Physics71-80-1.Pdf
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
2007 Abstracts Und Curricula Bewusstsein Und Quantencomputer
BEWUSSTSEIN UND QUANTENCOMPUTER CONSCIOUSNESS AND QUANTUMCOMPUTERS ______________________________________________________________ 7. SCHWEIZER BIENNALE ZU WISSENSCHAFT, TECHNIK + ÄSTHETIK THE 7th SWISS BIENNIAL ON SCIENCE, TECHNICS + AESTHETICS 20. / 21. Januar 2007 / January 20 - 21, 2007 Verkehrshaus der Schweiz, Luzern Swiss Museum of Transport, Lucerne Veranstalter: Neue Galerie Luzern, www.neugalu.ch Organized by: New Gallery Lucerne, www.neugalu.ch ______________________________________________________________ A B S T R A C T S Samstag, 20. Januar 2007 / Saturday, January 20, 2007 Verkehrshaus der Schweiz / Swiss Museum of Transport Keynote 12.15 - 12.45 BRIAN JOSEPHSON Quantenphysik Cambridge / UK IS QUANTUM MECHANICS OR COMPUTATION MORE FUNDAMENTAL? IST DIE QUANTENMECHANIK ODER DAS RECHNEN FUNDAMENTALER? Is quantum mechanics as currently conceived the ultimate theory of nature? In his book "Atomic Physics and Human Knowledge", Niels Bohr argued that because of the uncertainty principle quantum methodology might not be applicable to the study of the ultimate details of life. Delbruck disagreed, claiming that biosystems are robust to quantum disturbances, an assertion that is only partially valid rendering Bohr's argument still significant, even though normally ignored. The methods of the quantum physicist and of the biological sciences can be seen to involve two alternative approaches to the understanding of nature that can usefully complement each other, neither on its own containing the full story. That full story, taking into -
Famous Physicists Himansu Sekhar Fatesingh
Fun Quiz FAMOUS PHYSICISTS HIMANSU SEKHAR FATESINGH 1. The first woman to 6. He first succeeded in receive the Nobel Prize in producing the nuclear physics was chain reaction. a. Maria G. Mayer a. Otto Hahn b. Irene Curie b. Fritz Strassmann c. Marie Curie c. Robert Oppenheimer d. Lise Meitner d. Enrico Fermi 2. Who first suggested electron 7. The credit for discovering shells around the nucleus? electron microscope is often a. Ernest Rutherford attributed to b. Neils Bohr a. H. Germer c. Erwin Schrödinger b. Ernst Ruska d. Wolfgang Pauli c. George P. Thomson d. Clinton J. Davisson 8. The wave theory of light was 3. He first measured negative first proposed by charge on an electron. a. Christiaan Huygens a. J. J. Thomson b. Isaac Newton b. Clinton Davisson c. Hermann Helmholtz c. Louis de Broglie d. Augustin Fresnel d. Robert A. Millikan 9. He was the first scientist 4. The existence of quarks was to find proof of Einstein’s first suggested by theory of relativity a. Max Planck a. Edwin Hubble b. Sheldon Glasgow b. George Gamow c. Murray Gell-Mann c. S. Chandrasekhar d. Albert Einstein d. Arthur Eddington 10. The credit for development of the cyclotron 5. The phenomenon of goes to: superconductivity was a. Carl Anderson b. Donald Glaser discovered by c. Ernest O. Lawrence d. Charles Wilson a. Heike Kamerlingh Onnes b. Alex Muller c. Brian D. Josephson 11. Who first proposed the use of absolute scale d. John Bardeen of Temperature? a. Anders Celsius b. Lord Kelvin c. Rudolf Clausius d. -
Cambridge's 92 Nobel Prize Winners Part 2 - 1951 to 1974: from Crick and Watson to Dorothy Hodgkin
Cambridge's 92 Nobel Prize winners part 2 - 1951 to 1974: from Crick and Watson to Dorothy Hodgkin By Cambridge News | Posted: January 18, 2016 By Adam Care The News has been rounding up all of Cambridge's 92 Nobel Laureates, celebrating over 100 years of scientific and social innovation. ADVERTISING In this installment we move from 1951 to 1974, a period which saw a host of dramatic breakthroughs, in biology, atomic science, the discovery of pulsars and theories of global trade. It's also a period which saw The Eagle pub come to national prominence and the appearance of the first female name in Cambridge University's long Nobel history. The Gender Pay Gap Sale! Shop Online to get 13.9% off From 8 - 11 March, get 13.9% off 1,000s of items, it highlights the pay gap between men & women in the UK. Shop the Gender Pay Gap Sale – now. Promoted by Oxfam 1. 1951 Ernest Walton, Trinity College: Nobel Prize in Physics, for using accelerated particles to study atomic nuclei 2. 