Aspectos impressionistas em Bel-ami de Guy de Maupassant

Pós-graduação em Estudos Literários - FCLAR

As Cartas De Guy de Maupassant

Esse trabalho tem como objetivo tecer algumas considerações acerca de uma crônica de Guy de Maupassant (1850-1893), intitulada Le style épistolaire. Publicado no jornal Le Gaulois, no dia 11 de junho de 1888, o texto aborda alguns aspectos importantes do gênero em questão, entre outros, o missivista, tanto o remetente quanto o destinatário, ou ainda, o teor e o estilo das cartas. Revela como Maupassant concebia a arte de escrever cartas, e entender sua visão é um passo importante para adentrar a produção epistolar do próprio autor que, entre 1862 e 1891, escreveu mais de 750 cartas.

Search for gravitational wave ringdowns from perturbed intermediate mass black holes in LIGO-Virgo data from 2005-2010

We report results from a search for gravitational waves produced by perturbed intermediate mass black holes ( IMBH) in data collected by LIGO and Virgo between 2005 and 2010. The search was sensitive to astrophysical sources that produced damped sinusoid gravitational wave signals, also known as ringdowns, with frequency 50 <= f(0)/Hz <= 2000 and decay timescale 0.0001 less than or similar to tau/s less than or similar to 0.1 characteristic of those produced in mergers of IMBH pairs. No significant gravitational wave candidate was detected. We report upper limits on the astrophysical coalescence rates of IMBHs with total binary mass 50 <= M/ M circle dot <= 450 and component mass ratios of either 1: 1 or 4: 1. For systems with total mass 100 <= M/M circle dot <= 150, we report a 90% confidence upper limit on the rate of binary IMBH mergers with nonspinning and equal mass components of 6.9 x 10(-8) Mpc(-3) yr(-1). We also report a rate upper limit for ringdown waveforms from perturbed IMBHs, radiating 1% of their mass as gravitational waves in the fundamental, l = m = 2, oscillation mode, that is nearly three orders of magnitude more stringent than previous results.

The NINJA-2 project: detecting and characterizing gravitational waveforms modelled using numerical binary black hole simulations

The Numerical INJection Analysis (NINJA) project is a collaborative effort between members of the numerical relativity and gravitational-wave (GW) astrophysics communities. The purpose of NINJA is to study the ability to detect GWs emitted from merging binary black holes (BBH) and recover their parameters with next-generation GW observatories. We report here on the results of the second NINJA project, NINJA-2, which employs 60 complete BBH hybrid waveforms consisting of a numerical portion modelling the late inspiral, merger, and ringdown stitched to a post-Newtonian portion modelling the early inspiral. In a 'blind injection challenge' similar to that conducted in recent Laser Interferometer Gravitational Wave Observatory (LIGO) and Virgo science runs, we added seven hybrid waveforms to two months of data recoloured to predictions of Advanced LIGO (aLIGO) and Advanced Virgo (AdV) sensitivity curves during their first observing runs. The resulting data was analysed by GW detection algorithms and 6 of the waveforms were recovered with false alarm rates smaller than 1 in a thousand years. Parameter-estimation algorithms were run on each of these waveforms to explore the ability to constrain the masses, component angular momenta and sky position of these waveforms. We find that the strong degeneracy between the mass ratio and the BHs' angular momenta will make it difficult to precisely estimate these parameters with aLIGO and AdV. We also perform a large-scale Monte Carlo study to assess the ability to recover each of the 60 hybrid waveforms with early aLIGO and AdV sensitivity curves. Our results predict that early aLIGO and AdV will have a volume-weighted average sensitive distance of 300 Mpc (1 Gpc) for 10M circle dot + 10M circle dot (50M circle dot + 50M circle dot) BBH coalescences. We demonstrate that neglecting the component angular momenta in the waveform models used in matched-filtering will result in a reduction in sensitivity for systems with large component angular momenta. This reduction is estimated to be up to similar to 15% for 50M circle dot + 50M circle dot BBH coalescences with almost maximal angular momenta aligned with the orbit when using early aLIGO and AdV sensitivity curves.

Description of the larva of telebasis griffinii (Martin, 1896) (zygoptera: coenagrionidae)

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Modos de ler e ações de leitura waysto read and actions of reading

This paper is the result of discussions held during the initial research on ways of reading and reading activities, to obtain the title of the Ph.D. graduate program in Education at UNESP - Marilia. The paper seeks to rethink the practice followed the reality historically constructed as reference, creating a dialectic movement, and a constant construction, and the overcoming of it. In this perspective, we approach possible practices that can enhance the student's prior knowledge, and from it, to propose ways of action that lead to the development of the subject through the processes of teaching and learning of reading in school. From the study of actions that are agreed as reading practices, the study proposes to work with the Reading Strategies to promote the development of the individual. Among the different results that have been announced in the research, we highlight the need for conscious mediation of the teacher in the act of teaching reading and conscious participation of the student in the process. Partial results give evidence to confirm the hypothesis that: intentional actions are driving the learning of children in activity in the classroom, considering their experiences and choices of the teacher as mediator in the process. Students in third grade of elementary school are the subjects of research, theory and practice. The researcher is the mediator and proposer of the actions based on microgenetic research.

