Risk factors for positive tuberculin skin tests among migrant and resident children in Lausanne, Switzerland

Résumé en français Cadre : Policlinique pédiatrique à Lausanne en Suisse, pays rencontrant une proportion importante de tuberculose au sein de la population de migrants. But : Déterminer les facteurs de risque associés à un test tuberculinique positif (ou test de Mantoux), notamment l'influence du BCG (Bacille Calmette Guérin) et d'un contact avec un personne ayant une tuberculose active. Les patients concernés étaient des enfants examinés dans le cadre d'un contrôle de santé ou dans le cadre d'une étude d'entourage d'un cas déclaré de tuberculose. Méthode : Etude descriptive comprenant des enfants ayant eu un test tuberculinique (2 unités RT23) entre novembre 2002 et avril 2004. L'âge, le sexe, l'anamnèse de contact avec une personne ayant une tuberculose active, la vaccination par le BCG, le pays d'origine et le lieu de naissance (en Suisse ou hors de la Suisse) étaient répertoriés. Résultats : Parmi les 234 enfants de l'étude, 176 (75%) avaient une réaction tuberculinique égal à zéro et 31 (13%) avaient une réaction positive (> 10mm). Dans le modèle de régression linéaire, la taille de la réaction tuberculinique variait significativement selon l'anamnèse de contact avec une personne ayant une tuberculose active, l'âge, l'incidence de la tuberculose dans le pays d'origine et la vaccination par le BCG. Le sexe ou le lieu de naissance n'influençait pas la taille de la réaction. Dans le modèle de régression logistique incluant toutes les valeurs répertoriées, les paramètres significativement associés avec un Mantoux positif étaient l'âge (Odds Ratio = 1.21, 95% CI 1.08 ; 1.35), l'anamnèse de contact avec une personne ayant une tuberculose active (OR = 7.31, 95% CI 2.23 ; 24) et l'incidence de la tuberculose dans le pays d'origine (OR = 1.01, 95% CI 1.00 ; 1.02). Le sexe (OR = 1.18, 95% CI 0.50 ; 2.78) et la vaçcination par le BCG (OR = 2.97, 95% CI 0.91 ; 9.72) n'étaient pas associés avec une réaction tuberculinique positive. Conclusions : L'incidence de la tuberculose dans le pays d'origine, la vaccination par le BCG et l'âge influencent le test de Mantoux (taille ou proportion de réaction > 10mm). Toutefois, le facteur de risque le plus important d'avoir une réaction tuberculinique positive est l'anamnèse de contact avec. une personne ayant une tuberculose active

A concentration inequality for interval maps with an indifferent fixed point

For a map of the unit interval with an indifferent fixed point, we prove an upper bound for the variance of all observables of $n$ variables $K:[0,1]^n\to\R$ which are componentwise Lipschitz. The proof is based on coupling and decay of correlation properties of the map. We then give various applications of this inequality to the almost-sure central limit theorem, the kernel density estimation, the empirical measure and the periodogram.Comment: 26 pages, submitte

Complexity for extended dynamical systems

We consider dynamical systems for which the spatial extension plays an important role. For these systems, the notions of attractor, epsilon-entropy and topological entropy per unit time and volume have been introduced previously. In this paper we use the notion of Kolmogorov complexity to introduce, for extended dynamical systems, a notion of complexity per unit time and volume which plays the same role as the metric entropy for classical dynamical systems. We introduce this notion as an almost sure limit on orbits of the system. Moreover we prove a kind of variational principle for this complexity.Comment: 29 page

On the degenerated soft-mode instability

We consider instabilities of a single mode with finite wavenumber in inversion symmetric spatially one dimensional systems, where the character of the bifurcation changes from sub- to supercritical behaviour. Starting from a general equation of motion the full amplitude equation is derived systematically and formulas for the dependence of the coefficients on the system parameters are obtained. We emphasise the importance of nonlinear derivative terms in the amplitude equation for the behaviour in the vicinity of the bifurcation point. Especially the numerical values of the corresponding coefficients determine the region of coexistence between the stable trivial solution and stable spatially periodic patterns. Our approach clearly shows that similar considerations fail for the case of oscillatory instabilities.Comment: 16 pages, uses iop style files, manuscript also available at ftp://athene.fkp.physik.th-darmstadt.de/pub/publications/wolfram/jpa_97/ or at http://athene.fkp.physik.th-darmstadt.de/public/wolfram_publ.html. J. Phys. A in pres

