952 resultados para gravity gradient
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Due to its underlying gauge structure, teleparallel gravity achieves a separation between inertial and gravitational effects. It can, in consequence, describe the isolated gravitational interaction without resorting to the equivalence principle, and is able to provide a tensorial definition for the energy-momentum density of the gravitational field. Considering the conceptual conflict between the local equivalence principle and the nonlocal uncertainty principle, the replacement of general relativity by its teleparallel equivalent can be considered an important step towards a prospective reconciliation between gravitation and quantum mechanics. © 2006 American Institute of Physics.
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Running water is one of the most important of all the physical processes which fashion the landscape, allowing gravity to operate along the valley floors. Besides this, the streams show a fast adjustment to the crustal deformations, even to the most gentle ones. This geologic behavior turns them a potential tool for neotectonic studies, specially the analysis of morphotnetric parameters associated with hydraulic gradient and discharge, this second factor being directly proportional to the extension of the streams. Both elements, gradient and stream length, can be combined in the SL index. The purpose of this paper is to show the RDE index application in the neotectonics analysis of the Rio do Peixe hydrographic basin and to compare the obtained values with the geologic basement incised by the streams. This basement encompasses Cretaceous sedimentary rocks of post-Serra Oeral Formation magmatism (Caiuá and Bauru groups) and Quaternary deposits that include chiefly recent alluvial plains and some Pleistocene terrace deposits. In the final part of this paper, an attempt is made in order to correlate the RDE results and the neotectonic framework admitted to this portion of the São Paulo State territory, as well as with field geologic, seismologic and paleoseismologic known elements. The results indicate the presence of two groups of anomalies: The first set corresponds to the Marília-Exaporã Plateau border, and the second one, located in the central portion of the hydrographic basin, is correlated to the Presidente Prudente seimogenic zone.
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The gravitational properties of a straight cosmic string are studied in the linear approximation of higher-derivative gravity. These properties are shown to be very different from those found using linearized Einstein gravity: there exists a short range gravitational (anti-gravitational) force in the nonrelativistic limit; in addition, the deflection angle of a light ray moving in a plane orthogonal to the string depends on the impact parameter. © 2008 World Scientific Publishing Company.
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We derive an one-parameter family of consistency conditions to braneworlds in the Brans-Dicke gravity. The General Relativity case is recovered by taking a correct limit of the Brans-Dicke parameter. We show that it is possible to build a multiple AdS brane scenario in a six-dimensional bulk only if the brane tensions are negative. Besides, in the five-dimensional case, it is showed that no fine tuning is necessary between the bulk cosmological constant and the brane tensions, in contrast to the Randall-Sundrum model. Copyright © owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial- ShareAlike Licence.
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In this work we study a Hořava-like 5-dimensional model in the context of braneworld theory. The equations of motion of such model are obtained and, within the realm of warped geometry, we show that the model is consistent if and only if λ takes its relativistic value 1. Furthermore, we show that the elimination of problematic terms involving the warp factor second order derivatives are eliminated by imposing detailed balance condition in the bulk. Afterwards, Israel's junction conditions are computed, allowing the attainment of an effective Lagrangian in the visible brane. In particular, we show that the resultant effective Lagrangian in the brane corresponds to a (3 + 1)-dimensional Hořava-like model with an emergent positive cosmological constant but without detailed balance condition. Now, restoration of detailed balance condition, at this time imposed over the brane, plays an interesting role by fitting accordingly the sign of the arbitrary constant β, insuring a positive brane tension and a real energy for the graviton within its dispersion relation. Also, the brane consistency equations are obtained and, as a result, the model admits positive brane tensions in the compactification scheme if, and only if, β is negative and the detailed balance condition is imposed. © 2013 Springer-Verlag Berlin Heidelberg and Società Italiana di Fisica.
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The evolution of arboreality in snakes is accompanied by modifications that are remarkably similar across species. Gravity is one of the most important selective agents, and arboreal snakes present adaptations to circumvent the gradient of pressure, including modifications on heart position (HP) and body slenderness (BS). However, the degree to which different life-history traits influence the cardiovascular system of snakes remains unclear. Here, we used an ecological and a phylogenetic approach to explore the relationship between habitat, HP, BS, and heart size (HS) in five species of the neotropical whipsnakes genus Chironius that occupy terrestrial, semiarboreal, and arboreal habits. Our ecological comparison indicated that the arboreal species have the most posterior-positioned heart, the most slender body, and the smallest HS, whereas the terrestrial representative of the group exhibited the most anterior heart, the less flattened body, and the largest HS. After removing the phylogenetic effect, we found no difference in HP and BS between terrestrial and arboreal species. Habitat only differed when contrasting with HS. Body slenderness and HS were correlated with HP. Our results suggest that different restrictions, such as anatomical constraints, behavior, and phylogenetic inertia, may be important for the studied species. © 2013 The Royal Swedish Academy of Sciences.
