Reposs #9: the Early Reception of Bohr's Atomic Theory (1913-1915
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Warburg Effect(S)—A Biographical Sketch of Otto Warburg and His Impacts on Tumor Metabolism Angela M
Otto Cancer & Metabolism (2016) 4:5 DOI 10.1186/s40170-016-0145-9 REVIEW Open Access Warburg effect(s)—a biographical sketch of Otto Warburg and his impacts on tumor metabolism Angela M. Otto Abstract Virtually everyone working in cancer research is familiar with the “Warburg effect”, i.e., anaerobic glycolysis in the presence of oxygen in tumor cells. However, few people nowadays are aware of what lead Otto Warburg to the discovery of this observation and how his other scientific contributions are seminal to our present knowledge of metabolic and energetic processes in cells. Since science is a human endeavor, and a scientist is imbedded in a network of social and academic contacts, it is worth taking a glimpse into the biography of Otto Warburg to illustrate some of these influences and the historical landmarks in his life. His creative and innovative thinking and his experimental virtuosity set the framework for his scientific achievements, which were pioneering not only for cancer research. Here, I shall allude to the prestigious family background in imperial Germany; his relationships to Einstein, Meyerhof, Krebs, and other Nobel and notable scientists; his innovative technical developments and their applications in the advancement of biomedical sciences, including the manometer, tissue slicing, and cell cultivation. The latter were experimental prerequisites for the first metabolic measurements with tumor cells in the 1920s. In the 1930s–1940s, he improved spectrophotometry for chemical analysis and developed the optical tests for measuring activities of glycolytic enzymes. Warburg’s reputation brought him invitations to the USA and contacts with the Rockefeller Foundation; he received the Nobel Prize in 1931. -
Philosophical Magazine Vol
Philosophical Magazine Vol. 92, Nos. 1–3, 1–21 January 2012, 353–361 Exploring models of associative memory via cavity quantum electrodynamics Sarang Gopalakrishnana, Benjamin L. Levb and Paul M. Goldbartc* aDepartment of Physics, University of Illinois at Urbana-Champaign, 1110 West Green Street Urbana, Illinois 61801, USA; bDepartments of Applied Physics and Physics and E. L. Ginzton Laboratory, Stanford University, Stanford, CA 94305, USA; cSchool of Physics, Georgia Institute of Technology, 837 State Street, Atlanta, GA 30332, USA (Received 2 August 2011; final version received 24 October 2011) Photons in multimode optical cavities can be used to mediate tailored interactions between atoms confined in the cavities. For atoms possessing multiple internal (i.e., ‘‘spin’’) states, the spin–spin interactions mediated by the cavity are analogous in structure to the Ruderman–Kittel–Kasuya– Yosida (RKKY) interaction between localized spins in metals. Thus, in particular, it is possible to use atoms in cavities to realize models of frustrated and/or disordered spin systems, including models that can be mapped on to the Hopfield network model and related models of associative memory. We explain how this realization of models of associative memory comes about and discuss ways in which the properties of these models can be probed in a cavity-based setting. Keywords: disordered systems; magnetism; statistical physics; ultracold atoms; neural networks; spin glasses 1. Introductory remarks Since the development of laser cooling and trapping, a -
Experiencing Hubble
