Hawking radiation from rotating brane black holes

TL;DR

This paper reviews the methods and key features of Hawking radiation emitted by rotating brane black holes, focusing on particle fluxes and spectra relevant for LHC black hole event simulations.

Contribution

It provides a comprehensive overview of calculating particle, energy, and angular momentum fluxes from rotating brane black holes, highlighting spectral changes with extra dimensions and rotation.

Findings

Spectral features vary with extra dimensions and angular velocity.

Methodology for calculating quantum field emissions on the brane.

Insights useful for simulating black hole events at the LHC.

Abstract

We review recent work on the Hawking radiation of rotating brane black holes, as may be produced at the LHC. We outline the methodology for calculating the fluxes of particles, energy and angular momentum by spin-0, spin-1/2 and spin-1 quantum fields on the brane. We briefly review some of the key features of the emission, in particular the changes in the spectra as the number of extra dimensions or the angular velocity of the black hole increases. These quantities will be useful for accurate simulations of black hole events at the LHC.