On the performance of strain smoothing for quadratic and enriched finite element approximations (XFEM/GFEM/PUFEM)

By using the strain smoothing technique proposed by Chen et al. (Comput. Mech. 2000; 25: 137-156) for meshless methods in the context of the finite element method (FEM), Liu et al. (Comput. Mech. 2007; 39(6): 859-877) developed the Smoothed FEM (SFEM). Although the SFEM is not yet well understood mathematically, numerical experiments point to potentially useful features of this particularly simple modification of the FEM. To date, the SFEM has only been investigated for bilinear and Wachspress approximations and is limited to linear reproducing conditions. The goal of this paper is to extend the strain smoothing to higher order elements and to investigate numerically in which condition strain smoothing is beneficial to accuracy and convergence of enriched finite element approximations. We focus on three widely used enrichment schemes, namely: (a) weak discontinuities; (b) strong discontinuities; (c) near-tip linear elastic fracture mechanics functions. The main conclusion is that strain smoothing in enriched approximation is only beneficial when the enrichment functions are polynomial (cases (a) and (b)), but that non-polynomial enrichment of type (c) lead to inferior methods compared to the standard enriched FEM (e.g. XFEM). Copyright (C) 2011 John Wiley & Sons, Ltd.

Do controle social à gestão participativa: perspectivas (pós soberanas) da participação política no SUS

Este trabalho parte da hipótese de que discutir a participação política no SUS exige a problematização das opções e concepções que orientam sua definição como controle social, operacionalizado por meio de mecanismos de representação de interesses. A intenção de promover uma reflexão sobre a participação política no SUS pé remetida ao cotidiano institucional, como desafio de construção de modos de gestão participativos. A proposta metodológica baseis-se em uma abordagem filosófica, que tem por objetivo delinear os conceitos e dispositivos de gestão propostos no campo da Saúde Coletiva, as inovações teóricas que ofertam ao debate sobre a gestão em saúde, tendo por marcador o tema da política. Denominamos matrizes conceituais os dois planos filosófico que selecionamos para estudo no campo da Saúde Coletiva, a saber, o Planejamento em Saúde e o Modelo Assistencial em Defesa da Vida. O conceito de Política que adotamos se define não em termos de igualdade (formal) que se contrapões às diferenças (sociais), mas como coprodução de realidade que se concretiza nas relações entre Igualdade e Diferença, como acesso e uso dos bens-comuns, em sua capacidade indeterminada e aberta de criação de valor. Pensar a participação nestes termos significa tecer participações como possibilidade de instituir normas, e não apenas com controle da execução e fiscalização das normas existentes. Nessa concepção propõe-se pensar a gestão como coprodução de saúde, a partir da publicização e articulação reticular da dimensão normativa da atividade humana, o que implica questionar a produção concreta (portanto local) das políticas e intervenções públicas. Dentre as principais questões teóricas discutidas, destacamos a articulação de redes de cooperação e a construção de saberes, artifícios técnicos e dispositivos que viabilizem a produção e legitimação do valor-Saúde como bem comum. Perspectiva que explicita as implicações que desejamos incorporar ao conceito de gestão participativa, como possível tecnologia de governo pós-soberana. A participação na saúde é pensada, deste modo, a partir do problema de constituição de uma política pública que consiga permanecer aberta e imprevisível, resguardando, contudo, condições materiais de igualdade. Nesse sentido, uma política pública que rompa com os mecanismos da soberania moderna ao incorporar em seus desenhos institucionais a imprevisibilidade da produção normativa, forjando-se como dispositivo ético (portanto aberto e comum) de produção de valor.

