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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. -
Remembering Alvin Tollestrup: 1924-2020 – CERN Courier
3/26/2020 Remembering Alvin Tollestrup: 1924-2020 – CERN Courier PEOPLE | NEWS Remembering Alvin Tollestrup: 1924-2020 6 March 2020 Alvin Tollestrup, who passed away on 9 February at the age of 95, was a visionary. When I joined his group at Caltech in the summer of 1960, experiments in particle physics at universities were performed at accelerators located on campus. Alvin had helped build Caltech’s electron synchrotron, the highest energy photon-producing accelerator at the time. But he thought more exciting physics could be performed elsewhere, and managed to get approval to run an experiment at Berkeley Lab’s Bevatron to measure a rare decay mode of the K+ meson. This was the rst time an outsider was allowed to access Berkeley’s machine, much to the consternation of Luis Alvarez and other university faculty. When I joined Alvin’s group he asked a postdoc, Ricardo Gomez, and me to design, build and test https://cerncourier.com/a/remembering-alvin-tollestrup-1924-2020/ 1/5 3/26/2020 Remembering Alvin Tollestrup: 1924-2020 – CERN Courier Machine maestro – Alvin Tollestrup led the pioneering a new type of particle detector called a spark work of designing and testing the superconducting magnets for the Tevatron, the rst large-scale chamber. He gave us a paper by two Japanese application of superconductivity. Credit: Fermilab authors on “A new type of particle detector: the discharge chamber”, not what he wanted, but a place to start. In retrospect it was remarkable that Alvin was willing to risk the success of his experiment on the creation of new technology. -
ANTIMATTER a Review of Its Role in the Universe and Its Applications
A review of its role in the ANTIMATTER universe and its applications THE DISCOVERY OF NATURE’S SYMMETRIES ntimatter plays an intrinsic role in our Aunderstanding of the subatomic world THE UNIVERSE THROUGH THE LOOKING-GLASS C.D. Anderson, Anderson, Emilio VisualSegrè Archives C.D. The beginning of the 20th century or vice versa, it absorbed or emitted saw a cascade of brilliant insights into quanta of electromagnetic radiation the nature of matter and energy. The of definite energy, giving rise to a first was Max Planck’s realisation that characteristic spectrum of bright or energy (in the form of electromagnetic dark lines at specific wavelengths. radiation i.e. light) had discrete values The Austrian physicist, Erwin – it was quantised. The second was Schrödinger laid down a more precise that energy and mass were equivalent, mathematical formulation of this as described by Einstein’s special behaviour based on wave theory and theory of relativity and his iconic probability – quantum mechanics. The first image of a positron track found in cosmic rays equation, E = mc2, where c is the The Schrödinger wave equation could speed of light in a vacuum; the theory predict the spectrum of the simplest or positron; when an electron also predicted that objects behave atom, hydrogen, which consists of met a positron, they would annihilate somewhat differently when moving a single electron orbiting a positive according to Einstein’s equation, proton. However, the spectrum generating two gamma rays in the featured additional lines that were not process. The concept of antimatter explained. In 1928, the British physicist was born. -
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. -
Particle Detectors Lecture Notes
Lecture Notes Heidelberg, Summer Term 2011 The Physics of Particle Detectors Hans-Christian Schultz-Coulon Kirchhoff-Institut für Physik Introduction Historical Developments Historical Development γ-rays First 1896 Detection of α-, β- and γ-rays 1896 β-rays Image of Becquerel's photographic plate which has been An x-ray picture taken by Wilhelm Röntgen of Albert von fogged by exposure to radiation from a uranium salt. Kölliker's hand at a public lecture on 23 January 1896. Historical Development Rutherford's scattering experiment Microscope + Scintillating ZnS screen Schematic view of Rutherford experiment 1911 Rutherford's original experimental setup Historical Development Detection of cosmic rays [Hess 1912; Nobel prize 1936] ! "# Electrometer Cylinder from Wulf [2 cm diameter] Mirror Strings Microscope Natrium ! !""