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.

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.

"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).

Parasitoides de Cacopsylla pyri (L.) (= Psylla pyri (L.)) presentes en una plantación comercial de peral en Lleida no sometida a tratamientos insecticidas

Se ha seguido la evolución de las poblaciones de parasitoides de Cacopsylla pyri (L.) (= Psylla pyri (L.)) en una parcela comercial de peral de la variedad Blanquilla no sometida a tratamientos con productos insecticidas en Lleida. Se recogieron al azar semanalmente unas 150 ninfas de C. pyri desde abril a noviembre de 1991. Las ninfas fueron llevadas al laboratorio y colocadas en brotes de peral. Las momias fueron individualizadas en tubos de cristal hasta la emergencia del adulto del parasitoide. La especie parasitoide más abundante fue el encírtido Trechnites psyllae (Ruschka) (= Metallon psyllae (Ruschka)). También se encontró un encírtido hiperparasitoide, Aphidencyrtus mamitus (Walker) (= Syrphophagus mamitus Walker). Se observó un 18 % de parasitismo en la primera quincena de mayo sobre ninfas de la primera generación de C. pyri, época del año en la que no han hecho su aparición los depredadores de psylla.

Unidirectional quantum walks: Evolution and exit times

In this paper we focus our attention on a particle that follows a unidirectional quantum walk, an alternative version of the currently widespread discrete-time quantum walk on a line. Here the walker at each time step can either remain in place or move in a fixed direction, e.g., rightward or upward. While both formulations are essentially equivalent, the present approach leads us to consider discrete Fourier transforms, which eventually results in obtaining explicit expressions for the wave functions in terms of finite sums and allows the use of efficient algorithms based on the fast Fourier transform. The wave functions here obtained govern the probability of finding the particle at any given location but determine as well the exit-time probability of the walker from a fixed interval, which is also analyzed.

Cosmological networks

Networks often represent systems that do not have a long history of study in traditional fields of physics; albeit, there are some notable exceptions, such as energy landscapes and quantum gravity. Here, we consider networks that naturally arise in cosmology. Nodes in these networks are stationary observers uniformly distributed in an expanding open Friedmann-Lemaitre-Robertson-Walker universe with any scale factor and two observers are connected if one can causally influence the other. We show that these networks are growing Lorentz-invariant graphs with power-law distributions of node degrees. These networks encode maximum information about the observable universe available to a given observer.

Caminador amb assistència per a persones amb mobilitat reduïda

El projecte consisteix en el disseny d’un caminador per a persones amb mobilitatreduïda. Ens hem centrat en un caminador una mica més evolucionat que els caminadorsactuals, ja que no hi ha cap aparell intermedi entre un caminador i una cadira derodes i en conseqüència moltes persones que podrien caminar si tinguessin unapetita ajuda acaben impossibilitades de ver vida en una cadira de rodes. El majorproblema de dependència d’aquestes persones és el fet d’incorporar-se del llit, sofà,lavabo i per tant el nostre disseny està pensat perquè les persones puguin feraquest pas de manera més senzilla i així augmentar la seva autonomia i autoestima.La nostra solució ha consistit en una estructura més gran que la d’un caminadornormal i que incorpori un cilindre elèctric que ajuda a la persona a aixecar-se i queno hagi de fer-ho totalment sola. Aquest mecanismes també ens serveixen per donar seguretat i evitar possibles caigudes, de manera que la persona que en fa úses pugui sentir més segura de si mateixa