Potencial construtivo em projetos de habitação de interesse social: Jardim Edith / Comandante Taylor

Peer Reviewe

A Two-Parameter Recursion Formula For Scalar Field Theory

We present a two-parameter family of recursion formulas for scalar field theory. The first parameter is the dimension $(D)$. The second parameter ($\zeta$) allows one to continuously extrapolate between Wilson's approximate recursion formula and the recursion formula of Dyson's hierarchical model. We show numerically that at fixed $D$, the critical exponent $\gamma$ depends continuously on $\zeta$. We suggest the use of the $\zeta -$independence as a guide to construct improved recursion formulas.Comment: 7 pages, uses Revtex, one Postcript figur

High-precision abundances of elements in Kepler LEGACY stars. Verification of trends with stellar age

HARPS-N spectra with S/N > 250 and MARCS model atmospheres were used to derive abundances of C, O, Na, Mg, Al, Si, Ca, Ti, Cr, Fe, Ni, Zn, and Y in ten stars from the Kepler LEGACY sample (including the binary pair 16 Cyg A and B) selected to have metallicities in the range -0.15 < [Fe/H] < +0.15 and ages between 1 and 7 Gyr. Stellar gravities were obtained from seismic data and effective temperatures were determined by comparing non-LTE iron abundances derived from FeI and FeII lines. Available non-LTE corrections were also applied when deriving abundances of the other elements. The results support the [X/Fe]-age relations previously found for solar twins. [Mg/Fe], [Al/Fe], and [Zn/Fe] decrease by ~0.1 dex over the lifetime of the Galactic thin disk due to delayed contribution of iron from Type Ia supernovae relative to prompt production of Mg, Al, and Zn in Type II supernovae. [Y/Mg] and [Y/Al], on the other hand, increase by ~0.3 dex, which can be explained by an increasing contribution of s-process elements from low-mass AGB stars as time goes on. The trends of [C/Fe] and [O/Fe] are more complicated due to variations of the ratio between refractory and volatile elements among stars of similar age. Two stars with about the same age as the Sun show very different trends of [X/H] as a function of elemental condensation temperature Tc and for 16 Cyg, the two components have an abundance difference, which increases with Tc. These anomalies may be connected to planet-star interactions.Comment: 13 pages with 7 figures. Accepted for publication in A&

Evolving localizations in reaction-diffusion cellular automata

We consider hexagonal cellular automata with immediate cell neighbourhood and three cell-states. Every cell calculates its next state depending on the integral representation of states in its neighbourhood, i.e. how many neighbours are in each one state. We employ evolutionary algorithms to breed local transition functions that support mobile localizations (gliders), and characterize sets of the functions selected in terms of quasi-chemical systems. Analysis of the set of functions evolved allows to speculate that mobile localizations are likely to emerge in the quasi-chemical systems with limited diffusion of one reagent, a small number of molecules is required for amplification of travelling localizations, and reactions leading to stationary localizations involve relatively equal amount of quasi-chemical species. Techniques developed can be applied in cascading signals in nature-inspired spatially extended computing devices, and phenomenological studies and classification of non-linear discrete systems.Comment: Accepted for publication in Int. J. Modern Physics

Can we trust elemental abundances derived in late-type giants with the classical 1D stellar atmosphere models?

We compare the abundances of various chemical species as derived with 3D hydrodynamical and classical 1D stellar atmosphere codes in a late-type giant characterized by T_eff=3640K, log g = 1.0, [M/H] = 0.0. For this particular set of atmospheric parameters the 3D-1D abundance differences are generally small for neutral atoms and molecules but they may reach up to 0.3-0.4 dex in case of ions. The 3D-1D differences generally become increasingly more negative at higher excitation potentials and are typically largest in the optical wavelength range. Their sign can be both positive and negative, and depends on the excitation potential and wavelength of a given spectral line. While our results obtained with this particular late-type giant model suggest that 1D stellar atmosphere models may be safe to use with neutral atoms and molecules, care should be taken if they are exploited with ions.Comment: Poster presented at the IAU Symposium 265 "Chemical Abundances in the Universe: Connecting First Stars to Planets", Rio de Janeiro, 10-14 August 2009; 2 pages, 1 figur