Karl Herzfeld Retained Ties with His Family and with the German Physics Community by Occasional Visits to Germany
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Catholic Christian Christian
Religious Scientists (From the Vatican Observatory Website) https://www.vofoundation.org/faith-and-science/religious-scientists/ Many scientists are religious people—men and women of faith—believers in God. This section features some of the religious scientists who appear in different entries on these Faith and Science pages. Some of these scientists are well-known, others less so. Many are Catholic, many are not. Most are Christian, but some are not. Some of these scientists of faith have lived saintly lives. Many scientists who are faith-full tend to describe science as an effort to understand the works of God and thus to grow closer to God. Quite a few describe their work in science almost as a duty they have to seek to improve the lives of their fellow human beings through greater understanding of the world around them. But the people featured here are featured because they are scientists, not because they are saints (even when they are, in fact, saints). Scientists tend to be creative, independent-minded and confident of their ideas. We also maintain a longer listing of scientists of faith who may or may not be discussed on these Faith and Science pages—click here for that listing. Agnesi, Maria Gaetana (1718-1799) Catholic Christian A child prodigy who obtained education and acclaim for her abilities in math and physics, as well as support from Pope Benedict XIV, Agnesi would write an early calculus textbook. She later abandoned her work in mathematics and physics and chose a life of service to those in need. Click here for Vatican Observatory Faith and Science entries about Maria Gaetana Agnesi. -
Sterns Lebensdaten Und Chronologie Seines Wirkens
Sterns Lebensdaten und Chronologie seines Wirkens Diese Chronologie von Otto Sterns Wirken basiert auf folgenden Quellen: 1. Otto Sterns selbst verfassten Lebensläufen, 2. Sterns Briefen und Sterns Publikationen, 3. Sterns Reisepässen 4. Sterns Züricher Interview 1961 5. Dokumenten der Hochschularchive (17.2.1888 bis 17.8.1969) 1888 Geb. 17.2.1888 als Otto Stern in Sohrau/Oberschlesien In allen Lebensläufen und Dokumenten findet man immer nur den VornamenOt- to. Im polizeilichen Führungszeugnis ausgestellt am 12.7.1912 vom königlichen Polizeipräsidium Abt. IV in Breslau wird bei Stern ebenfalls nur der Vorname Otto erwähnt. Nur im Emeritierungsdokument des Carnegie Institutes of Tech- nology wird ein zweiter Vorname Otto M. Stern erwähnt. Vater: Mühlenbesitzer Oskar Stern (*1850–1919) und Mutter Eugenie Stern geb. Rosenthal (*1863–1907) Nach Angabe von Diana Templeton-Killan, der Enkeltochter von Berta Kamm und somit Großnichte von Otto Stern (E-Mail vom 3.12.2015 an Horst Schmidt- Böcking) war Ottos Großvater Abraham Stern. Abraham hatte 5 Kinder mit seiner ersten Frau Nanni Freund. Nanni starb kurz nach der Geburt des fünften Kindes. Bald danach heiratete Abraham Berta Ben- der, mit der er 6 weitere Kinder hatte. Ottos Vater Oskar war das dritte Kind von Berta. Abraham und Nannis erstes Kind war Heinrich Stern (1833–1908). Heinrich hatte 4 Kinder. Das erste Kind war Richard Stern (1865–1911), der Toni Asch © Springer-Verlag GmbH Deutschland 2018 325 H. Schmidt-Böcking, A. Templeton, W. Trageser (Hrsg.), Otto Sterns gesammelte Briefe – Band 1, https://doi.org/10.1007/978-3-662-55735-8 326 Sterns Lebensdaten und Chronologie seines Wirkens heiratete. -
Executive Committee Meeting 6:00 Pm, November 22, 2008 Marriott Rivercenter Hotel
Executive Committee Meeting 6:00 pm, November 22, 2008 Marriott Rivercenter Hotel Attendees: Steve Pope, Lex Smits, Phil Marcus, Ellen Longmire, Juan Lasheras, Anette Hosoi, Laurette Tuckerman, Jim Brasseur, Paul Steen, Minami Yoda, Martin Maxey, Jean Hertzberg, Monica Malouf, Ken Kiger, Sharath Girimaji, Krishnan Mahesh, Gary Leal, Bill Schultz, Andrea Prosperetti, Julian Domaradzki, Jim Duncan, John Foss, PK Yeung, Ann Karagozian, Lance Collins, Kimberly Hill, Peggy Holland, Jason Bardi (AIP) Note: Attachments related to agenda items follow the order of the agenda and are appended to this document. Key Decisions The ExCom voted to move $100k of operating funds to an endowment for a new award. The ExCom voted that a new name (not Otto Laporte) should be chosen for this award. In the coming year, the Award committee (currently the Fluid Dynamics Prize committee) should