COMUNICAÇÃO & ASTRONOMIA: UMA UNIÃO VIRTUAL Estudos para uma teoria de comunicação organizacional on-line a partir do caso Rede de Astronomia Observacional REA/Brasil

A tese Comunicação & Astronomia, uma união virtual aborda o universo da comunicação virtual, das organizações virtuais, da ciência virtual. Um universo novo e emocionante onde a relação assíncrona espaço-temporal é o fator comum a todos os atores sociais envolvidos. O universo do virtual, das ferramentas de comunicação relacionadas às novas tecnologias, do ciberespaço, da existência concreta de uma organização imaterial. Estes elementos abrem novos horizontes para o conhecimento e compreensão dos processos de comunicação humana e organizacional na era da revolução informacional, proporcionando a oportunidade de estabelecer uma teoria de comunicação organizacional on line. A pesquisa bibliográfica apoiou-se em três bases teóricas de referência: a comunicação mediada por computador, comunicação virtual e comunicação organizacional, estas bases tiveram ainda o suporte de um estudo de caso que constituiu o corpus da pesquisa. Pudemos então compreender como ocorre a comunicação em uma organização virtual, seus processos, ferramentas e pontos cruciais que podem ser resumidos no fator motivacional necessário ao estímulo à interação virtual cooperativa, necessidade de construção e manutenção de imagem institucional forte que delimite a organização no ciberespaço e definição clara dos códigos de conduta da organização virtual.(AU)

COMUNICAÇÃO & ASTRONOMIA: UMA UNIÃO VIRTUAL Estudos para uma teoria de comunicação organizacional on-line a partir do caso Rede de Astronomia Observacional REA/Brasil

A tese Comunicação & Astronomia, uma união virtual aborda o universo da comunicação virtual, das organizações virtuais, da ciência virtual. Um universo novo e emocionante onde a relação assíncrona espaço-temporal é o fator comum a todos os atores sociais envolvidos. O universo do virtual, das ferramentas de comunicação relacionadas às novas tecnologias, do ciberespaço, da existência concreta de uma organização imaterial. Estes elementos abrem novos horizontes para o conhecimento e compreensão dos processos de comunicação humana e organizacional na era da revolução informacional, proporcionando a oportunidade de estabelecer uma teoria de comunicação organizacional on line. A pesquisa bibliográfica apoiou-se em três bases teóricas de referência: a comunicação mediada por computador, comunicação virtual e comunicação organizacional, estas bases tiveram ainda o suporte de um estudo de caso que constituiu o corpus da pesquisa. Pudemos então compreender como ocorre a comunicação em uma organização virtual, seus processos, ferramentas e pontos cruciais que podem ser resumidos no fator motivacional necessário ao estímulo à interação virtual cooperativa, necessidade de construção e manutenção de imagem institucional forte que delimite a organização no ciberespaço e definição clara dos códigos de conduta da organização virtual.(AU)

Methods of Visualization and Analysis of Cardiac Depolarization in the Three Dimensional Space

Research analysis of electrocardiograms (ECG) today is carried out mostly using time depending signals of different leads shown in the graphs. Definition of ECG parameters is performed by qualified personnel, and requiring particular skills. To support decoding the cardiac depolarization phase of ECG there are methods to analyze space-time convolution charts in three dimensions where the heartbeat is described by the trajectory of its electrical vector. Based on this, it can be assumed that all available options of the classical ECG analysis of this time segment can be obtained using this technique. Investigated ECG visualization techniques in three dimensions combined with quantitative methods giving additional features of cardiac depolarization and allow a better exploitation of the information content of the given ECG signals.

COMUNICAÇÃO & ASTRONOMIA: UMA UNIÃO VIRTUAL Estudos para uma teoria de comunicação organizacional on-line a partir do caso Rede de Astronomia Observacional REA/Brasil

A tese Comunicação & Astronomia, uma união virtual aborda o universo da comunicação virtual, das organizações virtuais, da ciência virtual. Um universo novo e emocionante onde a relação assíncrona espaço-temporal é o fator comum a todos os atores sociais envolvidos. O universo do virtual, das ferramentas de comunicação relacionadas às novas tecnologias, do ciberespaço, da existência concreta de uma organização imaterial. Estes elementos abrem novos horizontes para o conhecimento e compreensão dos processos de comunicação humana e organizacional na era da revolução informacional, proporcionando a oportunidade de estabelecer uma teoria de comunicação organizacional on line. A pesquisa bibliográfica apoiou-se em três bases teóricas de referência: a comunicação mediada por computador, comunicação virtual e comunicação organizacional, estas bases tiveram ainda o suporte de um estudo de caso que constituiu o corpus da pesquisa. Pudemos então compreender como ocorre a comunicação em uma organização virtual, seus processos, ferramentas e pontos cruciais que podem ser resumidos no fator motivacional necessário ao estímulo à interação virtual cooperativa, necessidade de construção e manutenção de imagem institucional forte que delimite a organização no ciberespaço e definição clara dos códigos de conduta da organização virtual.(AU)

