46:41
publiée le 22 juin 2026
GRMHD Simulations of Spinning Supermassive Black Hole Binaries: Gas Dynamics and Observational Signatures
De Manuela Campanelli
On attempts and progresses towards proving the de Sitter no hair theorem using mean curvature flow
Apparaît dans la collection : 2024 - PC1 - WS - Curved spacetimes, field theory and beyond
I will review how mean curvature flow is providing progress towards proving the so-called de Sitter no-hair theorem, concerning the onset of a de Sitter phase of the universe out of inhomogenous initial conditions. This is relevant for the initial condition of Inflation in our universe.
