LIGO Magazine, Issue 9, 8/2016
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A Time of Great Growth
Newsletter | Spring 2019 A Time of Great Growth Heartfelt greetings from the UC Riverside Department of Physics and Astronomy. This is our annual newsletter, sent out each Spring to stay connected with our former students, retired faculty, and friends in the wider community. The Department continues to grow, not merely in size but also in stature and reputation. For the 2018-2019 academic year, we were pleased to welcome two new faculty: Professors Thomas Kuhlman and Barry Barish. Professor Kuhlman was previously on the faculty at the University of Illinois at Urbana-Champaign. He joins our efforts in the emerging field of biophysics. His research lies in the quantitative imaging and theoretical modeling of biological systems. He works on genome dynamics, quantification of the activity of transposable elements in living cells, and applications to the engineering of genome editing. Professor Barry Barish, who joins us from Caltech, is the winner of the 2017 Nobel Prize in Physics. He brings great prestige to our Department. Along with Professor Richard Schrock of the Department of Chemistry, who also joined UCR in 2018, UCR now has two Nobel Prize winners on its faculty. Professor Barish is an expert on the detection and physics of gravitational waves. He has been one of the key figures in the conception, construction, and operation of the LIGO detector, where gravitational waves were first discovered in 2015, and which led to his Nobel Prize. He is a member of the National Academy of Sciences and the winner of many other prestigious awards. The discovery of gravitational waves is one of the most exciting developments in physics so far this century. -
Ripples in Spacetime
editorial Ripples in spacetime The 2017 Nobel prize in Physics has been awarded to Rainer Weiss, Barry C. Barish and Kip S. Thorne “for decisive contributions to the LIGO detector and the observation of gravitational waves”. It is, frankly, difficult to find something original to say about the detection of gravitational waves that hasn’t been said already. The technological feat of measuring fluctuations in the fabric of spacetime less than one-thousandth the width of an atomic nucleus is quite simply astonishing. The scientific achievement represented by the confirmation of a century-old prediction by Albert Einstein is unique. And the collaborative effort that made the discovery possible — the Laser Interferometer Gravitational-Wave Observatory (LIGO) — is inspiring. Adapted from Phys. Rev. Lett. 116, 061102 (2016), under Creative Commons Licence. Rainer Weiss and Kip Thorne were, along with the late Ronald Drever, founders of the project that eventually became known Barry Barish, who was the director Last month we received a spectacular as LIGO. In the 1960s, Thorne, a black hole of LIGO from 1997 to 2005, is widely demonstration that talk of a new era expert, had come to believe that his objects of credited with transforming it into a ‘big of gravitational astronomy was no interest should be detectable as gravitational physics’ collaboration, and providing the exaggeration. Cued by detections at LIGO waves. Separately, and inspired by previous organizational structure required to ensure and Virgo, an interferometer based in Pisa, proposals, Weiss came up with the first it worked. Of course, the passion, skill and Italy, more than 70 teams of researchers calculations detailing how an interferometer dedication of the thousand or so scientists working at different telescopes around could be used to detect them in 1972. -
The History of Lasers at Stanford Group
