Albert Einstein and the Nature of Science"
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Honolulu Star-Advertiser
B CITY EDITOR: David Butts / [email protected] / 529-4310 WEDNESDAY 10/7/20 VANDALS AT WORK A $20,000 digital sign is damaged at Makapu‘u Lighthouse Trail over the weekend >> B2 ——— BIG Q >> B2 COMICS & PUZZLES >> B7-9 KOKUA LINE CHRISTINE DONNELLY Must apply for extended jobless benefits uestion: Are the extended benefits Q automatic once I run out of unemploy- ment? It’s getting close. What do I do? Answer: No, Pan- demic Emergency Unem- ployment Compensation is not automatic. You have to apply for this pro- gram, which adds 13 weeks of benefits for eligi- UCLA VIA AP / 2015 ble claimants, and you must have a zero balance Andrea Ghez, professor of physics and astronomy at UCLA, was one of three scientists who was awarded this year’s Nobel Prize in in your Unemployment In- physics for advancing the understanding of black holes. Ghez was photographed on the university’s campus. surance account before you do so, according to the state Department of Labor and Industrial Rela- Nobel winner is Keck Observatory user tions. You would apply through your online UI ac- Astronomer Andrea Ghez has been studying the ry’s telescopes, Lewis said count and answer a series Ghez probably uses them of questions to determine Galactic Center from Hawaii island since 1995 more often than anyone whether you are eligible. else — about a dozen nights For instructions on how Star-Advertiser staff covering a supermassive per year. to apply, see labor.hawaii. and news services black hole at the center of The observatory’s twin gov/ui/. -
Hendrik Antoon Lorentz's Struggle with Quantum Theory A. J
Hendrik Antoon Lorentz’s struggle with quantum theory A. J. Kox Archive for History of Exact Sciences ISSN 0003-9519 Volume 67 Number 2 Arch. Hist. Exact Sci. (2013) 67:149-170 DOI 10.1007/s00407-012-0107-8 1 23 Your article is published under the Creative Commons Attribution license which allows users to read, copy, distribute and make derivative works, as long as the author of the original work is cited. You may self- archive this article on your own website, an institutional repository or funder’s repository and make it publicly available immediately. 1 23 Arch. Hist. Exact Sci. (2013) 67:149–170 DOI 10.1007/s00407-012-0107-8 Hendrik Antoon Lorentz’s struggle with quantum theory A. J. Kox Received: 15 June 2012 / Published online: 24 July 2012 © The Author(s) 2012. This article is published with open access at Springerlink.com Abstract A historical overview is given of the contributions of Hendrik Antoon Lorentz in quantum theory. Although especially his early work is valuable, the main importance of Lorentz’s work lies in the conceptual clarifications he provided and in his critique of the foundations of quantum theory. 1 Introduction The Dutch physicist Hendrik Antoon Lorentz (1853–1928) is generally viewed as an icon of classical, nineteenth-century physics—indeed, as one of the last masters of that era. Thus, it may come as a bit of a surprise that he also made important contribu- tions to quantum theory, the quintessential non-classical twentieth-century develop- ment in physics. The importance of Lorentz’s work lies not so much in his concrete contributions to the actual physics—although some of his early work was ground- breaking—but rather in the conceptual clarifications he provided and his critique of the foundations and interpretations of the new ideas. -
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. -
Harry Truman, the Atomic Bomb and the Apocalyptic Narrative
Volume 5 | Issue 7 | Article ID 2479 | Jul 12, 2007 The Asia-Pacific Journal | Japan Focus The Decision to Risk the Future: Harry Truman, the Atomic Bomb and the Apocalyptic Narrative Peter J. Kuznick The Decision to Risk the Future: Harry stressed that the future of mankind would be Truman, the Atomic Bomb and theshaped by how such bombs were used and Apocalyptic Narrative subsequently controlled or shared.[3] Truman recalled Stimson “gravely” expressing his Peter J. Kuznick uncertainty about whether the U.S. should ever use the bomb, “because he was afraid it was so I powerful that it could end up destroying the whole world.” Truman admitted that, listening In his personal narrative Atomic Quest, Nobel to Stimson and Groves and reading Groves’s Prize-winning physicist Arthur Holly Compton, accompanying memo, he “felt the same who directed atomic research at the University fear.”[4] of Chicago’s Metallurgical Laboratory during the Second World War, tells of receiving an urgent visit from J. Robert Oppenheimer while vacationing in Michigan during the summer of 1942. Oppenheimer and the brain trust he assembled had just calculated the possibility that an atomic explosion could ignite all the hydrogen in the oceans or the nitrogen in the atmosphere. If such a possibility existed, Compton concluded, “these bombs must never be made.” As Compton said, “Better to accept the slavery of the Nazis than to run a chance of drawing the final curtain on mankind.”[1] Certainly, any reasonable human being could be expected to respond similarly. Three years later, with Hitler dead and the Nazis defeated, President Harry Truman faced Truman and Byrnes en route to Potsdam, July a comparably weighty decision. -
