Autumn Department of Physics Newsletter Issue
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TRAPPING a STAR in a MAGNETIC DOUGHNUT the Physics of Magnetic Confinement Fusion
Spring 2016, Number 8 Department of Physics Newsletter TRAPPING A STAR IN A MAGNETIC DOUGHNUT The physics of magnetic confinement fusion RATTLING DARK MATTER THE CAGE: IN OUR GALAXY Making new superconductors Novel dynamics is bringing the Galaxy's and gravitational waves: using lasers dark matter into much sharper focus a personal reaction ALUMNI STORIES EVENTS PEOPLE Richard JL Senior and Elspeth Garman Remembering Dick Dalitz; Oxford Five minutes with Geoff Stanley; reflect on their experiences celebrates Nobel Prize; Physics Challenge Awards and Prizes Day and many more events www.physics.ox.ac.uk SCIENCE NEWS SCIENCE NEWS www.physics.ox.ac.uk/research www.physics.ox.ac.uk/research Prof James Binney FRS Right: Figure 2. The red arrows show the direction of the Galaxy’s gravitational field by our current DARK MATTER reckoning. The blue lines show the direction the field would have if the disc were massless. The mass © JOHN CAIRNS JOHN © IN OUR GALAXY of the disc tips the field direction In the Rudolf Peierls Centre for Theoretical Physics novel dynamics is towards the equatorial plane. A more massive disc would tip it bringing the Galaxy's dark matter into much sharper focus further. Far right: Figure 3. The orbits in In 1937 Fritz Zwicky pointed out that in clusters of clouds of hydrogen to large distances from the centre of the R plane of two stars that both galaxies like that shown in Fig. 1, galaxies move much NGC 3198. The data showed that gas clouds moved on z move past the Sun with a speed of faster than was consistent with estimates of the masses perfectly circular orbits at a speed that was essentially 72 km s−1. -
Full TIPP 2011 Program Book
Second International Conference on Technology and Instrumentation in Particle Physics June 9-14, 2011 Program & Abstracts Sheraton Chicago Hotel and Towers, Chicago IL ii TIPP 2011 — June 9-14, 2011 Table of Contents Acknowledgements .................................................................................................................................... v Session Conveners ...................................................................................................................................vii Session Chairs .......................................................................................................................................... ix Agenda ....................................................................................................................................................... 1 Abstracts .................................................................................................................................................. 35 Poster Abstracts ..................................................................................................................................... 197 Abstract Index ........................................................................................................................................ 231 Poster Index ........................................................................................................................................... 247 Author List ............................................................................................................................................. -
How and Why Silicon Sensors Are Becoming More and More Intelligent?
How and why silicon sensors are becoming more and more intelligent? Daniela Bortolettoa a Physics Department, University of Oxford Keble Road, Oxford, UK E-mail: [email protected] ABSTRACT: This paper describes the historical evolution of silicon detectors from simple strip configurations to hybrid pixel detectors for high energy physics applications. This development has been critical to maintain the necessary physics performance in the high-rate and high- density environment of the LHC. The importance of pixel detectors and their evolution for future projects and other fields is also described. KEYWORDS: Si microstrip and pixel detectors Contents 1. Introduction 1 2. Strip Sensors 2 3. Pixel Sensors 5 3.1 Hybrid pixel 6 3.2 Hybrid pixel for X-ray detection 8 4. Fully depleted Thick CCD 8 