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Curso 2024-2025 Fase 1 de admisión: Del 26 de febrero al 25 de marzo de 2024 . Fase 2 de admisión: Del 13 de junio al 1 de julio de 2024.
Curso 2024-2025 Fase 1 de admisión: Del 26 de febrero al 25 de marzo de 2024 . Fase 2 de admisión: Del 13 de junio al 1 de julio de 2024.
Soundscape of gravitational waves: a new tool to access the fundamental blocks of the Universe Diego Blas is a researcher at UAB (Universidad Autónoma de Barcelona)
How dark matter came to be: Experimental constraints on dark matter production mechanisms Lecturer: David G. Cerdeño, UAM-IFT Abstract: : Despite various decades of ongoing experimental efforts, the nature of
SKA: the mother of all radio telescopes Miguel Á. Pérez Torres is a research scientist at the Instituto de Astrofísica de Andalucía
QCD axions as dark matter and their potential detection by gravitational microlensing Jordi Miralda Escudé es ICREA Professor of Astrophysics Institut de Ciències del Cosmos Abstract:The most distant single stars
Lecturer: Farida Fassi, Mohammed V University in Rabat, Faculty of Sciences. Morocco Abstract: The Large Hadron Collider (LHC) at CERN, the largest and most complex machine ever built will extend
Antoine Kouchner , Laboratoire Astroparticule et Cosmologie (APC) Paris, is the ANTARES experiment spokesperson Abstract: Messengers of the infinitely small, neutrinos provide us with valuable insights into the fundamental laws
Lecturer: Andrés del Pino Molina. Centro de Estudios de Física del Cosmos de Aragón (CEFCA). Astrophysics researcher with a strong computational and statistic background. Interested in resolved stellar populations, galaxies
Artwork by KM3NeT with Sandbox Studio, Chicago
Georg G. Raffelt, Max-Planck-Institut für Physik. His research is in the areas of theoretical astroparticle physics and cosmology. In particular, it revolves around weakly interacting particles (neutrinos, the hypothetical axion,