Comportamento à flexão de vigas eco-eficientes de ultra elevada durabilidade

Atualmente, o ecossistema mundial tem vindo a ser confrontado com problemas de grande importância, a elevada poluição do meio ambiente e a limitação dos recursos energéticos. Estes problemas têm contribuído para que a sustentabilidade da construção seja uma prioridade cada vez maior no presente e no futuro. A manutenção e a reabilitação do património construído surge como uma das medidas mais eficazes para prevenir ou reduzir o consumo de energia no setor da construção. No caso da construção nova, a tendência é para verificar-se um aumento da utilização de elementos estruturais pré-fabricados com partes betonadas em obra, obtendose uma maior rapidez de execução associada a um maior controlo de qualidade. O betão de ultra elevada durabilidade, reforçado com fibras metálicas, é considerado um material inovador desenvolvido nas últimas décadas, apresentando um conjunto de caraterísticas especiais, como a durabilidade, a facilidade de aplicação, as elevadas resistências mecânicas, tornando-o num produto particularmente atraente para a reabilitação e reforço de estruturas de betão. No entanto, este betão não deve ser produzido em grandes quantidades devido ao elevado consumo de cimento e adições, resultando em elevados custos económicos e ambientais. Considerando estas desvantagens é proposto que o betão de ultra elevada durabilidade seja usado apenas na camada de recobrimento, formando-se assim uma superskin que protege o elemento estrutural dos ambientes mais agressivos, isto é, aumenta a durabilidade das estruturas de betão sem que, no entanto, seja criado um impacte ambiental muito significativo (a quantidade de CO2 libertada para a atmosfera é menor devido ao menor consumo de cimento e adições). A presente dissertação pretende explorar o conceito de superskin do ponto de vista do comportamento estrutural, nomeadamente, estudar o comportamento de vigas sujeitas a esforços de flexão, compostas por uma camada exterior de betão de ultra elevada durabilidade, associado a um núcleo com betão eco-eficiente, com baixa dosagem de cimento, de modo a obter uma solução mais durável e ao mesmo tempo, ecologicamente mais eficiente. Foram realizadas oito vigas com diferentes taxas de armadura: quatro vigas produzidas apenas com betão com baixa dosagem de cimento (usadas como vigas de referência) e quatro vigas produzidas com um betão de ultra elevada durabilidade na camada de recobrimento e com um betão com baixa dosagem de cimento no núcleo. As diferentes taxas de armadura longitudinal permitem avaliar a influência da superskin em vigas com roturas dúcteis e frágeis. Com base nos dados recolhidos durante os ensaios experimentais estudou-se: (i) relação cargadeslocamento; (ii) os valores teóricos e experimentais do momento resistente; (iii) a evolução da curvatura nas secções críticas; (iv) a evolução da rigidez à flexão com a carga aplicada; (v) a ductilidade; e (vi) a fendilhação e o tipo de rotura. Da análise de resultados foi possível verificar que o recobrimento em betão de ultra elevada durabilidade é uma solução com aspetos muito positivos, nomeadamente, aumenta a resistência à flexão das vigas

ω−ρ\omega-\rho Mixing and the ω→ππγ\omega\to\pi\pi\gamma Decay

We reexamine the $\omega \to \pi^{0} \pi^{0} \gamma$ decay, adding the effect of $\omega-\rho$ mixing to the amplitude calculated with the aid of chiral perturbation theory and vector meson dominance. We predict the neutral decay to occur with a width of $\Gamma($\omega \to \pi^{0} \pi^{0} \gamma $) =(390\pm96) {\rm eV}$ and also analyze the effect of the $\omega-\rho$ mixing on the $\Gamma($\omega \to \pi^{0} \pi^{0} \gamma $)/ \Gamma($\omega \to \pi^{+} \pi^{-} \gamma $)$ ratio. Several remarks on the effect of $\omega-\rho$ mixing on certain radiative decays of vector mesons are presented.Comment: 10 pages, LaTeX, 1 ps-figure. Submitted to Phys. Rev.

Tri-meson-mixing of π\pi-η\eta-η′\eta' and ρ\rho-ω\omega-ϕ\phi in the light-cone quark model

The radiative transition form factors of the pseudoscalar mesons {$\pi$, $\eta$, $\eta'$} and the vector mesons {$\rho$, $\omega$, $\phi$} are restudied with $\pi$-$\eta$-$\eta'$ and $\rho$-$\omega$-$\phi$ in tri-meson-mixing pattern, which is described by tri-mixing matrices in the light-cone constituent quark model. The experimental transition decay widths are better reproduced with tri-meson-mixing than previous results in a two-mixing-angle scenario of only two-meson $\eta$-$\eta'$ mixing and $\omega$-$\phi$ mixing.Comment: 8 pages, 6 figures, final version to appear in EPJ