5. New Directions 9 6. Acknowledgments 10 1. Introduction Silicon is the dominant semiconductor material used in the production of position sensitive detectors for particle physics. The moderate band gap between the conduction and the valence band of 1.12 eV is large compared to the thermal energy at room temperature of 25.9 meV. Therefore cooling is necessary only in ultra-low noise applications or when required to mitigate radiation damage. The detection of minimum ionizing particles (MIP) is based on ionisation or excitation of atoms in the medium caused by the passage of charged particles. The energy required to create an electron-hole (e-h) pair is 3.6 eV yielding an ionization of about 80 e- h/µm. Thus silicon detector can be quite thin compared with gaseous detectors. -
Dansk Matematisk Forening Mat-Nyt Calendar
DANSK MATEMATISK FORENING MAT-NYT CALENDAR This document is a hard copy of all entries in the electronic Mat-Nyt calendar of the Danish Mathematical Society covering the period 2004-1-1 – 2004-2-1. Produced Thu Jan 5, 2006 1 MAT-NYT The Danish National Research Foundation Network in Mathematical Physics and Stochastics Mathematical Physics Seminar A Hamiltonian model for linear friction Stephan de Bievre, Villeneuve d’Ascq, France Mon Jan 19 2004, 14:15 - 15:15 Abstract I will present a Hamiltonian model of a particle coupled to a suitable wave field, describing the particle’s environment, in which a simple version of Ohm’s law is valid. When an external force is applied, the particle reaches asymptotically a constant speed proportional to the applied field. I will review the related literature, compare this phenomenon to the one of radiative dissipation, and indicate some of the many open problems Organized by MPS Editor 2004-01-16 13:44:36 ( [email protected] / [email protected] ) 2 MAT-NYT INSTITUT FOR MATEMATISKE FAG MATEMATISK AFDELING KØBENHAVNS UNIVERSITET ALGEBRA SEMINAR The Inverse problem in Gr¨obner basis theory Amelia Taylor, Assistant Professor, St. Olaf College USA Mon Jan 19 2004, 15:15 Abstract Given an ideal in a polynomial ring its initial ideal is easy to compute and is well studied using Gr¨obner basis theory. However, given a monomial ideal what can we say about the types of ideals it is the initial ideal for, that is do we know anything about the inverse problem for Gr¨obner basis theory? This question as stated is currently considered to be too broad, however progress has been made in determining when a monomial ideal is the initial ideal of a prime ideal and in most of the known cases we can we construct the prime ideal. -
Advanced Multi-Variate Analysis Methods for New Physics Searches at the Large Hadron Collider
Advanced Multi-Variate Analysis Methods for New Physics Searches at the Large Hadron Collider Anna Stakiaa, Tommaso Dorigob, Giovanni Banellic, Daniela Bortolettod, Alessandro Casae, Pablo de Castrob,p, Christophe Delaeref, Julien Doninig, Livio Finosh, Michele Gallinaroi, Andrea Giammancof, Alexander Heldj, Fabricio Jim´enezMoralesk, Grzegorz Kotkowskil, Seng Pei Liewc, Fabio Maltonif, Giovanna Menardil, Ioanna Papavergoum, Alessia Saggion, Bruno Scarpao, Giles C. Strongb,p, Cecilia Tosciriq, Jo~aoVarelai, Pietro Vischiaf, Andreas Weilerc aInstitute of Nuclear and Particle Physics, National Centre for Scientific Research `Demokritos', Athens, Greece bIstituto Nazionale di Fisica Nucleare, Sezione di Padova, Italy cPhysics Department, Technical University of Munich, Garching, Germany dDepartment of Physics, University of Oxford, UK eSchool of Mathematics and Statistics, University College Dublin, Ireland fCentre for Cosmology, Particle Physics and Phenomenology (CP3), Universit´ecatholique de Louvain, Louvain-la-Neuve, Belgium gLaboratoire de Physique de Clermont, Universit´eClermont Auvergne, IN2P3/CNRS, Clermont-Ferrand, France hDepartment of Developmental Psychology and Socialization, University of Padova, Italy iLaborat´oriode Instrumenta¸c~aoe F´ısica Experimental de Part´ıculas,LIP Lisbon, Portugal jNew York University, USA kLaboratoire Leprince-Ringuet, CNRS, Ecole´ polytechnique, Institut Polytechnique de Paris, Palaiseau, France. lDepartment of Statistical Sciences, University of Padova, Italy mNational and Kapodistrian University -
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. -
Oxfordcolleges
