Using di quark pairs as a way to obtain dark matter near the beginning of nucleation of a new universe

TL;DR

This paper proposes a novel mechanism involving di-quark pairs formed via topological defects and axion walls to set initial conditions for inflationary cosmology, potentially explaining early dark matter presence.

Contribution

It introduces a new approach using di-quark pairs and topological defects to explain initial conditions for inflation and dark matter in the early universe.

Findings

Di-quark pairs can serve as initial conditions for inflation.

Topological defects influence the formation of dark matter.

CP violation may trigger inflationary expansion.

Abstract

Using the Bogomolnyi inequality and the vanishing of topological charge at the onset of nucleation of a new universe permits a simpler, more direct of how topological defects(kinks and anti kinks) contribute to the onset of initial conditions at the beginning of inflationary cosmology. We find that it is possible to present inflationary cosmology with initial conditions with di-quark pairs formed using an axion wall as a way to start formation of di quarks as soliton-anti soltion type pairs. This allows for a transition to inflationary cosmology congruent with with an initial nucleation state of matter which would have a significant dark matter componet in the beginning. The separation between the di-quark pairs constituents would be due to CP violations in the initial phases of matter creation and would be a convenient trigger for inflationary expansion.