The End of a Black Hole's Evaporation -- Part II

TL;DR

This paper derives an explicit transition amplitude from black to white hole horizons at the end of Hawking evaporation using covariant loop quantum gravity, providing insights into black hole final states.

Contribution

It introduces a novel explicit expression for black-white hole transition amplitude within covariant loop quantum gravity.

Findings

Explicit transition amplitude derived for black-white hole transition.

Provides a quantum gravity framework for black hole end states.

Advances understanding of black hole evaporation endpoints.

Abstract

We derive an explicit expression for the transition amplitude from black to white hole horizon at the end of Hawking evaporation using covariant loop quantum gravity.