Gravitational Uncertainty and Black Hole Remnants

TL;DR

This paper explores the potential existence of black hole remnants as dark matter candidates by analyzing quantum gravitational effects on black hole entropy and temperature, and discusses observational detection methods and cosmological constraints.

Contribution

It introduces a framework for studying black hole remnants considering quantum gravitational corrections, providing new insights into their viability as dark matter.

Findings

Black hole remnants could serve as dark matter candidates.

Quantum gravitational corrections affect black hole thermodynamics.

Observational strategies for detecting remnants are proposed.

Abstract

Possible existence of black holes remnants provides a suitable candidates for dark matter. In this paper we study the possibility of existence for such remnants. We consider quantum gravitational induced corrections of black hole's entropy and temperature to investigate the possibility of such relics. Observational scheme for detection of these remnants and their cosmological constraints are discussed.