APS News, March 2018, Vol. 27, No. 3

Total Page:16

File Type:pdf, Size:1020Kb

APS News, March 2018, Vol. 27, No. 3 March 2018 • Vol. 27, No. 3 A PUBLICATION OF THE AMERICAN PHYSICAL SOCIETY New Members of the PhysTEC 5+ Club APS.ORG/APSNEWS Page 3 2018 APS April Meeting: “Hello, Columbus” Physical Review B: Condensed Attendees in fields from Matter, Then and Now “Quarks to the Cosmos,” includ- ing particle physics, nuclear phys- ics, astrophysics, and gravitation, Getty Images will gather in Columbus, Ohio, April 14–17, at the Columbus Convention Center for the 2018 APS April Meeting. The meeting theme this year is “A Feynman Century,” marking the 100th By Sarma Kancharla and Laurens lished by APS offers a chance to anniversary of the Nobel-winning Molenkamp look back at some of the landmark physicist’s birth with a Kavli The late Peter Adams, found- publications that have led to PRB Foundation Plenary Session and ing editor of Physical Review B becoming not only the largest an invited session on his legacy. (PRB), impishly used to say that journal in all of physics but also a venue for excellence. The Kavli session will be held the journal was created in 1970 on Saturday, April 14 (8:30 a.m.) because The Physical Review and will feature a presentation by had reached its binding limit. Joan Feynman (Jet Propulsion Lab, Forum on the History of Physics Professional Skills Development Apocryphal as that sounds, the retired) on life with her brother invited session on Monday, April Workshop for Women on persua- birth of PRB couldn't have hap- Richard and her concerns about cli- 16 (room B130) at 1:30 p.m., with sive communication, negotiation, mate change. Christopher Monroe Paul Halperin (University of the and leadership (Friday, April 13, pened sooner because solid state (University of Maryland and IonQ) Sciences), John Preskill (California 8 a.m.–4 p.m.). The second is a physics, the core charge of the will discuss Richard Feynman’s Institute of Technology), and Professional Skills Seminar specif- journal, would soon morph into involvement in the origins of quan- Virginia Trimble (University of ically for undergraduate and grad- the broader arena of condensed tum computing. Roxanne Springer California at Irvine). uate women in physics (Sunday, matter physics (CMP) and then There is no better place to start (Duke University) will talk about Two skill-building events for April 15 4-6 p.m.). The seminar materials physics. than the Nobel Prize–winning pair Feynman’s contributions to quan- women will take place at the will focus on professional skills The 125th anniversary of the of papers in 1971 by Wilson which tum field theory. Discussions about meeting. The first, for postdocs founding of The Physical Review Feynman will continue at an APS and early career researchers, is a MEETING continued on page 6 and the family of journals pub- PRB continued on page 4 APS Strategic Planning: Get Involved! Staying on Pointe: Physicist Twirls Her Way to Successful Ballet Career By Alaina G. Levine APS leadership is developing a new Strategic Plan for the Society and member input is vital for the success of Merritt Moore’s scientific resume is impressive: She recently this effort. Please attend one of the Town Hall meetings received her Ph.D. in quantum and submit comments via the website. physics from the University of Town Hall: 2018 APS March Meeting in Los Angeles, Oxford, and she graduated with her Thursday, March 8, 1:00-2:30 bachelor’s in physics from Harvard p.m., in room 305 of the Los with honors. Angeles Convention Center. But there is much more—she’s been a dancer since she was 13 Town Hall: 2018 APS April years old. Moore is an interna- Meeting in Columbus, Ohio, tionally known ballerina, and has Monday, April 16, 3:30-5:00 danced professionally with compa- p.m., in room B-130 of the Co- nies all over the world, including lumbus Convention Center. the Zürich Ballet Company, Boston Ballet, English National Ballet, Strategic planning will also be on the agenda of the an- and London Contemporary Ballet Theatre. She has performed at a nual APS Business Meeting in Columbus: Friday, April special exhibition at the Victoria Physicist Merritt Moore combines a career in science and acclaim as a performing artist. 