基本説明
Establishes the precise mathematical framework in which linearization stability of Einstein equation with matter makes sense, and once this is achieved, to find conditions for this type of stability when a Robertson-Walker model for the universe is considered.
Full Description
, 3 2 2 R ? /?x K i i g V T G g ?T , ? 2 2 2 2 ? 2 2 2 2 2 c ?t ?x ?x ?x 1 2 3 S T S T? ˜ T S 2 2 2 2 ? 2 2 2 2 2 c ?t ?x ?x ?x 1 2 3 g h h ?? g T T g vacuum M n R n R Acknowledgements n R Chapter I Pseudo-Riemannian Manifolds I.1 Connections M C n X M C M F M C X M F M connection covariant derivative M ? Y X +X X X 1 2 1 2 ? Y X 1 2 X 1 X 2 ?
