Avaliação de oleuropeína e de sanitizantes químicos, isolados ou associados, para eliminação de biofilmes de Staphylococcus aureus, Listeria monocytogenes e Escherichia coli em superfícies inertes

Este estudo avaliou a eficiência da oleuropeína (OLE) (composto fenólico extraído das folhas de Oliveira) isolada e associada aos sanitizantes comerciais ácido peracético 2% (APA), hipoclorito de sódio 2% (HS), peróxido de hidrogênio 3% (PH), digluconato de clorexidina 2% (DC), cloreto de benzalcônio 1% (CB) e iodofor 2% (IO), para inativação de células em suspensão e biofilmes monoespécie e multiespécie formados em superfícies de aço inoxidável ou microplaca de poliestireno por Listeria monocytogenes (ATCC 7644), Staphylococcus aureus (ATCC 25923) e Escherichia coli (ATCC 25922), todas classificadas como fortes produtores de biofilmes. Os isolados foram semeados em caldo TSB (caldo tripticase soja), incubados (37°C/24h) e corrigidos a ~108células/mL (escala 0,5 McFarland). Para bactérias em suspensão, a resistência a sanitizantes foi determinada pela Concentração Inibitória Mínima (CIM) em tubos e pelo método de Disco Difusão em Ágar (DDA), no qual as bactérias foram plaqueadas em ágar TSA contendo discos de 6mm de papel filtro embebidos nos sanitizantes. Após a incubação, a medição dos halos de inibição foi feita com paquímetro. Para os ensaios de resistência dos biofilmes aos compostos sanitizantes, foram utilizadas microplacas de poliestireno 96 poços, as quais foram preparadas para incubação-fixação dos biofilmes e submetidas à leitura em espectrofotômetro de ELISA (600 nm). Em seguida, as placas foram lavadas com solução salina tamponada (PBS, pH 7.4) e os sanitizantes inseridos por 1 minuto. Após neutralização com tiossulfato de sódio (5 minutos), as placas foram lavadas com PBS e metanol, coradas com cristal violeta 1% e coradas com ácido acético glacial (33%) para nova leitura a 570nm. A eficácia da remoção do biofilme pelos sanitizantes foi comparada pelo índice de formação de biofilme (IFB). As imagens do aço inoxidável após tratamento com sanitizante foram feitas através de Microscopia Eletrônica de Varredura (MEV) e Microscopia Confocal, para visualizar a persistência dos biofilmes. Os valores de CIM (diluição 1:2) mostraram que OLE não teve atividade bactericida. No método DDA, L. monocytogenes, foi resistente à OLE, enquanto E. coli e S. aureus apresentaram resistência intermediária. Os sanitizantes comerciais apresentaram boa atividade bactericida nos ensaios de CIM e DDA, sendo que as associações de OLE aos sanitizantes comerciais aumentaram o efeito germicida. Nos ensaios com biofilmes em monoespécie, somente os sanitizantes comerciais, isolados ou associados com OLE, foram eficazes de reduzir o valor de BFI em microplaca de poliestireno. Em biofilmes multiespécie, OLE apresentou efeito antimicrobiano, sobretudo sobre a associação de L. monocytogenes + E. coli + S. aureus (redução: 91,49%). Nenhum dos compostos avaliados foi capaz de inativar completamente os biofilmes nas superfícies de aço inoxidável, uma vez que células viáveis foram observadas após os tratamentos com os sanitizantes, indicando persistência dos biofilmes. Os resultados indicam que a oleuropeína apresentou potencial para incrementar o efeito bactericida de sanitizantes comerciais para eliminação de biofilmes em superfícies inertes, sendo necessários estudos para compreender os mecanismos de ação dessas combinações.

Fixed Mydriatic Pupil Associated with an Intraocular Pressure Rise as a Complication of the Implant of a Phakic Refractive Lens (PRL)

We describe a case report of a patient that was implanted with a posterior chamber phakic intraocular lens (Phakic Refractive Lens, PRL) for the correction of moderate myopia and who developed postoperatively a fixed mydriasis compatible with an Urrets-Zavalia Syndrome (UZS). Specifically, a sudden acute increase of IOP in the left eye was observed in the immediate postoperative period. After IOP stabilization, the refractive result was good, but a fixed and mydriatic pupil appeared. This condition led the patient to experience visual discomfort, halos, and glare associated with high levels of higher-order aberrations in spite of the good visual result. A tinted-contact lens was fitted in order to minimize those symptoms. The UZS should be considered as a possible complication after implantation of posterior chamber phakic intraocular lenses.

