Los puntos clave no están disponibles para este artículo en este momento.
Abstract The behaviour, on the Cauchy horizon, of a flux of gravitational and/or electromagnetic radiation crossing the event horizon of a Reissner-Nordström black-hole is investigated as a problem in the theory of one-dimensional potential-scattering. It is shown that the flux of radiation received by an observer crossing the Cauchy horizon, along a radial time-like geodesic, diverges for all physically reasonable perturbations crossing the event horizon, even including those with compact support.
Chandrasekhar et al. (Wed,) studied this question.
Synapse has enriched one closely related paper. Consider it for comparative context: