Hawking radiation from the holographic screen

TL;DR

This paper extends the Parikh-Wilczek tunneling model to holographic screens within self-complete quantum gravity, revealing modified radiation temperatures that uphold quantum unitarity.

Contribution

It introduces a generalized tunneling framework for holographic screens, showing deviations from standard Hawking temperature while maintaining unitarity.

Findings

Tunneling probabilities depend on particle energy and holographic screen mass.

Radiation temperature differs from Hawking temperature.

Quantum unitarity is preserved in the generalized model.

Abstract

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.