In　this　paper,　we　generalize　the　Parikh-Wilczek　scheme　to　a　holographic　screen　in　the　framework　of　the　ultraviolet　self-complete　quantum　gravity.　We　calculate　that　the　tunneling　probability　depends　on　the　energy　of　the　particle　and　the　mass　of　the　holographic　screen.　The　radiating　temperature　has　not　been　the　standard　Hawking　temperature.