On the stability of expanding black hole cosmologies [1]
星期四, 2 三月, 2017 - 11:15
Prénom de l'orateur:
Volker
Nom de l'orateur:
Schlue
Résumé :
In general relativity, the Kerr de Sitter spacetimes are a model of a black hole in an expanding universe. I will describe its geometry, and some of my current work on the propagation of gravitational waves in the expanding region of black hole cosmologies.
Thème du groupe de travail:
GT Relativité Générale
Institution:
Paris 6
Salle:
Salle 1, Tour IRMA