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In the language of black hole physics, Hawking radiation is one of the mostcontroversial subjects about which there exist lots of puzzles, including theinformation loss problem and the question of whether this radiation is thermalor not. In this situation, a possible way to face these problems is to bringquantum effects into play, also taking into account self-gravitational effectsin the scenario. We consider a quantum-corrected form of the Schwarzschildblack hole inspired by the pioneering work of Kazakov and Solodukhin to modifythe famous Parikh-Wilczek tunneling process for Hawking radiation. We provethat in this framework the radiation is not thermal, with a correlationfunction more effective than the Parikh-Wilczek result, and the informationloss problem can be addressed more successfully. Also, we realize that quantumcorrection affects things in the same way as an electric charge. So, it seemsthat quantum correction in this framework has something to do with the electriccharge.

A quantum-corrected approach to black hole radiation via a tunneling process