A Fundamental, Relativistic, and Irreversible Law of Motion: a Unification of Newton’S Second Law of Motion and the Second Law of Thermodynamics
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Nuclear Technology
Nuclear Technology Joseph A. Angelo, Jr. GREENWOOD PRESS NUCLEAR TECHNOLOGY Sourcebooks in Modern Technology Space Technology Joseph A. Angelo, Jr. Sourcebooks in Modern Technology Nuclear Technology Joseph A. Angelo, Jr. GREENWOOD PRESS Westport, Connecticut • London Library of Congress Cataloging-in-Publication Data Angelo, Joseph A. Nuclear technology / Joseph A. Angelo, Jr. p. cm.—(Sourcebooks in modern technology) Includes index. ISBN 1–57356–336–6 (alk. paper) 1. Nuclear engineering. I. Title. II. Series. TK9145.A55 2004 621.48—dc22 2004011238 British Library Cataloguing in Publication Data is available. Copyright © 2004 by Joseph A. Angelo, Jr. All rights reserved. No portion of this book may be reproduced, by any process or technique, without the express written consent of the publisher. Library of Congress Catalog Card Number: 2004011238 ISBN: 1–57356–336–6 First published in 2004 Greenwood Press, 88 Post Road West, Westport, CT 06881 An imprint of Greenwood Publishing Group, Inc. www.greenwood.com Printed in the United States of America The paper used in this book complies with the Permanent Paper Standard issued by the National Information Standards Organization (Z39.48–1984). 10987654321 To my wife, Joan—a wonderful companion and soul mate Contents Preface ix Chapter 1. History of Nuclear Technology and Science 1 Chapter 2. Chronology of Nuclear Technology 65 Chapter 3. Profiles of Nuclear Technology Pioneers, Visionaries, and Advocates 95 Chapter 4. How Nuclear Technology Works 155 Chapter 5. Impact 315 Chapter 6. Issues 375 Chapter 7. The Future of Nuclear Technology 443 Chapter 8. Glossary of Terms Used in Nuclear Technology 485 Chapter 9. Associations 539 Chapter 10. -
James Clerk Maxwell
James Clerk Maxwell JAMES CLERK MAXWELL Perspectives on his Life and Work Edited by raymond flood mark mccartney and andrew whitaker 3 3 Great Clarendon Street, Oxford, OX2 6DP, United Kingdom Oxford University Press is a department of the University of Oxford. It furthers the University’s objective of excellence in research, scholarship, and education by publishing worldwide. Oxford is a registered trade mark of Oxford University Press in the UK and in certain other countries c Oxford University Press 2014 The moral rights of the authors have been asserted First Edition published in 2014 Impression: 1 All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, without the prior permission in writing of Oxford University Press, or as expressly permitted by law, by licence or under terms agreed with the appropriate reprographics rights organization. Enquiries concerning reproduction outside the scope of the above should be sent to the Rights Department, Oxford University Press, at the address above You must not circulate this work in any other form and you must impose this same condition on any acquirer Published in the United States of America by Oxford University Press 198 Madison Avenue, New York, NY 10016, United States of America British Library Cataloguing in Publication Data Data available Library of Congress Control Number: 2013942195 ISBN 978–0–19–966437–5 Printed and bound by CPI Group (UK) Ltd, Croydon, CR0 4YY Links to third party websites are provided by Oxford in good faith and for information only. -
Radiation Friction: Shedding Light on Dark Energy
The African Review of Physics (2015) 10 :0044 361 Radiation Friction: Shedding Light on Dark Energy Randy Wayne * Laboratory of Natural Philosophy, Section of Plant Biology, School of Integrative Plant Science, Cornell University, Ithaca, NY 14853, USA In 1909, while working on the quantum nature of light, Einstein developed the notion of “radiation friction.” Radiation friction becomes significant when the temperature of the radiation and the velocities of the galaxies moving through it are great. Here I suggest that the decrease in the velocity-dependent radiation friction occurring as a result of the expansion of the universe may be the cause of the observed acceleration of the expansion of the universe. Interestingly, the decrease in the density of light energy and the apparent domination of dark energy, become one and the same. 1. Introduction 2. Results and Discussion Over the past two decades, observations of the I have recently reinterpreted the three crucial tests relationship between the luminosity (m) of type Ia of the General Theory of Relativity [7]: the supernovae and the redshift ( ) of their host precession of the perihelion of Mercury [8], the galaxies have provided strong evidence that the deflection of starlight [9], and the gravitational expansion of the universe is accelerating [1, 2]. The redshift [9] in terms of Euclidean space and cause of the acceleration however remains a Newtonian time. I have also reinterpreted the mystery [3]. Naming one of the possible causes of relativity of simultaneity [10], the optics of moving acceleration “dark energy” may be a first step in bodies [11,12], the inertia of energy [13] and the describing the acceleration [4], but is a panchreston reason charged particles cannot exceed the speed of that gives no deeper understanding to the problem light [14] in terms of the second order relativistic since there is no independent evidence of the Doppler effect occurring in Euclidean space and properties or even the existence of dark energy [5]. -
Great Physicists
Great Physicists Great Physicists The Life and Times of Leading Physicists from Galileo to Hawking William H. Cropper 1 2001 1 Oxford New York Athens Auckland Bangkok Bogota´ Buenos Aires Cape Town Chennai Dar es Salaam Delhi Florence HongKong Istanbul Karachi Kolkata Kuala Lumpur Madrid Melbourne Mexico City Mumbai Nairobi Paris Sao Paulo Shanghai Singapore Taipei Tokyo Toronto Warsaw and associated companies in Berlin Ibadan Copyright ᭧ 2001 by Oxford University Press, Inc. Published by Oxford University Press, Inc. 198 Madison Avenue, New York, New York 10016 Oxford is a registered trademark of Oxford University Press All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, electronic, mechanical, photocopying, recording, or otherwise, without the prior permission of Oxford University Press. Library of Congress Cataloging-in-Publication Data Cropper, William H. Great Physicists: the life and times of leadingphysicists from Galileo to Hawking/ William H. Cropper. p. cm Includes bibliographical references and index. ISBN 0–19–513748–5 1. Physicists—Biography. I. Title. QC15 .C76 2001 530'.092'2—dc21 [B] 2001021611 987654321 Printed in the United States of America on acid-free paper Contents Preface ix Acknowledgments xi I. Mechanics Historical Synopsis 3 1. How the Heavens Go 5 Galileo Galilei 2. A Man Obsessed 18 Isaac Newton II. Thermodynamics Historical Synopsis 41 3. A Tale of Two Revolutions 43 Sadi Carnot 4. On the Dark Side 51 Robert Mayer 5. A Holy Undertaking59 James Joule 6. Unities and a Unifier 71 Hermann Helmholtz 7. The Scientist as Virtuoso 78 William Thomson 8. -
Thermodynamic Physics and the Poetry and Prose of Gerard Manley Hopkins
Georgia State University ScholarWorks @ Georgia State University English Dissertations Department of English 5-11-2015 Literatures of Stress: Thermodynamic Physics and the Poetry and Prose of Gerard Manley Hopkins Thomas Mapes Follow this and additional works at: https://scholarworks.gsu.edu/english_diss Recommended Citation Mapes, Thomas, "Literatures of Stress: Thermodynamic Physics and the Poetry and Prose of Gerard Manley Hopkins." Dissertation, Georgia State University, 2015. https://scholarworks.gsu.edu/english_diss/134 This Dissertation is brought to you for free and open access by the Department of English at ScholarWorks @ Georgia State University. It has been accepted for inclusion in English Dissertations by an authorized administrator of ScholarWorks @ Georgia State University. For more information, please contact [email protected]. LITERATURES OF STRESS: THERMODYNAMIC PHYSICS AND THE POETRY AND PROSE OF GERARD MANLEY HOPKINS by THOMAS MAPES Under the Direction of Paul Schmidt, PhD ABSTRACT This dissertation examines two of the various literatures of energy in Victorian Britain: the scientific literature of the North British school of energy physics, and the poetic and prose literature of Gerard Manley Hopkins. As an interdisciplinary effort, it is intended for several audiences. For readers interested in science history, it offers a history of two terms – stress and strain – central to modern physics. As well, in discussing the ideas of various scientific authors (primarily William John Macquorn Rankine, William Thomson, P.G. Tait, and James Clerk Maxwell), it indicates several contributions these figures made to larger culture. For readers of Hopkins’ poems and prose, this dissertation corresponds with a recent trend in criticism in its estimation of Hopkins as a scientifically informed writer, at least in his years post-Stonyhurst. -
Abstract 1. Introduction 2. Robert Stirling
Stirling Stuff Dr John S. Reid, Department of Physics, Meston Building, University of Aberdeen, Aberdeen AB12 3UE, Scotland Abstract Robert Stirling’s patent for what was essentially a new type of engine to create work from heat was submitted in 1816. Its reception was underwhelming and although the idea was sporadically developed, it was eclipsed by the steam engine and, later, the internal combustion engine. Today, though, the environmentally favourable credentials of the Stirling engine principles are driving a resurgence of interest, with modern designs using modern materials. These themes are woven through a historically based narrative that introduces Robert Stirling and his background, a description of his patent and the principles behind his engine, and discusses the now popular model Stirling engines readily available. These topical models, or alternatives made ‘in house’, form a good platform for investigating some of the thermodynamics governing the performance of engines in general. ---------------------------------------------------------------------------------------------------------------- 1. Introduction 2016 marks the bicentenary of the submission of Robert Stirling’s patent that described heat exchangers and the technology of the Stirling engine. James Watt was still alive in 1816 and his steam engine was gaining a foothold in mines, in mills, in a few goods railways and even in pioneering ‘steamers’. Who needed another new engine from another Scot? The Stirling engine is a markedly different machine from either the earlier steam engine or the later internal combustion engine. For reasons to be explained, after a comparatively obscure two centuries the Stirling engine is attracting new interest, for it has environmentally friendly credentials for an engine. This tribute introduces the man, his patent, the engine and how it is realised in example models readily available on the internet. -
Laplace and the Speed of Sound
Laplace and the Speed of Sound By Bernard S. Finn * OR A CENTURY and a quarter after Isaac Newton initially posed the problem in the Principia, there was a very apparent discrepancy of almost 20 per cent between theoretical and experimental values of the speed of sound. To remedy such an intolerable situation, some, like New- ton, optimistically framed additional hypotheses to make up the difference; others, like J. L. Lagrange, pessimistically confessed the inability of con- temporary science to produce a reasonable explanation. A study of the development of various solutions to this problem provides some interesting insights into the history of science. This is especially true in the case of Pierre Simon, Marquis de Laplace, who got qualitatively to the nub of the matter immediately, but whose quantitative explanation performed some rather spectacular gyrations over the course of two decades and rested at times on both theoretical and experimental grounds which would later be called incorrect. Estimates of the speed of sound based on direct observation existed well before the Newtonian calculation. Francis Bacon suggested that one man stand in a tower and signal with a bell and a light. His companion, some distance away, would observe the time lapse between the two signals, and the speed of sound could be calculated.' We are probably safe in assuming that Bacon never carried out his own experiment. Marin Mersenne, and later Joshua Walker and Newton, obtained respectable results by deter- mining how far they had to stand from a wall in order to obtain an echo in a second or half second of time. -
January/February 2011