establish the award criteria, making sure to distinguish the criteria from those associated with the Batchelor prize. The committee should suggest appropriate wording for the award application and make a recommendation on the naming of the award. The ExCom voted to move Newsletter publication to the first weeks of June and December each year. The ExCom voted to continue the Ad Hoc Committee on Media and Public Relations for two more years (through 2010). The ExCom voted that $15,000 per year in 2009 and 2010 be allocated for Media and Public Relations activities. Most of these funds would be applied toward continuing to use AIP media services in support of news releases and Virtual Pressroom activities related to the annual DFD meeting. Meeting Discussion 1. -
Chapter 2 Challenging the Boundaries Between Classical and Quantum Physics: the Case of Optical Dispersion Marta Jordi Taltavull
Chapter 2 Challenging the Boundaries between Classical and Quantum Physics: The Case of Optical Dispersion Marta Jordi Taltavull This paper describes one significant episode in the transition between classical and quantum theories. It analyzes the first theory of optical dispersion that ensued from the extension of Niels Bohr’s quantum model of the atom to other optical phenomena outside of spectroscopy. This theory was initially developed by Peter Debye in 1915 and then was endorsed and extended by Arnold Sommerfeld in 1915 and 1917. The most interesting aspect of the Debye-Sommerfeld theory for the present paper is that it clearly typifies important features of debates concerning the boundaries between classical and quantum physics, focusing on the period from 1913 to the early 1920s. Optical dispersion consisted of splitting white light into different colors be- cause of its change of velocity when passing through a transparent, prismatic medium. From the 1870s onward, it was well known that light was continuously dispersed across the entire spectrum, except at those specific frequencies, charac- teristic of the medium, at which light was completely absorbed. In other words, dispersion and absorption of light were complementary phenomena. From 1872, this behavior was explained using one enduring theoretical representation: the Mitschwingungen model. This model pictured the interaction between light and matter as a continuous process of interaction between waves and particles per- forming induced vibrations, called Mitschwingungen. In 1913, this model conflicted with certain aspects of Bohr’s quantum model of the atom. Contrary to the Mitschwingungen model, Bohr envisioned the ex- change of energy between light and matter as a discrete process, mediated by the emission or absorption of quanta of energy. -
UC San Diego UC San Diego Electronic Theses and Dissertations
UC San Diego UC San Diego Electronic Theses and Dissertations Title The new prophet : Harold C. Urey, scientist, atheist, and defender of religion Permalink https://escholarship.org/uc/item/3j80v92j Author Shindell, Matthew Benjamin Publication Date 2011 Peer reviewed|Thesis/dissertation eScholarship.org Powered by the California Digital Library University of California UNIVERSITY OF CALIFORNIA, SAN DIEGO The New Prophet: Harold C. Urey, Scientist, Atheist, and Defender of Religion A dissertation submitted in partial satisfaction of the requirements for the degree Doctor of Philosophy in History (Science Studies) by Matthew Benjamin Shindell Committee in charge: Professor Naomi Oreskes, Chair Professor Robert Edelman Professor Martha Lampland Professor Charles Thorpe Professor Robert Westman 2011 Copyright Matthew Benjamin Shindell, 2011 All rights reserved. The Dissertation of Matthew Benjamin Shindell is approved, and it is acceptable in quality and form for publication on microfilm and electronically: ___________________________________________________________________ ___________________________________________________________________ ___________________________________________________________________ ___________________________________________________________________ ___________________________________________________________________ Chair University of California, San Diego 2011 iii TABLE OF CONTENTS Signature Page……………………………………………………………………...... iii Table of Contents……………………………………………………………………. iv Acknowledgements…………………………………………………………………. -
Chapter 6 Free Electron Fermi Gas