PRESCOTT ASTRONOMY CLUB PRESENTS EXPERIENCING HUBBLE John Carter August 7, 2019 GET OUT LOOK UP • When Galaxies Collide https://www.youtube.com/watch?v=HP3x7TgvgR8 • How Hubble Images Get Color https://www.youtube.com/watch? time_continue=3&v=WSG0MnmUsEY Experiencing Hubble Sagittarius Star Cloud 1. 12,000 stars 2. ½ percent of full Moon area. 3. Not one star in the image can be seen by the naked eye. 4. Color of star reflects its surface temperature. Eagle Nebula. M 16 1. Messier 16 is a conspicuous region of active star formation, appearing in the constellation Serpens Cauda. This giant cloud of interstellar gas and dust is commonly known as the Eagle Nebula, and has already created a cluster of young stars. The nebula is also referred to the Star Queen Nebula and as IC 4703; the cluster is NGC 6611. With an overall visual magnitude of 6.4, and an apparent diameter of 7', the Eagle Nebula's star cluster is best seen with low power telescopes. The brightest star in the cluster has an apparent magnitude of +8.24, easily visible with good binoculars. A 4" scope reveals about 20 stars in an uneven background of fainter stars and nebulosity; three nebulous concentrations can be glimpsed under good conditions. Under very good conditions, suggestions of dark obscuring matter can be seen to the north of the cluster. In an 8" telescope at low power, M 16 is an impressive object. The nebula extends much farther out, to a diameter of over 30'. It is filled with dark regions and globules, including a peculiar dark column and a luminous rim around the cluster. -
Shs-17-2018-14.Pdf
Science beyond borders Nobukata Nagasawa ORCID 0000-0002-9658-7680 Emeritus Professor of University of Tokyo [email protected] On social and psychological aspects of a negligible reception of Natanson’s article of 1911 in the early history of quantum statistics Abstract Possible reasons are studied why Ladislas (Władysław) Natanson’s paper on the statistical theory of radiation, published in 1911 both in English and in the German translation, was not cited properly in the early history of quantum statistics by outstanding scientists, such as Arnold Sommerfeld, Paul Ehrenfest, Satyendra Nath Bose and Albert Einstein. The social and psychological aspects are discussed as back- ground to many so far discussions on the academic evaluation of his theory. In order to avoid in the future such Natansonian cases of very limited reception of valuable scientific works, it is pro- posed to introduce a digital tag in which all the information of PUBLICATION e-ISSN 2543-702X INFO ISSN 2451-3202 DIAMOND OPEN ACCESS CITATION Nagasawa, Nobukata 2018: On social and psychological aspects of a negligible reception of Natanson’s article of 1911 in the early history of quantum statistics. Studia Historiae Scientiarum 17, pp. 391–419. Available online: https://doi.org/10.4467/2543702XSHS.18.014.9334. ARCHIVE RECEIVED: 13.06.2017 LICENSE POLICY ACCEPTED: 12.09.2018 Green SHERPA / PUBLISHED ONLINE: 12.12.2018 RoMEO Colour WWW http://www.ejournals.eu/sj/index.php/SHS/; http://pau.krakow.pl/Studia-Historiae-Scientiarum/ Nobukata Nagasawa On social and psychological aspects of a negligible reception... relevant papers published so far should be automatically accu- mulated and updated. -
President's Message
Journal of the Northern Sydney Astronomical Society Inc. February 2019 In this issue President’s Message Page 1: President’s message Editorial i everyone. Object of the Month as it had been an idea Page 2: Results of the Photo HWhat a magnificent summer! waiting for someone to bring it to life for Competition It seems ages since the lovely summer days some time. Page 5: Results of the Article have landed on our holiday period in such This past two months’ contributions have Competition a comprehensive way. It has been a great been interesting and seen some wonderful Page 7: The Jupiter/Venus Conjunction holiday period for me and I hope you have images come to life. all had such a great time as I have had. It showcases the skills that some of our The last month’s images and videos I am equally pleased to see the Reflections members have and a big congratulation to of Wirtanen 46P comet, along with magazine has had a resurgence and I Kym Haines, the winner for this month, this month’s incredible photo of M42 encourage everyone to take an interest in Phil Angilley and Daniel Patos, the runner- exemplify the talents that can be found it. ups, for their excellent work. amongst our club members. We are expanding the source of A quick shout out to some upcoming contributions for the magazine with the Kym’s M42 photo as seen on page 2 is events. inclusion of the Object of the Month and magnificent and the colours and framing In April we will be running our New other items of interest to our community. -