Implementation of an F-statistic all-sky search for continuous gravitational waves in Virgo VSR1 data

We present an implementation of the F-statistic to carry out the first search in data from the Virgo laser interferometric gravitational wave detector for periodic gravitational waves from a priori unknown, isolated rotating neutron stars. We searched a frequency f(0) range from 100 Hz to 1 kHz and the frequency dependent spindown f(1) range from -1.6(f(0)/100 Hz) x 10(-9) Hz s(-1) to zero. A large part of this frequency-spindown space was unexplored by any of the all-sky searches published so far. Our method consisted of a coherent search over two-day periods using the F-statistic, followed by a search for coincidences among the candidates from the two-day segments. We have introduced a number of novel techniques and algorithms that allow the use of the fast Fourier transform (FFT) algorithm in the coherent part of the search resulting in a fifty-fold speed-up in computation of the F-statistic with respect to the algorithm used in the other pipelines. No significant gravitational wave signal was found. The sensitivity of the search was estimated by injecting signals into the data. In the most sensitive parts of the detector band more than 90% of signals would have been detected with dimensionless gravitational-wave amplitude greater than 5 x 10(-24).

Search for gravitational radiation from intermediate mass black hole binaries in data from the second LIGO-Virgo joint science run

This paper reports on an unmodeled, all-sky search for gravitational waves from merging intermediate mass black hole binaries (IMBHB). The search was performed on data from the second joint science run of the LIGO and Virgo detectors (July 2009-October 2010) and was sensitive to IMBHBs with a range up to similar to 200 Mpc, averaged over the possible sky positions and inclinations of the binaries with respect to the line of sight. No significant candidate was found. Upper limits on the coalescence-rate density of nonspinning IMBHBs with total masses between 100 and 450 M-circle dot and mass ratios between 0.25 and 1 were placed by combining this analysis with an analogous search performed on data from the first LIGO-Virgo joint science run (November 2005-October 2007). The most stringent limit was set for systems consisting of two 88 M-circle dot black holes and is equal to 0.12 Mpc(-3) Myr(-1) at the 90% confidence level. This paper also presents the first estimate, for the case of an unmodeled analysis, of the impact on the search range of IMBHB spin configurations: the visible volume for IMBHBs with nonspinning components is roughly doubled for a population of IMBHBs with spins aligned with the binary's orbital angular momentum and uniformly distributed in the dimensionless spin parameter up to 0.8, whereas an analogous population with antialigned spins decreases the visible volume by similar to 20%.

First all-sky search for continuous gravitational waves from unknown sources in binary systems

We present the first results of an all-sky search for continuous gravitational waves from unknown spinning neutron stars in binary systems using LIGO and Virgo data. Using a specially developed analysis program, the TwoSpect algorithm, the search was carried out on data from the sixth LIGO science run and the second and third Virgo science runs. The search covers a range of frequencies from 20 Hz to 520 Hz, a range of orbital periods from 2 to similar to 2,254 h and a frequency-and period-dependent range of frequency modulation depths from 0.277 to 100 mHz. This corresponds to a range of projected semimajor axes of the orbit from similar to 0.6 x 10(-3) ls to similar to 6,500 ls assuming the orbit of the binary is circular. While no plausible candidate gravitational wave events survive the pipeline, upper limits are set on the analyzed data. The most sensitive 95% confidence upper limit obtained on gravitational wave strain is 2.3 x 10(-24) at 217 Hz, assuming the source waves are circularly polarized. Although this search has been optimized for circular binary orbits, the upper limits obtained remain valid for orbital eccentricities as large as 0.9. In addition, upper limits are placed on continuous gravitational wave emission from the low-mass x-ray binary Scorpius X-1 between 20 Hz and 57.25 Hz.