Interference effects in the extraction of trace metals from estuarine waters

We have found that a commonly used complexation and solvent extraction technique (using mixed dithiocarbamates/Freon/HNO3) does not always extract Cd, Co, Cu and Ni from estuarine samples with the same efficiency as from Milli-Q water. For samples collected from the Derwent Estuary (Australia), the reduced extraction efficiency only occurred for unfiltered samples, but low extraction efficiencies were also observed for a (filtered) riverine certified reference material (SLRS-3) suggesting that the effect may be widespread. We have not been able to identify the reason for the low extraction efficiency and, although it is strongly correlated with the presence of high concentrations of suspended solids, dissolved organic matter and particulate iron, we have no experimental evidence to directly link any of these parameters to the effect. It is possible that similar effects may occur in other techniques which rely on a preconcentration step prior to analysis and that some literature values of heavy metals in estuarine waters may be low. We propose a modification of the standard complexation/solvent extraction method which overcomes these difficulties without adding significantly to the time taken for analyses.

A novel breast tissue density classification framework

Oliver, A., Freixenet, J., Marti, R., Pont, J., Perez, E., Denton, E. R. E., Zwiggelaar, R. (2008). A novel breast tissue density classification framework. IEEE Transactions on Information Technology in BioMedicine, 12 (1), 55-65

The forage supply service in the Chaco native forest : an approach to economic analysis

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The forage supply service in the Chaco native forest : an approach to economic analysis

p.37-45

Analysis of the footprint in school age of 8-10 years old

Biomechanical problems in children, is an important subject currently, existing controversy in different areas, for example, the majority of children have a flattened footprint, or the hypermobility joint is linked to a musculoskeletal pain. The objective of the study was to determine what kind of footprint is most frequent in school-age children (8-10 years) in the area of Plasencia. This was taken as a sign 50 children, of whom 28 were males and 22 females. All the subjects in the study underwent an assessment of footprint planted in static as well as an exploration of different parameters through inspection in a standing position (formula digital, rearfoot). The results show that excavated footprint is present in a 72% cases of the population, 16% was belonging to an excavated footprint in which we find a higher percentage of weight related.For the digital formula we find that the most common is the Egyptian foot by 40% of the cases and that the prevalence in the rearfoot, is a normal hindfoot. In relation with the hypermobility joint, we check that it is more common in girls and that none of them presents an association to musculoskeletal pain. As a future line we could establish a more comprehensive study with new techniques and valuingchild’s statics and dynamics, to have a more accurate study of the different variables in the sample population studied.

WASP-1b and WASP-2b: Two new transiting exoplanets detected with SuperWASP and SOPHIE

We have detected low-amplitude radial-velocity variations in two stars, USNO-B1.0 1219-0005465 (GSC 02265-00107 = WASP-1) and USNO-B1.0 0964-0543604 (GSC 00522-01199 = WASP-2). Both stars were identified as being likely host stars of transiting exoplanets in the 2004 SuperWASP wide-field transit survey. Using the newly commissioned radial-velocity spectrograph SOPHIE at the Observatoire de Haute-Provence, we found that both objects exhibit reflex orbital radial-velocity variations with amplitudes characteristic of planetary-mass companions and in-phase with the photometric orbits. Line-bisector studies rule out faint blended binaries as the cause of either the radial-velocity variations or the transits. We perform preliminary spectral analyses of the host stars, which together with their radial-velocity variations and fits to the transit light curves yield estimates of the planetary masses and radii. WASP-1b and WASP-2b have orbital periods of 2.52 and 2.15 d, respectively. Given mass estimates for their F7V and K1V primaries, we derive planet masses 0.80-0.98 and 0.81-0.95 times that of Jupiter, respectively. WASP-1b appears to have an inflated radius of at least 1.33 RJup, whereas WASP-2b has a radius in the range 0.65-1.26 RJup.

Alternative financing instruments for Spanish cooperative

The search for funding is an ongoing task of the company, which is exacerbated, particularly in times of economic crisis, affecting also to the cooperatives. Cooperative legislation available to these entities various instruments of external financing through the issuance of securities (bonds, equity securities, special shares), to them accounts are added in participation, but without much detail in the legal texts. At work we investigate their potential, by looking, especially in those last; We seek to clarify their legal status and contrast their potential as a technical instrument, alternative for funding in the area of cooperative societies. Finally, we also see the impact of the recent Law 5/2015, of promoting business financing in the cooperative sector and ended up proposing some policy adjustments.

