# Black Hole Remnants

## TL;DR

This paper demonstrates that in a specific modified gravity theory, black hole singularities are resolved into de Sitter spaces, leading to stable remnants after evaporation with zero temperature.

## Contribution

It introduces a model where black hole singularities are replaced by de Sitter space, resulting in stable remnants, a novel resolution to classical singularities.

## Key findings

- Singularity replaced by de Sitter space
- Remnants remain after Hawking evaporation
- Remnants have zero Hawking temperature

## Abstract

We show that in asymptotically free mimetic gravity with limiting curvature the black hole singularity can be resolved and replaced by a static patch of de Sitter space. As a result of Hawking evaporation of these non-singular black holes, there remain stable remnants with vanishing Hawking temperature.