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Speaker Tipo de Evento
Ene 14 2020 - 15:00 NEXT ELUSIVES AND INVISIBLESPLUS WEBINAR: "Filtered Dark Matter: Setting the Dark Matter Abundance Through a First Order Phase Transition" Joachim Kopp Abstract: We discuss the critical role that first order phase transitions in the early Universe may play in the production Webinars
Ene 16 2020 - 12:00 The first ever image of a Black Hole: M87* made visible Antxon Alberdi Colloquium
Ene 20 2020 - 15:00 Do We Understand the Universe? Raul Jimenez Despite the phenomenal progress in our understanding of the laws of nature and the Universe, how much do we really understand at a fundamental level? Seminar
Ene 21 2020 - 11:30 SPLE, 2020 Edition Max and José will present the following papers: SPLE-Club
Ene 21 2020 - 15:00 Post-Newtonian expansions of relativistic symmetries. Patricio Salgado-Rebolledo We introduce an infinite-dimensional space whose isometries are given by an Seminar
Ene 23 2020 - 15:00 Fluxes, Twisted Theory and U(1) symmetries of the Supermembrane Maria Pilar Garcia del Moral In this talk I will discuss some recent results of the Supermembrane worldvolume theory compactified a on a toroidal target space with particular constant flux backgrounds. Seminar
Ene 24 2020 - 11:30 Pheno-Coffee An informal meeting where all the seniors and students are invited to discuss about phenomenology. Pheno-Coffee
Ene 27 2020 - 15:00 Cosmic optics Pierre Fleury As a branch of physical sciences, cosmology is quite peculiar; unlike in condensed-matter physics, quantum chemistry, or molecular biology, cosmology does not allow us to make controlled experiment Seminar
Ene 28 2020 - 11:30 Quantum gravity and matrix models Christian Copetti I wanted to give a rough understanding of what is being done in the context of (quantum) JT gravity and how it connects to older results. HoloClub
Ene 28 2020 - 15:00 NEXT ELUSIVES AND INVISIBLESPLUS WEBINAR: “Probing the Neutrino Mass Mechanism with the CMB” Samuel J. Witte I will present recent work investigating the extent to which the CMB can serve as an indirect probe of neutrino mass models that contain a light neutrino-philic goldstone boson (or bosons). Webinars

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