. "Particle Physics"@en . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . "Classical electrodynamics"@en . . "6" . "Specific Competition\nCE6 - Understand the structure of matter being able to solve problems related to the interaction between matter and radiation in different energy ranges\nCE11 - Know how to use current astrophysical instrumentation (both in terrestrial and space observatories) especially that which uses the most innovative technology and know the fundamentals of the technology used\nGeneral Competencies\nCG1 - Know the advanced mathematical and numerical techniques that allow the application of Physics and Astrophysics to the solution of complex problems using simple models\nCG3 - Analyze a problem, study the possible published solutions and propose new solutions or lines of attack\nBasic skills\nCB6 - Possess and understand knowledge that provides a basis or opportunity to be original in the development and/or application of ideas, often in a research context\nCB7 - That students know how to apply the knowledge acquired and their ability to solve problems in new or little-known environments within broader contexts\nCB10 - That students possess the learning skills that allow them to continue studying in a way that will be largely self-directed or autonomous\nExclusive to the Structure of Matter Specialty\nCX13 - Understand in depth the basic theories that explain the structure of matter and collisions as well as the state of matter in extreme conditions\n6. Subject contents\nTheoretical and practical contents of the subject\n- Professor: Vicente Daniel Rodríguez Armas\n- Topics (headings):\n1. Electromagnetic response of material means. Constitution Relations. Response function, causality, dispersion, complex permittivity, Kramers-Kronig relations. Experimental determination of permittivity.\n2. Classical treatment of the radiation-matter interaction. Classical Lorentz models, plasma frequency. Comparison with results of quantum treatment, interband and intraband electronic transitions.\n3. Plasmas and metals. Plasmas, Lorentz Model. Optical properties of metals. Drude model. Doped semiconductors. Plasma Oscillations, Plasmons.\n4. Semiconductors and insulators. Fundamental absorption edge in direct gap materials. Direct transitions with energies higher than the gap. Fundamental absorption edge in indirect gap materials." . . "Presential"@en . "FALSE" . . "Master in Astrophysics"@en . . "https://www.ull.es/en/masters/astrophysics/" . "90"^^ . "Presential"@en . "The exceptional atmospheric conditions for top-quality astronomic observation to be found in the Canary Islands, together with its geographic proximity and excellent connections with Europe, justify the presence here of the European Northern Hemisphere Observatory (ENO). This fact, along with the consequent concentration of teachers and researchers around the Canary Island Institute of Astrophysics, the ULL Department of Astrophysics and the Observatories, generates the ideal atmosphere for a Master in Astrophysics in which direct contact with leading professionals represents exceptional value added. The Master has been designed based on an ample and rigorous choice of subjects, options and itineraries that that take the form of three specialities: “Theory and Computing Speciality”, “Observation and Instrumentation Speciality” and “Material Structure”\n\nGeneral skills\nKnow the advanced mathematical and numerical techniques that allow Physics and Astrophysics to be applied to solving complex problems using simple models\nUnderstand the technologies associated with observation in Astrophysics and the design of instrumentation\nAnalyse a problem, study the possible solutions published and propose new solutions or lines of attack\nAssess orders of magnitude and develop a clear perception of physically different situations that show analogies allowing the use of synergies and known solutions for new problems\nSpecific skills\nUnderstand the basic conceptual schemes of Astrophysics\nUnderstand the structure and evolution of the stars\nUnderstand the mechanisms of nucleosynthesis\nUnderstand the structure and evolution of galaxies\nUnderstand the models of the origin and evolution of the Universe\nUnderstand the structure of matter to be able to solve problems related to the interaction between matter and radiation in different energy ranges\nKnow how to find solutions to specific astrophysical problems on your own, using specific bibliography with minimum supervision\nKnow how to work independently on new research projects\nKnow how to programme, at least in one important language for scientific calculation in Astrophysics\nUnderstand the instrumentation used to observe the universe in the different frequency ranges\nUse current scientific instrumentation (both Earth-based and Space-based) and have a command of their innovative technologies\nKnow how to use current astrophysical instrumentation (both in terrestrial and space observatories), especially the instrumentation that uses the most innovative technology and know the foundations of the technology used\nApply the knowledge acquired to undertake an original research work in Astrophysics"@en . . . "1.5"@en . "FALSE" . . . "Master"@en . "Thesis" . "Not informative" . "no data"@en . "Not informative" . "None" . "no data"@en . "no data" . "FALSE" . "Upstream"@en . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .