Quantum amplification effect in a horizon fluctuations

TL;DR

This paper investigates quantum amplification effects in black hole horizon fluctuations, revealing how including all emitted photons alters the radiation pattern and enhances understanding of Hawking radiation.

Contribution

It introduces a comprehensive intensity formula accounting for all emitted photons, improving the theoretical modeling of black hole horizon fluctuations.

Findings

Amplification effects cause observable bright flashes in Hawking radiation.

Including all transition weights modifies the predicted radiation pattern.

The new intensity formula provides a more consistent description of black hole emissions.

Abstract

The appearance of a few unevenly- spaced bright flashes of light on top of Hawking radiation is the sign of the amplification effect in black hole horizon fluctuations. Previous studies on this problem suffer from the lack of considering all emitted photons in the theoretical spectroscopy of these fluctuations. In this paper, we include all of the physical transition weights and present a consistent intensity formula. This modifies a black hole radiation pattern.