Controlled rippling of graphene via irradiation and applied strain modify its mechanical properties: a nanoindentation simulation study

Ripples, present in free standing graphene, have an important influence in the mechanical behavior of this two-dimensional material. In this work we show through nanoindentation simulations, how out-of-plane displacements can be modified by strain resulting in softening of the membrane under compression and stiffening under tension. Irradiation also induces changes in the mechanical properties of graphene. Interestingly, compressed samples, irradiated at low doses are stiffened by the irradiation while samples under tensile strain do not show significant changes in their mechanical properties. These simulations indicate that vacancies, produced by the energetic ions, cannot be the ones directly responsible for this behavior. However, changes in roughness induced by the momentum transferred from the energetic ions to the membrane, can explain these differences. These results provide an alternative explanation to recent experimental observations of stiffening of graphene under low dose irradiation, as well as paths to tailor the mechanical properties of this material via applied strain and irradiation.

Blazed Gratings Recorded in Absorbent Photopolymers

Phase diffractive optical elements, which have many interesting applications, are usually fabricated using a photoresist. In this paper, they were made using a hybrid optic-digital system and a photopolymer as recording medium. We analyzed the characteristics of the input and recording light and then simulated the generation of blazed gratings with different spatial periods in different types of photopolymers using a diffusion model. Finally, we analyzed the output and diffraction efficiencies of the 0 and 1st order so as to compare the simulated values with those measured experimentally. We evaluated the effects of index matching in a standard PVA/AA photopolymer, and in a variation of Biophotopol, a more biocompatible photopolymer. Diffraction efficiencies near 70%, for a wavelength of 633 nm, were achieved for periods longer than 300 µm in this kind of materials.

Are pulsars born with a hidden magnetic field?

The observation of several neutron stars in the centre of supernova remnants and with significantly lower values of the dipolar magnetic field than the average radio-pulsar population has motivated a lively debate about their formation and origin, with controversial interpretations. A possible explanation requires the slow rotation of the protoneutron star at birth, which is unable to amplify its magnetic field to typical pulsar levels. An alternative possibility, the hidden magnetic field scenario, considers the accretion of the fallback of the supernova debris on to the neutron star as responsible for the submergence (or screening) of the field and its apparently low value. In this paper, we study under which conditions the magnetic field of a neutron star can be buried into the crust due to an accreting, conducting fluid. For this purpose, we consider a spherically symmetric calculation in general relativity to estimate the balance between the incoming accretion flow and the magnetosphere. Our study analyses several models with different specific entropy, composition, and neutron star masses. The main conclusion of our work is that typical magnetic fields of a few times 1012 G can be buried by accreting only 10−3–10−2 M⊙, a relatively modest amount of mass. In view of this result, the central compact object scenario should not be considered unusual, and we predict that anomalously weak magnetic fields should be common in very young (< few kyr) neutron stars.

Measuring the stellar wind parameters in IGR J17544-2619 and Vela X-1 constrains the accretion physics in supergiant fast X-ray transient and classical supergiant X-ray binaries

