Actividades

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Speaker Tipo de Evento
Abr 18 2018 - 11:00 Hadronic tau decays and the strong coupling Maarten Golterman I will discuss our recent determination of the strong coupling from hadronic tau decays, as measured by ALEPH and OPAL.   This determination is controversial, because the rather low tau mass makes Seminar
Abr 18 2018 - 11:30 (A)dS is a mess ERC-SPLE organizes a bi-weekly journal club, the SPLE-club, in which IFT members and visitors interested in string model building and related topics gather to discuss recent papers, new results, an SPLE-Club
Abr 19 2018 - 15:00 Flavor physics in lattice QCD as a window into BSM physics: |Vcb| and the B -> D* l nu semileptonic decay Alejandro Vaquero Flavor physics provides a rich variety of phenomena that can be used to probe the SM without requiring the high energies present only in particle accelerators. Seminar
Abr 20 2018 - 11:30 Pheno-Coffee An informal meeting where all the seniors and students are invited to discuss about phenomenology. Pheno-Coffee
Abr 23 2018 - 15:00 Losing the IR: A New Framework for Holographic Area Laws Netta Engelhardt I will describe a new procedure for coarse-graining over the gravitational degrees of freedom inside a surface in the context of AdS/CFT. Seminar
Abr 24 2018 - 11:30 Holoclub Christian Copetti We continue the discussion of the bulk factorization in AdS-CFT with more toy model examples. HoloClub
Abr 24 2018 - 15:00 Searching for Dark Matter at the Cosmic Dawn​ J. B. Muñoz The nature of the dark matter is still a mystery, although current and upcoming 21-cm measurements during the cosmic dawn can provide a new arena on the search for the cosmological dark matter. Webinars
Abr 25 2018 - 12:00 PhD Forum Diego Medrano & Javier Alonso Testable ALP in the Minimal Linear Sigma Model (Javier Alonso) Seminar
Abr 25 2018 - 15:00 How clouds shape climate, and climate change Bjoern Stevens Paco Yndurain Colloquium
Abr 26 2018 - 15:00 New insights on the cosmic strings stochastic gravitational wave background Christophe Ringeval In less than two years, GW detections have confirmed the omnipresence of black holes in the Universe and have shed lights on the origin of short Seminar

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