(Table 1) Chemical composition and bulk densities of dolerites from ODP Hole 504B lower dikes

Chemical interactions between seawater and the oceanic crust have been widely investigated during recent years. However, most of these studies concern the uppermost volcanic part of the crust. The contribution of the underlying sheeted dike complex to the global budget of the oceans is inferred solely from some ophiolite studies and from the 500-m high-level dike section of DSDP/ODP 504B which was drilled in 1981. Hole 504B is the only place where a continuous and long (1260 m) section in the sheeted dike complex has been cored, and it is now regarded as a reference section for the upper oceanic crust. Many petrological and chemical data from these dolerites are available, including the relative proportions of veins, extensively altered adjacent rocks, and less altered 'host-rocks'. For these three reasons, considering the entire dike section penetrated by Hole 504B is a unique chance to study chemical fluxes related to hydrothermal alteration of this part of the oceanic crust. The calculation of any chemical flux implies knowledge of the chemical composition of the fresh precursor (protolith). Previously, mean compositions of glasses (=P1a) or basalts from the Hole 504B volcanics have been used as protoliths. In this paper, we calculate and discuss the use of various protoliths based on dolerites from Hole 504B. We show that the most adequate and realistic protolith is the mean of individual protoliths that we calculated from the acquisition, by automatic mode, of about 1000 microprobe analyses in each thin-section of dolerite from the Hole 504B lower dikes. Consequently, PFm is further used to calculate chemical fluxes in the dike section of Hole 504B. The chemical compositions of the host-rocks adjacent to alteration halos tend to converge to that of PFm with depth, except for Fe2O3t and TiO2. Because the volume percent of alteration halos increases with depth, the total fluxes related to these halos increase with depth. This explains why the mean flux (host-rocks+halos+veins) of the upper dikes is roughly similar to the mean flux of the lower dikes. During the alteration of the entire Hole 504B dike section, the dolerites gained relatively large quantities of Fe2O3t (+4.0 g/100 cm**3) and released much SiO2 (-6.8 g/100 cm**3), CaO (-5.8 g/100 cm**3), and TiO2 (1.6 g/100 cm**3), and minor Al2O3 (-0.7 g/100 cm**3) and MgO (-0.7 g/100 cm**3). We show the importance of the choice of the protolith in the calculation of chemical budget, particularly for elements showing low flux values. In Hole 504B, the Mg uptake by the volcanics during low temperature alteration added to the Mg release by the dikes gives a net flux of -0.07x10**14 g/year. We propose that part of the Mg uptake by the oceanic crust, which is necessary to compensate the rivers input (-1.33x10**14 g/year), occurs in the underlying gabbros and/or in sections which are altered such as Trinity and Troodos ophiolites. Compared with ophiolites, fluxes calculated for elements other than Mg for the entire crust are generally similar (in tendency, if not in absolute value) to that we obtained from Hole 504B.

Chemistry of very young basalts from ODP Hole 106-648B

Basalts in Hole 648B, located in the rift valley of the Mid-Atlantic Ridge at 23°N in crust estimated to be less than 100,000 years old, are mainly fresh, but small amounts of secondary phases are found on fracture surfaces and in alteration halos within the rocks. The halos are defined by dark bands 1-4 mm thick that have developed parallel to fracture surfaces or pillow margins and which in some cases have migrated some centimeters into the rock. The dark bands are the principal locus of secondary phases. The secondary phases are olive-green and yellow protoceladonites, of composition and structure intermediate between celadonite and iron-rich saponite, red (Mn-poor) to opaque (Mn-rich) iron oxyhydroxides, mixtures of protoceladonite and iron oxyhydroxide, and rare manganese oxides. These phases occur mainly as linings or fillings of open spaces in the basalt within the dark bands. Sulfides and intersertal glass are the only primary phases that can be seen to have been altered. Where dark bands have migrated into the rock, the rock behind the advancing band is almost devoid of secondary phases, implying redissolution. The potassium and magnesium in the secondary phases could have been supplied from ambient seawater. The aluminum in the protoceladonites must have been derived from local reaction of intergranular glass. The source of iron and silica could have been intergranular glass or low temperature mineralizing solutions of the type responsible for the formation of deposits of manganese oxides and iron oxyhydroxides and silicates on the seafloor.