13, 4:00-5:00 p.m. in room A-216 of the Columbus Con- & Albert Museum in which she vention Center. danced with robots, at a virtual intensely pursued dance, but as to be strong’.” It changed my reality and dance event at the she advanced she began to grow whole outlook.” And it reignited Please visit go.aps.org/strategicplan to learn more Barbican Centre in London, and tired of it. In fact, when she had Moore’s dancing fever. Pretty about the planning process and to upload comments. at the Imagine Science Film festi- the chance to study abroad in Italy soon, she traveled every weekend val, in which she collaborated with as a 15-year-old, she specifically from Viterbo, the little town she filmmakers to visualize scientific looked for a hamlet to live in that was studying in, to Rome, where principles through art. did not offer any dance classes. the teacher was based, where she A certified science junkie, But a chance encounter sent her would train by day, and sleep on Moore began her love affair with whirling back to ballet. her kitchen floor. The lessons were mathematics as a kid, and she One day in Italy Moore found so magnetic that even when Moore took her first physics class in high herself in a “dingy” gym and saw returned home, she continued train- school. “I knew I was going to a ballet class being taught with a ing with this teacher for six years, love it,” she says. “Then the more very different approach than she heading to Rome every chance she I learned about quantum mechanics was used to. “Many teachers want could get. and … new quantum technologies, you to look identical to the girl to “It’s different learning from the I was hooked.” So physics seemed your left and right, and there’s a top of the top. She was a prima bal- the logical career choice. perfect body type that everyone lerina,” adds Moore. “She would But first she had to balance is striving for, but this instruc- say if you want to be a ballet that with her love of ballet. In her tor … was like ‘no, be you, be dancer you can’t be a ballet dancer hometown of Los Angeles, she unique, and that will allow you BALLERINA continued on page 7 2 • March 2018 Spotlight on Development This Month in Physics History The Leo P. Kadanoff Prize March 22, 1895: Screening of the Lumière Brothers’ First Film APS is pleased to announce the establishment of the Leo P. illions flock to movie theaters every week- graph. Antoine snagged a sample of film from one Kadanoff Prize to honor the mem- Mend to view the latest Hollywood block- of the exhibitors there to show his sons. He thought ory and celebrate the legacy of one busters, and the multimillion-dollar film industry they could develop a better, cheaper alternative to of the giants in the field of statisti- dominates popular culture. Among the early pio- the kinetoscope and kinetograph, combining the cal and nonlinear physics. We have neers who made this revolution possible were viewing, developing, and recording functions into launched an effort to endow this two French brothers: Auguste and Louis Lumière. one device. Instead of the single-viewer kineto- Prize, and invite you to consider Auguste was the elder, born in 1862, while scope, he envisioned projecting films onto a large supporting it. Louis was born two years later. Their father, screen so that many people could watch all at once. The Kadanoff Prize was pro- Antoine, started out as a portrait painter before The brothers began experimenting at once, posed by the APS Topical Group on switching to photography, setting up his own small and by the following year they invented the Statistical and Nonlinear Physics business making photographic plates in Lyons. Cinematographe, which weighed just 11 pounds (GSNP) to recognize a scientist or Leo Kadanoff Both sons completed technical school, with a solid and could be operated with a simple hand crank scientists whose work (theoretical, Gifts of any amount will be grasp of organic chemistry, rather than relying on elec- experimental or computational) has greatly appreciated and recog- although Louis preferred trical power. Louis drew opened up new vistas for statistical nized on the Kadanoff website. physics and Auguste gravi- inspiration one sleepless and/or nonlinear physics. Moreover, gifts of $1,000 or more tated towards biochemistry night from how a sew- APS has launched a $300,000 will help us reach our goal for and medicine. They went to ing machine operates, and endowment campaign to allow the opening up the one-year nomina- work for their father. After invented a claw mechanism experimenting with his to pull the film through Kadanoff Prize to be given in per- tion process on-time and ensure wikimedia commons petuity. We are enormously grateful that the first Kadanoff Prize will father’s equipment, Louis in the camera. In contrast to to family members, friends, and be awarded at the 2019 APS March particular became fascinated the sprocket system used colleagues of Leo Kadanoff who Meeting in Boston. with the underlying science. by Edison, the Lumières’ have already raised commitments For more information on ways At just 17, he invented a device formed the basis totaling over $100,000 toward to make a gift in support of the new “dry plate” process for of subsequent early cin- the endowment goal, and are cur- Leo P.
