Iop Pab Group Newsletter
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The Institute of Physics
REGIONAL NEWS 21 The Institute of Physics The forerunner of the Institute of do involves physics - switching on a light, physicists in commerce and industry. The Physics, the Physical Society of London, making a phone call or even baking a Council has established several Profession was created in 1874 at a time when the potato in a microwave oven. In industry, al Groups in areas such as consultancy, understanding of the physical world had physicists are helping companies to devel engineering physics and advanced been given an enormous impetus with the op novel materials that have physical prop systems. publication by James Clerk Maxwell of his erties more versatile that those previously In these days of shrinking science theory of electromagnetism. The creation developed, and they are designing new budgets, the academic physics community of the Physical Society was the response of generations of microchips which are has turned increasingly to its professional the embryonic society of professional and smaller and hence faster. The information representative, the Institute of Physics, to amateur physicists in Britain to what they revolution within which we are currently lobby Government about the importance believed was a major progression of their being buffeted would have been impos and relevance of physics. In common with ideas. Indeed, one could say that it was at sible without physicists and their research other science subjects, calls to justify Gov this time that much of physics began to - transistors, liquid crystal displays, mag ernment expenditure have increased in take on the appearance we recognize netic discs, optical fibres, semiconductor recent years. -
Daresbury Open Week 2020 Free KS5 Masterclass Events 29Th and 30Th June 2020
Daresbury Open Week 2020 Free KS5 Masterclass events 29th and 30th June 2020 As part of the Sci-Tech Daresbury Open Week, we are dedicating two full days delivering activities for school children from upper primary school through to upper secondary school. • Monday 29 June: Key Stage 2 & Key Stage 5 • Tuesday 30 June: Key Stage 3, Key Stage 4 & Key Stage 5 These exciting days of talks, tours and interactive workshops will fire your students’ imagination and inspire them about cutting edge science and technology, as well as STEM career opportunities. KS5 Workshop 1 Workshop: Electron Microscopy Be prepared to be taken to one of the world’s most powerful electron microscopes, located in the SuperSTEM facility here at Daresbury. Students will witness live data coming from the microscope that will enable them to visualise individual atoms. Students will complete hands-on activities that will teach them how and why we need to use electrons to produce these inspiring images. They will learn that the technological developments incorporated into the SuperSTEM microscopes form some of the most precise optics used in science. KS5 Workshop 2 Workshop: Scientific Computing Did you know that computational science and engineering is vital for research into complex fields such as the origins of life, how medicines work in cells within the body, and designing new materials that could help us live on Mars? Did you also know, that computational science and engineering has contributed to the development of many everyday items such as cosmetics, tablets and vacuum cleaners? Although covering many different topics, computational science and engineering always follows the same procedure, whether it is being used to explore the air flow over a vehicle or looking at how molecules attach themselves to proteins within cells. -
Template: 10Th Anniversary Powerpoint
Science and Technology Facilities Council One of Europe’s largest multi-disciplinary scientific research organisations Dr Ling Xu How we’re funded Taxpayers HM Government (and HM Treasury) STFC science and technology delivers real benefits to peoples’ lives, and contributes to the prosperity and security of the UK Delivering Economic Growth through Innovation STFC’s Asset Base Innovation Resilient Economy Knowledge Skills Technology Inspiration What we spend £530m from government in 2015-16* • International Subscriptions (CERN, ESO, ILL, ESRF, FAIR) £155m • Domestic Facilities (ISIS, Diamond, CLF) £156m • Core (academic grants, lab operations, support services) £218m • Supplemented by project-based external revenue around £60m p.a. International Facilities Core Revenue What we do World Class Research, Innovation and Skills • Broad range of physical, life and computational sciences • Around 1,700 scientists in particle and nuclear physics, and astronomy mainly in the University Sector • Access for 7,500 scientists to world-leading, large-scale facilities • Science and Innovation Campuses at Daresbury and Harwell • Globally-recognised capabilities and expertise in technology R&D • Inspiring young people