Department of Physics Newsletter

Total Page:16

File Type:pdf, Size:1020Kb

Department of Physics Newsletter Summer 2012, Number 2 Department of Physics Newsletter Stargazingn Saturday, 21st Phil Marshall January, passers-by on Banbury Road were met with a remarkable sight:O a queue of people stretching from the door of the Denys Wilkinson Building all the artist MarionOxford... Yorston in the were universally positive, with our and wanted to find out more. way to the bottom of the steps. seminar room, blacked out for visitors excited and inspired by The event was planned as one This was “Stargazing Oxford,” our the occasion), and “AstroCrafts” their time spent inside the Oxford of the local activities associated first ever space science festival. (immensely popular with children Physics Department. with the BBC’s “Stargazing Live” Between 2pm and 10pm, we of all ages). We even borrowed programme, which aired on BBC2 This was really the goal of welcomed nearly 1200 people an inflatable Planetarium from the week before Saturday 21st. “Stargazing Oxford”: to reach out into the Physics Department, to the University of Kent, which The series was excellent – not to people in the local community hear about the latest research proved to be a very popular way only for featuring several Oxford who may not have been to a results in astrophysics and in to space science. It was a long, Physicists! University event before, but who planetary science, and to learn tiring but hugely successful day: were interested in astronomy how to get started observing the the feedback forms we collected Continued on page 2... night sky. The rooftop observing sessions, with Abingdon Astronomical Society, were a big hit. Inside, we put on short research talks in the Dennis Sciama lecture theatre, and filled the cafeteria with village fete-style stalls, manned by research staff wearing red T-shirts marked “got questions?”. We told everyone who was queuing to get in that the DWB was a building full of people whose job it was to ask questions, and so they were to ask us anything they wanted. It seemed to work: one office door in the Beecroft Institute (BIPAC) was covered in questions about space, many of them at the research level despite the childish handwriting! How many solar systems are there? How was the first galaxy made? Wouldn’t we all like to know! Other favourite activites included a N “Universe-ity Challenge” (our own version of the popular BBC eph Carua game show), “Dark Matter” (an S installation by local modern © Jo InsIde: VIrtual stargazIng • predIctIng predIctabIlIty • mappIng FermI surFaces oF Iron-based superconductors • nanotechnology & living cells • a state-oF-the-art www.physics.ox.ac.uk buIldIng For oxFord physIcs • WIll.I.am visIts oxFord • eVents • people • and more outreach neWs scIence neWs www.physics.ox.ac.uk/about-us/outreach www.physics.ox.ac.uk/research Virtual stargazing topological Insulators PRedicting... I’ve been developing methods But these days that’s not enough. discuss the evolution of the Andrew Pontzen Yulin Chen, Rahul Roy for turning computer simulations Static images just don’t cut it cosmos. Having seen a movie I’d and John Chalker Astronomy has a of galaxies into images for a in the age of YouTube. And the made based on a previous paper, Predictability gift: whenever we while, as part of my open source cosmos really is a fairly static place the production commissioned One of the successes want to convince project pynbody (http://pynbody. on human timescales; galaxies a series of videos taking us from of physics in the 1930s people we’re googlecode.com). It’s hugely evolve only over billions of years. the Big Bang through to a present was the use of quantum doing good work with telescopes, important in scientific analysis: This is where us computer nerds day ‘Milky Way’-like galaxy. mechanics to understand the difference between metals and insulators we can turn to a rich archive of whether we want to create a have the edge over observers of Using a portion of Oxford’s Berg in terms of electron energy bands. Remarkably, we have discovered gorgeous imagery. While not a literal analogue to a telescopic the real universe: the process of supercomputer, it was possible to over the past few years that a key feature was missing from the picture substitute for good science, it picture, or a more metaphorical simulation involves calculating generate 10TB of data and distill we’ve accepted for nearly eight decades. This is that insulators come in certainly helps. But for those of representation of the contents and storing the state of the it into about 50,000 separate two types, now known as ‘ordinary’ and ‘topological’. Oxford Physics is us who work on modelling the of our virtual universe, distilling computerised cosmos from images to create the final footage closely involved with these developments: one of the leading theorists universe inside a computer, things millions of numbers into an image its early stages through to the in just over six weeks. in the field, Rahul Roy, spent two years in the Oxford Condensed Matter is a critical step. present day. That means there’s are a little harder. Watching the videos has given Theory group as a postdoctoral research fellow before moving to a nothing to stop you from taking me a whole range of ideas for faculty position at UCLA; and Yulin Chen, an expert in the experimental technique (involving stochastic a picture of it at any stage of its Hannah Arnold new science we can do with these techniques used to probe these new materials, has recently joined the mathematics) for representing development. Or, better, taking simulations. We’re inherently Department from Stanford. the small scales in an a whole series of pictures at You want to go visual