As astrophysicists, we are used to extracting physical information from the observations. The usual procedure is to propose a parametric physical model to...
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TalkBuried in the noise.
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TalkComputación cuántica: física-matemática o matemática-física.
En una parte preliminar se recordarán unos pocos hechos experimentales obtenidos durante las últimas décadas, con énfasis en fenómenos puramente cuánticos como...
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TalkCurso de partículas
Programa del curso: 1.- Introduction 2.- Electromagnetic Interaction (QED) 3.- Strong Interaction (QCD) 4.- Electroweak Interaction 5.- Precision Tests 6.- CP...
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TalkCurso de partículas
Programa del curso: 1.- Introduction 2.- Electromagnetic Interaction (QED) 3.- Strong Interaction (QCD) 4.- Electroweak Interaction 5.- Precision Tests 6.- CP...
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TalkCurso de partículas
Las clases se impartirán en el aula los días 4, 5 y 6 de noviembre de 2008 en horario de 10:30 a 12:30 Programa del curso: 1.- Introduction 2.- Electromagnetic...
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TalkDALI, a pioneering dark matter telescope
Axion detection would be one of the most exciting moments in the entire history of science. This hypothetical particle can simultaneously explain two...
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TalkDiscerning the location of the gamma-ray emission region in AGN blazars from multi-messenger and multi-spectral-range observations
Relativistic jets in AGN in general, and in blazars in particular, are the most energetic and among the most powerful astrophysical objects known so far. Their...
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TalkElectron densities in HII regions across galaxy discs
When we measure the electron density within an H II region using ratios of emission lines we find characteristic values in the range of 100-300 cm -3. But when...
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TalkExtragalactic background light and its implications for galaxy evolution and gamma-ray astronomy
The extragalactic background light (EBL) is of fundamental importance both for understanding the entire process of galaxy evolution and for gamma-ray astronomy...