1951 John Cockcroft, St John's / Churchill Colleges: Nobel Prize in Physics, for using accelerated particles to study atomic nuclei Walton and Cockcroft shared the 1951 physics prize after they famously 'split the atom' in Cambridge 1932, ushering in the nuclear age with their particle accelerator, the Cockcroft-Walton generator. In later years Walton returned to his native Ireland, as a fellow of Trinity College Dublin, while in 1951 Cockcroft became the first master of Churchill College, where he died 16 years later. 3. 1952 Archer Martin, Peterhouse: Nobel Prize in Chemistry, for developing partition chromatography 4. -
Antony Hewish
PULSARS AND HIGH DENSITY PHYSICS Nobel Lecture, December 12, 1974 by A NTONY H E W I S H University of Cambridge, Cavendish Laboratory, Cambridge, England D ISCOVERY OF P U L S A R S The trail which ultimately led to the first pulsar began in 1948 when I joined Ryle’s small research team and became interested in the general problem of the propagation of radiation through irregular transparent media. We are all familiar with the twinkling of visible stars and my task was to understand why radio stars also twinkled. I was fortunate to have been taught by Ratcliffe, who first showed me the power of Fourier techniques in dealing with such diffraction phenomena. By a modest extension of existing theory I was able to show that our radio stars twinkled because of plasma clouds in the ionosphere at heights around 300 km, and I was also able to measure the speed of ionospheric winds in this region (1) . My fascination in using extra-terrestrial radio sources for studying the intervening plasma next brought me to the solar corona. From observations of the angular scattering of radiation passing through the corona, using simple radio interferometers, I was eventually able to trace the solar atmo- sphere out to one half the radius of the Earth’s orbit (2). In my notebook for 1954 there is a comment that, if radio sources were of small enough angular size, they would illuminate the solar atmosphere with sufficient coherence to produce interference patterns at the Earth which would be detectable as a very rapid fluctuation of intensity. -
From Theory to the First Working Laser Laser History—Part I
I feature_ laser history From theory to the first working laser Laser history—Part I Author_Ingmar Ingenegeren, Germany _The principle of both maser (microwave am- 19 US patents) using a ruby laser. Both were nom- plification by stimulated emission of radiation) inated for the Nobel Prize. Gábor received the 1971 and laser (light amplification by stimulated emis- Nobel Prize in Physics for the invention and devel- sion of radiation) were first described in 1917 by opment of the holographic method. To a friend he Albert Einstein (Fig.1) in “Zur Quantentheorie der wrote that he was ashamed to get this prize for Strahlung”, as the so called ‘stimulated emission’, such a simple invention. He was the owner of more based on Niels Bohr’s quantum theory, postulated than a hundred patents. in 1913, which explains the actions of electrons in- side atoms. Einstein (born in Germany, 14 March In 1954 at the Columbia University in New York, 1879–18 April 1955) received the Nobel Prize for Charles Townes (born in the USA, 28 July 1915–to- physics in 1921, and Bohr (born in Denmark, 7 Oc- day, Fig. 2) and Arthur Schawlow (born in the USA, tober 1885–18 November 1962) in 1922. 5 Mai 1921–28 April 1999, Fig. 3) invented the maser, using ammonia gas and microwaves which In 1947 Dennis Gábor (born in Hungarian, 5 led to the granting of a patent on March 24, 1959. June 1900–8 February 1972) developed the theory The maser was used to amplify radio signals and as of holography, which requires laser light for its re- an ultra sensitive detector for space research. -
“Kings of Cool” Superconductivity Who Are These People? SUPERCONDUCTORS
