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Stephan Hruszkewycz Tuesday, September 25 • 4 Pm • Tech L211
THE MATERIALS SCIENCE AND ENGINEERING DEPARTMENT COLLOQUIUM SERIES PRESENTS: Stephan Hruszkewycz Assistant Physicist, Argonne National Laboratory Opportunities for materials science with coherent x-ray diffraction imaging Recent progress in 3D coherent x-ray diffraction imaging methods can enable high resolution structural imaging of nano-structured crystalline materials under operating conditions. In this talk, I discuss developments in Bragg coherent diffraction imaging (BCDI) that aim to broaden the envelope of materials science problems that can be addressed with the technique. Following an introduction of the basic principles of the method, two specific topics will be discussed: 1) BCDI at high x-ray energies that provide dramatic penetrating ability, 2) Bragg ptychography that enable imaging of targeted sub- volumes of a crystal. Both approaches will be discussed in the context of materials science problems that can be addressed in-situ at next-generation synchrotron storage rings including the Upgraded Advanced Photon Source project now underway at Argonne National Laboratory. Stephan Hruszkewycz is a staff scientist in the Materials Science Division at Argonne National Laboratory. His research focuses on developing and using coherent x-ray scattering techniques to interrogate nanoscale materials structure and dynamics under working conditions to reveal structure-property relationships. Currently he is using strain- sensitive coherent Bragg diffraction to image subtle strain fields in nanoscale crystals for photonic and quantum information applications. These research thrusts are pursued at high-brightness synchrotron sources with state-of-the-art coherence-preserving beamlines, including those at the Advanced Photon Source, NSLS-II, and LCLS, and aim to broaden the applicability of coherent diffraction imaging within both the broader materials science community. -
MEMOIRS Row Standing on the Stern, Venetian Style, from the Lido, Where I Lived, to the School in Venice, Where I Studied
BRUNO BENEDETTO ROSSI April 13, 1905–November 21, 1993 BY GEORGE W. CLARK The initial motivation of the experiment which led to this discovery [of Sco X-1] was a subconscious feeling for the inexhaustible wealth of nature, a wealth that goes far beyond the imagination of man. That feeling was possi- bly generated by experiences in my previous work on cosmic rays; more likely it was inborn and was the reason why, as a young man, I went into the field of cosmic rays. In any case, whenever technical progress opened a new window into the surrounding world, I felt the urge to look through this window, hoping to see something unexpected.1 BEGINNINGS RUNO ROSSI WAS BORN April 13, 1905, in Venice, the el- Bdest of three sons of Rino Rossi and Lina Minerbi. His father was an electrical engineer whose successful career began with work on the electrification of Venice. He wrote in his autobiography2 that his father loved science and would have chosen it for a career except for practical consider- ations. He attributes to his father the influence that turned what may have been an “inborn tendency toward science . into a lifelong commitment.” He recalled: perfectly clear winter mornings when the air was so unusually transparent that the Alps surrounding Venice became clearly visible and appeared in- credibly close (Fata Morgana if you are a child or a poet, anomalous atmo- spheric refraction if you are a scientist). On those mornings I would try to find a sandalo (a small gondola) and, accompanied by a friend, I would 3 4 BIOGRAPHICAL MEMOIRS row standing on the stern, Venetian style, from the Lido, where I lived, to the school in Venice, where I studied. -
