Speaker
Dr
Zhiwei Wang
Description
We show that the apparent horizon and the region near r=0 of an evaporating charged, rotating black hole are timelike. It then follows that for black holes in nature, which invariably have some rotation, have a channel, via which classical or quantum information can escape to the outside, while the black hole shrinks in size. We discuss implications for the information loss problem.
Primary author
Dr
Zhiwei Wang
Co-authors
Prof.
Samuel Braunstein
(University of York)
Prof.
Saurya Das
(University of Lethbridge)