“““Kings of Cool” Superconductivity Who are these people? SUPERCONDUCTORS An Introduction by Prof George Walmsley Normal conductor eg copper • Current, I. • Voltage drop, V. • Resistance, R = ? • Ans: V/I = R eg 2 Volts/1 Amp = 2 Ohms I Copper I V Normal conductor eg copper • Source of resistance: • Electron collides with lattice ion to produce heat (phonon). Copper lattice Lower Temperature • What happens when we cool a metal? • Ans 1: The electrons slow down and current is reduced maybe to zero. R→∞ • Ans 2: The lattice stops vibrating and resistance disappears. R=0 How do we cool things? • Commonly used liquid refrigerants: Element Boiling Pt Oxygen 90K Nitrogen 77K Hydrogen 20K Helium 4.2K Thomas Andrews, Chemist • 9 Dec 1813 – 26 Nov 1885 • John (Flax spinner, Comber) [ggfather] • Michael (Linen, Ardoyne) [gfather] • Thomas (Linen merchant) [father] • Studied under James Thomson, RBAI • 1828 Univ of Glasgow, Thos Thomson • 1830 Paris, Dumas • 1830-34 Trinity College Dublin • 1835 MD U of Edinburgh • 1835-45 Prof of Chemistry RBAI • 1845 Vice-President, Queen’s College • 1847 Prof of Chemistry, Queen’s College • 1869 Bakerian Lecture on CO 2 • 1871 Visit by Dr Janssen of Leiden • Photo: Paris 1875 Andrews’ Isotherms • Note critical temperature NORMAL CONDUCTOR: Electrical properties Normal metal eg copper Resistance and (resistivity, ρ) >0 As temperature falls ρ falls smoothly too: ρ 0 100 200 273.15 Temperature/K SUPERCONDUCTOR: Electrical properties Superconductor eg mercury, lead Resistivity ( ρ) >0 like normal metal down to critical -
Kritikens Ordning Svenska Bokrecensioner 1906, 1956, 2006
Kritikens ordning Svenska bokrecensioner 1906, 1956, 2006 © lina samuelsson Grafisk form anita stjernlöf-lund Typografi AGaramond Papper Munken Pure Omslagets bild gertrud samén Tryck trt boktryckeri, Tallinn 2013 Förlag bild,text&form www.bildtextform.com isbn 978-91-980447-1-3 Lina Samuelsson Kritikens ordning Svenska bokrecensioner 1906, 1956, 2006 bild,text&form 7 tack 8 förkortningar 8 pseudonym- och signaturnyckel 9 inledning 10 Vad är litteraturkritik? 11 Institution – diskurs – normer 14 Tidigare forskning 1906 17 Det litterära året 18 Urval och undersökt material 21 kritikerna 1906 21 Litteraturbevakningen före kultursidan 23 Kritikerkåren 26 Litteraturen 28 Kritiken av kritiken 33 recensionerna 1906 33 Utveckling, mognad och manlighet. Författaren och verket 35 ”En verklig människa, som lefver och röres inför våra ögon”. Kritikens värderingskriterier I 38 ”Det själfupplefvdas egendomlighet och autopsi”. Kritikens värderingskriterier II 41 Vem är författare? Konstnärlighet, genus och rätten till ordet 46 För fosterlandet. Föreställningar om nationalism 50 exempelrecension 1956 56 Det litterära året 58 Urval och undersökt material 62 kritikerna 1956 62 Kultursidor och litteraturtidskrifter 66 Kritikerkåren 72 Litteraturen 75 Kampen om kritiken 79 recensionerna 1956 79 En ny och modern kritik. Verket och kritikern 82 Enkelt och äkta. Kritikens värderingskriterier I 84 Om att vara människa. Kritikens värderingskriterier II 88 ”Fem hekto nougat i lyxförpackning”. Populärlitteratur och genus 94 exempelrecension 2006 99 Det litterära året riginal 101 Urval och undersökt material 105 kritikerna 2006 105 Drakar, bloggar och tabloider 110 Kritikerkåren 116 Litteraturen 121 Kritik i kris? 125 recensionerna 2006 125 Subjektiv och auktoritär – kritikern i centrum 129 Personligt, biografiskt (och dessutom sant). Författaren och verket 134 Drabbande pageturner som man minns länge. -
April 17-19, 2018 the 2018 Franklin Institute Laureates the 2018 Franklin Institute AWARDS CONVOCATION APRIL 17–19, 2018
april 17-19, 2018 The 2018 Franklin Institute Laureates The 2018 Franklin Institute AWARDS CONVOCATION APRIL 17–19, 2018 Welcome to The Franklin Institute Awards, the a range of disciplines. The week culminates in a grand United States’ oldest comprehensive science and medaling ceremony, befitting the distinction of this technology awards program. Each year, the Institute historic awards program. celebrates extraordinary people who are shaping our In this convocation book, you will find a schedule of world through their groundbreaking achievements these events and biographies of our 2018 laureates. in science, engineering, and business. They stand as We invite you to read about each one and to attend modern-day exemplars of our namesake, Benjamin the events to learn even more. Unless noted otherwise, Franklin, whose impact as a statesman, scientist, all events are free, open to the public, and located in inventor, and humanitarian remains unmatched Philadelphia, Pennsylvania. in American history. Along with our laureates, we celebrate his