19,674 research outputs found
On The Orbital Evolution of Jupiter Mass Protoplanet Embedded in A Self-Gravity Disk
We performed a series of hydro-dynamic simulations to investigate the orbital
migration of a Jovian planet embedded in a proto-stellar disk. In order to take
into account of the effect of the disk's self gravity, we developed and adopted
an \textbf{Antares} code which is based on a 2-D Godunov scheme to obtain the
exact Reimann solution for isothermal or polytropic gas, with non-reflecting
boundary conditions. Our simulations indicate that in the study of the runaway
(type III) migration, it is important to carry out a fully self consistent
treatment of the gravitational interaction between the disk and the embedded
planet. Through a series of convergence tests, we show that adequate numerical
resolution, especially within the planet's Roche lobe, critically determines
the outcome of the simulations. We consider a variety of initial conditions and
show that isolated, non eccentric protoplanet planets do not undergo type III
migration. We attribute the difference between our and previous simulations to
the contribution of a self consistent representation of the disk's self
gravity. Nevertheless, type III migration cannot be completely suppressed and
its onset requires finite amplitude perturbations such as that induced by
planet-planet interaction. We determine the radial extent of type III migration
as a function of the disk's self gravity.Comment: 19 pages, 13 figure
Características de las secuencias deposicionales de alta frecuencia en el sistema arrecifal del Mioceno superior de Mallorca
Application of sequence stratigraphy concepts in well-exposed prograding carbonate complexes, such as the example of Mallorca, shows marked peculiarities differing from the commonly used as standard model of the Exxon group. These peculiarities are seen in high-frequency sequences bounded by well-definederosion surfaces. The standard model is incomplete in the sense that it shows no sedimentary record of the fall of the sea-level cycle, except for erosion or karstification. In contrast, the Mallorcan example shows more complete and continuous sedimentary record during the entire sea-level cycle: an offlapping package, commonly ignored or misinterpreted, is deposited during the internal of sea-level fall, and considered as a new systems tract. As a result, the most obvious and marked erosion surface separating these high-frequency packages is the sequence boundary. Furthermore, in the standard model the downlap surface is correlative with the maximum flooding surface and a condensed section. In contrast, the Mallorcan model shows that a condensed section and downlap surface are produced during the offlapping systems tract, whereas the maximum flooding surface are indistinct. There are two surfaces easily recognized in the Mallorcan example: an erosion surface and a downlap surface. On this basis there are two major systems packages or tracts: a lower package with aggradation in all the systems formed during sea-level rise and high-stillstand and an upper package with offlapping progradation formed during sea-level fall and low-stillstand. Al1 the above peculiarities of the Mallorcan prograding reef complex show the need for careful application of the dynamic concepts of sequence stratigraphy, rather than the strict reference to the standard scheme. The relationships between carbonate production and each segment of the sea-level cycle explain these departures from the standard 3rd-order sequencemodel developed from siliciclastic deposits on passive margins
Características de las secuencias deposicionales de alta frecuencia en el sistema arrecifal del Mioceno superior de Mallorca
Application of sequence stratigraphy concepts in well-exposed prograding carbonate complexes, such as the example of Mallorca, shows marked peculiarities differing from the commonly used as standard model of the Exxon group. These peculiarities are seen in high-frequency sequences bounded by well-definederosion surfaces. The standard model is incomplete in the sense that it shows no sedimentary record of the fall of the sea-level cycle, except for erosion or karstification. In contrast, the Mallorcan example shows more complete and continuous sedimentary record during the entire sea-level cycle: an offlapping package, commonly ignored or misinterpreted, is deposited during the internal of sea-level fall, and considered as a new systems tract. As a result, the most obvious and marked erosion surface separating these high-frequency packages is the sequence boundary. Furthermore, in the standard model the downlap surface is correlative with the maximum flooding surface and a condensed section. In contrast, the Mallorcan model shows that a condensed section and downlap surface are produced during the offlapping systems tract, whereas the maximum flooding surface are indistinct. There are two surfaces easily recognized in the Mallorcan example: an erosion surface and a downlap surface. On this basis there are two major systems packages or tracts: a lower package with aggradation in all the systems formed during sea-level rise and high-stillstand and an upper package with offlapping progradation formed during sea-level fall and low-stillstand. Al1 the above peculiarities of the Mallorcan prograding reef complex show the need for careful application of the dynamic concepts of sequence stratigraphy, rather than the strict reference to the standard scheme. The relationships between carbonate production and each segment of the sea-level cycle explain these departures from the standard 3rd-order sequencemodel developed from siliciclastic deposits on passive margins
Evolution of Migrating Planets Undergoing Gas Accretion
We analyze the orbital and mass evolution of planets that undergo run-away
gas accretion by means of 2D and 3D hydrodynamic simulations. The disk torque
distribution per unit disk mass as a function of radius provides an important
diagnostic for the nature of the disk-planet interactions. We first consider
torque distributions for nonmigrating planets of fixed mass and show that there
is general agreement with the expectations of resonance theory. We then present
results of simulations for mass-gaining, migrating planets. For planets with an
initial mass of 5 Earth masses, which are embedded in disks with standard
parameters and which undergo run-away gas accretion to one Jupiter mass (Mjup),
the torque distributions per unit disk mass are largely unaffected by migration
and accretion for a given planet mass. The migration rates for these planets
are in agreement with the predictions of the standard theory for planet
migration (Type I and Type II migration). The planet mass growth occurs through
gas capture within the planet's Bondi radius at lower planet masses, the Hill
radius at intermediate planet masses, and through reduced accretion at higher
planet masses due to gap formation. During run-away mass growth, a planet
migrates inwards by only about 20% in radius before achieving a mass of ~1
Mjup. For the above models, we find no evidence of fast migration driven by
coorbital torques, known as Type III migration. We do find evidence of Type III
migration for a fixed mass planet of Saturn's mass that is immersed in a cold
and massive disk. In this case the planet migration is assumed to begin before
gap formation completes. The migration is understood through a model in which
the torque is due to an asymmetry in density between trapped gas on the leading
side of the planet and ambient gas on the trailing side of the planet.Comment: 26 pages, 29 figures. To appear in The Astrophysical Journal vol.684
(September 20, 2008 issue
Stringy Black Holes and the Geometry of Entanglement
Recently striking multiple relations have been found between pure state 2 and
3-qubit entanglement and extremal black holes in string theory. Here we add
further mathematical similarities which can be both useful in string and
quantum information theory. In particular we show that finding the frozen
values of the moduli in the calculation of the macroscopic entropy in the STU
model, is related to finding the canonical form for a pure three-qubit
entangled state defined by the dyonic charges. In this picture the
extremization of the BPS mass with respect to moduli is connected to the
problem of finding the optimal local distillation protocol of a GHZ state from
an arbitrary pure three-qubit state. These results and a geometric
classification of STU black holes BPS and non-BPS can be described in the
elegant language of twistors. Finally an interesting connection between the
black hole entropy and the average real entanglement of formation is
established.Comment: 34 pages, 6 figure
Measures Matter: Scales for Adaptation, Cultural Distance, and Acculturation Orientation Revisited
Building upon existing measures, four new brief acculturation scales are presented, measuring sociocultural adaptation, psychological adaptation, perceived cultural distance, and acculturation orientation. Following good scale reliability in initial samples, the English scales were translated into nine different languages (Chinese, French, German, Italian, Japanese, Portuguese, Spanish, Thai, and Turkish). The translated scales were administered to a large sample of sojourners (N = 1,929), demonstrating good reliability and adequate structural equivalence across languages. In line with existing theory, sociocultural adaptation and psychological adaptation were positively correlated, and showed a negative association with perceived cultural distance. General measures of well-being were correlated with adaptation and distance, with better adaptation relating to higher well-being, and more distance relating to lower well-being. Acculturation orientation toward the home and host culture were measured separately and a weak negative correlation was found between the two, supporting their independence. Arguing against dichotomization, these subscales were analyzed as continuous variables. Regression analysis showed sojourners to be better adapted, if they were oriented more toward the host culture and less toward the home culture. These new scales are proposed as alternatives to existing measures
On the migration of protogiant solid cores
The increase of computational resources has recently allowed high resolution,
three dimensional calculations of planets embedded in gaseous protoplanetary
disks. They provide estimates of the planet migration timescale that can be
compared to analytical predictions. While these predictions can result in
extremely short migration timescales for cores of a few Earth masses, recent
numerical calculations have given an unexpected outcome: the torque acting on
planets with masses between 5 M_Earth and 20 M_Earth is considerably smaller
than the analytic, linear estimate. These findings motivated the present work,
which investigates existence and origin of this discrepancy or ``offset'', as
we shall call it, by means of two and three dimensional numerical calculations.
