Contribution to the biology and geographical distribution of Aegagropila sauteri (Nees) Kutz. [Translation of: Gidrobiologicheskie Zhurnal, Kiev 4(3), 68-69, 1967]

Aegagropila sauteri is a peculiar green algae, the branched thalli of which, according to the amount of growth, forms velvety spheres of a diameter of 3-4, sometimes to 5-6 cm. and bigger. Investigators attribute it to a special genus of green algae. The authors examine Aegagropila sauteri in Lake Markakol (Kazakhstan).

Volatiles in Protoplanetary Disks

Planets are assembled from the gas, dust, and ice in the accretion disks that encircle young stars. Ices of chemical compounds with low condensation temperatures (<200 K), the so-called volatiles, dominate the solid mass reservoir from which planetesimals are formed and are thus available to build the protoplanetary cores of gas/ice giant planets. It has long been thought that the regions near the condensation fronts of volatiles are preferential birth sites of planets. Moreover, the main volatiles in disks are also the main C-and O-containing species in (exo)planetary atmospheres. Understanding the distribution of volatiles in disks and their role in planet-formation processes is therefore of great interest.

This thesis addresses two fundamental questions concerning the nature of volatiles in planet-forming disks: (1) how are volatiles distributed throughout a disk, and (2) how can we use volatiles to probe planet-forming processes in disks? We tackle the first question in two complementary ways. We have developed a novel super-resolution method to constrain the radial distribution of volatiles throughout a disk by combining multi-wavelength spectra. Thanks to the ordered velocity and temperature profiles in disks, we find that detailed constraints can be derived even with spatially and spectrally unresolved data -- provided a wide range of energy levels are sampled. We also employ high-spatial resolution interferometric images at (sub)mm frequencies using the Atacama Large Millimeter Array (ALMA) to directly measure the radial distribution of volatiles.

For the second question, we combine volatile gas emission measurements with those of the dust continuum emission or extinction to understand dust growth mechanisms in disks and disk instabilities at planet-forming distances from the central star. Our observations and models support the idea that the water vapor can be concentrated in regions near its condensation front at certain evolutionary stages in the lifetime of protoplanetary disks, and that fast pebble growth is likely to occur near the condensation fronts of various volatile species.

A representação dos atores sociais e a imagem da mulher no contexto do discurso feminista em contos de Marina Colasanti

O livro Contos de amor rasgados, de Marina Colasanti, foi publicado em 1986, década de consolidação das conquistas do movimento feminista (Pinto, 2003). O feminismo almejava uma mudança de mentalidade, mudança nas práticas sociais e nos discursos sobre a mulher (ibid.). Entretanto, a mulher nos contos é representada de forma peculiar, frustrando as expectativas de uma imagem positiva esperada de uma literatura produzida por uma autora feminista. Este estudo propõe a análise dos contos de Marina Colasanti, destacando algumas questões acerca da representação dos atores sociais em textos-contos que pretendem veicular um discurso de liberação da mulher. Para tanto, dez contos representativos do todo foram selecionados para compor o corpus e utilizou-se o sistema sociossemântico para a representação dos atores sociais proposto por van Leeuwen (1997) e a Linguística Sistêmico Funcional de Halliday (2004) como ferramentas de análise. Nosso enfoque é o da Análise Crítica do Discurso de Fairclough (1995), que tem dedicado seus estudos às mudanças sociais através dos discursos. Consideramos que o movimento feminista se inscreve em algumas mudanças. Nessa perspectiva, Bourdieu (2005) afirma que, apesar do movimento feminista, muito pouco mudou, prevalecendo, ainda, a dominação masculina e a violência simbólica. As categorias de van Leeuwen (op. cit.) da exclusão e inclusão dos atores sociais no discurso servem de instrumental para uma análise mais detalhada das relações homem-mulher, permitindo desvelar algumas questões feministas tematizadas nos contos, questões descritas por Pinto (op. cit.) e apontadas por Bourdieu (op. cit.). Os resultados da análise dos contos demonstram que a mulher ora está totalmente excluída, ora é representada como um pano de fundo (encobrimento), ora é enfraquecida (apassivada) em favor de seu marido/amante. Assim, os conflitos gerados a partir das ações do homem sobre a mulher nos contos confirmam certas preocupações do discurso feminista

Direitos de propriedade intelectual e saúde pública: das normas de regulação às práticas de exame de patentes na área farmacêutica no Brasil.

