S.S. Bhatnagar, C.V. Raman, Homi Bhabha and Research in Physics at Lahore and Chandigarh
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Von Richthofen, Einstein and the AGA Estimating Achievement from Fame
Von Richthofen, Einstein and the AGA Estimating achievement from fame Every schoolboy has heard of Einstein; fewer have heard of Antoine Becquerel; almost nobody has heard of Nils Dalén. Yet they all won Nobel Prizes for Physics. Can we gauge a scientist’s achievements by his or her fame? If so, how? And how do fighter pilots help? Mikhail Simkin and Vwani Roychowdhury look for the linkages. “It was a famous victory.” We instinctively rank the had published. However, in 2001–2002 popular French achievements of great men and women by how famous TV presenters Igor and Grichka Bogdanoff published they are. But is instinct enough? And how exactly does a great man’s fame relate to the greatness of his achieve- ment? Some achievements are easy to quantify. Such is the case with fighter pilots of the First World War. Their achievements can be easily measured and ranked, in terms of their victories – the number of enemy planes they shot down. These aces achieved varying degrees of fame, which have lasted down to the internet age. A few years ago we compared1 the fame of First World War fighter pilot aces (measured in Google hits) with their achievement (measured in victories); and we found that We can estimate fame grows exponentially with achievement. fame from Google; Is the same true in other areas of excellence? Bagrow et al. have studied the relationship between can this tell us 2 achievement and fame for physicists . The relationship Manfred von Richthofen (in cockpit) with members of his so- about actual they found was linear. -
A Brief History of Nuclear Astrophysics
A BRIEF HISTORY OF NUCLEAR ASTROPHYSICS PART I THE ENERGY OF THE SUN AND STARS Nikos Prantzos Institut d’Astrophysique de Paris Stellar Origin of Energy the Elements Nuclear Astrophysics Astronomy Nuclear Physics Thermodynamics: the energy of the Sun and the age of the Earth 1847 : Robert Julius von Mayer Sun heated by fall of meteors 1854 : Hermann von Helmholtz Gravitational energy of Kant’s contracting protosolar nebula of gas and dust turns into kinetic energy Timescale ~ EGrav/LSun ~ 30 My 1850s : William Thompson (Lord Kelvin) Sun heated at formation from meteorite fall, now « an incadescent liquid mass » cooling Age 10 – 100 My 1859: Charles Darwin Origin of species : Rate of erosion of the Weald valley is 1 inch/century or 22 miles wild (X 1100 feet high) in 300 My Such large Earth ages also required by geologists, like Charles Lyell A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. Homer Lane ; 1880s :August Ritter : Sun gaseous Compressible As it shrinks, it releases gravitational energy AND it gets hotter Earth Mayer – Kelvin - Helmholtz Helmholtz - Ritter A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. Homer Lane ; 1880s :August Ritter : Sun gaseous Compressible As it shrinks, it releases gravitational energy AND it gets hotter Earth Mayer – Kelvin - Helmholtz Helmholtz - Ritter A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. -
Luis Alvarez: the Ideas Man
CERN Courier March 2012 Commemoration Luis Alvarez: the ideas man The years from the early 1950s to the late 1980s came alive again during a symposium to commemorate the birth of one of the great scientists and inventors of the 20th century. Luis Alvarez – one of the greatest experimental physicists of the 20th century – combined the interests of a scientist, an inventor, a detective and an explorer. He left his mark on areas that ranged from radar through to cosmic rays, nuclear physics, particle accel- erators, detectors and large-scale data analysis, as well as particles and astrophysics. On 19 November, some 200 people gathered at Berkeley to commemorate the 100th anniversary of his birth. Alumni of the Alvarez group – among them physicists, engineers, programmers and bubble-chamber film scanners – were joined by his collaborators, family, present-day students and admirers, as well as scientists whose professional lineage traces back to him. Hosted by the Lawrence Berkeley National Laboratory (LBNL) and the University of California at Berkeley, the symposium reviewed his long career and lasting legacy. A recurring theme of the symposium was, as one speaker put it, a “Shakespeare-type dilemma”: how could one person have accom- plished all of that in one lifetime? Beyond his own initiatives, Alvarez created a culture around him that inspired others to, as George Smoot put it, “think big,” as well as to “think broadly and then deep” and to take risks. Combined with Alvarez’s strong scientific standards and great care in execut- ing them, these principles led directly to the awarding of two Nobel Luis Alvarez celebrating the announcement of his 1968 Nobel prizes in physics to scientists at Berkeley – George Smoot in 2006 prize. -
