The Na+/H+ exchanger Nhx1 of Saccharomyces cerevisiae is essential to limit drug toxicity

Nhx1 est un antiport vacuolaire de Na+/H+ chez la levure Saccharomyces cerevisiae. Nhx1 joue un rôle important dans le maintien de l’homéostasie ionique du cytoplasme de la cellule. En effet, la mutation du gène NHX1 chez la levure nhx1Δ entraîne une perte de l’homéostasie cellulaire quand les cellules sont cultivées dans un milieu de faible osmolarité. Ce travail rapporte pour la première fois, et contrairement à la cellule parentale, que la mutation du gène NHX1 a pour effet une sensibilité du mutant nhx1Δ à une variété des drogues et des agents cationiques et anioniques lorsque les cellules sont cultivées dans un milieu riche. En outre, dans ces conditions de culture, aucune sensibilité n’a été observée chez le mutant nhx1Δ quand les cellules sont traitées avec différentes concentrations de sel. Nous avons aussi démontré que la sensibilité du mutant nhx1Δ aux différents agents ainsi que la sécrétion de l’enzyme carboxypeptidase Y observé chez ce mutant n’ont pas été restauré lorsque les cellules sont cultivées dans des milieux avec différents pH ou avec différentes concentrations de sel. Enfin, une analyse génétique a révélé que le mutant nhx1Δ montre un phénotype distinct d’autres mutants qui ont un défaut dans le trafic entre le compartiment pré-vacuolaire et l’appareil de Golgi quand ces cellules sont traitées avec différents agents. Cette analyse prouve que la sensibilité de nhx1Δ aux différents agents n’est pas liée au trafic entre le compartiment pré-vacuolaire et l’appareil de Golgi.

Programme d'entraînement aux habiletés sociales pour des enfants ayant un trouble envahissant du développement non spécifié

Rapport d'analyse d'intervention présenté à la Faculté des arts et sciences en vue de l'obtention du grade de Maîtrise ès sciences (M. Sc.) en psychoéducation.

Surveillance non invasive de la réponse neuroimmunitaire fœtale à l’infection

Introduction. In utero, l’infection des membranes maternelles et fœtales, la chorioamniotite, passe souvent inaperçue et, en particulier lorsque associée à une acidémie, due à l’occlusion du cordon ombilical (OCO), comme il se produirait au cours du travail, peut entrainer des lésions cérébrales et avoir des répercussions neurologiques péri - et postnatales à long terme chez le fœtus. Il n'existe actuellement aucun moyen de détecter précocement ces conditions pathologiques in utéro afin de prévenir ou de limiter ces atteintes. Hypothèses. 1)l’électroencéphalogramme (EEG) fœtal obtenu du scalp fœtal pourrait servir d’outil auxiliaire à la surveillance électronique fœtale du rythme cardiaque fœtal (RCF) pour la détection précoce d'acidémie fœtale et d'agression neurologique; 2) la fréquence d’échantillonnage de l’ECG fœtal (ECGf) a un impact important sur le monitoring continu de la Variabilité du Rythme Cardiaque (VRCf) dans la prédiction de l’acidémie fœtale ; 3) les patrons de la corrélation de la VRCf aux cytokines pro-inflammatoires refléteront les états de réponses spontanées versus inflammatoires de la Voie Cholinergique Anti-inflammatoire (VCA); 4) grâce au développement d’un modèle de prédictions mathématiques, la prédiction du pH et de l’excès de base (EB) à la naissance sera possible avec seulement une heure de monitoring d’ECGf. Méthodes. Dans une série d’études fondamentales et cliniques, en utilisant respectivement le mouton et une cohorte de femmes en travail comme modèle expérimental et clinique , nous avons modélisé 1) une situation d’hypoxie cérébrale résultant de séquences d’occlusion du cordon ombilical de sévérité croissante jusqu’à atteindre un pH critique limite de 7.00 comme méthode expérimentale analogue au travail humain pour tester les première et deuxième hypothèses 2) un inflammation fœtale modérée en administrant le LPS à une autre cohorte animale pour vérifier la troisième hypothèse et 3) un modèle mathématique de prédictions à partir de paramètres et mesures validés cliniquement qui permettraient de déterminer les facteurs de prédiction d’une détresse fœtale pour tester la dernière hypothèse. Résultats. Les séries d’OCO répétitives se sont soldés par une acidose marquée (pH artériel 7.35±0.01 à 7.00±0.01), une diminution des amplitudes à l'électroencéphalogramme( EEG) synchronisé avec les décélérations du RCF induites par les OCO accompagnées d'une baisse pathologique de la pression artérielle (PA) et une augmentation marquée de VRCf avec hypoxie-acidémie aggravante à 1000 Hz, mais pas à 4 Hz, fréquence d’échantillonnage utilisée en clinique. L’administration du LPS entraîne une inflammation systémique chez le fœtus avec les IL-6 atteignant un pic 3 h après et des modifications de la VRCf retraçant précisément ce profil temporel des cytokines. En clinique, avec nos cohortes originale et de validation, un modèle statistique basée sur une matrice de 103 mesures de VRCf (R2 = 0,90, P < 0,001) permettent de prédire le pH mais pas l’EB, avec une heure d’enregistrement du RCF avant la poussée. Conclusions. La diminution de l'amplitude à l'EEG suggère un mécanisme d'arrêt adaptatif neuroprotecteur du cerveau et suggère que l'EEG fœtal puisse être un complément utile à la surveillance du RCF pendant le travail à haut risque chez la femme. La VRCf étant capable de détecter une hypoxie-acidémie aggravante tôt chez le fœtus à 1000Hz vs 4 Hz évoque qu’un mode d'acquisition d’ECG fœtal plus sensible pourrait constituer une solution. Des profils distinctifs de mesures de la VRCf, identifiés en corrélation avec les niveaux de l'inflammation, ouvre une nouvelle voie pour caractériser le profil inflammatoire de la réponse fœtale à l’infection. En clinique, un monitoring de chevet de prédiction du pH et EB à la naissance, à partir de mesures de VRCf permettrait des interprétations visuelles plus explicites pour des prises de décision plus exactes en obstétrique au cours du travail.

