Smooth null hypersurfaces near the horizon in the presence of tails [PDF]
Carlos Kozameh, Osvaldo Moreschi, Alejandro PerezWe show that the power-law decay modes found in linear perturbations of Schwarzschild black holes, generally called tails, do not produce caustics on a naturally defined family of null surfaces in the neighborhood of i+ of a black hole horizon.View original: http://arxiv.org/abs/1207.4702
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