Intergalactic H II regions discovered in SINGG

A number of very small isolated H II regions have been discovered at projected distances up to 30 kpc from their nearest galaxy. These H II regions appear as tiny emission-line objects in narrowband images obtained by the NOAO Survey for Ionization in Neutral Gas Galaxies (SINGG). We present spectroscopic confirmation of four isolated H II regions in two systems; both systems have tidal H I features. The results are consistent with stars forming in interactive debris as a result of cloud-cloud collisions. The Halpha luminosities of the isolated H II regions are equivalent to the ionizing flux of only a few O stars each. They are most likely ionized by stars formed in situ and represent atypical star formation in the low-density environment of the outer parts of galaxies. A small but finite intergalactic star formation rate will enrich and ionize the surrounding medium. In one system, NGC 1533, we calculate a star formation rate of 1.5 x 10(-3) M-. yr(-1), resulting in a metal enrichment of similar to 1 x 10(-3) solar for the continuous formation of stars. Such systems may have been more common in the past and a similar enrichment level is measured for the metallicity floor'' in damped Lyalpha absorption systems.

(Table T1) Trace-element abundances for igneous basement at ODP Site 206-1256

In this report, I present trace element data for basement samples at Ocean Drilling Program (ODP) Site 1256. The samples analyzed represent a subset of the group ("pool") samples from ODP Leg 206, and these trace element data are part of a more comprehensive data suite for the same samples, with analyses of stable and radiogenic isotopes (e.g., Sr, Li, and O) in progress or recently completed that will be presented elsewhere. The trace element analyses were performed in the GeoAnalytical Lab at Washington State University. The following elements were analyzed: La, Ce, Pr, Nd, Sm, Eu, Gd, Tb, Dy, Ho, Er, Tm, Yb, Lu, Ba, Th, Nb, Y, Hf, Ta, U, Pb, Rb, Cs, Sr, Sc, and Zr. Trace element data indicate that the igneous basement at Site 1256 is geochemically normal mid-ocean-ridge basalt. A massive ponded flow sampled in both Holes 1256C and 1256D is distinguished by higher abundances of rare earth elements (REE) and most of the other trace elements analyzed. One interval of highly altered basalt has significantly higher concentrations of Cs, Rb, and Ba and lower concentrations of Sr, Pb, Zr, Hf, Sc, and most REE than the samples of background alteration or halos. No correlation is obvious between trace element abundance and macroscopic type of alteration within the background alteration or halos.

(Table 1) Sulfur and oxygen isotopes from two anhydrite samples recovered from DSDP Hole 70-504B

The first anhydrite reported from oceanic basalts occurs in altered basalts drilled during DSDP Leg 70 from Hole 504B. Anhydrite has been identified in several samples, two of which were studied in detail. Anhydrite in Sample 504B-40-3 (130-135 cm), which was acquired at 310 meters sub-basement, occurs in a dolerite at the center of a vug rimmed by saponite and calcite. Red iron-hydroxide-rich alteration halos occur from 0 to 310 meters sub-basement; primary sulfides in these halos are oxidized, and the rocks have lost large amounts of sulfur. The anhydrite in this sample has a d34S value of 18.5 per mil, and it is interpreted to have formed from a fluid containing a mixture of seawater sulfate (20.9 per mil) and basaltic sulfur (0 per mil) released during the oxidation of primary sulfides. Anhydrite in Sample 504B-48-3 (14-18 cm), which was found at 376 meters sub-basement, occurs intergrown with gyrolite at the center of a 1-cm-wide vein that is rimmed by saponite and quartz. At sub-basement depths below 310 meters to the bottom of the Leg 70 section (562 m sub-basement), the rocks exhibit the effects of anoxic alteration with common secondary pyrite. Anhydrite in Sample 504B-48-3 (14-18 cm) has a d34S value of 36.7 per mil, and it is interpreted to have formed from seawater-derived fluids enriched in 34S through sulfate reduction. Temperatures of alteration calculated from oxygen isotope data range from 60 to 100°C. Sulfate reduction may have occurred in situ, or elsewhere at higher temperature, possibly deeper in the crust. The secondary mineral paragenetic sequence indicates a progressive decrease in Mg and increase in Ca in the circulating fluids. This eventually led to anhydrite formation late in the alteration process.