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Aims.We investigate the dynamics of pebbles immersed in a gas disk interacting with a planet on an eccentric orbit. The model has a prescribed gap in the disk around the location of the planetary orbit, as is expected for a giant planet with a mass in the range of 0.1-1 Jupiter masses. The pebbles with sizes in the range of 1 cm to 3 m are placed in a ring outside of the giant planet orbit at distances between 10 and 30 planetary Hill radii. The process of the accumulation of pebbles closer to the gap edge, its possible implication for the planetary accretion, and the importance of the mass and the eccentricity of the planet in this process are the motivations behind the present contribution. Methods. We used the Bulirsch-Stoer numerical algorithm, which is computationally consistent for close approaches, to integrate the Newtonian equations of the planar (2D), elliptical restricted three-body problem. The angular velocity of the gas disk was determined by the appropriate balance between the gravity, centrifugal, and pressure forces, such that it is sub-Keplerian in regions with a negative radial pressure gradient and super-Keplerian where the radial pressure gradient is positive. Results. The results show that there are no trappings in the 1:1 resonance around the L 4 and L5 Lagrangian points for very low planetary eccentricities (e2 < 0.07). The trappings in exterior resonances, in the majority of cases, are because the angular velocity of the disk is super-Keplerian in the gap disk outside of the planetary orbit and because the inward drift is stopped. Furthermore, the semi-major axis location of such trappings depends on the gas pressure profile of the gap (depth) and is a = 1.2 for a planet of 1 MJ. A planet on an eccentric orbit interacts with the pebble layer formed by these resonances. Collisions occur and become important for planetary eccentricity near the present value of Jupiter (e 2 = 0.05). The maximum rate of the collisions onto a planet of 0.1 MJ occurs when the pebble size is 37.5 cm ≤ s < 75 cm; for a planet with the mass of Jupiter, it is15 cm ≤ s < 30 cm. The accretion stops when the pebble size is less than 2 cm and the gas drag dominates the motion. © 2013 ESO.
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By means of a triple master action we deduce here a linearized version of the new massive gravity (NMG) in arbitrary dimensions. The theory contains a 4th-order and a 2nd-order term in derivatives. The 4th-order term is invariant under a generalized Weyl symmetry. The action is formulated in terms of a traceless ημνΩμνρ=0 mixed symmetry tensor Ωμνρ=-Ωμρν and corresponds to the massive Fierz-Pauli action with the replacement e μν=∂ρΩμνρ. The linearized 3D and 4D NMG theories are recovered via the invertible maps Ωμνρ=Ïμνρβhβμ and Ωμνρ=ÏμνργδT [γδ]μ respectively. The properties h μν=hνμ and T[[γδ]μ]= 0 follow from the traceless restriction. The equations of motion of the linearized NMG theory can be written as zero curvature conditions ∂νTρμ-∂ρT νμ=0 in arbitrary dimensions. © 2013 American Physical Society.
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The correlation between vegetation patterns (species distribution and richness) and altitudinal variation has been widely reported for tropical forests, thereby providing theoretical basis for biodiversity conservation. However, this relationship may have been oversimplified, as many other factors may influence vegetation patterns, such as disturbances, topography and geographic distance. Considering these other factors, our primary question was: is there a vegetation pattern associated with substantial altitudinal variation (10-1,093 m a.s.l.) in the Atlantic Rainforest-a top hotspot for biodiversity conservation-and, if so, what are the main factors driving this pattern? We addressed this question by sampling 11 1-ha plots, applying multivariate methods, correlations and variance partitioning. The Restinga (forest on sandbanks along the coastal plains of Brazil) and a lowland area that was selectively logged 40 years ago were floristically isolated from the other plots. The maximum species richness (>200 spp. per hectare) occurred at approximately 350 m a.s.l. (submontane forest). Gaps, multiple stemmed trees, average elevation and the standard deviation of the slope significantly affected the vegetation pattern. Spatial proximity also influenced the vegetation pattern as a structuring environmental variable or via dispersal constraints. Our results clarify, for the first time, the key variables that drive species distribution and richness across a large altitudinal range within the Atlantic Rainforest. © 2013 Springer Science+Business Media Dordrecht.
