A evolução do lítio em estrelas do tipo-solar através do diagrama HR

Important advances have been made along the last decade in the study of the lithium behavior in solar-type stars. Among the most important discoveries what attracts attention is that the distribution of lithium abundance in the late F-type giant stars tends to be discontinuous, at the same time of a sudden decline in rotation and a gradual decline according to the temperature for giant red stars of such spectral type. Other studies have also shown that synchronized binary systems with evolved components seem to keep more of their original lithium than the unsynchronized systems. evertheless, the connection between rotation and lithium abundance as well as the role of tidal effects on lithium dilution seem to be more complicated matters, depending on mass, metallicity and age. This work brings an unprecedented study about the behavior of lithium abundance in solartype evolved stars based on an unique sample of 1067 subgiant, giant and supergiant stars, 236 of them presenting spectroscopic binary characteristics, with precise lithium abundance and projected rotational speed. Now the lithium-rotation connection for single and binary evolved stars is analyzed taking into account the role of mass and stellar age

Lítio e rotação nas estrelas análogas solares: análise teórica das observações

The projected rotational velocity together with lithium abundance and the onset of the dilution by the deepening in mass of the convective envelope provide a key tool to investigate the so far poorly understood processes at work in stellar interiors of solar-analog stars. To investigate the link between abundances, convection and rotational velocities in solar-analog G dwarf stars, we study a bona fide sample of 118 selected solar-analog G dwarf stars presenting measured lithium abundances, rotational velocities, and fundamental parameters together with computed evolutionary tracks (Toulouse-Geneva code) for a range of stellar masses around 1 M and metallicity consistent with the solar-analog range. The aim of this work is to build up an evolution of lithium and rotation as a function of stellar age, mass, effective temperature, and convection. We analyze the evolutionary status of the sample of 118 solar-analog G dwarf in the HR diagram based on Hipparcos data and using a grid of stellar models in the effective temperature and mass range of the solar-analog stars. We discuss the deepening (in mass) of the convective envelope and the influence on the Li abundances and projected rotational velocities. We determined the stellar mass and the mass of the convective envelope for a bona fide sample of 118 selected solar-analog G dwarf and checked the evolutionary link between the rotational velocity, lithium abundance, and the deepening of the convective envelope. Fast rotators (vsini 6 km s��1) are also stars with high Li content. Slow rotators present a wide range of values of log n(Li). Our results shed new light on the lithium and rotational behavior in G dwarf stars. We confirmed the presence of a large Li abundance spread among the solar-analog stars and concluded that the solar twins probably share a similar mixing history with the Sun

Evolução da atividade cromosférica, abundância de lítio e rotação das estrelas análogas e gêmeas solares

The study of solar-type stars also includes the familiar solar analogs and twins. These objects have been one of the major research subjects in astrophysics nowadays. A direct comparison of solar activity with chromospheric activity indices for a set of stars very similar to the Sun (twins and analogs) provides an excellent opportunity to study the evolution of stellar activity on timescales of the order of the lifetime on the main sequence. This work deals with the relationship between the abundance of lithium, chromospheric activity, X-ray emission and rotation period in terms of stellar ages. We explore the influence of stellar evolution in the global properties of the stars and the aspects linked to its coronal, chromospheric and magnetic activity. Our main objective is to probe the law of decay of each of these parameters based on a sample of stars classified as well-connected as analogs stars and solar twins.

Evolução hidrogeoquímica das águas sulfúreas de Entre-os-Rios: avaliação preliminar

O principal objectivo desta dissertação foi avaliar a evolução hidrogeoquímica das águas minerais de Entre‐os‐Rios, para uma melhor compreensão do modelo hidrogeológico conceptual deste sistema hidromineral. Desta forma, foram coligidos diversos dados hidroquímicos, quer das nascentes clássicas (Torre, Curveira, Ardias, Arcos Esquerda e Arcos Direita), quer do furo Barbeitos. Foram compiladas e analisadas oitenta análises hidroquímicas no período 1938‐2012, incluindo características organolépticas (cheiro, cor e turbidez), diversas propriedades físico-químicas (temperatura, pH, condutividade eléctrica, sulfuração, etc), os principais catiões e aniões (bicarbonato, fluoreto, sódio, lítio, etc) e os elementos vestigiários (chumbo, tungsténio, boro, etc). Além disso, foram integrados os dados históricos disponíveis de finais do século XIX e inícios do século XX. Foram igualmente reunidos e discutidos alguns dados isotópicos (oxigénio‐18, deutério e trítio). O recurso hidromineral de Entre‐os‐Rios está condicionado pela litologia e pelas condições tectónicas. As análises químicas revelaram que as águas minerais de Entre‐os‐Rios apresentam uma estabilidade química nos últimos 100 anos. Estas águas são orto‐ a hipertermais, fracamente mineralizadas, de reacção alcalina, sulfídricas, bicarbonatadas sódicas, carbonatadas e muito fluoretadas. Estas características são claramente distintas das águas normais da região. As águas de Entre‐os‐Rios são muito semelhantes às águas minerais de S. Vicente e, em diversos parâmetros, bastante diferentes das águas minerais das Caldas da Saúde. Os dados isotópicos permitiram concluir que as águas de Entre‐os‐Rios têm uma origem meteórica, com um tempo de residência longo no sistema aquífero, e que são, muito provavelmente, submodernas, com uma recarga anterior a 1952. Na região de Entre‐os‐Rios coexistem três sistemas aquíferos, um sistema granítico superficial, livre e um sistema livre a semi‐confinado, ambos com circulação de águas normais, e um sistema aquífero granítico, profundo, confinado, com circulação de água mineral.