legacy, which has fueled the Institute’s We hope this year’s remarkable class of laureates mission since its inception in 1824. sparks your curiosity as much as they have ours. We look forward to seeing you during The Franklin From sparking a gene editing revolution to saving Institute Awards Week. a technology giant, from making strides toward a unified theory to discovering the flow in everything, from finding clues to climate change deep in our forests to seeing the future in a terahertz wave, and from enabling us to unplug to connecting us with the III world, this year’s Franklin Institute laureates personify the trailblazing spirit so crucial to our future with its many challenges and opportunities. -
Physics Nobel Prize 1975
Physics Nobel Prize 1975 Nobel prize winners, left to right, A. Bohr, B. Mottelson and J. Rainwater. 0. Kofoed-Hansen (Photos Keystone Press, Photopress) Before 1949 every physicist knew that mooted, it was a major breakthrough from 1943-45. From December 1943 the atomic nucleus does not rotate. in thinking about the nucleus and he was actually in the USA. Back in The reasoning behind this erroneous opened a whole new field of research Denmark after the war, he obtained belief came from the following argu• in nuclear physics. This work has for his Ph. D. in 1954 for work on rota• ments. A quantum-mechanical rotator years been guided by the inspiration tional states in atomic nuclei. His with the moment of inertia J can take of Bohr and Mottelson. thesis was thus based on the work for up various energy levels with rota• An entire industry of nuclear which he has now been recognized at tional energies equal to h2(l + 1)| research thus began with Rainwater's the very highest level. He is Professor /8TC2J, where h is Planck's constant brief contribution to Physical Review at the Niels Bohr Institute of the ^nd I is the spin. As an example, I may in 1950 entitled 'Nuclear energy level University of Copenhagen and a nave values 0, 2, 4, ... etc. If the argument for a spheroidal nuclear member of the CERN Scientific Policy nucleus is considered as a rigid body, model'. Today a fair-sized library is Committee. then the moment of inertia J is very needed in order to contain all the Ben Mottelson was born in the USA large and the rotational energies papers written on deformed nuclei and in 1926 and has, for many years, become correspondingly very small. -
Date: To: September 22, 1 997 Mr Ian Johnston©
22-SEP-1997 16:36 NOBELSTIFTELSEN 4& 8 6603847 SID 01 NOBELSTIFTELSEN The Nobel Foundation TELEFAX Date: September 22, 1 997 To: Mr Ian Johnston© Company: Executive Office of the Secretary-General Fax no: 0091-2129633511 From: The Nobel Foundation Total number of pages: olO MESSAGE DearMrJohnstone, With reference to your fax and to our telephone conversation, I am enclosing the address list of all Nobel Prize laureates. Yours sincerely, Ingr BergstrSm Mailing address: Bos StU S-102 45 Stockholm. Sweden Strat itddrtSMi Suircfatan 14 Teleptelrtts: (-MB S) 663 » 20 Fsuc (*-«>!) «W Jg 47 22-SEP-1997 16:36 NOBELSTIFTELSEN 46 B S603847 SID 02 22-SEP-1997 16:35 NOBELSTIFTELSEN 46 8 6603847 SID 03 Professor Willis E, Lamb Jr Prof. Aleksandre M. Prokhorov Dr. Leo EsaJki 848 North Norris Avenue Russian Academy of Sciences University of Tsukuba TUCSON, AZ 857 19 Leninskii Prospect 14 Tsukuba USA MSOCOWV71 Ibaraki Ru s s I a 305 Japan 59* c>io Dr. Tsung Dao Lee Professor Hans A. Bethe Professor Antony Hewlsh Department of Physics Cornell University Cavendish Laboratory Columbia University ITHACA, NY 14853 University of Cambridge 538 West I20th Street USA CAMBRIDGE CB3 OHE NEW YORK, NY 10027 England USA S96 014 S ' Dr. Chen Ning Yang Professor Murray Gell-Mann ^ Professor Aage Bohr The Institute for Department of Physics Niels Bohr Institutet Theoretical Physics California Institute of Technology Blegdamsvej 17 State University of New York PASADENA, CA91125 DK-2100 KOPENHAMN 0 STONY BROOK, NY 11794 USA D anni ark USA 595 600 613 Professor Owen Chamberlain Professor Louis Neel ' Professor Ben Mottelson 6068 Margarldo Drive Membre de rinstitute Nordita OAKLAND, CA 946 IS 15 Rue Marcel-Allegot Blegdamsvej 17 USA F-92190 MEUDON-BELLEVUE DK-2100 KOPENHAMN 0 Frankrike D an m ar k 599 615 Professor Donald A. -
De Nobelprijzen Komen Eraan!