to undertake STEM What we are Boulby Underground UK Astronomy Technology Centre Laboratory Edinburgh, Scotland North Yorkshire Polaris House Daresbury Laboratory Swindon, Wiltshire Sci-Tech Daresbury Warrington, Cheshire Chilbolton Observatory Rutherford Appleton Laboratory Stockbridge, Hampshire Harwell Didcot, Oxfordshire …and internationally Our facilities drive research Neutron Sources • Providing powerful insights into key areas of energy, biomedical research, climate, environment and security. High Power Lasers • Providing applications on bioscience and nanotechnology and demonstrating laser driven fusion as a future source of sustainable, clean energy. Light Sources • Providing new breakthroughs in medicine, environmental and materials science, engineering, electronics and cultural heritage. -
E-310 Trojan Horse-II at FACET-II and the STFC PWFA-FEL Programme Thursday, 19 September 2019 19:00 (20 Minutes)
4th European Advanced Accelerator Concepts Workshop Contribution ID: 337 Type: talk E-310 Trojan Horse-II at FACET-II and the STFC PWFA-FEL programme Thursday, 19 September 2019 19:00 (20 minutes) The beam-driven plasma photocathode wakefield acceleration concept [1] allows decoupled laser injection of electron bunches with emittance and brightness reach many orders of magnitude better than state-of-the-art [2]. After successful proof-of-concept demonstration at SLAC FACET in the “E-210: Trojan Horse” project [3], we now embark on the next experimental phase around the “E-310: Trojan-II” flagship and five related experiments at FACET-II, where better incoming beams and improved setup may unleash the full potential of the scheme. Plans for FACET-II experiments and complementary progress and plans on hybrid LWFA- >PWFA with automatically synchronized plasma photocathodes will be presented. Looking further ahead, the UK STFC has initiated the UK-US “PWFA-FEL” programme, which aims to push exploitation of the ultralow emittance and ultrahigh brightness of beams which may be obtainable from upcoming installations ofplasma photocathodes. This project will explore the benefits of ultrahigh brightness beams and will alsobeusedto assist experimental programmes on PWFA and plasma photocathodes at Daresbury’s CLARA facility and at FACET-II, and at future hybrid LWFA->PWFA systems. [1] PRL 108, 035001 (2012) [2] Nat. Comm. 8,15705 (2017) [3] Generation and acceleration of electron bunches from a plasma photocathode, Nat. Phys., accepted (2019) Primary authors: ROSENZWEIG, James (UCLA); HOGAN, Mark (SLAC National Accelerator Laboratory); KARGER, Oliver (University of Hamburg, Institute for Experimental Physics); HEINEMANN, T. -
2013 January
Online Newsletter January 2013 Issue no 24 Branch committee REMS At Home - An Environmental Miscellany Dr Mark Telling CPhys MInstP, Chair On 10 January 71 members and guests were educated and entertained E-mail [email protected] by 5 invited speakers. The meeting was organised and orchestrated by Bob Boutland CPhys MInstP George Freeman, who unfortunately could not attend during Treasurer recuperation following an operation. Mike Quinton, (pictured below) Education representative introduced the speakers. and online newsletter editor E-mail [email protected] David Parkes CPhys MInstP Berkshire Centre representative E-mail [email protected] Stephen Elsmere Berkshire Centre representative E-mail [email protected] Leonard Lewell CPhys MInstP, London Centre Representative E-mail [email protected] Prof. R Mackintosh CPhys FInstP Milton Keynes Centre representative E-mail [email protected] Dr Diane Crann MInstP Hertfordshire Centre representative E-mail [email protected] J A Belling MInstP REMS visit secretary E-mail [email protected] The Barometer and its early use in forecasting on land and on sea” Marta Caballero E-mail [email protected] Anita McConnell Provided a very detailed story from the early days. It Student Representative was Torricelli and Viviani who showed in 1643-4 that there is such a thing as a vacuum noting that the height of the column mercury varied James Kneller daily with changes in the weather, but also with temperature. Pascal E-mail [email protected] Student Representative noted that a barometer recorded a lower pressure when taken up a mountain, the Puy de Dôme. -
Peter Kalmus, Rubab Khan, Luca Matone, Szabolcs Márka
