Trapped surfaces as boundaries for the constraint equations
General Relativity and Quantum Cosmology
2009-11-10 v2
Abstract
Trapped surfaces are studied as inner boundary for the Einstein vacuum constraint equations. The trapped surface condition can be written as a non linear boundary condition for these equations. Under appropriate assumptions, we prove existence and uniqueness of solutions in the exterior region for this boundary value problem. We also discuss the relevance of this result for the study of black holes collisions.
Cite
@article{arxiv.gr-qc/0308009,
title = {Trapped surfaces as boundaries for the constraint equations},
author = {Sergio Dain},
journal= {arXiv preprint arXiv:gr-qc/0308009},
year = {2009}
}
Comments
26 pages, 2 figures references updated, minor corrections