Speaker
Mr
James Cook
(King's College London)
Description
In Khronometric theory we break Lorentz invariance by introducing a preferred time direction, and hence, equipping our spacetime manifold with a foliation of space-like surfaces. Our primary tool to solve the equations of motion is such a spacetime is Numerical General Relativity (NGR). We investigate how we can use this tool, to solve the equations of motion for a blackhole solution in Khronometric Theory.
Primary author
Mr
James Cook
(King's College London)
