History of Physicists in Industry Final Report
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A Brief Tour Into the History of Gravity: from Emocritus to Einstein
American Journal of Space Science 1 (1): 33-45, 2013 ISSN: 1948-9927 © 2013 Science Publications doi:10.3844/ajssp.2013.33.45 Published Online 1 (1) 2013 (http://www.thescipub.com/ajss.toc) A Brief Tour into the History of Gravity: From Emocritus to Einstein Panagiotis Papaspirou and Xenophon Moussas Department of Physics, Section of Astrophysics, Astronomy and Mechanics, University of Athens, Athens, Greece ABSTRACT The History of Gravity encompasses many different versions of the idea of the Gravitational interaction, which starts already from the Presocratic Atomists, continues to the doctrines of the Platonic and Neoplatonic School and of the Aristotelian School, passes through the works of John Philoponus and John Bouridan and reaches the visions of Johannes Kepler and Galileo Galilei. Then, the major breakthrough in the Theory of Motion and the Theory of Gravity takes place within the realm of Isaac Newton’s most famous Principia and of the work of Gottfried Leibniz, continues with the contributions of the Post- newtonians, such as Leonhard Euler, reaches the epoch of its modern formulation by Ernst Mach and other Giants of Physics and Philosophy of this epoch, enriches its structure within the work of Henry Poincare and finally culminates within the work of Albert Einstein, with the formulation of the Theory of Special Relativity and of General Relativity at the begin of the 20th century. The evolution of the Theory of General Relativity still continues up to our times, is rich in forms it takes and full of ideas of theoretical strength. Many fundamental concepts of the Epistemology and the History of Physics appear in the study of the Theory of Gravity, such as the notions of Space, of Time, of Motion, of Mass, in its Inertial, Active Gravitational and Passive Gravitational form, of the Inertial system of reference, of the Force, of the Field, of the Riemannian Geometry and of the Field Equations. -
Newton.Indd | Sander Pinkse Boekproductie | 16-11-12 / 14:45 | Pag
omslag Newton.indd | Sander Pinkse Boekproductie | 16-11-12 / 14:45 | Pag. 1 e Dutch Republic proved ‘A new light on several to be extremely receptive to major gures involved in the groundbreaking ideas of Newton Isaac Newton (–). the reception of Newton’s Dutch scholars such as Willem work.’ and the Netherlands Jacob ’s Gravesande and Petrus Prof. Bert Theunissen, Newton the Netherlands and van Musschenbroek played a Utrecht University crucial role in the adaption and How Isaac Newton was Fashioned dissemination of Newton’s work, ‘is book provides an in the Dutch Republic not only in the Netherlands important contribution to but also in the rest of Europe. EDITED BY ERIC JORINK In the course of the eighteenth the study of the European AND AD MAAS century, Newton’s ideas (in Enlightenment with new dierent guises and interpre- insights in the circulation tations) became a veritable hype in Dutch society. In Newton of knowledge.’ and the Netherlands Newton’s Prof. Frans van Lunteren, sudden success is analyzed in Leiden University great depth and put into a new perspective. Ad Maas is curator at the Museum Boerhaave, Leiden, the Netherlands. Eric Jorink is researcher at the Huygens Institute for Netherlands History (Royal Dutch Academy of Arts and Sciences). / www.lup.nl LUP Newton and the Netherlands.indd | Sander Pinkse Boekproductie | 16-11-12 / 16:47 | Pag. 1 Newton and the Netherlands Newton and the Netherlands.indd | Sander Pinkse Boekproductie | 16-11-12 / 16:47 | Pag. 2 Newton and the Netherlands.indd | Sander Pinkse Boekproductie | 16-11-12 / 16:47 | Pag. -
Introduction
Introduction Queen's College, the predecessor of Rutgers University, was the eighth college to be founded in the American colonies. The early colonial colleges were founded to meet the emerging needs for an educated clergy, and to provide education to other leaders of the community. The religious leaders of the colonies were foremost in the movements to establish these colleges. Although denominational sponsorship was critical to the founding and early support of the colleges, there were generally no religious tests for students, and the colleges were chartered by the colonies. Leaders of the Puritan Congregational Church founded Harvard College in 1636 with a bequest of £400 from the Massachusetts Bay Colony. The College was organized and named Harvard College in 1639, and chartered in 1650. The traditional list of colonial colleges that followed Harvard College begins with William and Mary College, which was founded in 1693 by leaders of the Anglican Episcopal Church, followed by Yale College, which was founded in 1701 by leaders of the Puritan Congregational Church. The College of Philadelphia (later University of Pennsylvania) was founded in 1740 by Benjamin Franklin and other leading citizens of Philadelphia, and had the weakest religious connections of the colonial colleges. The College of New Jersey (later Princeton College) was founded in 1746 by leaders of the Presbyterian Church, King's College (later Columbia College) was founded in 1754 by leaders of the Anglican Episcopal Church, and the College of Rhode Island (later Brown College) was founded in 1764 by leaders of the Baptist Church. 1 History of Physics and Astronomy Some elements of physics and astronomy were taught in the colonial colleges from the time they opened. -
What's the Problem with the Cosmological Constant?