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. -
Booklet 2008-09.Indd
The Shaw Prize The Shaw Prize is an international award to honour individuals who are currently active in their respective fields and who have achieved distinguished and significant advances, who have made outstanding contributions in culture and the arts, or who in other domains have achieved excellence. The award is dedicated to furthering societal progress, enhancing quality of life, and enriching humanity’s spiritual civilization. Preference will be given to individuals whose significant work was recently achieved. Founder's Biographical Note The Shaw Prize was established under the auspices of Mr Run Run Shaw. Mr Shaw, born in China in 1907, is a native of Ningbo County, Zhejiang Province. He joined his brother’s film company in China in the 1920s. In the 1950s he founded the film company Shaw Brothers (Hong Kong) Limited in Hong Kong. He has been Executive Chairman of Television Broadcasts Limited in Hong Kong since the 1970s. Mr Shaw has also founded two charities, The Sir Run Run Shaw Charitable Trust and The Shaw Foundation Hong Kong, both dedicated to the promotion of education, scientific and technological research, medical and welfare services, and culture and the arts. ~ 1 ~ Message from the Chief Executive I am delighted to congratulate the six distinguished scientists who receive this year’s Shaw Prize. Their accomplishments enrich human knowledge and have a profound impact on the advancement of science. This year, the Shaw Prize recognises remarkable achievements in the areas of astronomy, life science and medicine, and mathematical sciences. The exemplary work and dedication of this year’s recipients vividly demonstrate that constant drive for excellence will eventually bear fruit. -
Bioluminescence Is Produced by a Firefly-Like Luciferase but an Entirely
www.nature.com/scientificreports OPEN New Zealand glowworm (Arachnocampa luminosa) bioluminescence is produced by a Received: 8 November 2017 Accepted: 1 February 2018 frefy-like luciferase but an entirely Published: xx xx xxxx new luciferin Oliver C. Watkins1,2, Miriam L. Sharpe 1, Nigel B. Perry 2 & Kurt L. Krause 1 The New Zealand glowworm, Arachnocampa luminosa, is well-known for displays of blue-green bioluminescence, but details of its bioluminescent chemistry have been elusive. The glowworm is evolutionarily distant from other bioluminescent creatures studied in detail, including the frefy. We have isolated and characterised the molecular components of the glowworm luciferase-luciferin system using chromatography, mass spectrometry and 1H NMR spectroscopy. The purifed luciferase enzyme is in the same protein family as frefy luciferase (31% sequence identity). However, the luciferin substrate of this enzyme is produced from xanthurenic acid and tyrosine, and is entirely diferent to that of the frefy and known luciferins of other glowing creatures. A candidate luciferin structure is proposed, which needs to be confrmed by chemical synthesis and bioluminescence assays. These fndings show that luciferases can evolve independently from the same family of enzymes to produce light using structurally diferent luciferins. Glowworms are found in New Zealand and Australia, and are a major tourist attraction at sites located across both countries. In contrast to luminescent beetles such as the frefy (Coleoptera), whose bioluminescence has been well characterised (reviewed by ref.1), the molecular details of glowworm bioluminescence have remained elusive. Tese glowworms are the larvae of fungus gnats of the genus Arachnocampa, with eight species endemic to Australia and a single species found only in New Zealand2. -
Understanding Bioluminescence in Dinoflagellates—How Far Have We Come?
