Centro de Excelencia Severo Ochoa
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Eventos Recientes
June 6, 2023
June 1, 2023
| Speaker | Event Type | ||||
|---|---|---|---|---|---|
 | Mar 23 2023 - 15:00 | Digital quantum simulation of higher-charge Schwinger model with topological term | Masazumi Honda | I am going to talk about application of quantum computation to numerical simulation of quantum field theory. | Seminar |
| Mar 27 2023 - 15:00 | The impact of model realism on interpretations of the Galactic Center Excess | Christopher Eckner | More than a decade has passed since a GeV gamma-ray excess in Fermi-LAT data above known astrophysical backgrounds has been detected in | Seminar |
| Mar 30 2023 - 15:00 | Axion couplings in Grand Unified Theories | Mario Reig | In this talk (based on 2206.07053) I discuss axion couplings to gauge bosons in Grand Unified Theories, where the Standard Model is embedded in a simple 4D gauge group. | Seminar |
 | Apr 13 2023 - 11:00 | Machine code of holography | Umut Gürsoy | Gauge-gravity duality plays a key role in understanding quantum gravity and strongly interacting gauge theories, however, lacks a satisfactory microscopic derivation. | Seminar |
 | Apr 13 2023 - 15:00 | Probing new neutrino interactions via light gauge boson mediators in proto-neutron stars | Marina Cermeño | Neutrinos are copiously produced in the interior of proto-neutron stars and crucial in their evolution, therefore making these compact objects ideal sites to test new neutrino interactions. | Seminar |
 | Apr 17 2023 - 15:00 | Hunting for axions: Shining light through (cosmic) walls | Manuel Meyer | Axions and axion-like particles are hypothetical particles that could explain the cold dark matter as well as the non-observation of an | Seminar |
 | Apr 19 2023 - 15:30 | Holographic baryonic matter without flavor branes | Carlos Hoyos | In holographic models flavor is usually realized by introducing additional branes in a dual supergravity background. | Seminar |
 | Apr 24 2023 - 15:00 | Beyond one scalar doublet | Per Osland | I will briefly review the shortcomings of the 2HDMs in terms of providing a new source of CP violation (desired for baryogenesis), as well as a Dark Matter candidate, before discussing how this is | Seminar |
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