Abstract
Let G(x) be a C0 function such that G(x) ≤ K x p for x ≤ c, for constants K, c > 0. We consider spherically symmetric solutions of □gφ = G(φ) where g is a Schwarzschild or more generally a Reissner-Nordström metric, and such that φ and ∇φ are 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, φ ≤ C(max{ν, 1})-1, where ν denotes an Eddington-Finkelstein advanced time coordinate.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 1147-1172 |
| Number of pages | 26 |
| Journal | Journal des Mathematiques Pures et Appliquees |
| Volume | 84 |
| Issue number | 9 |
| DOIs | |
| State | Published - Sep 2005 |
All Science Journal Classification (ASJC) codes
- General Mathematics
- Applied Mathematics
Keywords
- Black hole
- Non-linear wave equation
- Reissner-Nordström
- Schwarzschild