Physics, Lasers and the Nobel Prize
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Unrestricted Immigration and the Foreign Dominance Of
Unrestricted Immigration and the Foreign Dominance of United States Nobel Prize Winners in Science: Irrefutable Data and Exemplary Family Narratives—Backup Data and Information Andrew A. Beveridge, Queens and Graduate Center CUNY and Social Explorer, Inc. Lynn Caporale, Strategic Scientific Advisor and Author The following slides were presented at the recent meeting of the American Association for the Advancement of Science. This project and paper is an outgrowth of that session, and will combine qualitative data on Nobel Prize Winners family histories along with analyses of the pattern of Nobel Winners. The first set of slides show some of the patterns so far found, and will be augmented for the formal paper. The second set of slides shows some examples of the Nobel families. The authors a developing a systematic data base of Nobel Winners (mainly US), their careers and their family histories. This turned out to be much more challenging than expected, since many winners do not emphasize their family origins in their own biographies or autobiographies or other commentary. Dr. Caporale has reached out to some laureates or their families to elicit that information. We plan to systematically compare the laureates to the population in the US at large, including immigrants and non‐immigrants at various periods. Outline of Presentation • A preliminary examination of the 609 Nobel Prize Winners, 291 of whom were at an American Institution when they received the Nobel in physics, chemistry or physiology and medicine • Will look at patterns of -
Donna Strickland '89 (Phd), a Self-Described “Laser Jock,” Receives
Donna Strickland ’89 (PhD), a self-described “laser jock,” receives the Nobel Prize, along with her advisor, Gérard Mourou, for work they did at the Laboratory for Laser Energetics. By Lindsey Valich Donna Strickland ’89 (PhD) still recalls the visit she took to the On- tario Science Centre when she was a child growing up in the town of Guelph, outside Toronto. Her father pointed to a laser display. “ ‘Donna, this is the way of the future,’ ” Strickland remembers him telling her. Lloyd Strickland, an electrical engineer, along with Donna’s moth- er, sister, and brother, was part of the family that “continually sup- ported and encouraged me through all my years of education,” Donna Strickland wrote in the acknowledgments of her PhD thesis, “De- velopment of an Ultra-Bright Laser and an Application to Multi- Photon Ionization.” She was captivated by that laser display. And since then, she says, “I’ve always thought lasers were cool.” Her passion for laser science research and her commitment to be- ing a “laser jock,” as she has called herself, has led her across North America, from Canada to the United States and back again. But it’s the work that she did as a graduate student at Rochester in the 1980s that has earned her the remarkable accolade of Nobel Prize laureate. When Strickland entered the University’s graduate program in op- tics, laser physicists were grappling with a thorny problem: how could they create ultrashort, high-intensity laser pulses that wouldn’t de- stroy the very material the laser was used to explore in the first place? Working with former Rochester engineering professor Gérard Mourou, Strickland developed and made workable a method to over- come the barrier. -
Fotonica Ed Elettronica Quantistica
Fotonica ed elettronica quantistica http://www.dsf.unica.it/~fotonica/teaching/fotonica.html Fotonica ed elettronica quantistica Quantum optics - Quantization of electromagnetic field - Statistics of light, photon counting and noise; - HBT and correlation; g1 e g2 coherence; antibunching; single photons - Squeezing - Quantum cryptography - Quantum computer, entanglement and teleportation Light-matter Interaction - Two-level atom - Laser physics - Spectroscopy - Electronics and photonics at the nanometer scale - Cold atoms - Photodetectors - Solar cells http://www.dsf.unica.it/~fotonica/teaching/fotonica.html Energy Temperature LHC at CERN, Higgs, SUSY, ??? TeV 15 q q particle accelerators 10 K q GeV proton rest mass - quarks 1012K MeV electron rest mass / gamma rays 109K keV Nuclear Fusion, x rays, Sun