Microcrystalline silicon thin film transistors obtained by Hot-Wire CVD

Polysilicon thin film transistors (TFT) are of great interest in the field of large area microelectronics, especially because of their application as active elements in flat panel displays. Different deposition techniques are in tough competition with the objective to obtain device-quality polysilicon thin films at low temperature. In this paper we present the preliminary results obtained with the fabrication of TFT deposited by hot-wire chemical vapor deposition (HWCVD). Some results concerned with the structural characterization of the material and electrical performance of the device are presented.

Thin Film Transistors obtained by Hot-Wire CVD

Hydrogenated microcrystalline silicon films obtained at low temperature (150-280°C) by hot wire chemical vapour deposition at two different process pressures were measured by Raman spectroscopy, X-ray diffraction (XRD) spectroscopy and photothermal deflection spectroscopy (PDS). A crystalline fraction >90% with a subgap optical absortion 10 cm -1 at 0.8 eV were obtained in films deposited at growth rates >0.8 nm/s. These films were incorporated in n-channel thin film transistors and their electrical properties were measured. The saturation mobility was 0.72 ± 0.05 cm 2/ V s and the threshold voltage around 0.2 eV. The dependence of their conductance activation energies on gate voltages were related to the properties of the material.

High mass microquasars and low latitude gamma-ray sources

Population studies of unidentified EGRET sources suggest that there exist at least three different populations of galactic gamma-ray sources. One of these populations is formed by young objects distributed along the galactic plane with a strong concentration toward the inner spiral arms of the Galaxy. Variability, spectral and correlation analysis indicate that this population is not homogeneous. In particular, there is a subgroup of sources that display clear variability in their gamma-ray fluxes on timescales from days to months. Following the proposal by Kaufman Bernad\'o et al. (2002), we suggest that this group of sources might be high-mass microquasars, i.e. accreting black holes or neutron stars with relativistic jets and early-type stellar companions. We present detailed inhomogeneous models for the gamma-ray emission of these systems that include both external and synchrotron self-Compton interactions. We have included effects of interactions between the jet and all external photon fields to which it is exposed: companion star, accretion disk, and hot corona. We make broadband calculations to predict the spectral energy distribution of these objects from radio up to GeV energies. The results and predictions can be tested by present and future gamma-ray instruments like INTEGRAL, AGILE, and GLAST.

Microdoping compensation of microcrystalline silicon obtained by Hot-Wire Chemical Vapour Deposition

Undoped hydrogenated microcrystalline silicon was obtained by hot-wire chemical vapour deposition at different silane-to-hydrogen ratios and low temperature (<300 °C). As well as technological aspects of the deposition process, we report structural, optical and electrical characterizations of the samples that were used as the active layer for preliminary p-i-n solar cells. Raman spectroscopy indicates that changing the hydrogen dilution can vary the crystalline fraction. From electrical measurements an unwanted n-type character is deduced for this undoped material. This effect could be due to a contaminant, probably oxygen, which is also observed in capacitance-voltage measurements on Schottky structures. The negative effect of contaminants on the device was dramatic and a compensated p-i-n structure was also deposited to enhance the cell performance.

Massive protostars as gamma-ray sources.

Massive protostars have associated bipolar outflows with velocities of hundreds of km s-1. Such outflows can produce strong shocks when they interact with the ambient medium leading to regions of nonthermal radio emission. Aims. We aim at exploring under which conditions relativistic particles are accelerated at the terminal shocks of the protostellar jets and whether they can produce significant gamma-ray emission. Methods. We estimate the conditions necessary for particle acceleration up to very high energies and gamma-ray production in the nonthermal hot spots of jets associated with massive protostars embedded in dense molecular clouds. Results. We show that relativistic bremsstrahlung and proton-proton collisions can make molecular clouds with massive young stellar objects detectable by the Fermi satellite at MeV-GeV energies and by Cherenkov telescope arrays in the GeV-TeV range. Conclusions. Gamma-ray astronomy can be used to probe the physical conditions in star-forming regions and particle acceleration processes in the complex environment of massive molecular clouds.

Autoevaluación del aprendizaje en enfermería con ejercicios interactivos del programa Hot Potatoes

Los ejercicios interactivos de autoevaluación son una herramienta muy útil para fomentar el aprendizaje autónomo del estudiante. El programa Hot Potatoes permite el diseño de actividades interactivas para la evaluación formativa, con la incorporación de un sistema de retroacción que refuerza los contenidos no asimilados cuando la respuesta no es correcta. El objetivo de estudio es averiguar la opinión de los estudiantes sobre la utilización del programa Hot Potatoes. Materiales y métodos: Estudio descriptivo transversal en la promoción 2006-2007 de la asignatura Enfermería Maternal II. Los datos se recogieron a través de un cuestionario diseñado ad hoc. Resultados: Los ejercicios mejor valorados y considerados de menor dificultad fueron los de opción múltiple; los más difíciles fueron los textos desordenados y los ejercicios de rellenar huecos. Todos los estudiantes consideraron que el método motivó su interés por la asignatura y facilitó su aprendizaje. El 71% considera que el método le ha servido para adquirir conocimientos y ha sido muy útil como herramienta de estudio. Los aspectos que consideran más interesantes incluyen que: son un método de repaso y estudio, facilitan el aprendizaje de una forma amena y permiten conocer el nivel de conocimientos y corregir los errores durante el aprendizaje. Entre los aspectos que mejorarían destacan que incluirían más ejercicios y un número de preguntas más elevado. Conclusiones: El método ha tenido una buena aceptación y ha fomentado el aprendizaje autónomo. Consideramos que se trata de una estrategia de autoevaluación adecuada para la adaptación a los nuevos créditos europeos (ECTS).

