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Autumn Department of Physics Newsletter Issue
Autumn 2018, Number 13 Department of Physics Newsletter BEECROFT BUILDING OFFICIAL OPENING BEAUTIFUL HIGGS BOSON DECAYS MAGNETIC PINWHEELS EXTREME BEAM CONTROL COSMIC SHOCKS IN THE LABORATORY PEOPLE, EVENTS AND MORE www.physics.ox.ac.uk PROUD WINNERS OF: SCIENCE NEWS SCIENCE NEWS www.physics.ox.ac.uk/research www.physics.ox.ac.uk/research BEAUTIFUL HIGGS BOSON EXTREME BEAM CONTROL An Oxford team has succeeded in stabilising the arrival time of a ‘relativistic’ beam of electrons, travelling at almost the speed of light, to 50 femtoseconds. This overcomes one of the major challenges facing the proposed DECAYS Compact Linear Collider (CLIC). On 28 August 2018 the ATLAS and Higgs from the background. These Standard Model, the prevailing theory CMS collaborations announced, with results were used in the final Tevatron of particle physics. If this prediction had a seminar at CERN, the observation of combination, which reached almost turned out to be incorrect, it would have the Higgs boson decaying into pairs of three standard deviations in 2012, not shaken the foundations of the Standard beauty (b) quarks. Both experiments enough for a discovery. Model and pointed to new physics. at the Large Hadron Collider (LHC) Instead, this is an important milestone had surpassed the five standard and a beautiful confirmation of the EXPERIMENTAL CONFIRMATION deviations (sigma) mark for this process, so-called 'Yukawa couplings', which in Prof Daniela Bortoletto which is the convention in particle Goethe said: ‘Not art and science the Standard Model give masses to all Head of Particle Physics physics to claim a discovery. Five- serve alone; patience must in the quarks and leptons, the building blocks sigma corresponds to a probability of work be shown.’ It was with patience, of matter. -
Benefactors 2020
Contents 2 From the President 4 From the Development Director 6 Your Gifts 8 Graduate Scholars 12 Special Grants 18 Access and Outreach 22 Buildings 26 Why I Give 30 Financial Report 32 Roll of Benefactors Including Summary Financial Report, Sources and Use of Funds for the year 2018–19 Benefactors is now plastic free and can be recycled with your usual household paper recycling. The mailing bag is made of a compostable plastic-free material. 1 From the President St John’s continues to make progress on all fronts and I’m delighted to be able to share our news in this edition of Benefactors. This academic year we are celebrating the 40th anniversary will be independent evaluation of the effectiveness of since women were first admitted to St John’s. The this programme and we are hopeful that we have a great programme of events has been interesting and thought- model that can deliver a significant impact and that could provoking and has put a clear focus on issues of diversity, be rolled out more widely. equality and inclusion, not only in our day-to-day activities in College but also in our continuing efforts to attract the It was excellent to celebrate the opening of the new Study brightest and best to St John’s, irrespective of background. Centre last October and a wonderful opportunity to thank the donors who helped make the project happen. The College – and the University overall – are making We continue to invest substantially in the renovation significant progress on access. You may be aware of of College buildings with work in 2020 on St Giles the new Opportunity Oxford programme: students House, a redesign of the Lodge, and on the third and invited onto Opportunity Oxford are made the standard final phase of the Library project, including conservation offer for their course and then take part in a supportive improvements to the Old Library and Laudian Library bridging programme in the run-up to their first term. -
For Digital Simulation and Advanced Computation 2002 Annual Research Report