Search Method for Gravitational Wave Transients Associated with the SGR 1806-20 Giant Flare We describe a method for searching for transient gravitational waves associated with the SGR 1806-20 T Peter Kalmus, Rubab Khan, Luca Matone, Szabolcs Márka C giant flare of 27 December 2004 using data collected by the LIGO 4 km detector located at Hanford, WA. A We create an excess power time series from a time-frequency tiling by projecting elements in the R T frequency band of interest onto the time axis. This time series is calibrated with injections of known Columbia University Experimental Gravity Group S strength. An upper limit estimate can then be obtained by selecting the loudest event in the on-source B A region. Validations for the search and estimated sensitivity, obtained by performing the search on realistic simulated LIGO data, are presented. 7. Estimated Sensitivity From Simulated Data 5. The Search Algorithm Simulated Noise 1. An Extraordinary Event To create simulated noise, a segment of LIGO noise is taken as a model. The individual On 27 December 2004, SGR 1806-20, a 'Soft Gamma Repeater' located 6-15 kpc Creation of Tiling and Band Plot data samples are randomly shuffled. The amplitude spectral density of the result is then away [1, 2], emitted the brightest transient ever observed [1, 6, 8, 11, 15]. Data Conditioning Conditioned data is transformed into a spectrogram, which is a linear time- matched to the LIGO noise bin by bin in frequency space, and the resulting series is frequency tiling. We take the complex magnitude of the resulting matrix. -
Family Day Site
FAMILY DAY SITE MAP 15 17 14 18 16 TO PUBLIC CAR PARK 13 CAMPUS TECHNOLOGY HUB BUS STOP DROP OFF ZONE 12 11 10 8 KECKWICK LANE 9 WELCOME TENT 1 7 2 CATERING MARQUEE 6 19 3 RESTAURANT A BLOCK COCKCROFT INSTITUTE 5 BLUE BADGE 4 Map Key PARKING Food Water Stations INNOVATION CENTRE LOST CHILDREN Children identified as being separated from Mother and Baby 20 parents or guardians will initially be looked after Coffee Pods by staff in the vicinity of the area that they are Nursing Room found for 5 minutes. Toilets Baby Changing If parents or guardians are unable to reunite with their children within this time then children will be brought to the care of the Police who will be First Aid Lost Child Reunion BRIDGEWATER CANAL onsite in the Crime Prevention Roadshow. No 12 on the map 16 Dinozone YELLOW ZONE • Meet REX the T-Rex • Everything Dinosaur! 13 Campus Technology Hub • Digging for Fossils RED ZONE ORANGE ZONE Engineering and Innovation • Digital Dinosaurs • Laser Balloon Bursting with the • University of Manchester Central Laser Facility Palaeontology 1 Welcome Tent 9 Horizon Visitor Centre • Lego Space Rovers & Lego 17 SuperSTEM Dark Skies & Big Telescopes Challenge • Planetarium Star Shows Discover Electron Microscopes! 2 Security / Lost Property • 3D Printing in Action! (Limited Numbers Only) • Moon Rocks and Meteorites • 3D Scanning: Extreme Close Up! • Dry Ice Comet Show 3 Daresbury Laboratory • Riverside College F1 Pit Stop • Telescopes – See the Invisible Show • The Careers Hub Reception (Top Floor) • Build ‘n’ Launch a Rocket GREEN -
APPLICATION NO: 13/00350/FUL LOCATION: Sci Tech Daresbury
APPLICATION NO: 13/00350/FUL LOCATION: Sci Tech Daresbury, Keckwick Lane, Daresbury PROPOSAL: Proposed creation of a linear park and square, improvements to Innovation Way and Keckwick Lane together with associated landscaping, lighting, demolition of single bungalow and retrospective planting works WARD: Daresbury PARISH: Daresbury CASE OFFICER: Pauline Shearer AGENT(S) / APPLICANT(S): Daresbury Science and Innovation Centre LLP, Sci-Tech Daresbury, Keckwick Lane, Daresbury DEVELOPMENT PLAN ALLOCATION: National Planning Policy Framework (2012) North West Plan: Regional Spatial Strategy for the North West (2008) Halton Unitary Development Plan (2005) Halton Core Strategy Local Plan (2013) DEPARTURE No REPRESENTATIONS: No objections KEY ISSUES: Highway safety; design; landscaping RECOMMENDATION: Approval SITE MAP 1. APPLICATION SITE 1.1 The Site The site is located at the Daresbury Science and Innovation Centre (DSIC) on Keckwick Lane, Daresbury. The land either side of this application site on Keckwick Lane is in the ownership of DSIC containing buildings and infrastructure relating to the use of the campus for scientific developments. The site is identified as the Daresbury Strategic Site within the East Runcorn Key Area of Change in the Halton UDP and Core Strategy. 1.2 Planning History There is no particular planning history which is relevant to the development along Keckwick Lane. 2. THE APPLICATION 2.1 The proposal The proposal is a result of a site connectivity project undertaken by DSIC, now branded Sci-Tech Daresbury (and will be referred to as such during the remainder of this report), to deliver a joined up, public realm and highways scheme along Innovation Way and Keckwick Lane to improve access and movement to and within the campus. -
Status Solid I Physica
pssi c solid status www.pss-c.com physica current topics in solid state physics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phys. stat. sol. (c) 5, No. 8, 2621–2626 (2008) / DOI 10.1002/pssc.200779109 REPRINT phys. stat. sol. (c) 5, No. 8, 2621–2626 (2008) / DOI 10.1002/pssc.200779109 c solidi pssstatus www.pss-c.com physica current topics in solid state physics Reflection anisotropy spectroscopy of biological molecules with the 4GLS source P. -
Iop Pab Group Newsletter
