Impact d'une alcoolisation précoce sur le rat juvénile et conséquences sur la consommation d'alcool à l'âge adulte.

Contexte : l'adolescence est une période de transition au cours de laquelle l'enfant développe les capacités physiques et cognitives qui lui permettent de s'intégrer au monde adulte et qui se caractérise notamment par une prise de risque, une grande impulsivité et une constante recherche de sensations. Bien que des déterminants sociaux et familiaux entrent en jeu dans ce domaine, il y a également une composante neurobiologique importante. Les avancées techniques dans le domaine de l'imagerie ont permis de mettre en évidence plusieurs changements structurels à l'adolescence tels qu'un remodelage de la matière grise avec une perte de synapses plus ou moins importante selon la région observée et une augmentation de la myélinisation. En outre, le développement cérébral n'est pas uniforme dans le temps. En effet, la maturation du cortex préfrontal est ultérieure au développement du système limbique. Cet asynchronisme pourrait expliquer l'impulsivité des adolescents (consécutive à l'immaturité du cortex préfrontal) et leur comportement de recherche de sensation et/ou de prise de risque (consécutif au développement précoce du noyau accumbens notamment). Ces régions font également partie intégrante du système de récompense et modulent la motivation pour des récompenses naturelles et non-­‐naturelles, comme l'alcool et d'autres drogues. L'émergence d'une consommation d'alcool excessive est justement préoccupante chez les adolescents. En 2007, l'étude ESPAD (The European School Survey Project On Alcohol and Other Drugs) menée auprès de jeunes de 15 à 16 ans relève que 41% des jeunes questionnées ont régulièrement bu jusqu'à l'ivresse dans les 12 mois précédant l'entretien. Les conséquences neuropsychologiques à long terme de ce comportement de « binge-­‐drinking » commencent à alarmer le corps médical, mais l'interrogation demeure sur les risques de ce type de comportement vis-­‐à-­‐vis du développement d'un alcoolisme chronique à l'âge adulte. Objectifs du travail : en s'appuyant sur une revue de la littérature, ce travail a pour objectif d'expliquer les comportements qui émergent à l'adolescence à la lumière des modifications neurobiologiques qui s'opèrent durant cette période critique. Au niveau expérimental, nous proposons d'évaluer la propension de rats juvéniles exposés précocement à de l'alcool à développer un comportement d'abus de consommation d'alcool à l'âge adulte en comparaison avec un groupe contrôle. Dans un deuxième temps nous souhaitons déterminer la propension des rats exposés précocement à de l'alcool à montrer une préférence pour l'alcool par rapport à la saccharine, puis par rapport à de l'eau en comparaison au groupe contrôle. Méthode : nous comparons deux groupes de rongeurs adolescents (âgés de 32 jours à 67 jours). Le groupe test (groupe E, n=8), qui est exposé par un accès ad libitum à une solution d'éthanol 10 % contenant de la saccharine 0.2%, ceci afin de limiter l'aspect gustatif aversif de l'éthanol. Et le groupe témoin (groupe S, n=8), qui est exposé par un accès ad libitum à une solution de saccharine 0.2%. Ce conditionnement se fait sur 13 semaines. Une fois atteinte l'âge adulte, les animaux sont ensuite entraînés à appuyer sur un levier afin de recevoir de l'éthanol (0,1 ml d'une solution à 10%). Nous nous proposons d'évaluer la quantité d'alcool ainsi consommée, puis la motivation des animaux pour obtenir de l'éthanol et enfin leur capacité de résistance à un choc électrique non douloureux mais aversif, lorsque celui-­‐ci est associé à l'éthanol. Enfin, nous évaluerons, via un paradigme de choix à deux leviers, la propension des animaux à choisir de consommer volontairement de l'éthanol quand ils ont le choix entre de l'éthanol 10% et une solution de saccharine à différentes concentrations, puis entre de l'éthanol 10% et de l'eau. Résultats : la phase de tests de comportements à risque d'abus ne permet pas de mettre en évidence une différence significative entre les deux groupes. La phase de test de choix montre une diminution significative du pourcentage d'appuis sur le levier associé à la saccharine avec la diminution de la concentration de saccharine pour les deux groupes. Le groupe S a un pourcentage d'appuis sur le levier associé à l'éthanol significativement plus important que les rats du groupe E et a tendance à préférer l'éthanol pour une concentration de saccharine plus grande que le groupe E. Le groupe S montre également une préférence significative pour l'éthanol quand il n'a plus que le choix avec l'eau alors que le groupe E ne montre pas de préférence. Conclusions : chez des rats élevés dans les mêmes conditons, la consommation précoce d'éthanol n'est pas un facteur de risque de comportements d'abus de consommation d'alcool à l'âge adulte. Cependant un phénomène dit de « sensiblisation croisée » entre le goût sucrée et l'éthanol a été soulevé au cours de cette étude permettant de se questionner sur l'impact d'une consommation intermittente de substances au goût sucré à l'adolescence sur la consommation d'alcool à l'âge adulte