creatures; nothing atmospheric model, providing subsequent steps. To jazz it up, to the beach at compares to seeing things unfold a physically motivated way of you can start moving the virtual the weekend: in front of our eyes. While you’ve representing model uncertainty. telescope through space. And, which of the missed the chance to see it on live We have found the forecasts before you know it, you have a following do you think is the TV, there’s a digested version here: made using this technique are Hollywood-style movie of how more useful weather forecast: a) http://youtu.be/77zoF7y1pnk. very reliable; if you look at all galaxies form and evolve – but all next weekend will be dry; or b) the occasions when we have based on real physics. next weekend the probability of rain is just 10%? Both are forecast a 10% chance of rain, on Last November, luck sent the possible ways of presenting the average it rains 10% of the time. production team of BBC2’s Follow the same forecast, though only the This is very important for climate Stargazing Live in my direction. astrophysics blog! second acknowledges that our change prediction, where we are They were looking for ways to interested in how the statistics read about our research, and prediction about next weekend’s see our weekly “What’s up?” weather involves uncertainty. of the weather will change due Surface conduction of topological insulators: (A) The spin of electrons to anthropogenic forcing. We Left: The distribution of dark matter column for what to look out for on the surface is correlated with their direction of motion. (B) The There are two main sources must be confident that our over tens of millions of light years in the night sky. lattice structure of Bi Te and the predicted relativistic “Dirac cone” like of uncertainty in our weather during the formation of galaxies. 2 3 model accurately represents http://facebook.com/ electronic structure formed by the surface electrons. (C) The electronic forecast, both of which must today’s climate in order to trust OxfordAstrophysics structure measured by angle-resolved photoemission that confirmed be accurately represented. the climate it predicts for the the theoretical prediction and the topological nature of Bi Te . stargazing oxford 2 3 The first is initial condition future. uncertainty. The atmosphere Continued from page 1... is a chaotic system, so errors In the atmosphere, it has Rahul Roy writes: Imagine taking a block of wood and coating its been found that certain surfaces with silver. Then the block would be a bulk insulator with in the starting conditions for our forecast (i.e. errors in the weather patterns are very Inspired viewers could then look on the BBC “Things to do” website, a metallic conducting surface. A ‘topological insulator’ is similar to measurements we make of the predictable – the errors due and find out about Stargazing Oxford. We thought we might get a coated block, but whereas cutting the wood block would create weather today) can lead to large to initial condition and model quite a lot of interest, but the response was amazing: not many of us new insulating surfaces, cutting a topological insulator creates new deviations in the predicted uncertainty stay small as we had imagined people queuing for 45 minutes in the cold to get into conducting surfaces. My work uses the mathematics of topological weather for the weekend. The look to the future. However, on our building! For us, Stargazing Oxford was incredibly exciting, and invariants to predict that certain insulating materials will have surface second is model uncertainty. other occasions, including these also quite humbling: the public’s delighted fascination with space modes for electrons, which are robust because they are protected In order to make the forecast, representations of uncertainty science made a big impression on us all.
Recommended publications
  • Non-Thermal Behavior in Conformal Boundary States
    Prepared for submission to JHEP Non-Thermal Behavior in Conformal Boundary States Kevin Kuns and Donald Marolf Department of Physics, University of California, Santa Barbara, CA 93106, U.S.A. E-mail: [email protected], [email protected] Abstract: Cardy has recently observed that certain carefully tuned states of 1+1 CFTs on a timelike strip are periodic with period set by the light-crossing time. The states in question are defined by Euclidean time evolution of conformal boundary states associated with the particular boundary conditions imposed on the edges of the strip. We explain this behavior, and the associated lack of thermalization, by showing that such states are Lorentz-signature conformal transformations of the strip ground state. Taking the long- strip limit implies that states used to model thermalization on the Minkowski plane admit non-thermal conformal extensions beyond future infinity of the Minkowski plane, and thus retain some notion of non-thermal behavior at late times. We also comment on the holo- graphic description of these states. arXiv:1406.4926v2 [cond-mat.stat-mech] 6 Oct 2014 Contents 1 Introduction1 2 Periodicity and Tuned Rectangle States2 2.1 Tuned Rectangle States from Conformal Transformations2 2.2 One-Point Functions5 3 Conformal Transformations to the Thermal Minkowski Plane9 4 Discussion 12 A Holographic Description 13 1 Introduction The rapid change in a quantum system from a Hamiltonian H0 to a Hamiltonian H is known as a quantum quench. Quantum quenches are of experimental interest since they can be studied in laboratory systems involving ultracold atoms. They are also of theoretical interest as examples of out of equilibrium quantum systems whose thermalization, or lack thereof, can be used as a first step towards understanding thermalization in more general quantum systems.
