Centro de Excelencia Severo Ochoa
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Eventos Recientes
| Speaker | Event Type | ||||
|---|---|---|---|---|---|
 | Apr 15 2024 - 15:00 | Pros and cons of EFTs for new physics | Duarte Fontes | Physics beyond the Standard Model (BSM) can be described in a consistent and general way through an Effective Field Theory (EFT). | Seminar |
 | Apr 18 2024 - 15:00 | Higgs criticality in and beyond the Standard Model | Thomas Steingasser | Both parameters in the Higgs potential appear fine-tuned, relating to the hierarchy problem and the metastability of the electroweak vacuum. | Seminar |
 | Apr 22 2024 - 15:00 | Quantum complexity in the Krylov basis | Pawel Caputa | I will talk about the notion of Krylov complexity, its various recent applications and connections to quantum many-body systems and QCD. | Seminar |
| Apr 25 2024 - 15:00 | Vector Boson Scattering: Status and Prospects for the Large Hadron Collider and Beyond | Richard Ruiz | The scattering of electroweak bosons at TeV-scale super colliders is a powerful mechanism that prob | Seminar |
| Apr 29 2024 - 15:00 | Phenomenological consequences of the modern S-matrix Bootstrap programme | Joan Elias Miró | In this talk I will cover some of the recent successes of the S-matrix bootstrap. I will show how simple ideas of causality and unitarity lead to non-trivial bound on the space of EFTs. | Seminar |
 | May 6 2024 - 15:00 | Black Hole Binary Dynamics and Radiation from Classical and Quantum Gravitational Scattering | Thibault Damour | Gravitational wave signals from coalescing binary black holes are detected, and analyzed, by using large banks of template waveforms. The construction of these templates makes an essential use of t | Seminar |
| May 9 2024 - 15:00 | Distinguishing models with $\mu\to e$ observables | Marco Ardu | Neutrino masses and oscillations demonstrate that lepton flavour violation is new physics that must exist, but it is yet to be observed in processes involving char | Seminar |
| May 16 2024 - 15:00 | Probing new physics with Galactic (keV-MeV) gamma-ray emission | Pedro de la Torre Luque | Measurements of the 511 keV emission reveal the presence of a steady injection of positrons that is very concentrated around the Galactic bulge, and whose origin remains unknown. | Seminar |
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