990 resultados para X-parameters


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Previously degradation studies carried out, over a number of different mortars by the research team, have shown that observed degradation does not exclusively depend on the solution equilibrium pH, nor the aggressive anions relative solubility. In our tests no reason was found that could allow us to explain, why same solubility anions with a lower pH are less aggressive than others. The aim of this paper is to study cement pastes behavior in aggressive environments. As observed in previous research, this cement pastes behaviors are not easily explained only taking into account only usual parameters, pH, solubility etc. Consequently the paper is about studying if solution physicochemical characteristics are more important in certain environments than specific pH values. The paper tries to obtain a degradation model, which starting from solution physicochemical parameters allows us to interpret the different behaviors shown by different composition cements. To that end, the rates of degradation of the solid phases were computed for each considered environment. Three cement have been studied: CEM I 42.5R/SR, CEM II/A-V 42.5R and CEM IV/B-(P-V) 32.5 N. The pastes have been exposed to five environments: sodium acetate/acetic acid 0.35 M, sodium sulfate solution 0.17 M, a solution representing natural water, saturated calcium hydroxide solution and laboratory environment. The attack mechanism was meant to be unidirectional, in order to achieve so; all sides of cylinders were sealed except from the attacked surface. The cylinders were taking out of the exposition environments after 2, 4, 7, 14, 30, 58 and 90 days. Both aggressive solution variations in solid phases and in different depths have been characterized. To each age and depth the calcium, magnesium and iron contents have been analyzed. Hydrated phases evolution studied, using thermal analysis, and crystalline compound changes, using X ray diffraction have been also analyzed. Sodium sulphate and water solutions stabilize an outer pH near to 8 in short time, however the stability of the most pH dependent phases is not the same. Although having similar pH and existing the possibility of forming a plaster layer near to the calcium leaching surface, this stability is greater than other sulphate solutions. Stability variations of solids formed by inverse diffusion, determine the rate of degradation.

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In this paper, we report calculated values of the Stark widths and shifts for 72 spectral lines of Pb v. They were calculated using the Griem semi-empirical approach. A set of wavefunctions obtained from Hartree–Fock relativistic calculations including core polarization effects was used. Stark widths and shifts corresponding to lines arising from 5d9ns (n = 7, 8), 5d9 6p, 5d9 6d and 5d9 5f configurations of Pb v. Stark widths and shifts are presented for an electron density of 1017 cm−3 and temperatures T = 1.6–5.0 (104 K). The 2142.5, 2167.9 and 2278.6 Å lines of Pb v recently measured are included in our calculations. In this case, we have included for comparison calculations without core polarization effects. There is good agreement between our calculations and the above-cited experimental values.

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Due to the particular characteristics of the fusion products, i.e. very short pulses (less than a few μs long for ions when arriving to the walls; less than 1 ns long for X-rays), very high fluences ( 10 13 particles/cm 2 for both ions and X rays photons) and broad particle energy spectra (up to 10 MeV ions and 100 keV photons), the laser fusion community lacks of facilities to accurately test plasma facing materials under those conditions. In the present work, the ability of ultraintese lasers to create short pulses of energetic particles and high fluences is addressed as a solution to reproduce those ion and X-ray bursts. Based on those parameters, a comparison between fusion ion and laser driven ion beams is presented and discussed, describing a possible experimental set-up to generate with lasers the appropriate ion pulses. At the same time, the possibility of generating X-ray or neutron beams which simulate those of laser fusion environments is also indicated and assessed under current laser intensities. It is concluded that ultraintense lasers should play a relevant role in the validation of materials for laser fusion facilities.

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We studied a series of square lattice antidot arrays, with diameter and lattice parameter from hundreds of nanometers to some microns, fabricated using two lithography techniques in epitaxial Fe(001) films. The coercivity increase of each array with respect to its base film can be scaled to a simple geometric parameter, irrespective of the lithography technique employed. Magnetic transmission x-ray microscopy studies, in arrays fabricated on polycrystalline Fe films deposited on silicon nitride membranes, evidenced the propagation of reversed domains from the edges of the arrays, in agreement with the coercivity analysis of the epitaxial arrays and with micromagnetic models.

