Arqueologia do baixo Tapajós: ocupação humana na periferia do domínio tapajônico

Essa pesquisa investiga um sítio arqueológico localizado em área que seria o limite sul da dispersão da Tradição Inciso-Ponteada no baixo curso do rio Tapajós, e discute os resultados dessa pesquisa à luz dos demais dados e hipóteses que vêm sendo formulados sobre a ocupação indígena pré-colonial da região. Investigações arqueológicas realizadas na região nos últimos anos vêm revelando que a área de dispersão de sítios arqueológicos ligados a essa tradição cerâmica é maior do que se supunha anteriormente. As características estilísticas da cultura material e o modo de ocupação das paisagens parecem indicar contatos culturais entre habitantes do baixo rio Tapajós e os povos que habitavam as bacias dos rios Nhamundá e Trombetas ao final do primeiro milênio da Era Cristã. Sendo assim, esta pesquisa compreende dois exercícios: (1) o primeiro de escala local, com foco no sítio arqueológico Serraria Trombetas, e no estudo detalhado do espaço intra-sítio, entendido como um microcosmo de uma história regional; e (2) o segundo de escala regional, de comparação dos resultados locais com a cronologia e as características dos demais sítios arqueológico da região. Através da caracterização estilística da cerâmica, do estudo do material lítico, da distribuição espacial dos vestígios no sítio e em nível regional, além do exame da cronologia regional, buscou-se investigar a diversidade cultural dos grupos pré-coloniais no segundo milênio da Era Cristã.

Vêm de Belém e vêm da Grécia! Metamorfoses: fronteiras entre narrativas orais e os mitos

A metamorfose, de acordo com Jean Chevalier e Alan Gheerbrant, é definida neste estudo como a transformação física e/ou comportamental de um ser em outro, sem a perda da identidade e ciência do primeiro ser. Esta transformação é um fenômeno recursivo em diversas mitologias e culturas. O presente trabalho tem por objetivo estabelecer, numa abordagem comparativa, as correlações e diferenças entre o tema da metamorfose recorrente nos mitos gregos relatados por Homero, em sua Odisseia, nos mitos gregos descrevidos pelo poeta latino Publius Ovidius Naso, conhecido como Ovídio, em sua obra Metamorfoses, nos cinco primeiros livros, e entre as narrativas orais que referem casos de metamorfoses ocorridos no município de Belém do Pará, inventariadas no período de 1994 a 2004. Foram consideradas as obras Odisseia e Metamorfoses por serem ambas, respectivamente, expoentes da literatura ocidental de uma Grécia dos séculos VIII a VII a.C e de uma Grécia do século I d.C retratada pelo poeta latino Ovídio, e que carregam o tema da metamorfose. Isto porque o estudo prévio ratifica a formação de índices míticos não somente nas narrativas da mitologia grega, mas também nos casos de metamorfoses oriundos de Belém. Em todo o caso, nota-se a configuração espaço-temporal como entidades que sedimentam e organizam o mundo mítico, articulando tais dimensões a representações no mundo físico-espiritual. O tema da metamorfose, contudo, é conformado de forma diferenciada, conforme o contexto histórico-cultural de cada narrativa, o que é refletido na multiplicidade de símbolos e sentidos perseguidos por cada narrativa. A fim de enriquecer o estudo dos símbolos e do contexto histórico-geográfico dos mitos gregos abordados, utilizam-se como fonte complementar os manuais de Junito Brandão, a saber, a obra Mitologia de Junito Brandão, nos volumes I, II e III, bem como os dois volumes do Dicionário Mítico-Etimológico da Mitologia Grega. Para uma análise comparativa mais eficaz, precisou-se ir além do estudo contextual de produção e representação dos códigos subjacentes a cada narrativa, pois o mito, nas palavras de Ernest Cassirer, é experimentado na consciência, porém é anterior a ela; o homem vive o mito, logo, o mito é anterior ao homem, posto que à medida que toma consciência de sua existência e das relações que tece com o mundo, o homem se vale do mito para estabelecer relações de valor e sentido, bem como representações para singularizar suas experiências. Trata-se, portanto, de uma questão filosófica de vital importância, por isso, buscou-se, para este estudo lítero-narratológico, os fundamentos da Filosofia da mitologia, junto a considerações de uma Antropologia cultural, associado ao levantamento contextual-histórico do cosmo que constitui cada narrativa, a fim de lançar bases elucidativas sobre as relações do homem com seu mundo a partir de determinadas transformações. Sob este foco, diante da pesquisa prévia das narrativas que serão analisadas, percebeu-se que as metamorfoses apresentavam maiores ocorrências quando: 1) simbolizavam o mal na figura dos metamorfoseados; 2) apresentavam motivações de cunho sexual e 3) consistiam em explicações para acontecimentos do mundo físico-espiritual. Trata-se de uma divisão metodológica que objetiva viabilizar a organização e visualização do estudo comparado. Conclui-se, então, que além de possibilitar a leitura e o conhecimento dos mitos gregos e de relatos da Amazônia pelos símbolos constituídos na consciência mítica, este estudo pode servir como uma base para verificação do exercício literário da linguagem criadora por meio do narrar, bem como ampliar a compreensão do que seja e faz a consciência humana enquanto arrimo para a difusão de comportamentos e crenças compartilhados pelo indivíduo em sociedade.

