11 resultados para UNIVERSE

em Archivo Digital para la Docencia y la Investigación - Repositorio Institucional de la Universidad del País Vasco


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En las últimas décadas la cosmología ha experimentado notables avances como consecuencia del desarrollo de nuevos experimentos que nos han abastecido con precisos datos observacionales. La calidad de estos datos ha permitido construir una imagen global del universo actual; un universo acelerado compuesto principalmente por materia oscura (23%) distinta a la materia ordinaria (5%), y energía oscura (70%), la componente del universo que contrarresta el efecto gravitatorio y explica la expansión acelerada de éste. Con la existencia de estas dos principales componentes se puede explicar la situación actual del universo y los fenómenos que tienen lugar en él. Sin embargo, su naturaleza es todavía un misterio, por lo que nos encontramos ante un largo y apasionante camino que recorrer.Es en este contexto donde se enmarca el trabajo presentado en esta tesis, cuyo principal objetivo es ir más allá y obtener algunas pistas nuevas sobre la naturaleza de la energía oscura. Las investigaciones llevadas a cabo durante esta tesis tratan de hacer frente a este sector ¿oscuro" desde varias perspectivas, combinando la teoría y el análisis de datos astronómicos.Como primer acercamiento, en el capítulo 2 se propone un nuevo modelo para unificar el sector ¿oscuro¿: materia y energía oscura. En los capítulos 3 y 4 se aborda el problema de la energía oscura desde una nueva perspectiva y se presentan unas nuevas parametrizaciones de la ecuación de estado de la energía oscura. Por último, en el capítulo 5, a través de los datos del fondo cósmico de microondas, se da un paso más allá en física de las épocas tempranas del universo, y se obtienen restricciones sobre el exceso de densidad de radiación observado. Por otra parte, se da una explicación a este fenómeno: se atribuye este exceso al fondo cósmico de ondas gravitacionales primordiales producido por las cuerdas cósmicas, bajo condiciones adiabáticas.

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The territory of the European Union is made up of a rich and wide-ranging universe of languages, which is not circumscribed to the «State languages». The existence of multilingualism is one of Europe’s defining characteristics and it should remain so in the constantly evolving model of Europe’s political structure. Nonetheless, until now, the official use of languages has been limited to the «State languages» and has been based on a concept of state monolingualism that has led to a first level of hierarchization among the languages of Europe. This has affected the very concept of European language diversity. The draft of the treaty establishing a European Constitution contains various language-related references that can be grouped in two major categories: on the one hand, those references having to do the constitutional status of languages, and on the other, those regarding the recognition of European language diversity. Both issues are dealt with in this article. In analyzing the legal regime governing languages set forth in the draft of the constitutional treaty, we note that the draft is not based on the concept of the official status of languages. The language regulation contained in the draft of the constitutional treaty is limited in character. The constitutional language regime is based on the concept of Constitutional languages but the official status of languages is not governed by this rule. The European Constitution merely enunciates rights governing language use for European citizens vis-à-vis the languages of the Constitution and refers the regulation of the official status of languages to the Council, which is empowered to set and modify that status by unanimous decision. Because of its broad scope, this constitutes a regulatory reservation. In the final phase of the negotiation process a second level of constitutional recognition of languages would be introduced, linked to those that are official languages in the member states (Catalan, Basque, Galician, etc.). These languages, however, would be excluded from the right to petition; they would constitute a tertium genus, an intermediate category between the lan guages benefiting from the language rights recognized under the Constitution and those other languages for which no status is recognized in the European institutional context. The legal functionality of this second, intermediate category will depend on the development of standards, i.e., it will depend on the entrée provided such languages in future reforms of the institutional language regime. In a later section, the article reflects on European Union language policy with regard to regional or minority languages, concluding that the Union has not acted in accordance with defined language policy guidelines when it has been confronted, in the exercise of its powers, with regional or minority languages (or domestic legislation having to do with language demands). The Court of Justice has endeavoured to resolve on a case by case basis the conflicts raised between community freedoms and the normative measures that protect languages. Thus, using case law, the Court has set certain language boundaries for community freedoms. The article concludes by reflecting on the legal scope of the recognition of European language diversity referred to in Article II-82 of the European Constitution and the possible measures to implement the precept that might constitute the definition of a true European language policy on regional or minority languages. Such a policy has yet to be defined.

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[EN] Kerstin Hensel’s literary universe is haunted by fallen heroes, outsiders and gregarious figures with no success. They experience the German Wende in a very peculiar constellation, they perceive Post-Unification Germany at times from a fantastic perspective, always from a painful experience. In this context the analysis of the representations of the body in Hensel’s narrative before and after 1989 offers a rich insight on Hensel’s critical view of Post-Unification Germany. By analysing her texts such as Hallimasch and Lärchenau this article shows that the suffering grotesque bodies in both works stand for a political metaphor of a social body with hardly a cure.