for Digital Simulation and Advanced Computation 2002 Annual Research Report 2002 Annual Research Report of the Supercomputing Institute for Digital Simulation and Advanced Computation Visit us on the Internet: www.msi.umn.edu Supercomputing Institute for Digital Simulation and Advanced Computation University of Minnesota 599 Walter 117 Pleasant Street SE Minneapolis, Minnesota 55455 ©2002 by the Regents of the University of Minnesota. All rights reserved. This report was prepared by Supercomputing Institute researchers and staff. Editor: Tracey Bartlett This information is available in alternative formats upon request by individuals with disabilities. Please send email to [email protected] or call (612) 625-1818. The University of Minnesota is committed to the policy that all persons shall have equal access to its programs, facilities, and employment without regard to race, color, creed, religion, national origin, sex, age, marital status, disability, public assistance status, veteran status, or sex- ual orientation. contains a minimum of 10% postconsumer waste Table of Contents Introduction Supercomputing Resources Overview....................................................................................................................................2 Supercomputers ........................................................................................................................3 Research Laboratories and Programs ......................................................................................5 Supercomputing Institute -
Pandemics: a Very Short Introduction VERY SHORT INTRODUCTIONS Are for Anyone Wanting a Stimulating and Accessible Way Into a New Subject
Pandemics: A Very Short Introduction VERY SHORT INTRODUCTIONS are for anyone wanting a stimulating and accessible way into a new subject. They are written by experts, and have been translated into more than 40 different languages. The series began in 1995, and now covers a wide variety of topics in every discipline. The VSI library now contains over 450 volumes—a Very Short Introduction to everything from Indian philosophy to psychology and American history and relativity—and continues to grow in every subject area. Very Short Introductions available now: ACCOUNTING Christopher Nobes ANAESTHESIA Aidan O’Donnell ADOLESCENCE Peter K. Smith ANARCHISM Colin Ward ADVERTISING Winston Fletcher ANCIENT ASSYRIA Karen Radner AFRICAN AMERICAN RELIGION ANCIENT EGYPT Ian Shaw Eddie S. Glaude Jr ANCIENT EGYPTIAN ART AND AFRICAN HISTORY John Parker and ARCHITECTURE Christina Riggs Richard Rathbone ANCIENT GREECE Paul Cartledge AFRICAN RELIGIONS Jacob K. Olupona THE ANCIENT NEAR EAST AGNOSTICISM Robin Le Poidevin Amanda H. Podany AGRICULTURE Paul Brassley and ANCIENT PHILOSOPHY Julia Annas Richard Soffe ANCIENT WARFARE ALEXANDER THE GREAT Harry Sidebottom Hugh Bowden ANGELS David Albert Jones ALGEBRA Peter M. Higgins ANGLICANISM Mark Chapman AMERICAN HISTORY Paul S. Boyer THE ANGLO-SAXON AGE AMERICAN IMMIGRATION John Blair David A. Gerber THE ANIMAL KINGDOM AMERICAN LEGAL HISTORY Peter Holland G. Edward White ANIMAL RIGHTS David DeGrazia AMERICAN POLITICAL HISTORY THE ANTARCTIC Klaus Dodds Donald Critchlow ANTISEMITISM Steven Beller AMERICAN POLITICAL PARTIES ANXIETY Daniel Freeman and AND ELECTIONS L. Sandy Maisel Jason Freeman AMERICAN POLITICS THE APOCRYPHAL GOSPELS Richard M. Valelly Paul Foster THE AMERICAN PRESIDENCY ARCHAEOLOGY Paul Bahn Charles O. -
Revisiting the Mystery of Pg1407+265
REVISITING THE MYSTERY OF PG1407+265 Jonathan C. McDowell (CfA), Aneta Siemiginowska (CfA), Luigi Gallo (Halifax), Katherine Blundell (Oxford) The unusual z=0.94 quasar PG1407+265 shows anomalously weak emission lines and intermediate-level radio emission. It has been interpreted (Blundell, Beasley and Bicknell 2003) as an intrinsically radio-quiet quasar with a stunted, pole-on relativistic radio jet. We present a preliminary reanalysis of existing X-ray data in the light of recent theoretical developments, providing new clues to the nature of this object and the role of inflows and outflows in luminous AGN. X-ray Clusters and Quasar Feedback Chandra observations of X-ray clusters indicate that the powerful outbursts of radio activity in the central AGN can provide enough energy to heat up the cluster and prevent its cooling (see McNamara and Nulsen 2007 for review). This so-called “radio mode” feedback