Geochemistry of sheeted dike complex minerals of ODP Hole 140-504B

Diabases were recovered during Legs 137 and 140 at Hole 504B from depths between 1621.5 and 2000.4 meters below seafloor in the lower sheeted dike complex. The samples contain multiple generations of millimetric to centimetric veins. The orientation of the measured veins suggests that two main vein sets exist: one characterized by shallow dipping and the other by random trend. Thermal contraction during rock cooling is considered the main mechanism responsible for fracture formation. Vein infill is related to the circulation of hydrothermal fluids near the spreading axis. Some veins are surrounded by millimeter-sized alteration halos due to fluid percolation from the fractures through the host rock. Vein-filling minerals are essentially amphibole, chlorite, and zeolites. Amphibole composition is controlled by the microstructural site of the rock. Actinolite is the main amphibole occurring in the veins and also in the groundmass away from the halos. In the alteration halos, amphibole shows composition of actinolitic hornblende and Mg-hornblende. Late-stage tension gashes and interstitial spaces in some amphibole-bearing veins are filled with zeolites, suggesting that the veins likely suffered multiple opening stages that record the cooling history of the circulating fluids. Evidence of deformation recorded by the recovered samples seems to be restricted to veins that clearly represent elements of weakness of the rock. On the basis of vein geometry and microstructure we infer structural interpretations for the formation mechanism and for deformation of veins.

The effects of transients on photospheric and chromospheric power distributions

We have observed a quiet Sun region with the Swedish 1-meter Solar Telescope (SST) equipped with CRISP Imaging SpectroPolarimeter. High-resolution, high-cadence, H-alpha line scanning images were taken to observe different layers of the solar atmosphere from the photosphere to upper chromosphere. We study the distribution of power in different period-bands at different heights. Power maps of the upper photosphere and the lower chromosphere show suppressed power surrounding the magnetic-network elements, known as "magnetic shadows". These also show enhanced power close to the photosphere, traditionally referred to as"power halos". The interaction between acoustic waves and inclined magnetic fields is generally believed to be responsible for these two effects. In this study we explore if small-scale transients can influence the distribution of power at different heights. We show that the presence of transients, like mottles, Rapid Blueshifted Excursions (RBEs) and Rapid Redshifted Excursions (RREs), can strongly influence the power-maps. The short and finite lifetime of these events strongly affects all powermaps, potentially influencing the observed power distribution. We show that Doppler-shifted transients like RBEs and RREs that occur ubiquitously, can have a dominant effect on the formation ofthe power halos in the quiet Sun. For magnetic shadows, transients like mottles do not seem to have a significant effect in the power suppression around 3 minutes and wave interaction may play a key role here. Our high cadence observations reveal that flows, waves and shocks manifest in presence of magnetic fields to form a non-linear magnetohydrodynamic system.

Optimization of lipase production from yeasts strains isolated from olive mil wastewater

Dissertação submetida à Universidade de Lisboa, Faculdade de Ciências para a obtenção do Grau de Mestre em Microbiologia Aplicada.

Examining the growth and evolution of magnetic fields in clusters of galaxies: a numerical perspective

