3,203 research outputs found

    The local innovation system of the oil and gas industry in the North Sea : the application of patent data in the study of innovation systems

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    Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Nuclear Science and Engineering, 2008.Cataloged from PDF version of thesis.Includes bibliographical references (p. 177-179).The North Sea oil province, one of the world's major centers of petroleum and natural gas production, has been in play for four decades. Production rates have approached their peaks in recent years and are expected to decline continuously in the future. The economies of certain cities and regions bordering on the North Sea have become heavily dependent on the oil and gas industry. How these local economies will sustain themselves in the future as resource depletion continues is a critical question. To gain insight into this question, we selected a matched pair of city-regions, each of which is an important center of the oil and gas industry in the North Sea province: Aberdeen in Scotland and Stavanger in Norway. By studying the similarities and differences between the local innovation systems in the two regions, we can gain a general understanding of how local economies respond to changes in their environment. U.S. patenting data are used as a tool to describe the behavior and performance of the two local innovation systems. The patent data provide a means of systematically and consistently estimating knowledge flows. The use of U.S. patent and patent citation data provides evidence, references, and guidelines to the project from a quantitative perspective. Several indicators were developed to describe these knowledge flows, along with a model providing further insight into how knowledge was acquired and introduced into the two local innovation systems, how and to what extent local innovation capabilities were developed, and how knowledge created locally has spread elsewhere.(cont.) Both Stavanger and Aberdeen have worked hard to strengthen their local innovation capabilities by learning from the world's most advanced firms, especially those from the U.S.,and by building capabilities of their own. At the same time, attracted by the extensive reserves of oil and gas, multinational firms, many from the U.S., moved into the North Sea region. The involvement of multinational firms helped reinforce local innovation capabilities. However, because of the different policy approaches pursued in the two regions, U.S. firms, the international leaders in oil and gas technology, have played more important roles in Aberdeen than in Stavanger. In the Stavanger area, local innovation activities have been led by national oil companies rather than by foreign firms.by Wei Gao.Ph.D

    Convective-core overshooting and the final fate of massive stars

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    Massive stars can explode in powerful supernovae (SNe) forming neutron stars but they may also collapse directly into black holes (BHs). Understanding and predicting their final fate is increasingly important, e.g, in the context of gravitational-wave astronomy. The interior mixing of stars in general and convective boundary mixing remain some of the largest uncertainties in their evolution. Here, we investigate the influence of convective boundary mixing on the pre-SN structure and explosion properties of massive stars. Using the 1D stellar evolution code Mesa, we model single, non-rotating stars of solar metallicity with initial masses of 5−70M⊙5-70\mathrm{M_\odot} and convective core step-overshooting of 0.05−0.50HP0.05-0.50H_\mathrm{P}. Stars are evolved until the onset of iron core collapse, and the pre-SN models are exploded using a parametric, semi-analytic SN code. We use the compactness parameter to describe the interior structure of stars at core collapse. Larger convective core overshooting shifts the location of the compactness peak by 1−2M⊙1-2\mathrm{M_\odot} to higher MCOM_\mathrm{CO}. As the luminosity of the pre-SN progenitor is determined by MCOM_\mathrm{CO}, we predict BH formation for progenitors with luminosities 5.35<log⁡(L/L⊙)<5.505.35<\log(L/\mathrm{L_\odot})<5.50 and log⁡(L/L⊙)>5.80\log(L/\mathrm{L_\odot})>5.80. The luminosity range of BH formation agrees well with the observed luminosity of the red supergiant star N6946BH1 that disappeared without a bright SN and likely collapsed into a BH. While some of our models in the luminosity range log⁡(L/L⊙)=5.1−5.5\log(L/\mathrm{L_\odot})=5.1-5.5 indeed collapse to form BHs, this does not fully explain the lack of observed SN~IIP progenitors at these luminosities, ie the missing red-supergiant problem. Convective core overshooting affects the BH masses, the pre-SN location of stars in the Hertzsprung-Russell diagram, the plateau luminosity and duration of SN~IIP lightcurves.[Abridged]Comment: Accepted for publication in Astronomy & Astrophysics: 23 pages, 14 figure

    Evolution of Iron Kα_{\alpha} Line Emission in the Black Hole Candidate GX 339-4

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    GX 339-4 was regularly monitored with RXTE during a period (in 1999) when its X-ray flux decreased significantly (from 4.2×10−10\times 10^{-10} erg cm−2s−1^{-2} s^{-1} to 7.6×10−12\times 10^{-12} erg cm−2^{-2}s−1^{-1} in the 3--20 keV band), as the source settled into the ``off state''. Our spectral analysis revealed the presence of a prominent iron Kα_{\alpha} line in the observed spectrum of the source for all observations. The line shows an interesting evolution: it is centered at ∌\sim6.4 keV when the measured flux is above 5×10−11\times 10^{-11} erg cm−2s−1^{-2} s^{-1}, but is shifted to ∌\sim6.7 keV at lower fluxes. The equivalent width of the line appears to increase significantly toward lower fluxes, although it is likely to be sensitive to calibration uncertainties. While the fluorescent emission of neutral or mildly ionized iron atoms in the accretion disk can perhaps account for the 6.4 keV line, as is often invoked for black hole candidates, it seems difficult to understand the 6.7 keV line with this mechanism, because the disk should be less ionized at lower fluxes (unless its density changes drastically). On the other hand, the 6.7 keV line might be due to recombination cascade of hydrogen or helium like iron ions in an optically thin, highly ionized plasma. We discuss the results in the context of proposed accretion models.Comment: 18 pages, 2 figures, accepted for publication in the ApJ in v552n2p May 10, 2001 issu

    Pairing Symmetry in Iron-Pnictide Superconductor KFe2_2As2_2

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    The pairing symmetry is one of the major issues in the study of iron-based superconductors. We adopt a low-energy effective kinetic model based on the first-principles band structure calculations combined with the J1J_1-J2J_2 model for KFe2_2As2_2, the phase diagram of pairing symmetries is constructed. Putting the values of J1J_1 and J2J_2 of the J1J_1-J2J_2 model obtained by the first-principles calculations into this phase diagram, we find that the pairing symmetry for KFe2_2As2_2 is a nodal dxyd_{xy}-wave in the folded Brillouin zone with two iron atoms per unit cell. This is in good agreement with experiments observed a nodal order parameter.Comment: 5 pages, 4 figures (The pairing symmetry is dependent on choosing an effective tight-binding model. In the publication version, we adopt a ten-orbital model by using the maximally localized Wannier functions based on the first-principles band structure calculations, and give an s-wave pairing for KFe2_2As2_2

    A new critical curve for the Lane-Emden system

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    We study stable positive radially symmetric solutions for the Lane-Emden system −Δu=vp-\Delta u=v^p in RN\R^N, −Δv=uq-\Delta v=u^q in RN\R^N, where p,q≄1p,q\geq 1. We obtain a new critical curve that optimally describes the existence of such solutions.Comment: 13 pages, 1 figur
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