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. -
Nobel Prizes Social Network
Nobel prizes social network Marie Skłodowska Curie (Phys.1903, Chem.1911) Nobel prizes social network Henri Becquerel (Phys.1903) Pierre Curie (Phys.1903) = Marie Skłodowska Curie (Phys.1903, Chem.1911) Nobel prizes social network Henri Becquerel (Phys.1903) Pierre Curie (Phys.1903) = Marie Skłodowska Curie (Phys.1903, Chem.1911) Irène Joliot-Curie (Chem.1935) Nobel prizes social network Henri Becquerel (Phys.1903) Pierre Curie (Phys.1903) = Marie Skłodowska Curie (Phys.1903, Chem.1911) Irène Joliot-Curie (Chem.1935) = Frédéric Joliot-Curie (Chem.1935) Nobel prizes social network Henri Becquerel (Phys.1903) Pierre Curie (Phys.1903) = Marie Skłodowska Curie (Phys.1903, Chem.1911) Paul Langevin Irène Joliot-Curie (Chem.1935) = Frédéric Joliot-Curie (Chem.1935) Nobel prizes social network Henri Becquerel (Phys.1903) Pierre Curie (Phys.1903) = Marie Skłodowska Curie (Phys.1903, Chem.1911) Paul Langevin Maurice de Broglie Louis de Broglie (Phys.1929) Irène Joliot-Curie (Chem.1935) = Frédéric Joliot-Curie (Chem.1935) Nobel prizes social network Sir J. J. Thomson (Phys.1906) Henri Becquerel (Phys.1903) Pierre Curie (Phys.1903) = Marie Skłodowska Curie (Phys.1903, Chem.1911) Paul Langevin Maurice de Broglie Louis de Broglie (Phys.1929) Irène Joliot-Curie (Chem.1935) = Frédéric Joliot-Curie (Chem.1935) Nobel prizes social network (more) Sir J. J. Thomson (Phys.1906) Nobel prizes social network (more) Sir J. J. Thomson (Phys.1906) Owen Richardson (Phys.1928) Nobel prizes social network (more) Sir J. J. Thomson (Phys.1906) Owen Richardson (Phys.1928) Clinton Davisson (Phys.1937) Nobel prizes social network (more) Sir J. J. Thomson (Phys.1906) Owen Richardson (Phys.1928) Charlotte Richardson = Clinton Davisson (Phys.1937) Nobel prizes social network (more) Sir J. -
Marischal College
The Scientific Tourist: Aberdeen Marischal College George P Thomson – Nobel Prize winning physicist Sir George Paget Thomson FRS (1892-1975) was the only son of Sir J. J. Thomson, the Cavendish Professor of Physics who is probably most famous for discovering the existence of the electron and measuring its mass. G. P. Thomson was one of a select group of academics in the University of Aberdeen to be awarded the Nobel Prize. He earned it for his work in the Department of Natural Philosophy at Marischal College during his tenure from 1922-1930. There is now a commemorative plaque in the Marischal College quadrangle. Thomson was a high achieving Trinity College, Cambridge, scholar who graduated in 1913 and was elected Fellow and Lecturer at Corpus Christi College in the following year. He was, though, of the generation whose adult lives were to be shaped by two World Wars and their aftermaths. Thomson spent most of the First World War in France and in the research wing of the Royal Flying Corps. His first book1 came out of this experience and is simply entitled “Applied Aerodynamics”. It is a well-illustrated summary of the lessons of wartime work on the science of aircraft design and operation, underlining the basic physics involved. Upon Thomson’s return to Cambridge he took up research into his father’s long-standing interest of electrical discharges in gases. He brought this interest with him when he came to Aberdeen in 1922 and did much of the work enlarging J. J. Thomson’s “Conduction of Electricity through Gases” into a long awaited 3rd edition that was published in their joint names in 1928. -
Enrico Fermi
Fermi, Enrico Inventors and Inventions Enrico Fermi Italian American physicist Fermi helped develop Fermi-Dirac statistics, which liceo (secondary school) and, on the advice of Amidei, elucidate the group behavior of elementary particles. joined the Scuola Normale Superiore at Pisa. This elite He also developed the theory of beta decay and college, attached to the University of Pisa, admitted only discovered neutron-induced artificial radioactivity. forty of Italy’s top students, who were given free board Finally, he succeeded in producing the first sustained and lodging. Fermi performed exceedingly well in the nuclear chain reaction, which led to the discovery highly competitive entrance exam. He completed his of nuclear energy and the development of the university education after only four years of research and atomic bomb. studies, receiving his Ph.D. in