635 resultados para PIC 18F8722
Resumo:
Prenatal immune challenge (PIC) in pregnant rodents produces offspring with abnormalities in behavior, histology, and gene expression that are reminiscent of schizophrenia and autism. Based on this, the goal of this article was to review the main contributions of PIC models, especially the one using the viral-mimetic particle polyriboinosinic-polyribocytidylic acid (poly-I:C), to the understanding of the etiology, biological basis and treatment of schizophrenia. This systematic review consisted of a search of available web databases (PubMed, SciELO, LILACS, PsycINFO, and ISI Web of Knowledge) for original studies published in the last 10 years (May 2001 to October 2011) concerning animal models of PIC, focusing on those using poly-I:C. The results showed that the PIC model with poly-I:C is able to mimic the prodrome and both the positive and negative/cognitive dimensions of schizophrenia, depending on the specific gestation time window of the immune challenge. The model resembles the neurobiology and etiology of schizophrenia and has good predictive value. In conclusion, this model is a robust tool for the identification of novel molecular targets during prenatal life, adolescence and adulthood that might contribute to the development of preventive and/or treatment strategies (targeting specific symptoms, i.e., positive or negative/cognitive) for this devastating mental disorder, also presenting biosafety as compared to viral infection models. One limitation of this model is the incapacity to model the full spectrum of immune responses normally induced by viral exposure.
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We have completed a high-contrast direct imaging survey for giant planets around 57 debris disk stars as part of the Gemini NICI Planet-Finding Campaign. We achieved median H-band contrasts of 12.4 mag at 0.''5 and 14.1 mag at 1'' separation. Follow-up observations of the 66 candidates with projected separation <500 AU show that all of them are background objects. To establish statistical constraints on the underlying giant planet population based on our imaging data, we have developed a new Bayesian formalism that incorporates (1) non-detections, (2) single-epoch candidates, (3) astrometric and (4) photometric information, and (5) the possibility of multiple planets per star to constrain the planet population. Our formalism allows us to include in our analysis the previously known β Pictoris and the HR 8799 planets. Our results show at 95% confidence that <13% of debris disk stars have a ≥5 M Jup planet beyond 80 AU, and <21% of debris disk stars have a ≥3 M Jup planet outside of 40 AU, based on hot-start evolutionary models. We model the population of directly imaged planets as d 2 N/dMdavpropm α a β, where m is planet mass and a is orbital semi-major axis (with a maximum value of a max). We find that β < –0.8 and/or α > 1.7. Likewise, we find that β < –0.8 and/or a max < 200 AU. For the case where the planet frequency rises sharply with mass (α > 1.7), this occurs because all the planets detected to date have masses above 5 M Jup, but planets of lower mass could easily have been detected by our search. If we ignore the β Pic and HR 8799 planets (should they belong to a rare and distinct group), we find that <20% of debris disk stars have a ≥3 M Jup planet beyond 10 AU, and β < –0.8 and/or α < –1.5. Likewise, β < –0.8 and/or a max < 125 AU. Our Bayesian constraints are not strong enough to reveal any dependence of the planet frequency on stellar host mass. Studies of transition disks have suggested that about 20% of stars are undergoing planet formation; our non-detections at large separations show that planets with orbital separation >40 AU and planet masses >3 M Jup do not carve the central holes in these disks.