De Nobelprijzen komen eraan! De Nobelprijzen komen eraan! In de loop van volgende week worden de Nobelprijswinnaars van dit jaar aangekondigd. Daarna weten we wie in december deze felbegeerde prijzen in ontvangst mogen gaan nemen. De Nobelprijzen zijn wellicht de meest prestigieuze en bekende academische onderscheidingen ter wereld, maar waarom eigenlijk? Hoe zijn de prijzen ontstaan, en wie was hun grondlegger, Alfred Nobel? Afbeelding 1. Alfred Nobel.Alfred Nobel (1833-1896) was de grondlegger van de Nobelprijzen. Volgende week is de jaarlijkse aankondiging van de prijswinnaard. Alfred Nobel Alfred Nobel was een belangrijke negentiende-eeuwse Zweedse scheikundige en uitvinder. Hij werd geboren in Stockholm in 1833 in een gezin met acht kinderen. Zijn vader, Immanuel Nobel, was een werktuigkundige en uitvinder die succesvol was met het maken van wapens en stoommotoren. Immanuel wou dat zijn zonen zijn bedrijf zouden overnemen en stuurde Alfred daarom op een twee jaar durende reis naar onder andere Duitsland, Frankrijk en de Verenigde Staten, om te leren over chemische werktuigbouwkunde. In Parijs ontmoette bron: https://www.quantumuniverse.nl/de-nobelprijzen-komen-eraan Pagina 1 van 5 De Nobelprijzen komen eraan! Alfred de Italiaanse scheikundige Ascanio Sobrero, die drie jaar eerder het explosief nitroglycerine had ontdekt. Nitroglycerine had een veel grotere explosieve kracht dan het buskruit, maar was ook veel gevaarlijker om te gebruiken omdat het instabiel is. Alfred raakte geinteresseerd in nitroglycerine en hoe het gebruikt kon worden voor commerciele doeleinden, en ging daarom werken aan de stabiliteit en veiligheid van de stof. Een makkelijk project was dit niet, en meerdere malen ging het flink mis. -
Appendix E Nobel Prizes in Nuclear Science
Nuclear Science—A Guide to the Nuclear Science Wall Chart ©2018 Contemporary Physics Education Project (CPEP) Appendix E Nobel Prizes in Nuclear Science Many Nobel Prizes have been awarded for nuclear research and instrumentation. The field has spun off: particle physics, nuclear astrophysics, nuclear power reactors, nuclear medicine, and nuclear weapons. Understanding how the nucleus works and applying that knowledge to technology has been one of the most significant accomplishments of twentieth century scientific research. Each prize was awarded for physics unless otherwise noted. Name(s) Discovery Year Henri Becquerel, Pierre Discovered spontaneous radioactivity 1903 Curie, and Marie Curie Ernest Rutherford Work on the disintegration of the elements and 1908 chemistry of radioactive elements (chem) Marie Curie Discovery of radium and polonium 1911 (chem) Frederick Soddy Work on chemistry of radioactive substances 1921 including the origin and nature of radioactive (chem) isotopes Francis Aston Discovery of isotopes in many non-radioactive 1922 elements, also enunciated the whole-number rule of (chem) atomic masses Charles Wilson Development of the cloud chamber for detecting 1927 charged particles Harold Urey Discovery of heavy hydrogen (deuterium) 1934 (chem) Frederic Joliot and Synthesis of several new radioactive elements 1935 Irene Joliot-Curie (chem) James Chadwick Discovery of the neutron 1935 Carl David Anderson Discovery of the positron 1936 Enrico Fermi New radioactive elements produced by neutron 1938 irradiation Ernest Lawrence