Improved Upper Limits on the Stochastic Gravitational-Wave Background from 2009-2010 LIGO and Virgo Data

Gravitational waves from a variety of sources are predicted to superpose to create a stochastic background. This background is expected to contain unique information from throughout the history of the Universe that is unavailable through standard electromagnetic observations, making its study of fundamental importance to understanding the evolution of the Universe. We carry out a search for the stochastic background with the latest data from the LIGO and Virgo detectors. Consistent with predictions from most stochastic gravitational-wave background models, the data display no evidence of a stochastic gravitational-wave signal. Assuming a gravitational-wave spectrum of Omega(GW)(f) = Omega(alpha)(f/f(ref))(alpha), we place 95% confidence level upper limits on the energy density of the background in each of four frequency bands spanning 41.5-1726 Hz. In the frequency band of 41.5-169.25 Hz for a spectral index of alpha = 0, we constrain the energy density of the stochastic background to be Omega(GW)(f) < 5.6 x 10(-6). For the 600-1000 Hz band, Omega(GW)(f) < 0.14(f/900 Hz)(3), a factor of 2.5 lower than the best previously reported upper limits. We find Omega(GW)(f) < 1.8 x 10(-4) using a spectral index of zero for 170-600 Hz and Omega(GW)(f) < 1.0(f/1300 Hz)(3) for 1000-1726 Hz, bands in which no previous direct limits have been placed. The limits in these four bands are the lowest direct measurements to date on the stochastic background. We discuss the implications of these results in light of the recent claim by the BICEP2 experiment of the possible evidence for inflationary gravitational waves.

Realismo e impressionismo em contos de Guy de Maupassant

Dans ce texte on a étudié, afin de comprendre et d'analyser les contes réalistes de Guy de Maupassant, comment Erich Auerbach, dans Mimesis (2009), parcourt les sentiers de la littérature occidentale pour dresser un tableau des traits communs qui existent entre les grandes oeuvres réalistes de l'Occident. L'auteur a réalisé des recherches et des commentaires sur les caractéristiques les plus récurrentes du réalisme littéraire dans les oeuvres d'écrivains tels que Homero, Shakespeare, Voltaire, Flaubert, parmi d'autres. Notre recherche vise, dans sa première étape, à présenter, à expliquer ou à identifier dans les contes de Guy de Maupassant, écrivain de la fin du XIXe siècle, les tendances réalistes discutées par ce théoricien et par d'autres au fil du temps, comme, par exemple, Roland Barthes, dans Crítica e verdade (2007), Bersani, dans Le réalisme et la peur du désir (1975) et Philippe Hamon, dans Un discours contraint (1973, p. 411-445). À partir de ces chercheurs, on essaie d'expliciter et d'affirmer le caractère réaliste d'un des maîtres du récit court - sûrement un représentant du réalisme parmi les grands écrivains de cet art - car dans Mimesis (2009) Zola est considéré par Auerbach comme le dernier des grands réalistes français. En plus, pour la deuxième partie de ce travail, on a l'intention de traiter l'émergence de l'impressionnisme artistique en France, et de présenter les concepts et les thèmes qui ont influencé ce mouvement et se présentent dans la construction des récits de Maupassant. Pour le faire, O impressionismo (1962) de Balzi, O impressionismo (1965) de Serullaz, Impressionniste et symboliste devant la presse (1959) de Jacques Lethève, Impressionismo (2010) de Lobstein e autres, mentionnés dans la bibliographie de cette recherche, ont ouvert la voie aux analyses... (Completo abstract click electronic access below)

Aspectos das vertentes do fantástico e do realismo em obras de Guy de Maupassant

Pretende-se, com a apresentação deste trabalho, estudar não somente o escritor francês Guy de Maupassant no interior da vertente realista/naturalista, mas como explorador do veio do fantástico e como tais disposições literárias encontram-se trabalhadas em suas obras. As selecionadas para estudo são: o romance Bel- Ami de 1885 e os contos Bola de Sebo, publicado em 1880 e A Noite, publicado em 1887. Considera-se muito a vida literária de Maupassant, tanto como discípulo e correspondente de Gustave Flaubert (1821-1880), como grande amigo de Èmile Zola (1840- 1902), que o admirou. Por fim, como fundamentação teórica, utiliza-se de dois teóricos – Boris Tomachevski e Tezvetan Todorov –, com os quais se busca entender, prioritariamente, como ler Maupassant por meio dos conceitos de “interesse”, “motivação realista” e “estética”, propostos por Tomachevski e o Fantástico, pelas considerações de Tezvetan Todorov

A mentora literária de Guy de Maupassant

Laure Le Poittevin, Guy de Maupassant’s mother (1850-1893), had from his early childhood, a key role in the literary education of her son. This intelligent and sensitive woman, who was always passionate about arts, especially literature, to whom Maupasssant entrusted his projects and literary adventures, was his fi rst and eternal critic. In the letters he writes her, most of the time he takes the opportunity to plan and discuss his future projects; he presents a text in progress, he draws its guiding lines, he foreshadows its structures and points out some procedures based on a series of principles and recommendations of personal and universal values. Therefore, by reading again these letters, the readers nowadays can follow the writer’s daily life, the progression of his ideas and his literary development, the editing process of his book and his moments of sorrow and joy, anger and affection.

The genomes of two key bumblebee species with primitive eusocial organization

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)