A dramatização da crise dos valores sociais e humanos em Tess of the d'Urbervilles, de Thomas Hardy

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

As paixões humanas em Thomas Hobbes: entre a ciência e a moral, o medo e a esperança

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Diversidade morfológica e molecular do gênero Oecomys thomas, 1906 (Rodentia: Cricetidae) na Amazônia oriental brasileira

Os roedores arborícolas do gênero Oecomys possuem distribuição reconhecida para áreas de floresta tropical e subtropical da América Central e do Sul, e compreendem 17 espécies atualmente reconhecidas, além de duas descritas, mas não nomeadas, reconhecidas em estudos prévios. Destas, apenas seis têm ocorrência esperada para a Amazônia oriental brasileira. A delimitação das espécies com base apenas em caracteres morfológicos é complicada, de forma que diversos táxons nominais já foram associados ao gênero e diversos arranjos taxonômicos foram propostos. Na única revisão taxonômica para o gênero, realizada há 50 anos, foram reconhecidas apenas duas espécies politípicas. Desde então, vários trabalhos envolvendo análises morfológicas, moleculares e cariotípicas têm demonstrado que há uma maior diversidade de espécies em Oecomys, resultando em descrições de espécies novas e revalidações de espécies anteriormente sinonimizadas. Este trabalho buscou caracterizar a variação morfológica e a diversidade molecular das espécies com ocorrência na Amazônia oriental brasileira. Para isto, empregamos análises filogenéticas com base no gene mitocondrial citocromo-b a fim de definir clados que representassem espécies, para as quais descrevemos a morfologia externa e craniana. Como resultado, reconhecemos 11 espécies com ocorrência para o leste da Amazônia brasileira, das quais cinco são esperadas para a região (Oecomys auyantepui, O. bicolor, O. paricola, O. rex e O. rutilus), duas são registradas pela primeira vez para o bioma Amazônia (Oecomys catherinae e O. cleberi) e quatro espécies são novas ou não reconhecidas como válidas atualmente, aqui denominadas Oecomys sp. A, Oecomys sp. B, Oecomys sp. C e Oecomys sp. D. Além disso, corroboramos estudos moleculares prévios em que Oecomys bicolor é um complexo de espécies, com base na alta taxa de divergência nucleotídica apresentada (7,5 %). Observamos dimorfismo sexual e variação ontogenética na morfometria craniana da espécie Oecomys paricola, e para efeito de comparação extrapolamos estas variações para as demais espécies tratadas aqui. Sugerimos também uma hipótese filogenética entre as espécies do gênero a partir de 653 pb do gene citocromo-b, sendo esta a filogenia mais abrangente para Oecomys publicada até o momento, devido ao elevado número de espécies incluídas (11 das 16 espécies atualmente reconhecidas e sete prováveis novas espécies) e a amplitude geográfica das amostras aqui utilizadas.

Nematofauna de Proechimys cf. roberti (Thomas, 1901) (Rodentia: Echimyidae), mamífero silvestre da região amazônica, Pará-Brasil

Roedores do gênero Proechimys são mamíferos de pequeno porte conhecidos como “rato de espinho”, que ocorrem nas Américas Central e do Sul e estão distribuídos em vários Estados brasileiros sendo animais de hábitos silvestres. Existem poucos estudos evidenciando a ocorrência de helmintos em espécies de Proechimys no Brasil. Assim conhecer a diversidade de helmintos parasitos na Amazônia é importante não só para registros de novas espécies, como também para acrescentar dados a biologia desses hospedeiros. Neste trabalho nove tubos digestivos de espécimes de Proechimys cf. roberti fixados em Formaldeído a 10% foram dissecados para obtenção dos helmintos e duas espécies de nematódeos foram separados para estudo. A taxonomia foi realizada por microscopia de luz e microscopia eletrônica de varredura. Identificou-se uma espécie como pertencente ao gênero Spirura e outra como membro da Família Dromaeostrongylidae. No entanto, devido as suas características morfológicas não foi possível incluí-los nas espécies já descritas, sugerindo-se a criação de uma nova espécie do gênero Spirura e um novo gênero e uma nova espécie para a Família Dromaeostrongylidae.