The sky is the limit? The determinants and constraints of European airports' commercial revenues

This study investigates the determinants of commercial and retail airport revenues as well as revenues from real estate operations. Cross-sectional OLS, 2SLS and robust regression models of European airports identify a number of significant drivers of airport revenues. Aviation revenues per passenger are mainly determined by the national income per capita in which the airport is located, the percentage of leisure travelers and the size of the airport proxied by total aviation revenues. Main drivers of commercial revenues per passenger include the total number of passengers passing through the airport, the ratio of commercial to total revenues, the national income, the share of domestic and leisure travelers and the total number of flights. These results are in line with previous findings of a negative influence of business travelers on commercial revenues per passenger. We also find that a high amount of retail space per passenger is generally associated with lower commercial revenues per square meter confirming decreasing marginal revenue effects. Real estate revenues per passenger are positively associated with national income per capita at airport location, share of intra-EU passengers and percent delayed flights. Overall, aviation and non-aviation revenues appear to be strongly interlinked, underlining the potential for a comprehensive airport management strategy above and beyond mere cost minimization of the aviation sector.

Limit operators, collective compactness, and the spectral theory of infinite matrices

In the first half of this memoir we explore the interrelationships between the abstract theory of limit operators (see e.g. the recent monographs of Rabinovich, Roch and Silbermann (2004) and Lindner (2006)) and the concepts and results of the generalised collectively compact operator theory introduced by Chandler-Wilde and Zhang (2002). We build up to results obtained by applying this generalised collectively compact operator theory to the set of limit operators of an operator (its operator spectrum). In the second half of this memoir we study bounded linear operators on the generalised sequence space , where and is some complex Banach space. We make what seems to be a more complete study than hitherto of the connections between Fredholmness, invertibility, invertibility at infinity, and invertibility or injectivity of the set of limit operators, with some emphasis on the case when the operator is a locally compact perturbation of the identity. Especially, we obtain stronger results than previously known for the subtle limiting cases of and . Our tools in this study are the results from the first half of the memoir and an exploitation of the partial duality between and and its implications for bounded linear operators which are also continuous with respect to the weaker topology (the strict topology) introduced in the first half of the memoir. Results in this second half of the memoir include a new proof that injectivity of all limit operators (the classic Favard condition) implies invertibility for a general class of almost periodic operators, and characterisations of invertibility at infinity and Fredholmness for operators in the so-called Wiener algebra. In two final chapters our results are illustrated by and applied to concrete examples. Firstly, we study the spectra and essential spectra of discrete Schrödinger operators (both self-adjoint and non-self-adjoint), including operators with almost periodic and random potentials. In the final chapter we apply our results to integral operators on .