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We have carried out high contrast imaging of 70 young, nearby B and A stars to search for brown dwarf and planetary companions as part of the Gemini NICI Planet-Finding Campaign. Our survey represents the largest, deepest survey for planets around high-mass stars (≈1.5-2.5 M ☉) conducted to date and includes the planet hosts β Pic and Fomalhaut. We obtained follow-up astrometry of all candidate companions within 400 AU projected separation for stars in uncrowded fields and identified new low-mass companions to HD 1160 and HIP 79797. We have found that the previously known young brown dwarf companion to HIP 79797 is itself a tight (3 AU) binary, composed of brown dwarfs with masses 58$^{+21}_{-20}$ M Jup and 55$^{+20}_{-19}$ M Jup, making this system one of the rare substellar binaries in orbit around a star. Considering the contrast limits of our NICI data and the fact that we did not detect any planets, we use high-fidelity Monte Carlo simulations to show that fewer than 20% of 2 M ☉ stars can have giant planets greater than 4 M Jup between 59 and 460 AU at 95% confidence, and fewer than 10% of these stars can have a planet more massive than 10 M Jup between 38 and 650 AU. Overall, we find that large-separation giant planets are not common around B and A stars: fewer than 10% of B and A stars can have an analog to the HR 8799 b (7 M Jup, 68 AU) planet at 95% confidence. We also describe a new Bayesian technique for determining the ages of field B and A stars from photometry and theoretical isochrones. Our method produces more plausible ages for high-mass stars than previous age-dating techniques, which tend to underestimate stellar ages and their uncertainties.
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[EN] This paper describes the use of perhaps, maybe and possibly in a cross-disciplinary corpus of academic and popularised scientific writing. It accounts for their higher frequency in popularised discourse by investigating their functions in detail. The analysis, conducted from various perspectives (syntactic, semantic, pragmatic and rhetorical), suggests that two factors are at work: the evidential basis for the epistemic assessment and the mode of discourse the marker is most closely associated with.
Resumo:
[ES] Los efluentes ganaderos constituyen un beneficioso aporte de nutrientes para los cultivos, que es fundamental a la hora de garantizar la sostenibilidad de la gestión de las explotaciones ganaderas, pudiendo ocasionar graves problemas ambientales si se emplean mal. La intensificación agraria ha convertido los efluentes ganaderos de subproducto a residuo. Su tratamiento con materiales locales y tecnologías de baja intensidad es una solución de bajo coste financiero y energético. En el proyecto REAGUA se plantea la posibilidad de utilizar el “picón” (lapilli) como material para el tratamiento del estiércol líquido de rumiantes, para su posterior empleo en el riego enterrado de especies forrajeras y biocombustibles, actuando el suelo como medio de depuración avanzado. Para ello, se diseña un sistema en el que se aporte el efluente con un flujo subsuperficial vertical en un medio no saturado, que circule por tres fases (en serie). Para determinar las condiciones de manejo que optimicen el filtrado se caracterizó el comportamiento hidráulico del picón y su capacidad de eliminar sustancias. Utilizando tres columnas rellenas de picón y un efluente de rumiantes, las reducciones de la DQO, DBO5 y amonio, fósforo y SS superaron el 80, 90% y 95% respectivamente, obteniéndose valores asumibles para inyectarse al riego.
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Der erste Teil der vorliegenden Arbeit beschäftigt sich mit der Modifikation der spontanen Emission im Strong Coupling Regime. Hierzu wurden geeignete optische, organische 'Halbleiter'-Mikroresonatoren präpariert.Zunächst wurde das verwendete optisch aktive Material, das J-Aggregat PIC, spektroskopisch charakterisiert. In Transmissionsmessungen an den Mikroresonatoren wurden Vakuum-Rabi-Splitting-Energien zwischen 26 und 52 meV bestimmt. Es wurde die Abhängigkeit der Vakuum-Rabi-Splitting-Energie von der räumlichen Position der optisch aktiven Schicht innerhalb des Mikroresonators untersucht. Durch eine Simulation konnte nachgewiesen werden, daß der Grund für die Asymmetrie des Rabi-Splittings bei einer Verstimmung von 0 meV durch die Asymmetrie des Absorptionsspektrums des optisch aktiven Materials gegeben ist. Weiterhin wurde die Photolumineszenz der Mikroresonatoren untersucht. Es konnte in temperaturabhängigen Messungen gezeigt werden, daß die hochenergetische Bande gegenüber der niederenergetischen Bande bei steigender Temperatur entsprechend einer Boltzmann-Verteilung stärker besetzt wird.Im zweiten Teil der Arbeit wurden die optischen Eigenschaften von dünnen Filmen N´N´Bis (2,6-xylyl)perylene-3,4:9,10-bis(dicarboximide) (DPP-PTCDI) abhängig von der Schichtdicke untersucht. Die Photolumineszenzspektren der dünnen Filme wurden mit zunehmender Dicke durch eine neue Bande bei kleineren Energien bestimmt. Diese Bande kann mit der Emission aus Fallenzuständen erklärt werden. Durch Photolumineszenz-Anregungsspektroskopie konnte gezeigt werden, daß die Fallenzustände auch im Grundzustand existieren. Exzimere können daher als Ursache ausgeschlossen werden.