We show that the offset is indeed physical and arises from the coorbital
corotation torque, since (i) it scales with the disk vortensity gradient, (ii)
its asymptotic value depends on the disk viscosity, (iii) it is associated to
an excess of the horseshoe zone width. We show that the offset corresponds to
the onset of non-linearities of the flow around the planet, which alter the
streamline topology as the planet mass increases: at low mass the flow
non-linearities are confined to the planet's Bondi sphere whereas at larger
mass the streamlines display a classical picture reminiscent of the restricted
three body problem, with a prograde circumplanetary disk inside a ``Roche
lobe''. This behavior is of particular importance for the sub-critical solid
cores (M <~ 15 M_Earth) in thin (H/r <~0.06) protoplanetary disks. Their
migration could be significantly slowed down, or reversed, in disks with
shallow surface density profiles.Comment: Accepted for publication in Ap
Levels of genetic polymorphism: marker loci versus quantitative traits
Species are the units used to measure ecological diversity and alleles are the units of genetic diversity. Genetic variation within and among species has been documented most extensively using allozyme electrophoresis. This reveals wide differences in genetic variability within, and genetic distances among, species, demonstrating that species are not equivalent units of diversity. The extent to which the pattern observed for allozymes can be used to infer patterns of genetic variation in quantitative traits depends on the forces generating and maintaining variability. Allozyme variation is probably not strictly neutral but, nevertheless, heterozygosity is expected to be influenced by population size and genetic distance will be affected by time since divergence. The same is true for quantitative traits influenced by many genes and under weak stabilizing selection. However, the limited data available suggest that allozyme variability is a poor predictor of genetic variation in quantitative traits within populations. It is a better predictor of general phenotypic divergence and of postzygotic isolation between populations or species, but is only weakly correlated with prezygotic isolation. Studies of grasshopper and planthopper mating signal variation and assortative mating illustrate how these characters evolve independently of general genetic and morphological variation. The role of such traits in prezygotic isolation, and hence speciation, means that they will contribute significantly to the diversity of levels of genetic variation within and among species
Social recognition and social attraction in group-living fishes
This work was supported by a grant from the Australian Research Council, Discovery Project DP190100660, focusing on the social behavior of animals.Social aggregation is a widespread and important phenomenon among fishes. Understanding the questions of why and how aggregations form and are subsequently maintained is a central goal for behavioral ecologists. Research in this field has shown that aggregations are typically structured, non-random associations. This indicates that fish are able to differentiate between potential group-mates and that this ability mediates their association preferences, and, ultimately, the composition of their groups. In this review, we examine the characteristics that influence the expression of social attraction among fishes, before going on to describe the recognition mechanisms that underpin social attraction. Finally, we highlight a number of outstanding questions in the field with a view to generating a more complete understanding of social aggregation in fishes.Publisher PDFPeer reviewe
(Super)twistors and (super)strings
The Lagrangian formulation of the D=4 bosonic string and superstring in terms
of the (super)twistors is considered. The (super)twistor form of the equations
of motion is derived and the kappa-symmetry transformation for the
supertwistors is given. It is shown that the covariant kappa-symmetry gauge
fixation results in the action quadratic in the (super)twistor variables.Comment: LaTeX, 17 page
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