State of the art technologies for front-end hybrids

The front-end hybrids for solid state and gas detectors will be crucial components of the next generation particle detectors. Requirements such as high-density and high-speed interconnects, low mass, radiation resistance, high-current and high-power dissipation capabilities are examples of the challenges to be solved concurrently. The technologies for front-end hybrids developed at CERN are presented and future possibilities such as embedding active and passive circuits are described. Comments are made concerning the ability to use these technologies for large scale production by industry

Scattering of first and second sound waves by quantum vorticity in superfluid Helium

We study the scattering of first and second sound waves by quantum vorticity in superfluid Helium using two-fluid hydrodynamics. The vorticity of the superfluid component and the sound interact because of the nonlinear character of these equations. Explicit expressions for the scattered pressure and temperature are worked out in a first Born approximation, and care is exercised in delimiting the range of validity of the assumptions needed for this approximation to hold. An incident second sound wave will partly convert into first sound, and an incident first sound wave will partly convert into second sound. General considerations show that most incident first sound converts into second sound, but not the other way around. These considerations are validated using a vortex dipole as an explicitely worked out example.Comment: 24 pages, Latex, to appear in Journal of Low Temperature Physic

Clinical course and therapeutic approach to varicella zoster virus infection in children with rheumatic autoimmune diseases under immunosuppression.

To analyze the clinical presentation and complications of varicella zoster virus (VZV) infection in children with rheumatic diseases treated with immunosuppressive medication such as biological disease-modifying antirheumatic drugs (bDMARDs) and/or conventional disease-modifying antirheumatic drugs (cDMARDs), and to analyze the therapeutic approach to VZV infections with respect to the concomitant immunosuppressive treatment. Retrospective multicenter study using the Swiss Pediatric Rheumatology registry. Children with rheumatic diseases followed in a Swiss center for pediatric rheumatology and treated with cDMARD and/or bDMARD with a clinical diagnosis of varicella or herpes zoster between January 2004 and December 2013 were included. Twenty-two patients were identified, of whom 20 were treated for juvenile idiopathic arthritis, 1 for a polyglandular autoimmune syndrome type III, and 1 for uveitis. Of these 22 patients, 16 had varicella and 6 had herpes zoster. Median age at VZV disease was 7.6 years (range 2 to 17 years), with 6.3 years (range 2 to 17 years) for those with varicella and 11.6 years (range 5 to 16 years) for those with herpes zoster. The median interval between start of immunosuppression and VZV disease was 14.1 months (range 1 to 63 months). Two patients had received varicella vaccine (1 dose each) prior to start of immunosuppression. Concomitant immunosuppressive therapy was methotrexate (MTX) monotherapy (n = 9) or bDMARD monotherapy (n = 2), or a combination of bDMARD with prednisone, MTX or Leflunomide (n = 11). Four patients experienced VZV related complications: cellulitis in 1 patient treated with MTX, and cellulitis, sepsis and cerebellitis in 3 patients treated with biological agents and MTX combination therapy. Six children were admitted to hospital (range of duration: 4 to 9 days) and 12 were treated with valaciclovir or aciclovir. The clinical course of varicella and herpes zoster in children under immunosuppression is variable, with 4 (18 %) of 22 children showing a complicated course. Thorough assessment of VZV disease and vaccination history and correct VZV vaccination according to national guidelines at diagnosis of a rheumatic autoimmune disease is essential to minimize VZV complications during a later immunosuppressive treatment