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The challenge of the present work was to synthesize and to characterize new classes of N-containing polymers via palladium-catalyzed aryl amination. This work was inspired by a desire to combine the properties of high-performance polymers such as PEKs with those of N-containing conductive polymers such as polyaniline (PANI), poly(aromatic amides) (PAAs), and the ready synthesis of N-containing simple aromatic compound by the Buchwald-Hartwig reaction. Careful investigation of a model reaction was carried out to provide insights into the formation of side products which will have a negative effect upon the molecular weight or upon the materials properties of the desired polymers in the polycondensation reaction. In this thesis, five new different polymer classes namely, poly(imino ketone)s (PIKs), poly(imino acridine)s (PIAcs), poly(imino azobenzene)s (PIAzos), poly(imino fluorenone)s (PIFOs), and poly(imino carbazole)s (PICs) were synthesized and fully characterized by means of 1H-NMR, elemental analysis, UV, FT-IR, X-ray, GPC, TGA, DSC, DMA, and dielectric spectroscopy. To optimize the polycondensation process, the influence of the concentration, temperature, ligands and the reactivity of the halogen containing monomers were investigated. A temperature of 100-165 °C and a concentration of 30-36 % were found to be optimal for the palladium-catalyzed polycondensation to produce polymer with high molecular weight (Mn = 85 900, Mw = 474 500, DP = 126). Four different ligands were used successfully in the Pd-catalyzed process, of which the Pd/BINAP system was found to be the most effective catalyst, producing the highest yield and highest molecular weight polymers. It was found that the reactivity decreases strongly with increasing electronegativity of the halogen atoms, for example better yields, and higher molecular weights were obtained by using dibromo compounds than dichloro compounds while difluoro compounds were totally unreactive. Polymer analogous transformations, such as the protonation reaction of the ring nitrogens in PIAcs, or of the azobenzene groups of PIAzos, the photo and thermal cis-trans-isomerization of PIAzos, and of poly(imino alcohol)s were also studied. The values of the dielectric constants of PIKs at 1 MHz were in the range 2.71-3.08. These low values of the dielectric constant are lower than that of "H Film", a polyimide Kapton film which is one of the most preferred high-performance dielectrics in microelectronic applications having a dielectric constant of 3.5. In addition to the low values of the dielectric constants, PIKs have lower and glass transition temperatures (Tgs) than arimides such as Kapton which may make them more easily processable. Cyclic voltammetry showed that PICs exhibited low oxidation and reduction potentials and their values were shifted to low values with increasing degree of polymerization i.e. with increasing of the carbazole content in backbone of PICs (PIC-7, 0.44, 0.33 V, DP= 37, PIC-5, 0.63, 0.46, DP= 16, respectively).
