Abstract
In completely local settings, we establish that a spherically symmetric, dynamically evolving black hole horizon can be assigned a Hawking temperature under a mild assumption. Moreover, we calculate the Hawking flux and show that the radius of the horizon shrinks in accordance with the amount of emitted flux.
- Received 8 May 2012
DOI:https://doi.org/10.1103/PhysRevD.87.084051
© 2013 American Physical Society