structural:summarization, linguistic:translation
GISR mechanism resolution to the paradox

where ω s {\displaystyle \omega {}s} is the index of hawking-particles set with total energy ω {\displaystyle \omega }. In the short time evolution or single quantum emission, Wigner-Wiesskopf approximation allows one to show that the spectrum of GISR is exactly of thermal type and the corresponding temperature equals to that of Hawking radiation. In the long time evolution or continuous quantum emission, the process is off-equilibrium and is characterised by an initial state dependent black hole mass or temperature vs. time curve. The observers far away can retrieve the information stored in the initial black holes from their mass or temperature v.s. time curve.