17 resultados para Nuclear matter
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134 p.
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7 p.
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[EN]This paper undertakes the study of the occurrence of non-corresponding demonstrative forms in Spanish, Basque and English in exactly the same linguistic context. It is proposed that the differenccs in the choice of the demonstratives result from the differences in the kind of iniormation that must be coded in each of the languages. Thus, I will argue that in Spanish and Basque the obligatory coding of the aspectual categories of the imperfect and the preterit has the function of imposing specific viewing arrangements onto the situations they designate. By contrast, in English, where the aspectual distinction is not overtly coded, the demonstrativcs are proposed to fulfil this function.
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9 p. : il.
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Introducción: La medición de la concentración de hierro hepática (CHH) por RM es una técnica no invasiva de gran utilidad en el diagnóstico de los pacientes con sospecha de sobrecarga férrica en hígado. Objetivo:Validar la eficacia de la RM 1 Tesla en la determinación de la (CHH) en pacientes con sospecha de sobrecarga férrica. Validar su capacidad para diagnosticar o descartar la presencia de una CHH sugestiva de hemocromatosis. Pacientes y métodos:Estudio observacional, transversal, con inclusión prospectiva de pacientes consecutivos. De 2002 a 2010 hemos obtenido la CHH estimada mediante RM 1 Tesla (método Gandon) y de RM 1,5 Tesla (método Alústiza), y mediante BH, en 56 pacientes consecutivos (58RM:35/23). Resultados:Grupo RM 1 Tesla: de acuerdo con CHH en BH, 15 pacientes clasificados como normales (<36µmol/g)-la RM valoró correctamente 7; sobreestimó 8-; 15 grupo hemosiderosis (36-80 µmol/g)-RM valoró correctamente 5, sobreestimó 10-; 5 grupo hemocromatosis (>80 µmol/g)-valoró correctamente las 5-. Existió una correlación entre la determinación de la CHH por BH y RM 1 Tesla con r=0.619. Existieron diferencias estadísticamente significativas (p<0.05) entre CHH media por biopsia (53.43/DE45.67/IC95%37.74 a 69.12) y por RM 1 Tesla (76.14/DE47.31/IC95% 60.46 a 92.97), con sobrevaloración por parte de la RM. Grupo RM 1,5 Tesla: de acuerdo con CHH en BH, normal en 14, hemosiderosis en 6 y hemocromatosis en 3. La RM valoró correctamente 6 y sobreestimó 8 en grupo normal; grupo hemosiderosis, 3 correctamente, 3 sobrevalorados; grupo hemocromatosis, valoró correctamente los 3. La correlación entre CHH por BH y RM 1,5 Tesla fue de r=0.815. La CHH media obtenida por BH (69,34/DE152.1/IC95% 3.57 a 135.1 ) y RM 1,5 Tesla (70.43/DE 57.63/IC95% 45.51 a 95.36) no demostraron diferencias significativas (p>0.05). Conclusiones: La determinación de CHH por RM 1 Tesla (método Gandon) es útil para diagnosticar o descartar hemocromatosis y para diagnosticar CHH normal. Existe una importante tendencia a la sobreestimación en pacientes sin y con sobrecarga férrica en la CHH obtenida por RM 1 Tesla. La determinación de CHH por RM 1,5 Tesla (método Alústiza) es superior a la de RM 1 Tesla, aunque también existe una tendencia a sobreestimar. La CHH media obtenida por BH o RM 1,5 Tesla no tuvieron diferencias significativas. En cambio si existieron entre BH y RM 1 Tesla.
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4 p.
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18 p.
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[ES]Este trabajo surge de la inquietud del alumno sobre la energía nuclear y mas concretamente sobre la energía de fusión. Esta inquietud se plasma en una recopilación de información sobre los combustibles necesarios , su abundancia y su forma de obtención actual. Analizaremos la posibilidad de implantar alguna de estas plantas de combustible en el País Vasco, junto con un estudio de una posible central nuclear de fusión con la suma de la potencia de cada uno de los reactores de fisión que se encuentran actualmente en funcionamiento en el estado Español. Compararemos las cantidades de combustible necesarias en un año de uranio y el combustible de fusión, así como el coste de construcción de cada una.
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[EN] This study analyzes the relationship between board size and economic-financial performance in a sample of European firms that constitute the EUROSTOXX50 Index. Based on previous literature, resource dependency and agency theories, and considering regulation developed by the OECD and European Union on the normative of corporate governance for each country in the sample, the authors propose the hypotheses of both positive linear and quadratic relationships between the researched parameters. Using ROA as a benchmark of financial performance and the number of members of the board as measurement of the board size, two OLS estimations are performed. To confirm the robustness of the results the empirical study is tested with two other similar financial ratios, ROE and Tobin s Q. Due to the absence of significant results, an additional factor, firm size, is employed in order to check if it affects firm performance. Delving further into the nature of this relationship, it is revealed that there exists a strong and negative relation between firm size and financial performance. Consequently, it can be asseverated that the generic recommendation one size fits all cannot be applied in this case; which conforms to the Recommendations of the European Union that dissuade using generic models for all countries.
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120 p.
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EN]This is a document done to try to see the effect of a nuclear power plant accident. In particular, it studies what would be the radiation doses delivered to the people in the close areas around the power plant of Garoña, if it had suffered from a loss of coolant accident during its normal functioning.
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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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In the present study we have investigated the population genetic structure of albacore (Thunnus alalunga, Bonnaterre 1788) and assessed the loss of genetic diversity, likely due to overfishing, of albacore population in the North Atlantic Ocean. For this purpose, 1,331 individuals from 26 worldwide locations were analyzed by genotyping 75 novel nuclear SNPs. Our results indicated the existence of four genetically homogeneous populations delimited within the Mediterranean Sea, the Atlantic Ocean, the Indian Ocean and the Pacific Ocean. Current definition of stocks allows the sustainable management of albacore since no stock includes more than one genetic entity. In addition, short-and long-term effective population sizes were estimated for the North Atlantic Ocean albacore population, and results showed no historical decline for this population. Therefore, the genetic diversity and, consequently, the adaptive potential of this population have not been significantly affected by overfishing.
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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.