    [Show full text]
  • Lectures and Seminars, Trinity Term 2015
    WEDNESDay 22 april 2015 • SUpplEMENT (2) TO NO 5092 • VOl 145 Gazette Supplement Lectures and Seminars, Trinity term 2015 Romanes Lecture 462 Experimental psychology Buddhist Studies Orthopaedics, rheumatology and COMPAS Musculoskeletal Sciences Hebrew and Jewish Studies University Administration pathology Hindu Studies and Services 462 pharmacology Museum of the History of Science Disability Lecture physiology, anatomy and Genetics islamic Studies population Health reuters institute for the Study of Humanities 462 psychiatry Journalism Foundation for law, Justice and Society TOrCH | The Oxford research Centre in Social Sciences 470 the Humanities learning institute Maison Française rothermere american institute interdisciplinary research Methods Oxford Martin School Classics Sanjaya lall Memorial Trust population ageing English language and literature anthropology and Museum Ethnography ian ramsey Centre History Saïd Business School linguistics, philology and phonetics Economics Colleges, Halls and Societies 482 Medieval and Modern languages Education Music interdisciplinary area Studies all Souls Oriental Studies international Development (Queen Balliol philosophy Elizabeth House) Green Templeton Theology and religion Oxford internet institute Keble Law lady Margaret Hall Mathematical, Physical and politics and international relations linacre Life Sciences 466 Social policy and intervention lincoln Socio-legal Studies Chemistry Magdalen Sociology Computer Science Mansfield Nuffield Earth Sciences Department for Continuing Queen’s Engineering
    [Show full text]
  • A First Law of Entanglement Rates from Holography
    A First Law of Entanglement Rates from Holography Andy O'Bannon,1, ∗ Jonas Probst,2, y Ronnie Rodgers,1, z and Christoph F. Uhlemann3, 4, x 1STAG Research Centre, Physics and Astronomy, University of Southampton, Highfield, Southampton SO17 1BJ, U. K. 2Rudolf Peierls Centre for Theoretical Physics, University of Oxford, 1 Keble Road, Oxford OX1 3NP, U. K. 3Department of Physics, University of Washington, Seattle, WA 98195-1560, USA 4Mani L. Bhaumik Institute for Theoretical Physics, Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA For a perturbation of the state of a Conformal Field Theory (CFT), the response of the entanglement entropy is governed by the so-called “first law" of entanglement entropy, in which the change in entanglement entropy is proportional to the change in energy. Whether such a first law holds for other types of perturbations, such as a change to the CFT La- grangian, remains an open question. We use holography to study the evolution in time t of entanglement entropy for a CFT driven by a t-linear source for a conserved U(1) current or marginal scalar operator. We find that although the usual first law of entanglement entropy may be violated, a first law for the rates of change of entanglement entropy and energy still holds. More generally, we prove that this first law for rates holds in holography for any asymptotically (d + 1)-dimensional Anti-de Sitter metric perturbation whose t dependence first appears at order zd in the Fefferman-Graham expansion about the boundary at z = 0.
    [Show full text]
  • Reading in Fall 2003'S Inside Physics
    FFromrom thethe ChairChair available in the fall of 2001. Visits elcome to the first edition of our by prospective students nearly newsletter, created to keep us in doubled the number for the newsletter, created to keep us in previous year, and 33 new Wclose touch with our alumni and graduate students appeared in the friends. We’d like to hear your reaction: fall of 2001. We were especially friends. We’d like to hear your reaction: pleased that 30% of the entering what’s satisfying, what’s not, what’s class were women. I hope this is missing. Please let us know. no “fluke” and that we continue missing. Please let us know. to increase the participation of women in physics. The applica- tions for the fall of 2002 number Jim Allen over 500 and we look forward to Department Chair enrolling another strong class. OUR FUTURE Three new faculty joined our als. And Walter himself, the EXCITING TIMES ranks: Crystal Martin, an observa- founding director of the Institute “You can dismiss one Nobel Prize tional astrophysicist from Caltech; for Theoretical Physics, received as a statistical fluke,” Walter Kohn David Stuart, a high energy the 1998 prize in chemistry. remarked, “but a spate of three experimental physicist from Fermi signals something important and Lab; and Dik Bouwmeester from exciting happening at UCSB.” ENDOWED CHAIR Oxford, who works on quantum We are delighted that a chair in The three Nobels reflect UCSB’s optics and experimental quantum experimental physics has been longstanding commitment to information science. We continue endowed by Bruce and Susan excellence in science and engi- to search for new faculty in Worster.