Este trabalho discute o patenteamento farmacêutico no Brasil por meio de análises dos exames de patentes propriamente ditos, com a entrada em vigor da atual lei da propriedade industrial (Lei 9.279/1996). Para a compreensão de como funciona o exame de patentes, parte-se da apresentação de conceitos basilares da propriedade industrial. É dado destaque à importância das patentes como fonte de informação tecnológica (pesquisa bibliográfica em bancos de patentes e para a recuperação das informações contidas nestes documentos). Neste ponto, apresenta-se um estudo sobre as patentes relacionadas ao efavirenz, por tratar-se de um caso excepcional na discussão sobre propriedade industrial e saúde pública; já que ele foi o primeiro medicamento licenciado compulsoriamente pelo Governo brasileiro (dentro da política de controle da epidemia da Aids). Em seguida, o problema da associação entre os direitos de propriedade industrial e o acesso a medicamentos é abordado em dois capítulos relevantes: i) as questões sobre a atenteabilidade de polimorfos de fármacos; e ii) os procedimentos técnicos adotados no exame de patentes farmacêuticas no âmbito da Coordenação de Propriedade Intelectual da ANVISA (COOPI-ANVISA) e do Instituto Nacional da Propriedade Industrial (INPI). De fato, o primeiro tratado internacional relativo à propriedade industrial, a Convenção da União de Paris (CUP, de 1883), já propugnava o princípio da independência das patentes, ou seja, que cada país tem liberdade para decidir sobre a patenteabilidade ou não dos diferentes produtos e processos de invenção. Mais tarde, o Acordo TRIPS (de 1995) não vedará aos países a adoção de escopos de proteção distintos, visando o equilíbrio entre os interesses públicos e privados em diferentes domínios tecnológicos, nos diferentes países. Finalmente, a Declaração de Doha, de 2001, prevê dispositivos flexibilizadores de modo a favorecer precisamente políticas de saúde e acesso a medicamentos pela utilização de salvaguardas dos direitos de propriedade intelectual no exame de pedidos de patentes. Conclui-se, neste trabalho, que aspectos técnicos e jurídicos inerentes ao patenteamento aliados à capacidade política de decisão em favor da implementação de flexibilidades no exame de pedidos patentes de fármacos e medicamentos podem ser mais ou menos favoráveis à saúde pública.

Selective plankton feeding by the coregonid ”bondella” (Coregonus sp.) of Lake Maggiore [Translation from: Translation from: Memorie dell'Istituto Italiano di Idrobiologia Dott.Marco de Marchi 31 181-203, 1974]

In recent times, some specialists have begun to study the subject of food selection of fish in an organized way, thus highlighting its importance. In the present work, the author intends to evaluate the impact of predation on the eupelagic zooplanktonic biocenosis of Lake Maggiore, producing, in this way, as far as possible, a basis for a better understanding of the population dynamics of the species of zooplankton directly involved. Another aspect which has been studied is that related to the mechanism of selective capture set in action by the predator. To this end the study tries to bear in mind that the subject should be interpreted as a function of numerous factors acting contemporaneously, that is as the interaction of characters peculiar to the predator and to the prey. The species studied, locally called ”bondella”, belongs to the family Salmonidae, subfamily Coregoninae and was introduced into Lake Maggiore in 1950.

