As vogais médias pretônicas dos verbos na fala culta do interior paulista

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

Sugar cane variety research for the Caribbean

Includes bibliography

Potencial solar das radiações global, difusa e direta em Botucatu

Pós-graduação em Agronomia (Energia na Agricultura) - FCA

A elasticidade-renda do comércio regional de produtos manufaturados

Incluye Bibliografía

Os teoremas de índice de Poincaré

Pós-graduação em Matemática Universitária - IGCE

Reversão sexual da tilápia do Nilo com dietas microencapsuladas em spray dryer contendo diferentes doses de 17-'alfa'metiltestosterona e tempos de administração

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

Desenvolvimento de um método de análise por injeção em fluxo (FIA) para determinação de dissulfeto de tetrametiltiuram (tiram) utilizando reagente imobilizado em reator de fase sólida (RFS)

Pós-graduação em Química - IBILCE

Distribuição espacial e plano de amostragem seqüencial de ácaros fitófagos na cultura da seringueira [Hevea brasiliensis (Wild. Ex Adr. de Juss.) Müell.Arg.]

Pós-graduação em Agronomia - FEIS

Efeito do Diabetes mellitus e da insulinoterapia na osseointegração estabelecida ao redor de implantes instalados em tíbia de ratos

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Haplologia no falar paraense

O presente trabalho trata do fenômeno da Haplologia na fala espontânea de cidadãos paraenses. O estudo refere-se mais especificamente ao que chamamos de Haplologia entre frases. Avaliam-se os contextos de frases compostas apenas por /d/ - /d/, /t/ - /d/,/t/ - /t/ e /d/ - /t/, exemplificados respectivamente por: la(du) dʒi fora, per(tu) du, a gen(t∫i) t∫inha medu e tu(du) t∫inha. Os fatores avaliados dividem-se em dois grupos: linguísticos e extralinguísticos com o objetivo de mostrar os contextos favoráveis e desfavoráveis à aplicação do fenômeno em estudo. Os grupos de fatores linguísticos são: Relação entre palatalização e haplologia; Qualidade das vogais; Classe de palavra da sílaba elidida; Tonicidade das sílabas confinantes; e Estrutura silábica. No que se refere aos fatores extralinguísticos, analisamos: Sexo, Faixa etária e Escolaridade, seguindo a estratificação proposta no projeto Atlas Linguístico do Pará (ALIPA). Os dados analisados integram o corpus de duas cidades paraenses: Belém, a capital do Estado do Pará, e Itaituba, cidade paraense que fica a 891 km da capital mencionada. A coleta dos dados seguiu a orientação da Sociolinguística Variacionista. Os dados foram submetidos ao Programa de regra variável VARBRUL. Os resultados apontaram a haplologia como regra variável, entretanto, o fenômeno é pouco produtivo entre os informantes das duas cidades. Nos pressupostos da Sociolinguística Variacionista (Labov, 2008) a palatalização, o alteamento da vogal e a desconstrução do grupo consoantal podem ser considerados um processo de encaixamento, enquanto que, do ponto de vista fonético-fonológico, seriam considerados regras alimentadoras da haplologia (BISOL, 1996).

A ring system detected around the Centaur (10199) Chariklo

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

Ecological relevance of sentinels' biomarker responses: A multi-level approach

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

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.

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.