Recommended publications
  • Simulating Physics with Computers
    International Journal of Theoretical Physics, VoL 21, Nos. 6/7, 1982 Simulating Physics with Computers Richard P. Feynman Department of Physics, California Institute of Technology, Pasadena, California 91107 Received May 7, 1981 1. INTRODUCTION On the program it says this is a keynote speech--and I don't know what a keynote speech is. I do not intend in any way to suggest what should be in this meeting as a keynote of the subjects or anything like that. I have my own things to say and to talk about and there's no implication that anybody needs to talk about the same thing or anything like it. So what I want to talk about is what Mike Dertouzos suggested that nobody would talk about. I want to talk about the problem of simulating physics with computers and I mean that in a specific way which I am going to explain. The reason for doing this is something that I learned about from Ed Fredkin, and my entire interest in the subject has been inspired by him. It has to do with learning something about the possibilities of computers, and also something about possibilities in physics. If we suppose that we know all the physical laws perfectly, of course we don't have to pay any attention to computers. It's interesting anyway to entertain oneself with the idea that we've got something to learn about physical laws; and if I take a relaxed view here (after all I'm here and not at home) I'll admit that we don't understand everything.
    [Show full text]
  • Wiki Template-1Eb7p59
    Wikipedia Reader https://en.wikipedia.org/wiki/Aurora Selected by Julie Madsen - Entry 10 1 Aurora From Wikipedia, the free encyclopedia An aurora, sometimes referred to as a polar lights or north- ern lights, is a natural light display in the sky, predominantly seen in the high latitude (Arctic and Antarctic) regions.[1] Au- roras are produced when the magnetosphere is sufficiently disturbed by the solar wind that the trajectories of charged particles in both solar wind and magnetospheric plasma, mainly in the form of electrons and protons, precipitate them into the upper atmosphere (ther- mosphere/exosphere), where their energy is lost. The resulting ion- ization and excitation of atmospheric constituents emits light of varying color and complexity. The form of the aurora, occur- ring within bands around both polar regions, is also dependent on the amount of acceleration imparted to the precipitating parti- cles. Precipitating protons generally produce optical emissions as incident hydrogen atoms after gaining electrons from the atmosphere. Proton Images of auroras from around the world, auroras are usually observed at including those with rarer red and blue lower latitudes.[2] lights Wikipedia Reader 2 May 1 2017 Contents 1 Occurrence of terrestrial auroras 1.1 Images 1.2 Visual forms and colors 1.3 Other auroral radiation 1.4 Aurora noise 2 Causes of auroras 2.1 Auroral particles 2.2 Auroras and the atmosphere 2.3 Auroras and the ionosphere 3 Interaction of the solar wind with Earth 3.1 Magnetosphere 4 Auroral particle acceleration 5 Auroral events of historical significance 6 Historical theories, superstition and mythology 7 Non-terrestrial auroras 8 See also 9 Notes 10 References 11 Further reading 12 External links Occurrence of terrestrial auroras Most auroras occur in a band known as the auroral zone,[3] which is typically 3° to 6° wide in latitude and between 10° and 20° from the geomagnetic poles at all local times (or longitudes), most clearly seen at night against a dark sky.
