400 research outputs found
Trion dynamics in coupled double quantum wells. Electron density effects
We have studied the coherent dynamics of injected electrons when they are
either free or bounded both in excitons and in trions (charged excitons). We
have considered a remotely doped asymmetric double quantum well where an excess
of free electrons and the direct created excitons generate trions. We have used
the matrix density formalism to analyze the electron dynamics for different
concentration of the three species. Calculations show a significant
modification of the free electron inter-sublevel oscillations cWe have studied
the coherent dynamics of injected electrons when they are aused by electrons
bound in excitons and trions. Based on the present calculations we propose a
method to detect trions through the emitted electromagnetic radiation or the
current density.Comment: 14 pages, 13 figure
An All Sky Transmission Monitor: ASTMON
We present here the All Sky Transmission MONitor (ASTMON), designed to
perform a continuous monitoring of the surface brightness of the complete
night-sky in several bands. The data acquired are used to derive, in addition,
a subsequent map of the multiband atmospheric extinction at any location in the
sky, and a map of the cloud coverage. The instrument has been manufactured to
afford extreme weather conditions, and remain operative. Designed to be fully
robotic, it is ideal to be installed outdoors, as a permanent monitoring
station. The preliminary results based on two of the currently operative units
(at Do\~nana National Park - Huelva- and at the Calar Alto Observatory -
Almer\'ia -, in Spain), are presented here. The parameters derived using ASTMON
are in good agreement with previously reported ones, what illustrates the
validity of the design and the accuracy of the manufacturing. The information
provided by this instrument will be presented in forthcoming articles, once we
have accumulated a statistically amount of data.Comment: 12 Figures, Accepted for publishing in PAS
Tres notas sobre el lenguaje cinematográfico de Pasolini en el Decamerón
En estas breves notas se analizarán los elementos propios del lenguaje cinematográfico como son el montaje, el sonido, la estructura narrativa y el uso que de ellos hace Pasolini para lograr una visión popular de la obra de Boccaccio
Sonic hedgehog specifies flight feather positional information in avian wings
Classical tissue recombination experiments performed in the chick embryo provide evidence that signals operating during early limb development specify the position and identity of feathers. Here, we show that Sonic hedgehog (Shh) signalling in the embryonic chick wing bud specifies positional information required for the formation of adult flight feathers in a defined spatial and temporal sequence that reflects their different identities. We also reveal that Shh signalling is interpreted into specific patterns of Sim1 and Zic transcription factor expression, providing evidence of a putative gene regulatory network operating in flight feather patterning. Our data suggest that flight feather specification involved the co-option of the pre-existing digit patterning mechanism and therefore uncovers an embryonic process that played a fundamental step in the evolution of avian flight
A new flocking model through body attitude coordination
We present a new model for multi-agent dynamics where each agent is described by its position and body attitude: agents travel at a constant speed in a given direction and their body can rotate around it adopting different configurations. In this manner, the body attitude is described by three orthonormal axes giving an element in SO(3) (rotation matrix). Agents try to coordinate their body attitudes with the ones of their neighbours. In the present paper, we give the Individual Based Model (particle model) for this dynamics and derive its corresponding kinetic and macroscopic equations. The work presented here is inspired by the Vicsek model and its study in [24]. This is a new model where collective motion is reached through body attitude coordination
Análisis integral de la disolución de los metales preciosos con sistemas de lixiviación novedosos a base de aminas
En este trabajo de investigación se estudiaron, desde un enfoque electroquÃmico, los sistemas de lixiviación novedosos a base de aminas; la monoetanolamina (MEA) y la etilamina (EA), para mejorar el entendimiento del mecanismo de reacción de la disolución de los metales preciosos, i.e., el oro y la plata. Se presenta el efecto de la concentración de la MEA y la EA, en la velocidad de oxidación de los metales preciosos. El estudio es complementado por medio de técnicas electroquÃmicas tales como: Técnica del potencial de circuito abierto (OCP), voltametrÃa lineal (VL) y cronoamperometrÃas. Los resultados demuestran que estas aminas tienen un gran potencial al disolver el Au y la Ag, debido a que se alcanzan densidades de corriente promedio de 0.008 y 0.013 A/cm2 empleando la MEA y 0.023 y 0.029 A/cm2 utilizando la EA, respectivamente. Además, los resultados dictaminan que tanto la MEA como la EA podrÃan disminuir el..
