Hawking radiation from the holographic screen

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 probabilities of the massless and massive particles depend on their energies of the particles and the mass of the holographic screen. The radiating temperature has not been the standard Hawking temperature. On the contrary, the quantum unitarity principle always remains.