On the Mathematical Theory of Black Holes (3/4)
by Prof. Sergiu Klainerman (Princeton University & IHES)
at IHES ( Centre de conférences Marilyn et James Simons )
The gravitational waves detected by LIGO were produced in the final faze of the inward spiraling of two black holes before they collided to produce a more massive black hole. The experiment is entirely consistent with the so called Final State Conjecture of General Relativity according to which generic solutions of the Einstein vacuum equations can be described, asymptotically, by a finite number of Kerr solutions moving away from each other. Though the conjecture is so very easy to formulate and happens to be validated by both astrophysical observations as well as numerical experiments, it is far beyond our current mathematical understanding. In fact even the far simpler and fundamental question of the stability of one Kerr black hole remains wide open.
|Organisé par||Emmanuel Ullmo|