Microorganisms 2013, 1, 3-25; doi:10.3390/microorganisms1010003 OPEN ACCESS microorganisms ISSN 2076-2607 www.mdpi.com/journal/microorganisms Review Understanding Bioluminescence in Dinoflagellates—How Far Have We Come? Martha Valiadi 1,* and Debora Iglesias-Rodriguez 2 1 Department of Evolutionary Ecology, Max Planck Institute for Evolutionary Biology, August-Thienemann-Strasse, Plӧn 24306, Germany 2 Department of Ecology, Evolution and Marine Biology, University of California Santa Barbara, Santa Barbara, CA 93106, USA; E-Mail: [email protected] * Author to whom correspondence should be addressed; E-Mail: [email protected] or [email protected]; Tel.: +49-4522-763277; Fax: +49-4522-763310. Received: 3 May 2013; in revised form: 20 August 2013 / Accepted: 24 August 2013 / Published: 5 September 2013 Abstract: Some dinoflagellates possess the remarkable genetic, biochemical, and cellular machinery to produce bioluminescence. Bioluminescent species appear to be ubiquitous in surface waters globally and include numerous cosmopolitan and harmful taxa. Nevertheless, bioluminescence remains an enigmatic topic in biology, particularly with regard to the organisms’ lifestyle. In this paper, we review the literature on the cellular mechanisms, molecular evolution, diversity, and ecology of bioluminescence in dinoflagellates, highlighting significant discoveries of the last quarter of a century. We identify significant gaps in our knowledge and conflicting information and propose some important research questions -
NL#132 October
October 2006 Issue 132 AAS NEWSLETTER A Publication for the members of the American Astronomical Society PRESIDENT’S COLUMN J. Craig Wheeler, [email protected] August is a time astronomers devote to travel, meetings, and writing papers. This year, our routine is set 4-5 against the background of sad and frustrating wars and new terror alerts that have rendered our shampoo Calgary Meeting suspect. I hope that by the time this is published there is a return to what passes for normalcy and some Highlights glimmer of reason for optimism. In this summer season, the business of the Society, while rarely urgent, moves on. The new administration 6 under Executive Officer Kevin Marvel has smoothly taken over operations in the Washington office. The AAS Final transition to a new Editor-in-Chief of the Astrophysical Journal, Ethan Vishniac, has proceeded well, with Election some expectation that the full handover will begin earlier than previously planned. Slate The Society, under the aegis of the Executive Committee, has endorsed the efforts of Senators Mikulksi and Hutchison to secure $1B in emergency funding for NASA to make up for some of the costs of shuttle 6 return to flight and losses associated with hurricane Katrina. It remains to be seen whether this action 2007 AAS will survive the budget process. The Executive Committee has also endorsed a letter from the American Renewals Institute of Physics supporting educators in Ohio who are fending off an effort there to include intelligent design in the curriculum. 13 Interestingly, the primary in Connecticut was of relevance to the Society. -
Who Has the Light?
2004 Deep-Scope Expedition Who Has the Light? FOCUS TEACHING TIME Bioluminescence in deep-sea organisms One 45-minute class period, plus time for student research GRADE LEVEL 7-8 (Life Science) SEATING ARRANGEMENT Classroom style or groups of 3-4 students FOCUS QUESTION What deep-sea organisms are capable of bio- MAXIMUM NUMBER OF STUDENTS luminescence, and how does this ability benefit 30 these organisms? KEY WORDS LEARNING OBJECTIVES Chemiluminescence Students will be able to compare and contrast Bioluminescence chemiluminescence, bioluminescence, fluores- Fluorescence cence, and phosphorescence. Phosphorescence Luciferin Students will be able to explain at least three Luciferase ways in which the ability to produce light may be Photoprotein useful to deep-sea organisms. Counter-illumination Students will be able to explain how scientists BACKGROUND INFORMATION may be able to use light-producing processes in Deep-sea explorers face many challenges: deep-sea organisms to obtain new