Nós, os degredados filhos de Eva: angústia religiosa e alteridade entre rezadeiras do terço

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Análise estrutural do suporte de pastilha de grafite para lubrificação de roda ferroviária

This study aims to structurally evaluate a support of graphite pastille for the lubrication of railway wheels. The proper lubrication of wheel flanges of the railway extends the life of this component, so it is very important that this occurs lubrication to reduce the costs involved in railway maintenance. To prepar the evaluation structural will be used to International Electrotechnical Comission standard (IEC 61373) establishing which load cases should be applied to this component. The applied loads on the support (accordance with IEC) are random accelerations and accelerations due to shocks, thus simulating the conditions that exist along the route of the train. The structural analyzes are performed by the finite element method, with the aid of the Cosmos software. Thus, it is possible to determine the stresses acting on the support, and so the allowable stresses compared with the standard proposed by the AISC. The stress in the structural analyzes are lower than allowable therefore considered for the configuration presented, unexpected structural problems

Free massive particles with total energy E

We analyze free elementary particles with a rest mass m and total energy E

Scalar field description of decaying-Lambda cosmologies

The conditions under which cosmologies driven by time-varying cosmological terms can be described by a scalar field coupled to a perfect fluid are discussed. An algorithm to reconstruct potentials dynamically and thermodynamically analogous to given phenomenological λ models is presented. As a working example, the deflationary cosmology which evolves from a pure de Sitter vacuum state to a slightly modified Friedmann-Robertson-Walker cosmology is considered. It is found that this is an example of nonsingular warm inflation with an asymptotic exponential potential. Differences with respect to other scalar field descriptions of decaying vacuum cosmologies are addressed and possible extensions are indicated.

A high energy perspective of the co-evolution of black holes and their host galaxies

