266 research outputs found

    Advanced Fabrication Processes for Superconducting Very Large Scale Integrated Circuits

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    We review the salient features of two advanced nodes of an 8-Nb-layer fully planarized process developed recently at MIT Lincoln Laboratory for fabricating Single Flux Quantum(SFQ) digital circuits with very large scale integration on 200-mm wafers: the SFQ4ee and SFQ5ee nodes, where 'ee' denotes the process is tuned for energy efficient SFQ circuits. The former has eight superconducting layers with 0.5 {\mu}m minimum feature size and a 2 {\Omega}/sq Mo layer for circuit resistors. The latter has nine superconducting layers: eight Nb wiring layers with the minimum feature size of 350 nm and a thin superconducting MoNx layer (Tc ~ 7.5 K) with high kinetic inductance (about 8 pH/sq) for forming compact inductors. A nonsuperconducting (Tc < 2 K) MoNx layer with lower nitrogen content is used for 6 {\Omega}/sq planar resistors for shunting and biasing of Josephson junctions. Another resistive layer is added to form interlayer, sandwich-type resistors of m{\Omega} range for releasing unwanted flux quanta from superconducting loops of logic cells. Both process nodes use Au/Pt/Ti contact metallization for chip packaging. The technology utilizes one layer of Nb/AlOx-Al/Nb JJs with critical current density, Jc of 100 {\mu}A/{\mu}m^2 and minimum diameter of 700 nm. Circuit patterns are defined by 248-nm photolithography and high density plasma etching. All circuit layers are fully planarized using chemical mechanical planarization (CMP) of SiO2 interlayer dielectric. The following results and topics are presented and discussed: the effect of surface topography under the JJs on the their properties and repeatability, critical current and Jc targeting, effect of hydrogen dissolved in Nb, MoNx properties for the resistor layer and for high kinetic inductance layer, technology of m{\Omega}-range resistors.Comment: 10 pages, 12 figures, 1 table, 27 references. The paper was presented on September 8, 2015 at the 12th European Conference on Applied Superconductivity, EUCAS 2015, 6-10 September 2015, Lyon, France, IEEE Transaction on Applied Superconductivity, 201

    ‘Can you dig it?’ Developing an approach to validly assessing diverse skills in an archaeological context

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    This paper outlines a case study of an assessment development process which contrasts with more recent ‘top-down’ trends in assessment which tend to leave assessment development processes opaque to users. This paper describes the processes of a collaborative, multi-agency project which set out to develop an assessment framework which would appropriately recognise the various skills present in the Higher Education Field Academy; a widening participation programme aiming to boost the educational aspirations, enthusiasm and attainment of secondary school students through their engagement in archaeological excavation. The case study describes the stages of building an assessment framework that was sympathetic to the intentions of a learning programme whilst providing robust observation-based outcomes that avoided heavy assessment processes that could corrupt learning relationships. The challenges involved in this development process have important parallels with vocational assessment; not least in providing an example of a localised development of an observation-based assessment model which can be used in diverse settings. The insights gained from this case study are useful for others who are engaged in localised assessment development processes

    The use of routine outcome measures in two child and adolescent mental health services: a completed audit cycle

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    Background: Routine outcome measurement (ROM) is important for assessing the clinical effectiveness of health services and for monitoring patient outcomes. Within Child and Adolescent Mental Health Services (CAMHS) in the UK the adoption of ROM in CAMHS has been supported by both national and local initiatives (such as government strategies, local commissioning policy, and research). Methods: With the aim of assessing how these policies and initiatives may have influenced the uptake of ROM within two different CAMHS we report the findings of two case-note audits: a baseline audit conducted in January 2011 and a re-audit conducted two years later in December 2012-February 2013. Results: The findings show an increase in both the single and repeated use of outcome measures from the time of the original audit, with repeated use (baseline and follow-up) of the Health of the Nation Outcome Scale for Children and Adolescents (HoNOSCA) scale increasing from 10% to 50% of cases. Re-audited case-notes contained more combined use of different outcome measures, with greater consensus on which measures to use. Outcome measures that were applicable across a wide range of clinical conditions were more likely to be used than symptom-specific measures, and measures that were completed by the clinician were found more often than measures completed by the service user. Conclusions: The findings show a substantial improvement in the use of outcome measures within CAMHS. These increases in use were found across different service organisations which were subject to different types of local service priorities and drivers

