN-10 981-270-645-3 (pbk) Printed in Singapore. -
JUAN MANUEL 2016 NOBEL PEACE PRIZE RECIPIENT Culture Friendship Justice
Friendship Volume 135, № 1 Character Culture JUAN MANUEL SANTOS 2016 NOBEL PEACE PRIZE RECIPIENT Justice LETTER FROM THE PRESIDENT Dear Brothers, It is an honor and a privilege as your president to have the challenges us and, perhaps, makes us question our own opportunity to share my message with you in each edition strongly held beliefs. But it also serves to open our minds of the Quarterly. I generally try to align my comments and our hearts to our fellow neighbor. It has to start with specific items highlighted in each publication. This with a desire to listen, to understand, and to be tolerant time, however, I want to return to the theme “living our of different points of view and a desire to be reasonable, Principles,” which I touched upon in a previous article. As patient and respectful.” you may recall, I attempted to outline and describe how Kelly concludes that it is the diversity of Southwest’s utilization of the Four Founding Principles could help people and “treating others like you would want to be undergraduates make good decisions and build better treated” that has made the organization successful. In a men. It occurred to me that the application of our values similar way, Stephen Covey’s widely read “Seven Habits of to undergraduates only is too limiting. These Principles are Highly Effective People” takes a “values-based” approach to indeed critical for each of us at this particularly turbulent organizational success. time in our society. For DU to be a successful organization, we too, must As I was flying back recently from the Delta Upsilon be able to work effectively with our varied constituents: International Fraternity Board of Directors meeting in undergraduates, parents, alumni, higher education Arizona, I glanced through the February 2017 edition professionals, etc. -
Press Release (PDF)
American Association of Physics Teachers FOR IMMEDIATE RELEASE Mary Beth Monroe Recognized for Creative Leadership in Physics Education College Park, Maryland, United States, October 29, 2009 —The American Associa- tion of Physics Teachers (AAPT) announced today that The Melba Newell Phillips Medal has been awarded to Mary Beth Monroe, Professor of Physics at Southwest Texas Junior College, in recognition of her creative leadership and dedicated service that have resulted in exceptional contributions within AAPT. The Medal will be presented to at a Ceremonial Session of the AAPT Winter Meeting at the Washington Marriott Wardman Park in Washington, DC, on Monday, February 15, 2010. Lila Adair, Chairman, AAPT Awards Committee, said, “Mary Beth is an amazing lady. She has dedicated her entire ca- reer to sharing her passion for physics and AAPT with her students, colleagues and fellow AAPT members. She is one of the few experts I turn to for the institutional history of AAPT, and I am so proud to be presenting the Phillips Medal to her.” As a long time AAPT member, Monroe has quietly and tenaciously served the organization at the state and national level for more than three decades. She served as AAPT Secretary and Chair of the Publications Committee from 2001-2007 and is currently serving as a member of the Committee on the Interests of Senior Physicists and as Chair of the Gover- nance Review Committee. She has played a leading role in developing networks among physicists teaching in Two Year Colleges that have led both to their increasing involvement in AAPT and to better teaching for the students who study physics in these schools “The Melba Newell Phillips Medal is AAPT’s highest recognition for member leadership and service. -
Direct Measurement of the Neutron
Louisiana State University LSU Digital Commons LSU Doctoral Dissertations Graduate School 1-9-2020 Stellar Nucleosynthesis: Direct Measurement of the Neutron- Capture Cross Sections of Stable Germanium Isotopes and Design of a Next Generation Ion Trap for the Study of Beta- Delayed Neutron Emission Alexander Laminack Louisiana State University and Agricultural and Mechanical College Follow this and additional works at: https://digitalcommons.lsu.edu/gradschool_dissertations Part of the Instrumentation Commons, Nuclear Commons, Physical Processes Commons, and the Stars, Interstellar Medium and the Galaxy Commons Recommended Citation Laminack, Alexander, "Stellar Nucleosynthesis: Direct Measurement of the Neutron-Capture Cross Sections of Stable Germanium Isotopes and Design of a Next Generation Ion Trap for the Study of Beta- Delayed Neutron Emission" (2020). LSU Doctoral Dissertations. 