Carbon Nanotubes by a CVD Method. Part I: Synthesis and Characterization of the (Mg, Fe)O Catalysts

The controlled synthesis of carbon nanotubes by chemical vapor deposition requires tailored and wellcharacterized catalyst materials. We attempted to synthesize Mg1-xFexO oxide solid solutions by the combustion route, with the aim of performing a detailed investigation of the influence of the synthesis conditions (nitrate/urea ratio and the iron content) on the valency and distribution of the iron ions and phases. Notably, characterization of the catalyst materials is performed using 57Fe Mo¨ssbauer spectroscopy, X-ray diffraction, and electron microscopy. Several iron species are detected including Fe2+ ions substituting for Mg2+ in the MgO lattice, Fe3+ ions dispersed in the octahedral sites of MgO, different clusters of Fe3+ ions, and MgFe2O4-like nanoparticles. The dispersion of these species and the microstructure of the oxides are discussed. Powders markedly different from one another that may serve as model systems for further study are identified. The formation of carbon nanotubes upon reduction in a H2/CH4 gas atmosphere of the selected powders is reported in a companion paper

A statistical method to determine open cluster metallicities

The study of open cluster metallicities helps to understand the local stellar formation and evolution throughout the Milky Way. Its metallicity gradient is an important tracer for the Galactic formation in a global sense. Because open clusters can be treated in a statistical way, the error of the cluster mean is minimized. Our final goal is a semi-automatic statistical robust method to estimate the metallicity of a statistically significant number of open clusters based on Johnson BV data of their members, an algorithm that can easily be extended to other photometric systems for a systematic investigation. This method incorporates evolutionary grids for different metallicities and a calibration of the effective temperature and luminosity. With cluster parameters (age, reddening and distance) it is possible to estimate the metallicity from a statistical point of view. The iterative process includes an intrinsic consistency check of the starting input parameters and allows us to modify them. We extensively tested the method with published data for the Hyades and selected sixteen open clusters within 1000pc around the Sun with available and reliable Johnson BV measurements. In addition, Berkeley 29, with a distance of about 15kpc was chosen. For several targets we are able to compare our result with published ones which yielded a very good coincidence (including Berkeley 29).Comment: 14 pages, 6 figures, accepted for publication in Astronomy & Astrophysic

Drug vaping applied to cannabis: Is "Cannavaping" a therapeutic alternative to marijuana?

Therapeutic cannabis administration is increasingly used in Western countries due to its positive role in several pathologies. Dronabinol or tetrahydrocannabinol (THC) pills, ethanolic cannabis tinctures, oromucosal sprays or table vaporizing devices are available but other cannabinoids forms can be used. Inspired by the illegal practice of dabbing of butane hashish oil (BHO), cannabinoids from cannabis were extracted with butane gas, and the resulting concentrate (BHO) was atomized with specific vaporizing devices. The efficiency of "cannavaping," defined as the "vaping" of liquid refills for e-cigarettes enriched with cannabinoids, including BHO, was studied as an alternative route of administration for therapeutic cannabinoids. The results showed that illegal cannavaping would be subjected to marginal development due to the poor solubility of BHO in commercial liquid refills (especially those with high glycerin content). This prevents the manufacture of liquid refills with high BHO concentrations adopted by most recreational users of cannabis to feel the psychoactive effects more rapidly and extensively. Conversely, "therapeutic cannavaping" could be an efficient route for cannabinoids administration because less concentrated cannabinoids-enriched liquid refills are required. However, the electronic device marketed for therapeutic cannavaping should be carefully designed to minimize potential overheating and contaminant generation