center 106K Atoms ionize - visible light eV Sun surface fundamental components components fundamental room temperature 103K meV Liquid He, superconductors, space 1K dilution refrigerators, quantum Hall µeV laser-cooled atoms 10-3K neV Bose-Einstein condensates 10-6K peV low T record 480 picokelvin 10-9K -12 complexity, organization organization complexity, 10 K Nobel Prizes in Physics 2010 - Andre Geims, Konstantin Novoselov 2009 - Charles K. Kao, Willard S. Boyle, George E. Smith 2007 - Albert Fert, Peter Gruenberg 2005 - Roy J. Glauber, John L. Hall, Theodor W. Hänsch 2001 - Eric A. Cornell, Wolfgang Ketterle, Carl E. Wieman 1997 - Steven Chu, Claude Cohen-Tannoudji, William D. Phillips 1989 - Norman F. Ramsey, Hans G. Dehmelt, Wolfgang Paul 1981 - Nicolaas Bloembergen, Arthur L. Schawlow, Kai M. Siegbahn 1966 - Alfred Kastler 1964 - Charles H. Townes, Nicolay G. Basov, Aleksandr M. Prokhorov 1944 - Isidor Isaac Rabi 1930 - Venkata Raman 1921 - Albert Einstein 1907 - Albert A. -
DONNA STRICKLAND, PH.D. Professor, University of Waterloo
DONNA STRICKLAND, PH.D. Professor, University of Waterloo Donna Strickland is a professor in the Department of Physics and Astronomy at the University of Waterloo and is one of the recipients of the Nobel Prize in Physics 2018 for developing chirped pulse amplification with Gérard Mourou, her PhD supervisor at the time. They published this Nobel-winning research in 1985 when Strickland was a PhD student at the University of Rochester in New York state. Together they paved the way toward the most intense laser pulses ever created. The research has several applications today in industry and medicine — including the cutting of a patient’s cornea in laser eye surgery, and the machining of small glass parts for use in cell phones. Strickland was a research associate at the National Research Council Canada, a physicist at Lawrence Livermore National Laboratory and a member of technical staff at Princeton University. In 1997, she joined the University of Waterloo, where her ultrafast laser group develops high-intensity laser systems for nonlinear optics investigations. Strickland was named a Companion of the Order of Canada. She is a recipient of a Sloan Research Fellowship, a Premier’s Research Excellence Award and a Cottrell Scholar Award. She received the Rochester Distinguished Scholar Award and the Eastman Medal from the University of Rochester. Strickland served as the president of the Optical Society (OSA) in 2013 and is a fellow of OSA, the Royal Society of Canada, and SPIE (International Society for Optics and Photonics). She is an honorary fellow of the Canadian Academy of Engineering as well as the Institute of Physics. -
Nobel Laureates Endorse Joe Biden
Nobel Laureates endorse Joe Biden 81 American Nobel Laureates in Physics, Chemistry, and Medicine have signed this letter to express their support for former Vice President Joe Biden in the 2020 election for President of the United States. At no time in our nation’s history has there been a greater need for our leaders to appreciate the value of science in formulating public policy. During his long record of public service, Joe Biden has consistently demonstrated his willingness to listen to experts, his understanding of the value of international collaboration in research, and his respect for the contribution that immigrants make to the intellectual life of our country. As American citizens and as scientists, we wholeheartedly endorse Joe Biden for President. Name Category Prize Year Peter Agre Chemistry 2003 Sidney Altman Chemistry 1989 Frances H. Arnold Chemistry 2018 Paul Berg Chemistry 1980 Thomas R. Cech Chemistry 1989 Martin Chalfie Chemistry 2008 Elias James Corey Chemistry 1990 Joachim Frank Chemistry 2017 Walter Gilbert Chemistry 1980 John B. Goodenough Chemistry 2019 Alan Heeger Chemistry 2000 Dudley R. Herschbach Chemistry 1986 Roald Hoffmann Chemistry 1981 Brian K. Kobilka Chemistry 2012 Roger D. Kornberg Chemistry 2006 Robert J. Lefkowitz Chemistry 2012 Roderick MacKinnon Chemistry 2003 Paul L. Modrich Chemistry 2015 William E. Moerner Chemistry 2014 Mario J. Molina Chemistry 1995 Richard R. Schrock Chemistry 2005 K. Barry Sharpless Chemistry 2001 Sir James Fraser Stoddart Chemistry 2016 M. Stanley Whittingham Chemistry 2019 James P. Allison Medicine 2018 Richard Axel Medicine 2004 David Baltimore Medicine 1975 J. Michael Bishop Medicine 1989 Elizabeth H. Blackburn Medicine 2009 Michael S. -
