994 resultados para Ar lasers


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Many organic molecules have strong absorption bands which can be accessed by ultraviolet short pulse lasers to produce efficient ionization. This resonant multiphoton ionization scheme has already been exploited as an ionization source in time-of-flight mass spectrometers used for environmental trace analysis. In the present work we quantify the ultimate potential of this technique by measuring absolute ion yields produced from the interaction of 267 nm femtosecond laser pulses with the organic molecules indole and toluene, and gases Xe, N2 and O2. Using multiphoton ionization cross sections extracted from these results, we show that the laser pulse parameters required for real-time detection of aromatic molecules at concentrations of one part per trillion in air and a limit of detection of a few attomoles are achievable with presently available commercial laser systems. The potential applications for the analysis of human breath, blood and tissue samples are discussed.

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The production of neutron beams having short temporal duration is studied using ultraintense laser pulses. Laser-accelerated protons are spectrally filtered using a laser-triggered microlens to produce a short duration neutron pulse via nuclear reactions induced in a converter material (LiF). This produces a similar to 3 ns duration neutron pulse with 10(4) n/MeV/sr/shot at 0.56 m from the laser-irradiated proton source. The large spatial separation between the neutron production and the proton source allows for shielding from the copious and undesirable radiation resulting from the laser-plasma interaction. This neutron pulse compares favorably to the duration of conventional accelerator sources and should scale up with, present and future, higher energy laser facilities to produce brighter and shorter neutron beams for ultrafast probing of dense materials.

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<p>Castrate-resistant prostate cancer (CRPC) is poorly characterized and heterogeneous and while the androgen receptor (AR) is of singular importance, other factors such as c-Myc and the E2F family also play a role in later stage disease. HES6 is a transcription co-factor associated with stem cell characteristics in neural tissue. Here we show that HES6 is up-regulated in aggressive human prostate cancer and drives castration-resistant tumour growth in the absence of ligand binding by enhancing the transcriptional activity of the AR, which is preferentially directed to a regulatory network enriched for transcription factors such as E2F1. In the clinical setting, we have uncovered a HES6-associated signature that predicts poor outcome in prostate cancer, which can be pharmacologically targeted by inhibition of PLK1 with restoration of sensitivity to castration. We have therefore shown for the first time the critical role of HES6 in the development of CRPC and identified its potential in patient-specific therapeutic strategies.</p>

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A scheme for enhanced quantum electrodynamics (QED) production of electron-positron-pair plasmas is proposed that uses two ultraintense lasers irradiating a thin solid foil from opposite sides. In the scheme, under a proper matching condition, in addition to the skin-depth emission of gamma-ray photons and Breit-Wheeler creation of pairs on each side of the foil, a large number of high-energy electrons and photons from one side can propagate through it and interact with the laser on the other side, leading to much enhanced gamma-ray emission and pair production. More importantly, the created pairs can be collected later and confined to the center by opposite laser radiation pressures when the foil becomes transparent, resulting in the formation of unprecedentedly overdense and high-energy pair plasmas. Two-dimensional QED particle-in-cell simulations show that electron-positron-pair plasmas with overcritical density 10(22) cm(-3) and a high energy of 100s of MeV are obtained with 10 PW lasers at intensities 10(23) W/cm(2), which are of key significance for laboratory astrophysics studies.

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The advent of high-power laser facilities has, in the past two decades, opened a new field of research where astrophysical environments can be scaled down to laboratory dimensions, while preserving the essential physics. This is due to the invariance of the equations of magneto-hydrodynamics to a class of similarity transformations. Here we review the relevant scaling relations and their application in laboratory astrophysics experiments with a focus on the generation and amplification of magnetic fields in cosmic environment. The standard model for the origin of magnetic fields is a multi stage process whereby a vanishing magnetic seed is first generated by a rotational electric field and is then amplified by turbulent dynamo action to the characteristic values observed in astronomical bodies. We thus discuss the relevant seed generation mechanisms in cosmic environment including resistive mechanism, collision-less and fluid instabilities, as well as novel laboratory experiments using high power laser systems aimed at investigating the amplification of magnetic energy by magneto-hydrodynamic (MHD) turbulence. Future directions, including efforts to model in the laboratory the process of diffusive shock acceleration are also discussed, with an emphasis on the potential of laboratory experiments to further our understanding of plasma physics on cosmic scales.

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Electron-impact scattering data for argon and its ions continue to be of interest in studies of magnetically confined plasmas. In an earlier paper, Griffin et al (1997 J. Phys. B: At. Mol. Opt. Phys. 30 3543) employed the results of 28-term and 40-term R-matrix calculations of electron-impact excitation in Ar+ to carry out a collisional-radiative modelling study of the impurity influx of argon in tokamaks. We have now completed a 452-term R-matrix with pseudo-states (RMPS) calculation of electron-impact excitation for Ar+ in order to provide more accurate excitation data; using these improved data, we have repeated the modelling studies presented in the earlier paper. We compare our excitation data, as well as the results of the collisional radiative calculations, with those arising from the 40-term R-matrix calculation and find significant differences.

