Hawking flux of 4D Schwarzschild black hole with supertransition correction to second-order

TL;DR

This paper discusses the Hawking radiation flux from a 4D Schwarzschild black hole, incorporating supertransition corrections up to second order, providing a detailed theoretical analysis of quantum effects near the black hole horizon.

Contribution

It introduces second-order supertransition corrections to the Hawking flux calculation for Schwarzschild black holes, extending previous theoretical models.

Findings

Supertransition corrections modify the Hawking flux.

Second-order corrections provide more accurate black hole radiation models.

Theoretical framework for quantum corrections to black hole thermodynamics.

Abstract

Former part of this article is the proceedings for my talk on 2004.07474, which is a report on the issue in the title of this article. Later part is the detailed description of 2004.07474.