Resumo:
The laser driven ion acceleration is a burgeoning field of resarch and is attracting a growing number of scientists since the first results reported in 2000 obtained irradiating thin solid foils by high power laser pulses. The growing interest is driven by the peculiar characteristics of the produced bunches, the compactness of the whole accelerating system and the very short accelerating length of this all-optical accelerators. A fervent theoretical and experimental work has been done since then. An important part of the theoretical study is done by means of numerical simulations and the most widely used technique exploits PIC codes (“Particle In Cell'”). In this thesis the PIC code AlaDyn, developed by our research group considering innovative algorithms, is described. My work has been devoted to the developement of the code and the investigation of the laser driven ion acceleration for different target configurations. Two target configurations for the proton acceleration are presented together with the results of the 2D and 3D numerical investigation. One target configuration consists of a solid foil with a low density layer attached on the irradiated side. The nearly critical plasma of the foam layer allows a very high energy absorption by the target and an increase of the proton energy up to a factor 3, when compared to the ``pure'' TNSA configuration. The differences of the regime with respect to the standard TNSA are described The case of nearly critical density targets has been investigated with 3D simulations. In this case the laser travels throughout the plasma and exits on the rear side. During the propagation, the laser drills a channel and induce a magnetic vortex that expanding on the rear side of the targer is source of a very intense electric field. The protons of the plasma are strongly accelerated up to energies of 100 MeV using a 200PW laser.
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In questa tesi viene illustrato il progetto di un sistema di controllo per uno shaker elettrodinamico. L'architettura è basata su sistemi a microcontrollore Microchip PIC e implementa un controllo in retroazione al fine di ottenere una elevata precisione nell'ampiezza dell'oscillazione. Un prototipo del sistema è stato implementato con componenti commerciali. Vengono presentati i risultati del test funzionale dei sotto-circuiti realizzati.
Resumo:
Nach den Ergebnissen der vorliegenden Arbeit ist eine biologische Bekämpfung von Kleider- und Pelzmotten durch die gezielte Freilassungen von parasitoiden Hymenopteren als deren natürliche Gegenspieler möglich. Es wurden erstmalig ausführliche Versuche zur Parasitierung der Kleider- und Pelzmotte, insbesondere durch Eiaparasitoide der Gattung Trichogramma, durchgeführt. Für die braconide Schlupfwespe Apanteles carpatus wurde eine Zucht- und Freilassungsmethode entwickelt. Sie kann nun als neuer Nützlinge gegen textilschädigende Mottenlarven eingesetzt werden. Eine natürliche Parasitierung textilschädigender Motten durch Eiparasitoide ist bislang nicht nachgewiesen worden. Die Tineiden erwiesen sich im Laborversuch für Trichogramma als gut geeignete Wirte. Hinsichtlich der praktischen Anwendung von Eiparasitoiden der Gattung Trichogramma konnte aus einer Auswahl von 29 Arten und Stämmen aus einer Laborzucht mit T. piceum (Stamm: PIC M 91) eine besonders geeignete Art selektiert werden. Dieser Stamm zeigte die höchste Parasitierungsrate mit über 80 Eiern bei Temperaturen von 20-25°C und einer Lebensdauer von bis zu 17 Tagen. Im Präferenztest wurden sowohl Eier der Kleidermotte als auch der Getreidemotte, dem Massenzuchtwirt, von allen Stämmen mit Abstand am besten parasitiert. Das Geschlechterverhältnis von T. piceum lag bei über 80%. Der untersuchte Stamm von Apanteles carpatus zeigte bei 25°C eine durchschnittliche