Centro de Excelencia Severo Ochoa
Menú
Buscar
Speaker | Tipo de Evento | ||||
---|---|---|---|---|---|
Nov 12 2019 - 15:00 | Strong first-order phase transitions: Vorticity, droplets and gravitational waves | Daniel Cutting | Although in the Standard Model the electroweak phase transition is a crossover, many well-motivated extensions can generate a first-order phase transition at the electroweak scale. | Seminar | |
Nov 14 2019 - 15:00 | Instability of the Luttinger liquids towards a fractal phase | Huan-Qiang Zhou | A novel universality class is found to characterize quantum phase transitions arising from instability of a Luttinger liquid to a quantum state of matter with highly degenerate ground states | Seminar | |
Nov 18 2019 - 15:00 | Inconsistency of an inflationary sector coupled only (minimally) to gravity | Daniel Figueroa | The inflationary sector might very well have no direct couplings to other species, apart from inevitable gravitational interactions. | Seminar | |
Nov 19 2019 - 15:00 | Black holes with Sol horizon | Federico Faedo | Many are the ways to evade the topology theorems concerning black holes' horizon; in this | Seminar | |
Nov 21 2019 - 15:00 | Chiral Metric Hydrodynamics, Kelvin Circulation Theorem, and the Fractional Quantum Hall Effect | Dam Thanh Son | By extending the Poisson algebra of ideal hydrodynamics to include a two-index tensor field, we construct a new (2+1)-dimensional hydrodynamic theory that we call "chiral metric hydrodynamics." The | Seminar | |
Nov 25 2019 - 15:00 | Neutrino Oscillations in Dark Matter | Eung Jin Chun | We discuss neutrino oscillations in a medium of dark matter which generalizes the standard matter effect. | Seminar | |
Nov 26 2019 - 15:00 | Cosmology in the Machine Learning Era | Francisco Villaescusa-Navarro | The standard model of cosmology is a theoretical framework that accurately describes a large variety of cosmological observables, from the temperature anisotropies of the cosmic microwave backgroun | Seminar | |
Nov 28 2019 - 15:00 | The Dark Matter distribution of the Milky Way | Fabio Iocco | The distribution of Dark Matter in galaxies is one remarkable output ofstructure formation in a cosmological context, and an important input for | Seminar |
Social media