Aspectos econômicos do cajueiro.

bitstream/item/90085/1/ADM13001.pdfCampo & Negócio

Proposal to study Bs→DˉsJB_s \to \bar D_{sJ} transitions

It is proposed to clear some of the puzzles of B decay to the broad $\bar{D}^{\ast\ast}$ states by studying the corresponding decay with strange states $B_s^0 \to D_{s0}^{\ast -} \pi^+$ at LHCb. Interpretation of the results should be easier due to the narrowness of the $D_{s0}^{\ast -}$ state.Comment: 21 page

Study of Recurrent Miscarriage. Is Hysterosalpingography Necessary?

Overview and Aims: The investigation of recurrent miscarriage includes the study of uterine morphology. 3D ultrasound allows the evaluation of the morphology (cavity and outer contour), reducing the need for invasive tests such as hystero - salpingography (HSG), hysteroscopy and laparoscopy. We evaluated the diagnostic agreement between HSG and 3D ultrasound in the study of the uterine cavity morphology. Study Design: Prospective study. Population: A total of 34 women referred to our institution with a history of recurrent miscarriage. Methods: To compare the results of 3D ultrasound and HSG, all women underwent both exams. 3D scans were performed by the same operator and HSG were evaluated by the same clinician. The concordance study was performed using the Kappa coefficient. Results: With 3D ultrasound and HSG, uterine anomalies were diagnosed in 52.9% (18/34) and 47% (16/34) of the cases and congenital malformations were the most frequent findings. The agreement between the two techniques was excellent(K = 0.825). The three cases of diagnostic disagreement were analyzed. Conclusion: A high level of diagnostic agreement was observed between HSG and 3D ultrasound. The 3D ultrasound, a low cost and well tolerated technique, when performed by an experienced operator, is the first line exam to study the uterine morphology in women with recurrent miscarriage

Características fenológicas e produtivas da goiabeira "paluma" podada em diferentes épocas e intensidades no norte fluminense.

A poda de frutificação na goiabeira proporciona a produção de frutos na entres safra, mas a previsão de colheita depende da época de sua realização, além das condições edafoclimáticas. Neste trabalho, são apresentados dados sobre a fenologia e a produção da goiabeira 'Paluma', submetida a diferentes épocas e intensidades de poda de frutificação, em São Francisco do Itabapoana, RJ. O experimento foi realizado em delineamento inteiramente casualizado, e os tratamentos foram distribuídos em esquema de parcelas subdivididas, com as parcelas compostas pelas épocas de poda, realizadas nos meses de agosto, outubro, dezembro e fevereiro; e as subparcelas pelas intensidades de poda (curta, média e longa). O ciclo da goiabeira' Paluma', da poda à colheita dos frutos, variou de 168 dias para a poda realizada em outubro a 210 dias para a realizada em fevereiro. A poda longa, realizada em agosto, proporcionou maior número de ramos produtivos e maior número de frutos por ramo. A intensidade da poda afetou o crescimento dos ramos novos, mas não influenciou no tamanho dos frutos. A maior produção de frutos ocorreu nas plantas podadas em dezembro

Fluctuating hydrodynamic modelling of fluids at the nanoscale

A good representation of mesoscopic fluids is required to combine with molecular simulations at larger length and time scales (De Fabritiis {\it et. al}, Phys. Rev. Lett. 97, 134501 (2006)). However, accurate computational models of the hydrodynamics of nanoscale molecular assemblies are lacking, at least in part because of the stochastic character of the underlying fluctuating hydrodynamic equations. Here we derive a finite volume discretization of the compressible isothermal fluctuating hydrodynamic equations over a regular grid in the Eulerian reference system. We apply it to fluids such as argon at arbitrary densities and water under ambient conditions. To that end, molecular dynamics simulations are used to derive the required fluid properties. The equilibrium state of the model is shown to be thermodynamically consistent and correctly reproduces linear hydrodynamics including relaxation of sound and shear modes. We also consider non-equilibrium states involving diffusion and convection in cavities with no-slip boundary conditions

Early Science with the Large Millimetre Telescope: Molecules in the Extreme Outflow of a proto-Planetary Nebula

Extremely high velocity emission likely related to jets is known to occur in some proto-Planetary Nebulae. However, the molecular complexity of this kinematic component is largely unknown. We observed the known extreme outflow from the proto-Planetary Nebula IRAS 16342-3814, a prototype water fountain, in the full frequency range from 73 to 111 GHz with the RSR receiver on the Large Millimetre Telescope. We detected the molecules SiO, HCN, SO, and $^{13}$CO. All molecular transitions, with the exception of the latter are detected for the first time in this source, and all present emission with velocities up to a few hundred km s$^{-1}$. IRAS 16342-3814 is therefore the only source of this kind presenting extreme outflow activity simultaneously in all these molecules, with SO and SiO emission showing the highest velocities found of these species in proto-Planetary Nebulae. To be confirmed is a tentative weak SO component with a FWHM $\sim$ 700 km s$^{-1}$. The extreme outflow gas consists of dense gas (n$_{\rm H_2} >$ 10$^{4.8}$--10$^{5.7}$ cm$^{-3}$), with a mass larger than $\sim$ 0.02--0.15 M$_{\odot}$. The relatively high abundances of SiO and SO may be an indication of an oxygen-rich extreme high velocity gas.Comment: Accepted for publication in Monthly Notices of the Royal Astronomical Society Letter