Null singularities in general relativity

13 January 2014
Jonathan Luk
We consider spacetimes arising from perturbations of the interior of Kerr black holes. These spacetimes have a null boundary in the future such that the metric extends continuously beyond. However, the Christoffel symbols may fail to be square integrable in a neighborhood of any point on the boundary. This is joint work with M. Dafermos
  • Partial Differential Equations Seminar