The Nobel Laureate CV Raman and His Contacts with the European Men of Science in Political Context
The Global and the Local: The History of Science and the Cultural Integration of Europe. nd Proceedings of the 2 ICESHS (Cracow, Poland, September 6-9, 2006) / Ed. by M. Kokowski. Rajinder Singh * The Nobel Laureate CV Raman and his contacts with the European men of science in political context (1) Introduction In 1928 C.V. Raman1 (1888–1970) [see Figure 1 and Box 1] and K.S. Krishnan (1898–1961) observed that if monochromatic light is passed through a transparent medium, thereafter the scattering light is accompanied by other colours. This phenomenon was later named as Raman effect.2 The effect helps to find out the molecular structure of substances. In 1930 Raman was award the Physics Nobel prize ―for his work on light scattering and the discovery of the effect named after him.‖ He was the first Asian to receive this honour. This made him extremely popular. C.V. Raman interacted with the wide scientific community for about half a century and visited many countries. Some of the important physicists who corresponded with Raman were Wladyslaw Natanson,3 Niels Bohr, Max Born, Erwin Schrödinger, Arnold Sommerfeld and Ernest Rutherford. * University of Oldenburg, Faculty V, Institute of Physics – EHF, Research Group: Physics Education, History / Philosophy of Science, Oldenburg, Germany; email: [email protected] . 1 For biographical details, see: C.V. Raman: A Short Biographical Sketch (1938); J. Mehra, Chandrasekhara Venkata Raman, (in: Dictionary of Scientific Biography, C.C. Gillispie, ed.), Vol. XI (1975), pp. 264–267; G.H. Keswani, Raman and His Effect (1980); P.R. -
Einstein's Mistakes
Einstein’s Mistakes Einstein was the greatest genius of the Twentieth Century, but his discoveries were blighted with mistakes. The Human Failing of Genius. 1 PART 1 An evaluation of the man Here, Einstein grows up, his thinking evolves, and many quotations from him are listed. Albert Einstein (1879-1955) Einstein at 14 Einstein at 26 Einstein at 42 3 Albert Einstein (1879-1955) Einstein at age 61 (1940) 4 Albert Einstein (1879-1955) Born in Ulm, Swabian region of Southern Germany. From a Jewish merchant family. Had a sister Maja. Family rejected Jewish customs. Did not inherit any mathematical talent. Inherited stubbornness, Inherited a roguish sense of humor, An inclination to mysticism, And a habit of grüblen or protracted, agonizing “brooding” over whatever was on its mind. Leading to the thought experiment. 5 Portrait in 1947 – age 68, and his habit of agonizing brooding over whatever was on its mind. He was in Princeton, NJ, USA. 6 Einstein the mystic •“Everyone who is seriously involved in pursuit of science becomes convinced that a spirit is manifest in the laws of the universe, one that is vastly superior to that of man..” •“When I assess a theory, I ask myself, if I was God, would I have arranged the universe that way?” •His roguish sense of humor was always there. •When asked what will be his reactions to observational evidence against the bending of light predicted by his general theory of relativity, he said: •”Then I would feel sorry for the Good Lord. The theory is correct anyway.” 7 Einstein: Mathematics •More quotations from Einstein: •“How it is possible that mathematics, a product of human thought that is independent of experience, fits so excellently the objects of physical reality?” •Questions asked by many people and Einstein: •“Is God a mathematician?” •His conclusion: •“ The Lord is cunning, but not malicious.” 8 Einstein the Stubborn Mystic “What interests me is whether God had any choice in the creation of the world” Some broadcasters expunged the comment from the soundtrack because they thought it was blasphemous. -
Atomic Physics & Quantum Effects
