Centro de Excelencia Severo Ochoa
Menu
Search
Eventos Recientes
| Speaker | Event Type | ||||
|---|---|---|---|---|---|
 | Dec 18 2018 - 15:00 | Dark matter invisible axion and flavors from string GUT | Jihn E. Kim | I discuss the theta rolling during the QCD phase transition which can leadto a useful expression of the axion energy density in terms of the | Seminar |
| Jan 10 2019 - 15:00 | Dark Matter Hurricane | Ciaran O'Hare | The recent releases of data from the Gaia satellite have offered us a transformational view of our galaxy. | Seminar |
| Jan 21 2019 - 15:00 | Testable scenarios for the origin of neutrino masses & baryon asymmetry | J. Lopez Pavon | The simplest extension of the SM that can account for neutrino masses consists in the addition of 2 right-handed neutrinos to the SM field content. | Seminar |
| Jan 24 2019 - 15:00 | What we have learnt, are currently learning and will learn about the Neutrino Sector from nu_e disappearance experiments. | Stephen J. Parke | Neutrinos from reactors and the Sun have provided a great deal of information regarding the Neutrino Sector. | Seminar |
| Jan 28 2019 - 15:00 | Exploring fundamental physics with gravitational waves. | Alfredo Urbano | With the first direct observation of gravitational waves, a new era in astrophysics has begun. | Seminar |
| Jan 31 2019 - 15:00 | Meson interactions at Large Nc from Lattice QCD | Fernando Romero López | The Large Nc limit is often invoked in phenomenological approaches. | Seminar |
| Feb 4 2019 - 15:00 | Beyond the standard QCD axion cosmology | Fabrizio Rompineve | The QCD axion relic abundance is determined by the misalignment mechanism, as well as by the evolution of axionic topological defects, if the Peccei-Quinn (PQ) symmetry is broken after inflation. | Seminar |
| Feb 11 2019 - 15:00 | Circuit complexity for (euclidean) path-integral optimization | Michal Heller | | Seminar |
Pages
Social media