Context. Classical supergiant X-ray binaries (SGXBs) and supergiant fast X-ray transients (SFXTs) are two types of high-mass X-ray binaries (HMXBs) that present similar donors but, at the same time, show very different behavior in the X-rays. The reason for this dichotomy of wind-fed HMXBs is still a matter of debate. Among the several explanations that have been proposed, some of them invoke specific stellar wind properties of the donor stars. Only dedicated empiric analysis of the donors’ stellar wind can provide the required information to accomplish an adequate test of these theories. However, such analyses are scarce. Aims. To close this gap, we perform a comparative analysis of the optical companion in two important systems: IGR J17544-2619 (SFXT) and Vela X-1 (SGXB). We analyze the spectra of each star in detail and derive their stellar and wind properties. As a next step, we compare the wind parameters, giving us an excellent chance of recognizing key differences between donor winds in SFXTs and SGXBs. Methods. We use archival infrared, optical and ultraviolet observations, and analyze them with the non-local thermodynamic equilibrium (NLTE) Potsdam Wolf-Rayet model atmosphere code. We derive the physical properties of the stars and their stellar winds, accounting for the influence of X-rays on the stellar winds. Results. We find that the stellar parameters derived from the analysis generally agree well with the spectral types of the two donors: O9I (IGR J17544-2619) and B0.5Iae (Vela X-1). The distance to the sources have been revised and also agree well with the estimations already available in the literature. In IGR J17544-2619 we are able to narrow the uncertainty to d = 3.0 ± 0.2 kpc. From the stellar radius of the donor and its X-ray behavior, the eccentricity of IGR J17544-2619 is constrained to e< 0.25. The derived chemical abundances point to certain mixing during the lifetime of the donors. An important difference between the stellar winds of the two stars is their terminal velocities (ν∞ = 1500 km s-1 in IGR J17544-2619 and ν∞ = 700 km s-1 in Vela X-1), which have important consequences on the X-ray luminosity of these sources. Conclusions. The donors of IGR J17544-2619 and Vela X-1 have similar spectral types as well as similar parameters that physically characterize them and their spectra. In addition, the orbital parameters of the systems are similar too, with a nearly circular orbit and short orbital period. However, they show moderate differences in their stellar wind velocity and the spin period of their neutron star which has a strong impact on the X-ray luminosity of the sources. This specific combination of wind speed and pulsar spin favors an accretion regime with a persistently high luminosity in Vela X-1, while it favors an inhibiting accretion mechanism in IGR J17544-2619. Our study demonstrates that the relative wind velocity is critical in class determination for the HMXBs hosting a supergiant donor, given that it may shift the accretion mechanism from direct accretion to propeller regimes when combined with other parameters.

Topological spin waves in the atomic-scale magnetic skyrmion crystal

We study the spin waves of the triangular skyrmion crystal that emerges in a two-dimensional spin lattice model as a result of the competition between Heisenberg exchange, Dzyalonshinkii–Moriya interactions, Zeeman coupling and uniaxial anisotropy. The calculated spin wave bands have a finite Berry curvature that, in some cases, leads to non-zero Chern numbers, making this system topologically distinct from conventional magnonic systems. We compute the edge spin-waves, expected from the bulk-boundary correspondence principle, and show that they are chiral, which makes them immune to elastic backscattering. Our results illustrate how topological phases can occur in self-generated emergent superlattices at the mesoscale.

Organic distributed feedback laser to monitor solvent extraction upon thermal annealing in solution-processed polymer films

Solution-processed polymer films are used in multiple technological applications. The presence of residual solvent in the film, as a consequence of the preparation method, affects the material properties, so films are typically subjected to post-deposition thermal annealing treatments aiming at its elimination. Monitoring the amount of solvent eliminated as a function of the annealing parameters is important to design a proper treatment to ensure complete solvent elimination, crucial to obtain reproducible and stable material properties and therefore, device performance. Here we demonstrate, for the first time to our knowledge, the use of an organic distributed feedback (DFB) laser to monitor with high precision the amount of solvent extracted from a spin-coated polymer film as a function of the thermal annealing time. The polymer film of interest, polystyrene in the present work, is doped with a small amount of a laser dye as to constitute the active layer of the laser device and deposited over a reusable DFB resonator. It is shown that solvent elimination translates into shifts in the DFB laser wavelength, as a consequence of changes in film thickness and refractive index. The proposed method is expected to be applicable to other types of annealing treatments, polymer-solvent combinations or film deposition methods, thus constituting a valuable tool to accurately control the quality and reproducibility of solution-processed polymer thin films.

Realistic limits for subpixel movement detection

Object tracking with subpixel accuracy is of fundamental importance in many fields since it provides optimal performance at relatively low cost. Although there are many theoretical proposals that lead to resolution increments of several orders of magnitude, in practice this resolution is limited by the imaging systems. In this paper we propose and demonstrate through simple numerical models a realistic limit for subpixel accuracy. The final result is that maximum achievable resolution enhancement is connected with the dynamic range of the image, i.e., the detection limit is 1/2∧(nr.bits). The results here presented may aid in proper design of superresolution experiments in microscopy, surveillance, defense, and other fields.