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The number of visceral leishmaniasis (VL) cases has increased over the past 10 years in Brazil, especially in the North and Northeast regions of the country. The aim of this study was to evaluate the urbanisation of VL vectors in Barcarena, Pará, an area in northern Brazil where VL is endemic. Sandflies were captured using Centers for Disease Control (CDC) light traps along an urban-rural gradient. The CDC traps were installed inside hen houses at a height of 150 cm. A total of 5,089 sandflies were collected and 11 species were identified. The predominant species was Lutzomyia longipalpis (rate of 95.15%), which suggests its participation in the transmission of VL. A total of 1,451 Lu. longipalpis females were dissected and no Leishmania infections were detected. Most of the sandflies were captured at the border of a forest (88.25%) and no flies were captured in the urban area, which suggests that transmission is still restricted to rural sites. However, the fact that a specimen was collected in an intermediate area indicates that urbanisation is a real possibility and that vector monitoring is important.
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Apresentamos dois métodos de interpretação de dados de campos potenciais, aplicados à prospecção de hidrocarbonetos. O primeiro emprega dados aeromagnéticos para estimar o limite, no plano horizontal, entre a crosta continental e a crosta oceânica. Este método baseia-se na existência de feições geológicas magnéticas exclusivas da crosta continental, de modo que as estimativas das extremidades destas feições são usadas como estimativas dos limites da crosta continental. Para tanto, o sinal da anomalia aeromagnética na região da plataforma, do talude e da elevação continental é amplificado através do operador de continuação analítica para baixo usando duas implementações: o princípio da camada equivalente e a condição de fronteira de Dirichlet. A maior carga computacional no cálculo do campo continuado para baixo reside na resolução de um sistema de equações lineares de grande porte. Este esforço computacional é minimizado através do processamento por janelas e do emprego do método do gradiente conjugado na resolução do sistema de equações. Como a operação de continuação para baixo é instável, estabilizamos a solução através do funcional estabilizador de primeira ordem de Tikhonov. Testes em dados aeromagnéticos sintéticos contaminados com ruído pseudo-aleatório Gaussiano mostraram a eficiência de ambas as implementações para realçar os finais das feições magnéticas exclusivas da crosta continental, permitindo o delineamento do limite desta com a crosta oceânica. Aplicamos a metodologia em suas duas implementações a dados aeromagnéticos reais de duas regiões da costa brasileira: Foz do Amazonas e Bacia do Jequitinhonha. O segundo método delineia, simultaneamente, a topografia do embasamento de uma bacia sedimentar e a geometria de estruturas salinas contidas no pacote sedimentar. Os modelos interpretativos consistem de um conjunto de prismas bidimensionais verticais justapostos, para o pacote sedimentar e de prismas bidimensionais com seções verticais poligonais para as estruturas salinas. Estabilizamos a solução, incorporando características geométricas do relevo do embasamento e das estruturas salinas compatíveis com o ambiente geológico através dos estabilizadores da suavidade global, suavidade ponderada e da concentração de massa ao longo de direções preferenciais, além de vínculos de desigualdade nos parâmetros. Aplicamos o método a dados gravimétricos sintéticos produzidos por fontes 2D simulando bacias sedimentares intracratônicas e marginais apresentando densidade do pacote sedimentar variando com a profundidade segundo uma lei hiperbólica e abrigando domos e almofadas salinas. Os resultados mostraram que o método apresenta potencial para delinear, simultaneamente, as geometrias tanto de almofadas e domos salinos, como de relevos descontínuos do embasamento. Aplicamos o método, também, a dados reais ao longo de dois perfis gravimétricos sobre as Bacias de Campos e do Jequitinhonha e obtivemos interpretações compatíveis com a geologia da área.
