Isocrate, la seconde Confédération maritime et l’Aréopagitique

The Areopagiticus [VII], well known for its remarks about the Athenian constitution and internal politics, provides nonetheless an analysis of the naval power. If we date this speech after the Social War, in 354, it looks like a bitter observation connected with a condemnation of the maritime empire. But, if, as I try to prove it, the speech has been composed before, in 357/6, even earlier (Isocrates probably started to think about it as soon as 364-360), its impact and its significance are different. Isocrates would prevent the loss of the naval supremacy of Athens. He never condemns it (such a sentence he could not avoid after writing de Pace in 355). On the contrary, supremacy still remains his major preoccupation and he even praises it. The League of Delos was well working when Areopagos was still powerful. The transformation of the internal Athenian politics, and not the arche, is the reason of the polis’ bane, a polis which can’t keep what generals as Conon or Timothy gave to the Athenians

The Problems of Induction

All of us here are drawn together by our fascination with the lucid dream experience. We believe that it has the potential to enhance personal development and perhaps to increase our scientific understanding of dreams and consciousness. Without intentional induction procedures, lucid dreams tend to occur spontaneously but sporadically. An individual experiencing a lucid dream for the first time, will often become intrigued by it, and attempt to increase the frequency of these experiences by trial and error. These hit and miss methods do not often achieve their goal consistently. If we are to make progress toward scientific and the personal understanding of lucid dreams, we must first develop techniques to induce the lucid dream experience reliably. This is the most important task currently facing lucid dream research

The Problem of Induction: A Panel Discussion

All of us here are drawn together by our fascination with the lucid dream experience. We believe that it has the potential to enhance personal development and perhaps to increase our scientific understanding of dreams and consciousness. Without intentional induction procedures, lucid dreams tend to occur spontaneously but sporadically. An individual experiencing a lucid dream for the first time will often become intrigued by it, and attempt to increase the frequency of these experiences by trial and error. These hit and miss methods do not often achieve their goal consistently. If we are to make progress toward scientific and personal understanding of lucid dreams, we must first develop techniques to induce the lucid dream experience reliably. This is the most important task currently facing lucid dream research

Fast Evaluation of Interlace Polynomials on Graphs of Bounded Treewidth

We consider the multivariate interlace polynomial introduced by Courcelle (2008), which generalizes several interlace polynomials defined by Arratia, Bollobas, and Sorkin (2004) and by Aigner and van der Holst (2004). We present an algorithm to evaluate the multivariate interlace polynomial of a graph with n vertices given a tree decomposition of the graph of width k. The best previously known result (Courcelle 2008) employs a general logical framework and leads to an algorithm with running time f(k)*n, where f(k) is doubly exponential in k. Analyzing the GF(2)-rank of adjacency matrices in the context of tree decompositions, we give a faster and more direct algorithm. Our algorithm uses 2^{3k^2+O(k)}*n arithmetic operations and can be efficiently implemented in parallel.Comment: v4: Minor error in Lemma 5.5 fixed, Section 6.6 added, minor improvements. 44 pages, 14 figure

The Coyote Universe I: Precision Determination of the Nonlinear Matter Power Spectrum

Near-future cosmological observations targeted at investigations of dark energy pose stringent requirements on the accuracy of theoretical predictions for the clustering of matter. Currently, N-body simulations comprise the only viable approach to this problem. In this paper we demonstrate that N-body simulations can indeed be sufficiently controlled to fulfill these requirements for the needs of ongoing and near-future weak lensing surveys. By performing a large suite of cosmological simulation comparison and convergence tests we show that results for the nonlinear matter power spectrum can be obtained at 1% accuracy out to k~1 h/Mpc. The key components of these high accuracy simulations are: precise initial conditions, very large simulation volumes, sufficient mass resolution, and accurate time stepping. This paper is the first in a series of three, with the final aim to provide a high-accuracy prediction scheme for the nonlinear matter power spectrum.Comment: 18 pages, 22 figures, minor changes to address referee repor

Mass Function Predictions Beyond LCDM

The mass distribution of halos, as specified by the halo mass function, is a key input for several cosmological probes. The sizes of $N$-body simulations are now such that, for the most part, results need no longer be statistics-limited, but are still subject to various systematic uncertainties. We investigate and discuss some of the reasons for these differences. Quantifying error sources and compensating for them as appropriate, we carry out a high-statistics study of dark matter halos from 67 $N$-body simulations to investigate the mass function and its evolution for a reference $\Lambda$CDM cosmology and for a set of $w$CDM cosmologies. For the reference $\Lambda$CDM cosmology (close to WMAP5), we quantify the breaking of universality in the form of the mass function as a function of redshift, finding an evolution of as much as 10% away from the universal form between redshifts $z=0$ and $z=2$. For cosmologies very close to this reference we provide a fitting formula to our results for the (evolving) $\Lambda$CDM mass function over a mass range of $6\cdot 10^{11}-3\cdot 10^{15}$ M$_{\odot}$ to an estimated accuracy of about 2%. The set of $w$CDM cosmologies is taken from the Coyote Universe simulation suite. The mass functions from this suite (which includes a $\Lambda$CDM cosmology and others with $w\simeq-1$) are described by the fitting formula for the reference $\Lambda$CDM case at an accuracy level of 10%, but with clear systematic deviations. We argue that, as a consequence, fitting formulae based on a universal form for the mass function may have limited utility in high precision cosmological applications.Comment: 19 pages; 18 figures; accepted for publication in the Ap

