6,137 research outputs found
Ocorrência e controle da lesma Omalonyx sp. (Gastropoda: Succineidae), praga de capim-elefante (Pennisetum purpureum) em Manaus, Amazonas.
Neste trabalho descreveu-se a ocorrência atípica de Omalonyx sp. como praga em capim-elefante (Pennisetum purpureum), em habitat de terra firme, em Manaus-AM e sugere-se uma alternativa para o seu controle
Effects of Velocity Correlation on Early Stage of Free Cooling Process of Inelastic Hard Sphere System
The free cooling process in the inelastic hard sphere system is studied by
analysing the data from large scale molecular dynamics simulations on a three
dimensional system. The initial energy decay, the velocity distribution
function, and the velocity correlation functions are calculated to be compared
with theoretical predictions. The energy decay rate in the homogeneous cooling
state is slightly but distinctively smaller than that expected from the
independent collision assumption. The form of the one particle velocity
distribution is found not to be stationary. These contradict to the predictions
of the kinetic theory based on the Enskog-Boltzmann equation and suggest that
the velocity correlation is already important in the early stage of homogeneous
cooling state. The energy decay rate is analysed in terms of the velocity
correlation.Comment: 9 pages (figures included). To be published in J. Phys. Soc. Jpn.
Vol. 73 No. 1 (2004) Added two references and removed one. Changed the name
of T_{L}. Added unit constants in Sec. 5 and
Morphological transition between diffusion-limited and ballistic aggregation growth patterns
In this work, the transition between diffusion-limited and ballistic
aggregation models was revisited using a model in which biased random walks
simulate the particle trajectories. The bias is controlled by a parameter
, which assumes the value (1) for ballistic
(diffusion-limited) aggregation model. Patterns growing from a single seed were
considered. In order to simulate large clusters, a new efficient algorithm was
developed. For , the patterns are fractal on the small length
scales, but homogeneous on the large ones. We evaluated the mean density of
particles in the region defined by a circle of radius centered
at the initial seed. As a function of , reaches the asymptotic
value following a power law
with a universal exponent , independent of . The
asymptotic value has the behavior , where . The characteristic crossover length that determines the transition
from DLA- to BA-like scaling regimes is given by ,
where , while the cluster mass at the crossover follows a power
law , where . We deduce the
scaling relations \beta=\n u\gamma and between these
exponents.Comment: 7 pages, 8 figure
Radiocarbon and blue optically stimulated luminescence chronologies of the Oitavos consolidated dune (Western Portugal)
The dune of Oitavos, the underlying paleosol, and Helix sp. gastropod shells found within the paleosol were dated using a combination of radiocarbon and blue optically stimulated luminescence (OSL). The organic component of the paleosol produced a significantly older age (~20,000 cal BP) than the OSL age measurement (~15,000 yr), while 14C age measurements on the inorganic component and the gastropods produced ages of ~35,000 yr and ~34,000 yr, respectively. Rare-earth
element analyses provide evidence that the gastropods incorporate geological carbonate, making them an unreliable indicator of the age of the paleosol. We propose that the 14C age of the small organic component of the paleosol is also likely to be unreliable due to incorporation of residual material. The OSL age measurement of the upper paleosol (~15,000 yr) is consistent with the age for the base of the dune (~14,500 yr). The younger OSL age for the top of the dune (~12,000 yr) suggests that it was built up by at least 2 sand pulses or that there was a remobilization of material at the top during its evolution, prior to consolidation
The Solar Twin Planet Search II. A Jupiter twin around a solar twin
Through our HARPS radial velocity survey for planets around solar twin stars,
we have identified a promising Jupiter twin candidate around the star HIP11915.
We characterize this Keplerian signal and investigate its potential origins in
stellar activity. Our analysis indicates that HIP11915 hosts a Jupiter-mass
planet with a 3800-day orbital period and low eccentricity. Although we cannot
definitively rule out an activity cycle interpretation, we find that a planet
interpretation is more likely based on a joint analysis of RV and activity
index data. The challenges of long-period radial velocity signals addressed in
this paper are critical for the ongoing discovery of Jupiter-like exoplanets.
If planetary in nature, the signal investigated here represents a very close
analog to the solar system in terms of both Sun-like host star and Jupiter-like
planet.Comment: 8 pages, 5 figures; A&A accepted; typos corrected in this versio
Heterogeneous Dynamics, Marginal Stability and Soft Modes in Hard Sphere Glasses
In a recent publication we established an analogy between the free energy of
a hard sphere system and the energy of an elastic network [1]. This result
enables one to study the free energy landscape of hard spheres, in particular
to define normal modes. In this Letter we use these tools to analyze the
activated transitions between meta-bassins, both in the aging regime deep in
the glass phase and near the glass transition. We observe numerically that
structural relaxation occurs mostly along a very small number of
nearly-unstable extended modes. This number decays for denser packing and is
significantly lowered as the system undergoes the glass transition. This
observation supports that structural relaxation and marginal modes share common
properties. In particular theoretical results [2, 3] show that these modes
extend at least on some length scale where
corresponds to the maximum packing fraction, i.e. the jamming
transition. This prediction is consistent with very recent numerical
observations of sheared systems near the jamming threshold [4], where a similar
exponent is found, and with the commonly observed growth of the rearranging
regions with compression near the glass transition.Comment: 6 pages, improved versio
Granular cooling of hard needles
We have developed a kinetic theory of hard needles undergoing binary
collisions with loss of energy due to normal and tangential restitution. In
addition, we have simulated many particle systems of granular hard needles. The
theory, based on the assumption of a homogeneous cooling state, predicts that
granular cooling of the needles proceeds in two stages: An exponential decay of
the initial configuration to a state where translational and rotational
energies take on a time independent ratio (not necessarily unity), followed by
an algebraic decay of the total kinetic energy . The simulations
support the theory very well for low and moderate densities. For higher
densities, we have observed the onset of the formation of clusters and shear
bands.Comment: 7 pages, 8 figures; major changes, extended versio
Irrigação de salvação em culturas de subsistência.
Descrição da tecnologia; Área de captação; Tanque de armazenamento; Área de Plantio; Estudo de caso; Manejo de água de irrigação de salvação
Patterns and Long Range Correlations in Idealized Granular Flows
An initially homogeneous freely evolving fluid of inelastic hard spheres
develops inhomogeneities in the flow field (vortices) and in the density field
(clusters), driven by unstable fluctuations. Their spatial correlations, as
measured in molecular dynamics simulations, exhibit long range correlations;
the mean vortex diameter grows as the square root of time; there occur
transitions to macroscopic shearing states, etc.
The Cahn--Hilliard theory of spinodal decomposition offers a qualitative
understanding and quantitative estimates of the observed phenomena. When
intrinsic length scales are of the order of the system size, effects of
physical boundaries and periodic boundaries (finite size effects in
simulations) are important.Comment: 13 pages with 7 postscript figures, LaTeX (uses psfig). Submitted to
International Journal of Modern Physics
- …