    [Show full text]
  • Quantum Quenches: a Probe of Many-Body Quantum Mechanics
    Tata Institute of Fundamental Research Hyderabad Colloquium John Cardy University of California, Berkeley Professor John Cardy is well known for his application of quantum field theory and the renormalization group to condensed matter, especially to critical phenomena in both pure and disordered equilibrium and non-equilibrium systems. In the 1980s he helped develop the theory of conformal invariance and its applications to these problems, ideas which also had an impact in string theory and the physics of black holes. In the 1990s he used conformal invariance to derive many exact results in percolation and related probabilistic problems. More recently Professor Cardy has worked on questions of quantum entanglement and non-equilibrium dynamics in many-body systems. He is a Fellow of the Royal Society, a recipient of the 2000 Dirac Medal of the Institute of Physics, of the 2004 Lars Onsager Prize of the American Physical Society, of the 2010 Boltzmann Medal of the International Union of Pure and Applied Physics, and of the 2011 Dirac Medal and Prize of the International Centre for Theoretical Physics. Professor Cardy has a long-standing association with TIFR, and visited our Mumbai campus in 2007-08 as the Homi Bhabha Chair Professor. Quantum Quenches: a probe of many-body quantum mechanics In a quantum quench, a system is prepared in some state (typically the ground state of an initial hamiltonian) and then evolved coherently with a different hamiltonian, e.g. by instantaneously changing a parameter. Such protocols in many-body systems have recently become experimentally achievable with ultracold atoms. I shall discuss some of the theoretical approaches to this problem, and in particular discuss whether, and in what sense, such systems thermalize.
    [Show full text]
  • Beyond the Boson Graphene's 3D Counterparts Superconductivity
    Autumn 2014, Number 5 Department of Physics Newsletter Beyond the boson The next steps for particle physics Superconductivity: Strike while the iron is hot Oxford researchers synthesise new iron based high temperature superconductor Graphene’s 3D counterparts Oxford researchers have discovered a new series of materials that are a 3D version of graphene ALUMNI STORIES EVENTS MOSELEY & X-RAYS PEOPLE Jean Chu (Holmes) reflects Alumni day at the Clarendon Part II of Prof Derek Stacey’s Five minutes with David Lloyd; on life as a female physics Laboratory; Bonn in Oxford; remarkable story celebrating Comings, Goings and Awards student at St Hugh’s, 1956–59 Alumni experience the LHC Henry Moseley’s work www.physics.ox.ac.uk SCIENCE NEWS SCIENCE NEWS www.physics.ox.ac.uk/research www.physics.ox.ac.uk/research in research labs, to steering oxides were shown to exhibit superconductivity the beams around particle at temperatures well above 100 Kelvin (a accelerators (such as the phenomenon which is still far from understood). SUPERCONDUCTIVITY: Large Hadron Collider at CERN) and confining the EXPLORING NEW PHYSICS STRIKE WHILE THE IRON IS HOT plasma in a fusion reactor. But perhaps their most Here in Oxford our current focus is on the newly important application has A little over a century after the discovery of quantum coherent state, a concept also applicable to discovered materials that contain iron. Some been in magnetic resonance superconductivity we are still missing some vital superfluids and Bose-Einstein condensates of cold of these have transition temperatures above imaging (MRI), the clues in understanding how and why the effect atoms.
