Exotic Spinorial Structure and Black Holes in General Relativity

TL;DR

This paper investigates the relationship between exotic spinorial structures and black holes in general relativity, analyzing their effects on Hawking radiation and proposing methods to infer exotic terms from emission rates.

Contribution

It introduces a novel link between exotic spinors and black holes, and explores how exotic terms influence Hawking radiation emission in asymptotically flat solutions.

Findings

Exotic spinorial structures are linked to the presence of black holes.

Exotic terms can significantly affect Hawking radiation emission rates.

Emission rate extremum conditions can help infer exotic contributions.

Abstract

We explore different (and complementary) views of spinors and their exotic counterparts, linking the very existence of the later to the presence of black holes. Moreover, we investigate the effects of the exotic term in the Hawking radiation emission rate, as well as its extremes, for asymptotically flat black holes solutions of general relativity. We show that, under certain circumstances, the emission rate extreme condition fixates an equation from which the exotic term could be inferred.