11,990 research outputs found
Attachment system for silica tiles
An improved method for markedly increasing the bond strength between a rigid, porous refractory material and non-rigid substrate by densifying the face of the rigid material opposing the substrate is discussed. Densification is accomplished by wetting the refractory material and then impregnating it with a composite slurry having a particle size to fill voids of the porous material
Reduced regulator dependence of neutron-matter predictions with chiral interactions
We calculate the energy per particle in infinite neutron matter
perturbatively using chiral N3LO two-body potentials plus N2LO three-body
forces. The cutoff dependence of the predictions is investigated by employing
chiral interactions with different regulators. We find that the inclusion of
three-nucleon forces, which are consistent with the applied two-nucleon
interaction, leads to a strongly reduced regulator dependence of the results.Comment: 7 pages, 8 figures, 1 table, to be published in Physical Review
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Organization, atmosphere, and digital technologies: designing sensory order
We argue technology and organization are inherently spatial phenomenon. We conceptualize this conjunction as atmosphere: a gathering of mood, human practice, material and environmental conditions, and values that has sufficient coherence and distinction to constitute a distinct interior. Atmospheres, however, are not entirely stable and present: the interior is porous to outside influence, and the interior is never wholly ordered. We show this through the study of digitally mediated architectural design practice. We find the technological mediation of atmospheres is constituted in sensory and affective spatial arrangements, and not in rationally calculated configurations of assets and goals. An atmosphere is inherently aesthetic. This allows us to gesture toward a definition of organization as technologically mediated spatial struggle to reconcile interior coherence with outward exposure
The nuclear matter equation of state with consistent two- and three-body perturbative chiral interactions
We compute the energy per particle of infinite symmetric nuclear matter from
chiral N3LO (next-to-next-to-next-to-leading order) two-body potentials plus
N2LO three-body forces. The low-energy constants of the chiral three-nucleon
force that cannot be constrained by two-body observables are fitted to
reproduce the triton binding energy and the 3H-3He Gamow-Teller transition
matrix element. In this way, the saturation properties of nuclear matter are
reproduced in a parameter-free approach. The equation of state is computed up
to third order in many-body perturbation theory, with special emphasis on the
role of the third-order particle-hole diagram. The dependence of these results
on the cutoff scale and regulator function is studied. We find that the
inclusion of three-nucleon forces consistent with the applied two-nucleon
interaction leads to a reduced dependence on the choice of the regulator only
for lower values of the cutoff.Comment: 9 pages, 12 figures, 3 tables, to be published in Physical Review C.
arXiv admin note: text overlap with arXiv:1209.553
Chiral nucleon-nucleon forces in nuclear structure calculations
Realistic nuclear potentials, derived within chiral perturbation theory, are
a major breakthrough in modern nuclear structure theory, since they provide a
direct link between nuclear physics and its underlying theory, namely the QCD.
As a matter of fact, chiral potentials are tailored on the low-energy regime of
nuclear structure physics, and chiral perturbation theory provides on the same
footing two-nucleon forces as well as many-body ones. This feature fits well
with modern advances in ab-initio methods and realistic shell-model. Here, we
will review recent nuclear structure calculations, based on realistic chiral
potentials, for both finite nuclei and infinite nuclear matter.Comment: 10 pages, 8 figures, plenary talk presented at "Nucleus-Nucleus 2015"
Conference, 21-26 June 2015, Catania, to be published in the "Conference
Proceedings" Series of the Italian Physical Societ
Smart Materials as Intelligent Insulation
In order to provide a robust infrastructure for the transmission and distribution of electrical power, understanding and monitoring equipment ageing and failure is of paramount importance. Commonly, failure is associated with degradation of the dielectric material; therefore the introduction of a smart moiety into the material is a potentially attractive means of continual condition monitoring. It is important that any introduction of smart groups into the dielectric does not have any detrimental effect on the desirable electrical and mechanical properties of the bulk material. Initial work focussed on the introduction of fluorophores into a model dielectric system. Fluorescence is known to be a visible effect even at very low concentrations of active fluorophores and therefore was thought well suited to such an application. It was necessary both to optimise the active fluorophore itself and to determine the most appropriate manner in which to introduce the fluorophores into the insulating system. This presentation will describe the effect of introducing fluorophores into polymeric systems on the dielectric properties of the material and the findings thus far [1]. Alternative smart material systems will also be discussed along with the benefits and limitations of smart materials as electric field sensors
Dominant Nuclear Outflow Driving Mechanisms in Powerful Radio Galaxies
In order to identify the dominant nuclear outflow mechanisms in Active
Galactic Nuclei, we have undertaken deep, high resolution observations of two
compact radio sources (PKS 1549-79 and PKS 1345+12) with the Advanced Camera
for Surveys (ACS) aboard the Hubble Space Telescope. Not only are these targets
known to have powerful emission line outflows, but they also contain all the
potential drivers for the outflows: relativistic jets, quasar nuclei and
starbursts. ACS allows the compact nature (<0.15") of these radio sources to be
optically resolved for the first time. Through comparison with existing radio
maps we have seen consistency in the nuclear position angles of both the
optical emission line and radio data. There is no evidence for bi-conical
emission line features on the large-scale and there is a divergance in the
relative position angles of the optical and radio structure. This enables us to
exclude starburst driven outflows. However, we are unable to clearly
distinguish between radiative AGN wind driven outflows and outflows powered by
relativistic radio jets. The small scale bi-conical features, indicative of
such mechanisms could be below the resolution limit of ACS, especially if
aligned close to the line of sight. In addition, there may be offsets between
the radio and optical nuclei induced by heavy dust obscuration, nebular
continuum or scattered light from the AGN.Comment: 9 pages, 8 figures, emulateapj, ApJ Accepte
Beam and Torsion Tests of Aluminum-alloy 61S-T Tubing
Tests were made to determine the effect of length and the effect of ratios of diameter to wall thickness upon the flexural and torsional moduli of failure of 61S-T aluminum-alloy tubing. The moduli of failure in bending, as determined by tests in which the tubing was loaded on the neutral axis at the one-third points of the span, were found to bear an approximately linear relationship with diameter-thickness ratio and were practically independent of span within the limits investigated. Empirical equations are given describing the relations obtained. The moduli of failure in torsion were found to be dependent upon length as well as upon diameter-thickness ratios. Empirical equations are given for predicting strengths within the range of plastic buckling. Within the elastic range, available torsion theories were found to be satisfactory
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