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Speaker Tipo de Evento
Jun 3 2020 - 16:00 HoloSPLE: Nothing is certain in string compactifications Iñaki García Etxebarria, Miguel Montero, Kepa Sousa, Irene Valenzuela A bubble of nothing is a spacetime instability where a compact dimensioncollapses. After nucleation, it expands at the speed of light, leaving “nothing” behind. HoloClub
Jun 5 2020 - 16:00 Cosmic-ray antiproton production and dark matter hints in light of the AMS-02 data Pedro De La Torre Luque Webinars
Jun 9 2020 - 16:00 SL(2,R) lattices and networks as information mirrors and decoders Ayan Mukhopadhyay Quantum black holes past their Page times are unique objects in terms of how they process quantum information. Webinars
Jun 11 2020 - 16:00 Reflected entropy, symmetries and free fermions Pablo Bueno Entanglement entropy (EE) is an intrinsically divergent quantity in quantum field theory (QFT). Webinars
Jun 15 2020 - 16:00 Per aspera ad astra: Impact of high precision standard model predictions for new physics searches Alexander Lenz We review recent progress in increasing the precision of SM flavour observables, like heavy hadron lifetimes or B-mixing. Webinars
Jun 16 2020 - 11:30 The quantum information of a fermion on the torus Ignacio Reyes Concepts from quantum information theory have become increasingly important in our understanding of entanglement in QFTs. HoloClub
Jun 16 2020 - 12:00 Anomalies; String Pheno 2020 retrospective





SPLE-Club
Jun 16 2020 - 15:00 NEXT ELUSIVES WEBINAR: "Unravelling richness of dark sector by FASER$\nu$" Yasaman Farzan FASER$\nu$ is a newly proposed experiment which will take data in run III of the LHC during 2021-2023. Webinars
Jun 16 2020 - 16:00 Holography of the spin current Umut Gürsoy Recent developments both in high and low energy physics have increased the importance of hydrodynamics of matter with correlated spin degrees of freedom. Webinars
Jun 23 2020 - 16:00 Constraining Non-Relativistic RG Flows with Holography Sera Cremonini The basic question of how to organize the degrees of freedom of a quantum system as a function of energy scale has proven very difficult to address in a general context. Webinars

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