    [Show full text]
  • Feynman-Richard-P.Pdf
    A Selected Bibliography of Publications by, and about, Richard Phillips Feynman Nelson H. F. Beebe University of Utah Department of Mathematics, 110 LCB 155 S 1400 E RM 233 Salt Lake City, UT 84112-0090 USA Tel: +1 801 581 5254 FAX: +1 801 581 4148 E-mail: [email protected], [email protected], [email protected] (Internet) WWW URL: http://www.math.utah.edu/~beebe/ 07 June 2021 Version 1.174 Title word cross-reference $14.95 [Oni15]. $15 [Ano54b]. $18.00 [Dys98]. $19.99 [Oni15]. 2 + 1 [Fey81, Fey82c]. $22.00 [Dys98]. $22.95 [Oni15]. $24.95 [Dys11a, RS12]. $26.00 [Bro06, Ryc17, Dys05]. $29.99 [Oni15, Roe12, Dys11a]. $30.00 [Kra08, Lep07, W¨ut07]. $35 [Ano03b]. $50.00 [DeV00, Ano99]. $500 [Ano39]. $55.00 [Noe11]. $80.00hb/$30.00pb [Cao06]. $9.95 [Oni15]. α [GN87, Sla72]. e [BC18]. E = mc2 [KN19]. F (t) · r [BS96]. λ [Fey53c, Fey53a]. SU(3) [Fey65a]. U(6) ⊗ U(6) [FGMZ64]. π [BC18]. r [EFK+62]. -Transition [Fey53a]. 0-19-853948-7 [Tay97]. 0-226-42266-6 [W¨ut07]. 0-226-42267-4 [Kra08]. 0-691-03327-7 [Bro96c]. 0-691-03685-3 [Bro96c]. 1965 [Fey64e]. 1988 [Meh02]. 1 2 2.0 [BCKT09]. 2002 [FRRZ04]. 2007 [JP08]. 2010 [KLR13]. 20th [Anoxx, Bre97, Gin01, Kai02]. 235 [FdHS56]. 3 [Ish19, Ryc17]. 3.0 [Sem09]. 3.2 [Sem16]. 40th [MKR87]. 469pp [Cao06]. 8 [Roe12]. 9 [BFB82]. 978 [Ish19, Roe12, Ryc17]. 978-0-06135-132-7 [Oni15]. 978-0-300-20998-3 [Ryc17]. 978-0-8090-9355-7 [Oni15]. 978-1-58834-352-9 [Oni15].
    [Show full text]
  • Interplanetary Magnetic Field Control of the Entry of Solar Energetic Particles Into the Magnetosphere R
    JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 107, NO. A8, 1184, 10.1029/2001JA000099, 2002 Interplanetary magnetic field control of the entry of solar energetic particles into the magnetosphere R. L. Richard, M. El-Alaoui, M. Ashour-Abdalla,1 and R. J. Walker2 Institute of Geophysics and Planetary Physics, University of California at Los Angeles, Los Angeles, California, USA Received 2 April 2001; revised 6 February 2002; accepted 18 March 2002; published 15 August 2002. [1] We have investigated the entry of energetic ions of solar origin into the magnetosphere as a function of the interplanetary magnetic field orientation. We have modeled this entry by following high energy particles (protons and 3He ions) ranging from 0.1 to 50 MeV in electric and magnetic fields from a global magnetohydrodynamic (MHD) model of the magnetosphere and its interaction with the solar wind. For the most part these particles entered the magnetosphere on or near open field lines except for some above 10 MeV that could enter directly by crossing field lines due to their large gyroradii. The MHD simulation was driven by a series of idealized solar wind and interplanetary magnetic field (IMF) conditions. It was found that the flux of particles in the magnetosphere and transport into the inner magnetosphere varied widely according to the IMF orientation for a constant upstream particle source, with the most efficient entry occurring under southward IMF conditions. The flux inside the magnetosphere could approach that in the solar wind implying that SEPs can contribute significantly to the magnetospheric energetic particle population during typical SEP events depending on the state of the magnetosphere.
    [Show full text]
  • 16 Super Brain
    Engineering and Physical Sciences Research Council SPECIAL EDITION: SCIENCE FOR 16 A CONNECTED NATION Super brain Professor Steve Furber – building a computer to think like a human Greener trucking Cooler ice cream Safer water Smarter energy networks Faster supercomputers CONTENTS 4-5: News Recent EPSRC research and training investments 12 6-9: What we’ve learned Snapshots of EPSRC research and training from the world of engineering and physical sciences 10-15: People Movers, shakers and science in action – from slower melting ice cream, to pioneering technology to 34 help in the global fight against water pollution and water-borne parasites 16-23: Science for a connected nation EPSRC’s portfolio of investments spans the UK economy and society. Chief Executive Professor 26 Philip Nelson describes how it is more than the sum of its parts 24-25: Joined-up thinking New technologies for a smarter, safer, more connected world 26-27: Quantum ballet Doctoral student Merritt Moore describes her dual careers – quantum physics and professional ballet 28-33: Super brain Professor Steve Furber’s remarkable career reaches new heights 34-35: Driving ambition New research cuts road freight emissions and fuel bills by seven per cent 36-39: Only connect Professors Goran Strbac and Tim Green rewrite the 28 energy grid rulebook 40-41: Connected for success Young entrepreneurs’ brilliant businesses span the digital economy 42-43: Swinging wings Bat flight 44 inspires a new generation of micro air vehicles 44-49: EPSRC Science Photo Editor: Mark Mallett ([email protected]) EPSRC works alongside other Research Councils which have responsibility in other research areas.
