arXiv · hep-th/9502115
Hawking Radiation and Energy Conservation in an Evaporating Black Hole
Abstract
We define the Bondi energy for two-dimensional dilatonic gravity theories by generalizing the known expression of the ADM energy. We show that our definition of the Bondi energy is exactly the ADM energy minus the radiation energy at null infinity. An explicit calculation is done for the evaporating black hole in the RST model with the Strominger's ghost decoupling term. It is shown that the infalling matter energy is completely recovered through the Hawking radiation and the thunderpop.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Won T. Kim, Julian Lee. 1995-02-18. Hawking Radiation and Energy Conservation in an Evaporating Black Hole. https://doi.org/10.1103/physrevd.52.2232
Cite the original work for its findings. Save a collection to share your selection of sources.