Thanks to the Chandra and XMM–Newton surveys, the hard X-ray sky is now probed down to a flux limit where the bulk of the X-ray background is almost completely resolved into discrete sources, at least in the 2–8 keV band. Extensive programs of multiwavelength follow-up observations showed that the large majority of hard X–ray selected sources are identified with Active Galactic Nuclei (AGN) spanning a broad range of redshifts, luminosities and optical properties. A sizable fraction of relatively luminous X-ray sources hosting an active, presumably obscured, nucleus would not have been easily recognized as such on the basis of optical observations because characterized by “peculiar” optical properties. In my PhD thesis, I will focus the attention on the nature of two classes of hard X-ray selected “elusive” sources: those characterized by high X-ray-to-optical flux ratios and red optical-to-near-infrared colors, a fraction of which associated with Type 2 quasars, and the X-ray bright optically normal galaxies, also known as XBONGs. In order to characterize the properties of these classes of elusive AGN, the datasets of several deep and large-area surveys have been fully exploited. The first class of “elusive” sources is characterized by X-ray-to-optical flux ratios (X/O) significantly higher than what is generally observed from unobscured quasars and Seyfert galaxies. The properties of well defined samples of high X/O sources detected at bright X–ray fluxes suggest that X/O selection is highly efficient in sampling high–redshift obscured quasars. At the limits of deep Chandra surveys (∼10−16 erg cm−2 s−1), high X/O sources are generally characterized by extremely faint optical magnitudes, hence their spectroscopic identification is hardly feasible even with the largest telescopes. In this framework, a detailed investigation of their X-ray properties may provide useful information on the nature of this important component of the X-ray source population. The X-ray data of the deepest X-ray observations ever performed, the Chandra deep fields, allows us to characterize the average X-ray properties of the high X/O population. The results of spectral analysis clearly indicate that the high X/O sources represent the most obscured component of the X–ray background. Their spectra are harder (G ∼ 1) than any other class of sources in the deep fields and also of the XRB spectrum (G ≈ 1.4). In order to better understand the AGN physics and evolution, a much better knowledge of the redshift, luminosity and spectral energy distributions (SEDs) of elusive AGN is of paramount importance. The recent COSMOS survey provides the necessary multiwavelength database to characterize the SEDs of a statistically robust sample of obscured sources. The combination of high X/O and red-colors offers a powerful tool to select obscured luminous objects at high redshift. A large sample of X-ray emitting extremely red objects (R−K >5) has been collected and their optical-infrared properties have been studied. In particular, using an appropriate SED fitting procedure, the nuclear and the host galaxy components have been deconvolved over a large range of wavelengths and ptical nuclear extinctions, black hole masses and Eddington ratios have been estimated. It is important to remark that the combination of hard X-ray selection and extreme red colors is highly efficient in picking up highly obscured, luminous sources at high redshift. Although the XBONGs do not present a new source population, the interest on the nature of these sources has gained a renewed attention after the discovery of several examples from recent Chandra and XMM–Newton surveys. Even though several possibilities were proposed in recent literature to explain why a relatively luminous (LX = 1042 − 1043erg s−1) hard X-ray source does not leave any significant signature of its presence in terms of optical emission lines, the very nature of XBONGs is still subject of debate. Good-quality photometric near-infrared data (ISAAC/VLT) of 4 low-redshift XBONGs from the HELLAS2XMMsurvey have been used to search for the presence of the putative nucleus, applying the surface-brightness decomposition technique. In two out of the four sources, the presence of a nuclear weak component hosted by a bright galaxy has been revealed. The results indicate that moderate amounts of gas and dust, covering a large solid angle (possibly 4p) at the nuclear source, may explain the lack of optical emission lines. A weak nucleus not able to produce suffcient UV photons may provide an alternative or additional explanation. On the basis of an admittedly small sample, we conclude that XBONGs constitute a mixed bag rather than a new source population. When the presence of a nucleus is revealed, it turns out to be mildly absorbed and hosted by a bright galaxy.