BLOG: da Internet à sala de aula

Os diários de escrita íntima constituem tipo de texto do domínio confessional. Apresentam narrativas pessoais com características específicas ao gênero, como datação, marcas de subjetividade, escrita informal e coloquialidade. Durante muitos anos, eram escritos em cadernos e guardados a sete chaves por seus autores para que não fossem lidos por outras pessoas. Por volta dos anos 80, surgiram as agendas de adolescentes. Aproveitando o modelo pré-definido industrialmente, as agendas eram preenchidas dia a dia, como um diário, mas com a novidade do acréscimo de elementos semióticos, como fotos, papéis de bala, recortes de revistas, entre outros. Além disso, traziam como diferencial a presença de um leitor participativo: os textos eram compartilhados com amigos, e bilhetes e comentários eram escritos nas páginas das agendas. Com o advento da Internet, o diário e a agenda se fundem no blog que aproveita os recursos do suporte virtual para tornar o gênero interativo, hipertextual e multimídia, acentuando o processo de leitura e de escrita nos jovens produtores de blogs. Paralelamente, a escrita se torna grande ferramenta de comunicação no ambiente virtual, adquirindo características peculiares em função da rapidez na comunicação e da economia de digitação. A partir da teoria de Bakthin sobre gêneros do discurso e do conceito de gêneros digitais de Marcuschi, a pesquisa apresenta como objeto perceber e elencar categorias pertinentes aos gêneros diário e blog para analisá-las e compará-las, na intenção de mapear um possível percurso dos diários aos blogs de adolescentes, discutindo o contraste público-privado na escrita íntima, bem como suas principais marcas linguísticas, percebendo vantagens e desvantagens de sua utilização como ferramenta auxiliar no processo de aprendizagem da escrita e da leitura de Língua Portuguesa. A pesquisa foi motivada pela discussão de que a escrita digital pode prejudicar o desenvolvimento da produção textual de jovens em formação, o que não se confirmou, visto que a estrutura sintática da língua se mantém, e que a variação acontece apenas no nível vocabular, não interferindo na comunicação. Os resultados apontam para a utilização de blogs na educação como complementação do material pedagógico e como incentivo à leitura, à escrita, à construção da argumentação e do posicionamento crítico, aproximando a escola da vida cotidiana dos estudantes

Individual growth and seasonal cycle of Daphnia middendorffiana in an Alpine lake [Translation from: Memorie dell'Istituto Italiano di Idrobiologia Dott.Marco de Marchi 26 41-83, 1970]

The problem of the peculiar reproductive biology of the cladoceran Daphnia middendorffiana is investigated from a cytological viewpoint, and by direct observation the meiotic phenomena of the eggs both subitaneous and resting is studied. and during maturation, the true mechanism of the succession of reproductive phases of different ecological significance. Samples were collected in the Italian Alpine Lake of Campo 4°.

The astrophysics of strongly interacting systems

This thesis presents investigations in four areas of theoretical astrophysics: the production of sterile neutrino dark matter in the early Universe, the evolution of small-scale baryon perturbations during the epoch of cosmological recombination, the effect of primordial magnetic fields on the redshifted 21-cm emission from the pre-reionization era, and the nonlinear stability of tidally deformed neutron stars.

In the first part of the thesis, we study the asymmetry-driven resonant production of 7 keV-scale sterile neutrino dark matter in the primordial Universe at temperatures T >~ 100 MeV. We report final DM phase space densities that are robust to uncertainties in the nature of the quark-hadron transition. We give transfer functions for cosmological density fluctuations that are useful for N-body simulations. We also provide a public code for the production calculation.

In the second part of the thesis, we study the instability of small-scale baryon pressure sound waves during cosmological recombination. We show that for relevant wavenumbers, inhomogenous recombination is driven by the transport of ionizing continuum and Lyman-alpha photons. We find a maximum growth factor less than ≈ 1.2 in 10⁷ random realizations of initial conditions. The low growth factors are due to the relatively short duration of the recombination epoch.

In the third part of the thesis, we propose a method of measuring weak magnetic fields, of order 10^-19 G (or 10^-21 G if scaled to the present day), with large coherence lengths in the inter galactic medium prior to and during the epoch of cosmic reionization. The method utilizes the Larmor precession of spin-polarized neutral hydrogen in the triplet state of the hyperfine transition. We perform detailed calculations of the microphysics behind this effect, and take into account all the processes that affect the hyperfine transition, including radiative decays, collisions, and optical pumping by Lyman-alpha photons.