Oxford colleges Oxford University is made up of different colleges. Colleges are academic communities. They are where students usually have their tutorials. Each one has its own dining hall, bar, common room and library, and lots of college groups and societies. If you study here you will be a member of a college, and probably have your tutorials in that college. You will also be a member of the wider University, with access to University and department facilities like laboratories and libraries, as well as hundreds of University groups and societies. You would usually have your lectures and any lab work in your department, with other students from across the University. There is something to be said for an academic atmosphere wherein everyone you meet is both passionate about what they are studying and phenomenally clever to boot. Ziad 144| Does it matter which college I go to? What is a JCR? No. Colleges have a lot more in common than Junior Common Room, or JCR, means two they have differences. Whichever college you go different things. Firstly, it is a room in college: to, you will be studying for the same degree at the a lively, sociable place where you can take time end of your course. out, eat, watch television, play pool or table football, and catch up with friends. The term Can I choose my college? JCR also refers to all the undergraduates in a college. The JCR elects a committee which Yes, you can express a preference. When you organises parties, video evenings and other apply through UCAS (see ‘how to apply’ on p 6) events, and also concerns itself with the serious you can choose a college, or you can make an side of student welfare, including academic ‘open application’. -
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 -
RSE Fellows Ordered by Area of Expertise As at 11/10/2016
RSE Fellows ordered by Area of Expertise as at 11/10/2016 HRH Prince Charles The Prince of Wales KG KT GCB Hon FRSE HRH The Duke of Edinburgh KG KT OM, GBE Hon FRSE HRH The Princess Royal KG KT GCVO, HonFRSE A1 Biomedical and Cognitive Sciences 2014 Professor Judith Elizabeth Allen FRSE, FMedSci, Professor of Immunobiology, University of Manchester. 1998 Dr Ferenc Andras Antoni FRSE, Honorary Fellow, Centre for Integrative Physiology, University of Edinburgh. 1993 Sir John Peebles Arbuthnott MRIA, PPRSE, FMedSci, Former Principal and Vice-Chancellor, University of Strathclyde. Member, Food Standards Agency, Scotland; Chair, NHS Greater Glasgow and Clyde. 2010 Professor Andrew Howard Baker FRSE, FMedSci, BHF Professor of Translational Cardiovascular Sciences, University of Glasgow. 1986 Professor Joseph Cyril Barbenel FRSE, Former Professor, Department of Electronic and Electrical Engineering, University of Strathclyde. 2013 Professor Michael Peter Barrett FRSE, Professor of Biochemical Parasitology, University of Glasgow. 2005 Professor Dame Sue Black DBE, FRSE, Director, Centre for Anatomy and Human Identification, University of Dundee. ; Director, Centre for Anatomy and Human Identification, University of Dundee. 2007 Professor Nuala Ann Booth FRSE, Former Emeritus Professor of Molecular Haemostasis and Thrombosis, University of Aberdeen. 2001 Professor Peter Boyle CorrFRSE, FMedSci, Former Director, International Agency for Research on Cancer, Lyon. 1991 Professor Sir Alasdair Muir Breckenridge CBE KB FRSE, FMedSci, Emeritus Professor of Clinical Pharmacology, University of Liverpool. 2007 Professor Peter James Brophy FRSE, FMedSci, Professor of Anatomy, University of Edinburgh. Director, Centre for Neuroregeneration, University of Edinburgh. 2013 Professor Gordon Douglas Brown FRSE, FMedSci, Professor of Immunology, University of Aberdeen. 2012 Professor Verity Joy Brown FRSE, Provost of St Leonard's College, University of St Andrews. -
The Oxford Particle Physics Program