KEY CONCEPTS ATOMIC PHYSICS & QUANTUM EFFECTS 1. PHOTONS & THE PHOTOELECTRIC EFFECT Max Planck explained blackbody radiation with his quantum hypothesis, which states that the energy of a thermal oscillator, Eosc, is not continuous, but instead is a discrete quantity given by the equation: Eosc = nhf n = 1, 2, 3,... where f is the frequency and h is a constant now known as Planck’s constant. Albert Einstein extended the idea by adding that all emitted radiation is quantized. He suggested that light is composed of discrete quanta, rather than of waves. According to his theory, each particle of light, known as a photon, has an energy E given by: E = hf Einstein’s theory helped him explain a phenomenon known as the photoelectric effect, in which a photon of light strikes a photosensitive material and causes an electron to be ejected from the material. A photocell constructed from photosensitive material can produce an electrical current when light shines on it. The kinetic energy, K, of a photoelectron displaced by a photon of energy, hf, is given by: K = hf - φ where the work function, φ, is the minimum energy needed to free the electron from the photosensitive material. No photoemission occurs if the frequency of the incident light falls below a certain cutoff frequency – or threshold frequency – given by: φ f0 = h Einstein's theory explained several aspects of the photoelectric effect that could not be explained by classical theory: • The kinetic energy of photoelectrons is dependent on the light’s frequency. • No photoemission occurs for light below a certain threshold frequency. -
The Nobel Peace Prize
TITLE: Learning From Peace Makers OVERVIEW: Students examine The Dalai Lama as a Nobel Laureate and compare / contrast his contributions to the world with the contributions of other Nobel Laureates. SUBJECT AREA / GRADE LEVEL: Civics and Government 7 / 12 STATE CONTENT STANDARDS / BENCHMARKS: -Identify, research, and clarify an event, issue, problem or phenomenon of significance to society. -Gather, use, and evaluate researched information to support analysis and conclusions. OBJECTIVES: The student will demonstrate the ability to... -know and understand The Dalai Lama as an advocate for peace. -research and report the contributions of others who are recognized as advocates for peace, such as those attending the Peace Conference in Portland: Aldolfo Perez Esquivel, Robert Musil, William Schulz, Betty Williams, and Helen Caldicott. -compare and contrast the contributions of several Nobel Laureates with The Dalai Lama. MATERIALS: -Copies of biographical statements of The Dalai Lama. -List of Nobel Peace Prize winners. -Copy of The Dalai Lama's acceptance speech for the Nobel Peace Prize. -Bulletin board for display. PRESENTATION STEPS: 1) Students read one of the brief biographies of The Dalai Lama, including his Five Point Plan for Peace in Tibet, and his acceptance speech for receiving the Nobel Prize for Peace. 2) Follow with a class discussion regarding the biography and / or the text of the acceptance speech. 3) Distribute and examine the list of Nobel Peace Prize winners. 4) Individually, or in cooperative groups, select one of the Nobel Laureates (give special consideration to those coming to the Portland Peace Conference). Research and prepare to report to the class who the person was and why he / she / they won the Nobel Prize. -
Ripples in Spacetime
editorial Ripples in spacetime The 2017 Nobel prize in Physics has been awarded to Rainer Weiss, Barry C. Barish and Kip S. Thorne “for decisive contributions to the LIGO detector and the observation of gravitational waves”. It is, frankly, difficult to find something original to say about the detection of gravitational waves that hasn’t been said already. The technological feat of measuring fluctuations in the fabric of spacetime less than one-thousandth the width of an atomic nucleus is quite simply astonishing. The scientific achievement represented by the confirmation of a century-old prediction by Albert Einstein is unique. And the collaborative effort that made the discovery possible — the Laser Interferometer Gravitational-Wave Observatory (LIGO) — is inspiring. Adapted from Phys. Rev. Lett. 116, 061102 (2016), under Creative Commons Licence. Rainer Weiss and Kip Thorne were, along with the late Ronald Drever, founders of the project that eventually became known Barry Barish, who was the director Last month we received a spectacular as LIGO. In the 1960s, Thorne, a black hole of LIGO from 1997 to 2005, is widely demonstration that talk of a new era expert, had come to believe that his objects of credited with transforming it into a ‘big of gravitational astronomy was no interest should be detectable as gravitational physics’ collaboration, and providing the exaggeration. Cued by detections at LIGO waves. Separately, and inspired by previous organizational structure required to ensure and Virgo, an interferometer based in Pisa, proposals, Weiss came up with the first it worked. Of course, the passion, skill and Italy, more than 70 teams of researchers calculations detailing how an interferometer dedication of the thousand or so scientists working at different telescopes around could be used to detect them in 1972. -
How Science Works