On Max Born's Vorlesungen ¨Uber Atommechanik, Erster Band
On Max Born’s Vorlesungen uber¨ Atommechanik, Erster Band Domenico Giulini Institute for Theoretical Physics, University of Hannover Appelstrasse 2, D-30167 Hannover, Germany and Center of Applied Space Technology and Microgravity (ZARM), University of Bremen, Am Fallturm 1, D-28359 Bremen, Germany. [email protected] Abstract A little more than half a year before Matrix Mechanics was born, Max Born finished his book Vorlesungen uber¨ Atommechanik, Erster Band, which is a state-of-the-art presentation of Bohr-Sommerfeld quantisation. This book, which today seems almost forgotten, is remarkable for its epistemological as well as technical aspects. Here I wish to highlight one aspect in each of these two categories, the first being concerned with the roleˆ of axiomatisation in the heuristics of physics, the second with the problem of quantisation proper be- fore Heisenberg and Schrodinger.¨ This paper is a contribution to the project History and Foundations of Quantum Physics of the Max Planck Institute for the History of Sciences in Berlin and will appear in the book Research and Pedagogy. The History of Quantum Physics through its Textbooks, edited by M. Badino and J. Navarro. Contents 1 Outline 2 2 Structure of the Book 3 3 Born’s pedagogy and the heuristic roleˆ of the deductive/axiomatic method 7 3.1 Sommerfeld versus Born . 7 3.2 A remarkable introduction . 10 4 On technical issues: What is quantisation? 13 5 Einstein’s view 20 6 Final comments 23 1 1 Outline Max Born’s monograph Vorlesungen uber¨ Atommechanik, Erster Band, was pub- lished in 1925 by Springer Verlag (Berlin) as volume II in the Series Struktur der Materie [3]. -
Prof. Walther Ritz
Professor Walther Ritz (1878 – 1909) From Wikipedia, the free encyclopedia: http://en.wikipedia.org/wiki/Walther_Ritz Walther Ritz (b. February 22, 1878 in Sion, Switzerland - d. 7 July 1909 in Göttingen) was a Swiss theoretical physicist. His father, Raphael Ritz, a native of Valais, was a well-known landscape and interior scenes artist. His mother was the daughter of the engineer Noerdlinger of Tübingen. Ritz studied in Zurich and Göttingen. He is most famous for his work with Johannes Rydberg on the Rydberg–Ritz combination principle. Ritz is also known for the variational method named after him, the Ritz method. Ritz died in 1909, at the age of 31. According to Forman's Dictionary of Scientific Biography, Ritz contracted tuberculosis in 1900, which led to his death in 1909. According to Ritz's collected works (Œuvres) the disease was pleurisy. Criticism of Maxwell-Lorentz electromagnetic theory Not so well known is the fact that in 1908 Walter Ritz produced a lengthy criticism of Maxwell-Lorentz electromagnetic theory, in which he contended that the theory's connection with the luminescent ether (see Lorentz ether theory) made it "essentially inappropriate to express the comprehensive laws for the propagation of electrodynamic actions." Walter Ritz pointed out seven problems with Maxwell-Lorentz electromagnetic field equations: 1 Electric and magnetic forces really express relations about space and time and should be replaced with non- instantaneous elementary actions (his emission theory). 2 Advanced potentials don't exist (and their erroneous use led to the Rayleigh-Jeans ultraviolet catastrophe). 3 Localization of energy in the ether is vague. -
Chronological List of Correspondence, 1895–1920