Impact of non-hydrostatic effects and trapped lee waves on mountain wave drag in directionally sheared flow

The orographic gravity wave drag produced in flow over an axisymmetric mountain when both vertical wind shear and non-hydrostatic effects are important was calculated using a semi-analytical two-layer linear model, including unidirectional or directional constant wind shear in a layer near the surface, above which the wind is constant. The drag behaviour is determined by partial wave reflection at the shear discontinuity, wave absorption at critical levels (both of which exist in hydrostatic flow), and total wave reflection at levels where the waves become evanescent (an intrinsically non-hydrostatic effect), which produces resonant trapped lee wave modes. As a result of constructive or destructive wave interference, the drag oscillates with the thickness of the constant-shear layer and the Richardson number within it (Ri), generally decreasing at low Ri and when the flow is strongly non-hydrostatic. Critical level absorption, which increases with the angle spanned by the wind velocity in the constant-shear layer, shields the surface from reflected waves, keeping the drag closer to its hydrostatic limit. While, for the parameter range considered here, the drag seldom exceeds this limit, a substantial drag fraction may be produced by trapped lee waves, particularly when the flow is strongly non-hydrostatic, the lower layer is thick and Ri is relatively high. In directionally sheared flows with Ri = O(1), the drag may be misaligned with the surface wind in a direction opposite to the shear, a behaviour which is totally due to non-trapped waves. The trapped lee wave drag, whose reaction force on the atmosphere is felt at low levels, may therefore have a distinctly different direction from the drag associated with vertically propagating waves, which acts on the atmosphere at higher levels.

On translational superfluidity and the Landau criterion for Bose gases in the Gross-Pitaevski limit

The two-fluid and Landau criteria for superfluidity are compared for trapped Bose gases. While the two-fluid criterion predicts translational superfluidity, it is suggested, on the basis of the homogeneous Gross-Pitaevski limit, that a necessary part of Landau`s criterion, adequate for non-translationally invariant systems, does not hold for trapped Bose gases in the GP limit. As a consequence, if the compressibility is detected to be very large (infinite by experimental standards), the two-fluid criterion is seen to be the relevant one in case the system is a translational superfluid, while the Landau criterion is the relevant one if translational superfluidity is absent.

A Trotter-Kato product formula for a class of non-autonomous evolution equations

In this article dedicated to Professor V. Lakshmikantham on the occasion of the celebration of his 84th birthday, we announce new results concerning the existence and various properties of an evolution system UA+B(t, s)(0 <= s <= t <= T) generated by the sum -(A(t)+B(t)) of two linear, time-dependent and generally unbounded operators defined on time-dependent domains in a complex and separable Banach space B. In particular, writing G(B) for the algebra of all linear bounded operators on B, we can express UA+B(t, s)(0 <= s <= t <= T) as the strong limit in L(B) of a product of the holomorphic contraction semigroups generated by -A(t) and -B(t), thereby getting a product formula of the Trotter-Kato type under very general conditions which allow the domain D(A(t)+B(t)) to evolve with time provided there exists a fixed set D subset of boolean AND D-t epsilon[0,D-T](A(t)+B(t)) everywhere dense in B. We then mention several possible applications of our product formula to various classes of non-autonomous parabolic initial-boundary value problems, as well as to evolution problems of Schrodinger type related to the theory of time-dependent singular perturbations of self-adjoint operators in quantum mechanics. We defer all the proofs and all the details of the applications to a separate publication. (C) 2008 Elsevier Ltd. All rights reserved.

Coherent and semiclassical states in a magnetic field in the presence of the Aharonov-Bohm solenoid

A new approach to constructing coherent states (CS) and semiclassical states (SS) in a magnetic-solenoid field is proposed. The main idea is based on the fact that the AB solenoid breaks the translational symmetry in the xy-plane; this has a topological effect such that there appear two types of trajectories which embrace and do not embrace the solenoid. Due to this fact, one has to construct two different kinds of CS/SS which correspond to such trajectories in the semiclassical limit. Following this idea, we construct CS in two steps, first the instantaneous CS (ICS) and then the time-dependent CS/SS as an evolution of the ICS. The construction is realized for nonrelativistic and relativistic spinning particles both in (2 + 1) and (3 + 1) dimensions and gives a non-trivial example of SS/CS for systems with a nonquadratic Hamiltonian. It is stressed that CS depending on their parameters (quantum numbers) describe both pure quantum and semiclassical states. An analysis is represented that classifies parameters of the CS in such respect. Such a classification is used for the semiclassical decompositions of various physical quantities.