    [Show full text]
  • Causes of Extremely Fast Cmes
    Solar Activity and its Magnetic Origin Proceedings IAU Symposium No. 233, 2006 c 2006 International Astronomical Union V. Bothmer & A. A. Hady, eds. doi:10.1017/S1743921306002146 Causes of extremely fast CMEs Joan Feynman and Alexander Ruzmaikin Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA email: [email protected] Abstract. We study CMEs observed by LASCO to have plane of the sky velocities exceeding 1500 km/sec. We find that these extremely fast CMEs are typically associated with flares ac- companied by erupting prominences. Our results are consistent with a single CME initiation process that consists of three stages. The initial stage is brought about by the emergence of new magnetic flux, which interacts with the pre-existing magnetic configuration and results in a slow rise of the magnetic structure. The second stage is a fast reconnection phase with flaring, filament eruption and a sudden increase of the rise velocity of the magnetic structure (CME). The third stage consists of propagation in the corona. We discuss the sources of these CMEs and the need for improved understanding of the first and third stages. Keywords. Sun:coronal mass ejections (CMEs), Sun: prominences, Sun: flares, Sun: magnetic fields 1. Introduction The distribution of the plane of the sky velocities of CMEs observed by SOHO is showninFigure1(Yurchyshynet al., 2005). This distribution of 4315 CMEs shows few CMEs with velocities greater than 1500 km/sec and none with velocities exceeding 2000 km/sec. However these are the CMEs that cause the most important solar energetic particle events and the most intense geomagnetic storms.
    [Show full text]
  • Edward P. Richards, the Lessons of Human Adaptation to Climate
    RICHARDS - FINAL WORD (DO NOT DELETE) 11/30/2018 11:02 AM 18 Hous. J. Health L. & Pol’y 131 Copyright © 2018 Edward P. Richards Houston Journal of Health Law & Policy THE SOCIETAL IMPACTS OF CLIMATE ANOMALIES DURING THE PAST 50,000 YEARS AND THEIR IMPLICATIONS FOR SOLASTALGIA AND ADAPTATION TO FUTURE CLIMATE CHANGE1 Edward P. Richards INTRODUCTION................................................................................................ 132 I. PRE-SCIENTIFIC KNOWLEDGE OF THE NATURAL WORLD .......................... 134 II. UNDERSTANDING CLIMATE CHANGE AND CLIMATE ANOMALIES .......... 140 III. MEDIEVAL WARM PERIOD/MEDIEVAL CLIMATE ANOMALY IN THE AMERICAS ............................................................................................ 146 IV. IMPACT OF POST-LAST GLACIAL MAXIMUM SEA LEVEL RISE ................. 150 V. THE NEW THREAT: HEAT........................................................................... 154 VI. SENSE OF PLACE AND CLIMATE CHANGE DRIVEN MIGRATION ............. 158 VII. SOLASTALGIA AND FUTURE ENVIRONMENTAL RISK .............................. 164 CONCLUSION ................................................................................................... 167 1 This paper does not deal with mitigating global warming and ocean acidification through limiting carbon dioxide and other greenhouse gases. It also does not deal with potential con- sequences of ocean acidification. RICHARDS - FINAL WORD (DO NOT DELETE) 11/30/2018 11:02 AM 132 HOUS. J. HEALTH L. & POL’Y INTRODUCTION The earth is warming, local
    [Show full text]
  • Early Prediction of Geomagnetic Storms (And Other Space Weather Hazards) Abstract Introduction
    1 Early Prediction of GeomagneticStorms (andOther Space WeatherHazards) David H. Collins and Joan Feynman Jet Propulsion Laboratory, California Institute of Technology Abstract A detailed conceptual design has been developed for a mission and microspacecraft that can provide information needed to answer key questions about the physics of space weather and also both provide and validate a system for early warning of hazardous space weather. A single small launch vehicleand individually tailored Venus gravity assists disperse nine microspacecraft in a 0.53-0.85 AU band around the Sun. Collectively, the microspacecraft can investigate large-scale organization of coronal mass ejections (CMEs) andparticle acceleration mechanisms near their shocks. Radial and longitudinaldependencies, magnetohydrodynamic (MHD) turbulence in the solar wind, and variations in solar wind velocities and densities can allbe