5131. https://digitalcommons.lsu.edu/gradschool_dissertations/5131 This Dissertation is brought to you for free and open access by the Graduate School at LSU Digital Commons. It has been accepted for inclusion in LSU Doctoral Dissertations by an authorized graduate school editor of LSU Digital Commons. For more information, please [email protected]. STELLAR NUCLEOSYNTHESIS: DIRECT MEASUREMENT OF THE NEUTRON-CAPTURE CROSS SECTIONS OF STABLE GERMANIUM ISOTOPES AND DESIGN OF A NEXT GENERATION ION TRAP FOR THE STUDY OF β-DELAYED NEUTRON EMISSION A Dissertation Submitted to the Graduate Faculty of the Louisiana State University and Agricultural and Mechanical College in partial fulfillment of the requirements for the degree of Doctor of Philosophy in The Department of Physics and Astronomy by Alexander Laminack B. S., The Unviersity of Alabama, 2015 May 2020 To my wife and son: Kristy Allen Alexander Laminack and Daniel Allen Laminack. -
From the Executive Director Kathryn Sullivan to Receive Sigma Xi's Mcgovern Award
May-June 2011 · Volume 20, Number 3 Kathryn Sullivan to From the Executive Director Receive Sigma Xi’s McGovern Award Annual Report In my report last year I challenged the membership to consider ormer astronaut the characteristics of successful associations. I suggested that we Kathryn D. emulate what successful associations do that others do not. This FSullivan, the first year as I reflect back on the previous fiscal year, I suggest that we need to go even further. U.S. woman to walk We have intangible assets that could, if converted to tangible outcomes, add to the in space, will receive value of active membership in Sigma Xi. I believe that standing up for high ethical Sigma Xi’s 2011 John standards, encouraging the earlier career scientist and networking with colleagues of diverse disciplines is still very relevant to our professional lives. Membership in Sigma P. McGovern Science Xi still represents recognition for scientific achievements, but the value comes from and Society Award. sharing with companions in zealous research. Since 1984, a highlight of Sigma Xi’s Stronger retention of members through better local programs would benefit the annual meeting has been the McGovern Society in many ways. It appears that we have continued to initiate new members in Lecture, which is made by the recipient of numbers similar to past years but retention has declined significantly. In addition, the the McGovern Medal. Recent recipients source of the new members is moving more and more to the “At-large” category and less and less through the Research/Doctoral chapters. have included oceanographer Sylvia Earle and Nobel laureates Norman Borlaug, Mario While Sigma Xi calls itself a “chapter-based” Society, we have found that only about half of our “active” members are affiliated with chapters in “good standing.” As long Molina and Roald Hoffmann. -
January 2021 Newsletter
APS Division of In this issue Astrophysics • April Meeting Online • Upcoming DAP election alert Electronic Newsletter January 2021 • APS Fellows • Bethe Prize Winner • Student/Postdoc Travel Grants • April Meeting: DAP and Plenary Programs & Abstract Categories • Snowmass Update APS DAP Officers 2020–2021: Finalize your plans now to attend the April 2021 meeting held virtually this year. A • Chair: Glennys Farrar number of plenary and invited sessions will • Past Chair: Joshua Frieman feature presentations by DAP members. Here are the key details: • Chair Elect: Chris Fryer • Vice Chair: Daniel Holz What: April 2021 APS Meeting • Secretary/Treasurer: Judith Racusin When: April 17 - 20, 2021 • Deputy Sec./Treasurer: Amy Furniss Where: Online Abstract Deadline: Jan 8, 2021, 5 pm EST • Division Councilor: Cole Miller Travel Grant Deadline: Jan 31, 2021 • Member-at-Large: Stefano Profumo Early Registration Deadline: Feb 26, 2021 • Member-at-Large: Ignacio Taboada Late Registration Deadline: Mar 26, 2021 • Member-at-Large: Erin Kara • Member-at-Large: Laura Blecha The 2021 April Meeting will be virtual. Questions? Comments? Detailed information for the meeting, including details on registration and the scientific Newsletter editors: program can be found online at https://april.aps.org/ Amy Furniss [email protected] HEADS-UP: The ELECTION for next year’s DAP Executive Committee and chairline will Judith Racusin be held soon. Be on the lookout for the [email protected] announcement from APS, and please vote! 1 Dear DAP, Please see the January 2021 DAP newsletter below. It will be archived on the DAP website (https://www.aps.org/units/dap/newsletters/index.cfm).