observations extreme heat and cold, high pressures, and of these organisms. almost total darkness. The absence of light poses particular challenges to scientists who want to MATERIALS study organisms that inhabit the deep ocean envi- ❑ None ronment. Even though deep-diving submersibles carry bright lights, simply turning these lights on AUDIO/VISUAL MATERIALS creates another set of problems: At least some ❑ (Optional) Images of deep-sea environments mobile organisms are likely to move away from and organisms that use bioluminescence (see the light; organisms with light-sensitive organs Learning Procedure) may be permanently blinded by intense illumina- tion; even sedentary organisms may shrink back, ceasing normal life activities and possibly becom- ing less noticeable; and small cryptic organisms 1 2004 Deep-Scope Expedition – Grades 7-8 (Life Science) Focus: Bioluminescence in deep-sea organisms oceanexplorer.noaa.gov may simply be unnoticed. -
Sidney D. Drell Professional Biography
Sidney D. Drell Professional Biography Present Position Professor Emeritus, SLAC National Accelerator Laboratory, Stanford University (Deputy Director before retiring in 1998) Senior Fellow at the Hoover Institution since 1998 Present Activities Member, JASON, The MITRE Corporation Member, Board of Governors, Weizmann Institute of Science, Rehovot, Israel Professional and Honorary Societies American Physical Society (Fellow) - President, 1986 National Academy of Sciences American Academy of Arts and Sciences American Philosophical Society Academia Europaea Awards and Honors Prize Fellowship of the John D. and Catherine T. MacArthur Foundation, November (1984-1989) Ernest Orlando Lawrence Memorial Award (1972) for research in Theoretical Physics (Atomic Energy Commission) University of Illinois Alumni Award for Distinguished Service in Engineering (1973); Alumni Achievement Award (1988) Guggenheim Fellowship, (1961-1962) and (1971-1972) Richtmyer Memorial Lecturer to the American Association of Physics Teachers, San Francisco, California (1978) Leo Szilard Award for Physics in the Public Interest (1980) presented by the American Physical Society Honorary Doctors Degrees: University of Illinois (1981); Tel Aviv University (2001), Weizmann Institute of Science (2001) 1983 Honoree of the Natural Resources Defense Council for work in arms control Lewis M. Terman Professor and Fellow, Stanford University (1979-1984) 1993 Hilliard Roderick Prize of the American Association for the Advancement of Science in Science, Arms Control, and International Security 1994 Woodrow Wilson Award, Princeton University, for “Distinguished Achievement in the Nation's Service” 1994 Co-recipient of the 1989 “Ettore Majorana - Erice - Science for Peace Prize” 1995 John P. McGovern Science and Society Medalist of Sigma Xi 1996 Gian Carlo Wick Commemorative Medal Award, ICSC–World Laboratory 1997 Distinguished Associate Award of U.S. -
Firefly Luciferin-Activated Rose Bengal: in Vitro Photodynamic Therapy by Intracellular Chemiluminescence in Transgenic NIH 3T3 Cells1
[CANCER RESEARCH 63, 1818–1821, April 15, 2003] Firefly Luciferin-activated Rose Bengal: In Vitro Photodynamic Therapy by Intracellular Chemiluminescence in Transgenic NIH 3T3 Cells1 Theodossis Theodossiou,2,3 John S. Hothersall,2,3 Elizabeth A. Woods, Klaus Okkenhaug, Jake Jacobson, and Alexander J. MacRobert National Medical Laser Centre, Department of Surgery, University College London, W1W 7EJ London, United Kingdom [T. T., A. J. M.]; Department of Urology and Nephrology, University College London, London W1W 7EJ, United Kingdom [J. S. H.]; Ludwig Institute for Cancer Research, London W1W 7BS, United Kingdom [E. A. W., K. O.]; and Department of Molecular Pathogenesis, Institute of Neurology, London WC1N 3BG, United Kingdom [J. J.] ABSTRACT ATP. A photosensitizer that meets these criteria is the water-soluble xanthene dye, RB with a high singlet-oxygen quantum yield of ⌽⌬ Ϸ Photodynamic therapy (PDT) of cancer (1, 2) is a well-established 0.75, as reported in the literature (7). treatment modality that uses light excitation of a photosensitive substance to produce oxygen-related cytotoxic