11,488 research outputs found
As redes sociais e as mediações tecnológicas na comunicação interna das organizações: dificuldades e oportunidades.
Agroecologia e desenvolvimento sustentável.
O desenvolvimento sustentável tem suas bases conceituais assentadas na Agenda XXI de 1992, que será revisitada na Rio +20, em junho de 2012, como resultado do pacto firmado pelas Nações Unidas com o mundo, para enfrentar os desafios socioambientais e econômicos decorrentes da crise mundial iniciada na década de 1970. Assim, nos últimos 20 anos, todo o sistema econômico vem tentando se ajustar ao que é denominado desenvolvimento sustentável
Métodos para superar a dormência tegumentar em sementes de jurema-preta (Mimosa hostilis Benth.).
Este trabalho foi realizado com o objetivo de avaliar a eficiência de tratamentos físicos e químicos na germinação e no vigor (Índice de Velocidade de Germinação – IVG), em sementes de jurema-preta (Mimosa hostilis Benth.). Os tratamentos testados foram: sementes imersas em H2SO4 (98%) por 1, 5, 10 e 15 minutos; em água, a 100oC, por 1 e 3 minutos; em água à temperatura ambiente, por 36 e 72 horas; escarificação mecânica, por 20 e 40 segundos; choque térmico em estufa a 55oC por 24 e 48 horas e sementes em condições naturais. Os resultados obtidos que a escarificação ácida por 5 a 15 minuts, e a mecânica, por 20 a 40 segundos, mostraram-se mais eficientes na quebra da dormência de sementes dessa espécie
Cosmological constant constraints from observation-derived energy condition bounds and their application to bimetric massive gravity
Among the various possibilities to probe the theory behind the recent
accelerated expansion of the universe, the energy conditions (ECs) are of
particular interest, since it is possible to confront and constrain the many
models, including different theories of gravity, with observational data. In
this context, we use the ECs to probe any alternative theory whose extra term
acts as a cosmological constant. For this purpose, we apply a model-independent
approach to reconstruct the recent expansion of the universe. Using Type Ia
supernova, baryon acoustic oscillations and cosmic-chronometer data, we perform
a Markov Chain Monte Carlo analysis to put constraints on the effective
cosmological constant . By imposing that the cosmological
constant is the only component that possibly violates the ECs, we derive lower
and upper bounds for its value. For instance, we obtain that and within,
respectively, and confidence levels. In addition, about
30\% of the posterior distribution is incompatible with a cosmological
constant, showing that this method can potentially rule it out as a mechanism
for the accelerated expansion. We also study the consequence of these
constraints for two particular formulations of the bimetric massive gravity.
Namely, we consider the Visser's theory and the Hassan and Roses's massive
gravity by choosing a background metric such that both theories mimic General
Relativity with a cosmological constant. Using the
observational bounds along with the upper bounds on the graviton mass we obtain
constraints on the parameter spaces of both theories.Comment: 11 pages, 4 figures, 1 tabl
The conservation of energy-momentum and the mass for the graviton
In this work we give special attention to the bimetric theory of gravitation
with massive gravitons proposed by Visser in 1998. In his theory, a prior
background metric is necessary to take in account the massive term. Although in
the great part of the astrophysical studies the Minkowski metric is the best
choice to the background metric, it is not possible to consider this metric in
cosmology. In order to keep the Minkowski metric as background in this case, we
suggest an interpretation of the energy-momentum conservation in Visser's
theory, which is in accordance with the equivalence principle and recovers
naturally the special relativity in the absence of gravitational sources.
Although we do not present a general proof of our hypothesis we show its
validity in the simple case of a plane and dust-dominated universe, in which
the `massive term' appears like an extra contribution for the energy density.Comment: 9 pages, accepted for publishing in GR
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