  In the language of black hole physics, Hawking radiation is one of the most
controversial subjects about which there exist lots of puzzles, including the
information loss problem and the question of whether this radiation is thermal
or not. In this situation, a possible way to face these problems is to bring
quantum effects into play, also taking into account self-gravitational effects
in the scenario. We consider a quantum-corrected form of the Schwarzschild
black hole inspired by the pioneering work of Kazakov and Solodukhin to modify
the famous Parikh-Wilczek tunneling process for Hawking radiation. We prove
that in this framework the radiation is not thermal, with a correlation
function more effective than the Parikh-Wilczek result, and the information
loss problem can be addressed more successfully. Also, we realize that quantum
correction affects things in the same way as an electric charge. So, it seems
that quantum correction in this framework has something to do with the electric
charge.
