Abstract
A Vaidya-based model of a radiating black hole is studied in a 5-dimensional Einstein gravity with Gauss-Bonnet contribution of quadratic curvature terms. The structure and locations of the apparent and event horizons of the radiating black hole are determined.
- Received 17 August 2007
DOI:https://doi.org/10.1103/PhysRevD.77.047504
©2008 American Physical Society