Concerning Relativity Books. Published in June 2013 INTERVIEW WITH
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Samuel Goudsmit
NATIONAL ACADEMY OF SCIENCES SAMUEL ABRAHAM GOUDSMIT 1 9 0 2 — 1 9 7 8 A Biographical Memoir by BENJAMIN BEDERSON Any opinions expressed in this memoir are those of the author and do not necessarily reflect the views of the National Academy of Sciences. Biographical Memoir COPYRIGHT 2008 NATIONAL ACADEMY OF SCIENCES WASHINGTON, D.C. Photograph courtesy Brookhaven National Laboratory. SAMUEL ABRAHAM GOUDSMIT July 11, 1902–December 4, 1978 BY BENJAMIN BEDERSON AM GOUDSMIT LED A CAREER that touched many aspects of S20th-century physics and its impact on society. He started his professional life in Holland during the earliest days of quantum mechanics as a student of Paul Ehrenfest. In 1925 together with his fellow graduate student George Uhlenbeck he postulated that in addition to mass and charge the electron possessed a further intrinsic property, internal angular mo- mentum, that is, spin. This inspiration furnished the missing link that explained the existence of multiple spectroscopic lines in atomic spectra, resulting in the final triumph of the then struggling birth of quantum mechanics. In 1927 he and Uhlenbeck together moved to the United States where they continued their physics careers until death. In a rough way Goudsmit’s career can be divided into several separate parts: first in Holland, strictly as a theorist, where he achieved very early success, and then at the University of Michigan, where he worked in the thriving field of preci- sion spectroscopy, concerning himself with the influence of nuclear magnetism on atomic spectra. In 1944 he became the scientific leader of the Alsos Mission, whose aim was to determine the progress Germans had made in the development of nuclear weapons during World War II. -
A Brief Historical Perspective on the Consistent Histories Interpretation
A Brief Historical Perspective on the Consistent Histories Interpretation of Quantum Mechanics Gustavo Rodrigues Rocha1,4, Dean Rickles2,4, and Florian J. Boge3,4 1 Department of Physics, Universidade Estadual de Feira de Santana (UEFS), Feira de Santana, Brazil 2History and Philosophy of Science, University of Sydney, Sydney, Australia 3Interdisciplinary Centre for Science and Technology Studies (IZWT), Wuppertal University, Wuppertal, Germany 4Stellenbosch Institute for Advanced Study (STIAS), Wallenberg Research Centre at Stellenbosch University, Stellenbosch 7600, South Africa Contents 1Introduction...................................... 2 2 The Formalism of the Consistent Histories Approach . ............ 3 2.1HistorySpaces................................... 3 2.2 Consistency, Compatibility, and Grain . ......... 5 2.3Decoherence ..................................... 6 3 Interpreting and Understanding the Formalism in Historical Context . 8 3.1 Single-Framework Rule and Realm-Dependent Reality: From Method to Reality andBack....................................... 8 arXiv:2103.05280v1 [physics.hist-ph] 9 Mar 2021 3.2 Information, Formalization, and the Emergence of Structural Objectivity . 10 3.3 Cybernetics and Measurement: From von Neumann and the Cybernetics Group to theSantaFeInstitute................................ 11 1 4 Robert Griffiths and Roland Omn`es: Context and Logic . 17 5 Decoherent Histories: Consistent Histories A` La Gell-Mann and Hartle . 19 6Conclusion ........................................ 25 1 Introduction Developed, -
The Boundaries of Nature: Special & General Relativity and Quantum
“The Boundaries of Nature: Special & General Relativity and Quantum Mechanics, A Second Course in Physics” Edwin F. Taylor's acceptance speech for the 1998 Oersted medal presented by the American Association of Physics Teachers, 6 January 1998 Edwin F. Taylor Center for Innovation in Learning, Carnegie Mellon University, Pittsburgh, PA 15213 (Now at 22 Hopkins Road, Arlington, MA 02476-8109, email [email protected] , web http://www.artsaxis.com/eftaylor/ ) ABSTRACT Public hunger for relativity and quantum mechanics is insatiable, and we should use it selectively but shamelessly to attract students, most of whom will not become physics majors, but all of whom can experience "deep physics." Science, engineering, and mathematics students, indeed anyone comfortable with calculus, can now delve deeply into special and general relativity and quantum mechanics. Big chunks of general relativity require only calculus if one starts with the metric describing spacetime around Earth or black hole. Expressions for energy and angular momentum follow, along with orbit predictions for particles and light. Feynman's Sum Over Paths quantum theory simply commands the electron: Explore all paths. Students can model this command with the computer, pointing and clicking to tell the electron which paths to explore; wave functions and bound states arise naturally. A second full year course in physics covering special relativity, general relativity, and quantum mechanics would have wide appeal -- and might also lead to significant advancements in upper-level courses for the physics major. © 1998 American Association of Physics Teachers INTRODUCTION It is easy to feel intimidated by those who have in the past received the Oersted Medal, especially those with whom I have worked closely in the enterprise of physics teaching: Edward M. -
Ginling College, the University of Michigan and the Barbour Scholarship
Ginling College, the University of Michigan and the Barbour Scholarship Rosalinda Xiong United World College of Southeast Asia Singapore, 528704 Abstract Ginling College (“Ginling”) was the first institution of higher learning in China to grant bachelor’s degrees to women. Located in Nanking (now Nanjing) and founded in 1915 by western missionaries, Ginling had already graduated nearly 1,000 women when it merged with the University of Nanking in 1951 to become National Ginling University. The University of Michigan (“Michigan”) has had a long history of exchange with Ginling. During Ginling’s first 36 years of operation, Michigan graduates and faculty taught Chinese women at Ginling, and Ginlingers furthered their studies at Michigan through the Barbour Scholarship. This paper highlights the connection between Ginling and Michigan by profiling some of the significant people and events that shaped this unique relationship. It begins by introducing six Michigan graduates and faculty who taught at Ginling. Next we look at the 21 Ginlingers who studied at Michigan through the Barbour Scholarship (including 8 Barbour Scholars from Ginling who were awarded doctorate degrees), and their status after returning to China. Finally, we consider the lives of prominent Chinese women scholars from Ginling who changed China, such as Dr. Wu Yi-fang, a member of Ginling’s first graduating class and, later, its second president; and Miss Wu Ching-yi, who witnessed the brutality of the Rape of Nanking and later worked with Miss Minnie Vautrin to help refugees in Ginling Refugee Camp. Between 2015 and 2017, Ginling College celebrates the centennial anniversary of its founding; and the University of Michigan marks both its bicentennial and the hundredth anniversary of the Barbour Gift, the source of the Barbour Scholarship. -
Physics Today
Physics Today Observant Readers Take the Measure of Novel Approaches to Quantum Theory; Some Get Bohmed Murray Gell‐Mann, James Hahtle, Robert B. Griffiths, Anton Zeilinger, Robert T. Nachtrieb, James L. Anderson, Allen C. Dotson, William G. Hoover, Henry M. Bradford, and Sheldon Goldstein Citation: Physics Today 52(2), 11 (1999); doi: 10.1063/1.882512 View online: http://dx.doi.org/10.1063/1.882512 View Table of Contents: http://scitation.aip.org/content/aip/magazine/physicstoday/52/2?ver=pdfcov Published by the AIP Publishing This article is copyrighted as indicated in the article. Reuse of AIP content is subject to the terms at: http://scitation.aip.org/termsconditions. Downloaded to IP: 131.215.225.131 On: Mon, 24 Aug 2015 23:19:45 LETTERS Observant Readers Take the Measure of Novel Approaches to Quantum Theory; Some Get Bohmed n "Quantum Theory without Ob- beit discrete, intervals of time. How- DH, if two such quantities at the I servers—Part One" (PHYSICS TODAY, ever, he seems to think that we start same time do not commute, measure- March 1998, page 42), Sheldon Gold- with the union of many different fam- ments of them have to take place in stein discusses our work on the deco- ilies (with the possibility of inconsis- different alternative histories of the herent histories (DH) approach to tencies in statements connecting the universe.2 Our work is not com- quantum mechanics and the related probabilities of occurrence of various pletely finished, but the research work of Robert Griffiths and Roland histories) and are trying to find con- is not plagued by inconsistencies. -
A Contribuição De Chien Shiung Wu Para a Teoria Quântica
UNIVERSIDADE FEDERAL DA BAHIA UNIVERSIDADE ESTADUAL DE FEIRA DE SANTANA PROGRAMA DE PÓS-GRADUAÇÃO EM ENSINO, FILOSOFIA E HISTÓRIA DAS CIÊNCIAS ANGEVALDO MENEZES MAIA FILHO PARA UMA HISTÓRIA DAS MULHERES NA CIÊNCIA: A CONTRIBUIÇÃO DE CHIEN SHIUNG WU PARA A TEORIA QUÂNTICA Salvador 2018 ANGEVALDO MENEZES MAIA FILHO PARA UMA HISTÓRIA DAS MULHERES NA CIÊNCIA: A CONTRIBUIÇÃO DE CHIEN SHIUNG WU PARA A TEORIA QUÂNTICA Dissertação apresentada ao Programa de Pós- Graduação em Ensino, Filosofia e História das Ciências, da Universidade Federal da Bahia e da Universidade Estadual de Feira de Santana como requisito parcial para a obtenção do título de Mestre em Ensino, Filosofia e História das Ciências. Orientadora: Profa. Dra. Indianara Lima Silva Salvador 2018 ANGEVALDO MENEZES MAIA FILHO PARA UMA HISTÓRIA DAS MULHERES NA CIÊNCIA: A CONTRIBUIÇÃO DE CHIEN SHIUNG WU PARA A TEORIA QUÂNTICA Dissertação apresentada como requisito parcial para obtenção do grau de mestre em 19 de abril de 2018, Programa de Pós-Graduação em Ensino, Filosofia e História das Ciências, da Universidade Federal da Bahia e da Universidade Estadual de Feira de Santana. 19 de abril de 2018 Banca Examinadora _______________________________________________ Professora Doutora Indianara Lima Silva _______________________________________________ Professora Doutora Maria Margaret Lopes _______________________________________________ Professor Doutor Olival Freire Júnior AGRADECIMENTOS Como não poderia deixar de ser, os agradecimentos revelam o quão importante são as pessoas que nos cercam e o quanto pode ser difícil, no meu caso, absolutamente impossível, realizar um trabalho individualmente. Agradeço a Josenice Assunção Maia e Angevaldo Maia, pessoas que tive a sorte de ter enquanto genitores me apoiando incondicionalmente desde sempre, confiando e acreditando nas minhas escolhas, a maior e inesgotável fonte de amor que pude encontrar na vida. -
Orthodoxies on the Interpretation of Quantum Theory: the Case of the Consistent History Approach
Orthodoxies on the Interpretation of Quantum Theory: The Case of the Consistent History Approach Olival Freire Jr. Universidade Federal da Bahia, Brazil Talk’s outline: Introduction – on different meanings of quantum orthodoxy Consistent history approach – a brief presentation Has there been the birth of a new orthodoxy? The reception of the consistent history approach A short conclusion Jeffrey Bub – Interpreting the quantum world, Cambridge University Press, 1997. For most physicists, the measurement problem of quantum mechanics would hardly rate as even a ‘small cloud’ on the horizon. The standard view is that Bohr had it more or less right, and that anyone willing to waste a little time on the subject could easily straighten out the sort of muddle philosophers might get themselves into. There seems to be a growing consensus that a modern, definitive version of the Copenhagen interpretation has emerged, in terms of which the Bohr-Einstein debate can be seen as a rather old-fashioned way of dealing with issues that are now much more clearly understood. Jeffrey Bub (1997, 212) Indeed, Bub introduced the concept of orthodoxy in four different ways: “For most physicists, the measurement problem of quantum mechanics would hardly rate as even a ‘small cloud’ on the horizon.” #1 “the orthodox (Dirac-von Neumann) interpretation principle (the ‘eigenvalue-eigenstate link).” #2 Bohr’s ‘Copenhagen Interpretation.’ #3 New orthodoxy as the mix of several strands: environment-induced decoherence, elements of Everett’s ‘relative state’ formulation, and the notion of ‘consistent histories.” Omnès as its spokesman. #4 Thus, the issue of historical and practical interest seems to be: Is the “new orthodoxy”, meaning #4 (the consistent history approach), resuscitating orthodoxy meaning #1? If this be the case, such a symbiosis may have been harmful to the development of the research on the foundations of quantum mechanics. -
Stephen Hawking (1942-2018)
1 Stephen Hawking (1942-2018) Towards a Complete Understanding of the Universe [1] James Hartle University of California, Santa Barbara and Santa Fe Institute Stephen Hawking overcame the limitations of a debilitating disease to make major contributions to science. He did this through remarkable persistence, determination, conviction, courage, and will. He was supported in this by his family, his students, and his colleagues. Stephen said “My goal is simple. It is a complete understanding of the universe.” Stephen’s many contributions to science moved us significantly toward that goal. Much of his work was in two major areas — cosmology and the physics of black holes. I will only mention one contribution in each that stands out — his work on the beginning of the universe and his work on the end of black holes [2]. The Beginning of the Universe: Stephen’s Ph.D. advisor Dennis Sciama started him working on cosmology. An important question in the ’60s was: “Did the universe have a beginning?” Observations and the Einstein equation suggested that the early universe was very hot. But did the universe have a beginning or was it first big and then arXiv:1805.03746v1 [physics.hist-ph] 9 May 2018 contracted, heated, and then re-expanded? The singularity theorems worked out by Stephen and Roger Penrose settled the matter at the level of classical gravitational physics. The universe did have a beginning in a big bang of infinite temperature and density before which we can not not see, and at which the classical Einstein equation breaks down. Much of our confidence that there was a big bang rests on these theorems. -
An Exchange of Letters in PHYSICS TODAY on Quantum Theory Without Observers
See discussions, stats, and author profiles for this publication at: https://www.researchgate.net/publication/238958172 Observant Readers Take the Measure of Novel Approaches to Quantum Theory; Some Get Bohmed Article in Physics Today · February 1999 DOI: 10.1063/1.882512 CITATIONS READS 6 56 9 authors, including: Sheldon Goldstein Robert B. Griffiths Rutgers, The State University of New Jersey Carnegie Mellon University 187 PUBLICATIONS 7,521 CITATIONS 193 PUBLICATIONS 15,690 CITATIONS SEE PROFILE SEE PROFILE James L. Anderson Stevens Institute of Technology 81 PUBLICATIONS 2,728 CITATIONS SEE PROFILE Some of the authors of this publication are also working on these related projects: Gravitational Radiation and Radiation Reaction Research View project Noisy quantum channel capacity View project All content following this page was uploaded by Sheldon Goldstein on 12 July 2015. The user has requested enhancement of the downloaded file. An Exchange of Letters in PHYSICS TODAY on Quantum Theory Without Observers February 1999 In “Quantum Theory without Observers—Part One” (PHYSICS TODAY, March 1998, page 42), Sheldon Goldstein discusses our work on the decoherent histories (DH) approach to quantum mechanics and the related work of Robert Griffiths and Roland Omn`es. He describes correctly many aspects of the research and makes a number of favor- able remarks, such as “it seems likely that the program of DH can be brought successfully to completion.” However, he seems to have misunderstood one important point, and as aresulthemistakenlyattributescertain“inconsistencies”totheprogramatitspresent stage. We always consider a “realm”—a set of mutually exclusive decoherent histories with probabilities adding to one—and we typically impose some further conditions on a given realm. -
John Archibald Wheeler 1911 – 2008
John Archibald Wheeler 1911 – 2008 Peter Aufmuth Albert-Einstein-Institut Institut für Gravitationsphysik Leibniz Universität Hannover 9. Juli 2008 Kollegen über Wheeler Max Tegmark Die Geschichte wird JAW als einen Einige seiner Konzepte der überragenden sind so radikal, daß man Geister des 20. ihnen nicht gerecht wird, Jahrhunderts wenn man sie beurteilen. „revolutionär“ nennt. Für mich war er der letzte Titan, der einzige noch lebende Superheld der Physik. Paul C.W. Davies Anton Zeilinger Leben & Werk Jugend & Studium Geb. am 9. Juli 1911 in Jackson, FL als erstes von vier Kindern. Eltern: Joseph & Mabel Wheeler (Bibliothekar & Hausfrau). Häufige Umzüge: Florida, Kalifornien, Ohio, Washington, D.C., Maryland und Vermont. JAW beginnt das Studium an der Johns Hopkins University mit 16 und promoviert mit 21 Jahren bei Karl Ferdinand Herzfeld. „Dispersion and Absorption of He“ Dissertation 1932; Phys. Rev. (Jan. 1933) Mit 27 Jahren wird er als Professor nach Princeton berufen. Leben & Werk Akademische Karriere 1938 – 76 Prof. of Physics, Princeton University 1976 – 86 Center for Theoretical Physics University of Texas, Austin seit 1986 Joseph Henry Prof. of Physics Emeritus Princeton University Princeton Austin Leben & Werk Wissenschaftliche Karriere 1933 – 34 Arbeit mit Gegory Breit, NYU 1934 – 35 Arbeit mit Bohr, Kopenhagen 1935 – 38 Assistent Prof., UNC 1937 – 38 Arbeit mit Edward Teller 1938 – 39 Arbeit mit Willis Lamb 1945 Gründer & Direktor des Cosmic Ray Lab, Princeton 1952 – 55 Diskussionen mit Einstein Mitgliedschaften: American Physical Society (Präsident) American Philosophical Society Royal Academy Accademia Nazionale dei Lincei Royal Academy of Sciences Leben & Werk Auszeichnungen Enrico Fermi Award 1968 Franklin Medal 1969 National Medal of Science 1970 Niels Bohr Int. -
Events in Science, Mathematics, and Technology | Version 3.0
EVENTS IN SCIENCE, MATHEMATICS, AND TECHNOLOGY | VERSION 3.0 William Nielsen Brandt | [email protected] Classical Mechanics -260 Archimedes mathematically works out the principle of the lever and discovers the principle of buoyancy 60 Hero of Alexandria writes Metrica, Mechanics, and Pneumatics 1490 Leonardo da Vinci describ es capillary action 1581 Galileo Galilei notices the timekeeping prop erty of the p endulum 1589 Galileo Galilei uses balls rolling on inclined planes to show that di erentweights fall with the same acceleration 1638 Galileo Galilei publishes Dialogues Concerning Two New Sciences 1658 Christian Huygens exp erimentally discovers that balls placed anywhere inside an inverted cycloid reach the lowest p oint of the cycloid in the same time and thereby exp erimentally shows that the cycloid is the iso chrone 1668 John Wallis suggests the law of conservation of momentum 1687 Isaac Newton publishes his Principia Mathematica 1690 James Bernoulli shows that the cycloid is the solution to the iso chrone problem 1691 Johann Bernoulli shows that a chain freely susp ended from two p oints will form a catenary 1691 James Bernoulli shows that the catenary curve has the lowest center of gravity that anychain hung from two xed p oints can have 1696 Johann Bernoulli shows that the cycloid is the solution to the brachisto chrone problem 1714 Bro ok Taylor derives the fundamental frequency of a stretched vibrating string in terms of its tension and mass p er unit length by solving an ordinary di erential equation 1733 Daniel Bernoulli -
FOR IMMEDIATE RELEASE Nobel Laureate George F. Smoot Recognized for Outstanding Leadership in Physics Education
FOR IMMEDIATE RELEASE College Park, Maryland, United States, November 19, 2008 Nobel Laureate George F. Smoot Recognized for Outstanding Leadership in Physics Education The American Association of Physics Teachers (AAPT) announced today that the Oersted Medal will be awarded to George F. Smoot, Nobel Laureate, an astrophysicist at Lawrence Berkeley National Laboratory since 1974 and a University of California at Berkeley physics professor since 1994, in recognition of his outstanding, widespread, and lasting impact on the teaching of physics. The Oersted Medal will be presented to Dr. Smoot at a Ceremonial Session of the AAPT Winter Meeting in Chicago, Illinois, on Saturday, February 14, 2009. Following the presentation, Dr. Smoot will deliver his keynote address titled, “The History and Fate of the Universe.” Regarding the award, Smoot stated, “ Thank you for this esteemed award. I am honored to be part of this recognized group of scientists. It is special to me since I recently taught my freshman physics class about Oersted’s discovery that electric currents cause magnetic fields. It is wonderful to show the relation between teaching and research. The past two years have been very memorable and exciting for me, and this award is part of that process. I hope that my contribution will help pave the way for the next generation and for their teachers.’’ Dr. Harvey Leff, Chairman, AAPT Awards Committee, said, “It is a great honor to present the Oersted Medal to Dr. George Smoot, who has measured properties of the universe as it existed nearly 14 billion years ago. His detailed study of fluctuations in the cosmic background radiation has led to an understanding of why galaxies formed as they did.