#$%&'()*+,-)./0)1&$23456/)78096$/'9::9098)1912 $%&!'()*+,-.%!/0&1.)%21331&10!,0%))0!%42%!56784210462!1(,!9624,10462,:177%&!(2;! '()*+,-.%2!<=%4*1;%2%)%:0&67%0%&!;1&>!Victor F. Hess before his 1912 balloon flight in Austria during which he discovered cosmic rays. ?40! @4)*%! ;%&! /0%)),-.&1(8%! A! )1,,%2! ,4-.!;4%!BC;%2!;%,!D)%:0&67%0%&,!(7!;4%! EC2F,1-.,%!;%,!/0&1.)%21331&10,!;&%.%2G!(7!%42%!*H&!;4%!A8)%,(2F!FH2,04F%!I6,40462! %42,0%))%2! J(! :K22%2>! L10&4(7! =4&;! M%&=%2;%0G! (7! ;4%! E(*0! 47! 922%&%2! ;%,! 9624,10462,M6)(7%2!M62!B%(-.04F:%40!*&%4!J(!.1)0%2>! $%&!422%&%G!:)%42%&%!<N)42;%&!;4%20!;%&!O8%&3&H*(2F!;%&!9,6)10462!;%,!P%&C0%,>!'4&;!%&! H8%&! ;4%! BC;%2! F%,%2:0G! ,6! M%&&42F%&0! ,4-.!;1,!1:04M%!9624,10462,M6)(7%2!1(*!;%2! -
Accelerator Disaster Scenarios, the Unabomber, and Scientific Risks
Accelerator Disaster Scenarios, the Unabomber, and Scientific Risks Joseph I. Kapusta∗ Abstract The possibility that experiments at high-energy accelerators could create new forms of matter that would ultimately destroy the Earth has been considered several times in the past quarter century. One consequence of the earliest of these disaster scenarios was that the authors of a 1993 article in Physics Today who reviewed the experi- ments that had been carried out at the Bevalac at Lawrence Berkeley Laboratory were placed on the FBI's Unabomber watch list. Later, concerns that experiments at the Relativistic Heavy Ion Collider at Brookhaven National Laboratory might create mini black holes or nuggets of stable strange quark matter resulted in a flurry of articles in the popular press. I discuss this history, as well as Richard A. Pos- ner's provocative analysis and recommendations on how to deal with such scientific risks. I conclude that better communication between scientists and nonscientists would serve to assuage unreasonable fears and focus attention on truly serious potential threats to humankind. Key words: Wladek Swiatecki; Subal Das Gupta; Gary D. Westfall; Theodore J. Kaczynski; Frank Wilczek; John Marburger III; Richard A. Posner; Be- valac; Relativistic Heavy Ion Collider (RHIC); Large Hadron Collider (LHC); Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; CERN; Unabomber; Federal Bureau of Investigation; nuclear physics; accel- erators; abnormal nuclear matter; density isomer; black hole; strange quark matter; scientific risks. arXiv:0804.4806v1 [physics.hist-ph] 30 Apr 2008 ∗Joseph I. Kapusta received his Ph.D. degree at the University of California at Berkeley in 1978 and has been on the faculty of the School of Physics and Astronomy at the University of Minnesota since 1982. -
Chirped Pulse Amplification, CPA, Was Both Simple and Elegant
THE NOBEL PRIZE IN PHYSICS 2018 POPULAR SCIENCE BACKGROUND Tools made of light The inventions being honoured this year have revolutionised laser physics. Extremely small objects and incredibly fast processes now appear in a new light. Not only physics, but also chemistry, biology and medicine have gained precision instruments for use in basic research and practical applications. Arthur Ashkin invented optical tweezers that grab particles, atoms and molecules with their laser beam fingers. Viruses, bacteria and other living cells can be held too, and examined and manipulated without being damaged. Ashkin’s optical tweezers have created entirely new opportunities for observing and controlling the machinery of life. Gérard Mourou and Donna Strickland paved the way towards the shortest and most intense laser pulses created by mankind. The technique they developed has opened up new areas of research and led to broad industrial and medical applications; for example, millions of eye operations are performed every year with the sharpest of laser beams. Travelling in beams of light Arthur Ashkin had a dream: imagine if beams of light could be put to work and made to move objects. In the cult series that started in the mid-1960s, Star Trek, a tractor beam can be used to retrieve objects, even asteroids in space, without touching them. Of course, this sounds like pure science fic- tion. We can feel that sunbeams carry energy – we get hot in the sun – although the pressure from the beam is too small for us to feel even a tiny prod. But could its force be enough to push extremely tiny particles and atoms? Immediately after the invention of the first laser in 1960, Ashkin began to experiment with the new instrument at Bell Laboratories outside New York. -
