Disfagia orofaringea sindrome geriatrico en el paciente anciano

El present treball es basa per una banda en una revisió bibliogràfica de la disfàgia orofaríngia en el pacient ancià amb especial èmfasi en el pacient ancià fràgil. Aquest document ha estat dissenyat per a la publicació pròxima com capítol Nº29 del primer tractat de Geriatria en espanyol de l'editorial ELSEVIER organitzat pel Dr Pedro Abizanda Soler. El segon document és un protocol de recerca del meu primer disseny de projecte de tesi doctoral. El projecte ha estat aprovat recentment pel Comitè d´Ètica del nostre centre i ha estat presentat a l'oposició de beques hospitalàries de l'Acadèmia de Ciències Mèdiques de la Filial del Maresme

Sindrome de regresión caudal

El síndrome de regresión caudal o de agenesia sacra se caracteriza por un déficit funcional de los esfínteres y de la muscultatura de los miembros inferiores. Se suele asociar con otras malformaciones, como son las esqueléticas, genitourinarias y del tracto intestinal. La diabetes mellitus materna es uno de los factores predisponentes más destacados. Aquí se presenta un caso de síndrome de regresión caudal con insufiencia renal secundaria a la uropatía malformativa asociada. Se comentan los disrarfismos espinales ocultos y el síndrome de Vater.

OpenURL i l'enllaçat SFX

No fa gaires anys de les primeres recerques acadèmiques liderades per Herbert Van de Sompel a la Universitat de Gant a Bèlgica, les quals van donar com a resultat la formulació de l'estàndard OpenURL i el desenvolupament del servidor d'enllaços per a les biblioteques SFX, posant el control dels enllaços en mans del bibliotecari. Aquest article considera breument les primeres iniciatives sobre els enllaços, explica el propòsit i l'estructura d'OpenURL i el paper dels components: les fonts, els objectius i el servidor d'enllaços, centrant-se en el servidor d'enllaços SFX.

George W. Bush: diseño de un producto político

Treball que tracta d’explicar el procés de creació d’un personatge polític, en el que s’utilitza a George W. Bush com a exemple pràctic per il·lustrar les estratègies implementades pel seu assessor Karl Rove per portar-lo a la Casa Blanca.

Hearing loss in Adult Women with Turner Syndrome

L'objectiu d'aquest estudi és definir els patrons d’hipoacúsia en dones amb Síndrome de Turner i els possibles factors que poden afavorir el desenvolupament d’hipoacúsia neurosensorial en dones adultes amb Síndrome de Turner. Es va trobar que més de la meitat de les dones amb Sindrome de Turner presenten hipoacúsia a l’audiometria, confirmat pels potencials evocats auditius de tronc; la hipoacúsia neurosensorial és el tipus de pèrdua d'audició més freqüent entre dones de mitjana edat amb síndrome de Turner i l'edat, el cariotip i la història prèvia d'otitis mitja recurrent són possibles factors de risc per l’aparició d’hipoacúsia en aquestes pacients.

Noise induced transitions in semiclassical cosmology

A semiclassical cosmological model is considered which consists of a closed Friedmann-Robertson-Walker spacetime in the presence of a cosmological constant, which mimics the effect of an inflaton field, and a massless, non-conformally coupled quantum scalar field. We show that the back-reaction of the quantum field, which consists basically of a nonlocal term due to gravitational particle creation and a noise term induced by the quantum fluctuations of the field, are able to drive the cosmological scale factor over the barrier of the classical potential so that if the universe starts near a zero scale factor (initial singularity), it can make the transition to an exponentially expanding de Sitter phase. We compute the probability of this transition and it turns out to be comparable with the probability that the universe tunnels from ``nothing'' into an inflationary stage in quantum cosmology. This suggests that in the presence of matter fields the back-reaction on the spacetime should not be neglected in quantum cosmology.

Cosmological perturbations from stochastic gravity

In inflationary cosmological models driven by an inflaton field the origin of the primordial inhomogeneities which are responsible for large-scale structure formation are the quantum fluctuations of the inflaton field. These are usually calculated using the standard theory of cosmological perturbations, where both the gravitational and the inflaton fields are linearly perturbed and quantized. The correlation functions for the primordial metric fluctuations and their power spectrum are then computed. Here we introduce an alternative procedure for calculating the metric correlations based on the Einstein-Langevin equation which emerges in the framework of stochastic semiclassical gravity. We show that the correlation functions for the metric perturbations that follow from the Einstein-Langevin formalism coincide with those obtained with the usual quantization procedures when the scalar field perturbations are linearized. This method is explicitly applied to a simple model of chaotic inflation consisting of a Robertson-Walker background, which undergoes a quasi-de Sitter expansion, minimally coupled to a free massive quantum scalar field. The technique based on the Einstein-Langevin equation can, however, deal naturally with the perturbations of the scalar field even beyond the linear approximation, as is actually required in inflationary models which are not driven by an inflaton field, such as Starobinsky¿s trace-anomaly driven inflation or when calculating corrections due to nonlinear quantum effects in the usual inflaton driven models.

Stability of de Sitter spacetime under isotropic perturbations in semiclassical gravity

A spatially flat Robertson-Walker spacetime driven by a cosmological constant is nonconformally coupled to a massless scalar field. The equations of semiclassical gravity are explicitly solved for this case, and a self-consistent de Sitter solution associated with the Bunch-Davies vacuum state is found (the effect of the quantum field is to shift slightly the effective cosmological constant). Furthermore, it is shown that the corrected de Sitter spacetime is stable under spatially isotropic perturbations of the metric and the quantum state. These results are independent of the free renormalization parameters.