Improvement of leucocytic Na+K+ pump activity in uremic patients on low protein diet

Improvement of leucocytic Na+ K+ pump activity in uremic patients on low protein diet. Leucocytic Na+K+ pump activity was assessed in 20 patients with advanced renal failure. Na+K+-ATPase activity was reduced when compared with the values obtained from normal subjects (101.8 ± 48.6 versus 165.13 ± 8.9 µM of Pi hr-1 · g-1 P < 0.001) and the mean 86Rb uptake by U 937 cells was depressed by 38% after the addition of patients' sera. Subsequently, patients were put on a diet providing 0.3g protein/kg body weight daily and supplemented with ketoacids. After three months of dietary treatment Na+K+-ATPase activity increased to 142 ± 48.3 (P < 0.01) and reached normal values at the sixth month (162.8 ± 54.70 µM of Pi hr-1 · g-1; P < 0.001) whereas 86Rb uptake increased by 23 percent when compared to initial values. These data suggest that among the different mechanisms which have been advanced to explain the defects in the Na+ pump observed in uremic patients, circulating inhibitors deriving from alimentary protein intake may affect cation transport

The Sigma 13 (10-14) twin in alpha-Al2O3: A model for a general grain boundary

The atomistic structure and energetics of the Sigma 13 (10-14)[1-210] symmetrical tilt grain boundary in alpha-Al2O3 are studied by first-principles calculations based on the local-density-functional theory with a mixed-basis pseudopotential method. Three configurations, stable with respect to intergranular cleavage, are identified: one Al-terminated glide-mirror twin boundary, and two O-terminated twin boundaries, with glide-mirror and two-fold screw-rotation symmetries, respectively. Their relative energetics as a function of axial grain separation are described, and the local electronic structure and bonding are analysed. The Al-terminated variant is predicted to be the most stable one, confirming previous empirical calculations, but in contrast with high-resolution transmission electron microscopy observations on high-purity diffusion-bonded bicrystals, which resulted in an O-terminated structure. An explanation of this discrepancy is proposed, based on the different relative energetics of the internal interfaces with respect to the free surfaces

Bayesian model comparison in cosmology with Population Monte Carlo

We use Bayesian model selection techniques to test extensions of the standard flat LambdaCDM paradigm. Dark-energy and curvature scenarios, and primordial perturbation models are considered. To that end, we calculate the Bayesian evidence in favour of each model using Population Monte Carlo (PMC), a new adaptive sampling technique which was recently applied in a cosmological context. The Bayesian evidence is immediately available from the PMC sample used for parameter estimation without further computational effort, and it comes with an associated error evaluation. Besides, it provides an unbiased estimator of the evidence after any fixed number of iterations and it is naturally parallelizable, in contrast with MCMC and nested sampling methods. By comparison with analytical predictions for simulated data, we show that our results obtained with PMC are reliable and robust. The variability in the evidence evaluation and the stability for various cases are estimated both from simulations and from data. For the cases we consider, the log-evidence is calculated with a precision of better than 0.08. Using a combined set of recent CMB, SNIa and BAO data, we find inconclusive evidence between flat LambdaCDM and simple dark-energy models. A curved Universe is moderately to strongly disfavoured with respect to a flat cosmology. Using physically well-motivated priors within the slow-roll approximation of inflation, we find a weak preference for a running spectral index. A Harrison-Zel'dovich spectrum is weakly disfavoured. With the current data, tensor modes are not detected; the large prior volume on the tensor-to-scalar ratio r results in moderate evidence in favour of r=0. [Abridged]Comment: 11 pages, 6 figures. Matches version accepted for publication by MNRA

Séance spécialisée : géodynamique des bassins océaniques et des marges continentales

Une morphologie de fonds sous-marins bathyaux comportant des indurations liées à des dépôts ferro-manganésifères inclus dans des sédiments hémipélagiques peu ou pas cimentés a été découverte sur une ride volcanique tertiaire au large de la Nouvelle-Calédonie (SW Pacifique). Elle semble être en relation avec des circulations hydrothermales au travers de la couverture sédimentaire pendant l'activité volcanique miocène de la ride des Loyauté. (Résumé d'auteur