Statistical mechanics of broadcast channels using low-density parity-check codes

We investigate the use of Gallager's low-density parity-check (LDPC) codes in a degraded broadcast channel, one of the fundamental models in network information theory. Combining linear codes is a standard technique in practical network communication schemes and is known to provide better performance than simple time sharing methods when algebraic codes are used. The statistical physics based analysis shows that the practical performance of the suggested method, achieved by employing the belief propagation algorithm, is superior to that of LDPC based time sharing codes while the best performance, when received transmissions are optimally decoded, is bounded by the time sharing limit.

Numerical Solution of Fractional Diffusion-Wave Equation with two Space Variables by Matrix Method

Mathematics Subject Classi¯cation 2010: 26A33, 65D25, 65M06, 65Z05.

Moduli Space of (0,2) Conformal Field Theories

In this thesis we study aspects of (0,2) superconformal field theories (SCFTs), which are suitable for compactification of the heterotic string. In the first part, we study a class of (2,2) SCFTs obtained by fibering a Landau-Ginzburg (LG) orbifold CFT over a compact K\"ahler base manifold. While such models are naturally obtained as phases in a gauged linear sigma model (GLSM), our construction is independent of such an embedding. We discuss the general properties of such theories and present a technique to study the massless spectrum of the associated heterotic compactification. We test the validity of our method by applying it to hybrid phases of GLSMs and comparing spectra among the phases. In the second part, we turn to the study of the role of accidental symmetries in two-dimensional (0,2) SCFTs obtained by RG flow from (0,2) LG theories. These accidental symmetries are ubiquitous, and, unlike in the case of (2,2) theories, their identification is key to correctly identifying the IR fixed point and its properties. We develop a number of tools that help to identify such accidental symmetries in the context of (0,2) LG models and provide a conjecture for a toric structure of the SCFT moduli space in a large class of models. In the final part, we study the stability of heterotic compactifications described by (0,2) GLSMs with respect to worldsheet instanton corrections to the space-time superpotential following the work of Beasley and Witten. We show that generic models elude the vanishing theorem proved there, and may not determine supersymmetric heterotic vacua. We then construct a subclass of GLSMs for which a vanishing theorem holds.

Dealing with crisis: Early childhood teachers perceived role in supporting children

The study explored how two experienced early childhood teachers support children dealing with crisis in their home environment, namely divorce, domestic violence and imprisonment of parents. The focus was on the relationship between the educational environment (organisation of space, time and relationships in an ecological perspective) and children's emotional well-being. This study builds on studies in Portugal about emotional well-being (Portugal & Laevers, 2010) and about the impact on children from imprisoned parents (Afonso, 2005, Kominsky, Pinto & Miyashiro, 2005, Tavares, 2011), domestic violence (Batista, 2014, Lisboa et al., 2002, Ribeiro, 2010) and divorce (Martons, 2010, Rego, 2008). The theoretical framework was weaved with Laevers (2004) concepts of emotional well-being and involvement and Siraj-Blatchford (2002) and Figueiredo (2013) perspective of pedagogy as including different dimensions of which the educational environment is essential. In-depth interviews with both teachers and some observations of their classroom dynamics were analysed for emerging cross themes in this qualitative study. Anonymity was preserved throughout the study by the use of codes. The study was presented to the teachers and questions were presented in advance. Both teachers expressed preference for adapting existing pedagogical tools (e.g. the classroom diary) and the daily dynamic to support children instead of using special interventions. Domestic violence was seen as the most problematic situation for its repercussions. Attention to emotional well-being, a strong relationship with the child and the families was highlighted. Pedagogy was described as answering different challenges, with a strong emphasis on children's participation. Thematising teachers' pedagogical knowledge is important.

First Description of a Cluster of Acute/Subacute Paracoccidioidomycosis Cases and Its Association with a Climatic Anomaly