WASP-3b: a strongly irradiated transiting gas-giant planet

We report the discovery of WASP-3b, the third transiting exoplanet to be discovered by the WASP and SOPHIE collaboration. WASP-3b transits its host star USNO-B1.01256-0285133 every 1.846834 +/- 0.000002 d. Our high-precision radial velocity measurements present a variation with amplitude characteristic of a planetary-mass companion and in phase with the light curve. Adaptive optics imaging shows no evidence for nearby stellar companions, and line-bisector analysis excludes faint, unresolved binarity and stellar activity as the cause of the radial velocity variations. We make a preliminary spectroscopic analysis of the host star and find it to have Teff = 6400 +/- 100K and log g = 4.25 +/- 0.05 which suggests it is most likely an unevolved main-sequence star of spectral type F7-8V. Our simultaneous modelling of the transit photometry and reflex motion of the host leads us to derive a mass of 1.76+0.08-0.14 MJ and radius 1.31+0.07-0.14 RJ for WASP-3b. The proximity and relative temperature of the host star suggests that WASP-3b is one of the hottest exoplanets known, and thus has the potential to place stringent constraints on exoplanet atmospheric models.

WASP-4b: A 12th magnitude transiting hot Jupiter in the southern hemisphere

We report the discovery of WASP-4b, a large transiting gas-giant planet with an orbital period of 1.34 days. This is the first planet to be discovered by the SuperWASP-South observatory and CORALIE collaboration and the first planet orbiting a star brighter than 16th magnitude to be discovered in the southern hemisphere. A simultaneous fit to high-quality light curves and precision radial velocity measurements leads to a planetary mass of 1.22(-0.08)(+0.09) M-Jup and a planetary radius of 1.42(-0.04)(+0.07) R-Jup. The host star is USNO-B1.0 0479-0948995, a G7 V star of visual magnitude 12.5. As a result of the short orbital period, the predicted surface temperature of the planet is 1761 K, making it an ideal candidate for detections of the secondary eclipse at infrared wavelengths.

WASP-14b: 7.3 M-J transiting planet in an eccentric orbit

We report the discovery of a 7.3 M-J exoplanet WASP-14b, one of the most massive transiting exoplanets observed to date. The planet orbits the 10th-magnitude F5V star USNO-B1 11118-0262485 with a period of 2.243 752 d and orbital eccentricity e = 0.09. A simultaneous fit of the transit light curve and radial velocity measurements yields a planetary mass of 7.3 +/- 0.5 M-J and a radius of 1.28 +/- 0.08 R-J. This leads to a mean density of about 4.6 g cm(-3) making it the densest transiting exoplanets yet found at an orbital period less than 3 d. We estimate this system to be at a distance of 160 +/- 20 pc. Spectral analysis of the host star reveals a temperature of 6475 +/- 100 K, log g = 4.07 cm s(-2) and v sin i = 4.9 +/- 1.0 km s(-1), and also a high lithium abundance, log N(Li) = 2.84 +/- 0.05. The stellar density, effective temperature and rotation rate suggest an age for the system of about 0.5-1.0 Gyr.

WASP-10b: a 3M(J), gas-giant planet transiting a late-type K star

We report the discovery of WASP-10b, a new transiting extrasolar planet (ESP) discovered by the Wide Angle Search for Planets ( WASP) Consortium and confirmed using Nordic Optical Telescope FIbre-fed Echelle Spectrograph and SOPHIE radial velocity data. A 3.09-d period, 29 mmag transit depth and 2.36 h duration are derived for WASP-10b using WASP and high-precision photometric observations. Simultaneous fitting to the photometric and radial velocity data using a Markov Chain Monte Carlo procedure leads to a planet radius of 1.28R(J), a mass of 2.96M(J) and eccentricity of approximate to 0.06. WASP-10b is one of the more massive transiting ESPs, and we compare its characteristics to the current sample of transiting ESP, where there is currently little information for masses greater than approximate to 2M(J) and non-zero eccentricities. WASP-10's host star, GSC 2752-00114 (USNO-B1.0 1214-0586164) is among the fainter stars in the WASP sample, with V = 12.7 and a spectral type of K5. This result shows promise for future late-type dwarf star surveys.