理学院 物理系 沈嵘 Chapter 6 Free Electron Fermi Gas 6.1 Electron Gas Model and its Ground State 6.2 Thermal Properties of Electron Gas 6.3 Free Electrons in Electric Fields 6.4 Hall Effect 6.5 Thermal Conductivity of Metals 6.6 Failures of the free electron gas model 1 6.1 Electron Gas Model and its Ground State 6.1 Electron Gas Model and its Ground State I. Basic Assumptions of Electron Gas Model Metal: valence electrons → conduction electrons (moving freely) ü The simplest metals are the alkali metals—lithium, sodium, 2 potassium, cesium, and rubidium. 6.1 Electron Gas Model and its Ground State density of electrons: Zr n = N m A A where Z is # of conduction electrons per atom, A is relative atomic mass, rm is the density of mass in the metal. The spherical volume of each electron is, 1 3 1 V 4 3 æ 3 ö = = p rs rs = ç ÷ n N 3 è 4p nø Free electron gas model: Suppose, except the confining potential near surfaces of metals, conduction electrons are completely free. The conduction electrons thus behave just like gas atoms in an ideal gas --- free electron gas. 3 6.1 Electron Gas Model and its Ground State Basic Properties: ü Ignore interactions of electron-ion type (free electron approx.) ü And electron-eletron type (independent electron approx). Total energy are of kinetic type, ignore potential energy contribution. ü The classical theory had several conspicuous successes 4 6.1 Electron Gas Model and its Ground State Long Mean Free Path: ü From many types of experiments it is clear that a conduction electron in a metal can move freely in a straight path over many atomic distances. -
Free Executive Summary
http://www.nap.edu/catalog/573.html We ship printed books within 1 business day; personal PDFs are available immediately. Biographical Memoirs V.50 Office of the Home Secretary, National Academy of Sciences ISBN: 0-309-59898-2, 416 pages, 6 x 9, (1979) This PDF is available from the National Academies Press at: http://www.nap.edu/catalog/573.html Visit the National Academies Press online, the authoritative source for all books from the National Academy of Sciences, the National Academy of Engineering, the Institute of Medicine, and the National Research Council: • Download hundreds of free books in PDF • Read thousands of books online for free • Explore our innovative research tools – try the “Research Dashboard” now! • Sign up to be notified when new books are published • Purchase printed books and selected PDF files Thank you for downloading this PDF. If you have comments, questions or just want more information about the books published by the National Academies Press, you may contact our customer service department toll- free at 888-624-8373, visit us online, or send an email to [email protected]. This book plus thousands more are available at http://www.nap.edu. Copyright © National Academy of Sciences. All rights reserved. Unless otherwise indicated, all materials in this PDF File are copyrighted by the National Academy of Sciences. Distribution, posting, or copying is strictly prohibited without written permission of the National Academies Press. Request reprint permission for this book. i e h t be ion. om r ibut f r t cannot r at not Biographical Memoirs o f NATIONAL ACADEMY OF SCIENCES however, version ng, i t paper book, at ive at rm o riginal horit ic f o e h t he aut t om r as ing-specif t ion ed f peset y http://www.nap.edu/catalog/573.html Biographical MemoirsV.50 publicat her t iles creat is h t L f M of and ot X om yles, r f st version print posed e h heading Copyright © National Academy ofSciences. -
The World Around Is Physics
The world around is physics Life in science is hard What we see is engineering Chemistry is harder There is no money in chemistry Future is uncertain There is no need of chemistry Therefore, it is not my option I don’t have to learn chemistry Chemistry is life Chemistry is chemicals Chemistry is memorizing things Chemistry is smell Chemistry is this and that- not sure Chemistry is fumes Chemistry is boring Chemistry is pollution Chemistry does not excite Chemistry is poison Chemistry is a finished subject Chemistry is dirty Chemistry - stands on the legacy of giants Antoine-Laurent Lavoisier (1743-1794) Marie Skłodowska Curie (1867- 1934) John Dalton (1766- 1844) Sir Humphrey Davy (1778 – 1829) Michael Faraday (1791 – 1867) Chemistry – our legacy Mendeleev's Periodic Table Modern Periodic Table Dmitri Ivanovich Mendeleev (1834-1907) Joseph John Thomson (1856 –1940) Great experimentalists Ernest Rutherford (1871-1937) Jagadish Chandra Bose (1858 –1937) Chandrasekhara Venkata Raman (1888-1970) Chemistry and chemical bond Gilbert Newton Lewis (1875 –1946) Harold Clayton Urey (1893- 1981) Glenn Theodore Seaborg (1912- 1999) Linus Carl Pauling (1901– 1994) Master craftsmen Robert Burns Woodward (1917 – 1979) Chemistry and the world Fritz Haber (1868 – 1934) Machines in science R. E. Smalley Great teachers Graduate students : Other students : 1. Werner Heisenberg 1. Herbert Kroemer 2. Wolfgang Pauli 2. Linus Pauling 3. Peter Debye 3. Walter Heitler 4. Paul Sophus Epstein 4. Walter Romberg 5. Hans Bethe 6. Ernst Guillemin 7. Karl Bechert 8. Paul Peter Ewald 9. Herbert Fröhlich 10. Erwin Fues 11. Helmut Hönl 12. Ludwig Hopf 13. Walther Kossel 14. -