In the final part of the thesis, we study the non-linear effects of tidal deformations of neutron stars (NS) in a compact binary. We compute the largest three- and four-mode couplings among the tidal mode and high-order p- and g-modes of similar radial wavenumber. We demonstrate the near-exact cancellation of their effects, and resolve the question of the stability of the tidally deformed NS to leading order. This result is significant for the extraction of binary parameters from gravitational wave observations.

The equivalent conductance of solutions of picric acid

Picric acid possesses the property, which is rare among strong electrolytes, of having a convenient distribution ratio between water and certain organic solvents such as benzene, chloroform, etc. Because of this property, picric acid offers peculiar advantages for studying the well known deviations of strong electrolytes from the law of mass action, for; by means of distribution experiments, the activities of picric acid in various aqueous solutions may be compared.

In order to interpret the results of such distribution experiments, it is necessary to know the degree of ionization of picric acid in aqueous solutions.

At least three series of determinations of the equivalent conductance of picric acid have been published, but the results are not concordant; and therefore, the degree of ionization cannot be calculated with any degree of certainty.

The object of the present investigation was to redetermine the conductance of picric acid solutions in order to obtain satisfactory data from which the degrees of ionization of its solutions might be calculated.

O sonho de Bilac ou como transformar Sebastianópolis em vitrine do Brasil moderno

Esta dissertação apresenta um estudo da crônica, gênero utilizado por Olavo Bilac poeta das estrelas e cronista da cidade para divulgar o modelo republicano de ordem e progresso. No presente estudo encontra-se também a análise de algumas crônicas bilaquianas especialmente as do período das reformas do governo Pereira Passos cujo tema central é o progresso urbano, incluindo as noções de civilidade, higienização e sanitarismo. Esse pensamento correspondia ao movimento de urbanização pelo qual a cidade do Rio de Janeiro passava de modo a transformar-se em uma verdadeira cidade-capital e vitrine do Brasil moderno

Tratamento de efluentes líquidos na Estação Antártica Comandante Ferraz (EACF): avaliação da aplicabilidade do processo eletrolítico.

Esta pesquisa enfoca o uso do processo eletrolítico, como alternativa para tratamento de efluentes líquidos na Estação Antártica Comandante Ferraz (EACF), considerando as limitações ambientais locais e aspectos de consumo de energia. Este processo, classificado como não convencional, vem sendo estudado pela comunidade científica nacional e internacional para tratamento de diversos efluentes, inclusive esgotos domésticos, apresentando várias vantagens que estimularam a verificação de sua aplicabilidade para as condições peculiares da EACF. Foram realizados ensaios, em escala de laboratório, com esgotos domésticos coletados em um condomínio no Rio de Janeiro, usando reatores eletrolíticos com capacidade de 4 L, com eletrodos de desgaste de alumínio (Al) e de ferro (Fe), distância entre as placas de 0,9 cm e 1,8 cm, temperaturas na faixa de 7C a 22C, e ensaios para verificação da sua eficiência, por meio de parâmetros como DQO, DBO5, SST, turbidez e volume de lodo gerado. Sob temperatura de 15C e condições de condutividade da ordem de 900 S/cm, estimada para os esgotos da EACF, aplicando densidade de corrente de 22,9 A/m2, 4,5 V, tempo de retenção de 25 min, os resultados apresentaram valores de DQO no efluente tratado de 65 mg/L(redução de 89%), DBO de 56 mg/L (redução de 64 %), SST de 8 mg/L, com turbidez de 11,3 uT e, após filtração, turbidez de 3,2 uT, consumo de energia de 0,8 Wh/L. O aspecto é límpido e a qualidade final obtida é compatível para ser submetida a tratamento de desinfecção. A partir dos dados obtidos, foram avaliadas por meio de pré-projeto: a viabilidade de sua implantação em container, a estimativa de consumo de energia e de lodo gerado, requisitos de manutenção, operação, além da sugestão de monitoramentos e de medidas de mitigação de impactos ambientais associados à respectiva instalação.

