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Linear stability of the Schwarzschild black hole under electromagnetic and gravitational perturbations

URN to cite this document:
urn:nbn:de:bvb:355-epub-5810
DOI to cite this document:
10.5283/epub.581
Finster, Felix ; Smoller, Joel
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Date of publication of this fulltext: 05 Aug 2009 13:23


Abstract

We prove that the Schwarzschild black hole is linearly stable under electromagnetic and gravitational perturbations. Our method is to show that for spin s = 1 or s = 2, solutions of the Teukolsky equation with smooth, compactly supported initial data
outside the event horizon, decay in L1
loc.


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