A panchromatic view of the evolution of supermassive black holes

This PhD Thesis is devoted to the accurate analysis of the physical properties of Active Galactic Nuclei (AGN) and the AGN/host-galaxy interplay. Due to the broad-band AGN emission (from radio to hard X-rays), a multi-wavelength approach is mandatory. Our research is carried out over the COSMOS field, within the context of the XMM-Newton wide-field survey. To date, the COSMOS field is a unique area for comprehensive multi-wavelength studies, allowing us to define a large and homogeneous sample of QSOs with a well-sampled spectral coverage and to keep selection effects under control. Moreover, the broad-band information contained in the COSMOS database is well-suited for a detailed analysis of AGN SEDs, bolometric luminosities and bolometric corrections. In order to investigate the nature of both obscured (Type-2) and unobscured (Type-1) AGN, the observational approach is complemented with a theoretical modelling of the AGN/galaxy co-evolution. The X-ray to optical properties of an X-ray selected Type-1 AGN sample are discussed in the first part. The relationship between X-ray and optical/UV luminosities, parametrized by the spectral index αox, provides a first indication about the nature of the central engine powering the AGN. Since a Type-1 AGN outshines the surrounding environment, it is extremely difficult to constrain the properties of its host-galaxy. Conversely, in Type-2 AGN the host-galaxy light is the dominant component of the optical/near-IR SEDs, severely affecting the recovery of the intrinsic AGN emission. Hence a multi-component SED-fitting code is developed to disentangle the emission of the stellar populationof the galaxy from that associated with mass accretion. Bolometric corrections, luminosities, stellar masses and star-formation rates, correlated with the morphology of Type-2 AGN hosts, are presented in the second part, while the final part concerns a physically-motivated model for the evolution of spheroidal galaxies with a central SMBH. The model is able to reproduce two important stages of galaxy evolution, namely the obscured cold-phase and the subsequent quiescent hot-phase.

Testing future weak lensing surveys through simulations of observations

Weak lensing experiments such as the future ESA-accepted mission Euclid aim to measure cosmological parameters with unprecedented accuracy. It is important to assess the precision that can be obtained in these measurements by applying analysis software on mock images that contain many sources of noise present in the real data. In this Thesis, we show a method to perform simulations of observations, that produce realistic images of the sky according to characteristics of the instrument and of the survey. We then use these images to test the performances of the Euclid mission. In particular, we concentrate on the precision of the photometric redshift measurements, which are key data to perform cosmic shear tomography. We calculate the fraction of the total observed sample that must be discarded to reach the required level of precision, that is equal to 0.05(1+z) for a galaxy with measured redshift z, with different ancillary ground-based observations. The results highlight the importance of u-band observations, especially to discriminate between low (z < 0.5) and high (z ~ 3) redshifts, and the need for good observing sites, with seeing FWHM < 1. arcsec. We then construct an optimal filter to detect galaxy clusters through photometric catalogues of galaxies, and we test it on the COSMOS field, obtaining 27 lensing-confirmed detections. Applying this algorithm on mock Euclid data, we verify the possibility to detect clusters with mass above 10^14.2 solar masses with a low rate of false detections.

Tracing AGN accretion and star formation in Herschel galaxies

In this Thesis, we study the physical properties and the cosmic evolution of AGN and their host galaxies since z∼3. Our analysis exploits samples of star forming galaxies detected with Herschel at far-IR wavelengths (from 70 up to 500 micron) in different extragalactic surveys, such as COSMOS and the deep GOODS (South and North) fields. The broad-band ancillary data available in COSMOS and the GOODS fields, allows us to implement Herschel and Spitzer photometry with multi-wavelength ancillary data. We perform a multicomponent SED-fitting decomposition to decouple the emission due to star formation from that due to AGN accretion, and to estimate both host-galaxy parameters (such as stellar mass, M* and star formation rate, SFR), and nuclear intrinsic bolometric luminosities. We use the individual estimates of AGN bolometric luminosity obtained through SED-fitting decomposition to reconstruct the redshit evolution of the AGN bolometric luminosity function since z∼3. The resulting trends are used to estimate the overall AGN accretion rate density at different cosmic epochs and to trace the first ever estimate of the AGN accretion history from an IR survey. Later on, we focus our study on the connection between AGN accretion and integrated galaxy properties. We analyse the relationships of AGN accretion with galaxy properties in the SFR-M* plane and at different cosmic epochs. Finally, we infer what is the parameter that best correlates with AGN accretion, comparing our results with previous studies and discussing their physical implications in the context of current scenarios of AGN/galaxy evolution.