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Speaker Tipo de Evento
Feb 10 2020 - 16:30 Future Collider Network Workshop Workshop
Feb 11 2020 - 15:00 NEXT ELUSIVES AND INVISIBLESPLUS WEBINAR: "Neutrino masses from gravity" Jessica M. Turner In this talk I will discuss neutrino masses in general and demonstrate that non-zero neutrino masses can be generated from gravitational interactions. In this work we  solve the Schwin Webinars
Feb 12 2020 - 11:30 Entanglement Islands Martin Sasieta During this last year, there have been several "semiclassical" derivations of the Page curve for an evaporating black hole in AdS. HoloClub
Feb 17 2020 - 15:00 Non-metallic ground states from holography: features and observables. Alexander Krikun I will discuss the features of holographic models in case when the breaking of translations is relevant in the IR and the horizon geometry is not metallic. Seminar
Feb 18 2020 - 11:30 SPLE club: Separating the Bounds Alvaro and Pierre will present the following papers:
SPLE-Club
Feb 19 2020 - 15:00 QGI Webinar Juan Maldacena We will review the gravitational formula for fine grained entropy. We will discuss how it applies to an evaporating black hole and how we can compute the entropy of Hawking radiation.
Webinars
Feb 20 2020 - 15:00 New physics in rare decays Toshihiko Ota After two decades of the great discoveries, neutrino physics is now entering the era of precision measurements with massive detectors. Seminar
Feb 25 2020 - 11:30 Boomerang RG flows Gabriel Larios Abstract: HoloClub
Feb 27 2020 - 15:00 Validity of the EFT approach to LHC processes with wide range of energies probed. The Same-Sign WW case Pawel Kozow Vector boson scatterings are fundamental processes to shed light on the nature of the electroweak symmetry breaking mechanism. Seminar
Mar 2 2020 - 15:00 From agnostic to believer: model independent reconstruction of non standard cosmological models and the role of theoretical priors. Matteo Martinelli Upcoming Large Scale Structure surveys will provide information on the distribution of matter in the Universe which, united with Cosmic Microwave Background data from Planck, has the potential to s Seminar

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