Development and programming of Geophonino: A low cost Arduino-based seismic recorder for vertical geophones

The commercial data acquisition systems used for seismic exploration are usually expensive equipment. In this work, a low cost data acquisition system (Geophonino) has been developed for recording seismic signals from a vertical geophone. The signal goes first through an instrumentation amplifier, INA155, which is suitable for low amplitude signals like the seismic noise, and an anti-aliasing filter based on the MAX7404 switched-capacitor filter. After that, the amplified and filtered signal is digitized and processed by Arduino Due and registered in an SD memory card. Geophonino is configured for continuous registering, where the sampling frequency, the amplitude gain and the registering time are user-defined. The complete prototype is an open source and open hardware system. It has been tested by comparing the registered signals with the ones obtained through different commercial data recording systems and different kind of geophones. The obtained results show good correlation between the tested measurements, presenting Geophonino as a low-cost alternative system for seismic data recording.

Iluminando a las investigadoras en el Año Internacional de la Luz

El año 2015 fue declarado por las Naciones Unidas como el Año Internacional de la Luz y de las Tecnologías basadas en la luz. Varias personas pertenecientes al Grupo Especializado de Mujeres en Física de la Real Sociedad Española de Física (RSEF) y a la Sociedad Española de Óptica (SEDOPTICA) nos organizamos para llevar a cabo distintas actividades con objeto de visibilizar a algunas investigadoras que han realizado su labor científica en estos campos y cuyas contribuciones son poco o nada conocidas. Animadas por dos de los objetivos de la declaración del año 2015 como el Año Internacional de la Luz y de las Tecnologías basadas en la Luz, a saber: “promocionar el empoderamiento de la mujer en la Ciencia” y “fomentar vocaciones científicas en el ámbito de la luz y de sus aplicaciones”, surgió nuestra motivación. Indudablemente dando visibilidad a la labor de estas científicas y valorando sus aportaciones en el avance de las tecnologías ópticas y fotónicas de nuestra sociedad crearemos referentes para las futuras generaciones y, sobre todo, para las jóvenes estudiantes, contribuyendo a la consecución de la igualdad efectiva entre mujeres y hombres.

Seguimiento del Grado en Geología (Facultad de Ciencias, UA)

La red de trabajo formada por los profesores coordinadores de semestre y de titulación del Grado en Geología (Facultad de Ciencias, Universidad de Alicante) ha tenido como objetivos principales: afianzar la implementación de las enseñanzas conforme al contenido del plan de estudios del título verificado; elaborar planes de mejora para solventar las posibles deficiencias detectadas y colaborar con los instrumentos del Sistema de Garantía Interno de Calidad (SGIC) del centro en la elaboración de los informes de autoevaluación del título. El método de trabajo se basa en reuniones en las que los miembros de la red plantearán y debatirán los parámetros e indicadores de seguimiento de la red, en la que cada investigador (coordinador) aporta una investigación individualizada del semestre del que es responsable. Ante la inminente acreditación del título el próximo curso, buena parte de las tareas se han enfocado a colaborar en los informes de auto-evaluación del título y en los planes de mejora.

Coordinación y seguimiento del grado en ingeniería en sonido e imagen en telecomunicación para la acreditación

La red docente ha realizado durante el curso 2014/15 un proyecto para la recopilación de las evidencias para la acreditación en la ANECA del Grado en Ingeniería en Sonido e Imagen en Telecomunicación de la Escuela Politécnica Superior. Nos centramos en los criterios 8 y 9 de Acredita plus. Se relacionan las competencias del título y las competencias ENAEE. Cada competencia ENAEE se desarrolla por un grupo de asignaturas con una dedicación determinada de créditos. El informe de acreditación plus en el que se ha trabajado es para la obtención del sello EUR-ACE.

Análisis de resultados de las asignaturas de primer curso en la implantación del máster de Ingeniería de Caminos, Canales y Puertos en la EPS de la UA