Lítio e parâmetros orbitais em sistemas binários com componentes evoluídas

One of the best established properties of the single late type evolved stars is that their rotational velocity and lithium content decrease with effective temperature and age. Nevertheless, the root cause of this property, as well as the link between rotation and lithium abundance and, in particular, the effects of binarity on rotation and lithium content in binary systems with evolved component, are not yet completely established. How does the gravitational tides, in binary systems, affects rotational evolution and lithium dilution? Trying to answer these questions, we have carried out an observational survey, in the lithium region centered at the lithium I line A6707.81A, for a large sample of about 100 binary systems with evolved component along the spectral range F, G and K, with the CES spectrometer mounted at the CAT 1.44 m Telescope of the ESO, La Silla, Chile. By combining the abundances of lithium issued from these observations with rotational velocity and orbital parameters, we have found a number of important results. First of all, we confirm that in this class of binary systems rotation is effectively affected by tidal effects. Binary systems with orbital period lower than about 100 days and circular or nearly circular orbits, present rotational velocity enhanced in relation to the single giant stars and to the binary systems with an orbital period larger than 100 days. This is clearly the result of the synchonization between the rotational and orbital motions due to tidal effects. In addition, we have found that lithium abundances in binary systems with giant components present the same gradual decreasing with effective temperature, observed in the single giants of same luminosity class and spectral types. We have found no lithium-rich binary systems, in contrast with single giants. A remarkable result from the present study is the one showing that synchronized binary systems with giant component retains more of their original lithium than the unsynchronized systems. In fact, we have found a possible "inhibited zone", in which synchronized binary systems with giant component having lithium abundance lower than a threshold level should be unusual. Finally, the present study also shows that the binary systems with giant component presenting the highest lithium contents are those with the highest rotation rates

Um estudo da abundância de lítio, rotação, atividade cromosférica e magnetismo das estrelas análogas e gêmeas solares

The study physical process that control the stellar evolution is strength influenced by several stellar parameters, like as rotational velocity, convective envelope mass deepening, and magnetic field intensity. In this study we analyzed the interconnection of some stellar parameters, as Lithium abundance A(Li), chromospheric activity and magnetic field intensity as well as the variation of these parameters as a function of age, rotational velocity, and the convective envelope mass deepening for a selected sample of solar analogs and twins stars. In particular, we analyzed the convective envelope mass deepening and the dispersion of lithium abundance for these stars. We also studied the evolution of rotation in subgiants stars, because its belong to the following evolutionary stage of solar analogs, and twins stars. For this analyze, we compute evolutionary models with the TGEC code to derive the evolutionary stage, as well as the convective envelope mass deepening, and derive more precisely the stellar mass, and age for this 118 stars. Our Investigation shows a considerable dispersion of lithium abundance for the solar analogs stars. We also realize that this dispersion is not by the convective zone deep, in this way we observed which the scattering of A(Li) can not be explained by classical theories of mixing in the convective zone. In conclusion we have that are necessary extra-mixing process to explain this decrease of Lithium abundance in solar analogs and twins stars. We analyzed the subgiant stars because this are the subsequent evolutionary stage after the solar analogs and twins stars. For this analysis, we compute the rotational period for 30 subgiants stars observed by Co- RoT satellite. For this task we apply two different methods: Lomb-Scargle algorithm, and the Plavchan Periodogram. We apply the TGEC code we compute models with internal distribution of angular momentum to confront the predict results with the models, and the observational results. With this analyze, we showed which solid body rotation models are incompatible with the physical interpretation of observational results. As a result of our study we still concluded that the magnetic field, convective envelope mass deepening, and internal redistribution of angular momentum are essential to explain the evolution of low-mass stars, and its observational characteristics. Based on population synthesis simulation, we concluded that the solar neighborhood presents a considerable quantity of solar twins when compared with the discovered set nowadays. Altogether we foresee the existence around 400 solar analogs in the solar neighborhood (distance of 100 pc). We also study the angular momentum of solar analogs and twins, in this study we concluded that added angular momentum from a Jupiter type planet, putted in the Jupiter position, is not enough to explain the angular momentum predicted by Kraft law (Kraft 1970)