intermediates, such as singlet oxygen or free radicals (3, 4). Although PDT is advantageous over other forms of MATERIALS AND METHODS cancer treatments because of its limited side effects, its main disadvantage is the poor accessibility of light to more deeply lying malignancies. Exter- D-Luciferin CL Spectrum. Light emission from 100 lofD-luciferin- nal light sources such as lasers or lamps can be applied either noninva- luciferase solution (Labsystems ATP monitoring kit) in 2 ml PBS after the sively to reach tumors that lie well within the penetration depth of the addition of 10 M ATP was scanned in a Perkin-Elmer spectrofluorimeter light or in a minimally invasive fashion (interstitial treatments) in which (LS5) using a CL attachment. -
Faculty Award Winners by Award
Department of Physics and Astronomy Awards by Award Award Faculty Member Year Academia Europaea Kharzeev, Dmitri 2021 Academy of Teacher‐Scholar Award (Stony Brook) Jung, Chang Kee 2003 Academy Prize for Physics, Academy of Sciences, Goettingen, Germany Pietralla, Norbert 2004 AFOSR Young Investigator Award Allison, Thomas 2013 Albert Szent‐Gyorgi Fellowship (Hungary) Mihaly, Laszlo 2005 Alpha Epsilon Delta Premedical Honor Society (honorary member) Mendez, Emilio 1998 American Academy of Arts & Sciences Fellow Brown, Gerald 1976 Dill, Kenneth 2014 Zamolodchikov, Alexander 2012 American Association for the Advancement of Science Fellow Allen, Philip 2009 Ben‐Zvi, Ilan 2007 Jung, Chang Kee 2017 Dill, Kenneth 1997 Jacak, Barbara 2009 Sprouse, Gene 2012 Grannis, Paul 2000 Jacobsen, Chris 2002 Kharzeev, Dmitri 2010 Kirz, Janos 1985 Korepin, Vladmir 1998 Lee, Linwood 1985 Marburger, Jack 2000 Mihaly, Laszlo 2013 Stephens, Peter 2011 Sterman, George 2011 Swartz, Cliff 1973 American Association of Physics Teachers Distinguished Service Award Swartz, Cliff 1973 American Association of Physics Teachers Millikan Award Strassenburg, Arnold 1972 American Geophysical Union/U.S. Geological Survey ‐ naming of de Zafra Ridge, Antarctica de Zafra, Robert 2002 American Physical Society DAMOP Best Dissertation Weinacht, Thomas 2002 American Physical Society Fellow Abanov, Alexandre 2016 Allen, Philip 1986 Aronson, Meigan 2001 Averin, Dmitri 2004 Ben‐Zvi, Ilan 1994 Brown, Gerald 1976 Deshpande, Abhay 2014 Drees, Axel 2016 Essig, Rouven 2020 Nathan Leoce‐Schappin -
Sidney D. Drell 1926–2016
Sidney D. Drell 1926–2016 A Biographical Memoir by Robert Jaffe and Raymond Jeanloz ©2018 National Academy of Sciences. Any opinions expressed in this memoir are those of the authors and do not necessarily reflect the views of the National Academy of Sciences. SIDNEY daVID DRELL September 13, 1926–December 21, 2016 Elected to the NAS, 1969 Sidney David Drell, professor emeritus at Stanford Univer- sity and senior fellow at the Hoover Institution, died shortly after his 90th birthday in Palo Alto, California. In a career spanning nearly 70 years, Sid—as he was universally known—achieved prominence as a theoretical physicist, public servant, and humanitarian. Sid contributed incisively to our understanding of the elec- tromagnetic properties of matter. He created the theory group at the Stanford Linear Accelerator Center (SLAC) and led it through the most creative period in elementary particle physics. The Drell-Yan mechanism is the process through which many particles of the Standard Model, including the famous Higgs boson, were discovered. By Robert Jaffe and Raymond Jeanloz Sid advised Presidents and Cabinet Members on matters ranging from nuclear weapons to intelligence, speaking truth to power but with keen insight for offering politically effective advice. His special friendships with Wolfgang (Pief) Panofsky, Andrei Sakharov, and George Shultz highlighted his work at the interface between science and human affairs. He advocated widely for the intellectual freedom of scientists and in his later years campaigned tirelessly to rid the world of nuclear weapons. Early life1 and work Sid Drell was born on September 13, 1926 in Atlantic City, New Jersey, on a small street between Oriental Avenue and Boardwalk—“among the places on the Monopoly board,” as he was fond of saying.