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 : Inhomogeneous Random Systems
The time evolution of the eigenvectors of random matrices is an important problem that appears in different contexts, for example covariance matrices in (possibly time dependent) environments. We will review different recent ideas to separate a genuine evolution of the structure of the matrix from a mere disorder realization effect.