Aglomerado estelar M67: processos de diluição e a evolução do Momentum Angular

Galactic stellar clusters have a great variety of physical properties that make valuable probes of stellar and galactic chemical evolution. Current studies show a discrepancy between the standard evolutionary models and observations, mainly considering the level of mixing and convective dilution of light elements, as well as to the evolution of the angular momentum. In order to better settle some of these properties, we present a detailed spectroscopic analysis of 28 evolved stars, from the turn-off to the RGB, belonging to the stellar open cluster M67. The observations were performed using UVES+FLAMES at VLT/UT2. We determined stellar parameters and metallicity from LTE analysis of Fe I and Fe II lines between 420 1100 nm. The Li abundance was obtained using the line at 6707.78 ˚A, for the whole sample of stars. The Li abundances of evolved stars of M67 present a gradual decreasing when decreasing the effective temperature. The Li dilution factor for giant stars of M67 with Teff ∼ 4350K is at least 2300 times greater than that predicted by standard theory for single field giant stars. The Li abundance as a function of rotation exhibits a good correlation for evolved stars of M67, with a much smaller dispersion than the field evolved stars. The mass and the age seem to be some of the parameters that influence this connection. We discovered a Li-rich subgiant star in M67 (S1242). It is member of a spectroscopic binary system with a high eccentricity. Its Li abundance is 2.7, the highest Li content ever measured for an evolved star in M67. Two possibilities could explain this anomalous Li content: (i) preservation of the Li at the post turn off stage due to tidal effects, or (ii) an efficient dredge-up of Li, hidden below the convective zone by atomic diffusion occurring in the post turn off stage. We also study the evolution of the angular momentum for the evolved stars in M67. The results are in agreement with previous studies dedicated to evolved stars of this cluster, where stars in the same region of the CM-diagram have quite similar rotations, but with values that indicate an extra breaking along the main sequence. Finally, we analize the distributions of the average rotational velocity and of the average Li abundance as a function of age. With relation to the average Li abundances, stars in clusters and field stars present the same type of exponencial decay law t−β. Such decay is observed for ages lesser than 2 Gyr. From this age, is observed that the average Li abundance remain constant, differently of the one observed in the rotation age connection, where the average rotational velocity decreases slowly with age

O enigmático problema das gigantes ricas em Lítio e as perspectivas com o satélite Kepler

Lithium (Li) is a chemical element with atomic number 3 and it is among the lightest known elements in the universe. In general, the Lithium is found in the nature under the form of two stable isotopes, the 6Li and 7Li. This last one is the most dominant and responds for about 93% of the Li found in the Universe. Due to its fragileness this element is largely used in the astrophysics, especially in what refers to the understanding of the physical process that has occurred since the Big Bang going through the evolution of the galaxies and stars. In the primordial nucleosynthesis in the Big Bang moment (BBN), the theoretical calculation forecasts a Li production along with all the light elements such as Deuterium and Beryllium. To the Li the BNB theory reviews a primordial abundance of Log log ǫ(Li) =2.72 dex in a logarithmic scale related to the H. The abundance of Li found on the poor metal stars, or pop II stars type, is called as being the abundance of Li primordial and is the measure as being log ǫ(Li) =2.27 dex. In the ISM (Interstellar medium), that reflects the current value, the abundance of Lithium is log ǫ(Li) = 3.2 dex. This value has great importance for our comprehension on the chemical evolution of the galaxy. The process responsible for the increasing of the primordial value present in the Li is not clearly understood until nowadays. In fact there is a real contribution of Li from the giant stars of little mass and this contribution needs to be well streamed if we want to understand our galaxy. The main objection in this logical sequence is the appearing of some giant stars with little mass of G and K spectral types which atmosphere is highly enriched with Li. Such elevated values are exactly the opposite of what could happen with the typical abundance of giant low mass stars, where convective envelops pass through a mass deepening in which all the Li should be diluted and present abundances around log ǫ(Li) ∼1.4 dex following the model of stellar evolution. In the Literature three suggestions are found that try to reconcile the values of the abundance of Li theoretical and observed in these rich in Li giants, but any of them bring conclusive answers. In the present work, we propose a qualitative study of the evolutionary state of the rich in Li stars in the literature along with the recent discovery of the first star rich in Li observed by the Kepler Satellite. The main objective of this work is to promote a solid discussion about the evolutionary state based on the characteristic obtained from the seismic analysis of the object observed by Kepler. We used evolutionary traces and simulation done with the population synthesis code TRILEGAL intending to evaluate as precisely as possible the evolutionary state of the internal structure of these groups of stars. The results indicate a very short characteristic time when compared to the evolutionary scale related to the enrichment of these stars