Having a Good Time: a Triumph of Science & Technology
UDC’s Office of Research & Graduate Studies, SEAS, LSAMP, & STEM Center Invite You to a Seminar on Having a Good Time: A Triumph of Science & Technology Presented by Dr. William D. Phillips, NIST Nobel Laureate in Physics, 1997 © Robert Rathe © Robert Rathe Date: Tuesday, March 13, 2012 Time: 12:30 PM Location: Building 41-A03 Abstract: People have long been interested in timekeeping. In the 18th century, this interest became particularly keen because of technological demands: the need for accurate navigation on the high seas. While many people believed that the answer to sufficiently good timekeeping at sea would be found in astronomical measurements, it was earthbound engineering that literally won the prize. The construction of accurate seagoing clocks revolutionized navigation in the 18th and 19th centuries. The advent of even more accurate clocks—atomic clocks—in the 20th century gave birth to a new revolution in navigation—the Global Positioning System. This ever-more advanced system for satellite navigation owes its success both to excellent engineering and to seemingly arcane science. Dr. William D. Phillips is a Senior Fellow at the National Institute of Standards and Technology (NIST), where he leads the Laser Cooling and Trapping Group. He shared the 1997 Nobel Prize in physics with Dr. Steven Chu, now Secretary of Energy, and with Dr. Claude Cohen-Tannoudji, an Algerian-born French physicist, “for development of methods to cool and trap atoms with laser light.” With a physics bachelor’s degree from Juniata College in Pennsylvania and a Ph.D. from MIT, Phillips started his career at NIST only a few years after it left UDC’s Van Ness campus for its location in Gaithersburg. -
Calcium and Potassium Spectra in the EUV
atoms Review Calcium and Potassium Spectra in the EUV Elmar Träbert Fakultät für Physik und Astronomie, Ruhr-Universität Bochum, AIRUB, 44780 Bochum, Germany; [email protected]; Tel.: +49-234-322-3451; Fax: +49-234-321-4169 Received: 28 August 2020; Accepted: 2 October 2020; Published: 14 October 2020 Abstract: In online data bases, the entries on extreme ultraviolet (EUV) spectra of Ca are much more sparse than those of neighbouring elements such as Ar, K, Sc and Ti. This may be a result of experimental problems with Ca in the laboratory as well as of the limited role of multiply charged Ca ions in solar observations. Beam-foil EUV spectra of Ca and K are presented that provide survey data of a single element each. Keywords: atomic physics; EUV spectra; beam-foil spectroscopy 1. Introduction Early in the 19th century Wollaston and Fraunhofer detected dark lines in their prism spectra of the Sun, and Fraunhofer labelled the strongest of these lines by capital letters of the alphabet. A few decades later Kirchhoff and Bunsen recognized that those dark lines agreed in position with bright lines in the spectra of a flame seeded with specific materials. Thus it was eventually learned that Fraunhofer’s line ‘G’ (partly) originates from calcium (Ca, atomic number Z = 20) atoms, and his lines ‘H’ and ‘K’ belong to singly charged Ca+ ions. Evidently, Ca is abundant enough in the Sun to feature prominently in the solar visible spectrum. Subsequently, the various spectra of Ca have been studied in flames, arcs, sparks, and whatever plasma discharge light sources seemed appropriate, and the extent of the spectral coverage has expanded from the visible to the infrared (IR), ultraviolet (UV), vacuum ultraviolet (VUV, wavelengths below 200 nm), and extreme ultraviolet (EUV, wavelengths below 110 nm) to the X-ray range (wavelengths shorter than, say, 5 nm). -
Slides for 1920 and 1928)