Nachkommenzahl von 55 pro Weibchen. Die Parasitoide erreichten jedoch nur unter optimalen Bedingungen eine Lebensdauer von bis zu 14 Tagen. In den Käfigversuchen ohne zusätzliche Nahrungsquellen wurden die Tiere nicht älter als 4 Tage. Es war nicht möglich, für A. carpatus Ersatzwirte für eine Massenzucht zu finden, da sie offensichtlich auf Tineiden spezialisiert sind, jedoch konnte ein Zuchtsystem mit Kleidermotten als Zuchtwirte etabliert werden. Die ausgewählten Trichogramma-Arten wurden in Käfigversuchen ausführlich untersucht und im Hinblick auf ihre Suchleistung auf verschiedenen Stoffoberflächen geprüft. Es wurde festgestellt, dass die getesteten Arten sehr unterschiedlich geeignet sind, um Textilien nach Eiern abzusuchen. Die Arten T. evanescens (Stamm: Lager) und T. piceum (PIC M 91) erwiesen sich als in der Suchleistung als am besten geeignet. Im Vergleich dazu zeigte T. cacoeciae (CAC D 90 O) sehr wenig Suchleistugsvermögen auf Textilien. Die geeigneten Arten durchdrangen außer verschiedenen Textilien auch grobe Schafwolle bis zu 0,4 m vom Freilassungsort. Das Ködern von Larvalparasitoiden von tineiden Motten im Freiland erwies sich als nicht erfolgreich. Trotzdem in der Literatur eine Reihe parasitoider Hymenopteren als Gegenspieler von Tineiden beschrieben sind und in Innenräumen beobachtet wurden, war es nicht möglich, weitere freilebende Arten zu ködern. Sowohl für das Ködern im Freiland als auch für die Rückköderung in Lagern wurden Ködermethoden getestet und optimiert. Nebenwirkungstests haben ergeben, dass die Nützlinge ergänzend zum Einsatz von Niem-Präparaten an schlecht zugänglichen Befallsstellen eingesetzt werden können. Ebenso wurde ermittelt, dass eine Kombination des Nützlingseinsatzes mit Repellents möglich ist. Bei zu hoher Konzentration der Wirkstoffe, den reinen Niem-Öl und konzentriertem Lavendel-Öl, in geschlossenen Glaskäfigen, wurden starke Nebenwirkungen auf Trichogramma festgestellt. In größerem Raumvolumen oder geringerer Dosierung der Wirkstoffe parasitierte Trichogramma allerdings auch Ködereier, die sich auf Niem-behandeltem Stoff befanden. Erste Freilassungsversuche in der Praxis ergaben unterschiedliche Erfolge. Nach einer Freilassung von Apanteles carpatus in einem Wohnhaus, das mit Schafwolle gedämmt wurde, reduzierte sich Fang von adulten Motten auf Pheromon-Klebfallen deutlich. In einem Textillager hingegen war es mit einer einmaligen Freilassung jedoch nicht möglich, die Gegenspieler zu etablieren und den Mottenbefall zu kontrollieren. Die mehrwöchige Freilassung von Trichogramma in einem Textillager konnte dazu beitragen, einen Pelzmottenbefall zu reduzieren. Hier zeigten sich Möglichkeiten und Grenzen des Einsatzes von parasitoiden Schlupfwespen gegen Textilmotten gleichermaßen.
Resumo:
In this report a new automated optical test for next generation of photonic integrated circuits (PICs) is provided by the test-bed design and assessment. After a briefly analysis of critical problems of actual optical tests, the main test features are defined: automation and flexibility, relaxed alignment procedure, speed up of entire test and data reliability. After studying varied solutions, the test-bed components are defined to be lens array, photo-detector array, and software controller. Each device is studied and calibrated, the spatial resolution, and reliability against interference at the photo-detector array are studied. The software is programmed in order to manage both PIC input, and photo-detector array output as well as data analysis. The test is validated by analysing state-of-art 16 ports PIC: the waveguide location, current versus power, and time-spatial power distribution are measured as well as the optical continuity of an entire path of PIC. Complexity, alignment tolerance, time of measurement are also discussed.
