Avaliação da influência de antioxidantes na estabilização de biodiesel

O biodiesel é uma fonte de energia renovável, que se pode obter pela transformação dos resíduos domésticos, e é ambientalmente inócuo, e fácil de transportar, pois tem um ponto de fulgor elevado. Atualmente tem-se focado a atenção nos efeitos da oxidação do biodiesel causados pelo contato com o ar ambiente durante o seu armazenamento. Os produtores, fornecedores e consumidores, pretendem garantir que a qualidade do biodiesel e das suas misturas com combustíveis destilados do petróleo, mantém-se durante longos períodos de armazenamento. A maioria dos óleos vegetais e das gorduras animais, usados como matéria – prima, são triacilgliceróis com grupos ácido gordos de cadeia longa (C16 – C18) ligados por ligações éster a uma estrutura de glicerol. O objetivo deste estudo foi avaliar a eficiência do ácido gálhico e seus derivados alquilo ésteres aumentando a resistência relativa à oxidação do ácido linoléico, inibindo a peroxidação ácido gordos de cadeia longa insaturados. Outro objetivo foi estudar a taxa de inibição da auto-oxidação do ácido linoleico. Foi, ainda estudado o efeito que a concentração do antioxidante, tinha na estabilidade do ácido linoleico. No caso do ácido gálhico verificou-se que o aumento para o dobro da concentração do antioxidante utilizada, obtinha-se quase o dobro da taxa de inibição da oxidação do ácido linoleico. A auto-oxidação de ácido linoleico é acompanhada pela formação do seu dieno conjugado, o qual foi medido sua absorvância, durante 7 dias, por espetrofotometria de absorção UV a 234 nm. Uma diminuição da taxa de formação de dieno conjugado, indica o aumento da atividade antioxidante do composto adicionado à micela de ácido linoleico. Os resultados obtidos permitem concluir que de todos os antioxidantes testados o galhato de butilo é o que possibilita uma maior inibição da oxidação do ácido linoleico para as duas concentrações de antioxidantes testadas (0,1 mM e 1mM), obteve-se uma percentagem de inibição do ácido linoleico de 54,0% e 63,6%, respetivamente. O estudo comparativo da estabilização do ácido linoleico com o antioxidante de referência, o butil -hidroxitolueno, mostrou que este composto tem um poder de estabilização inferior a qualquer dos antioxidantes estudados. Os resultados deste estudo demonstraram que a utilização de compostos fenólicos, em especial o galhato de butilo, constitui uma boa alternativa para a estabilização de matrizes lipídicas, nomeadamente de combustíveis como o biodiesel.Biodiesel is a renewable fuel that is derived from domestic feedstock and described to be environmentally innocuous and safe to handle because it has a relatively high flash point. Currently, it has focused attention on the effects of biodiesel oxidation caused by contact with ambient air during storage. The manufacturers, suppliers and consumers want to ensure that the quality of biodiesel and their mixtures with petroleum distillate fuels, maintained for long storage periods. Most vegetable oils and animal fats, used as raw material, are triacylglycerols with fatty acid groups of long chain (C16 - C18) connected by ester linkages to a structure glycerol. The aim of this study was to examine the effectiveness of gallic acid and its alkyl esters derivatives in increasing the relative resistance to oxidation of linoleic acid by inhibiting unsaturated long-chain fatty acid peroxidation. Also, another aim, was to study the rate of inhibition of the linoleic acid autoxidation. The effect that concentration of the antioxidant had on the linoleic acid stability was investigated. Phenolic acids showed that the increase for the double of concentration resulted in improvement for the double on the the rate of inhibition of oxidation of linoleic acid. The linoleic acid autoxidation is accompanied by the formation of its conjugated diene, which absorbance was measured, for 7 days, by UV absorption spectrophotometry at 234 nm. A decrease in the rate of conjugated diene formation, indicate the increase of antioxidant activity of the compound added to the micelle of linoleic acid. The results obtained indicate that of all antioxidants tested the best antioxidant inhibiting the oxidation of linoleic acid is butyl gallate. Thus, for the two concentrations of antioxidants tested (0.1 mM and 1 mM), was obtained a percentage of linoleic acid inhibition of 54.0% and 63.6%, respectively. The comparative study of stability of linoleic acid with the reference antioxidant, butylhydroxytoluene, showed that this compound has a stabilizing power less than any of the antioxidants studied. The results of this study demonstrated that the use of phenolic compounds, especially butyl gallate, provides a good alternative for the stabilization of lipid matrices, such as biodiesel fuel

