Speaker
Michael Good
(Nazarbayev University)
Description
Constructing an exact correspondence between a black hole model and a particular moving mirror trajectory, we investigate a new model that preserves unitarity. The Bogolubov coefficients in 1+1 dimensions are computed analytically. The key modification limits the origin of coordinates (moving mirror) to sub-light asymptotic speed. Effective continuity across the metric ensures that there is no information loss. The black hole emits thermal radiation and the total evaporation energy emitted is finite without invoking the conservation of energy.
Author
Michael Good
(Nazarbayev University)