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Soil structure plays an important role in flow and transport phenomena, and a quantitative characterization of the spatial heterogeneity of the pore space geometry is beneficial for prediction of soil physical properties. Morphological features such as pore-size distribution, pore space volume or pore?solid surface can be altered by different soil management practices. Irregularity of these features and their changes can be described using fractal geometry. In this study, we focus primarily on the characterization of soil pore space as a 3D geometrical shape by fractal analysis and on the ability of fractal dimensions to differentiate between two a priori different soil structures. We analyze X-ray computed tomography (CT) images of soils samples from two nearby areas with contrasting management practices. Within these two different soil systems, samples were collected from three depths. Fractal dimensions of the pore-size distributions were different depending on soil use and averaged values also differed at each depth. Fractal dimensions of the volume and surface of the pore space were lower in the tilled soil than in the natural soil but their standard deviations were higher in the former as compared to the latter. Also, it was observed that soil use was a factor that had a statistically significant effect on fractal parameters. Fractal parameters provide useful complementary information about changes in soil structure due to changes in soil management. Read More: http://www.worldscientific.com/doi/abs/10.1142/S0218348X14400118?queryID=%24%7BresultBean.queryID%7D&

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As principais propriedades farmacológicas da Casearia sylvestris, uma espécie de árvore cujas folhas são utilizadas na medicina popular, já foram descritas na literatura. Recentemente foi demonstrada a potente atividade citotóxica in vitro da casearina X (CAS X), o diterpeno clerodânico majoritário isolado das folhas de C. sylvestris, contra linhagens de células tumorais humanas. Apesar dos resultados promissores, sua potente atividade citotóxica in vitro não pode ser extrapolada para uma potente atividade in vivo, a menos que possua boa biodisponibilidade e duração desejável do seu efeito. Tendo em vista que o avanço nas pesquisas de produtos naturais requer a avaliação pré-clínica de propriedades farmacocinéticas, no presente trabalho foi realizada a caracterização in vitro do metabolismo e da absorção intestinal da CAS X, com o objetivo de prever sua biodisponibilidade in vivo. Para os estudos de metabolismo in vitro, foi utilizado o modelo microssomal hepático de ratos e de humanos. Foi desenvolvido um método analítico para a quantificação da CAS X em microssomas, empregando a precipitação de proteínas com acetonitrila no preparo das amostras e a cromatografia líquida de alta eficiência para as análises. O método foi validado de acordo com os guias oficiais da Agência Nacional de Vigilância Sanitária e da European Medicine Agency (EMA). A CAS X demonstrou ser substrato para as reações de hidrólise mediada pelas carboxilesterases (CES) e apresentou um perfil cinético de Michaelis-Menten. Foram estimados os parâmetros de Vmax e KM, demonstrando que o clearance intrínseco em microssomas hepático de humanos foi 1,7 vezes maior que o de ratos. O clearance hepático foi estimado por extrapolação in vitro-in vivo, resultando em mais de 90% do fluxo sanguíneo hepático em ambas as espécies. Um estudo qualitativo para a pesquisa de metabólitos foi feito utilizando espectrometria de massas, pelo qual foi possível sugerir a formação da casearina X dialdeído como produto de metabolismo. Nos estudos de absorção intestinal in vitro foi utilizado o modelo de monocamadas de células Caco-2. Um método analítico por cromatografia líquida acoplada a espectrometria de massas foi desenvolvido e validado de acordo com o EMA, para as etapas de quantificação da CAS X no sistema de células. Os parâmetros cinéticos de permeabilidade aparente absortiva e secretória da CAS X foram estimados em um sistema celular, no qual a atividade hidrolítica da CES foi inibida. Assim, a CAS X foi capaz de permear a monocamada de células Caco-2, provavelmente por transporte ativo, sem a ocorrência de efluxo, mas com significativa retenção do composto dentro das células. Em conjunto, os ensaios in vitro realizados demonstraram a susceptibilidade da CAS X ao metabolismo de primeira passagem, como substrato para as CES específicas expressas no fígado e intestino.

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Nowadays, the analysis of the X-ray spectra of magnetically powered neutron stars or magnetars is one of the most valuable tools to gain insight into the physical processes occurring in their interiors and magnetospheres. In particular, the magnetospheric plasma leaves a strong imprint on the observed X-ray spectrum by means of Compton up-scattering of the thermal radiation coming from the star surface. Motivated by the increased quality of the observational data, much theoretical work has been devoted to develop Monte Carlo (MC) codes that incorporate the effects of resonant Compton scattering (RCS) in the modeling of radiative transfer of photons through the magnetosphere. The two key ingredients in this simulations are the kinetic plasma properties and the magnetic field (MF) configuration. The MF geometry is expected to be complex, but up to now only mathematically simple solutions (self-similar solutions) have been employed. In this work, we discuss the effects of new, more realistic, MF geometries on synthetic spectra. We use new force-free solutions [14] in a previously developed MC code [9] to assess the influence of MF geometry on the emerging spectra. Our main result is that the shape of the final spectrum is mostly sensitive to uncertain parameters of the magnetospheric plasma, but the MF geometry plays an important role on the angle-dependence of the spectra.