    Gamma-Ray Emission Concurrent with the Nova in the Symbiotic Binary V407 Cygni

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    Novae are thermonuclear explosions on a white dwarf surface fueled by mass accreted from a companion star. Current physical models posit that shocked expanding gas from the nova shell can produce X-ray emission but emission at higher energies has not been widely expected. Here, we report the Fermi Large Area Telescope detection of variable gamma-ray (0.1-10 GeV) emission from the recently-detected optical nova of the symbiotic star V407 Cygni. We propose that the material of the nova shell interacts with the dense ambient medium of the red giant primary, and that particles can be accelerated effectively to produce pi0 decay gamma-rays from proton-proton interactions. Emission involving inverse Compton scattering of the red giant radiation is also considered and is not ruled out.Comment: 38 pages, includes Supplementary Online Material; corresponding authors: C.C. Cheung, A.B. Hill, P. Jean, S. Razzaque, K.S. Woo

    Swift and Fermi observations of the early afterglow of the short Gamma-Ray Burst 090510

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    We present the observations of GRB090510 performed by the Fermi Gamma-Ray Space Telescope and the Swift observatory. This is a bright, short burst that shows an extended emission detected in the GeV range. Furthermore, its optical emission initially rises, a feature so far observed only in long bursts, while the X-ray flux shows an initial shallow decrease, followed by a steeper decay. This exceptional behavior enables us to investigate the physical properties of the GRB outflow, poorly known in short bursts. We discuss internal shock and external shock models for the broadband energy emission of this object.Comment: Comments: Submitted to ApJ Letters. Contact Authors: Massimiliano De Pasquale ([email protected]), Mathew Page ([email protected]), Kenji Toma ([email protected]), Veronique Pelassa ([email protected]). Minor change in the authorlis

    Electromagnetic Wave Theory and Applications

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    Contains table of contents for Section 3, reports on four research projects and a list of publications.National Aeronautics and Space Administration Grant NAGW-1617National Aeronautics and Space Administration Agreement 958461National Aeronautics and Space Administration Grant NAGW-1272U.S. Army Corp of Engineers Contract DACA39-87-K-0022U.S. Navy - Office of Naval Research Grant N00014-89-J-1107U.S. Navy - Office of Naval Research Grant N00014-92-J-1616Digital Equipment CorporationJoint Services Electronics Program Contract DAAL03-92-C-0001U.S. Navy - Office of Naval Research Grant N00014-90-J-1002U.S. Navy - Office of Naval Research Grant N00014-89-J-1019U.S. Department of Transportation Agreement DTRS-57-88-C-00078TTD13U.S. Department of Transportation Agreement DTRS-57-88-C-00078TTD30U.S. Department of Transportation Agreement DTRS-57-92-C-00054TTD1DARPA/Consortium for Superconducting Electronics Contract MDA972-90-C-0021National Science Foundation Fellowship MIP 88-5876

    Pairwise maximum entropy models for studying large biological systems: when they can and when they can't work

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    One of the most critical problems we face in the study of biological systems is building accurate statistical descriptions of them. This problem has been particularly challenging because biological systems typically contain large numbers of interacting elements, which precludes the use of standard brute force approaches. Recently, though, several groups have reported that there may be an alternate strategy. The reports show that reliable statistical models can be built without knowledge of all the interactions in a system; instead, pairwise interactions can suffice. These findings, however, are based on the analysis of small subsystems. Here we ask whether the observations will generalize to systems of realistic size, that is, whether pairwise models will provide reliable descriptions of true biological systems. Our results show that, in most cases, they will not. The reason is that there is a crossover in the predictive power of pairwise models: If the size of the subsystem is below the crossover point, then the results have no predictive power for large systems. If the size is above the crossover point, the results do have predictive power. This work thus provides a general framework for determining the extent to which pairwise models can be used to predict the behavior of whole biological systems. Applied to neural data, the size of most systems studied so far is below the crossover point
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