Review Essay

Midway was one of the most decisive naval battles of all time. It was a battle that should have been won by the Japanese but wasn’t. Future American writers would dub it an incredible or miraculous victory, based on the superiority of the Japanese and the widely held perception before the battle that the Imperial Japa- nese Navy was invincible

Attitudes of College Youth at Oklahoma State University Concerning the Parenthood Role

Family Relations and Child Developmen

"Dark energy" in the Local Void

The unexpected discovery of the accelerated cosmic expansion in 1998 has filled the Universe with the embarrassing presence of an unidentified "dark energy", or cosmological constant, devoid of any physical meaning. While this standard cosmology seems to work well at the global level, improved knowledge of the kinematics and other properties of our extragalactic neighborhood indicates the need for a better theory. We investigate whether the recently suggested repulsive-gravity scenario can account for some of the features that are unexplained by the standard model. Through simple dynamical considerations, we find that the Local Void could host an amount of antimatter ($\sim5\times10^{15}\,M_\odot$) roughly equivalent to the mass of a typical supercluster, thus restoring the matter-antimatter symmetry. The antigravity field produced by this "dark repulsor" can explain the anomalous motion of the Local Sheet away from the Local Void, as well as several other properties of nearby galaxies that seem to require void evacuation and structure formation much faster than expected from the standard model. At the global cosmological level, gravitational repulsion from antimatter hidden in voids can provide more than enough potential energy to drive both the cosmic expansion and its acceleration, with no need for an initial "explosion" and dark energy. Moreover, the discrete distribution of these dark repulsors, in contrast to the uniformly permeating dark energy, can also explain dark flows and other recently observed excessive inhomogeneities and anisotropies of the Universe.Comment: 6 pages, accepted as a Letter to the Editor by Astrophysics and Space Scienc

The origin of the mu_e - M_B and Kormendy relations in dwarf elliptical galaxies

The present work is aimed at studying the distribution of galaxies of different types and luminosities along different structural scaling relations to see whether massive and dwarf ellipticals have been shaped by the same formation process. This exercise is here done by comparing the distribution of Virgo cluster massive and dwarf ellipticals and star forming galaxies along the B band effective surface brightness and effective radius vs. absolute magnitude relations and the Kormendy relation to the predictions of models tracing the effects of ram-pressure stripping on disc galaxies entering the cluster environment and galaxy harassment. Dwarf ellipticals might have been formed from low luminosity, late-type spirals that recently entered into the cluster and lost their gas because of a ram-pressure stripping event, stopping their activity of star formation. The perturbations induced by the abrupt decrease of the star formation activity are sufficient to modify the structural properties of disc galaxies into those of dwarf ellipticals. Galaxy harassment induce a truncation of the disc and generally an increase of the effective surface brightness of the perturbed galaxies. The lack of dynamical simulations of perturbed galaxies spanning a wide range in luminosity prevents us to drive any firm conclusion on a possible harassment-induced origin of the low surface brightness dwarf elliptical galaxy population inhabiting the Virgo cluster. Although the observed scaling relations are consistent with the idea that the distribution of elliptical galaxies along the mentioned scaling relation is just due to a gradual variation with luminosity of the Sersic index n, the comparison with models indicates that dwarf ellipticals might have been formed by a totally different process than giant ellipticalsComment: Accepted for publication on A&

The hierarchical build-up of the Tully-Fisher relation

We use the semi-analytic model GalICS to predict the Tully-Fisher relation in the B, I and for the first time, in the K band, and its evolution with redshift, up to z~1. We refined the determination of the disk galaxies rotation velocity, with a dynamical recipe for the rotation curve, rather than a simple conversion from the total mass to maximum velocity. The new recipe takes into account the disk shape factor, and the angular momentum transfer occurring during secular evolution leading to the formation of bulges. This produces model rotation velocities that are lower by ~20-25% for the majority of the spirals. We implemented stellar population models with a complete treatment of the TP-AGB, which leads to a revision of the mass-to-light ratio in the near-IR. I/K band luminosities increase by ~0.3/0.5 mags at redshift z=0 and by ~0.5/1 mags at z=3. With these two new recipes in place, the comparison between the predicted Tully-Fisher relation with a series of datasets in the optical and near-IR, at redshifts between 0 and 1, is used as a diagnostics of the assembly and evolution of spiral galaxies in the model. At 0.4<z<1.2 the match between the new model and data is remarkably good, especially for later-type spirals (Sb/Sc). At z=0 the new model shows a net improvement in comparison with its original version of 2003, and in accord with recent observations in the K band, the model Tully-Fisher also shows a morphological differentiation. However, in all bands the z=0 model Tully-Fisher is too bright. We argue that this behaviour is caused by inadequate star formation histories in the model galaxies at low redshifts. The star-formation rate declines too slowly, due to continuous gas infall that is not efficiently suppressed. An analysis of the model disk scale lengths, at odds with observations, hints to some missing physics in the modeling of disk formation inside dark matter halos.Comment: Accepted for publication on MNRAS. 2 new plots, 1 new section, and extended discussion. 21 pages, 11 figures in tota

Dark Matter Substructure in Galactic Halos

We use numerical simulations to examine the substructure within galactic and cluster mass halos that form within a hierarchical universe. Clusters are easily reproduced with a steep mass spectrum of thousands of substructure clumps that closely matches observations. However, the survival of dark matter substructure also occurs on galactic scales, leading to the remarkable result that galaxy halos appear as scaled versions of galaxy clusters. The model predicts that the virialised extent of the Milky Way's halo should contain about 500 satellites with circular velocities larger than Draco and Ursa-Minor i.e. bound masses > 10^8Mo and tidally limited sizes > kpc. The substructure clumps are on orbits that take a large fraction of them through the stellar disk leading to significant resonant and impulsive heating. Their abundance and singular density profiles has important implications for the existence of old thin disks, cold stellar streams, gravitational lensing and indirect/direct detection experiments.Comment: Astrophysical Journal Letters. 4 pages, latex. Simulation images and movies at http://star-www.dur.ac.uk:80/~moore