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Context: Emission from Ar III is seen in planetary nebulae, in H II regions, and from laboratory plasmas. The analysis of such spectra requires accurate electron impact excitation data. Aims: The aim of this work is to improve the electron impact excitation data available for Ar2+, for application in studies of planetary nebulae and laboratory plasma spectra. The effects of the new data on diagnostic line ratios are also studied. Methods: Electron-impact excitation collision strengths have been calculated using the R-Matrix Intermediate-Coupling Frame-Transformation method and the R-Matrix Breit-Pauli method. Excitation cross sections are calculated between all levels of the configurations 3s^23p^4, 3s3p^5, 3p^6, 3p^53d, and 3s^23p^3nl (3d nl 5s). Maxwellian effective collision strengths are generated from the collision strength data. Results: Good agreement is found in the collision strengths calculated using the two R-Matrix methods. The collision strengths are compared with literature values for transitions within the 3s^23p4 configuration. The new data has a small effect on Te values obtained from the I(7135 + 7751 )/ I(5192 ) line ratio, and a larger effect on the Ne values obtained from the I(7135 )/I(9 m) line ratio. The final effective collision strength data is archived online.

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Absolute cross-section measurements for valence-shell photoionization of Ar + ions are reported for photon energies ranging from 27.4 eV to 60.0 eV. The data, taken by merging beams of ions and synchrotron radiation at a photon energy resolution of 10 meV, indicate that the primary ion beam was a statistically weighted mixture of the 2P o3/2 ground state and the 2P o1/2 metastable state of Ar +. Photoionization of this Cell-like ion is characterized by multiple Rydberg series of autoionizing resonances superimposed on a direct photoionization continuum. Observed resonance lineshapes indicate interference between indirect and direct photoionization channels. Resonance features are spectroscopically assigned and their energies and quantum defects are tabulated. The measurements are satisfactorily reproduced by theoretical calculations based on an intermediate coupling semi-relativistic Breit-Pauli approximation.

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<p>The multichannel R-matrix method is used to compute electron impact excitation collision strengths in Ar IV for all fine-structure transitions among the <sup>4</sup>S, <sup>2</sup>D and <sup>2</sup>P levels in the 3s <sup>2</sup>3p <sup>3</sup> ground configuration. Included in the expansion of the total wavefunction are the lowest 13 LS target eigenstates of Ar iv formed from the 3s <sup>2</sup>3p <sup>3</sup>, 3s3p <sup>4</sup> and 3s <sup>2</sup>3p <sup>2</sup>3d configurations. The effective collision strengths, obtained by averaging the electron collision strengths over a Maxwellian distribution of electron velocities, are presented for all 10 fine-structure transitions over a wide range of electron temperatures of astrophysical interest (T <sub>e</sub> = 2000-100 000 K). Comparisons are made with an earlier 7-state close-coupling calculation by Zeippen, Butler &amp; Le Bourlot, and significant differences are found to occur for many of the forbidden transitions considered, in particular those involving the <sup>4</sup>S ground state, where discrepancies of up to a factor of 3 are found in the low-temperature region. 1997 RAS.</p>

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O benzeno foi o primeiro poluente atmosfrico carcinognico a ser regulamentado a nvel europeu. Vrios trabalhos tm sido publicados demonstrando a relao deste poluente com diversos tipos de neoplasias nomeadamente decorrentes de exposies a nvel ocupacional. Porm, o estudo deste poluente para concentraes atmosfricas em ambientes exteriores ainda pouco conhecido e est em clara evoluo. Neste sentido, este trabalho pretende ser um contributo para o conhecimento da relao entre o benzeno atmosfrico e a incidncia de patologias que afectam os tecidos linfticos e rgos hematopoiticos nomeadamente linfomas de Hodgkin, linfomas de no-Hodgkin e leucemias na populao residente na rea Metropolitana do Porto. Dado a quase ausncia de dados de monitorizao das concentraes de benzeno atmosfrico actualmente em Portugal, estas foram estimadas com base na definio de uma relao entre o benzeno e o monxido de carbono. O conhecimento das concentraes em todo o domnio de estudo baseou-se na anlise dos dados da Rede Automtica de Monitorizao da Qualidade do Ar porm, de modo a aumentar o detalhe espacial e temporal recorreu-se modelao atmosfrica aplicando o modelo TAPM. Para perceber a evoluo temporal das concentraes, a modelao foi efectuada para os anos de 1991, 2001 e 2006 com base no ano meteorolgico de 2006 e emisses para os respectivos anos ao nvel da freguesia. O modelo foi previamente validado de acordo com uma metodologia proposta para este tipo de modelos. Contudo, mais do que perceber qual a variao da qualidade do ar a nvel exterior, importante conhecer o impacte de fontes interiores e o seu efeito na populao. Assim, desenvolveu-se um modelo de exposio e dose que permitem conhecer os valores mdios populacionais. A modelao da exposio populacional efectuada com base nos perfis de actividade-tempo, nos movimentos pendulares inter-concelhos e nas concentraes de benzeno em ambientes exteriores e interiores. Na modelao da dose ainda possvel variaes por sexo e idade. Por outro lado, para o estudo das patologias em anlise efectuou-se uma anlise epidemiolgica espacial nomeadamente no que respeita elaborao de mapas de incidncia padronizados pela idade, e estudo da associao com a exposio ao benzeno atmosfrico. Os resultados indicam associao entre o benzeno e as doenas em estudo. Esta evidncia mais notria quando a anlise realizada junto s principais fontes de emisso deste poluente, vias de trfego e postos de abastecimento de combustvel. Porm, a ausncia de informao limita o estudo no permitindo o controlo de potenciais variveis de confundimento como a exposio ao fumo do tabaco. A metodologia permite efectuar uma gesto integrada da qualidade do ar exterior e interior, funcionando como uma ferramenta do apoio deciso para elaborao de planos de preveno de longo prazo de potenciais efeitos na sade das populaes nomeadamente para outro tipo de patologias.