Wolfgang Pauli 1900 to 1930: His Early Physics in Jungian Perspective
Wolfgang Pauli 1900 to 1930: His Early Physics in Jungian Perspective A Dissertation Submitted to the Faculty of the Graduate School of the University of Minnesota by John Richard Gustafson In Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy Advisor: Roger H. Stuewer Minneapolis, Minnesota July 2004 i © John Richard Gustafson 2004 ii To my father and mother Rudy and Aune Gustafson iii Abstract Wolfgang Pauli's philosophy and physics were intertwined. His philosophy was a variety of Platonism, in which Pauli’s affiliation with Carl Jung formed an integral part, but Pauli’s philosophical explorations in physics appeared before he met Jung. Jung validated Pauli’s psycho-philosophical perspective. Thus, the roots of Pauli’s physics and philosophy are important in the history of modern physics. In his early physics, Pauli attempted to ground his theoretical physics in positivism. He then began instead to trust his intuitive visualizations of entities that formed an underlying reality to the sensible physical world. These visualizations included holistic kernels of mathematical-physical entities that later became for him synonymous with Jung’s mandalas. I have connected Pauli’s visualization patterns in physics during the period 1900 to 1930 to the psychological philosophy of Jung and displayed some examples of Pauli’s creativity in the development of quantum mechanics. By looking at Pauli's early physics and philosophy, we gain insight into Pauli’s contributions to quantum mechanics. His exclusion principle, his influence on Werner Heisenberg in the formulation of matrix mechanics, his emphasis on firm logical and empirical foundations, his creativity in formulating electron spinors, his neutrino hypothesis, and his dialogues with other quantum physicists, all point to Pauli being the dominant genius in the development of quantum theory. -
5 X-Ray Crystallography
Introductory biophysics A. Y. 2016-17 5. X-ray crystallography and its applications to the structural problems of biology Edoardo Milotti Dipartimento di Fisica, Università di Trieste The interatomic distance in a metallic crystal can be roughly estimated as follows. Take, e.g., iron • density: 7.874 g/cm3 • atomic weight: 56 3 • molar volume: VM = 7.1 cm /mole then the interatomic distance is roughly VM d ≈ 3 ≈ 2.2nm N A Edoardo Milotti - Introductory biophysics - A.Y. 2016-17 The atomic lattice can be used a sort of diffraction grating for short-wavelength radiation, about 100 times shorter than visible light which is in the range 400-750 nm. Since hc 2·10−25 J m 1.24 eV µm E = ≈ ≈ γ λ λ λ 1 nm radiation corresponds to about 1 keV photon energy. Edoardo Milotti - Introductory biophysics - A.Y. 2016-17 !"#$%&'$(")* S#%/J&T&U2*#<.%&CKET3&VG$GG./"#%G3&W.%-$/; +(."J&AN&>,%()&CTDB3&S.%)(/3&X.1*&W.%-$/; Y#<.)&V%(Z.&(/&V=;1(21&(/&CTCL&[G#%&=(1&"(12#5.%;&#G&*=.& "(GG%$2*(#/&#G&\8%$;1&<;&2%;1*$)1] 9/(*($));&=.&1*:"(."&H(*=&^_/F*./3&$/"&*=./&H(*=&'$`&V)$/2I&(/& S.%)(/3&H=.%.&=.&=$<()(*$*."&(/&CTBD&H(*=&$&*=.1(1&[a<.% "(.& 9/*.%G.%./Z.%12=.(/:/F./ $/&,)$/,$%$)).)./ V)$**./[?& 7=./&=.&H#%I."&$*&*=.&9/1*(*:*.&#G&7=.#%.*(2$)&V=;1(213&=.$"."& <;&>%/#)"&Q#--.%G.)"3&:/*()&=.&H$1&$,,#(/*."&G:))&,%#G.11#%&$*& *=.&4/(5.%1(*;&#G&0%$/IG:%*&(/&CTCL3&H=./&=.&$)1#&%.2.(5."&=(1& Y#<.)&V%(Z.?& !"#$%"#&'()#**(&8 9/*%#":2*#%;&<(#,=;1(21&8 >?@?&ABCD8CE Arnold Sommerfeld (1868-1951) ... Four of Sommerfeld's doctoral students, Werner Heisenberg, Wolfgang Pauli, Peter Debye, and Hans Bethe went on to win Nobel Prizes, while others, most notably, Walter Heitler, Rudolf Peierls, Karl Bechert, Hermann Brück, Paul Peter Ewald, Eugene Feenberg, Herbert Fröhlich, Erwin Fues, Ernst Guillemin, Helmut Hönl, Ludwig Hopf, Adolf KratZer, Otto Laporte, Wilhelm LenZ, Karl Meissner, Rudolf Seeliger, Ernst C. -
Who Got Moseley's Prize?