Magnetic fields are ubiquitous in galaxy cluster atmospheres and have a variety of astrophysical and cosmological consequences. Magnetic fields can contribute to the pressure support of clusters, affect thermal conduction, and modify the evolution of bubbles driven by active galactic nuclei. However, we currently do not fully understand the origin and evolution of these fields throughout cosmic time. Furthermore, we do not have a general understanding of the relationship between magnetic field strength and topology and other cluster properties, such as mass and X-ray luminosity. We can now begin to answer some of these questions using large-scale cosmological magnetohydrodynamic (MHD) simulations of the formation of galaxy clusters including the seeding and growth of magnetic fields. Using large-scale cosmological simulations with the FLASH code combined with a simplified model of the acceleration of cosmic rays responsible for the generation of radio halos, we find that the galaxy cluster frequency distribution and expected number counts of radio halos from upcoming low-frequency sur- veys are strongly dependent on the strength of magnetic fields. Thus, a more complete understanding of the origin and evolution of magnetic fields is necessary to understand and constrain models of diffuse synchrotron emission from clusters. One favored model for generating magnetic fields is through the amplification of weak seed fields in active galactic nuclei (AGN) accretion disks and their subsequent injection into cluster atmospheres via AGN-driven jets and bubbles. However, current large-scale cosmological simulations cannot directly include the physical processes associated with the accretion and feedback processes of AGN or the seeding and merging of the associated SMBHs. Thus, we must include these effects as subgrid models. In order to carefully study the growth of magnetic fields in clusters via AGN-driven outflows, we present a systematic study of SMBH and AGN subgrid models. Using dark-matter only cosmological simulations, we find that many important quantities, such as the relationship between SMBH mass and galactic bulge velocity dispersion and the merger rate of black holes, are highly sensitive to the subgrid model assumptions of SMBHs. In addition, using MHD calculations of an isolated cluster, we find that magnetic field strengths, extent, topology, and relationship to other gas quantities such as temperature and density are also highly dependent on the chosen model of accretion and feedback. We use these systematic studies of SMBHs and AGN inform and constrain our choice of subgrid models, and we use those results to outline a fully cosmological MHD simulation to study the injection and growth of magnetic fields in clusters of galaxies. This simulation will be the first to study the birth and evolution of magnetic fields using a fully closed accretion-feedback cycle, with as few assumptions as possible and a clearer understanding of the effects of the various parameter choices.

Isolamento, seleção e cultivo de leveduras com potencia biotecnológico para a produção de endo-xilaneses

Xilanases são enzimas que catalisam a hidrólise das xilanas e têm sido em grande parte, obtidas a partir de bolores e bactérias. No entanto poucos estudos têm sido relatados sobre a produção destas enzimas por leveduras. O presente trabalho teve como objetivo isolar leveduras de diferentes fontes vegetais visando à produção de xilanases, além de maximizar sua produção, estudar o uso de diferentes fontes de nitrogênio e cultivar as leveduras em meios contendo coprodutos agroindustriais. As amostras de alimentos e resíduos foram enriquecidas em caldo extrato de malte e levedura e isoladas em Ágar Nutriente Wallerstein, as leveduras isoladas foram, a seguir, avaliadas quanto à capacidade de degradar xilana presente no meio e produzir halos de hidrólise, os quais foram visualizados através do uso do corante vermelho congo. Os micro-organismos selecionados como potenciais produtores de xilanase foram crescidos em meio complexo líquido e as atividades enzimáticas de endoxilanase, β-xilosidase, carboximetilcelulase, celulase total, pH e concentração de biomassa foram avaliadas ao longo de 96 h de cultivo. Dentre as leveduras isoladas, sete foram selecionadas, e a 18Y foi a que apresentou a maior atividade de endo- xilanase (2,7 U.mL-1 ), sendo esta isolada de chicória e identificada como Cryptococcus laurentii. Esta estirpe apresentou capacidade de produzir xilanase com baixos níveis de celulase, sendo assim selecionada neste trabalho. A maximização de endo-xilanase foi avaliada fazendo uso de planejamento experimental onde primeiramente foi realizado um planejamento fracionário 2 6-2 para verificar os efeitos do pH inicial e as concentrações de xilana, peptona, (NH4)2SO4, extrato de levedura e KH2PO4 sobre a atividade enzimática. Após selecionar as variáveis xilana, peptona, pH e extrato de levedura foi realizado um delineamento composto central rotacional (24 ) onde todos os cultivos foram mantidos a 30°C, 150 rpm durante 96 h sendo retiradas alíquotas para determinação das atividades, pH e biomassa. A produção máxima foi de 6,9 U.mL-1 usando 10,0 g.L-1 de extrato de levedura, 10,0 g.L-1 de peptona, 10,0 g.L-1 de xilana, 1,0 g.L-1 de (NH4)2SO4 em pH 6,5 o que permitiu um incremento de mais de 250% sobre a atividade. Posteriormente foram realizados ensaios avaliando diferentes fontes e concentrações de nitrogênio orgânico e inorgânico. A presença de NH4NO3 e (NH₄)₂SO₄ usados na concentração de 3% proporcionaram as maiores atividades de endo-xilanase (6,2 e 6,0 U.mL-1 respectivamente). O sulfato de amônio foi selecionado e fixado em 1 g.L-1 e logo após um planejamento completo 22 foi realizado onde as variáveis xilana e extrato de levedura foram estudadas e as demais fixadas. As condições ótimas estabelecidas para a produção da enzima foram: concentração de xilana de 18,6 g.L-1 , concentração de extrato de levedura de 10 g.L-1 atingindo 14 U.mL-1 . Após a maximização enzimática estudou-se o crescimento de Pichia pastoris NRRL Y-1603 e Cryptococcus laurentti em cinco substratos agroindustriais visando a possibilidade estes substratos substituírem a xilana em cultivos para a produção de endo-xilanase. Os ensaios foram realizados utilizando os subtratos pré-tratados com NaOH 4% e não tratados. Para inserção dos mesmos aos meios de cultivo, estes foram moídos e adicionados na concentração de 2%. O pré-tratamento para todos as fontes de hemicelulose foi eficiente e promoveu aumento nas atividades produzidas. Cryptococcus laurentti apresentou maior atividade enzimática (8,7 U.mL-1 ) em farelo de arroz desengordurado e pré- tratado enquanto que a levedura Pichia pastoris NRRL Y-1603 apresentou sua melhor condição para produção de endo-xilanase quando cultivada em meio contendo casca de aveia e o farelo de arroz pré-tratados, alcançando atividades máximas de 7,6 e 7,5 U.mL-1 .