Background: Identifying clusters of acute paracoccidioidomycosis cases could potentially help in identifying the environmental factors that influence the incidence of this mycosis. However, unlike other endemic mycoses, there are no published reports of clusters of paracoccidioidomycosis. Methodology/Principal Findings: A retrospective cluster detection test was applied to verify if an excess of acute form (AF) paracoccidioidomycosis cases in time and/or space occurred in Botucatu, an endemic area in Sao Paulo State. The scan-test SaTScan v7.0.3 was set to find clusters for the maximum temporal period of 1 year. The temporal test indicated a significant cluster in 1985 (P<0.005). This cluster comprised 10 cases, although 2.19 were expected for this year in this area. Age and clinical presentation of these cases were typical of AF paracccidioidomycosis. The space-time test confirmed the temporal cluster in 1985 and showed the localities where the risk was higher in that year. The cluster suggests that some particularities took place in the antecedent years in those localities. Analysis of climate variables showed that soil water storage was atypically high in 1982/83 (similar to 2.11/2.5 SD above mean), and the absolute air humidity in 1984, the year preceding the cluster, was much higher than normal (similar to 1.6 SD above mean), conditions that may have favored, respectively, antecedent fungal growth in the soil and conidia liberation in 1984, the probable year of exposure. These climatic anomalies in this area was due to the 1982/83 El Nino event, the strongest in the last 50 years. Conclusions/Significance: We describe the first cluster of AF paracoccidioidomycosis, which was potentially linked to a climatic anomaly caused by the 1982/83 El Nino Southern Oscillation. This finding is important because it may help to clarify the conditions that favor Paracoccidioides brasiliensis survival and growth in the environment and that enhance human exposure, thus allowing the development of preventive measures.

Suppression of away-side jet fragments with respect to the reaction plane in Au plus Au collisions at root s(NN)=200 GeV

Pair correlations between large transverse momentum neutral pion triggers (p(T) = 4-7 GeV/c) and charged hadron partners (p(T) = 3-7 GeV/c) in central (0%-20%) and midcentral (20%-60%) Au + Au collisions at root s(NN) = 200 GeV are presented as a function of trigger orientation with respect to the reaction plane. The particles are at larger momentum than where jet shape modifications have been observed, and the correlations are sensitive to the energy loss of partons traveling through hot densematter. An out-of-plane trigger particle produces only 26 +/- 20% of the away-side pairs that are observed opposite of an in-plane trigger particle for midcentral (20%-60%) collisions. In contrast, near-side jet fragments are consistent with no suppression or dependence on trigger orientation with respect to the reaction plane. These observations are qualitatively consistent with a picture of little near-side parton energy loss either due to surface bias or fluctuations and increased away-side parton energy loss due to a long path through the medium. The away-side suppression as a function of reaction-plane angle is shown to be sensitive to both the energy loss mechanism and the space-time evolution of heavy-ion collisions.

On the mixing property for a class of states of relativistic quantum fields

Let omega be a factor state on the quasilocal algebra A of observables generated by a relativistic quantum field, which, in addition, satisfies certain regularity conditions [satisfied by ground states and the recently constructed thermal states of the P(phi)(2) theory]. We prove that there exist space- and time-translation invariant states, some of which are arbitrarily close to omega in the weak * topology, for which the time evolution is weakly asymptotically Abelian. (C) 2010 American Institute of Physics. [doi: 10.1063/1.3372623]

Perturbations of black p-branes

We consider black p-brane solutions of the low-energy string action, computing scalar perturbations. Using standard methods, we derive the wave equations obeyed by the perturbations and treat them analytically and numerically. We have found that tensorial perturbations obtained via a gauge-invariant formalism leads to the same results as scalar perturbations. No instability has been found. Asymptotically, these solutions typically reduce to a AdSd((p+2)) x Sd((8-p)) space which, in the framework of Maldacena's conjecture, can be regarded as a gravitational dual to a conformal field theory defined in a (p+1)-dimensional flat space-time. The results presented open the possibility of a better understanding the AdS/CFT correspondence, as originally formulated in terms of the relation among brane structures and gauge theories.

Aetherlike Lorentz-breaking actions

We show that CPT-even aetherlike Lorentz-breaking actions, for the scalar and electromagnetic fields, are generated via their appropriate Lorentz-breaking coupling to spinor fields, in three, four, and five space-time dimensions. Besides, we also show that aetherlike terms for the spinor field can be generated as a consequence of the same couplings. We discuss the dispersion relations in the theories with aetherlike Lorentz-breaking terms and find the tree-level effective (Breit) potential for fermion scattering and the one-loop effective potential corresponding to the action of the scalar field.

Instability of Higher-Dimensional Charged Black Holes in the de Sitter World

We have shown that higher-dimensional Reissner-Nordstrom-de Sitter black holes are gravitationally unstable for large values of the electric charge and cosmological constant in D >= 7 space-time dimensions. We have found the shape of the slightly perturbed black hole at the threshold point of instability.

Gravitational instability of simply rotating AdS black holes in higher dimensions

We study the stability of AdS black holes rotating in a single two-plane for tensor-type gravitational perturbations in D > 6 space-time dimensions. First, by an analytic method, we show that there exists no unstable mode when the magnitude a of the angular momentum is smaller than r(h)(2)/R, where r(h) is the horizon radius and R is the AdS curvature radius. Then, by numerical calculations of quasinormal modes, using the separability of the relevant perturbation equations, we show that an instability occurs for rapidly rotating black holes with a > r(h)(2)/R, although the growth rate is tiny (of order 10(-12) of the inverse horizon radius). We give numerical evidence indicating that this instability is caused by superradiance.