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Philsci-Archive What’s the problem with the cosmological constant? Mike D. Schneider∗y Abstract The “Cosmological Constant Problem” (CCP) is widely considered a crisis in contemporary theoretical physics. Unfortunately, the search for its resolution is hampered by open disagreement about what is, strictly, the problem. This disagreement stems from the observation that the CCP is not a problem within any of our current theories, and nearly all of the details of those future theories for which the CCP could be made a problem are up for grabs. Given this state of affairs, I discuss how one ought to make sense of the role of the CCP in physics and generalize some lessons from it. ∗To contact the author, write to: Mike D. Schneider, Department of Logic and Philosophy of Science, University of California, Irvine; e-mail: [email protected]. yI would like to thank James Owen Weatherall and Erik Curiel for their steering comments on earlier drafts of this paper. I am also grateful for the many questions and comments from members of the Southern California Philosophy of Physics reading group, as well as for the positive reception of the paper at the Philosophy of Logic, Math, and Physics graduate student conference at the Rotman Institute of Philosophy at Western University. Finally, I am indebted to Jeffrey Barrett, JB Manchak, Hannah Rubin, Kyle Stanford, and John Earman, as well as to an anonymous reviewer and an editor for pushing me to make my punchlines clearer. -
Galileo's Contribution to Mechanics
Loyola University Chicago Loyola eCommons Physics: Faculty Publications and Other Works Faculty Publications 5-4-2017 Galileo's Contribution to Mechanics Asim Gangopadhyaya Loyola University Chicago, [email protected] Follow this and additional works at: https://ecommons.luc.edu/physics_facpubs Part of the History of Science, Technology, and Medicine Commons, and the Physics Commons Recommended Citation Gangopadhyaya, Asim, "Galileo's Contribution to Mechanics" (2017). Physics: Faculty Publications and Other Works. 49. https://ecommons.luc.edu/physics_facpubs/49 This Book Chapter is brought to you for free and open access by the Faculty Publications at Loyola eCommons. It has been accepted for inclusion in Physics: Faculty Publications and Other Works by an authorized administrator of Loyola eCommons. For more information, please contact [email protected]. This work is licensed under a Creative Commons Attribution-Noncommercial-No Derivative Works 3.0 License. © Wipf and Stock Publishers 2017 WHERE HAVE ALL THE HEAVENS GONE? . Science and Religion, 400 B. C.toA.D.i550; From Aristotle to Copernicus. Greenwood Guides to Science and Religion. Westport, CT: Greenwood, 2004. Land, Barbara. The Telescope Makers: From Galileo to the Space Age. New York; Crowell, 1968. Lindberg, David C. The Beginnings of Western Science: The European Scientific Tradition in Philosophical, Religious, and Institutional Context, Prehistory to A.D. 1450. 2nd ed. Chicago: University of Chicago Press, 2007. "Galileo, the Church, and the Cosmos." In When Science and 5 Christianity Meet, edited by David C. Lindberg and Ronald L. Numbers, 33-60. Chicago: University of Chicago Press, 2003. Lindberg, David C, and Ronald L. Numbers. When Science and Christianity Galileo's Contribution to Mechanics Meet. -
Statistical Mechanics
3 d rB rB 3 d rA rA Statistical Mechanics Daniel F. Styer December 2007 Statistical Mechanics Dan Styer Department of Physics and Astronomy Oberlin College Oberlin, Ohio 44074-1088 [email protected] http://www.oberlin.edu/physics/dstyer December 2007 Although, as a matter of history, statistical mechanics owes its origin to investigations in thermodynamics, it seems eminently worthy of an independent development, both on account of the elegance and simplicity of its principles, and because it yields new results and places old truths in a new light. | J. Willard Gibbs Elementary Principles in Statistical Mechanics Contents 0 Preface 1 1 The Properties of Matter in Bulk 4 1.1 What is Statistical Mechanics About? . 4 1.2 Outline of Book . 4 1.3 Fluid Statics . 5 1.4 Phase Diagrams . 7 1.5 Additional Problems . 7 2 Principles of Statistical Mechanics 10 2.1 Microscopic Description of a Classical System . 10 2.2 Macroscopic Description of a Large Equilibrium System . 14 2.3 Fundamental Assumption . 15 2.4 Statistical Definition of Entropy . 17 2.5 Entropy of a Monatomic Ideal Gas . 19 2.6 Qualitative Features of Entropy . 25 2.7 Using Entropy to Find (Define) Temperature and Pressure . 34 2.8 Additional Problems . 44 3 Thermodynamics 46 3.1 Heat and Work . 46 3.2 Heat Engines . 50 i ii CONTENTS 3.3 Thermodynamic Quantities . 52 3.4 Multivariate Calculus . 55 3.5 The Thermodynamic Dance . 60 3.6 Non-fluid Systems . 67 3.7 Thermodynamics Applied to Fluids . 68 3.8 Thermodynamics Applied to Phase Transitions . -
A Short History of Physics (Pdf)