Lasers at 50: Byer The History of Lasers at Stanford Group Robert L. Byer Applied Physics Stanford University [email protected] Abstract In the fifty years since the demonstration of the laser, coherent light has changed the way we work, communicate and play. The generation and control of light is critical for meeting important challenges of the 21st century from fundamental science to the generation of energy. A look back at the early days of the laser at Stanford will be contrasted to the recent breakthroughs in solid state lasers and the applications to fundamental science of gravitational wave detection, remote sensing, and laser induced fusion for energy production. Stanford Historical Society 34th Annual Meeting & Reception May 25, 2010 The History of Lasers at Stanford May 25 2010 Cubberley Auditorium, Staford Byer California – Leader in advanced telescopes for astronomy Group Lick 36 inch refractor The Mount Wilson 100 inch The Palomar 200 inch 1888 1917 1948 The History of Lasers at Stanford May 25 2010 Cubberley Auditorium, Staford From Maser to Laser – stimulated emission at optical frequencies Byer proposed in 1958 – A. Schawlow and C. H. Townes Group The History of Lasers at Stanford May 25 2010 Cubberley Auditorium, Staford Early advances in lasers --- Byer 2009 a Special Year Group Concept of Optical Maser Schawlow & Townes 1958 Ruby Laser Ted Maiman 1960 Nobel Prize awarded in 1964 Townes, Prokhorov and Basov Hg+ Ion Laser Earl Bell 1965 Argon Ion Laser Bill Bridges Tunable cw parametric Laser Harris 1968 Diode bar 1Watt -
Rainer Weiss, Professor of Physics Emeritus and 2017 Nobel Laureate
Giving to the Department of Physics by Erin McGrath RAINER WEISS ’55, PHD ’62 Bryce Vickmark Rai Weiss has established a fellowship in the Physics Department because he is eternally grateful to his advisor, the late Jerrold Zacharias, for all that he did for Rai, so he knows firsthand the importance of supporting graduate students. Rainer Weiss, Professor of Physics Emeritus and 2017 Nobel Laureate. Rainer “Rai” Weiss was born in Berlin, Germany in 1932. His father was a physician and his mother was an actress. His family was forced out of Germany by the Nazis since his father was Jewish and a Communist. Rai, his mother and father fled to Prague, Czecho- slovakia. In 1937 a sister was born in Prague. In 1938, after Chamberlain appeased Hitler by effectively giving him Czechoslovakia, the family was able to obtain visas to enter the United States through the Stix Family in St. Louis, who were giving bond to professional Jewish emigrants. When Rai was 21 years-old, he visited Mrs. Stix and thanked her for what she had done for his family. The family immigrated to New York City. Rai’s father had a hard time passing the medi- cal boards because of his inability to answer multiple choice exams. His mother, who Rai says “held the family together,” worked in a number of retail stores. Through the services of an immigrant relief organization Rai received a scholarship to attend the prestigious Columbia Grammar School. At the end of 1945, when Rai was 13 years old, he became fascinated with electronics and music. -
A Joint Fermilab/SLAC Publication Dimensions of Particle Physics Issue
dimensions volume 03 of particle physics symmetryA joint Fermilab/SLAC publication issue 05 june/july 06 Cover Physicists at Fermilab ponder the physics of the proposed International Linear Collider, as outlined in the report Discovering the Quantum Universe. Photos: Reidar Hahn, Fermilab Office of Science U.S. Department of Energy volume 03 | issue 05 | june/july 06 symmetryA joint Fermilab/SLAC publication 3 Commentary: John Beacom “In a global fi eld, keeping up with all the literature is impossible. Personal contact is essential, and I always urge students and postdocs to go to meetings and talk to strangers.” 4 Signal to Background An industrial waterfall; education by placemats; a super-clean surface; horned owls; Garden Club for particle physicists; Nobel banners; US Congress meets Quantum Universe. 8 Voices: Milestones vs. History Celebrating a milestone is always enjoyable, but a complete and accurate historical record is invalu- able for the past to inform the future. 10 A Report Like No Other Can the unique EPP2010 panel steer US particle physics away from a looming crisis? Physicists and policy makers are depending on it. 14 SNS: Neutrons for ‘molecular movies’ A new research facility at Oak Ridge National Laboratory has produced its fi rst neutrons, presenting new opportunities for studying materials from semiconductors to human enzymes. 20 Battling the Clouds Electron clouds could reduce the brightness—and discovery potential—of the proposed International Linear Collider. Innovative solutions are on the way and might reduce the cost of the machine, too. 24 A (Magnus) Force on the Mound Professional baseball player Jeff Francis of the Colorado Rockies brings a strong arm and a physics background to the playing fi eld: “I bet Einstein couldn’t throw a curveball.” 26 Deconstruction: Spallation Neutron Source Accelerator-based neutron sources such as the SNS can provide pulses of neutrons to probe superconductors, aluminum bridges, lighter and stronger plastic products, and pharmaceuticals. -