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O presente trabalho consiste na interpretação de informações gravimétricas e aeromagnetométricas (Projeto Geofísico Brasil-Canadá - PGBC) da região setentrional da Faixa de Dobramentos Araguaia, envolvendo uma área de aproximadamente 129.000km2, compreendida entre os meridianos 47°50’W e 50°30’W e paralelos 4°50'S e 9°00'S. Abrange porções sudeste do Estado do Pará, noroeste de Goiás e oeste do Maranhão. Os trabalhos de campo constaram de levantamentos gravimétrico e altimétrico, ao longo de rodovias que constituem a rede viária regional, e os resultados obtidos, após correções e reduções, foram então organizados de forma a constituírem um mapa de anomalias Bouguer, apresentado em escala 1:500.000. O padrão gravimétrico da faixa de dobramentos Araguaia se caracteriza por mostrar feições predominantemente longitudinais, com curvas isoanômalas de direções submeridianas, concordante com o comportamento litológico-estrutural conhecido para a área. Na porção centro-meridional desse mapa aparece uma zona de anomalia negativa, alongada e intensa (menos de -100mgal), a qual sofre duas importantes inflexões para NW, sendo uma correlacionável ao Lineamento Carajás, e a outra na altura do paralelo 5°30'S. Apresenta zonas de altos gravimétricos, notadamente na porção noroeste (domínio cratônico), relacionada à influência das metavulcânicas do Grupo Grão Pará, e na porção nordeste, devida a massas densas introduzidas na crosta. Destaca-se também o relativo alto gravimétrico acompanhando o flanco oriental do eixo de ocorrência das braquidobras, podendo ser devido a massas excedentes colocadas sob essa região, através de esforços tectônicos, produzindo elevações do nível de base da crosta e consequentemente do embasamento. De forma genérica o flanco oriental da faixa mostra um gradiente mais intenso que o ocidental, devido principalmente à configuração geométrica das estruturas nesse setor. Da mesma forma merece destaque o gradiente regional ascendente de sul para norte. A análise das cartas de intensidade magnética do PGBC fornecem condições à individualização de diversos domínios magnéticos, perfeitamente correlacionáveis litológico e estruturalmente com as unidades geotectônicas que compõem o arcabouço regional, assim como suas subunidades. A execução de modelamento simples, quer para as informações gravimétricas como magnetométricas, objetivaram fornecer subsídios semi-quantitativos à interpretação, de forma a auxiliar no estabelecimento do padrão geométrico do embasamento da faixa de dobramentos Araguaia, assim como das estruturas a ela impostas. Assim, por meio do processamento das informações gravimétricas, verificou-se um padrão geométrico na forma de fatias imbricadas, estabelecidas sobre o substrato. A grande anomalia negativa da porção centro-meridional da faixa pode estar relacionada a uma deficiência de massa profunda (depressão na base da crosta) ou ainda a uma associação entre contraste de densidade e espessamento do pacote de supracrustais, nessa porção. O baixo gravimétrico da porção sudeste da área, entre Guarai e Tupirama, é devido a uma depressão do embasamento, da mesma forma como a anomalia negativa associada ao Lineamento Carajás está relacionada a uma estrutura sinformal conhecida.
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We prove the approximate controllability of the semilinear heat equation in RN, when the nonlinear term is globally Lipschitz and depends both on the state u and its spatial gradient Ñu. The approximate controllability is viewed as the limit of a sequence of optimal control problems. In order to avoid the difficulties related to the lack of compactness of the Sobolev embeddings, we work with the similarity variables and use weighted Sobolev spaces.
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Palmeiras apresentam padrões claros de segregação de nicho ao longo de gradientes topográficos, com algumas espécies associadas a florestas de terra firme e outras a áreas alagáveis. O objetivo desse estudo foi descrever quantitativamente as variações em pequena escala dentro de uma comunidade de palmeiras, investigando as mudanças na abundância de espécies ao longo de gradientes ambientais associados com um igarapé perene na Amazônia Oriental. O estudo de comunidades de palmeiras foi baseado em 60 parcelas florestais em que todos os adultos de palmeiras foram contados. Encontramos um total de 566 palmeiras em uma comunidade contendo 11 espécies. Além disso, encontramos uma separação significativa na comunidade de palmeiras entre florestas sazonalmente inundadas e florestas de terra firme e um gradiente das densidades das três espécies mais abundantes, ao longo dos primeiros 100 m de distância da área alagada. A abundância das seis espécies mais comuns variou em relação ao gradiente de umidade das áreas alagáveis para a terra firme, com a distribuição das palmeiras da mais tolerante a alagamentos a menos tolerante a alagamentos da seguinte forma: Euterpe oleracea, Attalea phalerata, Socratea exorrhiza (espécies associadas a áreas alagadas), Astrocaryum gynacanthum, Astrocaryum aculeatum, Attalea maripa (espécies com afinidade por terra firme).