Reduced density matrix hybrid approach: An efficient and accurate method for adiabatic and non-adiabatic quantum dynamics

We present a new approach to calculate real-time quantum dynamics in complex systems. The formalism is based on the partitioning of a system's environment into "core" and "reservoir" modes, with the former to be treated quantum mechanically and the latter classically. The presented method only requires the calculation of the system's reduced density matrix averaged over the quantum core degrees of freedom which is then coupled to a classically evolved reservoir to treat the remaining modes. We demonstrate our approach by applying it to the spin-boson problem using the noninteracting blip approximation to treat the system and core, and Ehrenfest dynamics to treat the reservoir. The resulting hybrid methodology is accurate for both fast and slow baths, since it naturally reduces to its composite methods in their respective regimes of validity. In addition, our combined method is shown to yield good results in intermediate regimes where neither approximation alone is accurate and to perform equally well for both strong and weak system-bath coupling. Our approach therefore provides an accurate and efficient methodology for calculating quantum dynamics in complex systems.Comment: 10 pages, 7 figure

Compétition par interférence, température et dynamique des populations structurées (étude expérimentale et théorique chez le collembole folsomia candida)

La compétition par interférence et ses effets sur la dynamique des populations suscitent un intérêt croissant. La température a aussi un fort effet sur la physiologie et les comportements individuels ainsi que sur les dynamiques des populations. Face au changement climatique, comprendre les interactions compétition-température-dynamique des populations est un enjeu majeur en biologie des populations. Les interactions entre individus sont liées à leur taille corporelle. La structure en taille de populations de deux clones du collembole Folsomia candida a été suivie pendant 2 à 4 ans à 4 températures. L'analyse des séries temporelles de leur structure à 21C a révélé une dépendance de la dynamique aux conditions individuelles d¿accès à la ressource, liées aux plus grands individus. Nous avons modifié la structure de populations à 21C et observé leur retour à l'équilibre, puis observé le comportement d'accès à la ressource. Cela a démontré le rôle des grands adultes dans la régulation des populations, en interférant avec les plus petits pour l'accès aux ressources. Grâce à un modèle de populations structurées intégrant l'interférence, nous avons montré que son intensité croissante cause : l'amortissement des cycles de générations, la survie de grands individus, des cycles induits par l'interférence. Nous avons enfin comparé les normes de réactions à la température sur des individus isolés et dans des populations afin de comprendre les interactions compétition-température dans la régulation des populations. Plusieurs niveaux de complexité permettent de comprendre l'effet des changements environnementaux sur les populations.Interference competition and its effects on population dynamics are of growing interest. Temperature also plays an important role on the physiology and individual behavior as well as on population dynamics populations. In the context of climate change, understanding the effect of interactions between individuals on population dynamics and their interactions with temperature is an important issue for population biology. Interactions between individuals are related to their body size. The size structure of several populations of two clones of Collembola Folsomia candida was monitored for 2-4 years at four temperatures from 11 C to 26 C. The time series analysis of their structure at 21 C revealed a dependence of the dynamics on individual access to the resource related to the presence of large individuals. We then changed some population structures at 21 C and observed their return to equilibrium. We observed real-time access to the resource behavior. These studies have shown the role of large adults in population control by interfering with smaller individuals for access to resources. Through a structured model incorporating interference competition, we have shown that its intensity may have different effects on the dynamics of structured populations: damping single generation cycles, allowing the survival of large individuals, and causing interference induced cycles. Finally, we compared the reaction norms to temperature on isolated individuals and populations in order to understand the competition-temperature interactions in regulating populations. Several levels of complexity allow us to understand the effect of environmental change on populationsPARIS-JUSSIEU-Bib.électronique (751059901) / SudocSudocFranceF

The minor house dust mite allergen Der p 13 is a fatty acid binding protein and an activator of a TLR2-mediated innate immune response

Background: The house dust mite (HDM) allergen Der p 13 could be a lipid-binding protein able to activate key innate signaling pathways in the initiation of the allergic response. We investigated the IgE reactivity of recombinant Der p 13 (rDer p 13), its lipid binding activities and its capacity to stimulate airway epithelium cells. Methods: Purified rDer p 13 was characterized by mass spectrometry, circular dichroism, fluorescence-based lipid binding assays and in-silico structural prediction. IgE binding activity and allergenic potential of Der p 13 were examined by ELISA, basophil degranulation assays and in-vitro airway epithelial cell activation assays. Results: Protein modeling and biophysical analysis indicated that Der p 13 adopts a β barrel structure with a predominately apolar pocket representing a potential binding site for hydrophobic ligands. Fluorescent lipid binding assays confirmed that the protein is highly selective for ligands and that it binds a fatty acid with a dissociation constant typical of lipid transporter proteins. The low IgE binding frequency (7%, n= 224) in Thai HDM-allergic patients as well as the limited propensity to activate basophil degranulation classifies Der p 13 as a minor HDM allergen. Nevertheless, the protein with its presumptively associated lipid(s) triggered the production of IL-8 and GM-CSF in respiratory epithelial cells through a TLR2-, MyD88-, NF-kB- and MAPK-dependent signaling pathway. Conclusions: Although a minor allergen, Der p 13 may, through its lipid binding capacity, play a role in the initiation of the HDM allergic response through TLR2 activation