pith. sign in

arxiv: 1805.03872 · v2 · pith:YOHVJQTGnew · submitted 2018-05-10 · 🌀 gr-qc · physics.hist-ph

Small black/white hole stability and dark matter

classification 🌀 gr-qc physics.hist-ph
keywords blackholesquantumwhitedarkformedholematter
0
0 comments X
read the original abstract

We show that the expected lifetime of white holes formed as remnants of evaporated black holes is consistent with their production at reheating. We give a simple quantum description of these objects and argue that a quantum superposition of black and white holes with large interiors is stable, because it is protected by the existence of a minimal eigenvalue of the area, predicted by Loop Quantum Gravity. These two results support the hypothesis that a component of dark matter could be formed by small black hole remnants.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Signatures of loop quantum gravity in primordial black hole cosmologies

    gr-qc 2026-05 unverdicted novelty 5.0

    PBH masses near 10^3 kg allow Hawking evaporation to reheat the universe while Planckian remnants comprise all present-day DM without fine-tuning initial abundance, yielding testable GW signals.