Efeitos não-gaussianos em astrofísica e cosmologia

The recent astronomical observations indicate that the universe has null spatial curvature, is accelerating and its matter-energy content is composed by circa 30% of matter (baryons + dark matter) and 70% of dark energy, a relativistic component with negative pressure. However, in order to built more realistic models it is necessary to consider the evolution of small density perturbations for explaining the richness of observed structures in the scale of galaxies and clusters of galaxies. The structure formation process was pioneering described by Press and Schechter (PS) in 1974, by means of the galaxy cluster mass function. The PS formalism establishes a Gaussian distribution for the primordial density perturbation field. Besides a serious normalization problem, such an approach does not explain the recent cluster X-ray data, and it is also in disagreement with the most up-to-date computational simulations. In this thesis, we discuss several applications of the nonextensive q-statistics (non-Gaussian), proposed in 1988 by C. Tsallis, with special emphasis in the cosmological process of the large structure formation. Initially, we investigate the statistics of the primordial fluctuation field of the density contrast, since the most recent data from the Wilkinson Microwave Anisotropy Probe (WMAP) indicates a deviation from gaussianity. We assume that such deviations may be described by the nonextensive statistics, because it reduces to the Gaussian distribution in the limit of the free parameter q = 1, thereby allowing a direct comparison with the standard theory. We study its application for a galaxy cluster catalog based on the ROSAT All-Sky Survey (hereafter HIFLUGCS). We conclude that the standard Gaussian model applied to HIFLUGCS does not agree with the most recent data independently obtained by WMAP. Using the nonextensive statistics, we obtain values much more aligned with WMAP results. We also demonstrate that the Burr distribution corrects the normalization problem. The cluster mass function formalism was also investigated in the presence of the dark energy. In this case, constraints over several cosmic parameters was also obtained. The nonextensive statistics was implemented yet in 2 distinct problems: (i) the plasma probe and (ii) in the Bremsstrahlung radiation description (the primary radiation from X-ray clusters); a problem of considerable interest in astrophysics. In another line of development, by using supernova data and the gas mass fraction from galaxy clusters, we discuss a redshift variation of the equation of state parameter, by considering two distinct expansions. An interesting aspect of this work is that the results do not need a prior in the mass parameter, as usually occurs in analyzes involving only supernovae data.Finally, we obtain a new estimate of the Hubble parameter, through a joint analysis involving the Sunyaev-Zeldovich effect (SZE), the X-ray data from galaxy clusters and the baryon acoustic oscillations. We show that the degeneracy of the observational data with respect to the mass parameter is broken when the signature of the baryon acoustic oscillations as given by the Sloan Digital Sky Survey (SDSS) catalog is considered. Our analysis, based on the SZE/X-ray data for a sample of 25 galaxy clusters with triaxial morphology, yields a Hubble parameter in good agreement with the independent studies, provided by the Hubble Space Telescope project and the recent estimates of the WMAP

Position-dependent effective mass Dirac equations with PT-symmetric and non-PT-symmetric potentials

We present a new procedure to construct the one-dimensional non-Hermitian imaginary potential with a real energy spectrum in the context of the position-dependent effective mass Dirac equation with the vector-coupling scheme in 1 + 1 dimensions. In the first example, we consider a case for which the mass distribution combines linear and inversely linear forms, the Dirac problem with a PT-symmetric potential is mapped into the exactly solvable Schrodinger-like equation problem with the isotonic oscillator by using the local scaling of the wavefunction. In the second example, we take a mass distribution with smooth step shape, the Dirac problem with a non-PT-symmetric imaginary potential is mapped into the exactly solvable Schrodinger-like equation problem with the Rosen-Morse potential. The real relativistic energy levels and corresponding wavefunctions for the bound states are obtained in terms of the supersymmetric quantum mechanics approach and the function analysis method.

Non-Zeeman splitting for a spin-resolved STM with a Kondo adatom in a spin-polarized two-dimensional electron gas

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

Non-lacunary Gibbs Measures for Certain Fractal Repellers

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Universal scaling in Bardeen-Cooper-Schrieffer superconductivity in two dimensions in non-s waves

The solutions of a renormalized BCS model are studied in two space dimensions for s, p and d waves for finite-range separable potentials. The gap parameter, the critical temperature T-c, the coherence length xi and the jump in specific heat at T-c as a function of the zero-temperature condensation energy exhibit universal scalings. In the weak-coupling limit, the present model yields a small xi and large T-c, appropriate for high-T-c cuprates. The specific heat, penetration depth and thermal conductivity as functions of temperature show universal scaling for p and d waves.

The impossibility of a universal relativistic temperature transformation

The non-existence of a relativistic temperature transformation is due to the fact that an observer moving in a heat reservoir cannot detect a blackbody spectrum. (C) 2004 Published by Elsevier B.V.