46:41
publiée le 22 juin 2026
GRMHD Simulations of Spinning Supermassive Black Hole Binaries: Gas Dynamics and Observational Signatures
De Manuela Campanelli
Apparaît dans la collection : 2024 - PC1 - WS - Curved spacetimes, field theory and beyond
My talk will focus on the recent resolution of the Kerr stability conjecture for the particular case of slowly rotating Kerr black holes.