8,980 research outputs found
Mechanisms of nonstoichiometry in HfN<sub>1-<i>x</i></sub>
Density functional theory is used to calculate defect structures that can accommodate nonstoichiometry in hafnium nitride: HfN1-x, 0 ≤ X ≤ 0.25. It is predicted that a mechanism assuming simple distributions of nitrogen vacancies can accurately describe the variation in the experimentally observed lattice parameter with respect to the nitrogen nonstoichiometry. Although the lattice parameter changes are remarkably small across the whole nonstoichiometry range, the variations in the bulk modulus are much greater
Production and Marketing Characteristics of U.S. Pork Producers, 2006
Livestock Production/Industries, Marketing,
Models and Strategies for Variants of the Job Shop Scheduling Problem
Recently, a variety of constraint programming and Boolean satisfiability
approaches to scheduling problems have been introduced. They have in common the
use of relatively simple propagation mechanisms and an adaptive way to focus on
the most constrained part of the problem. In some cases, these methods compare
favorably to more classical constraint programming methods relying on
propagation algorithms for global unary or cumulative resource constraints and
dedicated search heuristics. In particular, we described an approach that
combines restarting, with a generic adaptive heuristic and solution guided
branching on a simple model based on a decomposition of disjunctive
constraints. In this paper, we introduce an adaptation of this technique for an
important subclass of job shop scheduling problems (JSPs), where the objective
function involves minimization of earliness/tardiness costs. We further show
that our technique can be improved by adding domain specific information for
one variant of the JSP (involving time lag constraints). In particular we
introduce a dedicated greedy heuristic, and an improved model for the case
where the maximal time lag is 0 (also referred to as no-wait JSPs).Comment: Principles and Practice of Constraint Programming - CP 2011, Perugia
: Italy (2011
Enhancing efficiency of single, large-aperture antennas
Numerical analysis method provides means of describing energy distribution in focal plane of parabolic surface in terms of phase and wavelength. Two approaches for enhancing antenna efficiency include single, large reflector focused to feeding element, and array of smaller apertures whose individual outputs are summed
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Oxygen diffusion in Sr<sub>0.75</sub>Y<sub>0.25</sub>CoO<sub>2.625</sub>: a molecular dynamics study
Oxygen diffusion in Sr0.75Y0.25CoO2.625 is investigated using molecular dynamics simulations in conjunction with an established set of Born model potentials. We predict an activation energy of diffusion for 1.56 eV in the temperature range of 1000-1400 K. We observe extensive disordering of the oxygen ions over a subset of lattice sites. Furthermore, oxygen ion diffusion both in the a-b plane and along the c axis requires the same set of rate-limiting ion hops. It is predicted that oxygen transport in Sr0.75Y0.25CoO2.625 is therefore isotropic
A Chandra X-ray Investigation of the Violent Interstellar Medium: From Dwarf Starbursts to Ultraluminous Infrared Galaxies
We have analyzed observations with the Chandra X-ray Observatory of the
diffuse emission by hot gas in 7 dwarf starburst galaxies, 6 edge-on starburst
galaxies, and 9 Ultra Luminous Infrared Galaxies. These systems cover ranges of
\~ 10^4 in X-ray luminosity and several thousand in star formation rate and
K-band luminosity (a proxy for stellar mass). Despite this range in fundamental
parameters, we find that the properties of the diffuse X-ray emission are very
similar in all three classes of starburst galaxies. The spectrum of the diffuse
emission is well fit by thermal emission from gas with kT ~ 0.25 to 0.8 keV and
with several-times-solar abundance ratios of alpha elements to Fe. The ratio of
the thermal X-ray to far-infrared luminosity is roughly constant, as is the
characteristic surface brightness of the diffuse X-ray emission. The size of
the diffuse X-ray source increases systematically with both far-infrared and
K-Band luminosity. All three classes show strong morphological relationships
between the regions of hot gas probed by the diffuse X-ray emission and the
warm gas probed by optical line emission. These findings suggest that the same
physical mechanism is producing the diffuse X-ray emission in the three types
of starbursts, and are consistent with that mechanism being shocks driven by a
galactic "superwind'' powered by the kinetic energy collectively supplied by
stellar winds and supernovae in the starburst.Comment: 37 pages, 13 figure
Population Growth and Other Statistics of Middle-sized Irish Towns. General Research Series Paper No. 85, April 1976
The basic aim of the study is the presentation of tables of comparative
statistical data relating to 97 towns with population 5OO-1O,OOO in
1971 and analyses of such data. The exclusion of the four County Boroughs
and Dun Laoghaire together with twelve other large towns and all small
towns and villages, was to impart a degree of homogeneity to the inquiry, as
regards function of town. The 97 towns range from Mullingar, the largest
with a population of 9,245 to Cootehill with 1,542
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