Phase Space Analysis on some Black Hole Manifolds
arXiv:math/0511281 · doi:10.1016/j.jfa.2008.10.004
Abstract
The Schwarzschild and Reissner-Nordstrom solutions to Einstein's equations describe space- times which contain spherically symmetric black holes. We consider solutions to the linear wave equation in the exterior of a fixed black hole space- time of this type. We show that for solutions with initial data which decay at infinite, a weighted norm in space decays like . This weight vanishes at the event horizon, but not at infinite.
63 pages (correction to Morawetz multiplier- 14 August 2006)
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Cited by in corpus (39)
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- Characterisation of the Energy of Gaussian Beams on Lorentzian Manifolds - with Applications to Black Hole Spacetimes
- Uniform energy bound and Morawetz estimate for extreme components of spin fields in the exterior of a slowly rotating Kerr black hole II: linearized gravity
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