Análise espectroscópica da estrela HD 150050: uma nova estrela gigante rica em lítio

Conselho Nacional de Desenvolvimento Científico e Tecnológico

Preparação e caracterização eletroquímica de material catódico do tipo La2/3-xLi3xTiO3 para aplicações em baterias de Lítio

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Sistema de gerenciamento de energia para controle de carga/descarga entre baterias de lítio e ultracapacitores, envolvendo sistema de tração elétrica com frenagem regenerativa

Pós-graduação em Engenharia Elétrica - FEIS

Dissilicato de lítio

De forma a completar as necessidades estéticas, que são cada vez mais exigidas pela sociedade, as cerâmicas dentárias têm apresentado rápida evolução com o intuito de melhorar as suas propriedades físicas e mecânicas, como também óticas. O desenvolvimento de novos materiais permitiu a aplicação e o progresso dos sistemas totalmente cerâmicos utilizados na área da medicina dentária. Pelas suas características estéticas relativamente aos sistemas metalocerâmicos, rapidamente os sistemas totalmente cerâmicos ocuparam o seu lugar no mercado, levando à atenção de médicos dentistas, como dos próprios pacientes. Dentro destes sistemas totalmente cerâmicos, encontra-se a cerâmica reforçada com dissilicato de lítio. Esta revisão narrativa da literatura teve como objetivo descrever as características da cerâmica dissilicato de lítio de forma a tornar possível compreender em que situações clinicas poderá ser utilizada, bem como, de que forma é possível otimizar os processos laboratoriais. Para tal, foram utilizadas várias bases de dados, Pubmed, Scielo, JADA, e Science Direct, utilizando como palavras-chave: “Ceramic”, “Dental Ceramic” “Porcelain”, “Lithium Dissilicate”; “IPS e.max

A lenta evolução da gestão de obras públicas no Brasil

O artigo aborda a problemática da gestão de obras públicas no Brasil, alvo de recorrentes irregularidades apontadas pelos órgãos de controle e pela imprensa nacional. A pesquisa parte do diagnóstico constante do Relatório "O Retrato do Desperdício no Brasil", apresentado em novembro de 1995 pela Comissão Temporária do Senado Federal destinada a inventariar as obras inacabadas custeadas com recursos federais, e busca cotejar os problemas apontados naquele Relatório com as medidas adotadas pelo Governo Federal e pelo Congresso Nacional para aperfeiçoar a gestão de obras públicas. O autor argumenta que as medidas adotadas, conquanto corretas, receberam prioridade, intensidade e abrangência incompatíveis com a magnitude do problema.

O Colégio de Líderes : surgimento e evolução

Discute o funcionamento do Colégio de Líderes e seus efeitos sobre a atividade legislativa da Câmara dos Deputados. Para isso, a pesquisa se baseou em artigos científicos sobre o tema e documentos que demonstram o que motivou a criação do colegiado, como ele se reúne e de que modo ele colabora para a definição da pauta de votações do Plenário. Inclui entrevistas com figuras que participaram ativamente da criação e da evolução do Colégio de Líderes no cenário político. Descreve, ainda, de que forma a sua atuação limita a representatividade parlamentar e que soluções poderiam ser adotadas para amenizar esse conflito, já que, apesar de colaborar para a concentração de poderes no Congresso Nacional, esse órgão se tornou indispensável para a organização e agilidade dos trabalhos legislativos. Para ilustrar como se dá na prática a atuação do colegiado, procedeu-se a uma análise das reuniões realizadas no primeiro período da sessão legislativa ordinária de 2009, tudo com base em dados fornecidos pela Secretaria-Geral da Mesa da Câmara dos Deputados e em notícias da Agência Câmara divulgadas naquele semestre.

Cumprimento das metas fiscais da União em 2008 : evolução da dívida pública : resultado até dezembro

Consultoria de Orçamento e Fiscalização Financeira - Núcleo de Assuntos Econômico-Fiscais.