    [Show full text]
  • Parliamentary Debates (Hansard)
    Thursday Volume 566 18 July 2013 No. 39 HOUSE OF COMMONS OFFICIAL REPORT PARLIAMENTARY DEBATES (HANSARD) Thursday 18 July 2013 £5·00 © Parliamentary Copyright House of Commons 2013 This publication may be reproduced under the terms of the Open Parliament licence, which is published at www.parliament.uk/site-information/copyright/. 1295 18 JULY 2013 1296 Vince Cable: The hon. Gentleman is correct to say House of Commons that our overall export performance would improve considerably if more British companies were exporting. The big contrast with Germany is that roughly twice as Thursday 18 July 2013 many of its small and medium-sized enterprises are involved in exporting. UKTI has been substantially The House met at half-past Nine o’clock reformed in the past couple of years, and it now has a much more small and medium-sized company focus. It has activities around the country, and we have a lot of PRAYERS evidence that its outreach is substantially improving. I hope that it will reach the companies in the hon. Gentleman’s constituency too. [MR SPEAKER in the Chair] Mr Iain Wright (Hartlepool) (Lab): At the last Business, Innovation and Skills questions, the Secretary of State Oral Answers to Questions admitted: “The figures on exports are not great”.—[Official Report, 13 June 2013; Vol. 564, c. 470.] Since then, the UK trade deficit has widened to the BUSINESS, INNOVATION AND SKILLS point at which it is now the largest trade gap in the European Union, and the widest it has been since 1989. Following on from the question from my hon.
    [Show full text]
  • Extracting Cosmology from High Resolution CMB Data *Focused on ACT and SO
    Extracting cosmology from high resolution CMB data *focused on ACT and SO Jo Dunkley, Princeton University May 23, 2018 Jo Dunkley Cosmic Microwave Background T=2.7K ∆T/T ~0.00001 Also polarization: Rep.Two-point statistics: Prog. Phys. 81 (2018) 044901 Report on Progress TxT TxE BxB ExE Staggs, JD, Page 2018 review Figure 3. Example of recent CMB power spectra from [50–54]. Left. TT (top) and EE (bottom) data and power spectra plotted with logarithmic y axes. The TT and EE oscillations are out of phase by ∼π/2 as expected for acoustic oscillations (see section 1.4) since TT and EE trace density and velocity, respectively. The TT spectrum at low ℓ, corresponding to superhorizon scales at decoupling (see section 2.1), has post-decoupling contributions from gravitational redshifting of the photons as they pass through evolving potential wells, known as the integrated Sachs-Wolfe (ISW) effect [55, 56]. The EE spectrum peaks at higher ℓ than TT both because it lacks the ISW effect, and because the acoustic oscillation velocity gradients sourcing the polarization grow with k and thus with ℓ. The spectra are suppressed at large ℓ due to photon diffusion from smaller regions of space, also called Silk damping [57], and to geometric effects from compressing the 3d structure to 2d spectra. Right. TE with linear y axis. Since the ISW effect does not change the polarization, the negative peak at ℓ = 150 in TE confrmed that some of the largest scale features in the CMB are primordial, and not just late-time effects [58–60].
    [Show full text]
  • Neutrino Cosmology and Large Scale Structure
    Neutrino cosmology and large scale structure Christiane Stefanie Lorenz Pembroke College and Sub-Department of Astrophysics University of Oxford A thesis submitted for the degree of Doctor of Philosophy Trinity 2019 Neutrino cosmology and large scale structure Christiane Stefanie Lorenz Pembroke College and Sub-Department of Astrophysics University of Oxford A thesis submitted for the degree of Doctor of Philosophy Trinity 2019 The topic of this thesis is neutrino cosmology and large scale structure. First, we introduce the concepts needed for the presentation in the following chapters. We describe the role that neutrinos play in particle physics and cosmology, and the current status of the field. We also explain the cosmological observations that are commonly used to measure properties of neutrino particles. Next, we present studies of the model-dependence of cosmological neutrino mass constraints. In particular, we focus on two phenomenological parameterisations of time-varying dark energy (early dark energy and barotropic dark energy) that can exhibit degeneracies with the cosmic neutrino background over extended periods of cosmic time. We show how the combination of multiple probes across cosmic time can help to distinguish between the two components. Moreover, we discuss how neutrino mass constraints can change when neutrino masses are generated late in the Universe, and how current tensions between low- and high-redshift cosmological data might be affected from this. Then we discuss whether lensing magnification and other relativistic effects that affect the galaxy distribution contain additional information about dark energy and neutrino parameters, and how much parameter constraints can be biased when these effects are neglected.