MutLα heterodimers modify the molecular phenotype of Friedreich ataxia

This article has been made available through the Brunel Open Access Publishing Fund.Background: Friedreich ataxia (FRDA), the most common autosomal recessive ataxia disorder, is caused by a dynamic GAA repeat expansion mutation within intron 1 of FXN gene, resulting in down-regulation of frataxin expression. Studies of cell and mouse models have revealed a role for the mismatch repair (MMR) MutS-heterodimer complexes and the PMS2 component of the MutLα complex in the dynamics of intergenerational and somatic GAA repeat expansions: MSH2, MSH3 and MSH6 promote GAA repeat expansions, while PMS2 inhibits GAA repeat expansions. Methodology/Principal Findings: To determine the potential role of the other component of the MutLα complex, MLH1, in GAA repeat instability in FRDA, we have analyzed intergenerational and somatic GAA repeat expansions from FXN transgenic mice that have been crossed with Mlh1 deficient mice. We find that loss of Mlh1 activity reduces both intergenerational and somatic GAA repeat expansions. However, we also find that loss of either Mlh1 or Pms2 reduces FXN transcription, suggesting different mechanisms of action for Mlh1 and Pms2 on GAA repeat expansion dynamics and regulation of FXN transcription. Conclusions/Significance: Both MutLα components, PMS2 and MLH1, have now been shown to modify the molecular phenotype of FRDA. We propose that upregulation of MLH1 or PMS2 could be potential FRDA therapeutic approaches to increase FXN transcription. © 2014 Ezzatizadeh et al.This article has been made available through the Brunel Open Access Publishing Fund

The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIRE

A large sub-mm survey with Herschel will enable many exciting science opportunities, especially in an era of wide-field optical and radio surveys and high resolution cosmic microwave background experiments. The Herschel-SPIRE Legacy Survey (HSLS), will lead to imaging data over 4000 sq. degrees at 250, 350, and 500 micron. Major Goals of HSLS are: (a) produce a catalog of 2.5 to 3 million galaxies down to 26, 27 and 33 mJy (50% completeness; 5 sigma confusion noise) at 250, 350 and 500 micron, respectively, in the southern hemisphere (3000 sq. degrees) and in an equatorial strip (1000 sq. degrees), areas which have extensive multi-wavelength coverage and are easily accessible from ALMA. Two thirds of the of the sources are expected to be at z > 1, one third at z > 2 and about a 1000 at z > 5. (b) Remove point source confusion in secondary anisotropy studies with Planck and ground-based CMB data. (c) Find at least 1200 strongly lensed bright sub-mm sources leading to a 2% test of general relativity. (d) Identify 200 proto-cluster regions at z of 2 and perform an unbiased study of the environmental dependence of star formation. (e) Perform an unbiased survey for star formation and dust at high Galactic latitude and make a census of debris disks and dust around AGB stars and white dwarfs

Design concepts for the Cherenkov Telescope Array CTA: an advanced facility for ground-based high-energy gamma-ray astronomy

Ground-based gamma-ray astronomy has had a major breakthrough with the impressive results obtained using systems of imaging atmospheric Cherenkov telescopes. Ground-based gamma-ray astronomy has a huge potential in astrophysics, particle physics and cosmology. CTA is an international initiative to build the next generation instrument, with a factor of 5-10 improvement in sensitivity in the 100 GeV-10 TeV range and the extension to energies well below 100 GeV and above 100 TeV. CTA will consist of two arrays (one in the north, one in the south) for full sky coverage and will be operated as open observatory. The design of CTA is based on currently available technology. This document reports on the status and presents the major design concepts of CTA

Multi-messenger observations of a binary neutron star merger

On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of 40+8-8 Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 Mo. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ~40 Mpc) less than 11 hours after the merger by the One- Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ~10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position ~9 and ~16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta

Historical Pollution: In Search of a Legal Definition

The chapter introduces and investigates the concept of \u201chistorical pollution\u201d in the context of environmental law. The subject is complex, as the principal consideration in our analysis concerns the role of time in the causation of harmful consequences (both for the environment and human health), notably in view of the prolonged timeframe that separates the conduct (pollution) and the effect (contamination). The phenomenon under scrutiny has significant implications for both the legal and the social fields. Indeed, legal enforcement of putative crimes against the environment is generally ineffective precisely because of this temporal factor, and this also has consequences for social perceptions and the dynamics of victimization. Yet these considerations could also contribute to a definition of historical pollution, as\u2014 given the complexity and uncertainties that surround the phenomenon\u2014they suggest ways in which material cases could be used to frame a general understanding of the concept. Attention here is focused on pollution related to industrial activities since such cases are prominent in the field. The proposed definition strives to establish a general framework within which domestic analyses can be located, consistent with the particularities of each legal system. It represents one of the first steps into the unexplored terrain of historical pollution

Species diversification – which species should we use?

Large detector systems for particle and astroparticle physics; Particle tracking detectors; Gaseous detectors; Calorimeters; Cherenkov detectors; Particle identification methods; Photon detectors for UV. visible and IR photons; Detector alignment and calibration methods; Detector cooling and thermo-stabilization; Detector design and construction technologies and materials. The LHCb experiment is dedicated to precision measurements of CP violation and rare decays of B hadrons at the Large Hadron Collider (LHC) at CERN (Geneva). The initial configuration and expected performance of the detector and associated systems. as established by test beam measurements and simulation studies. is described. © 2008 IOP Publishing Ltd and SISSA