Quantum Theory Matters with thanks to John Clarke Slater (1900{1976), Per-Olov L¨owdin(1916{2000), and the many members of QTP (Gainesville, FL, USA) and KKUU (Uppsala, Sweden) Nelson H. F. Beebe Research Professor University of Utah Department of Mathematics, 110 LCB 155 S 1400 E RM 233 Salt Lake City, UT 84112-0090 USA Email: [email protected], [email protected], [email protected] (Internet) WWW URL: http://www.math.utah.edu/~beebe Telephone: +1 801 581 5254 FAX: +1 801 581 4148 Nelson H. F. Beebe (University of Utah) QTM 11 November 2015 1 / 1 11 November 2015 The periodic table of elements All from H (1) to U (92), except Tc (43) and Pm (61), are found on Earth. Nelson H. F. Beebe (University of Utah) QTM 11 November 2015 2 / 1 Correcting a common misconception Scientific Theory: not a wild @$$#% guess, but rather a mathematical framework that allows actual calculation for known systems, and prediction for unknown ones. Nelson H. F. Beebe (University of Utah) QTM 11 November 2015 3 / 1 Scientific method Theories should be based on minimal sets of principles, and be free of preconceived dogmas, no matter how widely accepted. [Remember Archimedes, Socrates, Hypatia, Galileo, Tartaglia, Kepler, Copernicus, Lavoisier, . ] Open publication and free discussion of physical theories and experimental results, so that others can criticize them, improve them, and reproduce them. Know who pays for the work, and judge accordingly! Science must have public support. History shows that such support is paid back many times over. If it ain't repeatable, it ain't science! Nelson H. -
Spectroscopy
Chapter 1, page 1 Spectroscopy An Introduction to the Theoretical and Experimental Fundamentals 1 Introduction In the year 1666 at Cambridge, Isaac Newton procured a triangular glass prism and let a ray of sunlight from a small round hole in the window illuminate it. He observed the image created thereby on a paper screen. The white light from the window dissociated into red, yellow, green, blue, and violet. He called the invisible colors in the white sunlight the “spectrum” (lat spectrum = image in the soul) [1]. It was at the end of the 19th century that the observation of spectra was first christened “Spectroscopy”. This word has both a Latin and Greek root (Greek skopein = to look). Arthur Schuster first used the term spectroscopy in 1882 during a lecture at the Royal Institution [2]. Newton led the way from speculation to spectral analysis by making exact measurement and having clear insights. The oldest observation of nature dealing with the properties of invisible light comes to us from the Roman scholar and philosopher Titus Carus Lucretius. Infrared spectroscopists therefore consider him to be their intellectual father. Around 60 B.C. he hypothesized the existence of infrared radiation: [3]: »Forsitan et rosea sol alte lampade lucens possideat multum caecis fervoribus ignem circum se, nullo qui sit fulgore notatus, aestifer ut tantum radiorum exaugeat ictum.« (original Latin) or freely translated into English: »Perhaps the sun, shining above with rosy lamp is surrounded by much fire and invisible heat. Thus the fire may be accompanied by radiance which increases the power of rays.« or translated by Knebel [3] into German: »Mag es auch sein, dass hoch die rosige Fackel der Sonne ringsum Feuer verbirgt in düsteren unscheinbaren Gluten, die beitragen, die Macht so heftiger Strahlen zu mehren«. -
Laser Spectroscopy to Resolve Hyperfine Structure of Rubidium
Laser spectroscopy to resolve hyperfine structure of rubidium Hannah Saddler, Adam Egbert, and Will Weigand (Dated: 12 November 2015) This experiment had two main goals: to create an absorption spectrum for rubidium using the technique of absorption spectroscopy and to resolve the hyperfine structures for the two rubidium isotopes using saturation absorption spectroscopy. The absorption spectrum was used to determine the frequency difference between the ground state and first excited state for both isotopes. The calculated frequency difference was 6950 MHz ± 90 MHz for rubidium 87 and 3060 MHz ± 60 MHz for rubidium 85. Both values agree with the literature values. The hyperfine structure for rubidium 87 was able to be resolved using this experimental setup. The energy differences were determined to be 260 MHz ± 10 MHz and 150 MHz ± 10 Mhz MHz. The hyperfine structure for rubidium 85 was unable to be resolved using this experimental setup. Additionally the theory of doppler broadening was used to make measurements of the full width half maximum. These values were used to calculate a temperature of 310K ± 40 K which makes sense because the experiments were performed at room temperature. I. INTRODUCTION in the theory section and how they were manipulated and used to derive the results from the recorded data. Addi- tionally there is an explanation of experimental error and The era of modern spectroscopy began with the in- uncertainty associated the results. Section V is a conclu- vention of the laser. The word laser was originally an sion that ties the results of the experiment we performed acronym that stood for light amplification by stimulated to the usefulness of the technique of laser spectroscopy. -