Biomimetic accommodating intraocular lens

The crystalline lens allows the eye to focus on near and far objects. During the aging process, it loses its ability to focus and often becomes cloudy during cataract formation. At this point, traditional medical therapy replaces the lens with an artificial replacement lens. Although replacement lenses for the crystalline lens have been implanted since 1949 for cataract surgery, none of the FDA-approved lenses mimic the anatomy of the natural lens. Hence, they are not able to focus in a manner similar to the youthful lens. Instead, they function in a manner similar to the aged lens and only provide vision at a single distance or at a very limited range of focal distances. Patients with the newest implants are often obliged to use reading glasses when using near vision, or suffer from optical aberrations, halos, or glare. Therefore, there is a need to provide youthful vision after lens surgery in terms of focusing ability, accurate optical power, and sharp focus without distortion or optical aberrations.

This thesis presents an approach to restoring youthful vision after lens replacement. An intraocular lens (IOL) that can provide accurate visual acuity along with focusing ability is proposed. This IOL relies on the natural anatomy and physiology of the eye, and therefore is actuated in a manner identical to the natural lens. In addition, the lens has the capability for adjustment during or after implantation to provide high-acuity vision throughout life.

The natural anatomy and physiology of the eye is described, along with lens replacement surgery. A lens design is proposed to address the unmet need of lens-replacement patients. Specific care in the design is made for small surgical incisions, high visual acuity, adjustable acuity over years, and the ability to focus similar to the natural lens. Methods to test the IOL using human donor tissue are developed based upon prior experiments on the ex vivo natural lens. These tools are used to demonstrate efficacy of the newly developed accommodating intraocular lens.

To further demonstrate implant feasibility, materials and processes for building the lens are evaluated for biocompatibility, endurance, repeatable manufacture, and stability. The lens biomechanics are determined after developing an artificial anatomy testing setup inspired by the natural anatomy of the human focusing mechanism. Finally, based upon a mechanical and optical knowledge of the lens, several improved lens concepts are proposed and demonstrated for efficacy.

Atividade fitotóxica de extratos e exsudatos radiculares de Guilandina bonduc (Fabaceae)

Dissertação (mestrado)—Universidade de Brasília, Departamento de Botânica, Programa de Pós-Graduação em Botânica, 2015.