studied.Simultaneously, at least one of themicrospacecraft is nearthe Sun-Earthline almost continuously and can be monitored for earlywarning of hazardous space weather. Introduction In their paper, “On Space Weather Consequences and Predictions,” Feynman and Gabriel [2000]conclude that an important next step in thedevelopment of the understanding and prediction of hazardous space weather is to observe CMEs at 2 heliocentric distances significantly less than 1 AU and along the Sun-Earth line. These observations are needed to test interplanetary shock acceleration and release models for protons and ions with energies >10 MeV and to provide improved long- lead-time predictions of geomagnetic storms. High-velocity CMEs cause geomagnetic storms [Tsurutani and Gonzalez, 19971 and energetic particle events [Kahler et a/., 1984; Gosling, 19931 that present major hazards to both space systems and humans in space [Feynmanand Gabriel, 20001.
    [Show full text]
  • The Physical Sciences Why They Matter
    The Physical Sciences Why they matter #PhysicalSciencesImpact Professor Kyriakos Porfyrakis, with a model of the world’s most expensive material (pages 12-13). 2 The Physical Sciences Why they matter Physics, chemistry and materials science – the physical sciences – comprise our global DNA. By understanding the fundamental building blocks of our universe – heat, light, atoms, the elements, matter, gravity itself – EPSRC-supported physical scientists are unlocking its secrets and providing solutions to the key questions of our age. Without the fundamental research carried out by physical scientists, the internet would run at a snail’s pace, not light-speed; doctors would still be using scalpels to see inside the human body, not X-rays; electric vehicles would barely make it to the shops and back; the water in our homes would not be safe to drink; and computer data would be stored in bungalows, not tiny memory chips. And electric light, fridges, television and mobile phones? There wouldn’t be any. Physical sciences is, above all, discovery-led, through which physicists, chemists and materials scientists ask vital new questions as current ones are answered. Theirs is a continuous process of enquiry and exploration, opening-up new boundaries in space, matter and time itself (pages 16-17). Because this research is fundamental and high-risk, its socio-economic impact can be many years away. For example, in 1917, Einstein proposed the process that makes lasers possible. But it would take nearly 40 years before scientists found a way to harness their potential. EPSRC has invested in fundamental research into lasers for many decades.
    [Show full text]
  • 16 Super Brain
    Engineering and Physical Sciences Research Council SPECIAL EDITION: SCIENCE FOR 16 A CONNECTED NATION Super brain Professor Steve Furber – building a computer to think like a human Greener trucking Cooler ice cream Safer water Smarter energy networks Faster supercomputers CONTENTS 4-5: News Recent EPSRC research and training investments 12 6-9: What we’ve learned Snapshots of EPSRC research and training from the world of engineering and physical sciences 10-15: People Movers, shakers and science in action – from slower melting ice cream, to pioneering technology to 34 help in the global fight against water pollution and water-borne parasites 16-23: Science for a connected nation EPSRC’s portfolio of investments spans the UK economy and society. Chief Executive Professor 26 Philip Nelson describes how it is more than the sum of its parts 24-25: Joined-up thinking New technologies for a smarter, safer, more connected world 26-27: Quantum ballet Doctoral student Merritt Moore describes her dual careers – quantum physics and professional ballet 28-33: Super brain Professor Steve Furber’s remarkable career reaches new heights 34-35: Driving ambition New research cuts road freight emissions and fuel bills by seven per cent 36-39: Only connect Professors Goran Strbac and Tim Green rewrite the 28 energy grid rulebook 40-41: Connected for success Young entrepreneurs’ brilliant businesses span the digital economy 42-43: Swinging wings Bat flight 44 inspires a new generation of micro air vehicles 44-49: EPSRC Science Photo Editor: Mark Mallett ([email protected]) EPSRC works alongside other Research Councils which have responsibility in other research areas.
