Study of Bose-Einstein Correlations in e+e- -> W+W- events at LEP

Bose-Einstein correlation between like-sign charged-particle pairs in e+e- -> W+W- events recorded with the OPAL detector at LEP at centre-of-mass energies between 183 GeV and 209 GeV are studied. Recently proposed methods which allow direct searches for correlations in the data via distributions of test variables are used to investigate the presence of correlations between hadrons originating from different W bosons in W+W- -> qqqq events. Within the statistics of the data sample no evidence for inter-WW Bose-Einstein correlations is obtained. The data are also compared with predictions of a recent implementation of Bose-Einstein correlation effects in the Monte Carlo model PYTHIA.Comment: 29 pages, 10 figures, Submitted to Eur. Phys. J.

Caracteres de produção e qualidade de clones de batata selecionados de população segregante para resistência ao vírus Y da batata.

bitstream/item/30412/1/boletim-67.pd

Near-Infrared Studies of V1280 Sco (Nova Scorpii 2007)

We present spectroscopic and photometric results of Nova V1280 Sco which was discovered in outburst in early 2007 February. The large number of spectra obtained of the object leads to one of the most extensive, near-infrared spectral studies of a classical nova. The spectra evolve from a P-Cygni phase to an emission-line phase and at a later stage is dominated by emission from the dust that formed in this nova. A detailed model is computed to identify and study characteristics of the spectral lines. Inferences from the model address the vexing question of which novae have the ability to form dust. It is demonstrated, and strikingly corroborated with observations, that the presence of lines in the early spectra of low-ionization species like Na and Mg - indicative of low temperature conditions - appear to be reliable indicators that dust will form in the ejecta. It is theoretically expected that mass loss during a nova outburst is a sustained process. Spectroscopic evidence for such a sustained mass loss, obtained by tracing the evolution of a P-Cygni feature in the Brackett gamma line, is presented here allowing a lower limit of 25-27 days to be set for the mass-loss duration. Photometric data recording the nova's extended 12 day climb to peak brightness after discovery is used to establish an early fireball expansion and also show that the ejection began well before maximum brightness. The JHK light curves indicate the nova had a fairly strong second outburst around 100 days after the first.Comment: Accepted in MNRAS. The paper contains 8 figures and 4 tables. Few typographical errors were correcte

Airway-centered interstitial fibrosis: etiology, clinical findings and prognosis

Background: Airway-centered Interstitial Fibrosis (ACIF) is a common pathologic pattern observed in our practice.Objectives: the objectives of this study are to describe the causes associated with ACIF in a large sample of patients and its effect on survival.Methods: A retrospective study in three centers of interstitial lung disease in São Paulo, between January of 1995 and December of 2012. the surgical lung biopsy specimens were reviewed by three pathologists. the clinical, functional and tomographic findings were analyzed by a standardized protocol.Results: There were 68 cases of ACIF, most of them women. the mean age was 57 +/- 12 yr. Dyspnea, cough, restrictive pattern at spirometry and oxygen desaturation at exercise were common. A reticular pattern with peribronchovascular infiltrates was found in 79% of the cases. the etiologies of ACIF were hypersensitivity pneumonitis in 29 (42.6%), gastroesophageal reflux disease in 17 (25.0%), collagen vascular disease in 4 (5.9%), a combination of them in 15 cases and idiopathic in 3 (4.4%). the median survival was 116 months (95% CI = 58.5 - 173.5). Lower values of oxygen saturation at rest, presence of cough and some histological findings - organizing tissue in the airways, fibroblastic foci and microscopic honeycombing - were predictors of worse survival.Conclusions: ACIF is an interstitial lung disease with a better survival when compared with IPF. the main etiologies are HP and GERD. the oxygen saturation at rest, the presence of cough and some histological findings are predictors of survival.Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)Universidade Federal de São Paulo, Dept Pulm, São Paulo, BrazilMayo Clin, Dept Pathol, Scottsdale, AZ USAUniversidade Federal de São Paulo, Dept Pathol, São Paulo, BrazilUniversidade Federal de São Paulo, Dept Pulm, São Paulo, BrazilUniversidade Federal de São Paulo, Dept Pathol, São Paulo, BrazilWeb of Scienc

Preferências do consumidor de batatas no sul do Estado do Rio Grande do Sul.

bitstream/item/31487/1/comunicado-212.pd

Expressão de caracteres de tubérculos em função do tamanho de recipiente usado no cultivo de batata na geração de plântulas.