physics from the Univer- sity of Pisa and his undergraduate diploma from the Born: September 29, 1901; Rome, Italy Scuola Normale Superiore in July, 1922. He became Died: November 28, 1954; Chicago, Illinois an expert theoretical physicist and a talented exper- Primary field: Physics imentalist. This rare combination provided a solid foun- Primary inventions: Controlled nuclear chain dation for all his subsequent inventions. reaction; Fermi-Dirac statistics; theory of beta decay Life’s Work After postdoctoral work at the University of Göttingen, Early Life in Germany (1922-1923), and the University of Leiden, Enrico Fermi (ehn-REE-koh FUR-mee) was the third in the Netherlands (fall, 1924), Fermi took an interim po- child of Alberto Fermi and Ida de Gattis. Enrico was very sition at the University of Florence in December, 1924. -
Physics 1928 OWEN WILLANS RICHARDSON
Physics 1928 OWEN WILLANS RICHARDSON <<for his work on the thermionic phenomenon and especially-for the discovery of the law named after him>> Physics 1928 Presentation Speech by Professor C. W. Oseen, Chairman of the Nobel Committee for Physics of the Royal Swedish Academy of Sciences Your Majesty, Your Royal Highnesses, Ladies and Gentlemen. Among the great problems that scientists conducting research in electro- technique are today trying to solve, is that of enabling two men to converse in whatever part of the world each may be. In 1928 things had reached the stage when we could begin to establish telephonic communication between Sweden and North America. On that occasion there was a telephone line of more than 22,000 kilometres in length between Stockholm and New York. From Stockholm, speech was transmitted via Berlin to England by means of a cable and overhead lines; from England by means of wireless to New York; then, via a cable and lines by land, over to Los Angeles and back to New York, and from there by means of a new line to Chicago, returning finally to New York. In spite of the great distance, the words could be heard distinctly and this is explained by the fact that there were no fewer than 166 amplifiers along the line. The principle of construction of an amplifier is very simple. A glowing filament sends out a stream of electrons. When the speech waves reach the amplifier, they oscillate in tune with the sound waves but are weakened. The speech waves are now made to put the stream of electrons in the same state of oscillation as they have themselves. -
EUGENE PAUL WIGNER November 17, 1902–January 1, 1995
NATIONAL ACADEMY OF SCIENCES E U G ENE PAUL WI G NER 1902—1995 A Biographical Memoir by FR E D E R I C K S E I T Z , E RICH V OG T , A N D AL V I N M. W E I NBER G 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 1998 NATIONAL ACADEMIES PRESS WASHINGTON D.C. Courtesy of Atoms for Peace Awards, Inc. EUGENE PAUL WIGNER November 17, 1902–January 1, 1995 BY FREDERICK SEITZ, ERICH VOGT, AND ALVIN M. WEINBERG UGENE WIGNER WAS A towering leader of modern physics Efor more than half of the twentieth century. While his greatest renown was associated with the introduction of sym- metry theory to quantum physics and chemistry, for which he was awarded the Nobel Prize in physics for 1963, his scientific work encompassed an astonishing breadth of sci- ence, perhaps unparalleled during his time. In preparing this memoir, we have the impression we are attempting to record the monumental achievements of half a dozen scientists. There is the Wigner who demonstrated that symmetry principles are of great importance in quan- tum mechanics; who pioneered the application of quantum mechanics in the fields of chemical kinetics and the theory of solids; who was the first nuclear engineer; who formu- lated many of the most basic ideas in nuclear physics and nuclear chemistry; who was the prophet of quantum chaos; who served as a mathematician and philosopher of science; and the Wigner who was the supervisor and mentor of more than forty Ph.D. -
Electron Microscopy