Arthur Ashkin (1922 - 2020)
September 2020 IN MEMORIAM Arthur Ashkin (1922 - 2020) Arthur Ashkin, IEEE Life Fellow, Throughout his life, Art also never failed to considered “the father of optical tweezers” mention the contributions of his for which he was awarded the Nobel Prize colleagues at Bell Labs that helped him in Physics 2018, has passed away at the achieve scientific breakthroughs, age of 98. especially his assistant Joseph Dziedzic. The IEEE Photonics Society and its And, the most significant support Ashkin members mourn this great loss of a friend, ever received is from Aline, his wife of 66 colleague and pioneer in the fields of years, who he met in college at Cornell optics and photonics. University. She herself is well trained in chemistry and taught at Holmdel High Art, as he was known in the community, School in New Jersey. One can find a worked most of his career at AT&T Bell comprehensive historical account of the Laboratories, from 1952 to 1991. There he scientific development of optical trapping began his work on manipulation of in a book written by Ashkin with the help microparticles with laser light in the late of Aline. 1960s which resulted in the invention of optical tweezers in 1986. He also Together, he and Aline raised three pioneered the optical trapping process. children and five grandchildren. Such traps have found a wide range of important and unique applications. They Ashkin was a mentor, collaborator, and are used to manipulate small objects friend to many within the scientific down to the size of atoms. community. René-Jean Essiambre, a close friend and mentee who presented This includes “small living things”, as the Nobel Lecture in Physics for Ashkin in Ashkin liked to say, such as viruses, 2018, expressed the profound impact he bacteria, living cells, organelles within had on the optics and photonics fields. -
Outline of Physical Science
Outline of physical science “Physical Science” redirects here. It is not to be confused • Astronomy – study of celestial objects (such as stars, with Physics. galaxies, planets, moons, asteroids, comets and neb- ulae), the physics, chemistry, and evolution of such Physical science is a branch of natural science that stud- objects, and phenomena that originate outside the atmosphere of Earth, including supernovae explo- ies non-living systems, in contrast to life science. It in turn has many branches, each referred to as a “physical sions, gamma ray bursts, and cosmic microwave background radiation. science”, together called the “physical sciences”. How- ever, the term “physical” creates an unintended, some- • Branches of astronomy what arbitrary distinction, since many branches of physi- cal science also study biological phenomena and branches • Chemistry – studies the composition, structure, of chemistry such as organic chemistry. properties and change of matter.[8][9] In this realm, chemistry deals with such topics as the properties of individual atoms, the manner in which atoms form 1 What is physical science? chemical bonds in the formation of compounds, the interactions of substances through intermolecular forces to give matter its general properties, and the Physical science can be described as all of the following: interactions between substances through chemical reactions to form different substances. • A branch of science (a systematic enterprise that builds and organizes knowledge in the form of • Branches of chemistry testable explanations and predictions about the • universe).[1][2][3] Earth science – all-embracing term referring to the fields of science dealing with planet Earth. Earth • A branch of natural science – natural science science is the study of how the natural environ- is a major branch of science that tries to ex- ment (ecosphere or Earth system) works and how it plain and predict nature’s phenomena, based evolved to its current state.