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[ES] En este artículo analizaremos el devenir del universo de mujeres de Gioconda Belli, a través de la mirada de tres personajes protagonistas femeninos que se pronuncian de forma contundente sobre la vida y la estética literaria de la autora. Partiremos del análisis de Lavinia, protagonista femenina de La mujer habitada (1988) la primera novela de la autora, a continuación analizaremos el perfil de Sofia protagonista de Sofía de los presagios (1990), su segunda novela. Y por último, escudriñaremos las características de un personaje femenino que propone una nueva lectura de la mítica Juana de Castilla, protagonista de El Pergamino de la seducción (2005). Las tres figuras femeninas literarias nacen de sus propias experiencias simultaneadas por la memoria, compañera inseparable en el afianzamiento del yo y son heroínas de su propia historia

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In this work we investigate if a small fraction of quarks and gluons, which escaped hadronization and survived as a uniformly spread perfect fluid, can play the role of both dark matter and dark energy. This fluid, as developed in [1], is characterized by two main parameters: beta, related to the amount of quarks and gluons which act as dark matter; and gamma, acting as the cosmological constant. We explore the feasibility of this model at cosmological scales using data from type Ia Supernovae (SNeIa), Long Gamma-Ray Bursts (LGRB) and direct observational Hubble data. We find that: (i) in general, beta cannot be constrained by SNeIa data nor by LGRB or H(z) data; (ii) gamma can be constrained quite well by all three data sets, contributing with approximate to 78% to the energy matter content; (iii) when a strong prior on (only) baryonic matter is assumed, the two parameters of the model are constrained successfully. (C) 2014 The Authors. Published by Elsevier B.V.

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Spanish Relativity Meeting (ERE 2014) Valencia, SPAIN, SEP 01-05, 2014

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We construct an F(R) gravity theory corresponding to the Weyl invariant two scalar field theory. We investigate whether such F (R) gravity can have the antigravity regions where the Weyl curvature invariant does not diverge at the Big Bang and Big Crunch singularities. It is revealed that the divergence cannot be evaded completely but can be much milder than that in the original Weyl invariant two scalar field theory. (C) 2014 The Authors. Published by Elsevier B.V.

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[ES] La astrología grecorromana es un código lingüístico con signos (planetas, signos del Zodíaco), y con leyes de interconexión entre ellos (eclíptica, aspectos, casas, límites), y ha de ser valorada no sólo desde la perspectiva de su cientificidad, sino desde la de sus funciones para el individuo y la sociedad: es un conocimiento del futuro singular que afecta a la totalidad de lo implicado, y en la totalidad de sus dimensiones. Suple así el conocimiento de la ciencia antigua, que no fue capaz de incluir ni lo futuro ni lo singular. La astrología integra al individuo en la comunidad, integrándolo previamente en su universo semántico. Cosmos, mundo humano y mundo natural se armonizan totalmente.

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Galaxies are clusters of millions and billions of stars dynamically stable, with gas, dust and dark matter. They are the biggest isolated objects known in the Universe . Even though they are very complex systems, today we have a clear knowledge about their evolution and about their physical phenomena. Aside from the stellar component there is a gaseous component, principally neutral Hydrogen (HI), and dust that, although is not a significant component in terms of the mass, plays an important role on the absorption phenomena. Finally, cinematic and other kind of observations suggest the existence of a spheric dark matter halo, dominant in terms of mass and more extensive than the barionic component.

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[ES] El presente trabajo tiene como objeto el estudio de la eficiencia y persistencia de los rendimientos del total de fondos de inversión inmobiliaria españoles, desde el inicio de su actividad a finales de 1994 a agosto de 2012. Para este propósito se ha utilizado el alfa de Jensen, la ratio de Sharpe, y la aproximación propuesta por Carhart (1997). En cuanto a la eficiencia, la ratio de Sharpe presenta valores negativos en los tres primeros años de actividad de cada fondo y valores muy bajos o incluso negativos en los tres o cuatro últimos años. El indicador de Jensen muestra que la mayoría de los fondos presentan un rendimiento inferior al del mercado, aproximado mediante la rentabilidad de la vivienda y una media de la rentabilidad de todos los fondos inmobiliarios. Carteras de referencia vinculadas a los mercados de deuda o bolsa, no resultan significativas. En el análisis de la persistencia de los rendimientos se confirma su existencia a plazo de uno, dos, tres y cuatro años, para todos los fondos. La evidencia obtenida en nuestro trabajo para los fondos inmobiliarios en España, eficiencia inferior a la del mercado y persistencia en los rendimientos, nos permite confirmar la difícil situación que ha atravesado y en la que sigue inmersa este tipo de inversión colectiva, poniendo de manifiesto la necesidad y la urgencia de medidas impulsoras de su actividad.

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We review the appropriateness of using SNIa observations to detect potential signatures of anisotropic expansion in the Universe. We focus on Union2 and SNLS3 SNIa datasets and use the hemispherical comparison method to detect possible anisotropic features. Unlike some previous works where nondiagonal elements of the covariance matrix were neglected, we use the full covariance matrix of the SNIa data, thus obtaining more realistic and not underestimated errors. As a matter of fact, the significance of previously claimed detections of a preferred direction in the Union2 dataset completely disappears once we include the effects of using the full covariance matrix. Moreover, we also find that such apreferred direction is aligned with the orthogonal direction of the SDSS observational plane and this suggests a clear indication that the SDSS subsample of the Union2 dataset introduces a significant bias, making the detected preferred direction unphysical. We thus find that current SNIa surveys are inappropriate to test anisotropic features due to their highly non-homogeneous angular distribution in the sky. In addition, after removal of the highest in homogeneous sub-samples, the number of SNIa is too low. Finally, we take advantage of the particular distribution of SNLS SNIa sub- sample in the SNLS3 data set, in which the observations were taken along four different directions. We fit each direction independently and find consistent results at the 1 sigma level. Although the likelihoods peak at relatively different values of Omega(m), the low number of data along each direction gives rise to large errors so that the likelihoods are sufficiently broad as to overlap within 1 sigma. (C) 2014 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY license (http:// creativecommons. org/licenses/by/4.0/).