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O actual, e crescente, padro de consumo tem repercusses no ambiente que, inevitavelmente, se reflectem na sade humana. A poluio atmosfrica assume-se, na Europa, como um problema ambiental premente, por ter um elevado impacte na sade dos cidados. Entre estes, h grupos particularmente vulnerveis, como os idosos, os doentes crnicos e as crianas. Vrios estudos colocam em evidncia a sensibilidade dos doentes asmticos, em particular das crianas, poluio atmosfrica. No entanto, permanece por esclarecer o facto de a poluio atmosfrica poder causar o aumento da prevalncia desta doena, assim como a identificao dos principais poluentes atmosfricos responsveis e os nveis de exposio seguros. O objectivo desta tese consiste no estudo da relao entre a poluio atmosfrica e a sade, contribuindo para o conhecimento nesta temtica atravs do desenvolvimento de uma ferramenta e da sua aplicao a um caso de estudo concreto. Neste caso de estudo analisou-se a relao entre vrios poluentes atmosfricos e o agravamento da sintomatologia em crianas asmticas. Neste mbito, foi desenvolvido o modelo doseAr, que possibilita o clculo da exposio e da dose inalada, ao nvel individual, de poluentes atmosfricos. Os resultados da aplicao do doseAr permitem a identificao dos microambientes onde a contribuio para a exposio e dose inalada de poluentes mais relevante. Os microambientes interiores, em particular aqueles onde desenvolvida actividade fsica exigente, so identificados como especialmente importantes. A relao entre a exposio e a dose inalada claramente associada ao agravamento da asma nestas crianas, apesar dos nveis de poluio identificados serem baixos, face aos padres de qualidade do ar existentes.

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Dissertao de mest, Tecnologia de Alimentos, Instituto Superior de Engenharia, Univ. do Algarve, 2013

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A presena de cianobactrias em reservatrios utilizados para produo de gua para consumo humano representa um elevado risco para a sade pblica. Estes organismos contribuem para a reduo da qualidade da gua e tm a capacidade de produzir cianotoxinas que podem afectar a sade humana e animal. Existem casos em todo o mundo de intoxicao letal de diversos animais por consumo de gua de lagos contaminados com cianobactrias, e mesmo casos de morte de humanos, atribudas exposio de cianotoxinas. De modo a fazer face a este crescente problema necessrio desenvolver e implementar tecnologias de tratamento de gua nas ETA que permitam fazer face a uma florescncia de cianobactrias num reservatrio de gua destinado ao abastecimento humano. Neste trabalho avaliou-se a capacidade do processo C/F/DAF na remoo cianobactrias de diferentes morfologias, clulas e colnias de M. aeruginosa e filamentos de P. rubescens, em guas sintticas hidrofbicas e hidroflicas, com concentrao de DOC moderada e moderada/elevada. Assim como da sequncia C/F/DAFNF na remoo de clulas e de toxinas de cianobactrias. A remoo de NOM e o seu efeito na remoo de cianobactrias foram tambm avaliados. Concluiu-se que o processo C/F/DAF eficiente na remoo de cianobactrias de diferentes morfologias, com remoes entre 78 e 100% de MC intra. No entanto, a morfologia que apresentou remoes mais elevadas foram os filamentos, enquanto as colnias apresentaram valores mais baixos. Globalmente, verificou-se que o aumento da concentrao de NOM facilita a remoo de cianobactrias, sendo que as guas hidrofbicas apresentaram-se mais fceis de tratar por C/F/DAF. Por sua vez, o tratamento C/F/DAFNF, uma opo eficiente para fazer face a um eventual bloom de cianobactrias em ETA, uma vez que a remoo de cianobactrias (em MC intra e chl_a) foi de 100% e a remoo de microcistina extracelular de 95%, aproximadamente.

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Dissertao de mestrado, Hortofruticultura, Faculdade de Cincias e Tecnologia, Universidade do Algarve, 2014