Piled Higher and Deeper (Revised)
10 th European Association for Consumer Research Conference, Barcelona/Spain, July 4 th -7th , 2013 PILED HIGHER AND DEEPER : INSIGHTS INTO “THE PHD COMICS” AS A CO-CREATIVE CONSUMPTION EXPERIENCE By Markus Wohlfeil Norwich Business School, University of East Anglia, UK Mar Solé Copenhagen Business School, Denmark Keywords: PhD Comics, brand community, life in academia, co-creation, netnography, experiential consumption ABSTRACT The Piled Higher and Deeper comic strips appeal to a very distinct brand community that is narrowly defined by common shared experiences as postgraduate researchers. This netnographic study explores whether and to what extent members of Piled Higher and Deeper brand community are getting actively involved in co-creation activities. EXTENDED ABSTRACT When Jorge Cham published his “Piled Higher and Deeper – The Life (or the Lack Thereof) in Academia” series in the fall of 1997, nobody could have foreseen that these newspaper- and web-based comic strips would eventually become a worldwide popular phenomenon (Choe 2011). Commonly known as “The PhD Comics” , they follow the lives of postgraduate research students and the different issues they constantly face at their US university from a humorous perspective (Fine and De Soucey 2005; Koziski 1984). These include their complicated student-supervisor relationships, the problematics of scientific research, the demands of teaching and marking assignments, the lack of a private/social life, the perils of procrastination and ‘the endless search for free food’ (Cham 2002). While Jorge Cham initially conceived the PhD Comics as a form of ‘therapy’ , by which he could exercise his own frustrations, anxieties and other demons while working towards a PhD in mechanical engineering at Stanford University (Choe 2011), they have enjoyed a growing popularity among postgraduates and young academics around the world who experience similar issues as the characters (Lawson 2011). -
The Strong and Weak Senses of Theory-Ladenness of Experimentation: Theory-Driven Versus Exploratory Experiments in the History of High-Energy Particle Physics
[Accepted for Publication in Science in Context] The Strong and Weak Senses of Theory-Ladenness of Experimentation: Theory-Driven versus Exploratory Experiments in the History of High-Energy Particle Physics Koray Karaca University of Wuppertal Interdisciplinary Centre for Science and Technology Studies (IZWT) University of Wuppertal Gaußstr. 20 42119 Wuppertal, Germany [email protected] Argument In the theory-dominated view of scientific experimentation, all relations of theory and experiment are taken on a par; namely, that experiments are performed solely to ascertain the conclusions of scientific theories. As a result, different aspects of experimentation and of the relation of theory to experiment remain undifferentiated. This in turn fosters a notion of theory- ladenness of experimentation (TLE) that is too coarse-grained to accurately describe the relations of theory and experiment in scientific practice. By contrast, in this article, I suggest that TLE should be understood as an umbrella concept that has different senses. To this end, I introduce a three-fold distinction among the theories of high-energy particle physics (HEP) as background theories, model theories and phenomenological models. Drawing on this categorization, I contrast two types of experimentation, namely, “theory-driven” and “exploratory” experiments, and I distinguish between the “weak” and “strong” senses of TLE in the context of scattering experiments from the history of HEP. This distinction enables to identify the exploratory character of the deep-inelastic electron-proton scattering experiments— performed at the Stanford Linear Accelerator Center (SLAC) between the years 1967 and 1973—thereby shedding light on a crucial phase of the history of HEP, namely, the discovery of “scaling”, which was the decisive step towards the construction of quantum chromo-dynamics (QCD) as a gauge theory of strong interactions. -