Enseignement moral et enseignement de l'éthique : analyse des ruptures et des continuités dans les programmes d'étude québécois au primiare et au secondaire depuis 1977

La discussion des résultats expose ce qui s'avère être des éléments de continuité majeurs transversaux. Ces huit éléments de continuité majeurs, soit finalement les résultats principaux de notre recherche, se détaillent ainsi: (1) Le développement de l'individu est au coeur des préoccupations de tous les programmes; (2) Les relations interpersonnelles sont toujours travaillées; (3) Bien qu'on touche des savoirs davantage théoriques, ce sont surtout des aptitudes et des habiletés qu'on désire développer en morale et en éthique; (4) L'évaluation formative est prédominante sur l'évaluation sommative, bien que celle-ci soit également utilisée; (5) Les valeurs et les normes composent une partie du contenu de tous les programmes; (6) Le développement du jugement (moral, éthique, critique) est une constante; (7) On s'attend à ce que l'élève soit actif dans le développement de son jugement; (8) L'enseignant a plusieurs rôles, les plus importants étant d'être un motivateur, une personne ressource et un modèle. Parce qu'ils marquent une cassure certaine entre l'enseignement de l'éthique et l'enseignement de la morale, certains éléments de rupture retiennent également l'attention : (1) La place et le rôle de la religion; (2) La question du positionnement. En conclusion, cette recherche théorique permet de faire le pont entre l'enseignement moral et l'enseignement de l'éthique, exposant entre autres ce qui peut être transféré du premier vers le second.

Statistique de photons d’une jonction tunnel déduite de mesures de potentiel électrique à l’aide d’un amplificateur paramétrique Josephson

On présente dans ce mémoire la mesure de la statistique de photons des fluctuations électromagnétiques micro-ondes d’une jonction tunnel placée à ultra-basse température. En particulier, on déduit cettedite statistique en mesurant les cumulants des fluctuations de courant générées par une jonction tunnel polarisée en courant continu et photoexcitée par un signal haute fréquence. On utilise un amplificateur paramétrique Josephson en tant que premier maillon de la chaîne d’amplification en raison de son bruit près de la limite quantique. On développe aussi un modèle pour tenir compte de sa saturation, celle-ci étant apparente à des puissances de signal incident très faibles. C’est, à ma connaissance, la première fois qu’un tel amplificateur est utilisé pour étudier la physique au sein du bruit émis par un conducteur mésoscopique. Les résultats mettent en évidence l’apparition d’un excès dans le quatrième cumulant lorsque la photoexcitation s’effectue au double de la fréquence de mesure. Un développement mathématique simple nous permet d’associer cet excès à la statistique de photons, sous la forme d’une augmentation – à nombre de photons fixe – de la variance du nombre moyen de photons contenue dans le signal. C’est en fait une signature de l’émission de paires de photons corrélés par la jonction tunnel photoexcitée. Ces résultats font le pont entre ceux obtenus précédemment par notre groupe de recherche quant aux cumulants d’ordre supérieur du bruit et ceux associées aux parallèles entre l’optique quantique et les fluctuations de courant des dispositifs mésoscopiques. [Gasse et al. PRL 111, 136601 (2013) ; Forgues et al. Scientific Reports 3, 2869 (2013) ; Forgues et al. PRL 113, 043602 (2014)] Ils dressent un portait intéressant du bruit photoexcité en termes normalement associés à l’optique quantique.