Nighttime chlorine monoxide observations by the Odin satellite and implications for the ClO/Cl2O2 equilibrium

We use measurements of chlorine monoxide (ClO) by the SMR instrument onboard the Odin satellite to study the nighttime thermal equilibrium between ClO and its dimer Cl2O2. Observations performed in the polar vortex during the 2002–2003 Arctic winter showed enhanced amounts of nighttime ClO over a wide range of stratospheric temperatures (185 < T < 225 K). Odin/SMR measurements are here compared to three-dimensional model calculations using various published estimations of the Keq equilibrium constant between ClO and Cl2O2. Our results show that the value of Keq currently recommended by JPL (Sander et al., 2003) leads to a large underestimation of the observed nighttime ClO amounts, and that a realistic estimation of Keq must lie between the values determined by Cox and Hayman (1988) and Von Hobe et al. (2005)

Convection, Thermal Bifurcation, and the Colors of A stars

Broad-band ultraviolet photometry from the TD-1 satellite and low dispersion spectra from the short wavelength camera of IUE have been used to investigate a long-standing proposal of Bohm-Vitense that the normal main sequence A- and early-F stars may divide into two different temperature sequences: (1) a high temperature branch (and plateau) comprised of slowly rotating convective stars, and (2) a low temperature branch populated by rapidly rotating radiative stars. We find no evidence from either dataset to support such a claim, or to confirm the existence of an "A-star gap" in the B-V color range 0.22 <= B-V <= 0.28 due to the sudden onset of convection. We do observe, nonetheless, a large scatter in the 1800--2000 A colors of the A-F stars, which amounts to ~0.65 mags at a given B-V color index. The scatter is not caused by interstellar or circumstellar reddening. A convincing case can also be made against binarity and intrinsic variability due to pulsations of delta Sct origin. We find no correlation with established chromospheric and coronal proxies of convection, and thus no demonstrable link to the possible onset of convection among the A-F stars. The scatter is not instrumental. Approximately 0.4 mags of the scatter is shown to arise from individual differences in surface gravity as well as a moderate spread (factor of ~3) in heavy metal abundance and UV line blanketing. A dispersion of ~0.25 mags remains, which has no clear and obvious explanation. The most likely cause, we believe, is a residual imprecision in our correction for the spread in metal abundances. However, the existing data do not rule out possible contributions from intrinsic stellar variability or from differential UV line blanketing effects owing to a dispersion in microturbulent velocity.Comment: 40 pages, 14 figures, 1 table, AAS LaTex, to appear in The Astrophysical Journa

Fe/Co Alloys for the Catalytic Chemical Vapor Deposition Synthesis of Single- and Double-Walled Carbon Nanotubes (CNTs). 1. The CNT−Fe/Co−MgO System

Mg0.90FexCoyO (x + y ) 0.1) solid solutions were synthesized by the ureic combustion route. Upon reduction at 1000 °C in H2-CH4 of these powders, Fe/Co alloy nanoparticles are formed, which are involved in the formation of carbon nanotubes, which are mostly single and double walled, with an average diameter close to 2.5 nm. Characterizations of the materials are performed using 57Fe Mo¨ssbauer spectroscopy and electron microscopy, and a well-established macroscopic method, based on specific-surface-area measurements, was applied to quantify the carbon quality and the nanotubes quantity. A detailed investigation of the Fe/Co alloys’ formation and composition is reported. An increasing fraction of Co2+ ions hinders the dissolution of iron in the MgO lattice and favors the formation of MgFe2O4-like particles in the oxide powders. Upon reduction, these particles form R-Fe/Co particles with a size and composition (close to Fe0.50Co0.50) adequate for the increased production of carbon nanotubes. However, larger particles are also produced resulting in the formation of undesirable carbon species. The highest CNT quantity and carbon quality are eventually obtained upon reduction of the iron-free Mg0.90Co0.10O solid solution, in the absence of clusters of metal ions in the starting material. Introduction Catalyti