PB 1 How science works The Scientific Method is traditionally presented in the first chapter of science text- books as a simple recipe for performing scientific investigations. Though many use- ful points are embodied in this method, it can easily be misinterpreted as linear and “cookbook”: pull a problem off the shelf, throw in an observation, mix in a few ques- tions, sprinkle on a hypothesis, put the whole mixture into a 350° experiment—and voila, 50 minutes later you’ll be pulling a conclusion out of the oven! That might work if science were like Hamburger Helper®, but science is complex and cannot be re- duced to a single, prepackaged recipe. The linear, stepwise representation of the process of science is simplified, but it does get at least one thing right. It captures the core logic of science: testing ideas with evidence. However, this version of the scientific method is so simplified and rigid that it fails to accurately portray how real science works. It more accurately describes how science is summarized after the fact—in textbooks and journal articles—than how sci- ence is actually done. The simplified, linear scientific method implies that scientific studies follow an unvarying, linear recipe. But in reality, in their work, scientists engage in many different activities in many different sequences. Scientific investigations often involve repeating the same steps many times to account for new information and ideas. The simplified, linear scientific method implies that science is done by individual scientists working through these steps in isolation. But in reality, science depends on interactions within the scientific community. -
I. I. Rabi Papers [Finding Aid]. Library of Congress. [PDF Rendered Tue Apr
I. I. Rabi Papers A Finding Aid to the Collection in the Library of Congress Manuscript Division, Library of Congress Washington, D.C. 1992 Revised 2010 March Contact information: http://hdl.loc.gov/loc.mss/mss.contact Additional search options available at: http://hdl.loc.gov/loc.mss/eadmss.ms998009 LC Online Catalog record: http://lccn.loc.gov/mm89076467 Prepared by Joseph Sullivan with the assistance of Kathleen A. Kelly and John R. Monagle Collection Summary Title: I. I. Rabi Papers Span Dates: 1899-1989 Bulk Dates: (bulk 1945-1968) ID No.: MSS76467 Creator: Rabi, I. I. (Isador Isaac), 1898- Extent: 41,500 items ; 105 cartons plus 1 oversize plus 4 classified ; 42 linear feet Language: Collection material in English Location: Manuscript Division, Library of Congress, Washington, D.C. Summary: Physicist and educator. The collection documents Rabi's research in physics, particularly in the fields of radar and nuclear energy, leading to the development of lasers, atomic clocks, and magnetic resonance imaging (MRI) and to his 1944 Nobel Prize in physics; his work as a consultant to the atomic bomb project at Los Alamos Scientific Laboratory and as an advisor on science policy to the United States government, the United Nations, and the North Atlantic Treaty Organization during and after World War II; and his studies, research, and professorships in physics chiefly at Columbia University and also at Massachusetts Institute of Technology. Selected Search Terms The following terms have been used to index the description of this collection in the Library's online catalog. They are grouped by name of person or organization, by subject or location, and by occupation and listed alphabetically therein. -
Pauling-Linus.Pdf
NATIONAL ACADEMY OF SCIENCES L I N U S C A R L P A U L I N G 1901—1994 A Biographical Memoir by J A C K D. D UNITZ 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 1997 NATIONAL ACADEMIES PRESS WASHINGTON D.C. LINUS CARL PAULING February 28, 1901–August 19, 1994 BY JACK D. DUNITZ INUS CARL PAULING was born in Portland, Oregon, on LFebruary 28, 1901, and died at his ranch at Big Sur, California, on August 19, 1994. In 1922 he married Ava Helen Miller (died 1981), who bore him four children: Linus Carl, Peter Jeffress, Linda Helen (Kamb), and Edward Crellin. Pauling is widely considered the greatest chemist of this century. Most scientists create a niche for themselves, an area where they feel secure, but Pauling had an enormously wide range of scientific interests: quantum mechanics, crys- tallography, mineralogy, structural chemistry, anesthesia, immunology, medicine, evolution. In all these fields and especially in the border regions between them, he saw where the problems lay, and, backed by his speedy assimilation of the essential facts and by his prodigious memory, he made distinctive and decisive contributions. He is best known, perhaps, for his insights into chemical bonding, for the discovery of the principal elements of protein secondary structure, the alpha-helix and the beta-sheet, and for the first identification of a molecular disease (sickle-cell ane- mia), but there are a multitude of other important contri- This biographical memoir was prepared for publication by both The Royal Society of London and the National Academy of Sciences of the United States of America.