This book is devoted to the Einstein's field equations of general
relativity for self-gravitating massive scalar fields. We formulate
the initial value problem when the initial data set is a
perturbation of an asymptotically flat, spacelike hypersurface in
Minkowski spacetime. We then establish the existence of an Einstein
development associated with this initial data set, which is proven
to be an asymptotically flat and future geodesically complete
spacetime.
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