4 resultados para Lua
em Biblioteca Digital da Produção Intelectual da Universidade de São Paulo
Resumo:
We aimed to investigate the role of betaine supplementation on muscle phosphorylcreatine (PCr) content and strength performance in untrained subjects. Additionally, we compared the ergogenic and physiological responses to betaine versus creatine supplementation. Finally, we also tested the possible additive effects of creatine and betaine supplementation. This was a double-blind, randomized, placebo-controlled study. Subjects were assigned to receive betaine (BET; 2 g/day), creatine (CR; 20 g/day), betaine plus creatine (BET + CR; 2 + 20 g/day, respectively) or placebo (PL). At baseline and after 10 days of supplementation, we assessed muscle strength and power, muscle PCr content, and body composition. The CR and BET + CR groups presented greater increase in muscle PCr content than PL ( = 0.004 and = 0.006, respectively). PCr content was comparable between BET versus PL ( = 0.78) and CR versus BET + CR ( = 0.99). CR and BET + CR presented greater muscle power output than PL in the squat exercise following supplementation ( = 0.003 and = 0.041, respectively). Similarly, bench press average power was significantly greater for the CR-supplemented groups. CR and BET + CR groups also showed significant pre- to post-test increase in 1-RM squat and bench press (CR: = 0.027 and < 0.0001; BET + CR: = 0.03 and < 0.0001 for upper- and lower-body assessments, respectively) No significant differences for 1-RM strength and power were observed between BET versus PL and CR versus BET + CR. Body composition did not differ between the groups. In conclusion, we reported that betaine supplementation does not augment muscle PCr content. Furthermore, we showed that betaine supplementation combined or not with creatine supplementation does not affect strength and power performance in untrained subjects.
Resumo:
A formação das classes sociais brasileiras de certo modo coincidiu com as hierarquias herdadas da colonização: os povos anteriormente conquistados ou escravizados, que passaram a ser definidos por meio da classificação por raças, nesse processo tornaram-se também subalternos. A extensão de direitos iguais para todos os membros da nação se constituiu igualmente de forma peculiar. Neste artigo, eu exploro o modo pelo qual as hierarquias sociais se mantiveram e se reproduziram no contexto em que a liberdade individual foi a base para a formação nacional, assim como a maneira com que os anseios históricos de liberdade cederam lugar, na motivação dos ativistas negros, à igualdade de oportunidades.
Resumo:
Este artigo analisa a emergência e difusão da regra da responsabilidade criminal individual por violações de direitos humanos a partir da jurisprudência contenciosa da Corte Interamericana de Direitos Humanos. Tendo como referência as pesquisas de Kathryn Sikkink sobre justiça de transição, procura-se identificar a maneira como o Sistema Interamericano de Direitos Humanos vem expandindo o sentido da responsabilidade criminal individual e também sugerir a incompatibilidade com a proteção dos direitos humanos que esse novo modelo pode ter.
Resumo:
In this communication we report results from the application to the study of the rotation of the Moon of the creeping tide theory just proposed (Ferraz-Mello, Cel. Mech. Dyn. Astron., submitted. ArXiv astro-ph 1204.3957). The choice of the Moon for the first application of this new theory is motivated by the fact that the Moon is one of the best observed celestial bodies and the comparison of the theoretical predictions of the theory with observations i may validate the theory or point out the need of further improvements. Particularly, the tidal perturbations of the rotation of the Moon - the physical libration of the Moon - have been detected in the Lunar Laser Ranging measurements (Williams et al. JGR 106, 27933, 2001). The major difficulty in this application comes from the fact that tidal torques in a planet-satellite system are very sensitive to the distance between the two-bodies, which is strongly affected by Solar perturbations. In the case of the Moon, the main solar perturbations - the Evection and the Variation - are more important than most of the Keplerian oscillations, being smaller only than the first Keplerian harmonic (equation of the centre). Besides, two of the three components of the Moon's libration in longitude whose tidal contributions were determined by LLR are related to these perturbations. The results may allow us to determine the main parameter of a possible Moon's creeping tide. The preliminary results point to a relaxation factor (gamma) 2 to 4 times smaller than the one predicted from the often cited values of thr Moon's quality factor Q (between 30 and 40), and points to larger Q values.