Autoevaluación del aprendizaje en enfermería con ejercicios interactivos del programa Hot Potatoes

Los ejercicios interactivos de autoevaluación son una herramienta muy útil para fomentar el aprendizaje autónomo del estudiante. El programa Hot Potatoes permite el diseño de actividades interactivas para la evaluación formativa, con la incorporación de un sistema de retroacción que refuerza los contenidos no asimilados cuando la respuesta no es correcta. El objetivo de estudio es averiguar la opinión de los estudiantes sobre la utilización del programa Hot Potatoes. Materiales y métodos: Estudio descriptivo transversal en la promoción 2006-2007 de la asignatura Enfermería Maternal II. Los datos se recogieron a través de un cuestionario diseñado ad hoc. Resultados: Los ejercicios mejor valorados y considerados de menor dificultad fueron los de opción múltiple; los más difíciles fueron los textos desordenados y los ejercicios de rellenar huecos. Todos los estudiantes consideraron que el método motivó su interés por la asignatura y facilitó su aprendizaje. El 71% considera que el método le ha servido para adquirir conocimientos y ha sido muy útil como herramienta de estudio. Los aspectos que consideran más interesantes incluyen que: son un método de repaso y estudio, facilitan el aprendizaje de una forma amena y permiten conocer el nivel de conocimientos y corregir los errores durante el aprendizaje. Entre los aspectos que mejorarían destacan que incluirían más ejercicios y un número de preguntas más elevado. Conclusiones: El método ha tenido una buena aceptación y ha fomentado el aprendizaje autónomo. Consideramos que se trata de una estrategia de autoevaluación adecuada para la adaptación a los nuevos créditos europeos (ECTS).

Spiders on a Hot Volcanic Roof: Colonisation Pathways and Phylogeography of the Canary Islands Endemic Trap-Door Spider Titanidiops canariensis (Araneae, Idiopidae)

Studies conducted on volcanic islands have greatly contributed to our current understanding of how organisms diversify. The Canary Islands archipelago, located northwest of the coast of northern Africa, harbours a large number of endemic taxa. Because of their low vagility, mygalomorph spiders are usually absent from oceanic islands. The spider Titanidiops canariensis, which inhabits the easternmost islands of the archipelago, constitutes an exception to this rule. Here, we use a multi-locus approach that combines three mitochondrial and four nuclear genes to investigate the origins and phylogeography of this remarkable trap-door spider. We provide a timeframe for the colonisation of the Canary Islands using two alternative approaches: concatenation and species tree inference in a Bayesian relaxed clock framework. Additionally, we investigate the existence of cryptic species on the islands by means of a Bayesian multi-locus species delimitation method. Our results indicate that T. canariensis colonised the Canary Islands once, most likely during the Miocene, although discrepancies between the timeframes from different approaches make the exact timing uncertain. A complex evolutionary history for the species in the archipelago is revealed, which involves two independent colonisations of Fuerteventura from the ancestral range of T. canariensis in northern Lanzarote and a possible back colonisation of southern Lanzarote. The data further corroborate a previously proposed volcanic refugium, highlighting the impact of the dynamic volcanic history of the island on the phylogeographic patterns of the endemic taxa. T. canariensis includes at least two different species, one inhabiting the Jandia peninsula and central Fuerteventura and one spanning from central Fuerteventura to Lanzarote. Our data suggest that the extant northern African Titanidiops lineages may have expanded to the region after the islands were colonised and, hence, are not the source of colonisation. In addition, T. maroccanus may harbour several cryptic species.

Els Hot Five : Louis Armstrong, l'avantguardista

Els objectius d’aquest treball són: reivindicar la faceta de Louis Armstrong com a músic al capdavant de l’avantguarda musical dels anys vint als Estats Units, analitzar les claus per entendre el seu ascens a la fama a partir dels anys trenta i valorar la seva contribució a la història de la música afroamericana. El cos del treball consta de dues parts: la primera, una biografia de l’artista per esbossar el seu context històric i el seu perfil psicològic; i la segona, que és el centre del treball, una anàlisi de les peces Savoy Blues, Cornet Chop Suey i Gully Low Blues, totes elles pertanyents al període dels Hot Five (1925-1929).