Speaker
Lukas Varnhorst
(University of Wuppertal)
Description
We report on the development of a lattice formalism for studying the realtime behaviour of radially symmetric configurations of massless scalar fields in radially symmetric, curved spacetimes in 3+1 dimensions.
It is intended to numerically study back reaction effects due to semiclassical gravity in the time evolution of scalar field configurations, especially for those that will eventually evolve into black holes.
Primary authors
Christian Hoelbling
Jana N. Guenther
(University of Wuppertal)
Lukas Varnhorst
(University of Wuppertal)