The Donald A. Glaser Papers, 1943-2013, Bulk 1949-2003
http://oac.cdlib.org/findaid/ark:/13030/c8n01cbt No online items Finding Aid for the Donald A. Glaser Papers, 1943-2013, bulk 1949-2003 Bianca Rios and Mariella Soprano California Institute of Technology. Caltech Archives ©2017 1200 East California Blvd. Mail Code B215A-74 Pasadena, CA 91125 [email protected] URL: http://archives.caltech.edu/ Finding Aid for the Donald A. 10285-MS 1 Glaser Papers, 1943-2013, bulk 1949-2003 Language of Material: English Contributing Institution: California Institute of Technology. Caltech Archives Title: The Donald A. Glaser papers creator: Glaser, Donald Arthur Identifier/Call Number: 10285-MS Physical Description: 15.97 Linear feet (41 boxes) Date (inclusive): 1918-2016, bulk 1949-2003 Abstract: Donald Arthur Glaser (1926 – 2013) earned his PhD in Physics and Mathematics from the California Institute of Technology in 1950 and won the 1960 Nobel Prize in Physics for his invention of the bubble chamber. He then changed his research focus to molecular biology and went on to co-found Cetus Corporation, the first biotechnology company. In the 1980s he again switched his focus to neurobiology and the visual system. The Donald A. Glaser papers consist of research notes and notebooks, manuscripts and printed papers, correspondence, awards, biographical material, photographs, audio-visual material, and born-digital files. Conditions Governing Access The collection is open for research. Researchers must apply in writing for access. General The collection is fully digitized and will be made available online by the beginning of 2018. Conditions Governing Use Copyright may not have been assigned to the California Institute of Technology Archives. -
JUAN MANUEL 2016 NOBEL PEACE PRIZE RECIPIENT Culture Friendship Justice
Friendship Volume 135, № 1 Character Culture JUAN MANUEL SANTOS 2016 NOBEL PEACE PRIZE RECIPIENT Justice LETTER FROM THE PRESIDENT Dear Brothers, It is an honor and a privilege as your president to have the challenges us and, perhaps, makes us question our own opportunity to share my message with you in each edition strongly held beliefs. But it also serves to open our minds of the Quarterly. I generally try to align my comments and our hearts to our fellow neighbor. It has to start with specific items highlighted in each publication. This with a desire to listen, to understand, and to be tolerant time, however, I want to return to the theme “living our of different points of view and a desire to be reasonable, Principles,” which I touched upon in a previous article. As patient and respectful.” you may recall, I attempted to outline and describe how Kelly concludes that it is the diversity of Southwest’s utilization of the Four Founding Principles could help people and “treating others like you would want to be undergraduates make good decisions and build better treated” that has made the organization successful. In a men. It occurred to me that the application of our values similar way, Stephen Covey’s widely read “Seven Habits of to undergraduates only is too limiting. These Principles are Highly Effective People” takes a “values-based” approach to indeed critical for each of us at this particularly turbulent organizational success. time in our society. For DU to be a successful organization, we too, must As I was flying back recently from the Delta Upsilon be able to work effectively with our varied constituents: International Fraternity Board of Directors meeting in undergraduates, parents, alumni, higher education Arizona, I glanced through the February 2017 edition professionals, etc. -
Muonium Gravity Seminar Wichita-6-17