Chapter 4 Who Got Moseley’s Prize? Virginia Trimble1 and Vera V. Mainz*,2 1Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, United States 2Department of Chemistry, University of Illinois at Urbana-Champaign, Urbana, Illinois 61802, United States *E-mail: [email protected]. Henry Gwyn Jeffreys Moseley (1887-1915) made prompt and very skilled use of the then new technique of X-ray scattering by crystals (Bragg scattering) to solve several problems about the periodic table and atoms. He was nominated for both the chemistry and physics Nobel Prizes by Svante Arrhenius in 1915, but was dead at Gallipoli before the committees finished their deliberations. Instead, the 1917 physics prize (announced in 1918 and presented on 6 June 1920) went to Charles Glover Barkla (1877-1944) “for discovery of the Röntgen radiation of the elements.” This, and his discovery of X-ray polarization, were done with earlier techniques that he never gave up. Moseley’s contemporaries and later historians of science have written that he would have gone on to other major achievements and a Nobel Prize if he had lived. In contrast, after about 1916, Barkla moved well outside the scientific mainstream, clinging to upgrades of his older methods, denying the significance of the Bohr atom and quantization, and continuing to report evidence for what he called the J phenomenon. This chapter addresses the lives and scientific endeavors of Moseley and Barkla, something about the context in which they worked and their connections with other scientists, contemporary, earlier, and later. © 2017 American Chemical Society Introduction Henry Moseley’s (Figure 1) academic credentials consisted of a 1910 Oxford BA with first-class honors in Mathematical Moderations and a second in Natural Sciences (physics) and the MA that followed more or less automatically a few years later. -
OTTO LAPORTE July 23,1902-March 28,1971
NATIONAL ACADEMY OF SCIENCES O T T O L APORTE 1902—1971 A Biographical Memoir by H. R. CR A N E A N D D. M . D ENNISON Any opinions expressed in this memoir are those of the author(s) and do not necessarily reflect the views of the National Academy of Sciences. Biographical Memoir COPYRIGHT 1979 NATIONAL ACADEMY OF SCIENCES WASHINGTON D.C. OTTO LAPORTE July 23,1902-March 28,1971 BY H. R. CRANE AND D. M. DENNISON* TTO LAPORTE was a member of the small group of brilliant O young theoretical physicists who received their training during the middle 1920s under the guidance of Arnold Sommer- feld in Munich. Otto Laporte was born in Mainz, Germany. His ancestral lineage came from French Huguenot families who fled from France to Switzerland during the period of intense religious persecution in the late seventeenth century. They were later allowed by Frederick the Great to move to Prussia, where they and their descendants became, for the most part, civil servants in the Prussian State. It appears that Otto was the first member of his family to devote himself to science or any other scholarly career. His father was a career officer in the Imperial German Army, and his specialty was heavy artillery. During the years before World War I, Colonel Laporte was successively stationed in the heavily fortified cities of Mainz, Cologne, and Metz, and it was in these cities that young Otto Laporte received his early schooling. After the war broke out, the family was evacuated from Metz and returned to Mainz, where Otto's mother's family lived.