No melhoramento genético de batata, para alguns caracteres, é possível eliminar genótipos inferiores já nas gerações iniciais, o que permite reduzir o número de genótipos avaliados a campo, proporcionando redução de custos. O objetivo deste trabalho foi verificar a influência do tamanho de vaso na expressão de caracteres de tubérculo, em famílias de batata, na geração de plântula. Em casa de vegetação, dez famílias de batata foram avaliadas em dois tamanhos de recipientes, vaso grande (1 L) e vaso pequeno (250 ml). Os caracteres de tubérculos avaliados foram: cor, aspereza, profundidade de olho, sobrancelha, formato, uniformidade de formato, apontamento, curvatura, achatamento, aparência geral, massa por planta, massa média e número de tubérculos. O vaso grande proporciona maior expressão da variação genética para os caracteres profundidade de olho, sobrancelha, curvatura, achatamento, aparência geral e todos os componentes de rendimento. As maiores médias de produção de tubérculos em número, tamanho e massa foram obtidas no vaso grande, enquanto o maior coeficiente de variação genético para os caracteres formato, uniformidade de formato e apontamento de tubérculo foi obtido no vaso pequeno

Mass extinctions and supernova explosions

A nearby supernova (SN) explosion could have negatively influenced life on Earth, maybe even been responsible for mass extinctions. Mass extinction poses a significant extinction of numerous species on Earth, as recorded in the paleontologic, paleoclimatic, and geological record of our planet. Depending on the distance between the Sun and the SN, different types of threats have to be considered, such as ozone depletion on Earth, causing increased exposure to the Sun's ultraviolet radiation, or the direct exposure of lethal x-rays. Another indirect effect is cloud formation, induced by cosmic rays in the atmosphere which result in a drop in the Earth's temperature, causing major glaciations of the Earth. The discovery of highly intensive gamma ray bursts (GRBs), which could be connected to SNe, initiated further discussions on possible life-threatening events in Earth's history. The probability that GRBs hit the Earth is very low. Nevertheless, a past interaction of Earth with GRBs and/or SNe cannot be excluded and might even have been responsible for past extinction events.Comment: Chapter for forthcoming book: Handbook of Supernovae, P. Murdin and A. Alsabeti (eds.), Springer International Publishing (in press

Water and ammonia abundances in S140 with the Odin satellite

We have used the Odin satellite to obtain strip maps of the ground-state rotational transitions of ortho-water and ortho-ammonia, as well as CO(5-4) and 13CO(5-4) across the PDR, and H218O in the central position. A physi-chemical inhomogeneous PDR model was used to compute the temperature and abundance distributions for water, ammonia and CO. A multi-zone escape probability method then calculated the level populations and intensity distributions. These results are compared to a homogeneous model computed with an enhanced version of the RADEX code. H2O, NH3 and 13CO show emission from an extended PDR with a narrow line width of ~3 kms. Like CO, the water line profile is dominated by outflow emission, however, mainly in the red wing. The PDR model suggests that the water emission mainly arises from the surfaces of optically thick, high density clumps with n(H2)>10^6 cm^-3 and a clump water abundance, with respect to H2, of 5x10^-8. The mean water abundance in the PDR is 5x10^-9, and between ~2x10^-8 -- 2x10^-7 in the outflow derived from a simple two-level approximation. Ammonia is also observed in the extended clumpy PDR, likely from the same high density and warm clumps as water. The average ammonia abundance is about the same as for water: 4x10^-9 and 8x10^-9 given by the PDR model and RADEX, respectively. The similarity of water and ammonia PDR emission is also seen in the almost identical line profiles observed close to the bright rim. Around the central position, ammonia also shows some outflow emission although weaker than water in the red wing. Predictions of the H2O(110-101) and (111-000) antenna temperatures across the PDR are estimated with our PDR model for the forthcoming observations with the Herschel Space Observatory.Comment: 13 pages, 14 figures, 10 tables. Accepted for publication in Astronomy & Astrophysics 14 November 200