CHRONOLOGICAL LIST OF CORRESPONDENCE, 1895–1920 In this chronological list of correspondence, the volume and document numbers follow each name. Documents abstracted in the calendars are listed in the Alphabetical List of Texts in this volume. 1895 13 or 20 Mar To Mileva Maric;;, 1, 45 29 Apr To Rosa Winteler, 1, 46 Summer To Caesar Koch, 1, 6 18 May To Rosa Winteler, 1, 47 28 Jul To Julia Niggli, 1, 48 Aug To Rosa Winteler, 5: Vol. 1, 48a 1896 early Aug To Mileva Maric;;, 1, 50 6? Aug To Julia Niggli, 1, 51 21 Apr To Marie Winteler, with a 10? Aug To Mileva Maric;;, 1, 52 postscript by Pauline Einstein, after 10 Aug–before 10 Sep 1,18 From Mileva Maric;;, 1, 53 7 Sep To the Department of Education, 10 Sep To Mileva Maric;;, 1, 54 Canton of Aargau, 1, 20 11 Sep To Julia Niggli, 1, 55 4–25 Nov From Marie Winteler, 1, 29 11 Sep To Pauline Winteler, 1, 56 30 Nov From Marie Winteler, 1, 30 28? Sep To Mileva Maric;;, 1, 57 10 Oct To Mileva Maric;;, 1, 58 1897 19 Oct To the Swiss Federal Council, 1, 60 May? To Pauline Winteler, 1, 34 1900 21 May To Pauline Winteler, 5: Vol. 1, 34a 7 Jun To Pauline Winteler, 1, 35 ? From Mileva Maric;;, 1, 61 after 20 Oct From Mileva Maric;;, 1, 36 28 Feb To the Swiss Department of Foreign Affairs, 1, 62 1898 26 Jun To the Zurich City Council, 1, 65 29? Jul To Mileva Maric;;, 1, 68 ? To Maja Einstein, 1, 38 1 Aug To Mileva Maric;;, 1, 69 2 Jan To Mileva Maric;; [envelope only], 1 6 Aug To Mileva Maric;;, 1, 70 13 Jan To Maja Einstein, 8: Vol. -
The Discovery of Thermodynamics
Philosophical Magazine ISSN: 1478-6435 (Print) 1478-6443 (Online) Journal homepage: https://www.tandfonline.com/loi/tphm20 The discovery of thermodynamics Peter Weinberger To cite this article: Peter Weinberger (2013) The discovery of thermodynamics, Philosophical Magazine, 93:20, 2576-2612, DOI: 10.1080/14786435.2013.784402 To link to this article: https://doi.org/10.1080/14786435.2013.784402 Published online: 09 Apr 2013. Submit your article to this journal Article views: 658 Citing articles: 2 View citing articles Full Terms & Conditions of access and use can be found at https://www.tandfonline.com/action/journalInformation?journalCode=tphm20 Philosophical Magazine, 2013 Vol. 93, No. 20, 2576–2612, http://dx.doi.org/10.1080/14786435.2013.784402 COMMENTARY The discovery of thermodynamics Peter Weinberger∗ Center for Computational Nanoscience, Seilerstätte 10/21, A1010 Vienna, Austria (Received 21 December 2012; final version received 6 March 2013) Based on the idea that a scientific journal is also an “agora” (Greek: market place) for the exchange of ideas and scientific concepts, the history of thermodynamics between 1800 and 1910 as documented in the Philosophical Magazine Archives is uncovered. Famous scientists such as Joule, Thomson (Lord Kelvin), Clau- sius, Maxwell or Boltzmann shared this forum. Not always in the most friendly manner. It is interesting to find out, how difficult it was to describe in a scientific (mathematical) language a phenomenon like “heat”, to see, how long it took to arrive at one of the fundamental principles in physics: entropy. Scientific progress started from the simple rule of Boyle and Mariotte dating from the late eighteenth century and arrived in the twentieth century with the concept of probabilities. -
History of Nonlinear Oscillations Theory in France (1880–1940)
Archimedes 49 New Studies in the History and Philosophy of Science and Technology Jean-Marc Ginoux History of Nonlinear Oscillations Theory in France (1880–1940) History of Nonlinear Oscillations Theory in France (1880–1940) Archimedes NEW STUDIES IN THE HISTORY AND PHILOSOPHY OF SCIENCE AND TECHNOLOGY VOLUME 49 EDITOR JED Z. BUCHWALD, Dreyfuss Professor of History, California Institute of Technology, Pasadena, USA. ASSOCIATE EDITORS FOR MATHEMATICS AND PHYSICAL SCIENCES JEREMY GRAY, The Faculty of Mathematics and Computing, The Open University, UK. TILMAN SAUER, Johannes Gutenberg University Mainz, Germany ASSOCIATE EDITORS FOR BIOLOGICAL SCIENCES SHARON KINGSLAND, Department of History of Science and Technology, Johns Hopkins University, Baltimore, USA. MANFRED LAUBICHLER, Arizona State University, USA ADVISORY BOARD FOR MATHEMATICS, PHYSICAL SCIENCES AND