Centro de Excelencia Severo Ochoa
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Speaker | Tipo de Evento | ||||
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Jun 3 2019 - 15:00 | LHC friendly avenues for freeze-in dark matter | José Miguel No | Freeze-in dark matter (DM) production constitutes an appealing mechanism to generate the DM relic density for very weakly coupled DM particles which never achieve thermal equilibrium with the | Seminar | |
Jun 7 2019 - 15:00 | Model independent reconstruction of Stochastic Gravitational Wave Backgrounds at LISA | Mauro Pieroni | In this seminar I discuss the possibility of performing a model independent reconstruction of stochastic gravitational wave backgrounds (SGWB) at LISA. | Seminar | |
Jun 10 2019 - 15:00 | Positivity in the cosmos | Mario Herrero Valea | We study the consequences of positivity of scattering amplitudes in the effective field theory description of Higgs-Dilaton inflation By requiring the EFT to be compatible with a unitar | Seminar | |
Sep 5 2019 - 15:00 | Computing isospin breaking corrections in massive QED on the lattice | Andrea Bussone | I present a preliminary calculation of the leading QED corrections to the hadronic vacuum-polarization (HVP) relevant for the determination of the leptonic anomalous magnetic moments. | Seminar | |
Sep 16 2019 - 11:00 | Irreversibility of the RG flow in quantum field theories with boundaries. | Ignacio Salazar Landea | Seminar | ||
Sep 23 2019 - 15:00 | Electron Hydrodynamics & Black Holes in Anti de Sitter Space-time | Rene Meyer | Recent advances in condensed matter experiments have allowed to synthesize materials in which the electrons flow collectively as a fluid. | Seminar | |
Sep 30 2019 - 15:00 | A New Prospect for Discovering Heavy Neutrinos at the LHC | Richard Efrain Ruiz | Collider processes that violate lepton flavor and lepton number symmetries are a key prediction of realistic, low-scale neutrino mass models. | Seminar | |
Oct 7 2019 - 15:00 | From generalized global symmetries to pulsar magnetospheres | N. Iqbal | Pulsars are thought to be surrounded by strong magnetic fields as well as a high density of charged particles; the resulting zero temperature system is highly nonlinear. | Seminar |
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