A eloquência no pensamento político de Thomas Hobbes

A presente pesquisa propõe-se a analisar os pressupostos teóricos que servem de apoio para Hobbes fundamentar a sua ciência civil, a qual aparentemente denotaria certa contradição quanto ao fato de ele lançar mão da eloquência enquanto arte da retórica implicitamente nos Elementos da Lei e no Do cidadão ao alinhar parte da bíblia sagrada à obediência civil. Ao mesmo tempo em que claramente o autor nas obras citadas acima condena o referido aspecto da eloquência, paradoxalmente, nas suas duas obras políticas posteriores, Leviatã e Behemoth, Hobbes lança mão explicitamente desta, chegando à conclusão de que ela é necessária como força coadjuvante da razão para conformar as paixões humanas na obediência civil.

Dieta de Micoureus demerarae (Thomas) (Mammalia, Didelphidae) associada às florestas contíguas de mangue e terra firme em Bragança, Pará, Brasil

A dieta de Micoureus demerarae (Thomas, 1905) foi estudada em bosques de mangue e terra firme através de amostras estomacais e fecais. O número de indivíduos capturados foi inversamente proporcional à disponibilidade de frutos e insetos, sendo Coleoptera e Hemiptera as ordens de artrópodes mais consumidos e Passifloraceae e Arecaceae os frutos mais ingeridos. Desse modo, tanto a maior variabilidade de frutos como a alta produção destes durante a estação seca, parecem explicar o aumento da captura desses animais nos bosques de terra firme, dos quais são originalmente provenientes. Os itens alimentares sugerem que esta espécie possui uma dieta do tipo onívora, independentemente da sazonalidade ou distribuição dos recursos disponíveis.

As paixões humanas em Thomas Hobbes

Pós-graduação em Filosofia - FFC

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.

Methods and results of a search for gravitational waves associated with gamma-ray bursts using the GEO 600, LIGO, and Virgo detectors

In this paper we report on a search for short-duration gravitational wave bursts in the frequency range 64 Hz-1792 Hz associated with gamma-ray bursts (GRBs), using data from GEO 600 and one of the LIGO or Virgo detectors. We introduce the method of a linear search grid to analyze GRB events with large sky localization uncertainties, for example the localizations provided by the Fermi Gamma-ray Burst Monitor (GBM). Coherent searches for gravitational waves (GWs) can be computationally intensive when the GRB sky position is not well localized, due to the corrections required for the difference in arrival time between detectors. Using a linear search grid we are able to reduce the computational cost of the analysis by a factor of O(10) for GBM events. Furthermore, we demonstrate that our analysis pipeline can improve upon the sky localization of GRBs detected by the GBM, if a high-frequency GW signal is observed in coincidence. We use the method of the linear grid in a search for GWs associated with 129 GRBs observed satellite-based gamma-ray experiments between 2006 and 2011. The GRBs in our sample had not been previously analyzed for GW counterparts. A fraction of our GRB events are analyzed using data from GEO 600 while the detector was using squeezed-light states to improve its sensitivity; this is the first search for GWs using data from a squeezed-light interferometric observatory. We find no evidence for GW signals, either with any individual GRB in this sample or with the population as a whole. For each GRB we place lower bounds on the distance to the progenitor, under an assumption of a fixed GW emission energy of 10(-2)M circle dot c(2), with a median exclusion distance of 0.8 Mpc for emission at 500 Hz and 0.3 Mpc at 1 kHz. The reduced computational cost associated with a linear search grid will enable rapid searches for GWs associated with Fermi GBM events once the advanced LIGO and Virgo detectors begin operation.

Search for Gravitational Waves Associated with gamma-ray Bursts Detected by the Interplanetary Network

We present the results of a search for gravitational waves associated with 223 gamma-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second, and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational wave data are available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational wave emission energy of 10(-2)M(circle dot)c(2) at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90% confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12 Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational wave detectors and a resulting examination of prospects for the advanced gravitational wave detectors.

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.

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.