Benchmarking Density Functional Based Tight-Binding for Silver and Gold Materials: From Small Clusters to Bulk

International audience

A novel route for FePO4 olivine synthesis from sarcopside oxidation

International audience

Formulación bioinsecticida a partir del aceite esencial de ambrosia arborescens mill (altamisa) de aplicación canina

La presente investigación se planteó reemplazar el uso de insecticidas sintéticos, formulando un champú bioinsecticida de aplicación canina mediante la acción biocida del aceite esencial deAmbrosia arborescens Mill (Altamisa). La planta se recolectó en las laderas del rio Tomebamba, cercanas al Campus Balzay de la Universidad de Cuenca Parroquia San Joaquín. La recolección se realizó durante los meses de Enero a Marzo del 2016. El desarrollo y formulación del producto se realizó en el Laboratorio de Biotecnología, Facultad de Ciencias Químicas de la Universidad de Cuenca. La obtención del aceite esencial de A. arborescens se realizó mediante hidrodestilación por el método Clevenger, con un rendimiento del 0,14%. La actividad biocida se estableció en un ensayo “in vitro” ante el nematodo Panagrellus redivirus, determinándose la dosis letal (DL50) de 250 uL/mL. Debido a la moderada DL50y bajo rendimiento, se planteó como estrategia, determinar el DL50 del extracto orgánico de A. arborescens, el cual se obtuvo mediante una extracción con metanol, consiguiendo un rendimiento del 2 % y DL50de 31,25 uL/mL. De acuerdo estos resultados se procedió a realizar pruebas en pulgas de perros(Ctenocephalides canis) con el extracto de A. arborescens, estableciendo una efectividad del 100 % a la concentración de 46,875 mg/mL en el periodo de tiempo más corto, siendo esta la dosis aplicada para la formulación del champú. El extracto metanólico de A. arborescens presentó elevada actividad biocida, comparado con el aceite esencial. Esta sustancia activa es promisoria en la formulación de bioinsecticidas para mascotas.

Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory

The Pierre Auger Collaboration has reported. evidence for anisotropy in the distribution of arrival directions of the cosmic rays with energies E > E(th) = 5.5 x 10(19) eV. These show a correlation with the distribution of nearby extragalactic objects, including an apparent excess around the direction of Centaurus A. If the particles responsible for these excesses at E > E(th) are heavy nuclei with charge Z, the proton component of the sources should lead to excesses in the same regions at energies E/Z. We here report the lack of anisotropies in these directions at energies above E(th)/Z (for illustrative values of Z = 6, 13, 26). If the anisotropies above E(th) are due to nuclei with charge Z, and under reasonable assumptions about the acceleration process, these observations imply stringent constraints on the allowed proton fraction at the lower energies.

Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory

The Pierre Auger Collaboration has reported. evidence for anisotropy in the distribution of arrival directions of the cosmic rays with energies E > E-th = 5.5 x 10(19) eV. These show a correlation with the distribution of nearby extragalactic objects, including an apparent excess around the direction of Centaurus A. If the particles responsible for these excesses at E > E-th are heavy nuclei with charge Z, the proton component of the sources should lead to excesses in the same regions at energies E/Z. We here report the lack of anisotropies in these directions at energies above E-th/Z (for illustrative values of Z = 6, 13, 26). If the anisotropies above E-th are due to nuclei with charge Z, and under reasonable assumptions about the acceleration process, these observations imply stringent constraints on the allowed proton fraction at the lower energies.

A chemical dictionary, containing the words generally used in chemistry, and many of the terms used in the related sciences of physics, astrophysics, mineralogy, pharmacy, and biology, with their pronunciations, based on recent chemical literature,

Mode of access: Internet.

Spanish-English chemical and medical dictionary; comprising terms employed in medicine, biochemistry, surgery, dentistry, veterinary, biology, pharmacy, allied sciences, and related scientific equipment.

Bibliography: p. 607-609.

English-Spanish chemical and medical dictionary; comprising terms employed in medicine, surgery, dentistry, veterinary, biochemistry, biology, pharmacy, allied sciences and related scientific equipment ...

Mode of access: Internet.

Chemical dictionary, American and British usage. Containing the words generally used in chemistry, and many of the terms used in the related sciences of physics, astrophysics, mineralogy, pharmacy, agriculture, biology, medicine, engineering, etc.; based on recent chemical literature.

Re-issue, with changes and additions of the 3d ed. pub. in 1944.

Researches on the chemical origin of various lines in solar and stellar spectra : being the results of investigations made at the Solar physics observatory, South Kensington, after discussion /

At head of title: Solar physics committee.

Study Of The Homogeneity Of Drug Loaded In Polymeric Films Using Near-infrared Chemical Imaging And Split-plot Design.

Split-plot design (SPD) and near-infrared chemical imaging were used to study the homogeneity of the drug paracetamol loaded in films and prepared from mixtures of the biocompatible polymers hydroxypropyl methylcellulose, polyvinylpyrrolidone, and polyethyleneglycol. The study was split into two parts: a partial least-squares (PLS) model was developed for a pixel-to-pixel quantification of the drug loaded into films. Afterwards, a SPD was developed to study the influence of the polymeric composition of films and the two process conditions related to their preparation (percentage of the drug in the formulations and curing temperature) on the homogeneity of the drug dispersed in the polymeric matrix. Chemical images of each formulation of the SPD were obtained by pixel-to-pixel predictions of the drug using the PLS model of the first part, and macropixel analyses were performed for each image to obtain the y-responses (homogeneity parameter). The design was modeled using PLS regression, allowing only the most relevant factors to remain in the final model. The interpretation of the SPD was enhanced by utilizing the orthogonal PLS algorithm, where the y-orthogonal variations in the design were separated from the y-correlated variation.

Chemical similarities between Galactic bulge and local thick disk red giant stars

Context. The evolution of the Milky Way bulge and its relationship with the other Galactic populations is still poorly understood. The bulge has been suggested to be either a merger-driven classical bulge or the product of a dynamical instability of the inner disk. Aims. To probe the star formation history, the initial mass function and stellar nucleosynthesis of the bulge, we performed an elemental abundance analysis of bulge red giant stars. We also completed an identical study of local thin disk, thick disk and halo giants to establish the chemical differences and similarities between the various populations. Methods. High-resolution infrared spectra of 19 bulge giants and 49 comparison giants in the solar neighborhood were acquired with Gemini/Phoenix. All stars have similar stellar parameters but cover a broad range in metallicity. A standard 1D local thermodynamic equilibrium analysis yielded the abundances of C, N, O and Fe. A homogeneous and differential analysis of the bulge, halo, thin disk and thick disk stars ensured that systematic errors were minimized. Results. We confirm the well-established differences for [O/Fe] (at a given metallicity) between the local thin and thick disks. For the elements investigated, we find no chemical distinction between the bulge and the local thick disk, which is in contrast to previous studies relying on literature values for disk dwarf stars in the solar neighborhood. Conclusions. Our findings suggest that the bulge and local thick disk experienced similar, but not necessarily shared, chemical evolution histories. We argue that their formation timescales, star formation rates and initial mass functions were similar.