has observational support, but the luminous quasars with highest mass black holes and highest accretion rates can also provide enough energy to drive powerful outflows and winds which can provide the required heat in cooling core clusters without help from the radio jet (e.g. Fabian 2009). The evidence for “quasar mode” feedback has been emerging only recently thanks to recent Chandra observations of two cooling core clusters associated with the luminous quasars 3C 186 (Siemiginowska et al 2010) and H1821+643 (Russell et al Fig 1: UV-optical-IR spectrum from McDowell et al 201). King (2009, 2010) argues that this “quasar mode” could be the more important mechanism but so far there are few 1995 showing anomalously weak lines; the high ionization lines show blueshifts of >10000 km/s examples of clusters where this phenomenon can be studied. -
Paul Goodall, Fathallah Alouani Bibi, Katherine Blundell
Hydrodynamic Simulations of the SS 433 -W50 Complex Paul Goodall, Fathallah Alouani Bibi, Katherine Blundell ABSTRACT METHOD RESULTS .. The compelling evidence for a connection between SS 433 and W50 The field-of-view of our simulation has been chosen carefully to match 51 Evolution of the SNR in the Galactic density gradient: Eblast = 10 ergs has provoked much imagination for decades. There are still many unan- that of the Dubner et al., (1998) image (see Fig.1), and we achieve a max- -120 -100 -80 -60 -40 -20 0 20 40 60 80 100 -120 -100 -80 -60 -40 -20 0 20 40 60 80 100 50 Entropy Index S(t) Entropy Index S(t) 50 swered questions; What was the nature of the progenitor of the compact imum spatial resolution ∆x = 0.014pc on the AMR grid. We create the 40 Sim-time: 38062 years. Sim-time: 38962 years. 40 30 30 object in SS 433? What causes the evident re-collimation in SS 433’s jets? local background environment of SS433 and W50, using the Galactic den- 20 20 10 10 How recent is SS 433’s current precession state? What mass and energy sity profile adapted from Dehnen & Binney (1998), according to: 0 0 -10 -10 contributions from a possible supernova explosion are required to produce -20 -20 Rm R z -30 -30 W50? Here we comment on two of our 53 models: (i) featuring the SNR ρ (R, z) = ρ exp − − − (1) -40 -40 ISM o ( ISM ) -50 -50 evolution alone, and (ii) the SNR combined with a simple jet model. -
Cosmic Concepts: Faster Than Light?
2 OCTOBER 2019 Cosmic Concepts: Faster than Light? PROFESSOR KATHERINE BLUNDELL How do we learn about the cosmos? Prior to a few years ago, the only way that humankind could glean information from the cosmos was via the detection of light. Light of all different colours and wavelengths propagates across the Universe encoding information about the physical properties of different phenomena. For the last few years, gravitational radiation is becoming a new way of learning about the Universe outside of Earth. How much faster is the speed of light than the speed of sound? In a thunder and lightning storm, we are used to hearing thunder a notable delay after seeing a fork of lightning. This is because light from the lightning travels faster than sound from the same event. In fact, light travels about one million times faster than sound. How is speed defined? Speed is defined as the ratio of the distance taken to travel and the time taken to travel that distance. Fast speeds are difficult to measure, especially when small distances (and short transit times) are involved. Making a measurement outside of planet Earth, and scaling up in size, for example to the solar system helps greatly. What’s orbiting around Jupiter? Although planet Earth has only one satellite, our Moon, orbiting around it, the planet Jupiter has very many moons orbiting around it. The number currently known is 79! The first four of these were discovered by Galileo Galilei in 1610. These first four, known as the Galilean moons, are the brightest of all the moons. -
Benefactors' Report 2014/15