Electron microscopy 1 Plan 1. De Broglie electron wavelength. 2. Davisson – Germer experiment. 3. Wave-particle dualism. Tonomura experiment. 4. Wave: period, wavelength, mathematical description. 5. Plane, cylindrical, spherical waves. 6. Huygens-Fresnel principle. 7. Scattering: light, X-rays, electrons. 8. Electron scattering. Born approximation. 9. Electron-matter interaction, transmission function. 10. Weak phase object (WPO) approximation. 11. Electron scattering. Elastic and inelastic scattering 12. Electron scattering. Kinematic and dynamic diffraction. 13. Imaging phase objects, under focus, over focus. Transport of intensity equation. 2 Electrons are particles and waves 3 De Broglie wavelength PhD Thesis, 1924: “With every particle of matter with mass m and velocity v a real wave must be associated” h p 2 h mv p mv Ekin eU 2 2meU Louis de Broglie (1892 - 1987) – wavelength h – Planck constant hc eU – electron energy in eV eU eU2 m c2 eU m0 – electron rest mass 0 c – speed of light The Nobel Prize in Physics 1929 was awarded to Prince Louis-Victor Pierre Raymond de Broglie "for his discovery of the wave nature of electrons." 4 De Broigle “Recherches sur la Théorie des Quanta (Researches on the quantum theory)” (1924) Electron wavelength 142 pm 80 keV – 300 keV 5 Davisson – Germer experiment (1923 – 1929) The first direct evidence confirming de Broglie's hypothesis that particles can have wave properties as well 6 C. Davisson, L. H. Germer, "The Scattering of Electrons by a Single Crystal of Nickel" Nature 119(2998), 558 (1927) Davisson – Germer experiment (1923 – 1929) The first direct evidence confirming de Broglie's hypothesis that particles can have wave properties as well Clinton Joseph Davisson (left) and Lester Germer (right) George Paget Thomson Nobel Prize in Physics 1937: Davisson and Thomson 7 C. -
52 Annual Greenville County
nd 52 Annual Greenville County and South Carolina Regional 1A Science and Engineering Fair 2006 Sponsored by Rotary Club of Greenville Roper Mountain Science Center and The South Carolina Academy of Science th th st Judging- March 14 , Public Exhibition – March 15 , Award Ceremony - March 21 Palmetto EXPO Center – Greenville, South Carolina For Immediate Release March 7, 2006 Regional Science & Engineering Fair announces new Charles H. Townes Student Research Award GREENVILLE, SC – The Greenville County and South Carolina Regional Science and Engineering Fair announces a new award recognizing a local high school student for excellence in science research. The Charles H. Townes Student Research Award is the top award in the 52nd Annual Greenville County and South Carolina Regional Science & Engineering Fair to be held at the Palmetto Expo Center. The award honors the career of Greenville’s Charles H. Townes, who received the 1964 Nobel prize in Physics for his research leading to the invention of the laser. To encourage our local future scientists Dr. Townes wrote: “Being a scientist can be a wonderful career. Science involves exploration, figuring things out, understanding our universe and ourselves, and new discoveries. We live in an amazing universe, understanding it is fascinating and inspiring, and also leads to new possibilities for humans. Applied science or engineering uses our scientific understanding to provide new tools, solutions to problems, and remarkable improvements in human life. To do good science, it's helpful to learn all one can, be familiar with a variety of fields, and enjoy exploring. The more we know, the better we can fit ideas together to make new ones. -
Spectroscopy & the Nobel
Newsroom 1971 CHEMISTRY NOBEL OSA Honorary Member Gerhard Herzberg “for his contributions to the knowledge of electronic structure and geometry of molecules, particularly free radicals” 1907 PHYSICS NOBEL 1930 PHYSICS NOBEL 1966 CHEMISTRY NOBEL OSA Honorary Member Albert OSA Honorary Member Sir Robert S. Mulliken “for Abraham Michelson “for his Chandrasekhara Venkata his fundamental work optical precision instruments Raman “for his work on the concerning chemical bonds and the spectroscopic and scattering of light and for and the electronic structure metrological investigations the discovery of the effect of molecules by the carried out with their aid” named after him” molecular orbital method” 1902 PHYSICS NOBEL 1919 PHYSICS NOBEL Hendrik Antoon Lorentz and Johannes Stark “for his Pieter Zeeman “for their discovery of the Doppler researches into the influence effect in canal rays and of magnetism upon radiation the splitting of spectral phenomena” lines in electric fields” 1955 PHYSICS NOBEL OSA Honorary Member Willis Eugene Lamb “for his discoveries concerning the fine structure of the hydrogen Spectroscopy spectrum” & the Nobel ctober is when scientists around the world await the results from Stockholm. O Since the Nobel Prize was established in 1895, a surprising number of the awards have gone to advances related to or enabled by spectroscopy—from the spectral splitting of the Zeeman and Stark effects to cutting-edge advances enabled by laser frequency combs. We offer a small (and far from complete) sample here; to explore further, visit www.nobelprize.org. 16 OPTICS & PHOTONICS NEWS OCTOBER 2018 1996 CHEMISTRY NOBEL OSA Fellow Robert F. Curl Jr., Richard Smalley and Harold 1999 CHEMISTRY NOBEL Kroto (not pictured) “for their Ahmed H.