The Oxford Particle Physics Program D. Bortoletto 30.11.2016 Graduate Opportunities 1 Oxford is addressing the science drivers of particle physics Higgs as a new tool for Identify the new discovery physics of dark matter The physics of Explore the unknown: new particles and new interactions Understanding cosmic Neutrino mass acceleration 2 Outline • Particle Physics Groups @ Oxford addresses these drivers through: – ATLAS Experiment – LHCb Experiment – Neutrino Experiments – Dark Matter Searches – Many detector based projects – For full list, look here: http://www2.physics.ox.ac.uk/study- here/postgraduates/particle-physics/thesis-topics 3 The Standard Model • 1964 SM Theory • 1984 LHC Design • 1996 Start LHC construction • 2009: first collisions 2013 4 Why look beyond the Standard Model? § Experimental Evidence § Non-baryonic dark matter (~23%) § Inferred from gravitational effects § Rotational speed of galaxies § Orbital velocities of galaxies in clusters § Gravitational lensing § ….. § Dark Energy (~73%) § Accelerated Expansion of the Universe § Neutrinos have mass and mix § Baryon asymmetry § ….. 5 Why look beyond the Standard Model? § Experimental Evidence § Non-baryonic dark matter (~23%) § Inferred from gravitational effects § Rotational speed of galaxies § Orbital velocities of galaxies in clusters § Gravitational lensing § ….. § Dark Energy (~73%) § Accelerated Expansion of the Universe § Neutrinos have mass and mix § Baryon asymmetry § ….. 6 Why look beyond the Standard Model? § Aesthetic/Theoretical Reasons § Hierarchy problem -
Exoplanets: Where the Wild Things Are
Autumn 2016, Number 9 Department of Physics Newsletter EXOPLANETS: WHERE THE WILD THINGS ARE MAGNETISM ORDERS EXOTIC FERMIONS THE LHC IN 2016: SOME ANSWERS, MORE QUESTIONS IOP NAMES OXFORD PHYSICS DEPARTMENT A GENDER EQUALITY CHAMPION ALUMNI STORIES EVENTS PEOPLE Christopher Roberts, Pembroke 1949, ‘New eyes on the universe’ exhibit; Five minutes with Dillon Liu; Letters reflects on his experiences Alumni reception at Canada House, to the editor; Awards and Prizes London; From Oxford to Mars! www.physics.ox.ac.uk SCIENCE NEWS SCIENCE NEWS www.physics.ox.ac.uk/research www.physics.ox.ac.uk/research Prof Ray Pierrehumbert, When it is possible to improvements in spectroscopic instrumentation made into a tight mass estimate. With this, in conjunction Halley Professor of observe a system with the implementation of the programme possible. The first with the size data from the transit depth, you know the Physics exoplanets were discovered by this method, known as density of the planet – and therefore something about EXOPLANETS: both the transit and RV the Radial Velocity (RV) method. The RV method gives what it is made of. Even without RV observations, transit method, then as a planet the period of a planet’s orbit, and using undergraduate- observations of systems with multiple planets (and there WHERE THE WILD THINGS ARE hunter you’ve really hit level Newtonian mechanics one can then determine are many such systems known) can provide mass and the distance of the planet from its star. Astrophysical density estimates through a technique called Transit the jackpot, since the two techniques tell us the power output (luminosity) of the Time Variation (TTV). -
Fellowships: Round Two Sift Panel Membership*
Fellowships: Round Two Sift Panel Membership* Panel Chairs Gordon Harold, University of Sussex Angela Hatton, National Oceanography Centre Susan Hunston, University of Birmingham Jonathan Legh-Smith, BT Group PLC Barbara Mable, University of Glasgow Julie Yeomans, University of Surrey Panel Members John Challiss, University of Leicester Sophia Ananiadou, The University of Jonathan Chubb, University College London Manchester Alison Condliffe, University of Sheffield Erika Andersson, Heriot-Watt University Paul Connolly, Queens University Belfast Jane Armitage, University of Oxford Jenny Cooper, CooperWalsh Ltd Marco Bacic, Rolls-Royce & Oxford John Couves, BP University Elaine Crooks, Swansea University Liz Baggs, University of Edinburgh James Davenport, University of Bath Susan Banducci, University of Exeter Simin Davoudi, Newcastle University Wendy Barclay, Imperial College Ineke De Moortel, University of St Andrews London John Barrett, University of David Demeritt, Kings College London Leeds Joe Devine, University of Bath Daniela Barilla, University of York Peter Diggle, Lancaster Steven Bell, Queens University Belfast University/Health Data Research UK Malcolm Bennett, University of Declan Diver, University of Glasgow Nottingham Nick Dun, Lancaster University Steve Benford, University of Alastair Edge, Durham University Nottingham Jonathan Elliot, University of London Lisa Belyea, Queen Mary University of Georgina Endfield, University of Liverpool London Alison Fell, University of Leeds Matthew Bennett, Bournemouth Teresa Fernandes,