    [Show full text]
  • Review of the Year 2009/10
    Invest in future scientific leaders and in innovation Review of the year 2009/10 1 Celebrating 350 years Review of the year 2009/10 02 Review of the year 2009/10 President’s foreword Executive Secretary’s report Review of the year 2009/10 03 Contents President’s foreword ..............................................................02 Inspire an interest in the joy, wonder Executive Secretary’s report ..................................................03 and excitement of scientific discovery ..................................16 Invest in future scientific leaders and in innovation ..............04 Seeing further: the Royal Society celebrates 350 years .......20 Influence policymaking with the best scientific advice ........08 Summarised financial statements .........................................22 Invigorate science and mathematics education ...................10 Income and expenditure statement ......................................23 Increase access to the best science internationally ..............12 Fundraising and support ........................................................24 List of donors ..........................................................................25 President’s Executive foreword Secretary’s report This year we have focused on the excellent This has been a remarkable year for the Society, our opportunity afforded by our 350th anniversary 350th, and we have mounted a major programme not only to promote the work of the Society to inspire minds, young and old alike, with the but to raise the profile of science
    [Show full text]
  • Parliamentary Debates House of Commons Official Report General Committees
    PARLIAMENTARY DEBATES HOUSE OF COMMONS OFFICIAL REPORT GENERAL COMMITTEES Public Bill Committee ENTERPRISE AND REGULATORY REFORM BILL Third Sitting Thursday 21 June 2012 CONTENTS Written evidence reported to the House. Examination of witnesses. Adjourned till Tuesday 26 June at half-past ten o’clock. PUBLISHED BY AUTHORITY OF THE HOUSE OF COMMONS LONDON – THE STATIONERY OFFICE LIMITED £5·00 PBC (Bill 007) 2012 - 2013 Members who wish to have copies of the Official Report of Proceedings in General Committees sent to them are requested to give notice to that effect at the Vote Office. No proofs can be supplied. Corrigenda slips may be published with Bound Volume editions. Corrigenda that Members suggest should be clearly marked in a copy of the report—not telephoned—and must be received in the Editor’s Room, House of Commons, not later than Monday 25 June 2012 STRICT ADHERENCE TO THIS ARRANGEMENT WILL GREATLY FACILITATE THE PROMPT PUBLICATION OF THE BOUND VOLUMES OF PROCEEDINGS IN GENERAL COMMITTEES © Parliamentary Copyright House of Commons 2012 This publication may be reproduced under the terms of the Parliamentary Click-Use Licence, available online through The National Archives website at www.nationalarchives.gov.uk/information-management/our-services/parliamentary-licence-information.htm Enquiries to The National Archives, Kew, Richmond, Surrey TW9 4DU; e-mail: [email protected] Public Bill Committee21 JUNE 2012 Enterprise and Regulatory Reform Bill The Committee consisted of the following Members: Chairs: HUGH BAYLEY,†MR
    [Show full text]
  • Parliamentary Debates (Hansard)
    Monday Volume 552 5 November 2012 No. 63 HOUSE OF COMMONS OFFICIAL REPORT PARLIAMENTARY DEBATES (HANSARD) Monday 5 November 2012 £5·00 © Parliamentary Copyright House of Commons 2012 This publication may be reproduced under the terms of the Open Parliament licence, which is published at www.parliament.uk/site-information/copyright/. 571 5 NOVEMBER 2012 572 compensation. Does my hon. Friend agree that the House of Commons position is unfair and should be reviewed by HMRC? Monday 5 November 2012 Steve Webb: I am grateful to my hon. Friend for raising that case. I have corresponded with Treasury The House met at half-past Two o’clock colleagues about the issue, and, subject to their consent, I shall be happy to share with him the reply that I have PRAYERS just received. [MR SPEAKER in the Chair] Disability Strategy 2. Stuart Andrew (Pudsey) (Con): What progress he Oral Answers to Questions has made on the Government’s disability strategy. [126299] WORK AND PENSIONS The Parliamentary Under-Secretary of State for Work and Pensions (Esther McVey): Fulfilling Potential, our The Secretary of State was asked— disability strategy, is being co-produced with disabled people. We published “Fulfilling Potential—The Discussions UK Pension-holders So Far” and “Fulfilling Potential—Next Steps” on 17 September. Our key themes, which we intend to 1. Dan Jarvis (Barnsley Central) (Lab): What steps he make a real difference, are early intervention, choice is taking to ensure that foreign conglomerates carry out and control, and inclusive communities. their responsibilities to UK pension-holders. [126298] The Minister of State, Department for Work and Stuart Andrew: Can the Minister explain what the Pensions (Steve Webb): As this is the first session of role of the disabled people’s user-led organisations will DWP questions since the announcement of the untimely be in the strategy? death of Malcolm Wicks, I hope that you will allow me, Mr.
    [Show full text]