S T J OHN ’ S C OLLEGE , O XFORD BENEFACTORS’ REPORTSources and Uses of Funds Issue 7 Hilary 2015 Contents From the President / 2 From the Founder’s Fellow / 4 Summary Financial Report / 8 Alumni Fund & 1555 Society/ 10 Scholarships & Grants / 12 Dr Yungtai Hsu & McLeod Graduate Scholarships/ 13 Lester B Pearson Scholarship / 14 Special Grants / 16 Roll of Benefactors / Insert Duveen Travel Scholarship/ 19 Mahindra Travel Scholarship / 22 Focus on Research / 25 Global Jet Watch Project / 26 A Legacy in Honor of Professor Thomas Kilner / 30 editors Professor John Pitcher, Founder’s Fellow Caitlin Tebbit, Development Officer Jennie Williams, Development Assistant Caitlyn Lindsay, Development Assistant Photography by Henry Tann (2011, History) Design by Caitlin Tebbit, Development Officer With heartfelt thanks to our contributors and advisors. The views or opinions expressed herein are the contributors’ own and may not reflect the views or opinions of St John’s College, Oxford. 2 – benefactors’ report issue 7 | hilary 2015 – 1 From the President Professor Maggie Snowling As I embark on my third year as President I now finally feel as though the 2000th woman matriculated. To celebrate this milestone and inspire I have my feet firmly under the table! This is in no small part because future generations of St John’s women, we are hosting programmes of how busy we have been and how many successes we have been lucky and events for female undergraduates and alumnae. These include the enough to celebrate during the year. Our Fellows continue to be elected to Springboard development programme for students, the inaugural Lady Fellowships of Learned Societies, to be granted Titles of Distinction and White lecture, a Gender Equality Festival and the launch of a specially to receive honorary degrees, and to do so while they offer teaching and commissioned anthem, ‘The Song of Wisdom’. -
Physics Meets Biology 2019 9–11 September 2019 University of Oxford, Oxford, UK
Delegate Handbook Physics Meets Biology 2019 9–11 September 2019 University of Oxford, Oxford, UK http://pmb2019.iopconfs.org Contents Contacts 2 Disclaimer 2 Social media 2 Sponsors 3 Committee 3 Venue 4 Site Maps 5 Accommodation 5 WiFi 5 Travel 5 Programme 6 Registration 6 Catering 6 Dietary requirements 6 Social Programme 7 Payment 7 Presenter instructions 8 Poster presentations 8 Safety and emergency evacuation procedures 9 Smoking 9 First aid 9 Weather 9 Conference app 10 1 | Page Contacts If you have any questions or require further information, please contact a member of the Institute of Physics conference organising team, Jason Eghan or Marcia Reais. Jason and Marcia will be on-site for the duration of the conference and will be based on Sunday in St. Anne’s College in the Lodge and then in the Department of Physics, Martin Wood Foyer on the Reception Desk during registration times (see page 6). Outside of these times and only in case of an emergency, please telephone 07884 426 8232. Jason Eghan Tel: +44 (0)207470 4984 Mobile: +44 (0)7884 426 8232 Email: [email protected] Marcia Reais Tel: +44 (0)207470 4831 Email: [email protected] Conferences Tel: +44 (0)20 7470 4800 Email: [email protected] We hope that your time at the conference is trouble free. If you do encounter any problems, please report them to the conferences team who will make every effort to rectify the issue as soon as possible. Disclaimer The Institute of Physics, University of Oxford and their approved representatives accept no responsibility for any accident, loss or damage to participant’s property during the conference. -
Oxford Physics Newsletter
Spring 2011, Number 1 Department of Physics Newsletter elcome to the first edition of Oxford Physics creates new solar-cell the Department technology Wof Physics Newsletter. In this takes place to generate free electrons, which edition, we describe some of Henry Snaith contribute to a current in an external circuit. The the wide range of research original dye-sensitised solar cell used a liquid currently being carried out in The ability to cheaply and efficiently harness the power of electrolyte as the “p-type” material. the Oxford Physics Department, the Sun is crucial to trying to slow The work at Oxford has focused on effectively and also describe some of down climate change. Solar cells replacing the liquid electrolyte with p-type the other activities where we aim to produce