Abstract
Using the late-time expansion we calculate the leading-order coefficients describing the evolution of a massless scalar field inside a Reissner-Nordström black hole. These coefficients may be interpreted as the reflection and transmission coefficients for scalar-field modes propagating from the event horizon to the Cauchy horizon. Our results agree with those obtained previously by Gursel et al. by a different method.
- Received 15 August 1997
DOI:https://doi.org/10.1103/PhysRevD.57.2621
©1998 American Physical Society