TECHNOLOGY HENK BOS, University of Utrecht, The Netherlands MORDECHAI FEINGOLD, California Institute of Technology, USA ALLAN D. FRANKLIN, University of Colorado at Boulder, USA KOSTAS GAVROGLU, National Technical University of Athens, Greece PAUL HOYNINGEN-HUENE, Leibniz University in Hannover, Germany TREVOR LEVERE, University of Toronto, Canada JESPER LÜTZEN, Copenhagen University, Denmark WILLIAM NEWMAN, Indiana University, Bloomington, USA LAWRENCE PRINCIPE, The Johns Hopkins University, USA JÜRGEN RENN, Max Planck Institute for the History of Science, Germany ALEX ROLAND, Duke University, USA ALAN SHAPIRO, University of Minnesota, USA NOEL SWERDLOW, California Institute of Technology, -
Spectroscopy from 1916 to 1940
PRE-1940 Spectroscopy from 1916 to 1940 Patricia Daukantas uring the first quarter century of The Optical Society (OSA), spectroscopy led to major insights into atomic and molecular physics and paved the way for important practical D applications. Optical spectroscopy existed for decades before the formation of OSA, but it was empirical and descriptive in its nature. Spectroscopists had carefully measured the wavelengths of spectral lines associated with various elements, but the subatomic mechanisms that created these lines were not yet fully understood. Twenty-four years later, as the world lurched toward the second all-encompassing war of the twentieth century, the spectroscopic fingerprints of atoms and molecules had provided vital evidence for the emerging quantum theory. Experimentalists refined their techniques and discovered previously unknown phenomena. Spectroscopy and Quantum Mechanics A few years before OSA was formed, Niels Bohr had proposed his model of the hydrogen atom, which explained the empirical Rydberg formula for the spectral lines of atomic hydrogen, at least to a first approximation. Theodore Lyman completed his investigations of the ultraviolet emission lines of hydrogen, beginning at 1216 Å in 1914. Little happened in spectroscopy during World War I, but the field came raging back shortly after the armistice. In 1919, Arnold Sommerfeld, doctoral adviser to multiple Nobel Laureates, published Atombau und Spektralinien (Atomic Structure and Spectral Lines). William F. Meggers, who would become the 1949–1950 OSA president, opined that “spectroscopists were amazed that our meager knowledge of atomic structure and the origin of spectra could be expanded into such a big book” [1]. The same year, Sommerfeld and another German physicist, Walther Kossel, formulated the displacement law now named after them [1]. -
Ether and Electrons in Relativity Theory (1900-1911) Scott Walter
Ether and electrons in relativity theory (1900-1911) Scott Walter To cite this version: Scott Walter. Ether and electrons in relativity theory (1900-1911). Jaume Navarro. Ether and Moder- nity: The Recalcitrance of an Epistemic Object in the Early Twentieth Century, Oxford University Press, 2018, 9780198797258. hal-01879022 HAL Id: hal-01879022 https://hal.archives-ouvertes.fr/hal-01879022 Submitted on 21 Sep 2018 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Ether and electrons in relativity theory (1900–1911) Scott A. Walter∗ To appear in J. Navarro, ed, Ether and Modernity, 67–87. Oxford: Oxford University Press, 2018 Abstract This chapter discusses the roles of ether and electrons in relativity the- ory. One of the most radical moves made by Albert Einstein was to dismiss the ether from electrodynamics. His fellow physicists felt challenged by Einstein’s view, and they came up with a variety of responses, ranging from enthusiastic approval, to dismissive rejection. Among the naysayers were the electron theorists, who were unanimous in their affirmation of the ether, even if they agreed with other aspects of Einstein’s theory of relativity. The eventual success of the latter theory (circa 1911) owed much to Hermann Minkowski’s idea of four-dimensional spacetime, which was portrayed as a conceptual substitute of sorts for the ether.