Members Elect Barry Barish As Next APS Vice-President
October 2008 Volume 17, No. 9 www.aps.org/publications/apsnews 21st Century Campaign Nears Goal APS NEWS and Needs Your Support! A PublicAtion of the AmericAn PhysicAl society • www.APs.org/PublicAtions/APsnews (See insert) Energy Efficiency Crucial to Achieving Energy Security Members Elect Barry Barish and Reducing Global Warming, States APS Report as next APS Vice-President Tapping wasted energy from miles per gallon mileage for cars needs because they require sig- APS members have elected in physics from the University of inefficient automobiles, homes and and other light-duty vehicles by nificant scientific and engineering Barry Barish, Linde Professor of California, Berkeley. He joined businesses is equivalent to discov- 2030 and the elimination of energy breakthroughs in several critical Physics Emeritus at Caltech, as the faculty at Caltech in 1963. ering a hidden energy reserve that from fossil fuels in new residential areas. the Society’s next vice president. Among his noteworthy experi- will help the United States improve buildings by 2020. The study also calls on Congress Barish will assume the office in ments were those performed at its energy security and reduce glob- and the White House to increase January 2009. At the same time, Fermilab using high-energy neu- al warming, an APS study panel has spending on research and develop- Curtis Callan of trino collisions to concluded. ment of next-generation building Princeton Univer- reveal the quark Their report, Energy Future: technologies, training scientists sity will become substructure of Think Efficiency, states that the key who work on building technologies president-elect, and the nucleon. -
Laser Interferometry Gravitational Wave Detection
Quantum Noise Limited Lasers and Byer The Search for Gravitational Waves Group Robert L. Byer Department of Applied Physics Stanford University Abstract Einstein formulated the general theory of relativity near 100 years ago and showed that gravity is curvature in space-time and further that ripples in space-time, gravitational waves, travel at the speed of light. Today the Laser Interferometer Gravitational Wave Observatory, LIGO, project is using ground based 4km long interferometers to search for gravitational waves. The progress for LIGO and other earth based gravitational wave interferometers will be reviewed. This summer the Laser Interferometer in Space Antenna, LISA, project, joint between NASA and ESA, will hold its 8th International meeting at Stanford. The design of the space-based 5 million kilometer path length LISA interferometer, scheduled for launch in 2020, will be discussed. The detection of gravitational waves requires the ultimate in precision measurement. The ‘ruler’ used to detect oscillations in space-time is the constant; the speed of light. The light source is a very stable diode-pumped Nd:YAG solid state laser oscillator-amplifier that operates reliably at the quantum limit in phase and amplitude. AAAS 2010 Annual Meeting San Diego, CA February 21, 2010 AAAS 2010 Annual Meeting February 21, 2010 Extreme Optical Tools and Applications Outline Byer Group Prelude: California – a leader in science and technology LIGO & LISA: Early History and Concepts LIGO and LISA at the beginning Gravitational Waves and Sources -
KITCHEN CHEMISTRY Bijeta Roynath & Prasanta Kumar Sahoo
Test Your Knowledge KITCHEN CHEMISTRY Bijeta Roynath & Prasanta Kumar Sahoo 1. The common cooking fuel, Liquefied Petroleum Gas 10. Which of the following could be produced by the gas (LPG), is a mixture of two hydrocarbons. These are: stove? (a) Methane and Butane (b) Propane and Butane (a) Nitrogen Oxides (b) Sulphur dioxides (c) Oxygen and Hydrogen (d) Hexane and Propane (c) Carbon monoxide (d) Dihydrogen oxide 2. Hydrocarbons in LPG are colourless and odourless. 