Mass measurements of some proton-rich nuclei

The Q values and 0^o cross sections of (He³, n) reactions forming seven proton-rich nuclei have been measured with accuracies varying from 6 to 18 keV. The Q values (in keV) are: Si²⁶ (85), S³⁰ (-573), Ar³⁴ (-759), Ti⁴² (-2865), Cr⁴⁸ (5550), Ni⁵⁶ (4513) and Zn⁶⁰ (818). At least one excited state was found for all but Ti⁴². The first four nuclei complete isotopic spin triplets; the results obtained agree well with charge-symmetry predictions. The last three, all multiples of the α particle, are important in the α and e-process theories of nucleo-synthesis in stars. The energy available for β decay of these three was found by magnetic spectrometer measurements of the (He³, p) Q values of reactions leading to V⁴⁸, Co⁵⁶, and Cu⁶⁰. Many excited states were seen: V⁴⁸ (3), Co⁵⁶ (15), Cu⁶⁰ (23). The first two states of S³⁰ are probably 0⁺ and 2⁺ from (He³, n) angular distribution measurements. Two NaI γ-ray measurements are described: the decay of Ar³⁴ (measured ^Ƭ1/2 = 1.2 ± 0.3s) and the prompt γ-ray spectrum from Fe⁵⁴(He³, nγ)Ni⁵⁶. Possible collective structure in Ni⁵⁶ and Ca⁴⁰, both doubly magic, is discussed.

The (He³, n) neutron energy and yield measurements utilized neutron-induced nuclear reactions in a silicon semiconductor detector. Cross sections for the most important detection processes, Si²⁸ (n, α) Mg²⁵ and Si²⁸ (n, p) Al²⁸, are presented for reactions leading to the first four states of both residual nuclei for neutron energies from 7.3 to 16.4 MeV. Resolution and pulse-height anomalies associated with recoil Mg²⁵ and Al²⁸ ions are discussed. The 0^o cross section for Be⁹ (α, n) C¹², used to provide calibration neutrons, has been measured with a stilbene spectrometer for n_o (5.0 ≤ E_α ≤ 12 MeV), n₁ (4.3 ≤ E_α ≤ 12.0 MeV) and n₂ (6.0 ≤ E_α ≤ 10.1 MeV). Resonances seen in the n_o yield may correspond to nine new levels in C¹³.

Deep near-infrared spectroscopy of high-redshift galaxies: the physical growth of passive systems

The assembly history of massive galaxies is one of the most important aspects of galaxy formation and evolution. Although we have a broad idea of what physical processes govern the early phases of galaxy evolution, there are still many open questions. In this thesis I demonstrate the crucial role that spectroscopy can play in a physical understanding of galaxy evolution. I present deep near-infrared spectroscopy for a sample of high-redshift galaxies, from which I derive important physical properties and their evolution with cosmic time. I take advantage of the recent arrival of efficient near-infrared detectors to target the rest-frame optical spectra of z > 1 galaxies, from which many physical quantities can be derived. After illustrating the applications of near-infrared deep spectroscopy with a study of star-forming galaxies, I focus on the evolution of massive quiescent systems.

Most of this thesis is based on two samples collected at the W. M. Keck Observatory that represent a significant step forward in the spectroscopic study of z > 1 quiescent galaxies. All previous spectroscopic samples at this redshift were either limited to a few objects, or much shallower in terms of depth. Our first sample is composed of 56 quiescent galaxies at 1 < z < 1.6 collected using the upgraded red arm of the Low Resolution Imaging Spectrometer (LRIS). The second consists of 24 deep spectra of 1.5 < z < 2.5 quiescent objects observed with the Multi-Object Spectrometer For Infra-Red Exploration (MOSFIRE). Together, these spectra span the critical epoch 1 < z < 2.5, where most of the red sequence is formed, and where the sizes of quiescent systems are observed to increase significantly.

We measure stellar velocity dispersions and dynamical masses for the largest number of z > 1 quiescent galaxies to date. By assuming that the velocity dispersion of a massive galaxy does not change throughout its lifetime, as suggested by theoretical studies, we match galaxies in the local universe with their high-redshift progenitors. This allows us to derive the physical growth in mass and size experienced by individual systems, which represents a substantial advance over photometric inferences based on the overall galaxy population. We find a significant physical growth among quiescent galaxies over 0 < z < 2.5 and, by comparing the slope of growth in the mass-size plane dlogR_e/dlogM_∗ with the results of numerical simulations, we can constrain the physical process responsible for the evolution. Our results show that the slope of growth becomes steeper at higher redshifts, yet is broadly consistent with minor mergers being the main process by which individual objects evolve in mass and size.

By fitting stellar population models to the observed spectroscopy and photometry we derive reliable ages and other stellar population properties. We show that the addition of the spectroscopic data helps break the degeneracy between age and dust extinction, and yields significantly more robust results compared to fitting models to the photometry alone. We detect a clear relation between size and age, where larger galaxies are younger. Therefore, over time the average size of the quiescent population will increase because of the contribution of large galaxies recently arrived to the red sequence. This effect, called progenitor bias, is different from the physical size growth discussed above, but represents another contribution to the observed difference between the typical sizes of low- and high-redshift quiescent galaxies. By reconstructing the evolution of the red sequence starting at z ∼ 1.25 and using our stellar population histories to infer the past behavior to z ∼ 2, we demonstrate that progenitor bias accounts for only half of the observed growth of the population. The remaining size evolution must be due to physical growth of individual systems, in agreement with our dynamical study.

Finally, we use the stellar population properties to explore the earliest periods which led to the formation of massive quiescent galaxies. We find tentative evidence for two channels of star formation quenching, which suggests the existence of two independent physical mechanisms. We also detect a mass downsizing, where more massive galaxies form at higher redshift, and then evolve passively. By analyzing in depth the star formation history of the brightest object at z > 2 in our sample, we are able to put constraints on the quenching timescale and on the properties of its progenitor.

A consistent picture emerges from our analyses: massive galaxies form at very early epochs, are quenched on short timescales, and then evolve passively. The evolution is passive in the sense that no new stars are formed, but significant mass and size growth is achieved by accreting smaller, gas-poor systems. At the same time the population of quiescent galaxies grows in number due to the quenching of larger star-forming galaxies. This picture is in agreement with other observational studies, such as measurements of the merger rate and analyses of galaxy evolution at fixed number density.

The reduced-alpha-width of the lowest 1¯ state of ^(16)O

Cross sections for the reaction ¹²C(α,γ)¹⁶O have been measured for a range of center-of-mass alpha particle energies extending from 1.72 MeV to 2.94 MeV. Two 8"x5" NaI (Tℓ) crystals were used to detect gamma rays; time-of-flight technique was employed to suppress cosmic ray background and background due to neutrons arising mainly from the ¹³C(α,n)¹⁶O reaction. Angular distributions were measured at center-of-mass alpha energies of 2.18, 2.42, 2.56 and 2.83 MeV. Upper limits were placed on the amount of radiation cascading through the 6.92 or 7.12-MeV states in ¹⁶O. By means of theoretical fits to the measured electric dipole component of the total cross section, in which interference between the 1¯ states in ¹⁶O at 7.12 MeV and at 9.60 MeV is taken into account, it is possible to extract the dimensionless, reduced-alpha-width of the 7.12-MeV state in ¹⁶O. A three-level R-matrix parameterization of the data yields the width Θ_α,F² = 0.14^+0.10_-0.08. A "hybrid" R-matrix-optical-model parameterization yields Θ_α,F² = 0.11^+0.11_-0.07. This quantity is of crucial importance in determining the abundances of ¹²C and ¹⁶O at the end of helium burning in stars.

Supernovae explosions induced by pair production instability

Stars with a core mass greater than about 30 M_⊙ become dynamically unstable due to electron-positron pair production when their central temperature reaches 1.5-2.0 x 10^{9 0}K. The collapse and subsequent explosion of stars with core masses of 45, 52, and 60 M_⊙ is calculated. The range of the final velocity of expansion (3,400 – 8,500 km/sec) and of the mass ejected (1 – 40 M_⊙) is comparable to that observed for type II supernovae.

An implicit scheme of hydrodynamic difference equations (stable for large time steps) used for the calculation of the evolution is described.

For fast evolution the turbulence caused by convective instability does not produce the zero entropy gradient and perfect mixing found for slower evolution. A dynamical model of the convection is derived from the equations of motion and then incorporated into the difference equations.