Antimatter Gravity MICE-U.S. Plans withDaniel Muons M. Kaplan US Spokesperson, MICE Collaboration Daniel M. Kaplan Physics Seminar WichitaMuTAC State Review Univ. June Fermilab16, 2017 16–17 March, 2006 Outline • Dramatis Personae • A Bit of History - antimatter, the baryon asymmetry of the universe, and all that... • The Ideas, The Issues, The Opportunities • Required R&D • Conclusions Our story’s a bit complicated, so please bear with me! ...and stop me if you have a question! D. M. Kaplan, IIT An#ma&er Gravity Seminar 2/41 Matter & Energy • After many decades of experimentation with subatomic particles, we now know whatDramatis everything is made of... Personae Baryons & antibaryons : p== uud & p uud ΛΛ==uds & uds ... Mesons : K00== ds & K ds B00== db & B db B+ == ub & B− ub ... ∓ ∓ ∓ Leptons : e , µ , τ , ν’s D. M. Kaplan, IIT An#ma&er Gravity Seminar 3/41 Matter & Energy • After many decades of experimentation with subatomic particles, we now know whatDramatis everything is made of... Personae “Imperfect mirror” Baryons & antibaryons : Antip== uud & p uud ΛΛ==uds & uds ... Mesons : Anti K00== ds & K ds B00== db & B db Anti B+ == ub & B− ub ... Antimatter Leptons : e∓, µ∓, τ∓, ν’s • And, don’t forget: antimatter and matter annihilate on contact D. M. Kaplan, IIT An#ma&er Gravity Seminar 3/41 Outline • Dramatis Personae ➡ • A Bit of History - antimatter, the baryon asymmetry of the universe, and all that... • The Ideas, The Issues, The Opportunities • Muonium Gravity Experiment • Required R&D • Conclusions D. M. Kaplan, IIT An#ma&er Gravity Seminar 4/41 Our story begins with.. -
Nfap Policy Brief » October 2019
NATIONAL FOUNDATION FOR AMERICAN POLICY NFAP POLICY BRIEF» OCTOBER 2019 IMMIGRANTS AND NOBEL PRIZES : 1901- 2019 EXECUTIVE SUMMARY Immigrants have been awarded 38%, or 36 of 95, of the Nobel Prizes won by Americans in Chemistry, Medicine and Physics since 2000.1 In 2019, the U.S. winner of the Nobel Prize in Physics (James Peebles) and one of the two American winners of the Nobel Prize in Chemistry (M. Stanley Whittingham) were immigrants to the United States. This showing by immigrants in 2019 is consistent with recent history and illustrates the contributions of immigrants to America. In 2018, Gérard Mourou, an immigrant from France, won the Nobel Prize in Physics. In 2017, the sole American winner of the Nobel Prize in Chemistry was an immigrant, Joachim Frank, a Columbia University professor born in Germany. Immigrant Rainer Weiss, who was born in Germany and came to the United States as a teenager, was awarded the 2017 Nobel Prize in Physics, sharing it with two other Americans, Kip S. Thorne and Barry C. Barish. In 2016, all 6 American winners of the Nobel Prize in economics and scientific fields were immigrants. Table 1 U.S. Nobel Prize Winners in Chemistry, Medicine and Physics: 2000-2019 Category Immigrant Native-Born Percentage of Immigrant Winners Physics 14 19 42% Chemistry 12 21 36% Medicine 10 19 35% TOTAL 36 59 38% Source: National Foundation for American Policy, Royal Swedish Academy of Sciences, George Mason University Institute for Immigration Research. Between 1901 and 2019, immigrants have been awarded 35%, or 105 of 302, of the Nobel Prizes won by Americans in Chemistry, Medicine and Physics. -
Modern Physics, the Nature of the Interaction Between Particles Is Carried a Step Further
44.1 Some Properties of Nuclei 1385 are the same, apart from the additional repulsive Coulomb force for the proton– U(r ) (MeV) proton interaction. 40 Evidence for the limited range of nuclear forces comes from scattering experi- n–p system ments and from studies of nuclear binding energies. The short range of the nuclear 20 force is shown in the neutron–proton (n–p) potential energy plot of Figure 44.3a 0 r (fm) obtained by scattering neutrons from a target containing hydrogen. The depth of 1 567432 8 the n–p potential energy well is 40 to 50 MeV, and there is a strong repulsive com- Ϫ20 ponent that prevents the nucleons from approaching much closer than 0.4 fm. Ϫ40 The nuclear force does not affect electrons, enabling energetic electrons to serve as point-like probes of nuclei. The charge independence of the nuclear force also Ϫ60 means that the main difference between the n–p and p–p interactions is that the a p–p potential energy consists of a superposition of nuclear and Coulomb interactions as shown in Figure 44.3b. At distances less than 2 fm, both p–p and n–p potential The difference in the two curves energies are nearly identical, but for distances of 2 fm or greater, the p–p potential is due to the large Coulomb has a positive energy barrier with a maximum at 4 fm. repulsion in the case of the proton–proton interaction. The existence of the nuclear force results in approximately 270 stable nuclei; hundreds of other nuclei have been observed, but they are unstable.