A Short History of Physics Bernd A. Berg Florida State University PHY 1090 FSU August 28, 2012. References: Most of the following is copied from Wikepedia. Bernd Berg () History Physics FSU August 28, 2012. 1 / 25 Introduction Philosophy and Religion aim at Fundamental Truths. It is my believe that the secured part of this is in Physics. This happend by Trial and Error over more than 2,500 years and became systematic Theory and Observation only in the last 500 years. This talk collects important events of this time period and attaches them to the names of some people. I can only give an inadequate presentation of the complex process of scientific progress. The hope is that the flavor get over. Bernd Berg () History Physics FSU August 28, 2012. 2 / 25 Physics From Acient Greek: \Nature". Broadly, it is the general analysis of nature, conducted in order to understand how the universe behaves. The universe is commonly defined as the totality of everything that exists or is known to exist. In many ways, physics stems from acient greek philosophy and was known as \natural philosophy" until the late 18th century. Bernd Berg () History Physics FSU August 28, 2012. 3 / 25 Ancient Physics: Remarkable people and ideas. Pythagoras (ca. 570{490 BC): a2 + b2 = c2 for rectangular triangle: Leucippus (early 5th century BC) opposed the idea of direct devine intervention in the universe. He and his student Democritus were the first to develop a theory of atomism. Plato (424/424{348/347) is said that to have disliked Democritus so much, that he wished his books burned. -
Verification, Validation, and Predictive Capability in Computational Engineering and Physics
SAND REPORT SAND2003-3769 Unlimited Release Printed February 2003 Verification, Validation, and Predictive Capability in Computational Engineering and Physics William L. Oberkampf, Timothy G. Trucano, and Charles Hirsch Prepared by Sandia National Laboratories Albuquerque, New Mexico 87185 and Livermore, California 94550 Sandia is a multiprogram laboratory operated by Sandia Corporation, a Lockheed Martin Company, for the United States Department of Energy’s National Nuclear Security Administration under Contract DE-AC04-94-AL85000. Approved for public release; further dissemination unlimited. Issued by Sandia National Laboratories, operated for the United States Department of Energy by Sandia Corporation. NOTICE: This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government, nor any agency thereof, nor any of their employees, nor any of their contractors, subcontractors, or their employees, make any warranty, express or implied, or assume any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represent that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise, does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government, any agency thereof, or any of their contractors or subcontractors. The views and opinions expressed herein do not necessarily state or reflect those of the United States Government, any agency thereof, or any of their contractors. Printed in the United States of America. This report has been reproduced directly from the best available copy. -
Subject Benchmark Statement: Physics, Astronomy and Astrophysics
QAA MEMBERSHIP Subject Benchmark Statement Physics, Astronomy and Astrophysics October 2019 Contents How can I use this document? ................................................................................................. 1 About the Statement ................................................................................................................ 2 Relationship to legislation ......................................................................................................... 2 Summary of changes from the previous Subject Benchmark Statement (2017) ....................... 2 1 Introduction ..................................................................................................................... 3 2 Nature and extent of physics, astronomy and astrophysics ............................................. 4 3 Subject-specific knowledge and understanding ............................................................... 6 4 Teaching, learning and assessment ................................................................................ 9 5 Benchmark standards ................................................................................................... 11 Appendix: Membership of the benchmarking and review groups for the Subject Benchmark Statement for Physics, Astronomy and Astrophysics ............................................................. 13 How can I use this document? This is the Subject Benchmark Statement for Physics, Astronomy and Astrophysics. It defines the academic standards that can be expected -
Physics and Medicine: a Historical Perspective