    [Show full text]
  • Annual Report 2010 Supporting Only the Best, So That They Can Become Even Better
    Foundation for Polish Science Annual Report 2010 Supporting only the best, so that they can become even better The programmes WELCOME, International PhD Projects (MPD), TEAM, VENTURES, HOMING PLUS and PARENT-BRIDGE are co-financed from the European Regional Development Fund within the Innovative Economy Operational Programme. annual report 2010 he Foundation for Polish Science is a non-governmental, apolitical, non-profit organization active T since 1991. Its mission is to support science in Poland. The Foundation fulfils its statutory role by financing individual projects of scientists and research teams, as well as initiatives serving Polish science. As the largest Polish non-budgetary source of funding scientific research, the Foundation also tries to propagate throughout society an understanding of the significance of science in the development of Poland. The Foundation presents individual awards, scholarships and research grants to the best scholars, while actively supporting international scientific cooperation and the development of initiatives that foster greater academic independence among young researchers. Beneficiaries of the Foundation’s programmes are selected through competitions. All the applications for competitions are assessed by way of the peer- -review system; the review body working with the Foundation comprises several thousand scientists from Poland and abroad, who are renowned specialists in their fields. The most important criterion for awarding financial support is the quality of the candidate’s scientific knowledge and achievements, in accordance with the Foundation’s guiding motto: Supporting only the best, so that they can become even better. The Foundation’s founding capital of 95 million zlotys originated from the Central Fund for the Development of Science and Technology, which was liquidated in 1990, whereupon the capital was directed to the FNP by a decision of the Polish parliament.
    [Show full text]
  • Annual Report 2018
    Annual Report 2018 The NQIT Entangler, developed by the University of Southampton / Paul Gow & Paolo Mennea Contributors Andru Gheorghiu Animesh Datta Chris Wade David Nadlinger Dominic O’Brien Evert Geurtsen Ezra Kassa Frances Sweeney Hannah Rowlands Ian Walmsley Iris Choi Jaewoo Joo Jason Smith Jonas Becker Nathan Walk Niel de Beaudrap Peter Leek Petros Wallden Philip Inglesant Rishi Deshmukh Rupesh Srivastava Simon Benjamin Weida Zhang Winfried Hensinger Xiao Yuan Editors Frances Sweeney Hannah Rowlands Rupesh Srivastava Design and Print Hunts Core Engineering Capabilities . 30 Contents Architecture Progress . 31 Qubits: quality vs . quantity . 33 Applications & Software . 34 Foreword . 1 Applications Introduction . 34 Introduction . 3 Secure Network Applications . 35 Year Three Achievements . 5 Networked Quantum Sensors . 35 Programme Structure . 6 Quantum Enabled Discovery . 36 The NQIT Consortium . 7 Quantum/Classical Emulation and Interfacing . 36 UK Partners Map . 8 Development of Quantum Applications . 38 Industry and Strategic Partners . 9 Quantum Optimisation and People . 10 Machine Learning . 39 NQIT Ecosystem . 12 How does quantum computing intersect Quantum Computing in a Global Context . 13 with machine learning? . 40 Science and Innovation Audit for Oxfordshire . 15 Wider Engagement . 41 Industry Engagement . 16 Responsible Research and Innovation . 41 NQIT Industry Day 2017 . 17 Public Engagement . 42 National Quantum An Evening of Quantum Discovery . 43 Technologies Showcase 2017 . 18 Quantum Photography Competition . 44 IBM Q Collaboration . 19 Walk-in Quantum Computer Installation . 45 Wireless Radio Frequency Inter-Hub Collaboration . 45 Feedthrough for Ion Traps with ColdQuanta . 20 Skills and Training . 46 Spinout Companies . 21 Oxford Quantum Circuits . 22 Future Plans . 47 Innovate UK: Commercialisation of Beecroft Building . 48 Quantum Technologies .
    [Show full text]