ASPB News THE NEWSLETTER OF THE AMERICAN SOCIETY OF PLANT BIOLOGISTS Volume 38, Number 1 January/February 2011 ASPB Members Among Those Honored by Inside This Issue President Obama President’s Letter Save the Date! Plant Biology 2011 Call for Abstracts: Plant Biology 2011 Susan Singer to Edit New ASPB–Wiley-Blackwell Book Series Jim Carrington Next President of Danforth Plant Science Center President Barack Obama poses for a group photo with the recipients of the Presidential Early The Plant Cell’s Teaching Career Award for Scientists and Engineers in the South Court Auditorium of the White House on Tools Garners Gold December 13, 2010. Among the awardees are ASPB members Dominique Bergmann and Award! Magdalena Bezanilla. (See page 9 for full coverage.) OFFICIAL WHITE HoUSE PHOTO BY CHUCK KENNEDY. Honoring Those Who Serve the Mission of ASPB As outlined in our established mission, the Ameri- scientist you’re thinking of served as a mentor who can Society of Plant Biologists was founded to pro- instilled in you a lifelong ambition and dedication mote the growth and development of plant biology, to our science. Or perhaps you envision a rising star to encourage and publish research in plant biology, who already demonstrates excellence early in his or and to promote the interests and growth of the plant her career. ASPB strives to recognize these individu- science discipline. Our members work in aca- als in many ways. One way is a call to service to the demia, government laboratories, and industrial and Society by nomination to ASPB’s Executive Com- commercial environments. -
Elizabeth F. Lewis Phd Thesis
PETER GUTHRIE TAIT NEW INSIGHTS INTO ASPECTS OF HIS LIFE AND WORK; AND ASSOCIATED TOPICS IN THE HISTORY OF MATHEMATICS Elizabeth Faith Lewis A Thesis Submitted for the Degree of PhD at the University of St Andrews 2015 Full metadata for this item is available in St Andrews Research Repository at: http://research-repository.st-andrews.ac.uk/ Please use this identifier to cite or link to this item: http://hdl.handle.net/10023/6330 This item is protected by original copyright PETER GUTHRIE TAIT NEW INSIGHTS INTO ASPECTS OF HIS LIFE AND WORK; AND ASSOCIATED TOPICS IN THE HISTORY OF MATHEMATICS ELIZABETH FAITH LEWIS This thesis is submitted in partial fulfilment for the degree of Ph.D. at the University of St Andrews. 2014 1. Candidate's declarations: I, Elizabeth Faith Lewis, hereby certify that this thesis, which is approximately 59,000 words in length, has been written by me, and that it is the record of work carried out by me, or principally by myself in collaboration with others as acknowledged, and that it has not been submitted in any previous application for a higher degree. I was admitted as a research student in September 2010 and as a candidate for the degree of Ph.D. in September 2010; the higher study for which this is a record was carried out in the University of St Andrews between 2010 and 2014. Signature of candidate ...................................... Date .................... 2. Supervisor's declaration: I hereby certify that the candidate has fulfilled the conditions of the Resolution and Regulations appropriate for the degree of Ph.D. -
Report on the First Quadrennial Technology Review (QTR)
REPORT ON THE FIRST QUADRENNIAL QTR TECHNOLOGY REVIEW September 2011 MESSAGE FROM THE SECRETARY OF ENERGY | I MESSAGE FROM THE SECRETARY OF ENERGY Today, our nation is at a cross road. While we have the world’s greatest innovation ma- chine, countries around the world are moving aggressively to lead in the clean energy economy. We can either lead in the development of the clean energy economy or we CANÏSTANDÏBACKÏANDÏWAITÏFORÏOTHERSÏTOÏMOVEÏlRSTÏTOWARDÏAÏSUSTAINABLEÏENERGYÏFUTUREÏ For the sake of our economic prosperity and our national security, we must lead. The Department of Energy (DOE) plays a central role in that effort by unleashing technologi- cal innovation, which can create new jobs and industries while building a cleaner, more EFlCIENT ÏANDÏMOREÏCOMPETITIVEÏECONOMY Steven Chu, Secretary of the United States $URINGÏTHISÏTIMEÏOFÏHARDÏBUDGETÏCHOICESÏANDÏlSCALÏCHALLENGE ÏWEÏMUSTÏENSUREÏTHATÏOURÏ Department of Energy WORKÏISÏIMPACTFULÏANDÏEFlCIENTÏ4HEÏQUESTIONÏWEÏFACEÏISÏh(OWÏSHOULDÏTHEÏ$EPARTMENTÏ CHOOSEÏAMONGÏTHEÏMANYÏTECHNICALLYÏVIABLEÏACTIVITIESÏITÏCOULDÏPURSUEvÏ4HISÏlRSTÏ1UA- drennial Technology Review (QTR), launched at the recommendation of the President’s Council of Advisors