Small-amplitude nonlinear waves on a black hole background
arXiv:math/0503024
Abstract
Let G(x) be a C^0 function such that |G(x)|\le K|x|^{p} for |x|\le c, for constants K,c>0. We consider spherically symmetric solutions of \Box_gÏ=G(Ï) where g is a Schwarzschild or more generally a Reissner-Nordstrom metric, and such that Ïand \nabla Ïare compactly supported on a complete Cauchy surface. It is proven that for p> 4, such solutions do not blow up in the domain of outer communications, provided the initial data are small. Moreover, |Ï|\le C(\max\{v,1\})^{-1}, where v denotes an Eddington-Finkelstein advanced time coordinate.
24 pages, 8 figures