electricity directly from sunlight, organic semiconductors. This solid-state system seek to engage the public in but are currently too expensive to have significant offers great advantages in ease of processing and impact. A new “spin-out” company, Oxford science and communicate with scalability. Photovoltaics Ltd, has recently been created to potential future physicists. I commercialise solid-state dye-sensitised solar Over the next two to three years, Oxford hope you enjoy reading it. If you cell technology developed at the Clarendon Photovoltaics will scale the technology from laboratory to production line, with the projected have passed through Oxford Laboratory. market being photovoltaic cells integrated into Physics as an undergraduate In conventional photovoltaics, light is absorbed windows and cladding for buildings. or postgraduate student, or in in the bulk of a slab of semiconducting material any other capacity, we would and the photogenerated charge is collected at metallic electrodes. -
4–9 June 2019
4–9 June 2019 Box Office 01242 850270 cheltenhamfestivals.com #cheltscifest THANK YOU to our Partners and Supporters WELCOME The Cheltenham Science Festival brings together the best scientists, thinkers and In Association with writers. This year we have over 200 events packed into six extraordinary days and, in a year of anniversaries, we are celebrating 50 years since the Apollo moon landing and the Periodic Table’s 150th birthday. In the Festival Village, our new Apollo free stage will feature music, comedy and our international FameLabbers and we’ll have interactive fun for all ages, including the return of the wildly popular GCHQ Cyber Zone and MakerShack. And be on the look out for a big spectacle across town… This year we welcome a new head of programming, Marieke Navin, who is uniquely Principal Partners qualified for the job. She was a participant in the FameLab International competition in 2007 and has been back every year since then as a performer. Add to all this the Science Festival’s best possible advisory group, our fabulous guest curators and the great Festival team and you’ll understand why I have every confidence that this year is going to be the best Science Festival yet. Thanks to them all. And enjoy! Vivienne Parry Chair of Cheltenham Science Festival Major Partners Need help deciding? We’ve picked some events not to miss at this year’s Festival. Best For Wellness Discover the full programme First-Timers from page 16. Woodland Wellness page 17 Strategic Partner Meals Of Tomorrow page 18 Heart Health page 25 LEGO® Lates -
Moduli Stabilisation and the Holographic Swampland
Prepared for submission to JHEP Moduli Stabilisation and the Holographic Swampland Joseph P. Conlon,a Filippo Revelloa aRudolf Peierls Centre for Theoretical Physics Beecroft Building, Clarendon Laboratory, Parks Road, University of Oxford, OX1 3PU, UK E-mail: [email protected], [email protected] Abstract: We investigate whether Swampland constraints on the low-energy dynamics of weakly coupled, moduli-stabilised string vacua in AdS can be related to inconsistencies of their putative holographic duals or, more generally, recast in terms of CFT data. We find that various swampland consistency constraints are equivalent to a negativity condition on the sign of certain mixed anomalous dimensions. This condition is similar to well- established CFT positivity bounds arising from causality and unitarity, but not known to hold in general. The studied scenarios include LVS, KKLT, and both perturbative and racetrack stabilisation. Interestingly, the LVS vacuum (with ∆ϕ = 8.038) also appears to live very close to a critical value (∆ϕ = 8) where the anomalous dimensions change sign. We finally point out an intriguing connection to the Swampland Distance Conjecture, both in its original and refined versions. arXiv:2006.01021v2 [hep-th] 28 Aug 2020 Contents 1 Introduction2 2 The Large Volume Scenario and its Holographic Properties4 2.1 Introduction to LVS and its low energy dynamics4 2.2 CFT interpretation6 2.3 Connection to the Swampland6 3 Holographic CFTs and Consistency Conditions8 3.1 Holographic CFTs8 3.2 The Bootstrap9