11. Which of the following chemical is found in dish- Therefore, a strong smelling agent added to LPG washing detergent? cylinders to detect leakage is: (a) Carbon monoxide (b) Chlorine (a) Ethyl mercaptan (b) Nitrous oxide (c) Sulphur dioxide (d) Lithium (c) Hydrogen sulfide (d) Chloroform 12. Proteins help build our body and carbohydrates 3. Chemical irritant produced during chopping an provide energy to the body. The protein and onion (Allium cepa) which makes our eye weepy is: carbohydrate found in milk are: (a) Allinase (b) Sulfoxide (a) Albumin and maltose (b) Pepsin and sucrose (c) Syn-propanethial-S-oxide (d) Allyl mercaptan (c) Collagen and fructose (d) Casein and lactose 4. The powerful anti-inflammatory and antioxidant 13. Salt readily absorbs water from the surroundings. properties of haldi or turmeric (Curcuma longa) are Sprinkling salt on salad releases water from it after due to presence of: few seconds. The process is: (a) Curcumin (b) Gingerol (a) Osmosis (b) Adsorption (c) Cymene (d) Capsaicin (c) Dehydration (d) Oxidation 5. The active ingredient in chilli peppers (Capsicum) 14. Washing hands before eating prevents illness which produces heat and burning sensation in the by killing germs. -
APS News July 2018, Vol. 27. No. 7
July 2018 • Vol. 27, No. 7 A PUBLICATION OF THE AMERICAN PHYSICAL SOCIETY Homer Neal 1942-2018 Page 3 APS.ORG/APSNEWS Update on the APS Strategic Plan Throughout 2018, APS mem- bers, leadership, and staff have been preparing a new Strategic Plan to guide the Society in coming years (see APS News, February 2018). Archiving Knowledge about Physics Teaching MISSION VALUES VISION The process began in early 2018 at By Charles Henderson and Paula Heron the APS Leadership Convocation Do laboratory experiments help at the founding and develop- when elected leaders of mem- students learn concepts? Why do ment of Physical Review Physics bership units (Divisions, Topical so few women choose to major in Education Research in 2005, now Groups, Forums, and Sections) pro- physics? What is the most impor- a central and open-access home for vided input. Town hall meetings tant skill for a high school physics this work. and invited focus groups convened teacher to develop? The close connection between at the APS March and April meet- and Increasing Organizational Physics education researchers PER and physics as a discipline ings to gather direct member com- Excellence. tackle these and many other ques- was acknowledged by the American ment. CEO Kate Kirby provided an At its June retreat, the Board tions about why students study Physical Society Council in its update at the annual APS Business spent considerable time discuss- physics, what they learn, and 1999 Statement on Research in common teaching strategies and Meeting on April 13 and a member ing progress on the Plan. In guid- how their experiences affect their Physics Education [1]. -
Barry C Barish
Barry C Barish Barry Barish earned his B.A. in physics (1957) and Ph.D. in experimental particle physics (1962) at the University of California, Berkeley. He came to Caltech as a postdoc in 1963, where he has pursued his academic and research careers and is currently the Maxine and Ronald Linde Professor of Physics, Emeritus. Barish’s primary research interest has been the Laser Interferometer Gravitational-wave Observatory (LIGO), since he became Principal Investigator in 1994 and Director in 1997. He led the effort through the final design stages, approval for funding by the NSF National Science Board in 1994, and then the construction and commissioning of the LIGO interferometers in Livingston, LA and Hanford, WA. In 1997, he created the LIGO Scientific Collaboration (LSC), which now enables more than 1000 collaborators world-wide to participate in LIGO. Suspended mass laser interferometers search for gravitational wave signals by monitoring motions of test masses separated by four kilometer baselines to a precision of less than 10–18 meters. The Initial LIGO detectors reached design sensitivity and set many significant limits on astrophysical sources of gravitational waves. A proposal for a more sensitive detector, Advanced LIGO, was developed from 1999 to 2003, while Barish was Director, and it was approved by the NSF in 2003. Advanced LIGO was funded as a major research project (MREFC) by Congress several years later. This project incorporated major new technological developments from the LIGO R&D efforts, including an active seismic isolation system to reduce seismic noise, a multiple suspension system with a large fused silica test mass to reduce thermal noise and a 200 watt NiYAG laser to reduce shot noise, as well as incorporate improved and a more flexible optics system.