Series Physics and Medicine 1 Physics and medicine: a historical perspective Stephen F Keevil Nowadays, the term medical physics usually refers to the work of physicists employed in hospitals, who are concerned Lancet 2011; 379: 1517–24 mainly with medical applications of radiation, diagnostic imaging, and clinical measurement. This involvement in Published Online clinical work began barely 100 years ago, but the relation between physics and medicine has a much longer history. In April 18, 2012 this report, I have traced this history from the earliest recorded period, when physical agents such as heat and light DOI:10.1016/S0140- 6736(11)60282-1 began to be used to diagnose and treat disease. Later, great polymaths such as Leonardo da Vinci and Alhazen used See Comment pages 1463 physical principles to begin the quest to understand the function of the body. After the scientifi c revolution in the and 1464 17th century, early medical physicists developed a purely mechanistic approach to physiology, whereas others applied This is the fi rst in a Series of ideas derived from physics in an eff ort to comprehend the nature of life itself. These early investigations led directly fi ve papers about physics to the development of specialties such as electrophysiology, biomechanics, and ophthalmology. Physics-based medical and medicine technology developed rapidly during the 19th century, but it was the revolutionary discoveries about radiation and Department of Medical radioactivity at the end of the century that ushered in a new era of radiation-based medical diagnosis and treatment, Physics, Guy’s and St Thomas’ thereby giving rise to the modern medical physics profession. -
NASA Goddard Space Flight Center Laboratory for High Energy Astrophysics Greenbelt, Maryland 20771
1 NASA Goddard Space Flight Center Laboratory for High Energy Astrophysics Greenbelt, Maryland 20771 This report covers the period from July 1, 2002 to June Stephen Henderson, Hans Krimm, John Krizmanic, Jeongin 30, 2003. Lee, John Lehan, James Lochner, Thomas McGlynn, Paul This Laboratory’s scientific research is directed toward McNamara, Alex Moiseev, Koji Mukai, James Reeves, Na- experimental and theoretical investigations in the areas of dine Saudraix, Chris Shrader, Steven Snowden, Yang Soong, X-ray, gamma-ray, gravitational wave and cosmic-ray astro- Martin Still, Steve Sturner, and Vigdor Teplitz. physics. The range of interests of the scientists includes the The following investigators are University of Maryland Sun and the solar system, stellar objects, binary systems, Scientists: Drs. Keith Arnaud, David Band ͑UMBC͒, Simon neutron stars, black holes, the interstellar medium, normal Bandler, Patricia Boyd ͑UMBC͒, John Cannizzo ͑UMBC͒, and active galaxies, galaxy clusters, cosmic ray particles, David Davis ͑UMBC͒, Ian George ͑UMBC͒, Masaharu gravitational wave astrophysics, extragalactic background ra- Hirayama ͑UMBC͒, Una Hwang, Yasushi Ikebe ͑UMBC͒, diation, and cosmology. Scientists and engineers in the Kip Kuntz ͑UMBC͒, Mark Lindeman, Michael Loewenstein, Laboratory also serve the scientific community, including Craig Markwardt, Julie McEnery ͑UMBC͒, Igor Moskalenko project support such as acting as project scientists and pro- ͑UMBC͒, Chee Ng, Patrick Palmeri, Dirk Petry ͑UMBC͒, viding technical assistance for various space missions. Also Christopher Reynolds, Ian Richardson, and Jane Turner at any one time, there are typically between ten and fifteen ͑UMBC͒. graduate students involved in Ph.D. research work in this Visiting scientists from other institutions: Drs. Hilary Laboratory. -
A Cultural History of Physics
Károly Simonyi A Cultural History of Physics Translated by David Kramer Originally published in Hungarian as A fizika kultûrtörténete, Fourth Edition, Akadémiai Kiadó, Budapest, 1998, and published in German as Kulturgeschichte der Physik, Third Edition, Verlag Harri Deutsch, Frankfurt am Main, 2001. First Hungarian edition 1978. CRC Press Taylor & Francis Group 6000 Broken Sound Parkway NW, Suite 300 Boca Raton, FL 33487-2742 © 2012 by Taylor & Francis Group, LLC CRC Press is an imprint of Taylor & Francis Group, an Informa business No claim to original U.S. Government works Printed in the United States of America on acid-free paper Version Date: 20111110 International Standard Book Number: 978-1-56881-329-5 (Hardback) This book contains information obtained from authentic and highly regarded sources. Reasonable efforts have been made to publish reliable data and information, but the author and publisher cannot assume responsibility for the validity of all materials or the consequences of their use. The authors and publishers have attempted to trace the copyright holders of all material reproduced in this publication and apologize to copyright holders if permission to publish in this form has not been obtained. If any copyright material has not been acknowl- edged please write and let us know so we may rectify in any future reprint. Except as permitted under U.S. Copyright Law, no part of this book may be reprinted, reproduced, transmitted, or utilized in any form by any electronic, mechanical, or other means, now known or hereafter invented, including photocopying, microfilming, and recording, or in any information storage or retrieval system, without written permission from the publishers.