INSTITUTE OF PHYSICS IOP PAB GROUP NEWSLETTER Issue 16 Editorial December 2017 When reading through the draft of this Newsletter, I was struck by the wide range of activities, research and impact that flows from the field of Particle Accelerators and Inside this issue: Beams. From adults given freedom to behave like children at the Accelerate! outreach event organised by the John Adams Institute, to Alisa Healy, an ASTeC and Lancaster University PhD student, winning a very competitive best student poster at the News from Daresbury — 2 3rd European Advanced Accelerator Concepts Workshop, to the new developments at Demonstration of Slow- the CLARA FEL test facility at Daresbury Laboratory and great progress at the MICE Light for Particle Acceleration, facility. A wide range of workshops, conferences and other developments with ASTeC and Lancaster significant international impact is also reported. The UK is certainly at the forefront of Student Wins Prize our field internationally. Cryogenic Cluster Day 3 STFC are currently undertaking a Strategic Review of its Accelerator Programme. This 2017 will affect the research commitments and directions pursued by STFC for the next Magnets For Cancer 4 twenty years and is therefore of great importance to the work we do and will have long Therapy -lasting consequences. So, if you can, engage with STFC and let them know what you First Accelerated Beam 5 and the beneficiaries of your science think are the important strategic areas that should Through Linac 1 be developed. News from RAL — 6 An update on MICE This year our annual meeting will be hosted by Lancaster University on Wednesday 18 April, 2018. -
Symposium Celebrating CERN's Discoveries and Looking Into the Future
CERN–EP–2003–073 CERN–TH–2003–281 December 1st, 2003 Proceedings Symposium celebrating the Anniversary of CERN’s Discoveries and a Look into the Future 111999777333::: NNNeeeuuutttrrraaalll CCCuuurrrrrreeennntttsss 111999888333::: WWW±±± &&& ZZZ000 BBBooosssooonnnsss Tuesday 16 September 2003 CERN, Geneva, Switzerland Editors: Roger Cashmore, Luciano Maiani & Jean-Pierre Revol Table of contents Table of contents 2 Programme of the Symposium 4 Foreword (L. Maiani) 7 Acknowledgements 8 Selected Photographs of the Event 9 Contributions: Welcome (L. Maiani) 13 The Making of the Standard Model (S. Weinberg) 16 CERN’s Contribution to Accelerators and Beams (G. Brianti) 30 The Discovery of Neutral Currents (D. Haidt) 44 The Discovery of the W & Z, a personal recollection (P. Darriulat) 57 W & Z Physics at LEP (P. Zerwas) 70 Physics at the LHC (J. Ellis) 85 Challenges of the LHC: – the accelerator challenge (L. Evans) 96 – the detector challenge (J. Engelen) 103 – the computing challenge (P. Messina) 110 Particle Detectors and Society (G. Charpak) 126 The future for CERN (L. Maiani) 136 – 2 – Table of contents (cont.) Panel discussion on the Future of Particle Physics (chaired by Carlo Rubbia) 145 Participants: Robert Aymar, Georges Charpak, Pierre Darriulat, Luciano Maiani, Simon van der Meer, Lev Okun, Donald Perkins, Carlo Rubbia, Martinus Veltman, and Steven Weinberg. Statements from the floor by: Fabiola Gianotti, Ignatios Antoniadis, S. Glashow, H. Schopper, C. Llewellyn Smith, V. Telegdi, G. Bellettini, and V. Soergel. Additional contributions: Comment on the occasion (S. L. Glashow) 174 Comment on Perturbative QCD in early CERN experiments (D. H. Perkins) 175 Personal remarks on the discovery of Neutral Currents (A. -
Newsletter, November 2017
ISSN 1756-168X (Print) ISSN 2516-3353 (Online) Newsletter No. 35 November 2017 Published by the History of Physics Group of the Institute of Physics (UK & Ireland) ISSN 1756-168X IOP History of Physics Newsletter November 2017 Contents Editorial 2 Meeting Reports Chairman’s Report 3 Rutherford’s chemists - abstracts 5 ‘60 Years on from ZETA’ by Chris Warrick 10 Letters to the editor 13 Obituary John W Warren by Stuart Leadstone 15 Features Anti-matter or anti-substance? by John W Warren 16 A Laboratory in the Clouds - Horace-Bénédict de Saussure by Peter Tyson 18 On Prof. W.H.Bragg’s December 1914 Letter to the Vice- Chancellor of the University of Leeds by Chris Hammond 34 Book Reviews Crystal Clear - Autobiographies of Sir Lawrence and Lady Bragg by Peter Ford 54 Forthcoming Meetings 69 Committee and contacts 70 61 2 Editorial A big ‘Thank you’! Around 45 people attended the Bristol meeting on the History of Particle Colliders, in April. It was a joint meeting between the History of Physics Group, the High Energy Physics Group, and the Particle Accelerators and Beams Group. With a joint membership of around 2000, that works out at well under 3% - and that was a good turnout. The Rutherford’s Chemists meeting held in Glasgow attracted probably a similar percentage - not very high you might think. But time and travel costs to attend come at a premium so any means by which the content of our meetings may be promulgated - reports in our newsletter and in those of the other groups - is a very worthwhile task.