on Science and Technology, lays out the principles I believe must GUIDEÏTHESEÏDIFlCULTÏCHOICESÏÏÏ Traditionally, the Department’s energy strategy has been organized along individual program lines and based on annual budgets. With this QTR, we bind together multiple energy technologies, as well as multiple DOE energy technology programs, in the common purpose of solving our energy challenges. In addition, the QTR provides a multi-year framework for our planning. Energy invest- ments are multi-year, multi-decade investments. Given this time horizon, we need to take a longer view. We also recognize that the Department is not the sole agent of energy transformation. Our efforts must be well coordinated with other federal agencies, state and local governments, and with the private sector, who are the major owners, operators, and inves- tors of the energy system. -
Self Evaluation 2019
Randy Wayne Self-Evaluation 2019 1. What are the central themes and priorities in your research, and what are you most pleased with? As a researcher, I try to ask and answer the most fundamental scientific questions related to how plants transform light energy into food, how plants sense and respond to the physical environment, and how plants respond and develop in time. Specifically I work on the following fundamental scientific questions: what is light, what is gravity, and what is time? I do this by critically analyzing the foundations of relativity and quantum mechanics that have given us the scientific description of light, gravity, and time that is accepted by the consensus. My unique and original work is based on a deep understanding of the history and philosophy of science, a deep need to resolve inconsistencies between standard theories that have been swept under the rug, and on my computational and experimental skills. Stanislaw Ulam said, “Ask not what physics can do for biology, ask what biology can do for physics.” Biophysics is currently populated by people who have moved from physics into biology. However, historically, biologists and physicians, including Thomas Young, Hermann von Helmholtz, Robert Brown, Robert Meyer, and Adolf Fick have had a profound influence on physics and there is still room for a biophysical cell biologist to make an impact. This is because cells live in the world of neglected dimensions between the world of macroscopic physics and the world of microscopic physics. Studying physico- chemical processes in such a world has its advantages and its disadvantages. -
Life: Past, Present and Future
Downloaded from rstb.royalsocietypublishing.org on February 10, 2011 Life: past, present and future Kenneth H. Nealson and Pamela G. Conrad Phil. Trans. R. Soc. Lond. B 1999 354, 1923-1939 doi: 10.1098/rstb.1999.0532 References Article cited in: http://rstb.royalsocietypublishing.org/content/354/1392/1923#related-urls Rapid response Respond to this article http://rstb.royalsocietypublishing.org/letters/submit/royptb;354/1392/1923 Receive free email alerts when new articles cite this article - sign up in the box at the top Email alerting service right-hand corner of the article or click here To subscribe to Phil. Trans. R. Soc. Lond. B go to: http://rstb.royalsocietypublishing.org/subscriptions This journal is © 1999 The Royal Society Downloaded from rstb.royalsocietypublishing.org on February 10, 2011 Life: past, present and future Kenneth H. Nealson and Pamela G. Conrad Jet Propulsion Laboratory, California Institute of Technology, 183^301, 4800 OakGrove Drive, Pasadena, CA 91109, USA ([email protected]) Molecular methods of taxonomy and phylogeny have changed the way in which life on earth is viewed; they have allowed us to transition from a eukaryote-centric (¢ve-kingdoms) view of the planet to one that is peculiarly prokarote-centric, containing three kingdoms, two of which are prokaryotic unicells. These prokaryotes are distinguished from their eukaryotic counterparts by their toughness, tenacity and metabolic diversity. Realization of these features has, in many ways, changed the way we feel about life on earth, about the nature of life past and about the possibility of ¢nding life elsewhere. In essence, the limits of life on this planet have expanded to such a degree that our thoughts of both past and future life have been altered.