Radiative Decays, Nonet Symmetry and SU(3) Breaking

We re-examine the problem of simultaneously describing in a consistent way all radiative and leptonic decays of light mesons (V -> P gamma, P -> V gamma, P -> gamma gamma, V -> e^+ e^-). For this purpose, we rely on the Hidden Local Symmetry model in both its anomalous and non--anomalous sectors. We show that the SU(3) symmetry breaking scheme proposed by Bando, Kugo and Yamawaki, supplemented with nonet symmetry breaking in the pseudoscalar sector, allows one to reach a nice agreement with all data, except for the K^{*+/-} radiative decay. An extension of this breaking pattern allows one to account for this particular decay mode too. Considered together, the whole set of radiative decays provides a pseudoscalar mixing angle theta_P ~ -11^o and a value for theta_V which is ~ 3^o from that of ideal mixing. We also show that it is impossible, in a practical sense, to disentangle the effects of nonet symmetry breaking and those of glue inside the eta', using only light meson decays.Comment: 36 pages. Published versio

Horizontal Branch Stars: The Interplay between Observations and Theory, and Insights into the Formation of the Galaxy

We review HB stars in a broad astrophysical context, including both variable and non-variable stars. A reassessment of the Oosterhoff dichotomy is presented, which provides unprecedented detail regarding its origin and systematics. We show that the Oosterhoff dichotomy and the distribution of globular clusters (GCs) in the HB morphology-metallicity plane both exclude, with high statistical significance, the possibility that the Galactic halo may have formed from the accretion of dwarf galaxies resembling present-day Milky Way satellites such as Fornax, Sagittarius, and the LMC. A rediscussion of the second-parameter problem is presented. A technique is proposed to estimate the HB types of extragalactic GCs on the basis of integrated far-UV photometry. The relationship between the absolute V magnitude of the HB at the RR Lyrae level and metallicity, as obtained on the basis of trigonometric parallax measurements for the star RR Lyrae, is also revisited, giving a distance modulus to the LMC of (m-M)_0 = 18.44+/-0.11. RR Lyrae period change rates are studied. Finally, the conductive opacities used in evolutionary calculations of low-mass stars are investigated. [ABRIDGED]Comment: 56 pages, 22 figures. Invited review, to appear in Astrophysics and Space Scienc

The composition and weathering of the continents over geologic time

The composition of continental crust records the balance between construction by tectonics and destruction by physical and chemical erosion. Quantitative constraints on how igneous addition and chemical weathering have modified the continents’ bulk composition are essential for understanding the evolution of geodynamics and climate. Using novel data analytic techniques we have extracted temporal trends in sediments’ protolith composition and weathering intensity from the largest available compilation of sedimentary major element compositions: ∼15,000 samples from 4.0 Ga to the present. We find that the average Archean upper continental crust was silica-rich and had a similar compositional diversity to modern continents. This is consistent with an early Archean, or earlier, onset of plate tectonics. In the Archean, chemical weathering sequestered ∼25 % more CO2 per mass eroded for the same weathering intensity than in subsequent time periods, consistent with carbon mass balance despite higher Archean outgassing rates and more limited continental exposure. Since 2.0 Ga, over long (>0.5 Gyr) timescales, crustal weathering intensity has remained relatively constant. On shorter timescales over the Phanerozoic, weathering intensity is correlated to global climate state, consistent with a weathering feedback acting in response to changes in CO2 sources or sinks

Associations of autozygosity with a broad range of human phenotypes

In many species, the offspring of related parents suffer reduced reproductive success, a phenomenon known as inbreeding depression. In humans, the importance of this effect has remained unclear, partly because reproduction between close relatives is both rare and frequently associated with confounding social factors. Here, using genomic inbreeding coefficients (F-ROH) for >1.4 million individuals, we show that F-ROH is significantly associated (p <0.0005) with apparently deleterious changes in 32 out of 100 traits analysed. These changes are associated with runs of homozygosity (ROH), but not with common variant homozygosity, suggesting that genetic variants associated with inbreeding depression are predominantly rare. The effect on fertility is striking: F-ROH equivalent to the offspring of first cousins is associated with a 55% decrease [95% CI 44-66%] in the odds of having children. Finally, the effects of F-ROH are confirmed within full-sibling pairs, where the variation in F-ROH is independent of all environmental confounding.Peer reviewe

Multi-ancestry study of blood lipid levels identifies four loci interacting with physical activity

Many genetic loci affect circulating lipid levels, but it remains unknown whether lifestyle factors, such as physical activity, modify these genetic effects. To identify lipid loci interacting with physical activity, we performed genome-wide analyses of circulating HDL cholesterol, LDL cholesterol, and triglyceride levels in up to 120,979 individuals of European, African, Asian, Hispanic, and Brazilian ancestry, with follow-up of suggestive associations in an additional 131,012 individuals. We find four loci, in/near CLASP1, LHX1, SNTA1, and CNTNAP2, that are associated with circulating lipid levels through interaction with physical activity; higher levels of physical activity enhance the HDL cholesterol-increasing effects of the CLASP1, LHX1, and SNTA1 loci and attenuate the LDL cholesterol- increasing effect of the CNTNAP2 locus. The CLASP1, LHX1, and SNTA1 regions harbor genes linked to muscle function and lipid metabolism. Our results elucidate the role of physical activity interactions in the genetic contribution to blood lipid levels