La puesta en funcionamiento del Primer Curso del Máster de Ingeniería de Caminos, Canales y Puertos en la Universidad de Alicante ha supuesto un reto de adaptación y modificación de los criterios que se venían empleando desde la entrada en vigor del Plan de Estudios de Ingeniería de Caminos, Canales y Puertos en el año 2005. Para ello, se ha partido de la información que se remitió en su momento para su aprobación a la Agencia Nacional de Acreditación (ANECA), implementando y aplicando todos aquellos parámetros que se definieron ex profeso en su momento, de forma que el alumnado pudiera adquirir los conocimientos y competencias asociadas a cada una de las asignaturas en las que ha recibido docencia en este primer curso de implantación del Máster de Ingeniería de Caminos, Canales y Puertos (MICCP) en la Universidad de Alicante. En ningún caso debe olvidarse que la entrada en vigor de este máster mantiene reservas profesionales (según Orden CIN 309/2009) [1] para los egresados de la titulación, obligando a que la totalidad de departamentos y docentes implicados en su desarrollo, implementaran criterios específicos relacionados con los sistemas de evaluación, enseñanza y planificación de la materia a impartir, si bien debe indicarse que, a tenor de los resultados obtenidos en las distintas asignaturas de este primer curso, no han sido todo los eficaces que en un primer momento pudieran esperarse.

Seguimiento y plan de mejora en el Máster Universitario en Ingeniería de Telecomunicación: Criterios, evidencias y resultados

En este trabajo se plantea estudiar los criterios, organizar las evidencias y recopilar los resultados que permiten desarrollar el auto-informe para la acreditación título en la ANECA de Máster Universitario en Ingeniería de Telecomunicación de la Universidad de Alicante. Por ello, la red de investigación en docencia universitaria planteada implica a todas las asignaturas de estos estudios, incluido el Trabajo Fin de Máster. Para alcanzar los objetivos se comienza por la recopilación detallada de los criterios para el desarrollo del auto-informe y la documentación a cumplimentar. En la organización de las evidencias relacionadas con cada uno de los criterios a evaluar, generadas en cada curso de implantación del título, el trabajo se ha centrado en el criterio 6 (Resultados del aprendizaje) y el criterio 7 (Indicadores de satisfacción). Las tablas comparativas elaboradas, donde se resumen los resultados del aprendizaje, facilitan la puesta en común y la concreción de un plan de mejora.

Red de coordinación y seguimiento de trabajos fin de máster en la titulación Máster en Prevención de Riesgos Laborales

El profesorado de la red participó durante el curso 2014/15 un proyecto para la coordinación y seguimiento de la asignatura trabajo fin de máster en la titulación Máster en Prevención de Riesgos Laborales. Este Máster comenzó a impartirse en la Escuela Politécnica Superior de la Universidad de Alicante en el curso 2012/13, por ello el desarrollo de la titulación en su tercera edición hace necesario el seguimiento de las asignaturas como instrumento para la coordinación y mejora de la calidad docente. En este sentido la red ha resultado ser un instrumento útil para la interacción y coordinación entre los tutores/as de los trabajos fin de máster propuestos en la titulación.

Um retrato do marginal brasileiro mediante o trabalho do ator com as personagens de Plínio Marcos em “Navalha na carne"

This thesis presented is to research the actor's work in the construction of physical actions, according to the methodology developed by Constantin Stanislavski in his analysis of dramatic action, called "method of physical action", applied to questions of scenic representation of the Brazilian marginal, according to the look "cruel" and realistic / naturalistic Plinio Marcos playwright. Based on the circumstances given by Pliniano universe, the intention is to contribute to the reflection on the actor's work on the scene with the marginal characters in "Razor in the Flesh", highlighting some important aspects, to assist in the construction of this fictional world. You want to create conditions for the formation of an actor that leverages the scene the contradictions and conflicts of this work. The research aims from the theoretical and practical study as a methodological hypothesis, producing critical reflection from the creative process of the agent with the realization of a scenic experiment focused on psychophysical technique of this Russian pedagogue. Thus, we intend to have a look at the method of physical actions focusing on his last great contribution to the work, especially the procedure of active analysis by doing a reading from "Razor in the Flesh" through this creative scenic exercise, extending the studies concerning the actor's art. This research is a general explanation about the trajectory of Stanislavski to his encounter with the physical action, while, highlights the inconsistencies of understanding of his work around the world. Stanislavski initially developed the "method" having as a backdrop, the realist aesthetic - a dialogue relationship between reality and the scene - through a style which creates a theatrical reality, and consequently, artistic, not literally naturalistic way through an integral mimicry. That is, the representation of work in realistic theater aesthetics should be developed in order to create a theatrical reality. Stanislavski believes that theater is convention, since the actor's work on himself should encourage this second nature, scenic.