Low-energy quantum gravity: new challenges for an experiment and observation

TL;DR

This paper discusses the implications of a low-energy quantum gravity model, highlighting new experimental challenges and the surprising prediction that black hole masses have a lower limit, contrary to classical expectations.

Contribution

It introduces a novel low-energy quantum gravity model with unique properties, including asymptotic freedom and a mass restriction for black holes formed from baryonic matter.

Findings

Black hole mass has a lower limit of about 10^7 solar masses.

Asymptotic freedom leads to new observational challenges.

The model predicts constraints on black hole formation from baryonic matter.

Abstract

Some new challenges for an experiment and observation, which are consequences of the model of low-energy quantum gravity by the author, are considered here. In particular, the property of asymptotic freedom of this model leads to the unexpected consequence: if a black hole arises due to a collapse of a matter with some characteristic mass of particles, its full mass should be restricted from the bottom. For usual baryonic matter, this limit of mass is of the order $10^{7}M_{\odot}$.