The night-sky at the Calar Alto Observatory II: The sky at the near infrared
We present here the characterization of the night sky-brightness at the
near-infrared, the telescope seeing, and the fraction of useful time at the
Calar Alto observatory. For this study we have collected a large dataset
comprising 7311 near-infrared images taken regularly along the last four years
for the ALHAMBRA survey (J, H and Ks-bands), together with a more reduced
dataset of additional near-infrared images taken for the current study. In
addition we collected the information derived by the meteorological station at
the observatory during the last 10 years, together with the results from the
cloud sensor for the last ~2 years. We analyze the dependency of the
near-infrared night sky-brightness with the airmass and the seasons, studying
its origins and proposing a zenithal correction. A strong correlation is found
between the night sky-brightness in the Ks-band and the air temperature, with a
gradient of ~ -0.08 mag per 1 C degree. The typical (darkest) night
sky-brightness in the J, H and Ks-band are 15.95 mag (16.95 mag), 13.99 mag
(14.98 mag) and 12.39 mag (13.55 mag), respectively. These values show that
Calar Alto is as dark in the near-infrared as most of the other astronomical
astronomical sites in the world that we could compare with. Only Mauna Kea is
clearly darker in the Ks-band. The typical telescope seeing at the 3.5m is
~1.0" when converted to the V-band, being only slightly larger than the
atmospheric seeing measured at the same time by the seeing monitor, ~0.9".
Finally we estimate the fraction of useful time based on the relative humidity,
gust wind speed and presence of clouds. This fraction, ~72%, is very similar to
the one derived in Paper I, based on the fraction of time when the extinction
monitor is working.Comment: 15 pages, 6 figures, accepted to be published in PAS
Continuum dynamics of the intention field under weakly cohesive social interaction
We investigate the long-time dynamics of an opinion formation model inspired by a work by Borghesi, Bouchaud and Jensen. First, we derive a Fokker–Planck-type equation under the assumption that interactions between individuals produce little consensus of opinion (grazing collision approximation). Second, we study conditions under which the Fokker–Planck equation has non-trivial equilibria and derive the macroscopic limit (corresponding to the long-time dynamics and spatially localized interactions) for the evolution of the mean opinion. Finally, we compare two different types of interaction rates: the original one given in the work of Borghesi, Bouchaud and Jensen (symmetric binary interactions) and one inspired from works by Motsch and Tadmor (non-symmetric binary interactions). We show that the first case leads to a conservative model for the density of the mean opinion whereas the second case leads to a non-conservative equation. We also show that the speed at which consensus is reached asymptotically for these two rates has fairly different density dependence
From Boltzmann to incompressible Navier-Stokes in Sobolev spaces with polynomial weight
We study the Boltzmann equation on the d-dimensional torus in a perturbative setting around a global equilibrium under the Navier-Stokes lineari- sation. We use a recent functional analysis breakthrough to prove that the linear part of the equation generates a C0-semigroup with exponential decay in Lebesgue and Sobolev spaces with polynomial weight, independently on the Knudsen number. Finally we show a Cauchy theory and an exponential decay for the perturbed Boltzmann equation, uniformly in the Knudsen number, in Sobolev spaces with polynomial weight. The polynomial weight is almost optimal and furthermore, this result only requires derivatives in the space variable and allows to connect to solutions to the incompressible Navier-Stokes equations in these spaces
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