Orateur
Natalia Pinzani-Fokeeva
(Florence University)
Description
A local symmetry is required to formulate fluid dynamics from a modern effective-field-theory perspective. Black hole horizons possess the same redundancy. In this talk, I will show how asymptotic symmetries of horizons can be interpreted as symmetries of a dual hydrodynamic theory in the context of holography. I will also show how the horizon structure implies additional symmetries and how these symmetries lead to chaotic behavior in the dual theory.
