Black hole tunneling in loop quantum gravity

TL;DR

This paper explores Hawking radiation from loop quantum gravity-corrected black holes using tunneling methods, revealing quantum corrections to entropy and emission rates.

Contribution

It introduces quantum gravity corrections to black hole entropy and radiation, extending traditional Hawking radiation analysis within the loop quantum gravity framework.

Findings

Quantum correction terms modify emission rates.

Black hole entropy includes a logarithmic correction.

Results align with established quantum gravity predictions.

Abstract

In this paper, we investigate the Hawking radiation of the quantum Oppenheimer- Snyde black hole with the tunneling scheme by Parikh and Wilczek. We calculate the emission rate of massless scalar particles. Compared to the traditional results within the framework of General Relativity, our findings include quantum correction terms arising from loop quantum gravity effects. Following the approach in [1, 2], we establish the entropy of the black hole. This entropy includes a logarithmic correction, which arises from quantum gravity effects. Our result is consistent with the well-known result in the context of quantum gravity.