Radiative isotropic cosmologies with extra dimensions

We solve Einsteins equations in an n-dimensional vacuum with the simplest ansatz leading to a Friedmann-Robertson-Walker (FRW) four-dimensional space time. We show that the FRW model must be of radiation. For the open models the extra dimensions contract as a result of cosmological evolution. For flat and closed models they contract only when there is one extra dimension.

Particle creation due to cosmological contraction of extra dimensions

Particle production in a cosmological spacetime with extra dimensions is discussed. A five-dimensional cosmological model with a three-dimensional space expanding isotropically like in a radiative Friedmann-Robertson-Walker model and an internal space contracting to a constant small size is considered. The parameters of the model are adjusted so that time variations in internal space are compatible with present limits on time variations of the fundamental constants. By requiring that the energy density of the particles produced be less than the critical density at the radiation era we set restrictions on two more parameters: namely, the initial time of application of the semiclassical approach and the relative sizes between the internal space and the horizon of the ordinary Universe at this time. Whereas the production of massless particles allows a large range of variation to these parameters, the production of massive particles sets severe constraints on them, since, if they are overproduced, their energy density might very soon dominate the Universe and make cosmological dimensional reduction by extradimensional contraction unlikely.

Generalization of the persistent random walk to dimensions greater than 1

We propose a generalization of the persistent random walk for dimensions greater than 1. Based on a cubic lattice, the model is suitable for an arbitrary dimension d. We study the continuum limit and obtain the equation satisfied by the probability density function for the position of the random walker. An exact solution is obtained for the projected motion along an axis. This solution, which is written in terms of the free-space solution of the one-dimensional telegraphers equation, may open a new way to address the problem of light propagation through thin slabs.

Morphological changes in convection-diffusion-limited deposition

The effect of hydrodynamic flow upon diffusion-limited deposition on a line is investigated using a Monte Carlo model. The growth process is governed by the convection and diffusion field. The convective diffusion field is simulated by the biased-random walker resulting from a superimposed drift that represents the convective flow. The development of distinct morphologies is found with varying direction and strength of drift. By introducing a horizontal drift parallel to the deposition plate, the diffusion-limited deposit changes into a single needle inclined to the plate. The width of the needle decreases with increasing strength of drift. The angle between the needle and the plate is about 45° at high flow rate. In the presence of an inclined drift to the plate, the convection-diffusion-limited deposit leads to the formation of a characteristic columnar morphology. In the limiting case where the convection dominates, the deposition process is equivalent to ballistic deposition onto an inclined surface.

Estudio comparativo entre una escala de desarrollo y una prueba basada en la teoría de Piaget, aplicadas a un grupo de niños con síndrome de Down

Este trabajo pretende analizar la similitud entre algunos de los ítems de dos escalas utilizadas en el psicodiignóstico de la primera infancia y construidas a partir de marcos conceptuales divergentes: Brunet-Uzine de estructura psicométrica clásica y Casati-Uzine, adaptación de las pruebas de Piaget. Asimismo deseamos.verificar si ambas escalas proporcionan dliagnósticos equivalentes al aplicarlas a niños con sindrome de Down. El análisis sistemático del contenido de 10s ítems de las dos escalas evidencia una gran similitud de las pautas de conducta que algunos de los items solicitan al niño. El tratamiento estadístic0 de 10s datos indica que para el tipo de niños estudiado la escala Casati-Lézine tiende a acordar edades de desarrollo más altas que la de Brunet-Lézine. La muestra esta compuesta por 18 niños, entre 6 y 24 meses, con sindrome de Down.

"Patron-driven acquisitions": la biblioteca propone y el lector dispone

Reseña de: Esposito, Joseph J.; Walker, Kizer; Ehling, Terry. PDA and the university press. A report prepared for The Andrew W. Mellon Foundation. [Baltimore, Md]: The Johns Hopkins University Press; [Ithaca, N.Y.]: Cornell University Library, Sept. 26th 2012. 65 p. Documento de trabajo disponible en línea en: . [Consulta: 10 de mayo de 2013].

Fauna parasitoide de Phyllonorycter spp. en plantaciones de manzano de Lleida

Se ha estudiado en 1992, 1993 y 1996 la fauna parasitaria de Phyllonorycter corylifoliella (Hübner) y de Phyllonorycter mespilella (Hübner) existente en 4 parcelas de manzano situadas en la zona frutícola de Lleida. La incidencia de estas especies fue baja en todas las parcelas estudiadas. La tasa de parasitismo alcanzó valores del 35% cuando la población larvaria de las minadoras estuvo compuesta fundamentalmente por larvas del cuarto y del quinto estadios. En general, se observó una marcada preferencia por las larvas histófagas y una proporción de sexos siempre favorable a los machos. Básicamente, se encontraron las mismas especies en los distintos años y parcelas, aunque su abundancia relativa fue diferente. Las especies más abundantes y frecuentes fueron Sympiesis gordius Walker, Sympiesis sericeicornis Nees, Sympiesis acalle Walker (Eulophidae) y Pholetesor bicolor (Nees) (Braconidae).