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This dissertation deals with the design and the characterization of novel reconfigurable silicon-on-insulator (SOI) devices to filter and route optical signals on-chip. Design is carried out through circuit simulations based on basic circuit elements (Building Blocks, BBs) in order to prove the feasibility of an approach allowing to move the design of Photonic Integrated Circuits (PICs) toward the system level. CMOS compatibility and large integration scale make SOI one of the most promising material to realize PICs. The concepts of generic foundry and BB based circuit simulations for the design are emerging as a solution to reduce the costs and increase the circuit complexity. To validate the BB based approach, the development of some of the most important BBs is performed first. A novel tunable coupler is also presented and it is demonstrated to be a valuable alternative to the known solutions. Two novel multi-element PICs are then analysed: a narrow linewidth single mode resonator and a passband filter with widely tunable bandwidth. Extensive circuit simulations are carried out to determine their performance, taking into account fabrication tolerances. The first PIC is based on two Grating Assisted Couplers in a ring resonator (RR) configuration. It is shown that a trade-off between performance, resonance bandwidth and device footprint has to be performed. The device could be employed to realize reconfigurable add-drop de/multiplexers. Sensitivity with respect to fabrication tolerances and spurious effects is however observed. The second PIC is based on an unbalanced Mach-Zehnder interferometer loaded with two RRs. Overall good performance and robustness to fabrication tolerances and nonlinear effects have confirmed its applicability for the realization of flexible optical systems. Simulated and measured devices behaviour is shown to be in agreement thus demonstrating the viability of a BB based approach to the design of complex PICs.
Resumo:
La tesi tratta il progetto di una piattaforma di simulazione per modulazioni back-scatter UWB su un sistema a microcontrollore PIC. Il sistema utilizza uno switch a UWB per eseguire la modulazione, modificando le condizioni di carico d'antenna; il software implementa la modulazione attraverso la variazione del segnale di controllo dello switch e si interfaccia con l'utente attraverso l'uso di una periferica USB, permettendo la modifica runtime della configurazione. Si interfaccia inoltre con strumenti esterni attraverso segnali di sincronizzazione.
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Theories and numerical modeling are fundamental tools for understanding, optimizing and designing present and future laser-plasma accelerators (LPAs). Laser evolution and plasma wave excitation in a LPA driven by a weakly relativistically intense, short-pulse laser propagating in a preformed parabolic plasma channel, is studied analytically in 3D including the effects of pulse steepening and energy depletion. At higher laser intensities, the process of electron self-injection in the nonlinear bubble wake regime is studied by means of fully self-consistent Particle-in-Cell simulations. Considering a non-evolving laser driver propagating with a prescribed velocity, the geometrical properties of the non-evolving bubble wake are studied. For a range of parameters of interest for laser plasma acceleration, The dependence of the threshold for self-injection in the non-evolving wake on laser intensity and wake velocity is characterized. Due to the nonlinear and complex nature of the Physics involved, computationally challenging numerical simulations are required to model laser-plasma accelerators operating at relativistic laser intensities. The numerical and computational optimizations, that combined in the codes INF&RNO and INF&RNO/quasi-static give the possibility to accurately model multi-GeV laser wakefield acceleration stages with present supercomputing architectures, are discussed. The PIC code jasmine, capable of efficiently running laser-plasma simulations on Graphics Processing Units (GPUs) clusters, is presented. GPUs deliver exceptional performance to PIC codes, but the core algorithms had to be redesigned for satisfying the constraints imposed by the intrinsic parallelism of the architecture. The simulation campaigns, run with the code jasmine for modeling the recent LPA experiments with the INFN-FLAME and CNR-ILIL laser systems, are also presented.
Resumo:
Argomento di questo lavoro di tesi è l’accelerazione di ioni tramite interazione laser-plasma. Nel particolare, uno studio teorico sui principali meccanismi di accelerazione e una campagna di simulazioni numeriche volte ad analizzare gli effetti sullo spettro energetico dei protoni accelerati dovuti al preplasma sono stati svolti. Quando laser ad impulsi brevi, ad alta intensità e a contrasto finito, interagiscono con un campione solido è presente un preimpulso che causa la formazione di una regione di preplasma antistante il bersaglio che può rendere più efficace l’accelerazione dei protoni. Vengono dunque introdotti nel primo capitolo i concetti e le tecniche base per studiare a livello teorico e numericamente le interazioni laser-plasma. Nel secondo capitolo sono trattati analiticamente alcuni meccanismi di accelerazione di ioni. Nel terzo ed ultimo capitolo vengono descritti gli effetti di preplasma ed esposti risultati di simulazioni PIC volte a trovare i parametri ottimali per ottenere ioni più energetici.